Matches in SemOpenAlex for { <https://semopenalex.org/work/W2808391388> ?p ?o ?g. }
- W2808391388 endingPage "104001" @default.
- W2808391388 startingPage "104001" @default.
- W2808391388 abstract "We present a comparison between several simulation codes designed to study the core-collapse supernova mechanism. We pay close attention to controlling the initial conditions and input physics in order to ensure a meaningful and informative comparison. Our goal is three-fold. First, we aim to demonstrate the current level of agreement between various groups studying the core-collapse supernova central engine. Second, we desire to form a strong basis for future simulation codes and methods to compare to. Lastly, we want this work to be a stepping stone for future work exploring more complex simulations of core-collapse supernovae, i.e., simulations in multiple dimensions and simulations with modern neutrino and nuclear physics. We compare the early (first ∼500 ms after core bounce) spherically-symmetric evolution of a 20 M⊙ progenitor star from six different core-collapse supernovae codes: 3DnSNe-IDSA, AGILE-BOLTZTRAN, FLASH, Fornax, GR1D, and PROMETHEUS-VERTEX. Given the diversity of neutrino transport and hydrodynamic methods employed, we find excellent agreement in many critical quantities, including the shock radius evolution and the amount of neutrino heating. Our results provide an excellent starting point from which to extend this comparison to higher dimensions and compare the development of hydrodynamic instabilities that are crucial to the supernova explosion mechanism, such as turbulence and convection." @default.
- W2808391388 created "2018-06-21" @default.
- W2808391388 creator A5003341938 @default.
- W2808391388 creator A5004575978 @default.
- W2808391388 creator A5008924957 @default.
- W2808391388 creator A5009527898 @default.
- W2808391388 creator A5011943627 @default.
- W2808391388 creator A5013266043 @default.
- W2808391388 creator A5027691460 @default.
- W2808391388 creator A5046630029 @default.
- W2808391388 creator A5055083096 @default.
- W2808391388 creator A5071454109 @default.
- W2808391388 creator A5073041667 @default.
- W2808391388 creator A5083648204 @default.
- W2808391388 creator A5091297081 @default.
- W2808391388 date "2018-09-14" @default.
- W2808391388 modified "2023-10-17" @default.
- W2808391388 title "Global comparison of core-collapse supernova simulations in spherical symmetry" @default.
- W2808391388 cites W1558338643 @default.
- W2808391388 cites W1823435599 @default.
- W2808391388 cites W1963527047 @default.
- W2808391388 cites W1965823636 @default.
- W2808391388 cites W1969760987 @default.
- W2808391388 cites W1972647751 @default.
- W2808391388 cites W1977449847 @default.
- W2808391388 cites W1978574709 @default.
- W2808391388 cites W1985996701 @default.
- W2808391388 cites W1997458345 @default.
- W2808391388 cites W1999620225 @default.
- W2808391388 cites W1999973957 @default.
- W2808391388 cites W2002989381 @default.
- W2808391388 cites W2003261636 @default.
- W2808391388 cites W2009497596 @default.
- W2808391388 cites W2011160154 @default.
- W2808391388 cites W2012387554 @default.
- W2808391388 cites W2012690553 @default.
- W2808391388 cites W2022896701 @default.
- W2808391388 cites W2023706338 @default.
- W2808391388 cites W2030167880 @default.
- W2808391388 cites W2032583746 @default.
- W2808391388 cites W2034555193 @default.
- W2808391388 cites W2034689551 @default.
- W2808391388 cites W2037450980 @default.
- W2808391388 cites W2037670418 @default.
- W2808391388 cites W2047047228 @default.
- W2808391388 cites W2060043292 @default.
- W2808391388 cites W2067172078 @default.
- W2808391388 cites W2071649523 @default.
- W2808391388 cites W2071725611 @default.
- W2808391388 cites W2073325059 @default.
- W2808391388 cites W2073945818 @default.
- W2808391388 cites W2086727759 @default.
- W2808391388 cites W2088079156 @default.
- W2808391388 cites W2093021464 @default.
- W2808391388 cites W2095327327 @default.
- W2808391388 cites W2109423684 @default.
- W2808391388 cites W2118275409 @default.
- W2808391388 cites W2123867568 @default.
- W2808391388 cites W2157214767 @default.
- W2808391388 cites W2161676506 @default.
- W2808391388 cites W2164893955 @default.
- W2808391388 cites W2174816156 @default.
- W2808391388 cites W2182987072 @default.
- W2808391388 cites W2255808692 @default.
- W2808391388 cites W2402693565 @default.
- W2808391388 cites W2488438158 @default.
- W2808391388 cites W2617573275 @default.
- W2808391388 cites W2763055876 @default.
- W2808391388 cites W2784694498 @default.
- W2808391388 cites W2995130828 @default.
- W2808391388 cites W3099399323 @default.
- W2808391388 cites W3099454656 @default.
- W2808391388 cites W3099570781 @default.
- W2808391388 cites W3100803178 @default.
- W2808391388 cites W3100844239 @default.
- W2808391388 cites W3101387273 @default.
- W2808391388 cites W3101573434 @default.
- W2808391388 cites W3101806906 @default.
- W2808391388 cites W3103226401 @default.
- W2808391388 cites W3105150775 @default.
- W2808391388 cites W3105269996 @default.
- W2808391388 cites W3105565441 @default.
- W2808391388 cites W3105628247 @default.
- W2808391388 cites W3106117519 @default.
- W2808391388 cites W3106134081 @default.
- W2808391388 cites W4295664431 @default.
- W2808391388 cites W644751317 @default.
- W2808391388 doi "https://doi.org/10.1088/1361-6471/aadeae" @default.
- W2808391388 hasPublicationYear "2018" @default.
- W2808391388 type Work @default.
- W2808391388 sameAs 2808391388 @default.
- W2808391388 citedByCount "97" @default.
- W2808391388 countsByYear W28083913882018 @default.
- W2808391388 countsByYear W28083913882019 @default.
- W2808391388 countsByYear W28083913882020 @default.
- W2808391388 countsByYear W28083913882021 @default.
- W2808391388 countsByYear W28083913882022 @default.
- W2808391388 countsByYear W28083913882023 @default.