Difference between revisions of "Calculating optical spectra including excitonic effects: a step-by-step guide"
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===Step 4: Include previous quasiparticle (GW) results === | ===Step 4: Include previous quasiparticle (GW) results === | ||
Follow the module on '''[[ | Follow the module on '''[[Bethe-Salpeter on top of quasiparticle energies|including the quasiparticle database]]''' and '''return to this tutorial''' | ||
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Revision as of 14:07, 24 March 2021
This tutorial guides you through the workflow of a calculation of the optical spectrum of a given material by solving the Bethe-Salpeter equation. Specifically, we will use bulk h-BN as an example.
Before starting, you need to obtain the tarballs for hBN. See instructions on the main tutorials page.
The target quantity in a Bethe-Salpeter calculation is the macroscopic dielectric matrix εM. The following quantities/steps are needed to obtain εM:
The optical absorption spectrum corresponds to ImεM(ω). Following this scheme we go through the flow of a calculation:
Step 1: Static screening
Use the SAVE folders that are already provided and type:
$ cd YAMBO_TUTORIALS/hBN/YAMBO
Follow the Static screening module and then return to this tutorial
Step 2: Bethe-Salpeter kernel
Follow the module on Bethe-Salpeter kernel and return to this tutorial
Step 3: Diagonalisation of the excitonic Hamiltonian
This is the step in which you obtain the spectra. Mathematically this implies solving a large eigenvalue problem. In this case we are going to directly diagonalise the matrix, but there are different numerical approaches available in Yambo. The difference between the various other approaches and when they should be used is the object of one of the next tutorials.
Follow the module on Bethe-Salpeter solver: diagonalization then return to this tutorial
Step 4: Include previous quasiparticle (GW) results
Follow the module on including the quasiparticle database and return to this tutorial