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= Valence Bond State correlation diagrams =
  
 +
== Exercise 1 : Computation of state correlation Diagrams for a 3 centers / 4 electrons system ==
 +
In this exercise the <math>\textrm{S}_{\textrm{N}}2</math> reaction Cl<math>{}^{-}</math> + CH<math>{}_3</math>Cl -> ClCH<math>{}_3</math> + Cl<math>{}^{-}</math> will be studied in both vacuum and solution. Valence Bond State Correlation Diagrams (VBSCD) will be constructed at <math>\pi</math>-D-BOVB level. There are two parts in this exercise: basic part and optional part. The basic part is performed with MCP-DZP basis set in which the inner orbitals in Cl and C are described with MCP pseudo potential. The optional part is performed with 6-31+G* basis set, using the general specification for the xmvb input (expert users). Only reactant and transition state will be computed in this exercise, which is sufficient to build the VBSCD diagrams. <br>
  
 +
{| class="collapsible collapsed wikitable"
 +
|-
 +
!'''Note:How to perform a VBPCM calculation'''
 +
|-
 +
|
 +
A VBPCM calculation is performed in the similar way as the VB calculations in vacuum. One should prepare a GAMESS input file with solvent assigned such as:<br><br>
 +
<center><big>$PCM SOLVNT=WATER $END</big></center><br>
 +
The details of PCM calculation in the GAMESS can be found in GAMESS manual. Keyword "VBTYP=XMVB" in CONTRL section is also essential. After the GAMESS input file is prepared, an XMI file with keyword "VBPCM" should be prepared with the same file name as GAMESS input file. In the current XMVB package, VBSCF/PCM and BOVB/PCM calculations are both supported.
 +
|}
  
<center><big><big><big> '''State correlation diagrams''' </big></big></big></center>
+
{| class="collapsible collapsed wikitable"
 +
|-
 +
!<big>'''Basic part'''</big>
 +
|-
 +
|
 +
==== 1. Compute the Energies and Wavefunctions at Reactant and Transition State with Different Sets of VB Structures====
 +
 
 +
We advise you to create the first xmvb input file (''.xmi'' file) for this study starting from a ''.xmi'' file taken from tutorial1 as a template. Alternatively, you may copy the input file corresponding for the first calculation of this study (L-VBSCF on reactant state geometry in vacuum) from the ''answer'' folder of this exercise (''cp answer/rs_vac_vbscf.xmi .''), run directly the first calculation, inspect input/outputs, and then use this ''.xmi'' file as a template for the following calculations.
 +
 
 +
# Write the following VB structure sets for a 3 centers / 4 electrons system :
 +
## all structures;
 +
## minimal structures for reactant;
 +
## minimal structures for product.
 +
# How would you define your different fragment orbitals for this calculation (''$frag'' section) ? You will find the answer for this case is in the [[General_guidelines_for_BOVB_calculations#Recommended_definition_for_the_orbital_blocks|"recommended definition for the orbital blocks" section of the "practical for BOVB calculations" document]]
 +
# Perform <math>\pi</math>-D-BOVB calculation for reactant [[General_guidelines_for_BOVB_calculations#High_symmetry_case:|(see "high symmetry cases" here)]]:
 +
## Perform all-structure <math>\pi</math>-D-BOVB calculation as following:
 +
### Perform L-VBSCF (file name: rs_vac_vbscf) calculation with "''orbtyp=hao frgtyp=sao guess=mo''", in which the orbitals are all localized on the Cl and CH<math>{}_3</math> groups;
 +
### Perform π-D-VBSCF calculation where <math>\pi</math> orbitals are delocalized in the whole system and the <math>\sigma</math> orbitals are kept localized (file name: rs_vac_d-vbscf). Use the L-VBSCF orbitals as initial guess;
 +
### Perform π-D-BOVB (file name: rs_vac_d-bovb) calculation with π-D-VBSCF orbitals as initial guess.
 +
## Perform <math>\pi</math>-D-BOVB calculations with minimal structures for reactant (file names: rs_vac_*_rs) and product (file names: rs_vac_*_ps) with the same procedure as all-structure calculation.
 +
# Perform <math>\pi</math>-D-BOVB calculation for transition state  (file names: ts_vac_*). The procedure is the same as step 2.
 +
# Perform <math>\pi</math>-D-BOVB/PCM calculations for reactant:
 +
## Perform all-structure <math>\pi</math>-D-BOVB/PCM  (file name: rs_pcm_d-bovb) calculation for the reactant, starting directly from the <math>\pi</math>-D-BOVB orbitals computed in vacuum (2.1)
 +
## Perform <math>\pi</math>-D-BOVB/PCM calculations with minimal structures for reactant  (file name: rs_pcm_d-bovb_rs) and product  (file name: rs_pcm_d-bovb), also starting from the corresponding <math>\pi</math>-D-BOVB orbitals computed in vacuum (2.2)
 +
# Perform BOVB/PCM calculations for transition state  (file names: rs_pcm_d-bovb*) with the same procedure as step 4.
  
 +
==== 2. Analysis: Wavefunctions and Energies====
 +
# Compare the weights of structures at both reactant and transition state points, find the differences.
 +
# Compute the Barrier height of the <math>\textrm{S}_{\textrm{N}}2</math> reaction in both vacuum and solution. See the difference of the barrier heights, and find out the reason.
 +
# Compare the energies of reactant and product structures at reactant and transition state geometries, in both vacuum and solution. What's the difference of the energies at different points? Why?
 +
# Compute the resonance energy at the crossing point of diabatic curves state points in vacuum.
  
