Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube
Dwaipayan Mukherjee, Mohamed Rameez, Basudeb Dasgupta
Tata Inst. · Tata Inst. · Tata Inst.
astro-ph.SR, astro-ph.HE, hep-ex, hep-ph
Submitted: 2026-06-29
Comments: 15 pages, 8 figures, 1 table
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
- On the rate of core collapse supernovae in the Milky Way
- Supernova Simulations Confront SN 1987A Neutrinos
- Old Data, New Forensics: The First Second of SN 1987A Neutrino Emission
- IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae
- The IceCube Neutrino Observatory: Instrumentation and Online Systems
- Search for Galactic core-collapse supernovae in a decade of data taken with the IceCube Neutrino Observatory
- The KM3NeT potential for the next core-collapse supernova observation with neutrinos
- IceCube-Gen2: The Window to the Extreme Universe
- Supernova Model Discrimination with Hyper-Kamiokande
- Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume I: Introduction to DUNE
- Supernova Pointing Capabilities of DUNE
- Observing the Next Galactic Supernova
- Exciting Prospects for Detecting Late-Time Neutrinos from Core-Collapse Supernovae
- Supernova Neutrinos: Production, Oscillations and Detection
- Neutrino Emission from Supernovae
- How much can we learn from SN1987A events? Or: An analysis with a two-Component model for the antineutrino signal
- Neutrinos from core-collapse supernovae
- Fornax: a Flexible Code for Multiphysics Astrophysical Simulations
- Chimera: A massively parallel code for core-collapse supernova simulation
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