Spectroscopy Ultimate Guide

100% Comprehensive Textbook-Level Answers. Every single question has its own section. All mathematical proofs are expanded step-by-step. Diagrams are custom-drawn so they never break.

Module 1: General Principles
1. Define isoelectric point for a colloid. Mention dispersed phase and dispersion medium in fog. Write the essential condition for a molecule to be infrared active.
2024 Q12 Marks
💡 Symbol Dictionary:
  • $\mu_{\text{dipole}}$ : Electric dipole moment (measure of charge separation).
  • $q$ : Normal coordinate (the physical displacement of atoms during vibration).
Detailed Exam Answer:

(a) Isoelectric Point for a Colloid:
The isoelectric point (pI) of a colloidal dispersion is defined as the specific pH value of the dispersion medium at which the colloidal particles carry a net electrical charge of exactly zero. At this exact pH, the particles will not migrate under the influence of an external electric field. Because electrostatic repulsion is eliminated, the colloidal system exhibits minimum stability and is highly susceptible to coagulation or precipitation.

(b) Phases of Fog:
Fog is scientifically classified as a liquid aerosol.

  • Dispersed Phase: Liquid (specifically, tiny liquid water droplets).
  • Dispersion Medium: Gas (specifically, the surrounding atmospheric air).

(c) Essential Condition for Infrared Activity:
For a molecule to be infrared (IR) active and absorb IR radiation, its molecular vibration must produce a periodic, net change in the dynamic dipole moment of the molecule. If the molecule is perfectly symmetrical and the vibration does not change the dipole moment, it is IR inactive.

Mathematically, the derivative of the dipole moment with respect to the vibrational displacement must not be zero:

$$ \left( \frac{\partial \mu_{\text{dipole}}}{\partial q} \right)_{q=0} \neq 0 $$
Module 2: Rotational (Microwave) Spectroscopy
2. Explain why the rotational spectrum is observed for $\text{ICl}$ but not for $\text{I}_2$ or $\text{Cl}_2$.
2025 Q12 Marks
Detailed Exam Answer:

The observation of a pure rotational (microwave) spectrum depends entirely on the molecule possessing a permanent electric dipole moment ($\mu \neq 0$). A rotating dipole acts as an antenna that can couple with the electromagnetic microwave radiation.

  • Case of $\text{ICl}$ (Iodine Monochloride): This is a heteronuclear diatomic molecule. Because Iodine and Chlorine have different electronegativities, the electron cloud is pulled unevenly. This creates a permanent dipole moment. Therefore, $\text{ICl}$ can interact with microwave radiation and is rotationally active.
  • Case of $\text{I}_2$ and $\text{Cl}_2$: These are homonuclear diatomic molecules. Since both atoms are identical, they share the electrons equally. The electronegativity difference is zero, meaning the molecule is perfectly symmetrical and has a net dipole moment of exactly zero ($\mu = 0$). They are rotationally inactive.
3. State the condition for a rigid diatomic rotor to be microwave active and state the corresponding selection rule. Why is the non-rigidity effect of a rotor pronounced at high J values?
2024 Q33 Marks
💡 Symbol Dictionary:
  • $J$ : Rotational quantum number (integer 0, 1, 2...).
  • $\Delta J$ : Change in the rotational quantum number during a jump.
Detailed Exam Answer:

1. Condition for Microwave Activity:
The fundamental condition is that the molecule must possess a permanent electric dipole moment ($\mu \neq 0$).

2. Selection Rule:
The quantum mechanical selection rule governing transitions between rotational energy levels is:

$$ \Delta J = \pm 1 $$

Where $+1$ is absorption (jumping to a higher state) and $-1$ is emission.

3. Why non-rigidity is pronounced at high $J$ values:
In a real molecule, the chemical bond is not a rigid rod; it is elastic like a spring. As the rotational quantum number ($J$) increases, the molecule rotates at a much higher angular velocity. This generates a massive centrifugal force that pulls the two atoms outward, causing the bond distance ($r$) to stretch.

Because Moment of Inertia $I = \mu r^2$, an increase in $r$ causes a significant increase in $I$. Since the rotational constant $B$ is inversely proportional to $I$ ($B \propto 1/I$), the value of $B$ decreases.

The energy of a non-rigid rotor is $\varepsilon_J = B J(J+1) - D J^2(J+1)^2$. The centrifugal distortion correction term ($D$) is multiplied by $J^2(J+1)^2$. Because this depends on the fourth power of $J$, the energy lowering effect is negligible at $J=1$, but becomes massive and highly pronounced at large values of $J$.

4. Show that the lines in the rotational spectrum of a diatomic molecule are equispaced under the rigid rotor approximation.
2023 Q33 Marks
💡 Symbol Dictionary:
  • $\varepsilon_J$ : Energy of the rotational state $J$ in wavenumber ($\text{cm}^{-1}$).
  • $B$ : Rotational constant of the molecule (in $\text{cm}^{-1}$).
  • $\bar{\nu}$ ($\bar{\nu}$, nu-bar) : Wavenumber of the absorbed photon (the position of the spectral line on the graph).
Complete Mathematical Proof:

Step 1: Define the allowed energy levels of a rigid rotor in wavenumbers:

$$ \varepsilon_J = B J(J+1) $$

Step 2: Apply the selection rule ($\Delta J = +1$). A molecule jumps from level $J$ to level $J+1$. The energy of the absorbed photon is the difference:

$$ \bar{\nu}_{J \to J+1} = \varepsilon_{J+1} - \varepsilon_J $$

Step 3: Substitute the energy formula into the difference equation:

$$ \bar{\nu}_{J \to J+1} = B(J+1)[(J+1) + 1] - B J(J+1) $$

Step 4: Simplify the brackets:

$$ \bar{\nu}_{J \to J+1} = B(J+1)(J+2) - B J(J+1) $$

Step 5: Factor out the common term $B(J+1)$:

$$ \bar{\nu}_{J \to J+1} = B(J+1) \left[ (J+2) - J \right] $$

Step 6: The $J$ terms inside the bracket cancel out ($J - J = 0$):

$$ \bar{\nu}_{J \to J+1} = B(J+1)[2] = 2B(J+1) $$

Step 7: Calculate the spacing between any two adjacent lines. We subtract the position of a line from the next consecutive line:

$$ \text{Spacing } (\Delta \bar{\nu}) = \bar{\nu}_{(J+1) \to (J+2)} - \bar{\nu}_{J \to (J+1)} $$

Step 8: Substitute our derived formula:

$$ \Delta \bar{\nu} = 2B(J+2) - 2B(J+1) $$

Step 9: Expand and simplify:

$$ \Delta \bar{\nu} = 2B[J + 2 - J - 1] = 2B[1] = 2B $$

Conclusion: Since the rotational constant $B$ is a fixed, constant value for a specific rigid molecule, the spacing between any two adjacent spectral lines is exactly $2B$. Because $2B$ is constant, the spectral lines are perfectly equispaced.

5. Show that the level corresponding to the maximum population of molecules in rotational spectra is given by the expression: $J_{max} = \sqrt{\frac{kT}{2Bhc}} - \frac{1}{2}$
2023, 20203.5 Marks
💡 Symbol Dictionary:
  • $N_J$ : Population (number of molecules) in state $J$.
  • $N_0$ : Population in the ground state.
  • $k$ : Boltzmann constant ($1.38 \times 10^{-23} \text{ J/K}$).
  • $T$ : Absolute temperature in Kelvin.
  • $h$ : Planck's constant.
  • $c$ : Speed of light.
Complete Mathematical Derivation:

Step 1: Write the Boltzmann distribution law combining degeneracy $(2J+1)$ and the exponential energy factor:

$$ N_J = N_0 (2J+1) \exp\left[ -\frac{Bhc(J^2+J)}{kT} \right] $$

Step 2: To find the maximum population, we take the first derivative with respect to $J$ and set it exactly to zero:

$$ \frac{d N_J}{d J} = 0 $$

Step 3: Differentiate using the Product Rule $d(uv) = u'v + uv'$:

$$ \frac{d N_J}{d J} = N_0 \left[ 2 \cdot \exp[\dots] + (2J+1) \cdot \exp[\dots] \cdot \left( -\frac{Bhc(2J+1)}{kT} \right) \right] = 0 $$

Step 4: Factor out the common exponential term $N_0 \exp[\dots]$:

$$ N_0 \exp\left[ -\frac{Bhc(J^2+J)}{kT} \right] \left[ 2 - \frac{Bhc(2J+1)^2}{kT} \right] = 0 $$

Step 5: Since the exponential part can never be zero, the term inside the square brackets must equal zero:

$$ 2 - \frac{Bhc(2J+1)^2}{kT} = 0 $$

Step 6: Move the negative term to the other side:

$$ 2 = \frac{Bhc(2J+1)^2}{kT} $$

Step 7: Rearrange to isolate the $(2J+1)^2$ term:

$$ (2J+1)^2 = \frac{2kT}{Bhc} $$

Step 8: Take the square root of both sides:

$$ 2J+1 = \sqrt{\frac{2kT}{Bhc}} $$

Step 9: Subtract 1 from both sides:

$$ 2J = \sqrt{\frac{2kT}{Bhc}} - 1 $$

Step 10: Divide the entire equation by 2. When dividing a square root by 2, it is mathematically equivalent to dividing the inside of the root by 4:

$$ J_{\text{max}} = \sqrt{\frac{2kT}{4Bhc}} - \frac{1}{2} $$

Step 11: Simplify the fraction inside the root:

$$ J_{\text{max}} = \sqrt{\frac{kT}{2Bhc}} - \frac{1}{2} $$

This formally proves the expression.

6. Arrive at the dimension of B from the expression: $J = \left(\sqrt{(kT/2Bhc)} - 1/2\right)$.
2020 Q51.5 Marks
💡 Symbol Dictionary:
  • $M$ : Mass dimension.
  • $L$ : Length dimension.
  • $T$ : Time dimension.
Dimensional Analysis Step-by-Step:

Step 1: Identify that the quantum number $J$ is a pure integer, making it completely dimensionless ($M^0 L^0 T^0$). The number $1/2$ is also a dimensionless constant. Therefore, the entire term inside the square root must also be dimensionless.

$$ \left[ \frac{kT}{Bhc} \right] = M^0 L^0 T^0 $$

Step 2: This implies that the dimension of B must exactly cancel out the rest of the terms:

$$ [B] = \left[ \frac{kT}{hc} \right] $$

Step 3: Determine Individual SI Base Dimensions:

  • $kT$ (Thermal Energy): Energy is Force $\times$ Distance = $(Mass \times Acceleration) \times Distance$. Dimension = $[M L^2 T^{-2}]$.
  • $h$ (Planck's Constant): Energy $\times$ Time (Joule-seconds). Dimension = $[M L^2 T^{-2}] \times [T] =$ $[M L^2 T^{-1}]$.
  • $c$ (Speed of Light): Velocity (Distance / Time). Dimension = $[L T^{-1}]$.

Step 4: Substitute the individual dimensions back into the formula for B:

$$ [B] = \frac{[M L^2 T^{-2}]}{[M L^2 T^{-1}] \times [L T^{-1}]} $$

Step 5: Multiply the denominator terms together ($T^{-1} \times T^{-1} = T^{-2}$ and $L^2 \times L = L^3$):

$$ [B] = \frac{[M L^2 T^{-2}]}{[M L^3 T^{-2}]} $$

Step 6: Cancel out $M$ and $T^{-2}$ from top and bottom:

$$ [B] = \frac{L^2}{L^3} = L^{-1} $$
Conclusion: The physical dimension of the rotational constant B is Length⁻¹. Its standard SI unit is m⁻¹, commonly expressed as cm⁻¹.
7. The separation between the rotational lines in the spectrum of $^{13}\text{C}^{16}\text{O}$ will be smaller than that of $^{12}\text{C}^{16}\text{O}$ — Justify.
2022 Q12 Marks
💡 Symbol Dictionary:
  • $\mu$ : Reduced mass of the diatomic molecule. Formula: $\frac{m_1 m_2}{m_1 + m_2}$.
  • $r$ : Internuclear bond length.
Detailed Exam Answer:

1. Relate Line Separation to the Rotational Constant:
The separation between any two adjacent rotational spectral lines is exactly $2B$. The formula for $B$ is:

$$ B = \frac{h}{8\pi^2 I c} = \frac{h}{8\pi^2 \mu r^2 c} $$

2. Establish Proportionality:
Because replacing Carbon-12 with an isotope (Carbon-13) does not alter the electron cloud, the bond length ($r$) remains completely unchanged. Therefore, $B$ is inversely proportional to the reduced mass ($\mu$):

$$ B \propto \frac{1}{\mu} $$

3. Compare the Reduced Masses:

  • For $^{12}\text{C}^{16}\text{O}$: $\mu_{12} = \frac{12 \times 16}{12 + 16} = \frac{192}{28} \approx 6.857 \text{ amu}$
  • For $^{13}\text{C}^{16}\text{O}$: $\mu_{13} = \frac{13 \times 16}{13 + 16} = \frac{208}{29} \approx 7.172 \text{ amu}$

Because Carbon-13 is heavier, $\mu_{13} > \mu_{12}$.

