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What is the Separation Between Rotational Energy Levels?

Published in Rotational Spectroscopy 5 mins read

The separation between rotational energy levels in a diatomic or linear polyatomic molecule, modeled as a rigid rotor, is $2B(J+1)$, where $B$ is the rotational constant and $J$ is the rotational quantum number of the lower energy level. These energy separations correspond to the microwave region of the electromagnetic spectrum.

Understanding Rotational Energy Levels

Molecules are not static; they can rotate in space. The energy associated with these rotations is quantized, meaning molecules can only exist at specific, discrete rotational energy levels, not at energies in between. For a simple model, such as a rigid diatomic molecule, these energy levels can be described mathematically.

The Rigid Rotor Model

The simplest model for molecular rotation is the rigid rotor, which assumes that the bond length between atoms does not change during rotation. While an approximation, it provides an excellent foundation for understanding rotational spectroscopy.

The energy ($E_J$) of a rotational level for a rigid rotor is given by:

$E_J = BJ(J+1)$

Where:

  • $E_J$ is the rotational energy of a specific level.
  • $J$ is the rotational quantum number, which can take integer values: $0, 1, 2, 3, \ldots$. Higher $J$ values correspond to higher rotational speeds and energies.
  • $B$ is the rotational constant, a value specific to each molecule. It is inversely proportional to the moment of inertia ($I$) of the molecule and is typically expressed in units of wavenumbers (cm⁻¹) or Hertz (Hz). The rotational constant is crucial as it depends on the molecule's geometry (bond lengths) and atomic masses:
    $B = \frac{h}{8\pi^2 c I}$ (in cm⁻¹) or $B = \frac{h}{8\pi^2 I}$ (in Hz)
    where $h$ is Planck's constant, $c$ is the speed of light, and $I$ is the moment of inertia.

Calculating the Energy Level Separation

The separation between adjacent rotational energy levels ($\Delta EJ$) is the difference between an upper level ($E{J+1}$) and a lower level ($E_J$).

Let's calculate the energy separation for a transition from $J$ to $J+1$:

$\Delta EJ = E{J+1} - E_J$
$\Delta E_J = B(J+1)(J+1+1) - BJ(J+1)$
$\Delta E_J = B(J+1)(J+2) - BJ(J+1)$
$\Delta E_J = B(J+1)[(J+2) - J]$
$\Delta E_J = B(J+1)(2)$
$\Delta E_J = 2B(J+1)$

This formula shows that the energy separation is not constant but increases linearly with the rotational quantum number $J$ of the lower level.

Table of Rotational Separations

Transition Lower J Upper J Energy Level Separation (ΔE)
J=0 → J=1 0 1 2B(0+1) = 2B
J=1 → J=2 1 2 2B(1+1) = 4B
J=2 → J=3 2 3 2B(2+1) = 6B
J=3 → J=4 3 4 2B(3+1) = 8B
... ... ... ...

Factors Influencing Rotational Energy Separation

Several factors determine the magnitude of these separations:

  • Rotational Constant (B): This is the primary determinant. Molecules with smaller moments of inertia (e.g., lighter atoms, shorter bond lengths) will have larger rotational constants and thus larger separations between their energy levels. For instance, HCl will have larger separations than HI because of its smaller moment of inertia.
  • Rotational Quantum Number (J): As shown by the $2B(J+1)$ formula, the energy spacing between consecutive levels increases as $J$ increases. This means rotational absorption lines are not equally spaced.
  • Non-Rigidity (Centrifugal Distortion): In reality, molecules are not perfectly rigid. As they rotate faster (higher $J$), centrifugal force causes bonds to stretch slightly. This stretching increases the moment of inertia, which in turn slightly decreases the rotational constant $B$ at higher $J$ values. This effect leads to a slight decrease in the spacing between higher rotational lines, meaning the $2B(J+1)$ formula needs a small correction term for highly accurate measurements.

Spectroscopic Observation and Selection Rules

Rotational energy level separations are primarily observed using microwave spectroscopy, also known as pure rotational spectroscopy.

Gross Selection Rule

For a molecule to absorb microwave radiation and undergo a pure rotational transition, it must possess a permanent electric dipole moment (μ ≠ 0). This condition is known as the gross selection rule for microwave spectroscopy.

  • Examples of molecules with permanent dipole moments: HCl, H₂O, CO, OCS. These molecules are "microwave active."
  • Examples of molecules without permanent dipole moments: O₂, N₂, CO₂ (linear, dipoles cancel), CH₄ (tetrahedral, dipoles cancel). These molecules are "microwave inactive" and do not exhibit pure rotational spectra.

Specific Selection Rule

For a transition to occur, the rotational quantum number must change by $\Delta J = \pm 1$. This means a molecule can only transition to an immediately adjacent rotational energy level (e.g., from $J=0$ to $J=1$, or $J=1$ to $J=2$).

Why Microwave Region?

The energy differences between rotational levels are relatively small, corresponding to frequencies in the gigahertz (GHz) range and wavelengths in the millimeter to centimeter range. This range falls squarely within the microwave region of the electromagnetic spectrum. Observing these transitions allows scientists to probe the rotational behavior of molecules.

Practical Implications and Examples

  • Molecular Structure Determination: By analyzing the rotational spectrum (specifically the spacing between lines), the rotational constant $B$ can be determined. From $B$, the moment of inertia ($I$) can be calculated, which, in turn, provides highly precise information about bond lengths and bond angles in molecules.
  • Interstellar Chemistry: Microwave spectroscopy is a crucial tool in radio astronomy for identifying molecules in interstellar space, nebulae, and planetary atmospheres. The unique "fingerprint" of rotational transitions helps astronomers identify various molecules in the universe.
  • Quality Control: In industrial settings, microwave spectroscopy can be used for quality control, such as monitoring the purity of gases.

Example: Carbon Monoxide (CO)
Carbon monoxide is a diatomic molecule with a permanent dipole moment. Its rotational spectrum shows a series of equally spaced lines (in an ideal rigid rotor) separated by $2B$. From these separations, the bond length of CO can be accurately determined.