From 63e3653fb789159462141c1fde8c76ce73dacaad Mon Sep 17 00:00:00 2001 From: "Jose M. Pizarro" <112697669+JosePizarro3@users.noreply.github.com> Date: Sat, 25 May 2024 00:27:45 +0200 Subject: [PATCH] Testing --- README.md | 3 +++ 1 file changed, 3 insertions(+) diff --git a/README.md b/README.md index 1a43c99..9a77d24 100644 --- a/README.md +++ b/README.md @@ -3,3 +3,6 @@ The Slave-Spin Mean-Field (SSMF) approach is a methodology based on solving the Hubbard-Kanamori model based on tight-bindings to obtain the orbital **quasiparticle weights** and **occupations**. It is based on the Brinkmann-Rice picture, so that it can trace the evolution of these quantities in terms of U, JH, T, total nominal filling; but once the Mott phase is reached (i.e., all quasiparticle weights are 0), then there is not more information. Thus it is a good approach to study how strongly correlated are certain metals: weakly correlated if the quasiparticle weights are 0.7 - 1.0, strongly correlated if the quasiparticle weights are lower than 0.4 - 0.5. It can also reproduce the **orbital-selective Mott transitions**, meaning some orbital quasiparticles weights are zero, while others are finite. + + +This is a test to check if Github copilot can do summaries of my pull requests! \ No newline at end of file