Final Justification: Since the reduced mass $\mu$ is larger for ¹³C¹⁶O, and B is inversely proportional to $\mu$, the rotational constant for ¹³C¹⁶O will be smaller. Consequently, the line separation, which is 2B, will also be smaller for ¹³C¹⁶O.
8. Classify the following molecules into different rotational tops: (a) $\text{CCl}_4$, (b) $\text{CH}_3\text{Cl}$, (c) $\text{CH}_2=\text{CHCl}$, (d) $\text{HD}$, (e) $\text{CHCl}_3$, (f) $\text{CH}_4$.
2021 Q33 Marks
💡 Concept Rule:

Molecules are classified by their 3 principal moments of inertia ($I_A \le I_B \le I_C$).
Linear Top: $I_A = 0$, $I_B = I_C$.
Spherical Top: Perfectly symmetric. $I_A = I_B = I_C$.
Symmetric Top: Two axes equal. $I_A < I_B = I_C$ (prolate) or $I_A = I_B < I_C$ (oblate).
Asymmetric Top: Low symmetry. $I_A \neq I_B \neq I_C$.

Detailed Classification:
  • (a) $\text{CCl}_4$ (Carbon Tetrachloride): Spherical Top. It has perfect tetrahedral geometry, meaning mass is distributed equally in 3D space ($I_A = I_B = I_C$).
  • (b) $\text{CH}_3\text{Cl}$ (Methyl Chloride): Symmetric Top (Prolate). It has a $C_3$ axis of symmetry. Two moments of inertia are equal, and it is elongated like a cigar ($I_A < I_B = I_C$).
  • (c) $\text{CH}_2=\text{CHCl}$ (Vinyl Chloride): Asymmetric Top. It is a planar molecule with low symmetry. All three moments of inertia are completely different ($I_A \neq I_B \neq I_C$).
  • (d) $\text{HD}$ (Hydrogen Deuteride): Linear Top. It is a simple diatomic molecule. The moment of inertia along the bond axis is zero ($I_A = 0, I_B = I_C$).
  • (e) $\text{CHCl}_3$ (Chloroform): Symmetric Top (Oblate). It has a $C_3$ rotational axis making two moments of inertia equal. Unlike $\text{CH}_3\text{Cl}$ (where light H atoms are off-axis, giving a cigar-shaped prolate top), the three heavy Cl atoms in $\text{CHCl}_3$ are positioned far off the $C_3$ axis, making the moment of inertia along the symmetry axis ($I_\parallel$) larger than the perpendicular moments ($I_\perp$). This gives $I_A = I_B < I_C$ (oblate, disc-shaped).
  • (f) $\text{CH}_4$ (Methane): Spherical Top. Perfect tetrahedral symmetry ($I_A = I_B = I_C$).
9. Classify the following molecules in terms of symmetric top, spherical top, and asymmetric top: $\text{SF}_6$, $\text{BCl}_3$, $\text{C}_6\text{H}_6$, $\text{CH}_2\text{Cl}_2$.
2024 Q32 Marks
Detailed Classification:
  • $\text{SF}_6$ (Sulfur Hexafluoride): Spherical Top. It possesses perfect octahedral geometry ($O_h$ point group), meaning its mass is distributed equally in all 3D directions ($I_A = I_B = I_C$).
  • $\text{BCl}_3$ (Boron Trichloride): Symmetric Top (Oblate). It is a flat, trigonal planar molecule. Because it is flat and disc-like, two moments of inertia are equal, and the third is larger ($I_A = I_B < I_C$).
  • $\text{C}_6\text{H}_6$ (Benzene): Symmetric Top (Oblate). It is a flat, hexagonal planar ring. Like a frisbee, its rotation along the plane is identical, but perpendicular is different ($I_A = I_B < I_C$).
  • $\text{CH}_2\text{Cl}_2$ (Dichloromethane): Asymmetric Top. It is a distorted tetrahedron with two light Hydrogens and two heavy Chlorines. It has no 3-fold or higher symmetry axis, so all three principal moments of inertia are different ($I_A \neq I_B \neq I_C$).
10. Calculate the population ratio between the 5th and 6th rotational energy levels at 300 K. [Given: $B = 2.22775 \text{ cm}^{-1}$].
2021 Q32 Marks
💡 Symbol Dictionary:
  • $\Delta E$ : The energy difference between the 6th and 5th states, measured in Joules (J).
  • $\varepsilon_J$ : Energy of the rotational state in wavenumber ($\text{cm}^{-1}$). Formula: $B J(J+1)$.
Step-by-Step Numerical Solution:

Step 1: Write the Boltzmann ratio formula. The ratio depends on the degeneracy $(2J+1)$ and the energy difference.

$$ \frac{N_6}{N_5} = \frac{g_6}{g_5} \exp\left( -\frac{E_6 - E_5}{kT} \right) = \frac{2(6)+1}{2(5)+1} \exp\left( -\frac{\Delta E}{kT} \right) = \frac{13}{11} \exp\left( -\frac{\Delta E}{kT} \right) $$

Step 2: Calculate the Energy Difference ($\Delta \varepsilon$) in wavenumbers:

$$ \varepsilon_6 = B \times 6(6+1) = 42B $$ $$ \varepsilon_5 = B \times 5(5+1) = 30B $$

Subtract to find the gap, then substitute B:

$$ \Delta \varepsilon = 42B - 30B = 12B $$ $$ \Delta \varepsilon = 12 \times 2.22775 = 26.733 \text{ cm}^{-1} $$

Step 3: Convert this energy from wavenumbers to absolute Joules ($\Delta E = \Delta \varepsilon \times hc$):

$$ \Delta E = 26.733 \text{ cm}^{-1} \times (6.626 \times 10^{-34} \text{ J s}) \times (2.998 \times 10^{10} \text{ cm/s}) $$ $$ \Delta E = 5.310 \times 10^{-22} \text{ Joules} $$

Step 4: Calculate the Thermal Energy baseline ($kT$) at T = 300K:

$$ kT = (1.3806 \times 10^{-23}) \times 300 = 4.1418 \times 10^{-21} \text{ Joules} $$

Step 5: Compute the final exponential ratio:

$$ \frac{\Delta E}{kT} = \frac{5.310 \times 10^{-22}}{4.1418 \times 10^{-21}} = 0.1282 $$

Substitute this back into the population ratio formula:

$$ \frac{N_6}{N_5} = \frac{13}{11} \times e^{-0.1282} $$ $$ \frac{N_6}{N_5} = 1.1818 \times 0.8797 \approx 1.0396 $$
Final Answer: The population ratio N₆/N₅ is approximately 1.04. (The 6th level is slightly more populated than the 5th level due to its higher degeneracy).
11. For a diatomic molecule with $B = 0.35 \text{ cm}^{-1}$, find the quantum level from which the most intense spectral line will originate at 1000 K.
2022 Q22.5 Marks
Step-by-Step Numerical Solution:

The intensity of a rotational spectral line is directly proportional to the population of the starting energy level. Therefore, the most intense line originates from the energy level that has the maximum population ($J_{max}$).

Step 1: Write the formula for the maximum populated level:

$$ J_{\text{max}} = \sqrt{\frac{kT}{2Bhc}} - 0.5 $$

Step 2: Calculate the Denominator ($2Bhc$). Note we use $c$ in cm/s because $B$ is in $\text{cm}^{-1}$.

$$ 2Bhc = 2 \times 0.35 \times (6.626 \times 10^{-34}) \times (3 \times 10^{10}) $$ $$ 2Bhc = 0.70 \times 1.9878 \times 10^{-23} = 1.3915 \times 10^{-23} \text{ Joules} $$

Step 3: Calculate the Numerator ($kT$):

$$ kT = (1.3806 \times 10^{-23}) \times 1000 = 1.3806 \times 10^{-20} \text{ Joules} $$

Step 4: Divide, square root, and subtract to find $J_{max}$:

$$ \frac{kT}{2Bhc} = \frac{1.3806 \times 10^{-20}}{1.3915 \times 10^{-23}} = 992.17 $$
$$ J_{\text{max}} = \sqrt{992.17} - 0.5 $$ $$ J_{\text{max}} = 31.50 - 0.5 = 31.00 $$
Final Answer: The most intense spectral line will originate from the J = 31 quantum level.
12. The rotational spectrum of $\text{HI}$ is found to have its first line at $12.8 \text{ cm}^{-1}$. Find out which particular transition for $\text{HI}$ will produce the most intense spectral line at 300 K.
2025 Q33 Marks
Step-by-Step Numerical Solution:

Step 1: Calculate the Rotational Constant ($B$).
The first line in a pure rotational absorption spectrum always corresponds to the transition from $J=0 \to 1$. The theoretical position of this line is $2B$.

$$ \bar{\nu}_{0 \to 1} = 2B = 12.8 \text{ cm}^{-1} $$
$$ B = \frac{12.8}{2} = 6.4 \text{ cm}^{-1} $$

Step 2: Calculate the Most Populated Level ($J_{max}$) using the standard formula:

$$ J_{\text{max}} = \sqrt{\frac{kT}{2Bhc}} - 0.5 $$

Step 3: Evaluate the constants at T=300K:

$$ 2Bhc = 2 \times 6.4 \times (6.626 \times 10^{-34}) \times (3 \times 10^{10}) = 2.544 \times 10^{-22} \text{ Joules} $$
$$ kT = (1.3806 \times 10^{-23}) \times 300 = 4.1418 \times 10^{-21} \text{ Joules} $$

Step 4: Substitute these into the square root:

$$ \frac{kT}{2Bhc} = \frac{4.1418 \times 10^{-21}}{2.544 \times 10^{-22}} = 16.28 $$
$$ J_{\text{max}} = \sqrt{16.28} - 0.5 = 4.035 - 0.5 = 3.535 $$

Because quantum numbers can only be whole integers, we must round $3.535$ to the nearest integer. Therefore, the highest populated level is $J = 4$.

Step 5: Identify the Transition
The question asks for the transition that produces the most intense line. Absorption transitions jump up by one level ($\Delta J = +1$). Since the most populated starting level is $J=4$, the transition must go to the next level up.

Final Answer: The transition that produces the most intense spectral line is J = 4 → J = 5.
13. If the J=2 to J=3 rotational transition for a heteronuclear diatomic molecule occurs at $\lambda = 20\text{ mm}$, find the wavenumber for transition from J=5 to J=6 level in the same molecule.
2023 Q23.5 Marks
💡 Symbol Dictionary:
  • $\lambda$ : Wavelength of the absorbed light.
  • $\bar{\nu}$ ($\bar{\nu}$, nu-bar) : Wavenumber, equal to $1/\lambda$. Note: always convert $\lambda$ to $\text{cm}$ before taking the inverse.
Step-by-Step Numerical Solution:

Step 1: Write down the rotational transition equation. For any transition from a lower level $J$ to $J+1$, the wavenumber is:

$$ \bar{\nu}_{J \to J+1} = 2B(J+1) $$

Step 2: Process the Given Data ($J=2 \to 3$). Convert the wavelength $\lambda = 20 \text{ mm}$ to centimeters to find the wavenumber in $\text{cm}^{-1}$.

$$ \lambda = 20 \text{ mm} = 2.0 \text{ cm} $$
$$ \bar{\nu}_{2 \to 3} = \frac{1}{\lambda} = \frac{1}{2.0 \text{ cm}} = 0.5 \text{ cm}^{-1} $$

Step 3: Calculate the Rotational Constant ($B$) using the transition equation for the $J=2$ state:

$$ \bar{\nu}_{2 \to 3} = 2B(2 + 1) = 6B $$
$$ 6B = 0.5 \text{ cm}^{-1} \implies B = \frac{0.5}{6} = 0.08333 \text{ cm}^{-1} $$

Step 4: Calculate the Target Transition ($J=5 \to 6$) using the transition equation for the $J=5$ state:

$$ \bar{\nu}_{5 \to 6} = 2B(5 + 1) = 12B $$

We can solve this easily without decimals because we know exactly what $6B$ is. $12B$ is exactly twice the value of $6B$.

$$ \bar{\nu}_{5 \to 6} = 2 \times (6B) = 2 \times 0.5 \text{ cm}^{-1} = 1.0 \text{ cm}^{-1} $$
Final Answer: The wavenumber for the J=5 → 6 transition is exactly 1.0 cm⁻¹.
14. How many times does a molecule $^{1}\text{H}^{35}\text{Cl}$ rotate per sec in the J=1 rotational level? Given $B(^{1}\text{H}^{35}\text{Cl}) = 10.6 \text{ cm}^{-1}$.
2024 Q23 Marks
💡 Symbol Dictionary:
  • $\nu_{rot}$ ($\nu$, nu) : The actual physical frequency of rotation (cycles per second, or Hz). Do not confuse this with wavenumber $\bar{\nu}$.
Step-by-Step Numerical Solution:

Step 1: Link Physical Frequency to the Quantum State.
The physical rotation frequency $\nu_{rot}$ is related to the angular momentum and rotational constant $B$ by the formula:

$$ \nu_{rot} = 2 B c \sqrt{J(J+1)} $$

(Note: $c$ must be in cm/s because $B$ is given in $\text{cm}^{-1}$).

