Characterizing a supernova's Standing Accretion Shock Instability with neutrinos and gravitational waves
Zidu Lin, Abhinav Rijal, Cecilia Lunardini, Manuel D. Morales and, Michele Zanolin

TL;DR
This paper introduces a multi-messenger analysis method combining neutrino and gravitational wave data to detect and characterize the Standing Accretion Shock Instability in supernovae, improving detection probability over single-channel approaches.
Contribution
It develops a novel joint analysis framework for SASI detection using neutrino and GW signals, enhancing detection confidence and parameter estimation accuracy.
Findings
Joint analysis increases detection probability by up to 40% at 5 kpc.
Method effectively estimates SASI frequency and duration.
Approach is suitable for real data and multi-messenger applications.
Abstract
We perform a novel multi-messenger analysis for the identification and parameter estimation of the Standing Accretion Shock Instability (SASI) in a core collapse supernova with neutrino and gravitational wave (GW) signals. In the neutrino channel, this method performs a likelihood ratio test for the presence of SASI in the frequency domain. For gravitational wave signals we process an event with a modified constrained likelihood method. Using simulated supernova signals, the properties of the Hyper-Kamiokande neutrino detector, and O3 LIGO Interferometric data, we produce the two-dimensional probability density function (PDF) of the SASI activity indicator and calculate the probability of detection as well as the false identification probability . We discuss the probability to establish the presence of the SASI as a function of the source distance in each…
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
