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Computational Spectroscopy II. ab initio Methods

Computational Spectroscopy II. ab initio Methods. Chemistry 713 Updated: January 29, 2008. (b) Optimized Structures and Rotational Constants. Calculation of the ab initio energy at a single molecular geometry my involve significant computational effort.

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Computational Spectroscopy II. ab initio Methods

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  1. Computational SpectroscopyII. ab initio Methods Chemistry 713 Updated: January 29, 2008

  2. (b) Optimized Structures and Rotational Constants • Calculation of the ab initio energy at a single molecular geometry my involve significant computational effort. • To find a relative minimum, the geometry is changed along the line of steepest decent (fall line). • The program calculates the energies for slight changes in the geometry along each atomic coordinate to determine the fall line. • Second derivatives of the energy w.r.t. the coordinates are used to determine how far to go along the fall line. (Some methods allow analytic second derivatives: HF, B3LYP, MP2, CASSCF; for others the derivatives must be computed numerically). • Process is repeated until a minimum is found. (all 1st derivatives equal zeros and second derivatives are positive.) • Gaussian allows various convergence criteria to be set.

  3. G03 example files • Gaussian provides over 700 example input files and the corresponding output files. • Mac (UNIX) • Input files: /Applications/g03/tests/com/testxxx.com • Output files: /Applications/g03/tests/rs6k/testxxx.log • Test file index: /Applications/g03/tests/test.idx • Windows • Input files: C:\G03W\tests\gif\testxxx.gif • Output files: … missing • Test file index: C:\G03W\tests\tests.idx

  4. Example: …/g03/tests/com/test083.com Water dimer geometry optimization • #p rhf/6-31g* opt=tight test • Gaussian Test Job 83: • Water dimer optimization • 0,1 • O • O,1,ROO • X,1,1.,2,X3O • H,1,RO1H,3,HOX3,2,90.,0 • H,1,RO1H,3,HOX3,2,-90.,0 • X,2,1.,1,52.5,3,180.,0 • H,2,RO2H1,6,H7OX,1,180.,0 • H,2,RO2H2,6,H8OX,1,0.,0 • ROO=2.98308 • RO1H=0.94839 • X3O=120.2827 • HOX3=52.90868 • RO2H1=0.94686 • RO2H2=0.95173 • H7OX=52.98178 • H8OX=51.9632 Input file: “.com” or “.gif” => Input file viewed with GaussView Distance matrix (angstroms): 1 2 3 4 5 1 O .000000 2 O 2.983080 .000000 3 H .948390 3.393962 .000000 4 H .948390 3.393962 1.513015 .000000 5 H 3.362029 .946860 3.869192 3.869192 .000000 6 H 2.031411 .951730 2.491320 2.491320 1.505701 (Initial geometry from top of log file)

  5. Example: …/g03/tests/rs6k/test083.log Water dimer geometry optimization • #p rhf/6-31g* opt=tight test • … • Gaussian Test Job 83: Water dimer optimization • … • Berny optimization. • Internal Forces: Max .000871642 RMS .000359230 • Search for a local minimum. • Step number 1 out of a maximum of 23 • … • Item Value Threshold Converged? • Maximum Force .000851 .000015 NO • RMS Force .000275 .000010 NO • Maximum Displacement .013238 .000060 NO • RMS Displacement .005575 .000040 NO • Predicted change in Energy=-5.784113D-06 • … • GradGradGradGradGradGradGradGradGradGradGradGradGradGradGradGradGradG • Berny optimization. • Internal Forces: Max .000000441 RMS .000000186 • Search for a local minimum. • Step number 18 out of a maximum of 23 • …. • Item Value Threshold Converged? • Maximum Force .000000 .000015 YES • RMS Force .000000 .000010 YES • Maximum Displacement .000008 .000060 YES • RMS Displacement 000004 .000040 YES • Predicted change in Energy=-2.034343D-12 • Optimization completed. • -- Stationary point found Output file: “.log” or “.out” => Distance matrix (angstroms): 1 2 3 4 5 1 O .000000 2 O 2.971263 .000000 3 H .948352 3.360777 .000000 4 H .948352 3.360777 1.512866 .000000 5 H 3.422316 .946706 3.905657 3.905657 .000000 6 H 2.025317 .951801 2.481287 2.481287 1.510657 (from bottom of log file)