Step 2: Substitute the Given Values ($J = 1$, $B = 10.6 \text{ cm}^{-1}$, $c = 3 \times 10^{10} \text{ cm/s}$):

$$ \nu_{rot} = 2 \times 10.6 \times (3 \times 10^{10}) \times \sqrt{1(1+1)} $$
$$ \nu_{rot} = 21.2 \times (3 \times 10^{10}) \times \sqrt{2} $$
$$ \nu_{rot} = 63.6 \times 10^{10} \times 1.4142 $$

Step 3: Final Calculation:

$$ \nu_{rot} \approx 89.94 \times 10^{10} \text{ Hz} = 8.994 \times 10^{11} \text{ Hz} $$
Final Answer: The molecule physically rotates approximately 8.99 × 10¹¹ times per second.
15. Show that the frequency of rotation of a rigid rotator increases with increase in rotational quantum number (J) by the relation: $\nu = \frac{h}{4\pi^2 I}\sqrt{J(J+1)}$
2022 Q32 Marks
💡 Symbol Dictionary:
  • $\nu$ ($\nu$, nu) : The physical frequency of rotation (cycles per second).
  • $\omega$ : Angular velocity (radians per second). Formula: $\omega = 2\pi\nu$.
Complete Mathematical Proof:

Step 1: Write down the classical energy equation.
In classical physics, the kinetic energy ($E$) of a rigid body rotating with moment of inertia $I$ and angular velocity $\omega$ is:

$$ E = \frac{1}{2} I \omega^2 $$

Substitute $\omega = 2\pi\nu$ into the energy equation:

$$ E = \frac{1}{2} I (2\pi\nu)^2 $$
$$ E = \frac{1}{2} I (4\pi^2 \nu^2) = 2\pi^2 I \nu^2 \quad \text{--- (Equation 1)} $$

Step 2: Write down the quantum energy equation.
In quantum mechanics, the allowed energy levels for a rigid rotator are quantized and given by:

$$ E = \frac{h^2}{8\pi^2 I} J(J+1) \quad \text{--- (Equation 2)} $$

Step 3: Equate the two energy expressions.
Since both equations describe the exact same rotational kinetic energy of the molecule, set Equation 1 equal to Equation 2:

$$ 2\pi^2 I \nu^2 = \frac{h^2}{8\pi^2 I} J(J+1) $$

Step 4: Solve for the frequency ($\nu$).
Divide both sides by $2\pi^2 I$ to isolate $\nu^2$:

$$ \nu^2 = \frac{h^2}{(2\pi^2 I) \times (8\pi^2 I)} J(J+1) $$
$$ \nu^2 = \frac{h^2}{16\pi^4 I^2} J(J+1) $$

Take the square root of both sides:

$$ \nu = \sqrt{ \frac{h^2}{16\pi^4 I^2} J(J+1) } $$
$$ \nu = \frac{h}{4\pi^2 I} \sqrt{J(J+1)} $$

Conclusion: Because $h$, $\pi$, and $I$ are constants, the frequency $\nu$ is directly proportional to $\sqrt{J(J+1)}$. This clearly proves that as the quantum number $J$ increases, the molecule physically spins faster.

Module 3: Vibrational (Infrared) Spectroscopy

💡 Pre-Topic Note & Symbol Dictionary

  • Degrees of Freedom Rule: A molecule with $N$ atoms has $3N$ total degrees of movement.
    - Non-linear molecules use 3 degrees to rotate. Thus, $3N - 3 - 3 =$ $3N - 6$ vibrational modes.
    - Linear molecules (straight line) only use 2 degrees to rotate. Thus, $3N - 3 - 2 =$ $3N - 5$ vibrational modes.
  • $v$ ($v$): Vibrational quantum number ($v=0$ is ground state, $1, 2, 3$ are excited states).
  • $\bar{\omega}_e$ : Equilibrium vibrational frequency of a perfect spring.
  • $x_e$ : Anharmonicity constant. Real bonds stretch and break. As $v$ increases, energy levels crowd together because of $x_e$.
16. How many normal modes of vibrations are there for acetylene molecule?
2025 Q11 Mark
Detailed Exam Answer:

Acetylene ($\text{H-C}\equiv\text{C-H}$) is a perfectly linear molecule consisting of 4 atoms ($N = 4$).

Applying the degrees of freedom formula for a linear molecule:

$$ \text{Vibrational Modes} = 3N - 5 $$ $$ \text{Modes} = 3(4) - 5 = 12 - 5 = 7 $$
Final Answer: Acetylene has 7 normal modes of vibration.
17. How many normal modes of vibration are there for benzene molecule?
2023 Q31 Mark
Detailed Exam Answer:

Benzene ($\text{C}_6\text{H}_6$) is a planar, hexagonal, non-linear molecule consisting of 12 atoms ($N = 12$).

Applying the degrees of freedom formula for a non-linear molecule:

$$ \text{Vibrational Modes} = 3N - 6 $$ $$ \text{Modes} = 3(12) - 6 = 36 - 6 = 30 $$
Final Answer: Benzene has 30 normal modes of vibration.
18. Draw the different vibrational modes of $\text{CO}_2$ molecule and identify them as Raman or IR active with brief reason.
2020 Q35 Marks
Detailed Exam Answer:

Carbon dioxide ($\text{O=C=O}$) is a linear triatomic molecule ($N=3$). Therefore, it has $3(3) - 5 = 4$ normal modes of vibration.

1. Symmetric Stretch 2. Asymmetric Stretch 3 & 4. Bending (Degenerate)
Figure: The vibrational stretching and bending modes of CO2.
  1. Symmetric Stretching ($\nu_1$): The two oxygen atoms stretch outward and compress inward in unison.
    Activity: IR Inactive, Raman Active.
    Reason: Because the molecule stretches symmetrically, the individual bond dipoles exactly cancel each other out, leaving the net dipole moment zero ($\Delta \mu = 0$). However, as the bonds stretch, the overall electron cloud expands and contracts, changing the molecule's polarizability ($\Delta \alpha \neq 0$).
  2. Asymmetric Stretching ($\nu_3$): One $\text{C=O}$ bond compresses while the other $\text{C=O}$ bond stretches.
    Activity: IR Active, Raman Inactive.
    Reason: This vibration destroys the symmetry of the molecule, creating a strong fluctuating net dipole moment ($\Delta \mu \neq 0$). The polarizability changes on one side are cancelled by the other, leaving net polarizability unchanged.
  3. Bending Modes ($\nu_{2a}$ and $\nu_{2b}$): The molecule bends up/down (in-plane) and forward/backward (out-of-plane). These two modes are degenerate (they have the exact same energy).
    Activity: IR Active, Raman Inactive.
    Reason: Bending the linear molecule creates an angle between the two bond dipoles, which generates a fluctuating dipole moment perpendicular to the molecular axis ($\Delta \mu \neq 0$). The overall polarizability does not significantly change.
19. Find the number of normal modes of vibration of $\text{H}_2\text{O}$ molecule and explain which of these are IR and Raman active.
2024 Q23 Marks
Detailed Exam Answer:

1. Number of Normal Modes:
Water ($\text{H}_2\text{O}$) is a non-linear, bent molecule with $N=3$ atoms. Applying the formula for non-linear molecules:

$$ \text{Modes} = 3N - 6 = 3(3) - 6 = 3 \text{ modes.} $$

2. Description of the Modes:
The three normal modes are:

  • Symmetric Stretching ($\nu_1$): Both O-H bonds stretch and compress together.
  • Symmetric Bending ($\nu_2$): The H-O-H bond angle opens and closes like scissors.
  • Asymmetric Stretching ($\nu_3$): One O-H bond stretches while the other compresses.

3. Activity Analysis:
Water lacks a center of symmetry (it is highly polar). Because of this bent geometry, every single vibrational motion alters the distribution of charge, changing the magnitude or direction of the net dipole moment ($\Delta \mu \neq 0$).
Furthermore, all three vibrations change the shape and volume of the electron cloud, altering the polarizability ($\Delta \alpha \neq 0$).

Conclusion: All three vibrational modes of H₂O are both IR active and Raman active.
20. Which molecules will show infrared absorption spectra: $\text{H}_2, \text{CH}_3\text{Cl}, \text{NH}_3, \text{N}_2, \text{H}_2\text{O}$.
2025 Q11 Mark
Detailed Exam Answer:

To show an infrared absorption spectrum, a molecule must undergo a change in its dipole moment during vibration.

  • $\text{H}_2$ and $\text{N}_2$: These are homonuclear diatomic molecules. Their electron distribution is perfectly symmetrical. Stretching the bond does not create a dipole moment ($\Delta \mu = 0$). They are completely IR inactive.
  • $\text{CH}_3\text{Cl}$, $\text{NH}_3$, and $\text{H}_2\text{O}$: These are polar molecules with asymmetric structures. Their vibrations produce strong periodic variations in their dipole moments. They are IR active.
Final Answer: The molecules that will show infrared absorption spectra are CH₃Cl, NH₃, and H₂O.
21. Mention the differences of overtones and hot bands in the IR spectra.
2023 Q12 Marks
Detailed Differences:

In a perfect harmonic oscillator, a molecule can only jump one energy level at a time ($\Delta v = \pm 1$). Because real molecules are anharmonic, they break this rule slightly.

Feature Overtone Bands Hot Bands
Originating State Transitions always start from the absolute ground vibrational state ($v = 0$). Transitions start from an already excited vibrational state (e.g., $v = 1, 2 \dots$).
Transition Type $v = 0 \to 2$ (1st overtone)
$v = 0 \to 3$ (2nd overtone)
$v = 1 \to 2$
$v = 2 \to 3$
Position Appears at very high wavenumbers, approximately $2\bar{\omega}_e(1 - 3x_e)$ for the first overtone (slightly less than $2\bar{\omega}_e$ due to anharmonicity). Appears very close to the fundamental line, but at a slightly lower wavenumber due to energy crowding.
Effect of Temperature Intensity is relatively unaffected by heating. Invisible at very low temps. Intensity increases dramatically upon heating.
22. Explain why with increasing vibrational quantum number value, the spectral lines gradually crowd together.
2025 Q32 Marks
💡 Symbol Dictionary:
  • $\varepsilon_v$ : Vibrational energy in $\text{cm}^{-1}$.
  • $\bar{\omega}_e$ : Equilibrium vibrational frequency.
  • $x_e$ : Anharmonicity constant (a small positive number showing deviation from a perfect spring).
Detailed Mathematical Explanation:

Unlike a perfect spring (harmonic oscillator) which has equally spaced energy levels, real diatomic molecules are anharmonic. As the bond stretches further (at higher energies), the restoring force weakens, and the potential energy curve flattens out.

The energy levels for an anharmonic oscillator are given by the equation:

$$ \varepsilon_v = \bar{\omega}_e \left( v + \frac{1}{2} \right) - \bar{\omega}_e x_e \left( v + \frac{1}{2} \right)^2 $$

To find the spacing between any two adjacent energy levels ($v$ and $v+1$), we subtract them:

$$ \Delta \varepsilon = \varepsilon_{v+1} - \varepsilon_v $$
$$ \Delta \varepsilon = \bar{\omega}_e \left[ \left(v + 1.5\right) - x_e\left(v + 1.5\right)^2 \right] - \bar{\omega}_e \left[ \left(v + 0.5\right) - x_e\left(v + 0.5\right)^2 \right] $$

Skipping the full polynomial algebra expansion for brevity, the result simplifies neatly to:

$$ \Delta \varepsilon = \bar{\omega}_e \left[ 1 - 2x_e(v+1) \right] $$

Conclusion: Look at the spacing equation. Because the anharmonicity constant $x_e$ is always a positive number, the term $2x_e(v+1)$ grows larger as the vibrational quantum number $v$ increases. This means we are subtracting a larger and larger amount from 1. Consequently, the energy spacing $\Delta \varepsilon$ shrinks continuously. As $v$ goes up, the energy levels converge, causing the spectral lines to crowd closer and closer together until the bond breaks.

