BSE hBN Yambo Virtual 2021 version: Difference between revisions
Jump to navigation
Jump to search
No edit summary |
No edit summary |
||
| Line 3: | Line 3: | ||
We are going to compute optical absorption spectra when strong excitonic effects are present via the Bethe-Salpeter equation. | We are going to compute optical absorption spectra when strong excitonic effects are present via the Bethe-Salpeter equation. | ||
We will use bulk hBN as an example system. Before starting, you need to obtain the appropriate tarball. See instructions on the [[Tutorials|main tutorials page]]. <br> | We will use bulk hBN as an example system. Before starting, you need to obtain the appropriate tarball: [http://www.yambo-code.org/educational/tutorials/files/hBN.tar.gz hBN.tar.gz]. See instructions on the [[Tutorials|main tutorials page]]. <br> | ||
We strongly recommend that you first complete the [[First steps: a walk through from DFT to optical properties]] and [[GW hBN Yambo Virtual 2021 version]] tutorials. | We strongly recommend that you first complete the [[First steps: a walk through from DFT to optical properties]] and [[GW hBN Yambo Virtual 2021 version]] tutorials. | ||
Revision as of 13:06, 24 March 2021
This is a modified version of the standard tutorial prepared for the Yambo 2021 virtual school.
We are going to compute optical absorption spectra when strong excitonic effects are present via the Bethe-Salpeter equation.
We will use bulk hBN as an example system. Before starting, you need to obtain the appropriate tarball: hBN.tar.gz. See instructions on the main tutorials page.
We strongly recommend that you first complete the First steps: a walk through from DFT to optical properties and GW hBN Yambo Virtual 2021 version tutorials.
In this tutorial you will learn how to: