par Baxter, Amanda A.L.;Benzvi, Segev;Jaimes, Joahan Castaneda;Coleiro, Alexis;Colomer Molla, Marta 
;Dornic, Damien;Griswold, Spencer;Goldhagen, Tomer;Graf, Anne;Habig, Alec;Hill, Remington;Horiuchi, Shunsaku;Kneller, James J.P.;Lamoureux, Mathieu;Lang, Rafael R.F.;Lincetto, Massimiliano;Migenda, Jost;Myers, McKenzie;O'Connor, Evan;Renshaw, Andrew;Scholberg, Kate;Sheshukov, Andrey;Tseng, Jeff;Tunnell, Christopher;Uberoi, Navya;Worlikar, Arkin
Référence Journal of Open Source Software, 6, 67, page (3772)
Publication Publié, 2021-11
;Dornic, Damien;Griswold, Spencer;Goldhagen, Tomer;Graf, Anne;Habig, Alec;Hill, Remington;Horiuchi, Shunsaku;Kneller, James J.P.;Lamoureux, Mathieu;Lang, Rafael R.F.;Lincetto, Massimiliano;Migenda, Jost;Myers, McKenzie;O'Connor, Evan;Renshaw, Andrew;Scholberg, Kate;Sheshukov, Andrey;Tseng, Jeff;Tunnell, Christopher;Uberoi, Navya;Worlikar, ArkinRéférence Journal of Open Source Software, 6, 67, page (3772)
Publication Publié, 2021-11
Article révisé par les pairs
| Résumé : | Current neutrino detectors will observe hundreds to thousands of neutrinos from a Galactic supernova, and future detectors will increase this yield by an order of magnitude or more. With such neutrino data sets, the next Galactic supernova will significantly increase our un- derstanding of the explosions of massive stars, nuclear physics under extreme conditions, and the fundamental properties of neutrinos. However, there is a gulf between supernova simu- lations and the corresponding signals in detectors, making comparisons between theory and observation, as well as between different detectors, very difficult. SNEWPY offers a unified interface for hundreds of supernova simulations, a large library of flux transformations on the way towards the detector, and an interface to SNOwGLoBES (Scholberg & SNOwGLoBES Contributors, 2021), allowing users to easily calculate and compare expected event rates from many supernova models in many different neutrino detectors. |
