Molecular Spectroscopy Flashcards
(74 cards)
absorption spectroscopy
molecule undergoes a transition from a state of lower energy, E1, to one of higher energy, E2
emission spectroscopy
molecule undergoes a transition from a state of higher energy, E2, to one of lower energy, E1
transition dipole moment
intensity of spectral line - arising from a molecular transition between initial state (Ψi) and final state (Ψf) depends on the electric dipole moment
for a transition to be dipole allowed, the expectation value of the dipole moment operator (the transition dipole moment, R) must be non-zero
the (electric) dipole moment
Born-Oppenheimer approximation
nuclei of a molecule, being much heavier than the electrons, moves relatively slowly and may be treated as stationary while the electrons move in their field
approximation allows us to select an internuclear separation in a diatomic molecule and solve the Schrodinger equation for electrons at that nuclear separation
- this calculation can be repeated for different nuclear separations
- allowing us to explore how the energy of a molecule varies with bond length
- obtain a molecular potential energy surface
Born-Oppenheimer approximation: approximate molecular wavefunction as a product of electronic, vibrational and rotational wavefunctions
electron motion much faster that molecular vibrations which are much faster than molecular rotations
all of the different types of molecular energy can be treated separately
rotational spectroscopy: rigid rotor energy levels (in Joules, J)
J - rotational angular momentum quantum number (0, 1, 2,…)
r - bond length
I - moment of inertia
moment of intertia, I
mi - masses of the atoms
ri - their distances from the centre of mass of molecule
molecule rotates about its centre of mass:
m1r1 = m2r2
reduced mass of a molecule
μ = m1m2/(m1 + m2)
energy levels of rotational states
expressed as a rotational term
in cm-1
B - rotation constant
depends on the moment of intertia of the molecule
has units of cm-1
F(J) ∝ J(J+1)
energy separation between adjacent rotational energy levels increases as J increases
B for small molecules is typically in the region 0.1 - 10 cm-1
B ∝ 1/I
- therefore larger molecules have more closely spaces rotational energy levels than smaller molecules
centrifugal distortion
reduces the rotation constant and the energy levels are slightly closer together than the rigid rotor expression predicts
D - centrifugal distortion ~ related to the vibrational wavenumber of a diatomic molecule, ωe
effect of centrifugal distortion is taken into account empirically by writing the rotational energy term as:
selection rules for rotational spectroscopy
selection rules are found by evaluating the transition dipole moment
Ψr - rotation wavefunction
double prime ‘’ - initial state
single prime ‘ - final state
this integral is only non-zero if the molecule has a permanent dipole moment, μ and ΔJ = ±1
- these are the rotational selection rules for linear rotors
ΔJ = ±1
when a photon is absorbed by a molecule, angular momentum of the system must be conserved
photon has a spin angular momentum of 1, when molecule absorbs photon, its rotational angular momentum J must increase by 1
applying the selection rules to the expression for the energy levels of a rigid rotor
the wavenumbers of the allowed J + 1 ← 1 transitions are:
spectrum consists of a series of equally spaced lines with wavenumbers: 2B, 4B, 6B….
- separated by 2B
intensities of lines in rotational spectra
intensities increase with increasing J and pass through a maximum before tailing off as J becomes large
existence of maximum arises because of a maximim in the population of rotational energy levels
population of a rotational energy level, J
given by the Boltzmann expression
N - total number of molecules in the sample
gJ = (2J +1) - degeneracy of the level J
k - Boltzmann constant
T - rotational temperature of the sample
relative population of rotational level, J
harmonic oscillator
for small molecular vibrations, molecular bond obeys Hooke’s law and the restoring force, dV(x)/dx = -kx
k - force constant of bond
x = r - re
re - equilibrium bond length
integrating expression for restoring force gives the potential energy:
V(x) = 1/2 kx^2
energy levels of harmonic oscillator (in J)
vibrational energy levels are quantised
v - vibrational quantum number (v = 0, 1, 2,…)
ω - vibration angular frequency in rad s-1
ω = (k/μ)^1/2
energy levels of the vibrational states are expressed as a vibrational term:
G(v) = Ev/hc (in cm-1)
ωe - harmonic vibration wavenumber (in cm-1)
ωe - harmonic vibration wavenumber
depends on the force constant and reduced mass of the diatomic molecule