<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://wiki.yambo-code.eu/wiki/index.php?action=history&amp;feed=atom&amp;title=BSE_tutorial_on_hBN</id>
	<title>BSE tutorial on hBN - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://wiki.yambo-code.eu/wiki/index.php?action=history&amp;feed=atom&amp;title=BSE_tutorial_on_hBN"/>
	<link rel="alternate" type="text/html" href="https://wiki.yambo-code.eu/wiki/index.php?title=BSE_tutorial_on_hBN&amp;action=history"/>
	<updated>2026-05-17T16:56:08Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.39.8</generator>
	<entry>
		<id>https://wiki.yambo-code.eu/wiki/index.php?title=BSE_tutorial_on_hBN&amp;diff=6703&amp;oldid=prev</id>
		<title>Fulvio: New page for 2023 school (necessary because the title of the old page explicitly mentioned the 2021 school)</title>
		<link rel="alternate" type="text/html" href="https://wiki.yambo-code.eu/wiki/index.php?title=BSE_tutorial_on_hBN&amp;diff=6703&amp;oldid=prev"/>
		<updated>2023-05-19T12:01:43Z</updated>

		<summary type="html">&lt;p&gt;New page for 2023 school (necessary because the title of the old page explicitly mentioned the 2021 school)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;We are going to compute optical absorption spectra when strong excitonic effects are present via the Bethe-Salpeter equation.&lt;br /&gt;
&lt;br /&gt;
We will use bulk hBN as an example system. Before starting, you need to obtain the appropriate tarball: [https://www.yambo-code.org/educational/tutorials/files/hBN.tar.gz hBN.tar.gz]. For the last part of the convergence tutorial (step 4.), you will also need the [https://www.yambo-code.org/educational/tutorials/files/hBN-convergence-kpoints.tar.gz hBN-convergence-kpoints.tar.gz] tarball. See instructions on the [[Tutorials|main tutorials page]]. &amp;lt;br&amp;gt;&lt;br /&gt;
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.&lt;br /&gt;
&lt;br /&gt;
==Contents==&lt;br /&gt;
In this tutorial you will learn how to:&lt;br /&gt;
# [[Calculating optical spectra including excitonic effects: a step-by-step guide|Perform a Bethe-Salpeter calculation from beginning to end]]&lt;br /&gt;
# [[How to analyse excitons - CECAM 2021 school|Analyse your results (exciton wavefunctions in real and reciprocal space, etc.)]]&lt;br /&gt;
# [[BSE solvers overview|Solve the BSE eigenvalue problem with different numerical methods]] &lt;br /&gt;
# [[How to choose the input parameters|Choose the input parameters for a meaningful converged calculation]]&lt;br /&gt;
&lt;br /&gt;
==Links for schools==&lt;br /&gt;
* Back to [[Rome 2023#Tutorials]]&lt;br /&gt;
* Back to [[ICTP 2022]]&lt;br /&gt;
* Back to [[CECAM VIRTUAL 2021]]&lt;br /&gt;
* Back to [[ICTP2020]]&lt;br /&gt;
* [[Modules|Back to technical modules menu]]&lt;br /&gt;
* [[Tutorials|Back to tutorials menu]]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br&amp;gt;&lt;br /&gt;
{| style=&amp;quot;width:100%&amp;quot; border=&amp;quot;1&amp;quot;&lt;br /&gt;
|style=&amp;quot;width:15%; text-align:left&amp;quot;|Prev: [[Tutorials| Tutorials Home]] &lt;br /&gt;
|style=&amp;quot;width:70%; text-align:center&amp;quot;|Now: [[Tutorials| Tutorials Home]] --&amp;gt; [[Linear response from real time simulations|Linear Response]]&lt;br /&gt;
|style=&amp;quot;width:15%; text-align:right&amp;quot;|Next: [[Introduction to Real Time propagation in Yambo|Theory]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Fulvio</name></author>
	</entry>
</feed>