= Remarks=
+
{| class="collapsible collapsed wikitable"
[[Tutorial 3 remarks for tutors |>> Initial remarks for tutors]]
+
|-
 +
!'''Answer'''
 +
|-
 +
|
 +
=====VB Structures in the Computations======
 +
<center>[[File:ClCH3Cl_Structures.png|600px]]</center><br>
 +
<center>Total VB Structure Set</center>
 +
<br>
 +
<center>[[File:ClCH3Cl_Reactant_Structures.png|600px]]</center><br>
 +
<center>VB Structure Set of The Reactant</center>
 +
<br>
 +
<center>[[File:ClCH3Cl_Product_Structures.png|600px]]</center><br>
 +
<center>VB Structure Set of The Product</center>
  
= Exercises =
+
=====Weights of Structures=====
 +
<center>
 +
{| border="1"
 +
|+ Weights of structures at Reactant Geometry
 +
! scope="col" |
 +
! scope="col" | S1
 +
! scope="col" | S2
 +
! scope="col" | S3
 +
! scope="col" | S4
 +
! scope="col" | S5
 +
! scope="col" | S6
 +
|-
 +
! scope="row"      |VBSCF
 +
| 0.590 || 0.002 || 0.001 || 0.338 || 0.070 || -0.000
 +
|-
 +
! scope="row"    | BOVB
 +
|0.587 ||  ||    || 0.352 || 0.061 ||
 +
|-
 +
! scope="row"      | VBSCF/PCM
 +
|0.604 || 0.001 || 0.001 || 0.316 || 0.078 || 0.000
 +
|-
 +
! scope="row"      | BOVB/PCM
 +
|0.639 ||    ||    || 0.413 || 0.131 || 
 +
|}
 +
</center>
 +
<br>
 +
<center>
 +
{| border="1"
 +
|+ Weights of structures at Transition State Geometry
 +
! scope="col" |
 +
! scope="col" | S1
 +
! scope="col" | S2
 +
! scope="col" | S3
 +
! scope="col" | S4
 +
! scope="col" | S5
 +
! scope="col" | S6
 +
|-
 +
! scope="row"      |VBSCF
 +
| 0.239 || 0.240 || 0.027 || 0.496 || -0.001 || -0.001
 +
|-
 +
! scope="row"    | BOVB
 +
| 0.228 || 0.228 || 0.041 || 0.502 ||    || 
 +
|-
 +
! scope="row"      | VBSCF/PCM
 +
|0.221 || 0.221 || 0.022 || 0.538 || -0.001 || -0.001
 +
|-
 +
! scope="row"      | BOVB/PCM
 +
|0.215 || 0.215 || 0.034 || 0.536 ||    || 
 +
|}
 +
</center>
  
<big><big>Main Exercise</big></big>
+
=====Barrier of the Reaction=====
 +
<center>
 +
{| border="1"
 +
|+ Energies (a.u.) and Barriers (kcal/mol) of <math>\textrm{S}_{\textrm{N}}2</math> Reaction
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | BOVB
 +
! scope="col" | VBSCF/PCM
 +
! scope="col" | BOVB/PCM
 +
|-
 +
! scope="row"      |Reactant
 +
| -37.03384 || -37.05085 || -37.13644 || -37.15356
 +
|-
 +
! scope="row"    | Trasition State
 +
| -36.98034  || -37.02508  || -37.06980 || -37.11346
 +
|-
 +
! scope="row"      | Barrier
 +
| 33.6 || 16.2 || 41.8 || 25.2
 +
|}
 +
</center>
  
<big>
+
=====Resonance Energ of Transition State=====
== Exercise 1 : Computation of state correlation Diagrams for a 3 centers / 4 electrons system ==
+
<center>
</big>
+
{| border="1"
 +
|+ Energies (a.u.) and Resonance Energies (kcal/mol) of Transition State
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | BOVB
 +
! scope="col" | BOVB/PCM
 +
|-
 +
! scope="row"    | All Structures
 +
| -36.98034 ||-37.02508 || -37.11346
 +
|-
 +
! scope="row" | Reactant
 +
| -36.95984 || -36.98719 || -37.07951
 +
|-
 +
! scope="row" | Product
 +
| -36.95984 ||-36.98718  || -37.07949
 +
|-
 +
! scope="row"      | Resonance Energy
 +
| 12.9 || 23.8  || 21.3
 +
|}
 +
</center>
  
* Computer exercise :
 
  
In this exercise the <math>\textrm{S}_{\textrm{N}}2</math> reaction Cl<math>{}^{-}</math> + CH3Cl -> ClCH3 + Cl<math>{}^{-}</math> will be computed in both vacuum and solution, at <math>\pi</math>-D-BOVB level. The basis set is 6-31+G*, for there is an anoin in the system. To make the computation simplified, only reactant and transition state will be computed in the exercise. It is recommended to the advanced users to draw the whole VBSCD.
 
<br>
 
<br>
 
<big>Compute the Energies and Wavefunctions at Reactant and Transition State with Different Set of VB Structures</big>
 
<br>
 
# Write the following VB structure sets, compare and see the difference, and think about why:
 
## all structures;
 
## minimal structures for reactant;
 
## minimal structures for product.
 
# Compute reactant in vacuum at <math>\pi</math>-D-BOVB level:
 
## Compute reactant at VBSCF level, with delocalized <math>\pi</math>-spaces, localized <math>\sigma</math>-space and all VB structures;
 
## Compute reactant at BOVB level, with VBSCF orbital as initial guess. The VB structures and orbital descriptions are the same as at VBSCF level.
 
