Joint Analysis Method on Gravitational Waves and Low-Energy Neutrinos to Detect Core-Collapse Supernovae

2021/10/29 by O. Halim, C. Casentini, Halim, O +10
Physics and Astronomy · #FOS: Physical sciences #Gamma-ray bursts and supernovae #General Relativity and Quantum Cosmology (gr-qc) #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Experiment (hep-ex) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Neutrino Physics Research #Pulsars and Gravitational Waves Research

paper · pdf · doi:10.48550/arxiv.2110.15620

openalex publication_date 2021/10/29 · openalex created_date 2021/11/08 · openalex updated_date 2026/08/01

Abstract

Core-collapse supernovae produce copious low-energy neutrinos and are also predicted to radiate gravitational waves. These two messengers can give us information regarding the explosion mechanism. The gravitational wave detection from these events are still elusive even with the already advanced detectors. Here we give a concise and timely introduction to a new method that combines triggers from GW and neutrino observatories; more details shall be given in a forthcoming paper [1]. Keywords: multimessenger, supernova, core-collapse, low-energy neutrino, gravitational wave.

Citations

• An Overview of the KamLAND 1-kiloton Liquid Scintillator
• Advanced Virgo: a second-generation interferometric gravitational wave detector

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