  6. Hints: How to cope with Gaussian output • “.log” or “.out” are plain text files. • may be over 100 pages long! • If your input file was “MyMolecule1.com” (or “… .gif”), then the ouput file is named “MyMolecule1.log” (or “… .out”). • ALWAYS us a different file name for every job, so that you don’t over-write any of your old outputs. • The next job might be “MyMolecule2.com”, etc. • NEVER delete any of your input or output files! • Use a spreadsheet (or lab notebook) to keep a log of your Gaussian (& Spartan) jobs. • One line of a spreadsheet can summarize the essential info:Date, File name, Molecule, Purpose, Command lne (e.g., #p rhf/6-31g* opt=tight test), Any problem encountered. • If you don’t keep meticulous records of your calculations, you will risk drowning in your data! THE BEST WAY TO CONVINCE A FOOL THAT HE IS WRONG IS TO LET HIM HAVE HIS OWN WAY. JOSH BILLINGS

  7. Hints: How to read Gaussian output • Open your “.log” or “.out” files with a simple text editor such as NotePad (Windows) or TextEdit (Mac). • Microsoft Word is NOT recommended because, for this purpose, it is big, clumsy, and slow. • It you find a cryptic bit of philosophy at the bottom of the file, the Gaussian thinks it completed the job successfully. • You will also find the CPU time and a densely packed summary of the results. … from file test083,log 1\1\GINC-JERRY\FOpt\RHF\6-31G(d)\H4O2\FRISCH\07-Apr-2004\0\\#P RHF/6-3 1G* OPT=TIGHT TEST\\Gaussian Test Job 83: Water dimer optimization\\0, 1\O,-0.0029670399,0.,-1.4285923793\O,-0.0012160547,0.,1.5426696978\H,0 .504461364,0.7564331492,-1.6925928276\H,0.504461364,-0.7564331492,-1.6 925928276\H,-0.8866727134,0.,1.8776611243\H,-0.0887852583,0.,0.5949059 822\\Version=IBM64-G03RevC.02\State=1-A'\HF=-152.0304565\RMSD=7.932e-0 9\RMSF=1.778e-07\Dipole=0.0596938,0.,-1.0577951\PG=CS [SG(H2O2),X(H2)] \\@ THERE'S SMALL CHOICE IN A BOWL OF ROTTEN APPLES. SHAKESPEARE Job cpu time: 0 days 0 hours 0 minutes 36.7 seconds. File lengths (MBytes): RWF= 18 Int= 0 D2E= 0 Chk= 10 Scr= 1 Normal termination of Gaussian 03 at Wed Apr 7 15:20:15 2004.

  8. Item Value Threshold Converged? Maximum Force .000000 .000015 YES RMS Force .000000 .000010 YES Maximum Displacement .000008 .000060 YES RMS Displacement .000004 .000040 YES Predicted change in Energy=-2.034343D-12 Optimization completed. -- Stationary point found. ---------------------------- Hints: How to read Gaussian output • Use your text editor to search for certain words or phrases that will take you directly to the part of the output that you need. • E.g., “#p”, “Job CPU time”, “Optimization completed” • Some phases like “Converged?” occur after each step of the optimization. • With 100 pages of output, this is MUCH faster than scrolling through the file. • You can also open any Gaussian input or output or . chk file with Gaussview, but less information is accessible that way.

