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IR and NMR Spectroscopy

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Gaussian Defaults Split. RHF and RDFT for Closed Shell ... This parameter is used in spin orbit coupling (see CASSCF=SpinOrbit), and the ... – PowerPoint PPT presentation

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Title: IR and NMR Spectroscopy


1
IR and NMR Spectroscopy
  • Gaussian Workshop Day 4

2
Restricted vs. Unrestricted Redux
  • Gaussian Defaults Split.
  • RHF and RDFT for Closed Shell
  • UHF and UDFT for Open Shell and Excited States
  • Pg 10 in Foresman and Frisch
  • Reason has to do with differences in magnetic
    environment
  • Consider Be 1s22s2 vs. 1s22s12p1

3
Basics of Spectra
  • Optimize First!
  • Require only one word command NMR or Freq.
  • Extraction of Spectra for Publication requires
    program like SWizard.
  • UV/Vis spectra not so simple.

4
NMR Basics
  • Do not need to optimize with same basis as you
    run NMR
  • Must compare with TMS Si(CH3)4 for relative
    shifts in same Basis/Method

5
IR Spectra
  • Must Optimize with Same Basis Set/Method
  • Calculation must be fully optimized or
    imaginary/negative frequencies will result.
  • Also gives thermochemical information for 1Atm
    and 298K.

6
IR Spectra Accuracy
  • Calculations rely on Harmonic approximation
  • Often overestimate frequencies as a result
  • Results usually scaled
  • Scale factors dependent on both method and basis

7
Isotopes (From Help File)
  • C(Iso13,Spin3) 0.0 0.0 0.0
  • The line specifies a 13C atom with a nuclear spin
    of 3/2 (3 1/2), located at the origin. The
    following items may be included in the list of
    parameters
  • Ison Isotope selection. If integers are used to
    specify the atomic masses, the program will
    automatically use the corresponding actual exact
    isotopic mass (e.g., 18 specifies 18O, and
    Gaussian uses the value 17.99916).
  • Spinn Nuclear spin, in units of 1/2.
  • ZEffn Effective charge. This parameter is used
    in spin orbit coupling (see CASSCFSpinOrbit),
    and the ESR g tensor and the electronic
    spin-molecular rotation hyperfine tensor (NMR
    OutputPickett).
  • QMomn Nuclear quadrupole moment.
  • GFacn Nuclear g-factor.

8
Homework
  • Read Introduction to Part 2, Chapters 5/6.
  • Get comfortable with the basics
  • Solvation next? Or move onto Part 2?
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