From 96fea4389bfc6f19a68a5c7013b1400e070738be Mon Sep 17 00:00:00 2001 From: Dylan Simon Date: Mon, 25 Jun 2018 10:23:30 -0400 Subject: [PATCH] [doc] Update old link to hubbardI to github --- doc/guide/dftdmft_singleshot.rst | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/doc/guide/dftdmft_singleshot.rst b/doc/guide/dftdmft_singleshot.rst index 3d2e1135..07408c7a 100644 --- a/doc/guide/dftdmft_singleshot.rst +++ b/doc/guide/dftdmft_singleshot.rst @@ -33,7 +33,7 @@ The next step is to setup an impurity solver. There are different solvers available within the :ref:`TRIQS ` framework. E.g. for :ref:`SrVO3 `, we will use the hybridization expansion :ref:`CTHYB solver `. Later on, we will -see also the example of the `Hubbard-I solver `_. +see also the example of the `Hubbard-I solver `_. They all have in common, that they are called by an uniform command:: S.solve(params)