Crossaemma
Comments
It's great that you have a working wiki—you did a good job. However, the wavenumber and intensity values were rounded incorrectly—please double-check those for accuracy. If you have any queries or want more detailed feedback on your computational lab, please contact Prof. Hunt.
NH3 Molecule
Calculation Data
| Name of Sumbitted log | NH3_optf.log |
|---|---|
| Molecule | NH3 |
| Method | RB3LYP |
| Basis Set | 6-31G(d,p) |
| Final Energy | -56.557769 |
| RMS Gradient | 0.000003 |
| Point Group | C3V |
Convergence
Item table confirming forces and displacements are converged.
Item Value Threshold Converged? Maximum Force 0.000000 0.000015 YES RMS Force 0.000000 0.000010 YES Maximum Displacement 0.000003 0.000060 YES RMS Displacement 0.000001 0.000040 YES
Confirming a minimum, the CoM motion is near zero
Low frequencies --- -5.6864 -3.6131 -3.6124 0.0017 0.0048 0.0162 Low frequencies --- 1089.3674 1693.9284 1693.9284
Optimised Molecule Image
Rotateable Molecule: Logfile: Media:ECROSAN_NH3_OPTF_POP.LOG
Optimised NH Molecule |
Important Gemoetric Parameters
| Coord | Value |
|---|---|
| Bond Length (N-H) | 1.02Â |
| Bond Angle θ (H-N-H) | 106° |
Vibrations
| Mode | 1 | 2 | 3 | 4 | 5 | 6 |
|---|---|---|---|---|---|---|
| Wavenumber (cm-1) | 1089.37 | 1693.93 | 1693.93 | 3461.38 | 3589.93 | 3589.93 |
| Symmetry | A1 | E | E | A1 | E | E |
| Intensity | 145 | 14 | 14 | 1 | 0 | 0 |
Computed Spectrum
Questions to Answer
- How many modes do you expect from the 3N-6 rule?
Using the 3N-6 rule, where N=the number of atoms: N=4 so 12-6=6, therefore we expect 6 modes.
- How many bands (peaks) do you see in the computed spectrum of gaseous ammonia?
Only two vibrational bands are observed in the computed IR spectrum. While computational methods calculate all vibrational modes, only those involving a dipole moment change are IR active, and thus appear as observable peaks.
- Which modes are degenerate (ie have the same energy)?
The E modes at 1694 cm-1 and 3590 cm-1 are degenerate, as each consists of two vibrations with the same energy.
- Which modes have essentially no intensity?
The A1 mode at 3461 cm-1 and the E mode at 3590 cm-1 show essentially no intensity in the IR spectrum because they do not involve a change in dipole moment, which is required for a vibration to be IR active.
- What is the selection rule for IR vibrations?
A vibrational mode is IR active only if it involves a change in the molecular dipole moment. If the dipole moment of the molecule changes (the separation of positive and negative charge varies), the vibration can absorb infrared radiation and will appear in the IR spectrum.
- Why are there fewer modes in the spectrum than you would predict from the 3N-6 rule?
In the spectrum, there are less than the 6 calculated modes because some modes have very low or no IR intensity, and degenerate modes (e.g the E modes) appear as a single peak.
- Which modes are "bending" vibrations and which are "bond stretch" vibrations?
"Bending" vibrations correspond to lower energy modes 1, 2, and 3; "bond stretch" vibrations correspond to higher energy modes 4, 5, and 6.
- One mode is known as the "umbrella" mode, which one is this?
Mode 1 is known as the umbrella mode as it resembles an umbrella folding up and down.
- Why is the umbrella mode so intense?
The umbrella mode is intense because it involves a large dipole moment and is thus very IR active.
Charges
| Atom | Charge |
|---|---|
| N | -1.13 |
| H | +0.38 |
Molecular Orbitals
| Real 2a1 MO | LCAO MO |
|---|---|
Project Molecule: N2F2
Calculation Data
| Name of Sumbitted log | N2F2_optf.log |
|---|---|
| Molecule | N2F2 |
| Method | RB3LYP |
| Basis Set | 6-31G(d,p) |
| Final Energy | -309.01241 |
| RMS Gradient | 0.00000 |
| Point Group | C2V |
Convergence
Data from log confirming forces and displacements are converged
Item Value Threshold Converged? Maximum Force 0.000001 0.000015 YES RMS Force 0.000000 0.000010 YES Maximum Displacement 0.000001 0.000060 YES RMS Displacement 0.000001 0.000040 YES
Low Frequencies from log
Low frequencies --- -0.0017 -0.0013 -0.0005 3.2224 4.3531 5.1001 Low frequencies --- 347.8772 561.2472 771.6105
Optimised Molecule
Jmol Rotateable Molecule:
Logfile: Media:ECROSAN_N2F2_OPTF_POP.LOG
Optimised NF Molecule |
Geometric Parameters
Optimised bond angles for N2F2
| Coord | Value |
|---|---|
| Bond Length (N-F) | 1.4Â |
| Bond Length (N-N) | 1.2Â |
| Bond Angle θ (N-N-F) | 114° |
Vibrations
| Mode | 1 | 2 | 3 | 4 | 5 | 6 |
|---|---|---|---|---|---|---|
| Wavenumber | 347.88 | 561.25 | 771.61 | 949.45 | 987.25 | 1636.61 |
| Symmetry | A1 | A2 | B2 | A1 | B2 | A1 |
| Intensity | 0 | 0 | 74 | 75 | 81 | 20 |
Computed Spectrum
Questions To Answer
- The molecule from the log file does not have bonds between the F and N atoms, what is going on here?
- The bond distances are likely too far away for the computer program to register. Other possible reasons could be:
- - Unstable simulation
- - Incorrect or incomplete simulation
- - Atoms are too far apart
- How many vibrations do you expect from the 3N-6 rule?
- 4 atoms in N2F2
- 3(4)-6=6
- 6 vibrational modes.
- Why are there only 4 peaks in the IR spectrum?
- Some normal modes may be degenerate (two modes of nearly identical energy overlap into a single band) or some may be IR inactive. In the case of N2F2, the two lowest vibrations at 347.88 and 561.25 have very low values or no infrared, meaning they are not visible in the spectra.
- Which vibration is the asymmetric N-F stretch?
- Mode 4, at a frequency of 949.45 is associated with N-F stretching.
- What is the nature of the highest energy vibration?
- Generally, stretching vibrations occur at higher wavenumbers compared to bending ones. Stronger bonds = higher wavenumber
- In this molecule, the highest energy vibration is associated with N=N stretching.
- Which MOs are core orbital MOs
- Orbitals 1-4 are core bonding orbitals, who are not affected by reactions.
Charges
NBO charges colour coded green for positive and red for negative. The charge range is +/- 0.215
| Atom | Charge |
|---|---|
| N | +0.22 |
| F | -0.22 |
Molecular Orbitals
Molecular orbitals (MOs) 1-4 are core orbitals.
| MO 9 | LCAO MO |
|---|---|
