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Rep:MOD:YZ20215

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NH3 Molecule

The optimisation file is linked to here

General Information

Optimisation is done and seven intermediates were shown with the final result below:

N-H bond distance/Angstroms=1.01798

H-N-H bond angle/degrees=105.741

File Name: yanzhang_nh3_optf

Molecule Name: NH3

Calculation Type: FREQ

Calculation Method: RB3LYP

Basis Set: 6-31G(d,p)

E(RB3LYP): -56.55776873 a.u.

Point Group: C3V

         Item               Value     Threshold  Converged?
 Maximum Force            0.000004     0.000450     YES
 RMS     Force            0.000004     0.000300     YES
 Maximum Displacement     0.000072     0.001800     YES
 RMS     Displacement     0.000035     0.001200     YES
test molecule

Vibrations

Questions 1.how many modes do you expect from the 3N-6 rule?

 3*4-6=6

2.which modes are degenerate (ie have the same energy)?

 5 and 6

3.which modes are "bending" vibrations and which are "bond stretch" vibrations?

 Bending:1,2,3 Bond stretch:4,5,6

4.which mode is highly symmetric?

 4

5.one mode is known as the "umbrella" mode, which one is this?

 1

6.how many bands would you expect to see in an experimental spectrum of gaseous ammonia?

 2, because there are N-H bending and streching.

Charge

Charge on N atom=-1.125

Charge on H atom=0.375

N atom is expected to have negative as it is much more electronegative than hydrogen atoms, and the H atoms are expected to have positive charge.

H2 Molecule

The optimisation file is linked to here

test molecule

General Information

File Name: yz20215_H2_OPTF

Molecule Name: H2

Calculation Type: FREQ

Calculation Method: RB3LYP

Basis Set: 6-31G(d,p)

Charge: 0

as there is no overall polarity, the charge on both atoms is zero

Spin: Singlet

E(RB3LYP): -1.17853936 a.u.

RMS Gradient Norm: 0.00000017 a.u.

Imaginary Freq: 0

Dipole Moment: 0.0000 Debye

Point Group: D∞H


        Item               Value     Threshold  Converged?
Maximum Force            0.000000     0.000450     YES
RMS     Force            0.000000     0.000300     YES
Maximum Displacement     0.000000     0.001800     YES
RMS     Displacement     0.000001     0.001200     YES

Vibrations

1 vibration mode is expected as 3N-5 rules apply to linear molecules.


N2 Molecule

The optimisation file is linked to here

test molecule

General Information

File Name: yz20215_N2_OPTF

Molecule Name: N2

Calculation Type: FREQ

Calculation Method: RB3LYP

Basis Set: 6-31G(d,p)

Charge: 0

as there is no overall polarity, the charge on both atoms is zero

Spin:Singlet

E(RB3LYP): -109.52412868 a.u.

RMS Gradient Norm: 0.00000060 a.u.

Imaginary Freq: 0

Dipole Moment: 0.0000 Debye

Point Group:D∞H

        Item               Value     Threshold  Converged?
Maximum Force            0.000001     0.000450     YES
RMS     Force            0.000001     0.000300     YES
Maximum Displacement     0.000000     0.001800     YES
RMS     Displacement     0.000000     0.001200     YES

Vibrations

1 vibration mode is expected as 3N-5 rules apply to linear molecules.

Haber-Bosch Reaction Energy

E(NH3)=-56.55776873 a.u.

2*E(NH3)=-113.11553746 a.u.

E(N2)=-109.52412868 a.u.

E(H2)=-1.17853936 a.u.

3*E(H2)=-3.53561808 a.u.

ΔE=2*E(NH3)-[E(N2)+3*E(H2)]=-0.0557907 a.u.=-146.47849401 kJ/mol

The process is exothermic, indicating that the ammonia molecule is more stable.

Literature value=-92.4 kJ/mol

The value calculated deriviates largely from the literature value, so the method using the software to obtained the energy is not very accurate.

Project Molecule: S2 Molecule

The optimisation file is linked to here

test molecule

General Information

File Name: YZ20215_S2_OPTF

Molecule Name: S2

S=S double bond distance/Angstroms=1.77760

Calculation Type: FREQ

Calculation Method: RB3LYP

Basis Set: 6-31G(d,p)

Charge: 0 on both atoms

as there is no overall polarity, the charge on both atoms is zero

Spin: Singlet

E(RB3LYP): -796.32599779 a.u.

RMS Gradient Norm: 0.00000372 a.u.

Imaginary Freq: 0

Dipole Moment: 0.0000 Debye

Point Group: D∞H

        Item               Value     Threshold  Converged?
Maximum Force            0.000006     0.000450     YES
RMS     Force            0.000006     0.000300     YES
Maximum Displacement     0.000011     0.001800     YES
RMS     Displacement     0.000016     0.001200     YES

Vibrations

1 vibration mode is expected as 3N-5 rules apply to linear molecules.

Molecular Orbital Diagrams

1. 3s sigma* u antibonding orbital

Components: two 3s valence shell atomic orbitals from both S atoms

Character: ocuppied antibonding orbital with no mixing

Energy: -0.61535 a.u.

High in energy compared with 2s,2p,and 1s orbitals, but the second lowest in the valence shell orbitals.

A Gaussview image of 3s sigma* antibonding orbital

2. 3p sigma g bonding orbital(in z direction)

Components: two 3pz valence shell atomic orbitals from both S atoms overlap head-to-head

Character: ocuppied bonding orbital with mixing with 3s sigma orbital

Energy: -0.39516 a.u.

High in energy compared with 2s,2p,and 1s orbitals, but the third lowest in the valence shell orbitals.

The red lobes are larger due to mixing.

A Gaussview image of 3p sigma bonding orbital(in z direction)

3. 3p pi u bonding orbital(in y direction)

Components: two 3py valence shell atomic orbitals from both S atoms

Character: ocuppied bonding orbital with no mixing

Energy: -0.36284 a.u.

High in energy compared with 2s,2p,and 1s orbitals, but the third highest in the valence shell orbitals.

A Gaussview image of 3p pi bonding orbital(in y direction)

4. 3p pi u bonding orbital(in x direction)

Components: two 3px valence shell atomic orbitals from both S atoms

Character: ocuppied bonding orbital with no mixing

Energy: -0.34959 a.u.

High in energy compared with 2s,2p,and 1s orbitals, the second highest in the valence shell orbitals.

A Gaussview image of 3p pi bonding orbital(in x direction)

5. 3p pi* u antibonding orbital(in x direction)

Components: two 3px valence shell atomic orbitals from both S atoms

Character: ocuppied bonding orbital with no mixing, HOMO

Energy: -0.21842 a.u.

Highest in energy compared with 2s,2p,and 1s orbitals.

A Gaussview image of 3p pi* antibonding orbital(in x direction)