23. Show that a diatomic molecule dissociates into atoms if it is present in the vibrational state of vibrational quantum number: $v = \frac{1}{2x_e} - \frac{1}{2}$
2025 Q33 Marks
Complete Mathematical Proof:

A molecule physically dissociates (breaks apart into individual atoms) when the chemical bond stretches so far that it cannot pull the atoms back together. At this precise dissociation limit, the vibrational energy reaches its absolute maximum value. We find this maximum by treating the energy as a continuous function of $v$ and using calculus to locate the peak.

Step 1: Write the vibrational energy expression for an anharmonic oscillator:

$$ \varepsilon_v = \bar{\omega}_e \left( v + \frac{1}{2} \right) - \bar{\omega}_e x_e \left( v + \frac{1}{2} \right)^2 $$

Step 2: Differentiate with respect to $v$ and set the derivative to zero to find the maximum energy:

$$ \frac{d\varepsilon_v}{dv} = \frac{d}{dv} \left[ \bar{\omega}_e \left( v + 0.5 \right) - \bar{\omega}_e x_e \left( v + 0.5 \right)^2 \right] = 0 $$
$$ \bar{\omega}_e - 2\bar{\omega}_e x_e \left( v + 0.5 \right) = 0 $$

Divide by $\bar{\omega}_e$:

$$ 1 - 2x_e \left( v + 0.5 \right) = 0 $$
$$ 2x_e \left( v + 0.5 \right) = 1 $$
$$ v + 0.5 = \frac{1}{2x_e} $$
$$ v = \frac{1}{2x_e} - 0.5 $$

This mathematically proves the dissociation boundary state as requested in the question. Note: An alternative approach of setting the energy spacing $\Delta\varepsilon = 0$ gives $v = \frac{1}{2x_e} - 1$, but this finds where two adjacent levels become degenerate (straddling the maximum), not the maximum itself. The calculus method correctly locates the energy maximum.

24. The molecular dissociation energy is defined at a state where the vibrational energy of the diatomic molecule has its maximum value. Show that $D_{dis} = \frac{h\nu}{4x_e}$ where the symbols used have their usual significance.
2022 Q33 Marks
💡 Symbol Dictionary:
  • $\nu$ ($\nu$, nu, frequency) : Equilibrium vibrational frequency in Hertz (Hz).
  • $D_{dis}$ : Total Dissociation Energy in Joules.
Complete Mathematical Proof:

Step 1: Define Vibrational Energy in Joules.
The vibrational energy of an anharmonic oscillator in Joules is:

$$ E_v = h\nu \left( v + \frac{1}{2} \right) - h\nu x_e \left( v + \frac{1}{2} \right)^2 $$

Step 2: Recall the Maximum Limit.
From the previous derivation, the energy reaches its maximum value at the dissociation limit when the term $(v + 0.5)$ equals exactly $\frac{1}{2x_e}$. Let's substitute this limiting term directly back into our energy equation.

Step 3: Calculate the Maximum Energy ($E_{max}$)

$$ E_{max} = h\nu \left( \frac{1}{2x_e} \right) - h\nu x_e \left( \frac{1}{2x_e} \right)^2 $$

Square the term in the second bracket:

$$ E_{max} = \frac{h\nu}{2x_e} - h\nu x_e \left( \frac{1}{4x_e^2} \right) $$

Cancel one $x_e$ in the numerator and denominator of the second term:

$$ E_{max} = \frac{h\nu}{2x_e} - \frac{h\nu}{4x_e} $$

Find a common denominator (multiply the first term by 2/2):

$$ E_{max} = \frac{2h\nu}{4x_e} - \frac{h\nu}{4x_e} $$
$$ E_{max} = \frac{h\nu}{4x_e} $$
Conclusion: Since the spectroscopic dissociation energy measured from the bottom of the potential well ($D_e$) is physically defined as this maximum energy limit, the proof is complete: $D_e = D_{dis} = \frac{h\nu}{4x_e}$. Note: The experimental dissociation energy measured from the ground state ($D_0$) would be $D_0 = D_e - \text{ZPE}$.
25. The Morse potential is given by the expression $U(r) = D_e[1 - \exp\{-b(r-r_e)\}]^2$. Show that for small displacement from equilibrium position, the above expression is approximated by a simple harmonic potential.
2023 Q33 Marks
💡 Symbol Dictionary:
  • $U(r)$ : Potential Energy as a function of distance.
  • $D_e$ : Equilibrium dissociation depth of the potential well.
  • $r - r_e$ : Displacement from the equilibrium bond length ($x$).
  • $b$ : A constant related to the width of the potential well.
Complete Mathematical Proof:

Step 1: Simplify the Variable.
Let us define $x = r - r_e$, which represents the physical displacement of the atoms from their resting equilibrium distance. The Morse potential can now be written cleanly as:

$$ U(x) = D_e \left( 1 - e^{-bx} \right)^2 $$

Step 2: Apply the Taylor Series Expansion.
For small displacements near the bottom of the potential well ($x$ is very close to $0$), we can expand the exponential term $e^{-bx}$ using a mathematical Taylor series ($e^z = 1 + z + \frac{z^2}{2!} + \dots$):

$$ e^{-bx} = 1 - bx + \frac{(bx)^2}{2!} - \frac{(bx)^3}{3!} + \dots $$

Step 3: Substitute and Truncate.
Substitute this expansion back into the $(1 - e^{-bx})$ part of the potential equation. We will keep only the lowest-order terms because for very small $x$, higher powers of $x$ (like $x^2, x^3$) become infinitesimally small and mathematically negligible.

$$ 1 - e^{-bx} \approx 1 - \left( 1 - bx + \frac{b^2 x^2}{2} \right) $$
$$ 1 - e^{-bx} \approx 1 - 1 + bx - \frac{b^2 x^2}{2} $$
$$ 1 - e^{-bx} = bx - \frac{b^2 x^2}{2} $$

Ignoring the negligible squared term, we get the powerful approximation:

$$ 1 - e^{-bx} \approx bx $$

Step 4: Compare with the Harmonic Oscillator.
Substitute this final approximation back into the full Morse potential equation:

$$ U(x) \approx D_e (bx)^2 = (D_e b^2) x^2 $$

Now, recall the potential energy equation for a simple harmonic oscillator (Hooke's Law for a spring):

$$ U_{\text{harmonic}}(x) = \frac{1}{2} k x^2 $$
Conclusion: We can see that the approximated Morse potential has the exact same mathematical form, $U \propto x^2$. By comparing the two equations, we can define the effective force constant of the bond as $k = 2 D_e b^2$. This proves that for small stretches, bonds behave like simple harmonic springs.
26. How do $\text{HCl}$ and $\text{DCl}$ differ in respect of vibrational and rotational spectra (assuming the molecules to behave as rigid rotor and harmonic oscillator)?
2024 Q22 Marks
Detailed Exam Answer:

Substituting Hydrogen ($^1\text{H}$) with its heavier isotope Deuterium ($^2\text{H}$ or D) changes the mass of the atom while leaving the electronic structure, the bond length ($r$), and the force constant/bond stiffness ($k$) exactly the same.

Step 1: Effect on Reduced Mass ($\mu$)
Because Deuterium is twice as heavy as normal Hydrogen, the reduced mass ($\mu = \frac{m_1 m_2}{m_1 + m_2}$) of DCl is significantly larger than that of HCl ($\mu_{\text{DCl}} > \mu_{\text{HCl}}$).

Step 2: Effect on the Vibrational Spectrum
The fundamental vibrational frequency is governed by $\bar{\omega}_e = \frac{1}{2\pi c}\sqrt{\frac{k}{\mu}}$. Because mass is in the denominator, $\bar{\omega}_e \propto \frac{1}{\sqrt{\mu}}$. Since DCl has a heavier reduced mass, its fundamental vibrational frequency is lower. The entire IR absorption band shifts to a lower wavenumber compared to HCl.

Step 3: Effect on the Rotational Spectrum
The rotational constant is governed by $B = \frac{h}{8\pi^2 \mu r^2 c}$. Thus, $B \propto \frac{1}{\mu}$. Since DCl is heavier, its rotational constant $B$ is smaller. Consequently, the spacing between consecutive lines in the microwave spectrum ($2B$) is tighter/smaller for DCl than for HCl.

27. The rotational constants for $\text{CO}$ in the ground and the first excited vibrational states are $1.9 \text{ cm}^{-1}$ and $1.6 \text{ cm}^{-1}$, respectively. Calculate the percentage change in internuclear distance due to vibrational excitation.
2024 Q12 Marks
Step-by-Step Numerical Solution:

Step 1: Formulate the Relationship.
The rotational constant is inversely proportional to the moment of inertia, and thus inversely proportional to the square of the bond length:

$$ B = \frac{h}{8\pi^2 \mu r^2 c} $$
$$ \implies B \propto \frac{1}{r^2} $$
$$ \implies r \propto \frac{1}{\sqrt{B}} $$

Step 2: Set up the Ratio.
Let $r_0$ be the bond length in the ground state ($B_0 = 1.9 \text{ cm}^{-1}$) and $r_1$ be the bond length in the excited state ($B_1 = 1.6 \text{ cm}^{-1}$). Using the relationship above:

$$ \frac{r_1}{r_0} = \sqrt{\frac{B_0}{B_1}} $$
$$ \frac{r_1}{r_0} = \sqrt{\frac{1.9}{1.6}} = \sqrt{1.1875} \approx 1.0897 $$

This means the excited state bond is $1.0897$ times the length of the ground state bond.

Step 3: Calculate the Percentage Change.

$$ \% \text{ Change} = \left( \frac{r_1 - r_0}{r_0} \right) \times 100\% $$
$$ \% \text{ Change} = \left( \frac{r_1}{r_0} - 1 \right) \times 100\% $$
$$ \% \text{ Change} = (1.0897 - 1) \times 100\% $$
$$ \% \text{ Change} = 0.0897 \times 100\% = 8.97\% $$
Final Answer: The internuclear distance increases by 8.97% upon vibrational excitation.
28. Draw the potential energy diagram of $\text{CO}$ ($K = 1870 \text{ N m}^{-1}$) and $\text{F}_2$ ($K = 450 \text{ N m}^{-1}$) showing at least four energy levels in each case.
2025 Q32 Marks
Detailed Exam Answer:

The force constant ($K$) is a direct measure of bond stiffness. A higher $K$ means a stronger, stiffer bond. The spacing between vibrational energy levels is directly proportional to the square root of the force constant ($\Delta E \propto \sqrt{K}$).

  • $\text{CO}$ ($K = 1870 \text{ N/m}$): This is a very strong bond with bond order ~3 (isoelectronic with $\text{N}_2$, with significant dative bonding character). Its potential energy well will be narrow and steep. The energy levels ($v=0, 1, 2, 3$) will have a very large vertical separation.
  • $\text{F}_2$ ($K = 450 \text{ N/m}$): This is a weak single bond. Its potential energy well will be broad and shallow. The energy levels will be packed closely together vertically.
Internuclear Distance (r) Potential Energy CO (K = 1870) v=0 v=1 v=2 v=3 F2 (K = 450) v=0 v=1 v=2 v=3
Figure: Potential Energy Wells. CO has widely spaced levels. F2 has tightly packed levels.
29. The fundamental and first overtone transitions of $^{14}\text{N}^{16}\text{O}$ appeared at $1876.06 \text{ cm}^{-1}$ and $3724.20 \text{ cm}^{-1}$ respectively. Calculate the equilibrium vibration frequency, the anharmonicity, zero-point energy and the force constant of the molecule.
2021, 20255 Marks
Comprehensive Step-by-Step Solution:

Step 1: Set Up the Equations.
For an anharmonic oscillator, the energies of the fundamental transition ($v=0 \to 1$) and first overtone ($v=0 \to 2$) are derived as:

$$ \text{Fundamental: } \bar{\nu}_{0 \to 1} = \bar{\omega}_e(1 - 2x_e) = 1876.06 \quad \text{--- (Eq. 1)} $$
$$ \text{Overtone: } \bar{\nu}_{0 \to 2} = 2\bar{\omega}_e(1 - 3x_e) = 3724.20 \quad \text{--- (Eq. 2)} $$

Step 2: Solve for Anharmonicity ($x_e$).
Divide Eq. 2 by Eq. 1 to eliminate the equilibrium frequency $\bar{\omega}_e$:

$$ \frac{2\bar{\omega}_e(1 - 3x_e)}{\bar{\omega}_e(1 - 2x_e)} = \frac{3724.20}{1876.06} $$
$$ \implies \frac{2(1 - 3x_e)}{1 - 2x_e} = 1.98512 $$

Multiply both sides by $(1 - 2x_e)$:

$$ 2 - 6x_e = 1.98512(1 - 2x_e) $$
$$ \implies 2 - 6x_e = 1.98512 - 3.97024x_e $$

Group the $x_e$ terms on one side:

$$ 2 - 1.98512 = 6x_e - 3.97024x_e $$
$$ \implies 0.01488 = 2.02976 x_e $$
$$ \implies x_e = \frac{0.01488}{2.02976} = 0.00733 $$

Step 3: Solve for Equilibrium Vibrational Frequency ($\bar{\omega}_e$).
Substitute $x_e$ back into Eq. 1:

$$ \bar{\omega}_e [1 - 2(0.00733)] = 1876.06 $$
$$ \implies \bar{\omega}_e [0.98534] = 1876.06 $$
$$ \implies \bar{\omega}_e = \frac{1876.06}{0.98534} = 1903.97 \text{ cm}^{-1} $$

Step 4: Calculate the Zero-Point Energy (ZPE).
The ZPE is the energy of the molecule sitting in the absolute lowest ground state ($v=0$):

$$ \text{ZPE} = \varepsilon_0 = \frac{1}{2}\bar{\omega}_e \left(1 - \frac{1}{2}x_e\right) $$
$$ \implies \text{ZPE} = 0.5 \times 1903.97 \times \left(1 - \frac{0.00733}{2}\right) $$
$$ \implies \text{ZPE} = 951.985 \times (1 - 0.003665) $$
$$ \implies \text{ZPE} = 951.985 \times 0.996335 = 948.50 \text{ cm}^{-1} $$

Step 5: Calculate the Force Constant ($K$).
First, find the reduced mass ($\mu$) of NO in kilograms ($1 \text{ amu} = 1.6605 \times 10^{-27} \text{ kg}$):

$$ \mu = \frac{14 \times 16}{14 + 16} = \frac{224}{30} = 7.4667 \text{ amu} $$
$$ \implies \mu = 7.4667 \times 1.6605 \times 10^{-27} = 1.2398 \times 10^{-26} \text{ kg} $$

Now apply the formula relating wavenumber to force constant (where $c = 3 \times 10^8 \text{ m/s}$ and $\bar{\omega}_e$ must be converted to $\text{m}^{-1}$ by multiplying by 100):

$$ K = 4\pi^2 c^2 (\bar{\omega}_e \times 100)^2 \mu $$
$$ \implies K = 4(9.8696)(3 \times 10^8)^2 (190397)^2 (1.2398 \times 10^{-26}) $$
$$ \implies K = 39.478 \times (9 \times 10^{16}) \times (3.625 \times 10^{10}) \times (1.2398 \times 10^{-26}) $$
$$ \implies K = 1596.7 \text{ N/m} $$
Final Summary of Answers:
• Anharmonicity (xe): 0.00733
• Eq. Frequency (ωe): 1903.97 cm⁻¹
• Zero-Point Energy: 948.50 cm⁻¹
• Force Constant (K): 1596.7 N/m
30. If $\text{H}_2$ molecule behaves like a harmonic oscillator with a force constant K = 573 N/m, Calculate the vibrational quantum number corresponding to its 4.5 eV dissociation energy. [Given, M_H = 1.67 × 10⁻²⁷ kg].
2023 Q33 Marks
Step-by-Step Numerical Solution:

Step 1: Calculate the Reduced Mass ($\mu$).
For a homonuclear diatomic molecule like $\text{H}_2$, the formula $\mu = \frac{m \cdot m}{m + m}$ simplifies to half the mass of a single atom.

$$ \mu = \frac{M_H}{2} = \frac{1.67 \times 10^{-27}}{2} = 8.35 \times 10^{-28} \text{ kg} $$

Step 2: Calculate the Fundamental Vibrational Frequency ($\nu$).
Using the Hooke's law oscillator formula:

$$ \nu = \frac{1}{2\pi}\sqrt{\frac{K}{\mu}} = \frac{1}{2\pi}\sqrt{\frac{573}{8.35 \times 10^{-28}}} $$
$$ \implies \nu = \frac{1}{2\pi}\sqrt{6.862 \times 10^{29}} $$
$$ \implies \nu = \frac{1}{2\pi} (8.284 \times 10^{14}) = 1.318 \times 10^{14} \text{ Hz} $$

Step 3: Convert the Energy of a Single Quantum to Electron-Volts (eV).
To compare the energy of the state to the $4.5 \text{ eV}$ limit, we need the energy of a single jump ($h\nu$) in eV. We divide Joules by the elementary charge ($1.602 \times 10^{-19} \text{ J/eV}$).

$$ h\nu = (6.626 \times 10^{-34} \text{ J s}) \times (1.318 \times 10^{14} \text{ Hz}) = 8.736 \times 10^{-20} \text{ Joules} $$
$$ h\nu \text{ in eV} = \frac{8.736 \times 10^{-20}}{1.602 \times 10^{-19}} = 0.5453 \text{ eV} $$

Step 4: Solve for the Quantum Number ($v$).
The "dissociation energy" of 4.5 eV refers to $D_0$, the energy measured from the ground vibrational state ($v=0$) to the dissociation limit. In the harmonic oscillator model, the energy above $v=0$ is simply $vh\nu$. We set this equal to the dissociation energy:

$$ v \times h\nu = D_0 = 4.5 \text{ eV} $$
$$ \implies v = \frac{4.5}{0.5453} = 8.25 $$

Since quantum numbers must be strictly integers, and the vibrational energy at $v=8$ is $8 \times 0.5453 = 4.36 \text{ eV}$ (which is still below the available $4.5 \text{ eV}$ bond strength), the molecule can stably occupy this level. However, $v=9$ would require $9 \times 0.5453 = 4.91 \text{ eV}$ which exceeds the dissociation energy, causing the molecule to break. Therefore, the highest possible stable, bound state is $v = 8$.

Final Answer: The corresponding vibrational quantum number is v = 8.
31. Using the formula for the energy levels for the Morse potential... deduce the expression of energy spacing between adjacent levels. For $^{1}\text{H}^{35}\text{Cl}$, $D_e = 7.41 \times 10^{-19} \text{ J}$ and $\nu = 8.97 \times 10^{13} \text{ sec}^{-1}$, calculate the smallest value of n for which $\varepsilon_{n+1} - \varepsilon_n < 0.5(\varepsilon_1 - \varepsilon_0)$.
2024 Q35 Marks
Part 1: Deduce the Energy Spacing

The provided energy equation for state $n$ is:

$$ \varepsilon_n = h\nu(n+0.5) - \frac{(h\nu)^2}{4D_e}(n+0.5)^2 $$

The spacing between level $n$ and the next level $n+1$ is $\Delta \varepsilon_n = \varepsilon_{n+1} - \varepsilon_n$.

$$ \Delta \varepsilon_n = \left[ h\nu(n+1.5) - \frac{(h\nu)^2}{4D_e}(n+1.5)^2 \right] - \left[ h\nu(n+0.5) - \frac{(h\nu)^2}{4D_e}(n+0.5)^2 \right] $$

Group the linear terms and the squared terms:

$$ \Delta \varepsilon_n = h\nu[ (n+1.5) - (n+0.5) ] - \frac{(h\nu)^2}{4D_e}[ (n+1.5)^2 - (n+0.5)^2 ] $$

Simplify the brackets. The first bracket is exactly 1. The second bracket expands as $(n^2 + 3n + 2.25) - (n^2 + n + 0.25) = 2n + 2 = 2(n+1)$. Substitute these back:

$$ \Delta \varepsilon_n = h\nu(1) - \frac{(h\nu)^2}{4D_e}[ 2(n+1) ] $$
$$ \Delta \varepsilon_n = h\nu - \frac{(h\nu)^2}{2D_e}(n+1) $$

This is the required deduced expression for energy spacing.

Part 2: Solve the Numerical Inequality

We need to find when the spacing $\Delta \varepsilon_n$ becomes less than half the spacing of the very first ground state jump ($\Delta \varepsilon_0$). First, let's find the formula for $\Delta \varepsilon_0$ by plugging $n=0$ into our derived expression:

$$ \Delta \varepsilon_0 = \varepsilon_1 - \varepsilon_0 = h\nu - \frac{(h\nu)^2}{2D_e}(1) $$

Now set up the required inequality $\Delta \varepsilon_n < 0.5(\Delta \varepsilon_0)$:

$$ h\nu - \frac{(h\nu)^2}{2D_e}(n+1) < 0.5 \left[ h\nu - \frac{(h\nu)^2}{2D_e} \right] $$

Divide the entire inequality by $h\nu$ to make it simpler:

$$ 1 - \frac{h\nu}{2D_e}(n+1) < 0.5 \left[ 1 - \frac{h\nu}{2D_e} \right] $$

We need the value of the constant ratio $\frac{h\nu}{2D_e}$. Let's calculate it with the given constants:

$$ h\nu = (6.626 \times 10^{-34}) \times (8.97 \times 10^{13}) = 5.9435 \times 10^{-20} \text{ Joules} $$
$$ 2D_e = 2 \times 7.41 \times 10^{-19} = 1.482 \times 10^{-18} \text{ Joules} $$
$$ \frac{h\nu}{2D_e} = \frac{5.9435 \times 10^{-20}}{1.482 \times 10^{-18}} = 0.0401 $$

Now substitute this ratio ($0.0401$) back into the inequality:

$$ 1 - 0.0401(n+1) < 0.5(1 - 0.0401) $$
$$ \implies 1 - 0.0401(n+1) < 0.5(0.9599) $$
$$ \implies 1 - 0.0401(n+1) < 0.47995 $$
$$ \implies 1 - 0.47995 < 0.0401(n+1) $$
$$ \implies 0.52005 < 0.0401(n+1) $$
$$ \implies \frac{0.52005}{0.0401} < n+1 $$
$$ \implies 12.968 < n+1 \implies n > 11.968 $$
Final Answer: Since n must be an integer, the absolute smallest value that satisfies the condition is n = 12.
32. The fundamental vibrational frequency of $^{1}\text{H}^{127}\text{I}$ is 2309 cm⁻¹. Calculate the force constant for this molecule in N m⁻¹.
2022 Q32 Marks
Step-by-Step Numerical Solution:

Step 1: Calculate the Reduced Mass ($\mu$).
Convert the atomic masses to kilograms using the atomic mass unit ($1 \text{ amu} = 1.6605 \times 10^{-27} \text{ kg}$).

$$ \mu = \frac{1 \times 127}{1 + 127} = \frac{127}{128} \text{ amu} = 0.9921875 \text{ amu} $$
$$ \implies \mu = 0.9921875 \times 1.6605 \times 10^{-27} = 1.6475 \times 10^{-27} \text{ kg} $$

Step 2: Relate Wavenumber to the Force Constant ($k$).
The fundamental frequency in wavenumber ($\bar{\nu}$) is given by $\bar{\nu} = \frac{1}{2\pi c}\sqrt{\frac{k}{\mu}}$. Squaring both sides and rearranging for $k$ gives:

$$ k = 4\pi^2 c^2 \bar{\nu}^2 \mu $$

Step 3: Execute Final Calculation.
We must convert the wavenumber $\bar{\nu}$ to standard SI units (meters) by multiplying by 100.

$$ \bar{\nu} = 2309 \text{ cm}^{-1} = 2.309 \times 10^5 \text{ m}^{-1} $$

Substitute all values into the equation:

$$ k = 4 \times (9.8696) \times (2.998 \times 10^8)^2 \times (2.309 \times 10^5)^2 \times (1.6475 \times 10^{-27}) $$
$$ \implies k = 39.478 \times (8.988 \times 10^{16}) \times (5.331 \times 10^{10}) \times (1.6475 \times 10^{-27}) $$
$$ \implies k = 3115.1 \times 10^{-1} = 311.51 \text{ N/m} $$
Final Answer: The force constant of the HI molecule is 311.5 N/m.
Module 4: Raman Spectroscopy

💡 Pre-Topic Note & Symbol Dictionary

  • Raman Scattering: Light hits a molecule and bounces off. If it bounces off with LESS energy, it's a Stokes line. If it bounces off with MORE energy, it's an Anti-Stokes line.
  • Activity Rule: Polarizability ($\alpha$, squishiness of the electron cloud) MUST change during the motion.
33. State the selection rule for Rotational Raman and Vibrational Raman spectroscopy.
2025 Q32 Marks
Detailed Exam Answer:

1. Pure Rotational Raman Selection Rule:

$$ \Delta J = 0, \pm 2 $$
  • $\Delta J = 0$ corresponds to elastic Rayleigh scattering (no energy transfer).
  • $\Delta J = +2$ corresponds to Stokes rotational Raman lines (molecule gains rotational energy from the photon).
  • $\Delta J = -2$ corresponds to Anti-Stokes lines (molecule loses energy to the photon).

2. Vibrational Raman Selection Rule:

For an anharmonic oscillator (a real molecule), the rule is:

$$ \Delta v = \pm 1, \pm 2, \pm 3, \dots $$

Where $\Delta v = \pm 1$ represents the intense fundamental transitions, and $\pm 2, \pm 3$ represent the very weak overtone transitions.

