From 7884acfafeb4e2ec0a920a66159b3c56849669ec Mon Sep 17 00:00:00 2001 From: nkavokine Date: Fri, 29 Nov 2024 07:53:39 -0500 Subject: [PATCH] [paper] fix reference formatting --- paper/paper.md | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/paper/paper.md b/paper/paper.md index 9f4002c..5383755 100644 --- a/paper/paper.md +++ b/paper/paper.md @@ -62,8 +62,8 @@ Currently, there exist implementations of `CTHYB` within three different librari However, a simpler and potentially faster version of the `CTHYB` algorithm, called `CTSEG`, can be used under the restriction of density-density -interactions on the impurity[@werner2006a,@werner2006b,@haule2007]. `CTSEG` can be further generalized to allow for time-dependent[@werner2007,@werner2010] and -spin-spin interactions [@otsuki2013,@steiner2015]: see [@werner2016] for a review. To our knowledge, there exists so far one published implementation of `CTSEG` based on ALPS [@ALPS-CTSEG], but it does not allow for spin-spin interactions. +interactions on the impurity [@werner2006a;@werner2006b;@haule2007]. `CTSEG` can be further generalized to allow for time-dependent[@werner2007;@werner2010] and +spin-spin interactions [@otsuki2013;@steiner2015]: see `@werner2016` for a review. To our knowledge, there exists so far one published implementation of `CTSEG` based on ALPS [@ALPS-CTSEG], but it does not allow for spin-spin interactions. Our `CTSEG` solver is about twice as fast as `TRIQS-CTHYB` for a single orbital problem, and has better scaling with the number of orbitals (40 times faster in our 5 orbital test case, see Fig. 1a).