  9. R.N. Zare, Angular Momentum, pp 253-258. Rotational constants • The rotational Hamiltonian iswith A = 1/2Ia, etc., where Ia, Ib, and Ic are the principal monents of inertia. (Beware of units!) • where i labels the atoms in the molecule. • Gaussian calculates the rotational constants, A, B, and C: Standard orientation: ---------------------------------------------------------------------------- Center Atomic Atomic Coordinates (Angstroms) Number Number Type X Y Z ---------------------------------------------------------------------------- 1 8 0 .003321 -1.427751 .000000 2 8 0 .003321 1.555329 .000000 3 1 0 -.490596 -1.716172 .756507 4 1 0 -.490596 -1.716172 -.756507 5 1 0 .915824 1.808076 .000000 6 1 0 .012237 .603641 .000000 ----------------------------------------------------------------------------- Rotational constants (GHZ): 215.8670694 6.1508112 6.1482646 A B C

  10. (c) Infrared and Raman Spectra • Vibrations of Diatomic Molecules • Vibration in Polyatomic Molecules: Normal Modes • Infrared Spectra • Raman Spectra • “Frequency” Calculations in Gaussian

  11. Vibrations of diatomic molecules • Chemical bonds will break at large interatomic distances. (red curve) • A harmonic potential approximates the true potential near the equilibrium geometry. (orange) • The real potential is ANHARMONIC.

  12. The Harmonic Oscillator • Harmonic oscillator wavefunctions are shown in red, n = 0, 1,2, …. • Allowed optical (infrared) transitions are n = ±1. (thick arrows) • Real molecules are anharmonic, therefore overtone transitions (n = ±2, 3, …) are also allowed, but are 1 or 2 orders of magnitude weaker for each higher overtone. (thinner arrows) • At room temperature, most of the molecules are in n = 0, so the n = 1  0 “fundamental” transition dominates the observed IR spectrum. • Note that anharmonicity shifts the observed IR fundamental transition to a frequency lower than the harmonic frequency by about 1 - 5%.

  13. Vibrations in polyatomic molecules • A nonlinear molecule with N atoms has 3N-6 vibrations: • 3N degrees of freedom • minus 3 translations and 3 rotations • Each vibration is assumed to be a harmonic oscillator and treated as an independent “normal” mode. • For each mode, all atoms move in hase with the same frequency. • The commonly used functional group vibrations (e.g., C-F stretch) are only rough descriptions. • The n = 1  0 “fundamental” transitions (one for each normal mode) dominate the IR spectrum. • Overtone and combination bands are often observed as small peaks in the experimental spectrum, but are NOT included in the simulated spectra produced by Spartan and Gaussian. • As with diatomics, anharmocity shifts the obesrved IR fundamentals are shift to lower frequency. Methyl fluoride Movies created by GaussView, captured by Snapz Pro X, and edited by QuickTime. Similar movies can be obtained from Spartan 04 or 06 without additional software.

  14. Calculation of molecular vibrations • In the harmonic approximation, the vibrational frequencies depend on: • all of the second derivatives of the potential, including the diagonal and mixed second derivatives • The molecular geometry, including all bond lengths, angles, and dihedral angles • The atmoic masses • The calculation is only valid at a stationary point • A place where all of the first derivatives are zero • Local minima, maxima, saddlepoints • MUST optimize the structure first, and then run the frequency calculation at ezacly the same level of theory and same basis set.

  15. Calculation of molecular vibrations:More on the harmonic approximation • Expand the potential in a multidimensional Taylor series”: The higher derivatives are neglected in most calculations causing most calculated frequencies to be too high. These 2nd derivatives (force constants) are used to determine the normal mode frequencies in the harmonic approximation. The the 1st derivatives (forces) are all zero at the equilibrium geometry. The energy of the molecule at it equilibrium geometry.

  16. Porcedure for calculating vibrational frequencies • In Gaussian, optimized the molecular geometry first (OPT) • Then run a frequency calculation (FREQ) at the same level of theory. • You can run both at the same time, but it is not recommended until you have had some experience. • Analytical second derivatives are available for the following methods: • HF, B3LYP, MP2, CASSCF • 2nd derivatives are calculated numericaly for other methods, and are MUCH more time consuming.

  17. Porcedure for calculating vibrational frequencies • In Gaussview: • Build the molecule. • From the Edit menu, click “Symmetrize” • Job type is “OPT” ,then “FREQ”. • From the Results menu, select “Vibrations …”.

  18. # opt freq hf/3-21g geom=connectivity . . . Full point group D2H NOp 8 . . . Harmonic frequencies (cm**-1), IR intensities (KM/Mole), Raman scattering activities (A**4/AMU), depolarization ratios for plane and unpolarized incident light, reduced masses (AMU), force constants (mDyne/A), and normal coordinates: 1 2 3 B2U B3U B2G Frequencies -- 941.6104 1114.4412 1156.0372 Red. masses -- 1.0439 1.1607 1.5215 Frc consts -- .5453 .8494 1.1980 IR Inten -- 1.3937 133.9954 .0000 Raman Activ -- .0000 .0000 4.9745 Depolar (P) -- .3940 .0000 .7500 Depolar (U) -- .5653 .0000 .8571 Atom AN X Y Z X Y Z X Y Z 1 6 .00 -.04 .00 .08 .00 .00 .15 .00 .00 2 6 .00 -.04 .00 .08 .00 .00 -.15 .00 .00 3 1 .00 .24 -.44 -.50 .00 .00 -.49 .00 .00 4 1 .00 .24 .44 -.50 .00 .00 -.49 .00 .00 5 1 .00 .24 -.44 -.50 .00 .00 .49 .00 .00 6 1 .00 .24 .44 -.50 .00 .00 .49 .00 .00 4 5 6 AU B3G AG Frequencies -- 1164.9569 1386.3705 1521.8389 Red. masses -- 1.0078 1.5294 1.2818 Frc consts -- .8059 1.7319 1.7491 IR Inten -- .0000 .0000 .0000 Raman Activ -- .0000 .9300 45.6702 Depolar (P) -- .0000 .7500 .4294 Depolar (U) -- .0000 .8571 .6008 Atom AN X Y Z X Y Z X Y Z 1 6 .00 .00 .00 .00 .15 .00 .00 .00 .11 2 6 .00 .00 .00 .00 -.15 .00 .00 .00 -.11 3 1 .50 .00 .00 .00 -.15 .47 .00 -.19 .46 4 1 -.50 .00 .00 .00 -.15 -.47 .00 .19 .46 5 1 .50 .00 .00 .00 .15 -.47 .00 .19 -.46 6 1 -.50 .00 .00 .00 .15 .47 .00 -.19 -.46 . . . E (Thermal) CV S KCal/Mol Cal/Mol-Kelvin Cal/Mol-Kelvin Total 36.426 7.387 52.029 Electronic .000 .000 .000 Translational .889 2.981 35.927 Rotational .889 2.981 15.788 Vibrational 34.649 1.425 .313 . . . Vibrations in Gaussian output • Check that the Point Group is what you expect. • The information for each vibrational mode is given. • Gaussian assumes that each atom is the most abundant isotope of each element, but other istoppes can be set with the ReadIsotopes option to te FREQ command. • Thermochemical data, e.g., U, CV, S are included. The default temperature is 298 K, but this can be changed

  19. Y Z X Infrared Intensities • Infrared intensities are proportional to • The transition moment vectorsare represented graphically by GaussView (amber). • The infrared fundamental bands are allowed or forbidden according to the irreducible representation (e.g., B2u) in the character table for the point group. 1: 941.6 cm-1B2u Infraredallowedfundamentals Peter Bernath, Spectra of Atoms and Molecules, Oxford University Press, New York, 1995, p 381.