## Do the same to computations with minimal structures for reactant and product.
 
# Compute transition state at BOVB level in vacuum. The procedure is the same as computations for reactant.
 
# Compute reactant in solution at  <math>\pi</math>-D-BOVB level:
 
## Compute reactant in solution at VBSCF level, with the same orbital descriptions and VB structures in vacuum, using VBSCF orbital in vacuum as initial guess.
 
## Do the BOVB calculation for reactant in solution, using VBSCF/PCM orbitals as initial guess.
 
## Do the BOVB calculations with structures at reactant and product point.
 
# Compute transition state in vacuum with the same procedure as for reactant in solution.
 
  
<br>
 
<big>Analyze the Data from Above Computations at <math>\pi</math>-D-BOVB level</big>
 
<br>
 
# Compute the Barrier height of the <math>\textrm{S}_{\textrm{N}}2</math> reaction in both vacuum and solution. See the difference of the barrier heights, and find out the reason.
 
# Compare the energies of reactant and product structures at reactant and transition state, in both vacuum and solution. What's the difference of the energies at different points? Why?
 
# Compute the resonance energies at both reactant and transition state points, see the difference of the resonance energies.
 
  
 +
{| class="collapsible collapsed wikitable"
 +
|-
 +
!<big>'''Optional part (expert users)'''</big>
 +
|-
 +
|
 +
In this part, calculations with BFI section are performed, which is a technique for the experienced users. The 6-31+G* basis set is used. The inner orbitals are frozen as HF orbitals in all VB calculations and the valence basis functions are reorganized to hybrid basis functions so that the <math>\sigma</math>, <math>\pi_x</math> and <math>\pi_y</math> spaces can be separated well. A D-BOVB calculation is performed in 2 steps:
 +
# Perform a VBSCF calculation with <math>\pi</math> orbitals delocalized in the whole system and <math>\sigma</math> orbitals localized on the Cl and CH<math>{}_3</math> groups;
 +
# Perform a BOVB calculation with VBSCF orbitals as initial guess.
 +
The VB calculations are the same as the calculations performed above. Try to understand the BFI section, perform the calculations and compare the differences of barrier heights, resonance energies and cpu performances with and without $BFI.
  
 +
{| class="collapsible collapsed wikitable"
 +
|-
 +
!'''Answer'''
 +
|-
 +
|
  
* ''Compute VBSCD diagrams for Cl(-) + CH3Cl -> ClCH3 + Cl(-), at π-D-BOVB levels, first in gas phase then using VB(PCM)... Which basis set should we use : 6-31+G*. As this is an anion we should add a set of diffuse functions, but then there may be trouble with BOVB... Check first that everything is fine at BOVB level (no instability)...''
+
=====Weights of Structures=====
 +
<center>
 +
{| border="1"
 +
|+ Weights of structures at Reactant Geometry
 +
! scope="col" |
 +
! scope="col" | S1
 +
! scope="col" | S2
 +
! scope="col" | S3
 +
! scope="col" | S4
 +
! scope="col" | S5
 +
! scope="col" | S6
 +
|-
 +
! scope="row"      |VBSCF
 +
| 0.632 || 0.003 || 0.001 || 0.299 || 0.064 || 0.000
 +
|-
 +
! scope="row"    | BOVB
 +
| 0.566 || 0.061 || 0.005 || 0.288 || 0.081 || 0.000
 +
|-
 +
! scope="row"      | VBSCF/PCM
 +
| 0.645 || 0.002 || 0.001 || 0.279 || 0.073 || 0.000
 +
|-
 +
! scope="row"      | BOVB/PCM
 +
| 0.599 || -0.019 || -0.007 || 0.337 || 0.089 || 0.000
 +
|}
 +
</center>
 +
<br>
 +
<center>
 +
{| border="1"
 +
|+ Weights of structures at Transition State Geometry
 +
! scope="col" |
 +
! scope="col" | S1
 +
! scope="col" | S2
 +
! scope="col" | S3
 +
! scope="col" | S4
 +
! scope="col" | S5
 +
! scope="col" | S6
 +
|-  
 +
! scope="row"      |VBSCF
 +
| 0.239 || 0.240 || 0.027 || 0.496 || -0.001 || -0.001
 +
|-
 +
! scope="row"    | BOVB
 +
| 0.263 || 0.263 || 0.043 || 0.416 || 0.007 || 0.007
 +
|-
 +
! scope="row"      | VBSCF/PCM
 +
| 0.220 || 0.220 || 0.020 || 0.542 || -0.001 || -0.001
 +
|-
 +
! scope="row"      | BOVB/PCM
 +
| 0.251 || 0.251 || 0.036 || 0.452 || 0.005 || 0.005
 +
|}
 +
</center>
  
* ''Reactant and product geometry will be CH3Cl and Cl(-) computed separately (CH3Cl has already been computed in tutorial 1, we just have to change the basis set, which is easy with XMVB 2.0 !) ;''
+
=====Barrier of the Reaction=====
* ''TS transition state : we take the linear TS, with orientation of the x or y axis along a C-H bond this will make a <math>\sigma</math>, <math>\pi_x</math>, <math>\pi_y</math> separation, so we could apply π-D-BOVB level, localizing all <math>\sigma</math> pairs (including inactive <math>\sigma</math> lone pairs and cores of Carbon and Chlorine atoms, and delocalizing the and <math>\pi_x</math> and <math>\pi_y</math> inactive orbitals from the beginning ([[General_guidelines_for_BOVB_calculations#High_symmetry_case:|(see also "high symmetry cases" here)|]].''
+
<center>
 +
{| border="1"
 +
|+ Energies (a.u.) and Barriers (kcal/mol) of <math>\textrm{S}_{\textrm{N}}2</math> Reaction
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | BOVB
 +
! scope="col" | VBSCF/PCM
 +
! scope="col" | BOVB/PCM
 +
|-
 +
! scope="row"      |Reactant
 +
| -958.65818 || -958.67599 || -958.75774 || -958.78203
 +
|-
 +
! scope="row"    | Trasition State
 +
| -958.62157 || -958.65321 || -958.71004 || -958.73960
 +
|-
 +
! scope="row"       | Barrier
 +
| 23.0 || 14.3 || 29.9 || 26.6
 +
|}
 +
</center>
  
[[Answer Exercise1 of tutorial 3|>> Answer]]
+
=====Resonance Energ of Transition State=====
 +
<center>
 +
{| border="1"
 +
|+ Energies (a.u.) and Resonance Energies (kcal/mol) of Transition State
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | BOVB
 +
! scope="col" | VBSCF/PCM
 +
! scope="col" | BOVB/PCM
 +
|-
 +
! scope="row"    | All Structures
 +
| -958.62157 || -958.65321 || -958.71004 || -958.73960
 +
|-
 +
! scope="row" | Reactant
 +
| -958.59188 || -958.60816 || -958.68547 || -958.70142
 +
|-
 +
! scope="row" | Product
 +
| -958.59188 || -958.60816 || -958.68547 || -958.70142
 +
|-
 +
! scope="row"      | Resonance Energy
 +
| 18.6 || 28.3 || 15.4 || 23.9
 +
|}
 +
</center>
  
 +
=====Resonance Energies of Reactant=====
 +
<center>
 +
{| border="1"
 +
|+ Energies(a.u.) and Resonance Energies (kcal/mol) of Reactant
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | BOVB
 +
! scope="col" | VBSCF/PCM
 +
! scope="col" | BOVB/PCM
 +
|-
 +
! scope="row"    | All Structures
 +
| -958.65818 || -958.67599 || -958.75774 || -958.78203
 +
|-
 +
! scope="row" | Reactant
 +
| -958.56752 || -958.67272 || -958.75734 || -958.77250 
 +
|-
 +
! scope="row" | Product
 +
| -958.31845 || -958.31845 || -958.57917 || -958.58246
 +
|-
 +
! scope="row"      | Resonance Energy
 +
| 0.4 || 2.1 || 0.3 || 6.0
 +
|}
 +
</center>
 +
|}
 +
|}
  
<big>[[General_guidelines_for_BOVB_calculations| >> general guidelines for BOVB calculations]]</big>
+
[[General_guidelines_for_BOVB_calculations| >> general guidelines for BOVB calculations]]
  
  
<big>
+
{| class="collapsible collapsed wikitable"
 +
|-
 +
!<big><big><big>'''Optional exercises - Homework'''</big></big></big>
 +
|-
 +
|
  
 
== Exercise 2 : computation of H—H + H. -> H. + H—H radical exchange VBSCD diagram ==
 
== Exercise 2 : computation of H—H + H. -> H. + H—H radical exchange VBSCD diagram ==
</big>
 
  
1/ Paper exercise :<br>
+
===1/ Paper exercise :===
  
 
[[File:vb-diagram.png]]
 
[[File:vb-diagram.png]]
Ligne 82 : Ligne 321 :
 
</math> (X = A = Y = hydrogen atom)
 
</math> (X = A = Y = hydrogen atom)
  
Write the HL wave functions for R and R* and derive the value of G using semiempirical VB theory. Indications : neglect the overlap beween the external atoms X and Y, and neglect the overlap between two different determinants.
+
Write the HL wave functions for R and R* and derive the value of G using semiempirical VB theory. Hints : 1) write the wave functions of R and R* so that their overlap is positive; 2) neglect the overlap beween the external atoms X and Y, and neglect the overlap between two different determinants.
  
 
b/ Considering the following reaction:
 
b/ Considering the following reaction:
Ligne 88 : Ligne 327 :
 
X^{\bullet} + H-X \rightarrow X-H +^{\bullet}X
 
X^{\bullet} + H-X \rightarrow X-H +^{\bullet}X
 
</math> <br>
 
</math> <br>
Use semiempirical VB theory to derive the following expression for the avoided crossing term B: <br>
+
Use semiempirical VB theory to derive the following expression for the avoided crossing term <big><math> B </math></big> : <br>
 
<big>
 
<big>
 
<math>B = 0.25\Delta E_{ST} </math>'</big>
 
<math>B = 0.25\Delta E_{ST} </math>'</big>
 
where <big> <math>\Delta E_{ST} </math>'</big> is the singlet-triplet transition energy of the X-H bond at the geometry of the transitions state.<br>
 
where <big> <math>\Delta E_{ST} </math>'</big> is the singlet-triplet transition energy of the X-H bond at the geometry of the transitions state.<br>
Now it is known that for strong binders, at any given bonding distance the singlet-triplet transition energy is larger than twice the bonding energy of the dimer at equilibrium distance, so that one can write the approximate expression <big> <math>\Delta E_{ST} </math>' <math> = 2  BDE </math></big>, where <big><math> BDE </math></big> is the bonding energy of the dimer at equilibrium distance. Using the latter expression, express the avoided crossing term <big><math> B </math></big>  as a function of the bonding energy of <big><math> H_{2}</math></big>.
+
Indication: the resonance energy arising from the mixing of two degenerate VB structures is given by the following expression:
 +
 
 +
<big><math>RE = [H_{12}-E_{ind}S_{12}]/(1+S_{12}) </math></big>
  
c/ Use semiempirical VB theory to show why the reaction: <math> X^{\bullet} + H-X \rightarrow X-H + ^{\bullet}X</math> has a barrier for <big><math>X= CH_{3}</math>, <math>SiH_{3}</math>, <math>GeH_{3}</math>, <math>SnH_{3}</math>, <math>PbH_{3}</math>, <math>H</math></big>, while the <big><math>Li_{3}</math></big> species in the process <math> Li^{\bullet} + Li-Li \rightarrow Li-Li + ^{\bullet}Li</math>  is a stable intermediate.
+
where <big><math> E_{ind} </math></big> is the energy of an individual VB structure, and <big><math> S_{12} </math></big> and <big><math> H_{12} </math></big> are respectively the overlap and Hamiltonian matrix element between R and R*.
First construct a VBSCD with the usual parameters <math>\Delta E_{ST}, f, G, B</math>.
 
Where <math>\Delta E_{ST}</math> is the singlet-triplet transition energy of the X-H bond at the geometry of the transition state. For convenience, define the energy of a Lewis bond, for example, H-X (or X-X), relative to the nonbonded quasiclassical reference determinant, as follows:<br>
 
<big><math>E_{S}(H-X)=-\lambda_{S}</math><small> and </small> <math>D(H-X)=\lambda_{S}</math></big> where <big><math>\lambda_{S}</math></big> is used as a shorthand notation for <math>2\beta S/(1+S^2)</math>.
 
Similarly, denote the energy of the triplet pair <math>H \uparrow \uparrow X</math> (or of <math>X \uparrow \uparrow X</math>) by: <math>E_{T}(H \uparrow \uparrow X)=\lambda_{T}</math>, where <big><math>\lambda_{T}</math></big> is the corresponding <math>-2\beta S/(1-S^2)</math> terms for the triplet repulsion. While <big><math>\lambda_{S}</math></big> and <big><math>\lambda_{T}</math></big> are defined at the equilibrium distance of the H-X (or X-X) bond, analogous parameters <big><math>\lambda'_{S}</math></big> and <big><math>\lambda'_{T}</math></big> are defined for the stretched H-X (or X-X) bond corresponding to the geometry of the transition state. Based on these notations derive the following relations and quantities:<br>
 
- Express <math>\Delta E_{ST}</math> and <big><math>G</math></big> as functions of <big><math>\lambda_{S}</math></big> and <big><math>\lambda_{T}</math></big>.<br>
 
- Express the avoided crossing interaction <big><math>B</math></big> as a function of <big><math>\lambda'_{S}</math></big> and <big><math>\lambda'_{T}</math></big>.<br>
 
- Express the energy of the crossing point (relative to the reference quasiclassical determinant) as a function of <big><math>\lambda'_{S}</math></big> and <big><math>\lambda'_{T}</math></big>.<br>
 
- To enable yourself to derive a simple expression for the barrier, assume that <big><math>\lambda'_{S}=\lambda'_{T}</math></big>. Then express <math>\Delta E_{C}</math>, the height of the crossing point relative to the reactants, and derive an expression for <math>f</math>, as a function of <math>\alpha</math>, defined as follows: <math>\alpha=\lambda_{S}/\lambda_{T}</math>.<br>
 
- Derive an expression for the barrier <math>\Delta E^{\neq}</math>, as a function of <math>\Delta E_{ST}</math> and <math>\alpha</math>. Knowing that <math>\lambda_{T}</math> is generally larger than <math>\lambda_{S}</math> for strong binders, such as X-H (<math>X= CH_{3}</math>, <math>SiH_{3}</math>, <math>GeH_{3}</math>, <math>SnH_{3}</math>, <math>PbH_{3}</math>, <math>H</math>) while the opposite is true for weak binders, such as alkali atoms, show that the reaction <math>X^{\bullet} + H-X \rightarrow X-H + ^{\bullet}X</math> has a barrier while the <big><math>Li_{3}</math></big> species is a stable intermediate in the process <math> Li^{\bullet} + Li-Li \rightarrow Li-Li + ^{\bullet}Li</math>.
 
  
 +
c/ It is known that for strong binders, at any given bonding distance the singlet-triplet transition energy is larger than twice the bonding energy of the dimer at equilibrium distance, so that one can write the approximate expression <big> <math>\Delta E_{ST} </math>' <math> = 2  BDE </math></big>, where <big><math> BDE </math></big> is the bonding energy of the dimer at equilibrium distance. Using the latter expression, express the avoided crossing term <big><math> B </math></big>  as a function of the bonding energy of <big><math> H_{2}</math></big>.
  
2/ Computer exercise :VBSCD for H—H + H. -> H. + H—H at VBSCF then VBCISD level.
+
{| class="collapsible collapsed wikitable"
 +
|-
 +
!'''Answer'''
 +
|-
 +
|
 +
a - Considering the R and R* states for the radical exchange process, the HL wave functions for R and R* are the following :<br>
 +
<math>\psi (R)=(|xa\overline{y}|-|x\overline{a}y|)(1/2)^{-1/2} </math><br>
 +
<math>\psi (R^{*})=(|x\overline{a}y|-|\overline{x}ay|)(1/2)^{-1/2}</math><br>
 +
At the equilibrium distance of R, A and Y are close together while X is far away. Therefore R is stabilized by a covalent bond and its energy is <big><math> 2 \beta S </math></big>. In R*, the AY entity has two parallel spins 50% of the time (a repulsive situation), and alternated spins 50% of the time (a non-bonding situation). Therefore the energy of R* is half a triplet repulsion, i.e. <big><math> - \beta S </math></big>. As <big><math>\Delta E_{ST} (A-Y)= 4  \beta S </math></big>, the final G expression is:<br>
 +
<big><math>G=0.75 \Delta E_{ST} (A-Y)</math></big><br>
 +
 
 +
b - Let us express the various energies and matrix elements in terms of the usual <big><math> \beta </math></big> and  <big><math> S </math></big> integrals between the X and H orbitals:
 +
 
 +
<big><math> E_{ind} = \beta S </math></big>
 +
 
 +
<big><math> S_{12} = 0.5 </math></big>
 +
 
 +
<big><math> H_{12} = 2 \beta S </math></big>
 +
 
 +
<big><math> RE = (2 \beta S - 0.5 \beta S )/1.5 = \beta S </math></big>
 +
 
 +
Since at the transition state geometry <big> <math>\Delta E_{ST} </math>'</big> = <big><math> 4 \beta S </math></big>, we have:
 +
 
 +
<big> <math>B = 0.25\Delta E_{ST} </math>'</big>
 +
 
 +
c - Since <big> <math>\Delta E_{ST} </math>' <math> = 2  BDE </math></big>, we may re-express the avoided crossing term as:
 +
 
 +
<big> <math>B = 0.5BDE </math></big>
 +
|}
 +
 
 +
=== 2/ Computer exercise ===
 +
VBSCD for H—H + H. -> H. + H—H at VBSCF then VBCISD level.
  
 
In this exercise the VBSCD for H—H + H. -> H. + H—H at VBSCF then VBCISD level will be computed with 6-31G**. Computations for reactant and transition state are requested and other points are optional for advanced users.
 
In this exercise the VBSCD for H—H + H. -> H. + H—H at VBSCF then VBCISD level will be computed with 6-31G**. Computations for reactant and transition state are requested and other points are optional for advanced users.
 
<br>
 
<br>
 
<br>
 
<br>
<big>Compute the Energies and Wavefunctions at Reactant and Transition State with Different Set of VB Structures</big>
+
<big>'''2.1 Computations'''</big>
<br>
+
 
# Write the following VB structure sets, compare and see the difference, and think about why:
+
Compute the Energies and Wavefunctions at Reactant and Transition State with Different Sets of VB Structures
 +
 
 +
# Write the following VB structure sets, compare and see the difference:
 
## all structures;
 
## all structures;
 
## minimal structures for reactant;
 
## minimal structures for reactant;
 
## minimal structures for product.
 
## minimal structures for product.
# Compute reactant at VBSCF and VBCISD level:
+
# Perform VBSCF and VBCISD calculations for reactant:
## Compute reactant at VBSCF level with "''orbtyp=hao''" and "''boys''";
+
## Perform a VBSCF calculation (file name: rs_vbscf) with "''orbtyp=hao''" and "''boys''";
## Compute reactant at VBCISD level, with VBSCF orbital as initial guess.
+
## Perform a VBCISD calculation (file name: rs_vbcisd) with VBSCF orbital as initial guess.
## Do the same to computations with minimal structures for reactant and product point.
+
## Perform VBSCF and VBCISD calculations with minimal structures for reactant (file names: rs_*_rs) and product (file names: rs_*_ps).
# Compute transition state at VBCISD level with the same procedure as for reactant.
+
# Perform VBSCF and VBCISD calculations for transition state (file names: ts_*) with the same procedure as in step 2.
  
 
<br>
 
<br>
<big>Analyze the Data from Above Computations at <math>\pi</math>-D-BOVB level</big>
+
<big>'''2.2 Analysis: Wavefunctions and Energies'''</big>
 
<br>
 
<br>
 
# Compute the Barrier height of the <math>\textrm{S}_{\textrm{N}}2</math> reaction at VBSCF and VBCISD levels. See the difference of the barrier heights.
 
# Compute the Barrier height of the <math>\textrm{S}_{\textrm{N}}2</math> reaction at VBSCF and VBCISD levels. See the difference of the barrier heights.
Ligne 131 : Ligne 397 :
  
 
<br>
 
<br>
<big>Optional:</big> Compute all points and draw the VBSCDs at VBSCF and VBCISD levels.
+
<big>'''2.3 Optional : Compute all points and draw the VBSCDs at VBSCF and VBCISD levels.'''</big>
 
<br>
 
<br>
  
 +
{| class="collapsible collapsed wikitable"
 +
|-
 +
!'''Answer'''
 +
|-
 +
|
 +
a- VB Structures used in the computations
 +
<center>[[File:Structures.png|600px]] </center><br>
 +
<center>Total 8 Structures of The System</center>
 +
<br>
 +
<center>[[File:Reactant_Structures.png|400px]] </center><br>
 +
<center>Structures of The Reactant State</center>
 +
<br>
 +
<center>[[File:Product_Structures.png|400px]] </center><br>
 +
<center>Structures of The Product State</center>
 +
<br>
 +
b- Computational results
 +
<br>
 +
<center>
 +
{| border="1"
 +
|+ Weights of VB Structures of H-H-H Abstract Reaction at Reactant Geometry
 +
|-
 +
! scope="col" |
 +
! scope="col" | S1
 +
! scope="col" | S2
 +
! scope="col" | S3
 +
! scope="col" | S4
 +
! scope="col" | S5
 +
! scope="col" | S6
 +
! scope="col" | S7
 +
! scope="col" | S8
 +
|-
 +
! scope="row" | VBSCF
 +
| 0.803 || 0.003 || 0.096 || 0.001 || 0.095 || 0.000 || 0.000 || 0.000
 +
|-
 +
! scope="row" | VBCISD
 +
| 0.770 || 0.005 || 0.110 || 0.003 || 0.111 || 0.000 || 0.000 || 0.001
 +
|-
 +
|}
 +
</center>
 +
<br>
 +
<center>
 +
{| border="1"
 +
|+ Weights of VB Structures of H-H-H Abstract Reaction at Transition State Geometry
 +
|-
 +
! scope="col" |
 +
! scope="col" | S1
 +
! scope="col" | S2
 +
! scope="col" | S3
 +
! scope="col" | S4
 +
! scope="col" | S5
 +
! scope="col" | S6
 +
! scope="col" | S7
 +
! scope="col" | S8
 +
|-
 +
! scope="row" | VBSCF
 +
| 0.344 || 0.344 || 0.096 || 0.035 || 0.025 || 0.025 || 0.096 || 0.035
 +
|-
 +
! scope="row" | VBCISD
 +
| 0.358 || 0.358 || 0.059 || 0.036 || 0.046 || 0.046 || 0.059 || 0.036
 +
|-
 +
|}
 +
</center>
 +
<br>
 +
<center>
 +
{| border="1"
 +
|+ Energies (a.u.) and Barriers (kcal/mol) of H-H-H Abstract Reaction
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | VBCISD
 +
|-
 +
! scope="row"      |Reactant 
 +
| -1.64637 || -1.66241
 +
|-
 +
! scope="row"    | Transition State
 +
| -1.60706 || -1.63827
 +
|-
 +
! scope="row"      | Barrier
 +
| 24.7 || 15.1
 +
|-
 +
|}
 +
</center>
 +
<br>
 +
<center>
 +
{| border="1"
 +
|+ Energies(a.u.) and Resonance Energies (''B'', in kcal/mol) of H-H-H Abstract Reaction at Reactant Geometry
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | VBCISD
 +
|-
 +
! scope="row"      | All Structures 
 +
| -1.64637 || -1.66241
 +
|-
 +
! scope="row"      | Reactant
 +
| -1.64617 || -1.66208
 +
|-
 +
! scope="row"      | Product
 +
| -1.40873 || -1.41851
 +
|-
 +
! scope="row"      | ''B''
 +
| 0.1 || 0.2
 +
|-
 +
|}
 +
</center>
 +
<br>
 +
<center>
 +
{| border="1"
 +
|+ Energies (a.u.) and Resonance Energies (''B'', in kcal/mol) of H-H-H Abstract Reaction at Transition State Geometry
 +
! scope="col" |
 +
! scope="col" | VBSCF
 +
! scope="col" | VBCISD
 +
|-
 +
|-
 +
! scope="row"    | All Structures
 +
| -1.60706 || -1.63827
 +
|-
 +
! scope="row"    | Reactant
 +
| -1.54798 || -1.56655
 +
|-
 +
! scope="row"    | Product
 +
| -1.54798 || -1.56655
 +
|-
 +
! scope="row"      | ''B''
 +
| 37.1 || 45.0
 +
|-
 +
|}
 +
</center>
 +
<br>
 +
<br>
  
[[Answer Exercise2 of tutorial 3|>> Answer]]
+
<center><big>Optional : VBSCDs for H-H-H abstract reaction by VBSCF and VBCISD</big></center>
 +
 
 +
[[File:H3-VBSCD-VBSCF.png|500px]]  [[File:H3-VBSCD-VBCISD.png|500px]]<br>
 +
<big> {{pad|250px}} VBSCF  {{pad|420px}}  VBCISD </big>
 +
|}
  
 
== Exercise 3 (paper exercise) : Conical intersection in H<sub>3</sub><sup>•</sup> radical ==
 
== Exercise 3 (paper exercise) : Conical intersection in H<sub>3</sub><sup>•</sup> radical ==
Ligne 151 : Ligne 549 :
  
 
'''Appendix : Thumb rules for the calculations of effective Hamiltonian matrix elements between determinants.'''
 
'''Appendix : Thumb rules for the calculations of effective Hamiltonian matrix elements between determinants.'''
# Energy of a determinant D : [[File:E(D).png|120px]]]  (if orbitals i and j have parallel spins)
 
# Matrix element between determinants differing by spin inversion of two spin-orbitals :[[File:Hij.png|220px]]]
 
  
[[Answer Exercise3 of tutorial 3|>> Answer]]
+
* Energy of a determinant D : <math><D|H|D> = -2 \sum_{i<j}^{ } \beta_{ij} S_{ij}</math>  (if orbitals i and j have parallel spins)
 +
 
 +
* Matrix element between determinants differing by spin inversion of two spin-orbitals :
 +
 
 +
<big><math> <D|H|D'>=<|...i\overline{j}...||H||...\overline{i}j...|>= -2 \beta_{ij} S_{ij}</math></big> (for <big><math>D</math>, <math>D'</math></big> differing by spin inversion of two spin-orbitals)
 +
 
