From f453433e58332b459b8c40675864e430b6028ee3 Mon Sep 17 00:00:00 2001 From: Michael Zingale Date: Thu, 5 Dec 2024 11:34:01 -0500 Subject: [PATCH] fix refs --- sphinx_docs/source/refs.bib | 1 - 1 file changed, 1 deletion(-) diff --git a/sphinx_docs/source/refs.bib b/sphinx_docs/source/refs.bib index 3e871c8c0..d0f234fbc 100644 --- a/sphinx_docs/source/refs.bib +++ b/sphinx_docs/source/refs.bib @@ -669,7 +669,6 @@ @article{langanke:2001 year = {2001}, issn = {0092-640X}, doi = {https://doi.org/10.1006/adnd.2001.0865}, -url = {https://www.sciencedirect.com/science/article/pii/S0092640X01908654}, author = {K. LANGANKE and G. MARTÍNEZ-PINEDO}, abstract = {The weak interaction rates in stellar environments are computed for pf-shell nuclei in the mass range A=45–65 using large-scale shell-model calculations. The calculated capture and decay rates take into consideration the latest experimental energy levels and log ft-values. The rates are tabulated at the same grid points of density and temperature as those used by Fuller, Fowler, and Newman for densities ρY e =10–1011 g/cm3 and temperatures T=107–1011 K, and hence are relevant for both types of supernovae (Type Ia and Type II). Effective 〈ft〉 values for capture rates and average neutrino (antineutrino) energies are also given to facilitate the use of interpolated rates in stellar evolution codes.} } \ No newline at end of file