From 52b081737ced87c97209446e589731f3cdf90b79 Mon Sep 17 00:00:00 2001 From: Valentin Niess Date: Wed, 5 Jan 2022 10:13:23 +0100 Subject: [PATCH] Patch doc for v0.4 --- include/danton.h | 9 +++------ 1 file changed, 3 insertions(+), 6 deletions(-) diff --git a/include/danton.h b/include/danton.h index 0ccca7c..2ed42c5 100644 --- a/include/danton.h +++ b/include/danton.h @@ -551,20 +551,17 @@ DANTON_API int danton_error_push( * The corresponding parameter *value* can be set to `NULL`, resulting in * Danton's default value to be used. Otherwise, for tau energy losses, the * parameter value must correspond to a model available in PUMAS, see e.g. - * reference below. + * [pumas_physics_settings](https://pumas.readthedocs.io/en/latest/api/#HEAD/type/pumas_physics_settings). * * For DIS cross-sections, the supported parameter values are `"LO"` (Leading * Order computation using the PDF), `"CSMS"` (Cooper-Sarkar, Mertsch and * Sarkar) and `"BGR18"` (Bertone, Gold and Rojo). Alternatively, one can - * provide a path to a file containing cross-section values in ENT's format. + * provide a path to a file containing cross-section values in + * [ENT](https://github.com/niess/ent/tree/master/share/cs)'s format. * * For PDF sets, the built-in models are `"HERAPDF15NLO"`, `"CT14nlo"` and * `"NNPDF31sx"`. Alternatively, one can provide a path to a file containing * cross-section values in Les Houches Accord (LHA) format. - * - * References: - * ENT: https://github.com/niess/ent - * PUMAS: https://pumas.readthedocs.io/en/latest/api/#HEAD/type/pumas_physics_settings */ DANTON_API int danton_physics_set(const char * process, const char * model);