stardis-solver

commit c2a6440996030409417f1fa680b299faa3ca951e
parent c28451b7b47ccf4dd9e75ca65dc64543fd152a8b
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Fri, 20 Nov 2020 11:33:33 +0100

Add a link toward the Eymet et al. 2020 article

Diffstat:
M
README.md
 | 
3
++-

1 file changed, 2 insertions(+), 1 deletion(-)
diff --git a/README.md b/README.md
@@ -6,7 +6,8 @@ library internally relies on *Monte-Carlo* algorithms based on reformulations
 of the main heat transfer phenomena as cross-recursive "thermal paths" that
 explore space and time until a boundary condition or an initial condition is
 found. The key concept here is that heat transfer phenomena are not considered
-separately but naturally coupled via cross-recursive Monte-Carlo algorithms.
+separately but naturally coupled via cross-recursive [Monte-Carlo
+algorithms](https://hal.archives-ouvertes.fr/hal-02419604/).
 
 The hypothesis these algorithms are based upon are the following: