lecture 34 rotational spectroscopy: intensities
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Lecture 34 Rotational spectroscopy: intensities. Rotational spectroscopy. In the previous lecture, we have considered the rotational energy levels. In this lecture, we will focus more on selection rules and intensities. Selection rules and intensities (review). Transition dipole moment - PowerPoint PPT PresentationTRANSCRIPT
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Lecture 34Rotational spectroscopy: intensities
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Rotational spectroscopy
In the previous lecture, we have considered the rotational energy levels.
In this lecture, we will focus more on selection rules and intensities.
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Selection rules and intensities (review) Transition dipole moment
Intensity of transition
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Rotational selection rules
Transition moment
Oscillating electric field (microwave)
No electronic / vibrational transition
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Rotational selection rules Gross selection rule:
nonzero permanent dipole
Does H2O have microwave spectra? Yes Does N2 have microwave spectra? No Does O2 have microwave spectra? No
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Quantum in natureHow could
astrochemists know H2O exist in interstellar
medium?
Microwave spectroscopy
Public imageNASA
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Selection rules of atomic spectra(review)
From the mathematical properties of spherical harmonics, this integral is zero unless
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Rotational selection rules Specific selection rule:
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Spherical & linear rotors In units of wave number (cm–1):
( ) 1F J BJ J
( ) ( 1) 2F J F J BJ
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Nonrigid rotor: Centrifugal distortion
Diatomic molecule
221 1JF J BJ J D J J
Vibrationalfrequency
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Nonrigid rotor: Centrifugal distortion
Rigid
221 1JF J BJ J D J J Nonrigid
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Appearance of rotational spectra Rapidly increasing
and then decreasing intensities
2
2 12 2 1
2 1J
Jg J
J
Transition moment2
Degeneracy
Boltzmann distribution(temperature effect)
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Rotational Raman spectra
xy, etc. are essentially Y0,0, Y2,0, Y2,±1, Y2,±2
Linear rotors: ΔJ = 0, ±2
Spherical rotors: inactive (rotation cannot change the polarizability)
Gross selection rule: polarizability changes by rotation
Specific selection rule: x2 + y2 + z2 ~ Y0,0
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Rotational Raman spectra Anti-Stokes wing slightly less intense than
Stokes wing – why? Boltzmann distribution (temperature effect)
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Rotational Raman spectra Each wing’s envelope is explained by the
competing effects of Degeneracy Boltzmann distribution (temperature effect)
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H2 rotational Raman spectra Why does the intensity alternate?
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H2 rotational Raman spectra Why does the intensity alternate?
Answer: odd J levels are triply degenerate (triplets), whereas even J levels are singlets.
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Nuclear spin statistics Electrons play no role here; we are concerned
with the rotational motion of nuclei. The hydrogen’s nuclei (protons) are fermions
and have α / β spins . The rotational wave function (including
nuclear spin part) must be antisymmetric with respect to interchange of the two nuclei.
The molecular rotation through 180° amounts to interchange.
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Para and ortho H2
Sym.Antisym.
Antisym.Sym.Singlet (para-H2)
Triplet (ortho-H2)Nuclear (proton) spins
With respect to interchange (180° molecular rotation)
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Spatial part of rotational wave function By 180 degree rotation, the wave function
changes sign as (–1)J (cf. particle on a ring)
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Para and ortho H2 Sym.Antisym.
Antisym.Sym.Singlet (para-H2)
Triplet (ortho-H2)
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Summary We have learned the gross and specific
selection rules of rotational absorption and Raman spectroscopies.
We have explained the typical appearance of rotational spectra where the temperature effect and degeneracy of states are important.
We have learned that nonrigid rotors exhibit the centrifugal distortion effects.
We have seen the striking effect of the antisymmetry of proton wave functions in the appearance of H2 rotational Raman spectra.