 +
{| class="collapsible collapsed wikitable"
 +
|-
 +
!'''Answer'''
 +
|-
 +
|
 +
<math> R = \frac{1}{\sqrt{2}} (|ab\overline{c}|-|a\overline{b}c|) </math><br>
 +
<math> P = \frac{1}{\sqrt{2}} (|a\overline{b}c|-|\overline{a}bc|) </math><br>
 +
 
 +
1 - Using the thumb rules 
 +
 
 +
<big><math> <D|H|D>= -2 \sum_{i<j}^{ } \beta_{ij} S_{ij} </math>(if orbitals i and j have parallel spins)  </big>
 +
<big><math> <D|H|D'>=<|...i\overline{j}...||H||...\overline{i}j...|>= -2 \beta_{ij} S_{ij} </math>(for D, D' differing by spin inversion of two spin-orbitals</big>
 +
 
 +
It comes,<br>
 +
<big><math> <R|H|R>= \frac{1}{2} (4\beta_{bc}S_{bc} -2\beta_{ab}S_{ab} -2\beta_{ac}S_{ac})</math></big><br>
 +
<big><math> <P|H|P>= \frac{1}{2} (4\beta_{ab}S_{ab} -2\beta_{bc}S_{bc} -2\beta_{ac}S_{ac})</math></big><br>
 +
 +
<big><math> <R|H|P>= \frac{1}{2} (4\beta_{ac}S_{ac} -2\beta_{ab}S_{ab} -2\beta_{bc}S_{bc})</math></big><br>
 +
 
 +
 
 +
2 - If <math>\theta </math> > 60° ,<big> <math>\beta_{ac}S_{ac} < \beta_{ab}S_{ab}=\beta_{bc}S_{bc} </math></big> Hence <big><math><R|H|P> > 0 </math></big> (<math>\beta_{ij} < 0</math>) <br>
 +
 
 +
Finally, ground state is out of phase and the excited state is in phase.
 +
 
 +
It comes:<br>
 +
:<big><math> \Psi^{\neq} = R-P</math></big><br>
 +
:<big><math> \Psi^{\star} = R+P</math></big><br>
 +
 
 +
Expanding on the determinants
 +
:<big><math> \Psi^{\neq} = 1/\sqrt{2} (|ab\overline{c}|+|\overline{a}bc|-2|a\overline{b}c|)</math></big><br>
 +
:<big><math> \Psi^{\star} =1/\sqrt{2} (|ab\overline{c}|-|\overline{a}bc|)</math></big><br>
 +
 
 +
<math> \Psi^{\star} </math>, wave function of the excited state represent a bonding between hydrogens a and c.<br>
 +
 
 +
3- Using geometric considerations
 +
* If <math>\theta </math> = 180° ,<big> <math>\beta_{ac}S_{ac}=0</math></big> and <big><math> <R|H|P>=-(\beta_{ab}S_{ab} +\beta_{bc}S_{bc})</math> </big><br>
 +
 
 +
* If <math>\theta </math> = 60° ,<big> <math>\beta_{ac}S_{ac}=\beta_{ab}S_{ab}=\beta_{bc}S_{bc}=\beta S</math></big> and <big><math> <R|H|P>=0</math></big> <br>
 +
 
 +
4- If <math>\theta </math> = 60°, <big><math> <R|H|P>=0 = <R|H|R>= <P|H|P></math></big> <br>
 +
Hence R and P are degenerated eigenfunction of the CI Hamiltonian :  <math>E_R=E_P=0</math><br>
 +
Their linear combination <math> \Psi^{\neq}  </math> and  <math>\Psi^{\star} </math> are also degenerated, with the same value.
 +
 
 +
5- Allyl radical <math>\pi</math> system is isoelectronic to the <math>H_3</math> radical case. 
 +
R corresponds to the covalent right coupling (radical on the left carbone atom). P to the covalent right coupling.
 +
* <math> \Psi^{\neq}  </math> corresponds to the resonance (mesomery) between these 2 bonding schemes.
 +
* <math>\Psi^{\star} </math> to the "through space" (a,c) electronic coupling ("long bond", the radical is centered on the middle atom).
 +
 
 +
The geometrical distortion to make the two states degenerated in allyl radical would be a rotation of the two CH2 end groups: by such a rotation, the resonance structures are destabilized (pi bonds break), and the a-c coupling is re-inforced (sigma bond forms).
 +
 
 +
The end product obtained  from the first excited state of allyl radical is a cyclopropyl radical (formation of the a-c bond).
 +
 
 +
 
 +
|}
 +
 
 +
|}
 +
 
 +
 
 +
 
 +
 
 +
 
 +
----

Dernière version du 18 janvier 2013 à 15:56

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Valence Bond State correlation diagrams

Exercise 1 : Computation of state correlation Diagrams for a 3 centers / 4 electrons system

In this exercise the <math>\textrm{S}_{\textrm{N}}2</math> reaction Cl<math>{}^{-}</math> + CH<math>{}_3</math>Cl -> ClCH<math>{}_3</math> + Cl<math>{}^{-}</math> will be studied in both vacuum and solution. Valence Bond State Correlation Diagrams (VBSCD) will be constructed at <math>\pi</math>-D-BOVB level. There are two parts in this exercise: basic part and optional part. The basic part is performed with MCP-DZP basis set in which the inner orbitals in Cl and C are described with MCP pseudo potential. The optional part is performed with 6-31+G* basis set, using the general specification for the xmvb input (expert users). Only reactant and transition state will be computed in this exercise, which is sufficient to build the VBSCD diagrams.