Neutrino signatures of 100 2D Axisymmetric Core-Collapse Supernova Simulations

David Vartanyan, Adam Burrows

Research output: Contribution to journalArticlepeer-review

8 Scopus citations


We present in this paper a public data release of an unprecedentedly large set of core-collapse supernova (CCSN) neutrino emission models, comprising 100 detailed 2D axisymmetric radiation-hydrodynamic simulations evolved out to as late as ∼5 s post-bounce and spanning an extensive range of massive-star progenitors. The motivation for this paper is to provide a physically and numerically uniform benchmark data set to the broader neutrino detection community to help it characterize and optimize subsurface facilities for what is likely to be a once-in-a-lifetime galactic supernova burst event. With this release, we hope to (1) help the international experiment and modelling communities more efficiently optimize the retrieval of physical information about the next galactic CCSN, (2) facilitate the better understanding of core-collapse theory and modelling among interested experimentalists, and (3) help further integrate the broader supernova neutrino community.

Original languageEnglish (US)
Pages (from-to)5900-5910
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Issue number4
StatePublished - Dec 1 2023

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


  • neutrinos
  • supernovae: general


Dive into the research topics of 'Neutrino signatures of 100 2D Axisymmetric Core-Collapse Supernova Simulations'. Together they form a unique fingerprint.

Cite this