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Difference between revisions of "User:Delphi/Worktodo"
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* Continue the analysis and increment the trimer temp to ~150K | * Continue the analysis and increment the trimer temp to ~150K | ||
| − | : Nose @ 50K - inc. microcanonical run for 5ps | + | : Nose @ 50K - inc. microcanonical run for 5ps - <span style="color:green;"> Both input files on cluster ready inc. m/c run</span> |
: Nose @ 100K - inc. microcanonical run for 5ps | : Nose @ 100K - inc. microcanonical run for 5ps | ||
: Nose @ 150K - inc. microcanonical run for 5ps | : Nose @ 150K - inc. microcanonical run for 5ps | ||
| Line 22: | Line 22: | ||
:: Run NEB simulation on capa | :: Run NEB simulation on capa | ||
| + | == Report == | ||
| + | |||
| + | * Finish DFT theory section | ||
| + | * Add graphs to work section | ||
| + | * Do dimer section | ||
| + | * Do trimer section | ||
| + | * Do tetramer section | ||
| + | * Do LDA subsection | ||
| + | * Do GGA subsection | ||
| + | * Future work section | ||
| + | * Conclusion | ||
| + | * Edit the mono/di/tri images to include geometrical information | ||
[[Category:User:Delphi]] | [[Category:User:Delphi]] | ||
Latest revision as of 15:42, 17 June 2008
NB. This is a personal page test - please do not edit
University Work to do:
Trimer
- Continue the analysis and increment the trimer temp to ~150K
- Nose @ 50K - inc. microcanonical run for 5ps - Both input files on cluster ready inc. m/c run
- Nose @ 100K - inc. microcanonical run for 5ps
- Nose @ 150K - inc. microcanonical run for 5ps
- Then run microcanonical sim for 15ps with last 10ps with &DIPOLE card switched on for the molecule polarisation
- Calculate dipole moment classically for the Trimer (uud)
- Then run microcanonical sim for 15ps with last 10ps with &DIPOLE card switched on for the molecule polarisation
Dimer
- Do NEB calculations for the dimer dissociation
- Run on capablanca the initial configuration
- Including electronic and ionic GS configurations
- Run on capablanca the final configuration
- Including electronic and ionic GS configurations
- Create NEB input file with final positions for the GS of the initial/final
- Run NEB simulation on capa
Report
- Finish DFT theory section
- Add graphs to work section
- Do dimer section
- Do trimer section
- Do tetramer section
- Do LDA subsection
- Do GGA subsection
- Future work section
- Conclusion
- Edit the mono/di/tri images to include geometrical information