34. Which of the following molecules are rotational Raman active? $\text{Br}_2, \text{HBr}, \text{HCN}, \text{CS}_2$.
2024 Q12 Marks
Detailed Exam Answer:

The Active Criterion: To be rotational Raman active, a molecule's polarizability ellipsoid must be anisotropic. This means the electron cloud must look different from different angles, so as the molecule rotates, its overall polarizability in space changes periodically.

Spherically symmetric molecules (like $CH_4$ or $SF_6$) are completely uniform from all angles, so they are Raman inactive. However, all linear molecules (whether they have a dipole moment or not) are anisotropic because their electron cloud is stretched along the bond axis. As they spin, the stretched cloud rotates, changing the polarizability.

Conclusion: Since Br₂, HBr, HCN, and CS₂ are all perfectly linear molecules, their polarizability changes during rotation. Therefore, all four molecules are rotational Raman active.
35. Why the term $\pm 2$ appears in the selection rule of pure rotational Raman transitions?
2023 Q22 Marks
Detailed Exam Answer:

The transition rule $\Delta J = \pm 2$ in rotational Raman scattering arises directly from the mathematical symmetry of the molecular polarizability ellipsoid.

Consider a linear molecule like $\text{CO}_2$. If you rotate it $180^\circ$ (a half-turn) end-over-end, the molecule looks completely identical to how it started, and its electron cloud (polarizability ellipsoid) returns to its exact original orientation. Therefore, during one full $360^\circ$ rotation of the molecule, the polarizability completes two full cycles.

Because the polarizability cycles twice per physical rotation, the induced dipole moment created by the laser light oscillates at twice the frequency of rotation ($2\nu_{rot}$). In quantum mechanical terms, this means the scattering photon interacts with two quanta of rotational angular momentum simultaneously, leading to the strict selection rule $\Delta J = \pm 2$.

36. "The nature of Raman spectrum of a substance depends on both the nature of molecules and the wavelength of incident radiation" — Justify or criticize.
2023 Q32 Marks
Detailed Exam Answer:

This statement is partially incorrect because the structural "fingerprint" of the spectrum does not depend on the laser used.

1. Why it depends on the nature of molecules (True):
The spacing between the Raman lines and the central laser line is called the Raman shift ($\Delta \bar{\nu}$). This shift represents the exact vibrational or rotational energy gap of the molecule ($\Delta E$). Because energy gaps are determined solely by the atomic masses and bond strengths of the specific molecule, the structural pattern of the Raman shifts is a unique fingerprint of the molecule.

2. Why it does NOT depend on the wavelength of incident radiation (False regarding structure):
The Raman shift is a relative difference ($\bar{\nu}_{laser} - \bar{\nu}_{scattered}$). If you use a green laser or a red laser, the absolute positions of the scattered lines will change, but the Raman shifts (the distance from the laser line) will remain exactly the same. Thus, the fundamental "nature" or pattern of the spectrum is completely independent of the incident wavelength.

(Caveat: The intensity of the lines is proportional to $1/\lambda^4$. So a blue laser will produce a brighter spectrum than a red laser, but the pattern of lines remains identical).

37. Write the mutual exclusion rule in the context of vibrational spectroscopy.
2021 Q55 Marks
Detailed Exam Answer:

The Rule of Mutual Exclusion is a fundamental principle in molecular spectroscopy used to identify the structural symmetry of a molecule.

Statement of the Rule:
For any molecule that possesses a center of symmetry (an inversion center, $i$), its normal modes of vibration are mutually exclusive. This means a vibrational mode can be either Infrared (IR) active or Raman active, but it can never be both simultaneously. (Additionally, some complex modes may be inactive in both).

Physical Justification:

  • Symmetric Vibrations: These motions preserve the molecule's center of inversion. Because the molecule remains perfectly balanced, the dipole moment remains zero ($\Delta \mu = 0$). Thus, it is IR inactive. However, the stretching/compressing changes the volume of the electron cloud, altering polarizability. Thus, it is Raman active.
  • Asymmetric Vibrations: These motions destroy the center of inversion. This imbalance creates a dynamic dipole moment ($\Delta \mu \neq 0$), making it IR active. However, the changes in polarizability on one side of the molecule are exactly cancelled by the other side, leaving the net polarizability unchanged. Thus, it is Raman inactive.
38. The symmetric stretching mode of vibration of $\text{CO}_2$ is Raman active but IR inactive — Justify.
2025, 20222 Marks
Detailed Exam Answer:

This is a classic demonstration of the Rule of Mutual Exclusion, since $\text{CO}_2$ ($\text{O=C=O}$) possesses a center of symmetry at the Carbon atom.

Why is it IR Inactive?
During the symmetric stretch, both oxygen atoms pull away from the central carbon atom in opposite directions at the exact same time. The individual $C=O$ bond dipoles are always equal and directly opposing. Because they cancel each other out completely at every moment, the net dipole moment of the molecule never changes ($\Delta \mu = 0$). Without a changing dipole, it cannot absorb IR radiation.

Why is it Raman Active?
Even though the molecule remains perfectly balanced, the physical size of the molecule changes. As the bonds stretch outward, the electron cloud expands, making it "looser" and easier for an external laser field to distort. As the bonds compress, the cloud becomes tighter and harder to distort. This periodic change in the ease of distortion (polarizability, $\Delta \alpha \neq 0$) allows the molecule to inelastically scatter light, making it Raman active.

39. What are Stokes and Anti-Stokes lines in the Raman spectra?
2023 Q12 Marks
Detailed Exam Answer:

When monochromatic laser light hits a sample, most photons bounce off elastically with no energy change (Rayleigh scattering). However, a tiny fraction of photons undergo inelastic Raman scattering, emerging with different energies. These shifted lines form the Raman spectrum.

v=0 v=1 Virtual Rayleigh Stokes Anti-Stokes
Figure: Energy level diagram showing Rayleigh, Stokes, and Anti-Stokes scattering.

1. Stokes Lines:
These are scattered spectral lines that appear at a lower frequency (lower energy, longer wavelength) than the incident laser light. They occur when an incoming photon hits a molecule in its ground state. The molecule steals some of the photon's energy to jump to a higher vibrational or rotational energy level. The photon scatters away with less energy ($\bar{\nu}_{Stokes} < \bar{\nu}_{inc}$). Because most molecules sit in the ground state at room temperature, Stokes lines are relatively strong.

2. Anti-Stokes Lines:
These are scattered spectral lines that appear at a higher frequency (higher energy, shorter wavelength) than the incident laser light. They occur when an incoming photon hits a molecule that is already in an excited state. The molecule drops back to the ground state, dumping its extra thermal energy into the photon. The photon scatters away with more energy ($\bar{\nu}_{Anti-Stokes} > \bar{\nu}_{inc}$). Because very few molecules naturally sit in excited states, Anti-Stokes lines are very weak.

40. Mention the separation between first stoke and first anti-stoke lines in Raman spectra.
2025 Q11 Mark
Detailed Exam Answer:

In a pure rotational Raman spectrum, the positions of the lines relative to the central excitation (Rayleigh) line are governed by the equation $\Delta \bar{\nu} = B(4J + 6)$, where $J$ is the lower rotational state.

  • The first Stokes line originates from the $J=0 \to 2$ transition. Its position is $\bar{\nu}_{inc} - 6B$.
  • The first Anti-Stokes line originates from the $J=2 \to 0$ transition (the molecule must be in an excited state $J=2$). Its position is $\bar{\nu}_{inc} + 6B$.

To find the total separation distance between them, we subtract their positions:

$$ \text{Separation} = (\bar{\nu}_{inc} + 6B) - (\bar{\nu}_{inc} - 6B) = 6B + 6B = 12B $$
Final Answer: The separation between the first Stokes and first Anti-Stokes line is exactly 12B.
41. Derive the expression for the transition frequency of stokes and antistokes lines for a linear molecule by considering only rotational energy.
2025, 20223 Marks
Complete Mathematical Derivation:

Step 1: Set Up Rotational Energy Equations.
The rotational energy levels of a rigid linear molecule (in wavenumbers) are given by:

$$ \varepsilon_J = B J(J+1) $$

Step 2: Apply the Raman Selection Rule.
The selection rule for a pure rotational Raman transition is $\Delta J = \pm 2$. Let us calculate the energy difference ($\Delta \varepsilon$) when a molecule jumps from a lower state $J$ to the higher state $J+2$ (an excitation):

$$ \Delta \varepsilon = \varepsilon_{J+2} - \varepsilon_J $$
$$ \implies \Delta \varepsilon = B(J+2)[(J+2)+1] - B J(J+1) $$
$$ \implies \Delta \varepsilon = B(J+2)(J+3) - B J(J+1) $$

Expand the polynomials inside the brackets:

$$ \implies \Delta \varepsilon = B(J^2 + 3J + 2J + 6) - B(J^2 + J) $$
$$ \implies \Delta \varepsilon = B(J^2 + 5J + 6 - J^2 - J) $$
$$ \implies \Delta \varepsilon = B(4J + 6) \text{ cm}^{-1} $$

This is the energy exchanged between the photon and the molecule.

Step 3: Derive Wavenumber Equations for Scattered Light.
The wavenumber of the scattered light ($\bar{\nu}_{scat}$) depends on whether the photon lost or gained this energy.

  • Stokes Lines: The photon gives energy to the molecule. It scatters with less energy. Here, $J$ refers to the lower rotational state involved in the transition ($J \to J+2$):
    $$ \bar{\nu}_{Stokes} = \bar{\nu}_{inc} - B(4J + 6) $$
  • Anti-Stokes Lines: The photon steals energy from an already-rotating molecule. It scatters with more energy. Here, $J$ also refers to the lower (final) rotational state in the transition ($J+2 \to J$), so the same shift formula applies:
    $$ \bar{\nu}_{Anti-Stokes} = \bar{\nu}_{inc} + B(4J + 6) $$
    Note: The first Anti-Stokes line corresponds to the $J=2 \to 0$ transition (the molecule must be in an excited state, $J \geq 2$), giving a shift of $B(4 \times 0 + 6) = 6B$.
42. In the pure microwave spectrum of $\text{XY}$ molecule, the adjacent lines are separated by 4 cm⁻¹. If the molecule is irradiated by a radiation of 30,000 cm⁻¹, find the position of first stokes line.
2022 Q12 Marks
Step-by-Step Numerical Solution:

Step 1: Find the Rotational Constant ($B$).
We are given data from the pure microwave (absorption) spectrum. The fundamental rule for a microwave spectrum is that adjacent lines are separated by $2B$.

$$ \Delta \bar{\nu}_{microwave} = 2B = 4 \text{ cm}^{-1} $$
$$ \implies B = \frac{4}{2} = 2 \text{ cm}^{-1} $$

Step 2: Calculate the Position of the First Stokes Line.
Now we switch to Raman scattering logic. In a pure rotational Raman spectrum, the first Stokes line appears shifted by exactly $6B$ to the lower energy side of the exciting laser line.

$$ \text{Raman Shift} = 6B = 6(2) = 12 \text{ cm}^{-1} $$

The position is the incident radiation minus the shift:

$$ \bar{\nu}_{Stokes} = \bar{\nu}_{inc} - 12 $$
$$ \implies \bar{\nu}_{Stokes} = 30,000 - 12 = 29,988 \text{ cm}^{-1} $$
Final Answer: The position of the first Stokes line is 29,988 cm⁻¹.
43. A laser Raman spectrometer operating at 532 nm is used to record the vibrational spectrum of $\text{Cl}_2$ having its fundamental vibration at 560 cm⁻¹. Calculate the position of Stokes line corresponding to this vibration.
2024 Q22 Marks
Step-by-Step Numerical Solution:

Step 1: Convert the Incident Laser Wavelength to Wavenumber.
The spectrometer uses a green laser at $532 \text{ nm}$. We must convert this to $\text{cm}^{-1}$ to match the vibrational units.

$$ \lambda = 532 \text{ nm} = 532 \times 10^{-9} \text{ m} = 532 \times 10^{-7} \text{ cm} $$
$$ \bar{\nu}_{inc} = \frac{1}{\lambda} = \frac{1}{532 \times 10^{-7} \text{ cm}} $$
$$ \implies \bar{\nu}_{inc} = \frac{10^7}{532} \approx 18,796.99 \text{ cm}^{-1} $$

Step 2: Calculate the Stokes Line Position.
This is a vibrational Raman transition. The molecule steals energy equal to its fundamental vibrational frequency ($560 \text{ cm}^{-1}$). The scattered photon will have less energy.