  20. Scaling calculated infrared spectra • Calculated harmonic frequencies may be higher or lower than the true harmonic frequencies, according to the level of theory and basis set. • The true harmonic frequencies are higher than the experimental frequencies because of the neglect of anharmonicity. • To compare with experiment, the calculated frequencies are SCALED empirically (fudged) according to the level of theory and basis set. • It is advisable to check the literature on what scaling people have done for similar systems. Foresman and Frisch, p 64.

  21. Conventions of vibrational spectroscopy • By convention, the highest frequency mode of the highest symmetry (most symmetric irreducible representation) is 1, the next highest of that symmetry is 2 etc., through all th emodes of that symmetry. • Then the modes of the next greatest symmetry get the next available mode numbers from highest frequenct to lowest, until all modes have a number. • Gaussian does NOT follow this convention, but the literature does, and you should. • The z-axis is always the highest symmetry axis. Conventionally numbered Ethylene modes Ag 1 3329.6 cm-1 2 1841.8 cm-1 3 1521.8 cm-1 B2g4 1156.0 cm-1 B3g5 3373.1 cm-1 6 1386.3 cm-1 Au7 1164.9 cm-1 B1u8 3307.8 cm-1 9 1604.0 cm-1 B2u10 3404.5 cm-1 11 941.6 cm-1 B2u12 1114.4 cm-1 The frequencies are from our calculation above. Lesssymmetry

  22. Figures from Peter Bernath, Spectra of Atoms and Molecules, Oxford University Press, New York, 1995, p 284, 285. Raman Spectroscopy • Most routine Raman spectra are Q-branches in the Stokes vibrational Raman band. • The scattered light is shifted to lower frequencies. • The dfference between the scattered and incident frequencies corresponds to a vibrational excitation of the molecules • Many nonlinear Raman rechniques are also available.

  23. Selection rules for Raman spectroscopy • Raman spectra derive their intensity from the dependence of the molecular polarizability on the various vibrational coordinates. • The polarizability at the equilibrium geometry gives rise to Rayleigh scattering (light scattered at the same frequency as the incident light), which is MUCH more intense that the Raman scattered light. • The polarizability components multiply bilinear combinations of the the coordinates, which are listed in point group character tables. • For molecules with a center of symmetry, vibrational bands that are allowed in Raman are forbidden in the infrared, and vice versa. Raman allowed Ag: Raman allowed; Infrared forbidden Infrared allowed

  24. Calculation of Raman spectra • Calculated in Gaussian by default with FREQ command. (No Raman intensities in Spartan). • Raman spectra can be polarized or depolarized, or both according to whether the scattered light has the same or different polarization as the incident laser beam. • A useful aid in assignments • The same scalling as for IR spectra may be applied.

  25. Advantages and disadvantages of Raman spectroscopy* • Advantages • Complements IR spectroscopy: Provides access to vibrations that are weak or forbidden in IR. • Systematic studies of molecular vibrations always involve both IR and Raman spectra. • The effective resolution of routine spectra is higher. • Gas phase rotational structure: The Q-branch (J=0) is strong and produces as a sharp, narrow peak for each vibration, whereas in the infrared, the P, Q, and R branches (J=-1,0,+1) all have substantial intensity resulting in broad bands that may overlap the bands of other vibrations. O and S branches (J=-2, +2) are allowed in Raman, but are weak and very speard out, and so usually disappear into the baseline. • Condensed phase: Rotations become librations, but the qualitative effect is the same. • Disadvantages • The Raman effect is weak, so the signal levels are low. • It is much harder to observe overtone and combination bands. • Raman spectra are less routinely available because a Raman spectrometer requires a laser light source and so is more expensive. (For both IR and Raman, current spectrometers are usually Fourier transform spectrometers.) * Common Old-fashioned Ordinary Raman Spectroscopy (COORS). Other specialized forms include Coherent Antistokes Raman Spectroscopy (CARS), Coherent Stokes Raman Spectroscopy (CSRS), Box-CARS, and Resonance Raman Spectroscopy.

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