Changed repo name from SSMF to pySSMF

README.md

@@ -1,10 +1,4 @@
-# SSMF
-
-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, J<sub>H</sub>, 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.
-
-
+# pySSMF
 
 ## Installation steps
 

mkdocs.yml

@@ -1,8 +1,8 @@
-site_name: "SSMF Documentation"
+site_name: "pySSMF Documentation"
 site_description: |
-  SSMF Documentation for strongly correlated metals 
-site_author: JMPizarro
-repo_url: https://github.com/JosePizarro3/SSMF
+  oySSMF Documentation for strongly correlated systems
+site_author: JoseMPizarro
+repo_url: https://github.com/JosePizarro3/pySSMF
 nav:
   - Home: index.md
 theme:

pyproject.toml

@@ -22,9 +22,9 @@ dependencies = [
 ]
 
 [project.urls]
-"Homepage" = "https://github.com/JosePizarro3/SSMF"
-"Bug Tracker" = "https://github.com/JosePizarro3/SSMF/issues"
-"Documentation" = "https://josepizarro3.github.io/SSMF/"
+"Homepage" = "https://github.com/JosePizarro3/pySSMF"
+"Bug Tracker" = "https://github.com/JosePizarro3/pySSMF/issues"
+"Documentation" = "https://josepizarro3.github.io/pySSMF/"
 
 [project.optional-dependencies]
 dev = [