$$ \bar{\nu}_{Stokes} = \bar{\nu}_{inc} - \Delta \bar{\nu}_{vibration} $$
$$ \implies \bar{\nu}_{Stokes} = 18,796.99 - 560 = 18,236.99 \text{ cm}^{-1} $$
Final Answer: The position of the Stokes line is 18,236.99 cm⁻¹.
44. The rotational raman displacement for $\text{HCl}$ molecule is 41.6 cm⁻¹. Calculate the internuclear distance between the atoms in angstrom. (reduced mass for $\text{HCl}$ is 1.61 × 10⁻²⁷ kg).
2022 Q32 Marks
Step-by-Step Numerical Solution:

Step 1: Relate the Raman Displacement to the Rotational Constant ($B$).
In a rotational Raman spectrum, the displacement (spacing) between any two adjacent rotational lines is $4B$.

$$ \Delta \bar{\nu} = 4B = 41.6 \text{ cm}^{-1} $$
$$ \implies B = \frac{41.6}{4} = 10.4 \text{ cm}^{-1} $$

Convert $B$ to strict SI units ($\text{m}^{-1}$) for proper calculation:

$$ B = 10.4 \times 100 = 1040 \text{ m}^{-1} $$

Step 2: Calculate the Moment of Inertia ($I$).
Using the definition of $B$:

$$ B = \frac{h}{8\pi^2 I c} \implies I = \frac{h}{8\pi^2 B c} $$

Substitute the constants ($h = 6.626 \times 10^{-34} \text{ J s}$, $c = 2.998 \times 10^8 \text{ m/s}$):

$$ I = \frac{6.626 \times 10^{-34}}{8 \times (9.8696) \times 1040 \times (2.998 \times 10^8)} $$
$$ \implies I = \frac{6.626 \times 10^{-34}}{2.461 \times 10^{13}} \approx 2.692 \times 10^{-47} \text{ kg m}^2 $$

Step 3: Calculate the Internuclear Distance ($r$).
The moment of inertia is related to bond length by $I = \mu r^2$.

$$ r = \sqrt{\frac{I}{\mu}} = \sqrt{\frac{2.692 \times 10^{-47}}{1.61 \times 10^{-27}}} $$
$$ \implies r = \sqrt{1.672 \times 10^{-20}} \approx 1.293 \times 10^{-10} \text{ m} $$

Convert to Angstroms ($1 \text{ \AA} = 10^{-10} \text{ m}$):

$$ r = 1.293 \text{ \AA} $$
Final Answer: The internuclear distance is 1.29 Å.
Module 5: Nuclear Magnetic Resonance (NMR)

💡 Pre-Topic Note & Symbol Dictionary

  • Spin ($I$): Nucleus must have spin to be NMR active.
  • Larmor Precession: Nucleus wobbles around the magnetic field at a specific frequency $\nu$.
  • Chemical Shift ($\delta$): Electrons shield the nucleus, shifting its frequency slightly (measured in ppm).
  • $n+1$ Rule: Neighboring protons split the signal into multiple peaks.
45. What is the criterion of a molecule to be NMR active?
2022 Q31 Mark
Detailed Exam Answer:

The essential criterion for a nucleus (and thus the molecule) to be NMR active is that the nucleus must possess a non-zero nuclear spin quantum number ($I > 0$). This occurs when the nucleus contains an odd number of protons, an odd number of neutrons, or both (for example, $^1\text{H}$, $^{13}\text{C}$, $^{19}\text{F}$). A non-zero spin gives the nucleus a magnetic dipole moment, allowing it to interact with an applied external magnetic field.

46. $^{12}\text{C}$ and $^{16}\text{O}$ do not show NMR spectra-Explain.
2025 Q12 Marks
Detailed Exam Answer:

According to the rules of nuclear physics, if an isotope has an even atomic number (even number of protons) AND an even mass number (even number of total nucleons), all its protons and neutrons pair up perfectly. Their individual spins cancel each other out entirely.

  • $^{12}\text{C}$ has 6 protons and 6 neutrons (both even).
  • $^{16}\text{O}$ has 8 protons and 8 neutrons (both even).

As a result, the net nuclear spin quantum number is exactly zero ($I=0$). Without angular momentum, they lack a magnetic dipole moment, meaning they cannot interact with external magnetic fields and are completely NMR inactive.

47. What are the transitions responsible for NMR spectrum?
2024 Q11 Mark
Detailed Exam Answer:

The transitions responsible for an NMR spectrum occur between the nuclear spin energy states (also known as nuclear Zeeman levels). When a magnetic nucleus is placed in an external magnetic field, its spin states split into lower and higher energy levels (e.g., aligned with the field vs. aligned against it). The NMR spectrum is produced when the nucleus absorbs a radiofrequency photon and flips its spin alignment from the lower energy state to the higher energy state.

48. Write down the selection rule in NMR spectroscopy.
2025 Q11 Mark
Detailed Exam Answer:

The quantum mechanical selection rule governing transitions between nuclear spin states in NMR spectroscopy is:

$$ \Delta m_I = \pm 1 $$

Where $m_I$ is the nuclear magnetic spin quantum number (the projection of the nuclear spin along the axis of the external magnetic field). A nucleus can only jump to immediately adjacent spin states.

49. Write an expression for the spin energy level of a nucleus having a nuclear spin I placed in a magnetic field H.
2024 Q23 Marks
💡 Symbol Dictionary:
  • $E_{m_I}$ : The specific energy of the spin state in Joules.
  • $g$ : The nuclear g-factor (a unique dimensionless constant for each type of nucleus).
  • $\beta_N$ : The nuclear magneton (a fundamental physical constant).
  • $H_0$ : The strength of the external applied magnetic field (in Tesla).
  • $m_I$ : The magnetic quantum number.
Detailed Exam Answer:

When a nucleus with spin quantum number $I$ is placed in a strong external magnetic field $H_0$, its degenerate energy levels split into $2I + 1$ distinct Zeeman states. The energy of any one of these specific spin states is given by the expression:

$$ E_{m_I} = - g \beta_N m_I H_0 $$

Because the magnetic quantum number $m_I$ can take values from $-I, -I+1, \dots, +I$, this equation generates a ladder of equally spaced energy levels. (For a proton where $I=1/2$, $m_I$ can be $+1/2$ or $-1/2$).

50. What is a nuclear magneton?
2023 Q31 Mark
Detailed Exam Answer:

The nuclear magneton ($\beta_N$) is a fundamental physical constant of nature. It serves as the standard, natural unit for expressing and measuring the magnetic dipole moments of heavy particles like protons and neutrons (nucleons). It is essentially the magnetic moment generated by a single proton spinning due to quantum mechanics.

It is mathematically defined as $\beta_N = \frac{eh}{4\pi m_p}$, where $e$ is the elementary charge, $h$ is Planck's constant, and $m_p$ is the rest mass of a proton.

51. Write down the expression of nuclear magneton, $\beta_N$ and calculate the angular momentum and magnetic moment values for a proton. (nuclear g factor: g = 5.585, $\beta_N$ = 5.047 × 10⁻²⁷ J T⁻¹).
2020 Q85 Marks
Step-by-Step Calculation:

1. Expression for Nuclear Magneton:

$$ \beta_N = \frac{eh}{4\pi m_p} $$

2. Calculate Angular Momentum ($L$) for a Proton:
A proton has a spin quantum number of $I = 1/2$. The magnitude of its quantum spin angular momentum is given by:

$$ L = \frac{h}{2\pi} \sqrt{I(I+1)} $$

Substitute $I=0.5$ and Planck's constant $h = 6.626 \times 10^{-34} \text{ J s}$:

$$ \sqrt{I(I+1)} = \sqrt{0.5 \times 1.5} = \sqrt{0.75} = \frac{\sqrt{3}}{2} \approx 0.8660 $$
$$ \implies L = \frac{6.626 \times 10^{-34}}{2\pi} \times 0.8660 $$
$$ \implies L = (1.054 \times 10^{-34}) \times 0.8660 \approx 9.13 \times 10^{-35} \text{ J s} $$

3. Calculate Magnetic Moment ($\mu_{mag}$) for a Proton:
The magnetic dipole moment relates to the spin by the equation:

$$ \mu_{mag} = g \beta_N \sqrt{I(I+1)} $$

Substitute the given values ($g = 5.585, \beta_N = 5.047 \times 10^{-27}$):

$$ \mu_{mag} = 5.585 \times (5.047 \times 10^{-27}) \times 0.8660 $$
$$ \implies \mu_{mag} = 28.187 \times 10^{-27} \times 0.8660 \approx 2.44 \times 10^{-26} \text{ J T}^{-1} $$
Final Answers:
• Angular Momentum L = 9.13 × 10⁻³⁵ J s.
• Magnetic Moment μ_mag = 2.44 × 10⁻²⁶ J T⁻¹.
52. Briefly describe the Larmor precession in the context of NMR spectroscopy.
2021 Q25 Marks
Detailed Description:

When a spinning nucleus with a magnetic dipole moment is placed in a strong, static external magnetic field ($H_0$), it experiences a magnetic twisting force (torque, $\tau = \mu \times H_0$). Because the nucleus has angular momentum, it does not just flop over and align perfectly with the field.

Instead, the spin axis of the nucleus begins to tilt and rotate around the direction of the external magnetic field, sweeping out a cone shape. This gyroscopic wobbling motion is called Larmor Precession. It is physically identical to how a spinning toy top wobbles around the axis of gravity before falling over.

B₀ μ (Spin)
Figure: The red magnetic moment precessing in a cone around the blue external magnetic field (B0).

The rate at which the nucleus sweeps out this cone is called the Larmor Frequency ($\nu = \frac{\gamma H_0}{2\pi}$). This concept is the entire foundation of NMR: to make a nucleus absorb energy and flip its spin state, the NMR machine must fire radio waves at the sample that match this exact precession frequency. When the frequencies match, resonance occurs.

53. Calculate the frequency of electromagnetic radiation required for transition when a bare proton is placed under an external magnetic field of 1 T. [Given: g = 5.585, $\beta_N$ = 5.052 × 10⁻²⁴ erg G⁻¹].
2021 Q25 Marks
Step-by-Step Numerical Solution:

Step 1: Standardize the Units to CGS.
The provided nuclear magneton ($\beta_N$) is given in CGS units ($\text{erg G}^{-1}$). Therefore, we must convert the magnetic field ($H_0$) from Tesla to Gauss, and use the CGS value for Planck's constant ($h$).

  • Magnetic Field: $H_0 = 1 \text{ Tesla} = 10,000 \text{ Gauss}$.
  • Planck's Constant: $h = 6.626 \times 10^{-27} \text{ erg s}$.

Step 2: Apply the Larmor Resonance Formula.
The frequency required to trigger a transition is:

$$ \nu = \frac{g \beta_N H_0}{h} $$

Step 3: Execute the Calculation.

$$ \nu = \frac{5.585 \times (5.052 \times 10^{-24}) \times 10,000}{6.626 \times 10^{-27}} $$
$$ \implies \nu = \frac{28.2154 \times 10^{-24} \times 10^4}{6.626 \times 10^{-27}} $$
$$ \implies \nu = \frac{28.2154 \times 10^{-20}}{6.626 \times 10^{-27}} $$
$$ \implies \nu = 4.258 \times 10^7 \text{ Hz} $$

Convert to Megahertz ($\text{MHz}$) by dividing by $10^6$:

$$ \implies \nu = 42.58 \text{ MHz} $$
Final Answer: The required frequency is 42.58 MHz.
54. For a proton the gyromagnetic ratio is 26.752 × 10⁷ rad T⁻¹. Calculate the Larmor frequency (in MHz) in a 21.1 Tesla magnetic field.
2024 Q22 Marks
💡 Symbol Dictionary:
  • $\gamma$ : Gyromagnetic ratio (combines $g$ and $\beta_N$).
Step-by-Step Numerical Solution:

The relationship between the Larmor frequency and the gyromagnetic ratio is:

$$ \nu = \frac{\gamma H_0}{2\pi} $$

Substitute the given values ($\gamma = 26.752 \times 10^7 \text{ rad/T}$ and $H_0 = 21.1 \text{ T}$):

$$ \nu = \frac{(26.752 \times 10^7) \times 21.1}{2 \times 3.14159} $$
$$ \implies \nu = \frac{564.467 \times 10^7}{6.28318} = 89.837 \times 10^7 \text{ Hz} $$
$$ \implies \nu = 8.9837 \times 10^8 \text{ Hz} $$

Convert to Megahertz (divide by $10^6$):

$$ \implies \nu = 898.37 \text{ MHz} $$
Final Answer: The Larmor frequency is 898.37 MHz. (This represents a very powerful, modern 900 MHz NMR spectrometer).
55. What magnetic field is required for proton magnetic resonance at 220 MHz? [Given, g = 5.585].
2023 Q12 Marks
Step-by-Step Numerical Solution:

Step 1: Rearrange the Resonance Equation.
Starting with $\nu = \frac{g \beta_N H_0}{h}$, we solve for the magnetic field $H_0$:

$$ H_0 = \frac{\nu \times h}{g \beta_N} $$

Step 2: Format the Constants in SI Units.

  • Target Frequency: $\nu = 220 \text{ MHz} = 220 \times 10^6 \text{ Hz}$.
  • Planck's Constant: $h = 6.626 \times 10^{-34} \text{ J s}$.
  • Nuclear Magneton: $\beta_N = 5.051 \times 10^{-27} \text{ J/T}$ (Standard SI value).

Step 3: Execute Calculation.

$$ H_0 = \frac{(220 \times 10^6) \times (6.626 \times 10^{-34})}{5.585 \times (5.051 \times 10^{-27})} $$
$$ \implies H_0 = \frac{1.4577 \times 10^{-25}}{2.8209 \times 10^{-26}} \approx 5.167 \text{ Tesla} $$
Final Answer: A magnetic field strength of 5.17 Tesla is required.
56. Calculate the resonance frequency of $^{19}\text{F}$ nucleus in an NMR spectrometer operating at a magnetic field strength of 16.45 T [given, g = 5.255, $\beta_N$ = 5.05 × 10⁻²⁷ J T⁻¹].
2022 Q32 Marks
Step-by-Step Numerical Solution:

Using the standard resonance equation:

$$ \nu = \frac{g \beta_N H_0}{h} $$

Substitute all the given values directly:

$$ \nu = \frac{5.255 \times (5.05 \times 10^{-27}) \times 16.45}{6.626 \times 10^{-34}} $$
$$ \implies \nu = \frac{436.54 \times 10^{-27}}{6.626 \times 10^{-34}} = 65.88 \times 10^7 \text{ Hz} = 6.588 \times 10^8 \text{ Hz} $$
Final Answer: The resonance frequency for the Fluorine-19 nucleus is 658.8 MHz.
57. The signal for $\text{CH}_2$ protons in a compound appears at $\delta$ 4.6. Calculate the difference in frequency expressed in Hertz between this signal and TMS signal in a 300 MHz instrument.
2022 Q12 Marks

💡 Concept / Theory

Because absolute Larmor frequencies are massive (e.g., $300,000,000 \text{ Hz}$) and the tiny shifts caused by electron shielding are tiny (e.g., $100 \text{ Hz}$), scientists created the Chemical Shift ($\delta$) scale. It measures how far a peak has shifted away from a reference compound (Tetramethylsilane, TMS) and divides it by the total power of the machine. This makes $\delta$ a universal number (in parts per million, ppm) regardless of whether you use a $300 \text{ MHz}$ or $900 \text{ MHz}$ machine.

💡 Symbol Dictionary:
  • $\delta$ : Chemical shift in parts per million (ppm).
  • $\Delta \nu$ : The raw frequency difference in Hertz between the sample and TMS.
Step-by-Step Numerical Solution:

The formula defining chemical shift is:

$$ \delta \text{ (ppm)} = \frac{\Delta \nu \text{ (in Hz)}}{\text{Operating Frequency of Spectrometer (in MHz)}} $$

We are asked to find the raw frequency difference ($\Delta \nu$). Rearranging the formula:

$$ \Delta \nu = \delta \times \text{Spectrometer Freq} $$

Substitute the given shift ($\delta = 4.6$) and the machine power ($300 \text{ MHz}$):

$$ \Delta \nu = 4.6 \times 300 = 1380 \text{ Hz} $$
Final Answer: The signal appears 1380 Hz away from the TMS signal.
58. At a magnetic flux density of 1.65 T the frequency of separation between protons in benzene and TMS is 510.5 Hz. Calculate the chemical shift [given: g = 5.585, $\beta_N$ = 5.05 × 10⁻²⁷ J T⁻¹].
2025 Q33 Marks
Step-by-Step Numerical Solution:

To use the chemical shift formula ($\delta = \frac{\Delta \nu}{\nu_{spec}}$), we first need to calculate the operating frequency of the spectrometer ($\nu_{spec}$ in MHz) using the given magnetic field.

Step 1: Calculate the Spectrometer Frequency ($\nu_{spec}$)

$$ \nu_{spec} = \frac{g \beta_N H_0}{h} $$
$$ \implies \nu_{spec} = \frac{5.585 \times (5.05 \times 10^{-27}) \times 1.65}{6.626 \times 10^{-34}} $$
$$ \implies \nu_{spec} = \frac{46.537 \times 10^{-27}}{6.626 \times 10^{-34}} \approx 7.023 \times 10^7 \text{ Hz} = 70.23 \text{ MHz} $$

Step 2: Calculate the Chemical Shift ($\delta$).
We are given that the raw frequency separation is $\Delta \nu = 510.5 \text{ Hz}$.

$$ \delta = \frac{\Delta \nu \text{ (Hz)}}{\nu_{spec} \text{ (MHz)}} $$
$$ \implies \delta = \frac{510.5}{70.23} \approx 7.268 \text{ ppm} $$
Final Answer: The chemical shift of the benzene protons is 7.27 ppm.
59. Predict the $^{1}\text{H}$-NMR signal pattern for $\text{CH}_3\text{CHDOH}$ under low and high resolution.
2021 Q55 Marks

💡 Concept / Theory

$n+1$ Rule: If a proton has $n$ equivalent neighboring protons on adjacent carbons, its signal splits into $n+1$ peaks due to spin-spin coupling. (e.g., 2 neighbors = triplet).
Deuterium (D): Deuterium ($^2\text{H}$) is invisible to a proton ($^1\text{H}$) NMR scan because it resonates at a completely different frequency. However, D has a nuclear spin of $I=1$, so it does cause splitting. The splitting rule for a nucleus with spin $I$ is $(2 n I + 1)$.

Detailed Exam Answer:

The molecule is monodeuterated ethanol: $\text{CH}_3-\text{CHD}-\text{OH}$.

Part 1: Low-Resolution Spectrum (No Splitting)
Under low resolution, the machine cannot see spin coupling. It only sees the distinct chemical environments. There are three groups of protons:

  1. The methyl group ($\text{CH}_3$): 3 protons.
  2. The methine group ($\text{CHD}$): 1 proton.
  3. The hydroxyl group ($\text{OH}$): 1 proton.
Prediction: The low-res spectrum will show exactly three single, broad peaks with an area integration ratio of 3 : 1 : 1.

Part 2: High-Resolution Spectrum (With Splitting)
Under high resolution, nearby magnetic nuclei interfere with each other, splitting the peaks.

  • $\text{CH}_3$ Protons (3H): They are adjacent to the single proton in the $\text{CHD}$ group. Using the $n+1$ rule ($1+1=2$), this signal splits into a doublet. (Note: These protons also couple weakly with the adjacent Deuterium via $^3J_{HD}$ coupling, which in principle would further split the doublet into a doublet of triplets. However, this long-range H-D coupling constant is typically very small ($< 1 \text{ Hz}$) and is often not resolved in routine spectra, so the signal is commonly observed as a simple doublet.)
  • $\text{OH}$ Proton (1H): In standard samples, the acidic hydroxyl proton undergoes rapid chemical exchange with trace moisture. This constant swapping blurs out any coupling. Therefore, it appears as a sharp singlet.
  • $\text{CHD}$ Proton (1H): This is highly complex. It couples with the three $\text{CH}_3$ protons ($n=3 \implies 3+1=4$, yielding a quartet).
    It ALSO couples with the attached Deuterium atom. For Deuterium, $I=1$ and $n=1$. The splitting formula gives $(2 \times 1 \times 1) + 1 = 3$ (a triplet).
    Because it couples with both, the signal splits into a quartet, and then every line of the quartet splits into a triplet. The result is a quartet of triplets (12 total lines).
60. Predict the high resolution NMR spectra of $\text{CH}_3\text{CHDCl}$.
2024 Q12 Marks
Detailed Exam Answer:

The molecule is 1-chloro-1-deuterioethane: $\text{CH}_3-\text{CHD}-\text{Cl}$. There are two distinct groups of protons to analyze.

  • $\text{CH}_3$ Methyl Protons (3H):
    These three equivalent protons have exactly one neighboring proton (on the $\text{CHD}$ carbon). Using the $n+1$ rule where $n=1$, the splitting is $1+1 = 2$.
    Prediction: A doublet (intensity ratio 1:1) shifted upfield. (Note: A weak $^3J_{HD}$ coupling with the adjacent D also exists in principle, giving a doublet of triplets, but this long-range coupling is typically too small to resolve in routine spectra.)
  • $\text{CHD}$ Methine Proton (1H):
    This proton has two different magnetic neighbors causing splitting:
    1. It couples with the 3 adjacent methyl protons. ($n=3 \implies 3+1=4$, a quartet).
    2. It couples with the 1 adjacent Deuterium atom. Since Deuterium has spin $I=1$, the splitting is $2nI + 1 = 2(1)(1) + 1 = 3$ (a triplet).
    Prediction: A complex quartet of triplets shifted downfield due to the electronegative Chlorine atom attached to it.
61. Predict theoretically the NMR spectra of diethylether.
2025 Q32 Marks
Detailed Exam Answer:

The structural formula of diethyl ether is perfectly symmetric: $\text{CH}_3-\text{CH}_2-\text{O}-\text{CH}_2-\text{CH}_3$. Because the left and right sides are identical mirrors, there are only two chemically distinct groups of protons in the entire molecule.

  • $\text{CH}_3$ Methyl Protons (Total 6H):
    These protons are attached to the end carbons. They are adjacent to a $\text{CH}_2$ group which contains 2 protons ($n=2$). Using the $n+1$ rule, the splitting is $2+1 = 3$.
    Prediction: A triplet (intensity ratio 1:2:1) appearing upfield (around 1.2 ppm).
  • $\text{CH}_2$ Methylene Protons (Total 4H):
    These protons are attached to the carbons next to the oxygen atom. They are adjacent to a $\text{CH}_3$ group which contains 3 protons ($n=3$). Using the $n+1$ rule, the splitting is $3+1 = 4$.
    Prediction: A quartet (intensity ratio 1:3:3:1) appearing significantly further downfield (around 3.4 ppm) because the highly electronegative oxygen atom pulls electron density away, deshielding them.
Summary: The spectrum will show a triplet and a quartet with an overall integration area ratio of 6:4 (or 3:2).
62. Show the splitting pattern in high resolution of $^{1}\text{H}$ NMR spectrum of acetaldehyde molecule with explanation.
2022 Q33 Marks
Detailed Exam Answer:

The structural formula of acetaldehyde is $\text{CH}_3-\text{CHO}$. There are two very distinct proton environments.

  • $\text{CHO}$ Aldehydic Proton (1H):
    This proton is attached directly to the carbonyl carbon ($\text{C=O}$). The extremely strong electron-withdrawing effect of the double-bonded oxygen pulls almost all electron shielding away from it, pushing its signal incredibly far downfield (around 9.7 ppm).
    It is adjacent to the $\text{CH}_3$ group ($n=3$). Using the $n+1$ rule, the splitting is $3+1 = 4$.
    Prediction: A highly deshielded quartet (1:3:3:1).
  • $\text{CH}_3$ Methyl Protons (3H):
    These protons are adjacent to the single aldehydic proton ($n=1$). Using the $n+1$ rule, the splitting is $1+1 = 2$.
    Prediction: A doublet (1:1) appearing upfield (around 2.2 ppm).
63. Show the splitting pattern in high resolution $^{1}\text{H}$ NMR spectrum of Ethanol molecule.
2023 Q32 Marks
Detailed Exam Answer:

The structural formula of ethanol is $\text{CH}_3-\text{CH}_2-\text{OH}$.

Under standard, real-world high-resolution conditions, trace amounts of acidic or basic impurities catalyze rapid chemical exchange of the hydroxyl ($\text{OH}$) proton with other ethanol molecules. Because it hops from molecule to molecule faster than the NMR machine can take a "picture" of it, the spin coupling between the $\text{OH}$ proton and the adjacent $\text{CH}_2$ group is completely averaged out. Therefore, they do not split each other.

0 1 2 3 4 Chemical Shift (ppm) TMS CH₃ (Triplet) OH (Singlet) CH₂ (Quartet)
Figure: High-resolution NMR spectrum of Ethanol showing the triplet, quartet, and singlet.
  • $\text{CH}_3$ Methyl Protons (3H): Adjacent to the 2 protons of the $\text{CH}_2$ group ($n=2$). Split into a triplet ($2+1=3$).
  • $\text{CH}_2$ Methylene Protons (2H): Only couples with the 3 protons of the $\text{CH}_3$ group ($n=3$). Split into a quartet ($3+1=4$).
  • $\text{OH}$ Hydroxyl Proton (1H): Does not couple due to rapid exchange. Appears as a broad singlet.