SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals
Amanda L. Baxter, Segev BenZvi, Joahan Castaneda Jaimes, Alexis, Coleiro, Marta Colomer Molla, Damien Dornic, Tomer Goldhagen, Anne M. Graf,, Spencer Griswold, Alec Habig, Remington Hill, Shunsaku Horiuchi James P., Kneller Rafael F. Lang, Massimiliano Lincetto, Jost Migenda

TL;DR
SNEWPY is an open-source software that connects supernova simulation data to neutrino detector signals, enabling better comparison between theoretical models and observations for various types of supernovae.
Contribution
It introduces a comprehensive, open-source pipeline that converts supernova simulation outputs into neutrino signals for detectors, bridging a critical gap in supernova neutrino research.
Findings
Includes data from hundreds of supernova simulations
Automates data processing for neutrino signal prediction
Facilitates comparison between models and observations
Abstract
Current neutrino detectors will observe hundreds to thousands of neutrinos from a 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 which 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,…
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae
