Open AccessSNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals
Author(s) -
A. Baxter,
S. BenZvi,
Joahan Castaneda Jaimes,
A. Coleiro,
M. Colomer-Molla,
D. Dornic,
Tomer Goldhagen,
Anne Graf,
Spencer Griswold,
A. Habig,
R. Hill,
Shunsaku Horiuchi,
James P. Kneller,
R. F. Lang,
Massimiliano Lincetto,
J. Migenda,
Ko Nakamura,
Evan O’Connor,
A. Renshaw,
K. Scholberg,
C. Tunnell,
Navya Uberoi,
Arkin Worlikar
Publication year - 2022
Publication title -
astrophysical journal/the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.3847/1538-4357/ac350f
Subject(s) - physics , neutrino , supernova , neutrino detector , astrophysics , event (particle physics) , detector , astronomy , neutrino oscillation , nuclear physics , optics
Current neutrino detectors will observe hundreds to thousands of neutrinos from Galactic supernovae, and future detectors will increase this yield by an order of magnitude or more. With such a data set comes the potential for a huge increase in our understanding of the explosions of massive stars, nuclear physics under extreme conditions, and the properties of the neutrino. However, there is currently a large gap between supernova simulations and the corresponding signals in neutrino detectors, which will make any comparison between theory and observation very difficult. SNEWPY is an open-source software package that bridges this gap. The SNEWPY code can interface with supernova simulation data to generate from the model either a time series of neutrino spectral fluences at Earth, or the total time-integrated spectral fluence. Data from several hundred simulations of core-collapse, thermonuclear, and pair-instability supernovae is included in the package. This output may then be used by an event generator such as sntools or an event rate calculator such as the SuperNova Observatories with General Long Baseline Experiment Simulator (SNOwGLoBES). Additional routines in the SNEWPY package automate the processing of the generated data through the SNOwGLoBES software and collate its output into the observable channels of each detector. In this paper we describe the contents of the package, the physics behind SNEWPY, the organization of the code, and provide examples of how to make use of its capabilities.