Rome 2023: Difference between revisions
Jump to navigation
Jump to search
No edit summary |
No edit summary |
||
| Line 9: | Line 9: | ||
* [[First steps: walk through from DFT(standalone)|First steps: Initialization and more ]] | * [[First steps: walk through from DFT(standalone)|First steps: Initialization and more ]] | ||
* [[Next steps: RPA calculations (standalone)|Next steps: RPA calculations ]] | * [[Next steps: RPA calculations (standalone)|Next steps: RPA calculations ]] | ||
* [[Yambopy tutorial: band structures| | * [[Yambopy tutorial: band structures|QE band structures, orbital-projected and spin-polarised: Tutorial 1]] | ||
* [[Yambopy tutorial: band structures|QE band structures, orbital-projected and spin-polarised: Tutorial 2]] | |||
=== DAY 2 - Tuesday, 23 May === | === DAY 2 - Tuesday, 23 May === | ||
Revision as of 15:43, 4 May 2023
A general description of the goal(s) of the school can be found on the Yambo main website
Tutorials
DAY 1 - Monday, 22 May
16:15 - 18:30 From the DFT ground state to the complete setup of a Many Body calculation using Yambo
- First steps: Initialization and more
- Next steps: RPA calculations
- QE band structures, orbital-projected and spin-polarised: Tutorial 1
- QE band structures, orbital-projected and spin-polarised: Tutorial 2
DAY 2 - Tuesday, 23 May
DAY 3 - Wednesday, 24 May
DAY 4 - Thursday, May 25
17:00 - 18:30 Real-time approach and Calculation of linear response functions and optical properties Myrta Gruning (), Davide Sangalli (CNR-ISM, Italy)
14:00 - 16:30 Real time approach and Calculation of non linear properties (second harmonic generation) Myrta Gruning (), and Davide Sangalli (CNR-ISM, Italy)