End-to-End Tests of the Sensitivity of IceCube to the Neutrino Burst from a Core-Collapse Supernova
Spencer Griswold (for the IceCube Collaboration)

TL;DR
This paper evaluates IceCube's ability to detect neutrino bursts from galactic supernovae, emphasizing its high sensitivity, real-time alert capabilities, and role in the SuperNova Early Warning System.
Contribution
It presents an end-to-end testing framework for IceCube's supernova neutrino detection sensitivity and alert readiness, including simulated signal injections and coordination with SNEWS 2.0.
Findings
IceCube can detect supernova neutrino bursts within the Milky Way with >10σ significance.
The system demonstrates >99% uptime and prompt alert issuance.
Coordination with SNEWS 2.0 enhances early warning capabilities.
Abstract
The next galactic supernova presents a once-in-a-lifetime opportunity to obtain detailed information about the explosion of a star and the extreme conditions found within its core. A core-collapse supernova will produce a neutrino burst visible up to half a day before the electromagnetic radiation from the explosion, so the burst will provide an early warning for optical follow-up. Since local supernovae are exceedingly rare, it is critical that neutrino detectors provide prompt alerts after the arrival of a burst. The IceCube Neutrino Observatory operates with uptime and is sensitive to a variety of supernova models at levels within the Milky Way. IceCube will issue supernova alerts in real time. IceCube's high sensitivity to supernovae, near perfect uptime, and ability to issue prompt alerts makes it a critical component of the worldwide network of detectors known…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Gamma-ray bursts and supernovae
