@@ -1150,3 +1150,38 @@ @ARTICLE{amrex-ecp
11501150 adsnote = { Provided by the SAO/NASA Astrophysics Data System}
11511151}
11521152
1153+
1154+ @article {brady:2025 ,
1155+ doi = { 10.3847/2515-5172/add686} ,
1156+ url = { https://doi.org/10.3847/2515-5172/add686} ,
1157+ year = { 2025} ,
1158+ month = { may} ,
1159+ publisher = { The American Astronomical Society} ,
1160+ volume = { 9} ,
1161+ number = { 5} ,
1162+ pages = { 113} ,
1163+ author = { Brady, Ryan and Zingale, Michael} ,
1164+ title = { Numerical Treatment of Shock-induced Nuclear Burning in Double Detonation Type Ia Supernovae} ,
1165+ journal = { Research Notes of the AAS} ,
1166+ abstract = { We present a benchmark problem to assess the treatment of
1167+ shock-induced nuclear burning in the context of
1168+ double detonation Type Ia supernovae. In a
1169+ stratified white dwarf model, we implement a
1170+ shock-detection criterion that suppresses burning in
1171+ zones characterized by compression and significant
1172+ pressure gradients, controlled by a tunable
1173+ parameter, fshock. One-dimensional simulations,
1174+ using the open-source Castro suite, were conducted
1175+ across three treatments—burning fully enabled, and
1176+ burning suppressed with fshock = 2/3 and
1177+ fshock = 1—across three spatial resolutions (5.0,
1178+ 2.5, and 0.3125 km). At the finest resolution, the
1179+ burning-enabled and fshock = 1 models converge,
1180+ while the fshock = 2/3 front continues to show
1181+ slight offset behavior. Since most simulations are
1182+ carried out at much lower resolutions, our tests
1183+ support the idea that burning in shocks should
1184+ always be disabled in practice. We also observe that
1185+ the behavior of lower-resolution simulations remains
1186+ extremely sensitive to the choice of fshock.}
1187+ }
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