Conference proceeding
An End-to-End Test of the Sensitivity of IceCube to the Neutrino Burst from a Core-Collapse Supernova
Pos : proceedings of science, v 395, 1085
18 Mar 2022
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 >99% uptime and is sensitive to a variety of supernova models at levels >10σ
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 as the SuperNova Early Warning System (SNEWS 2.0). A ''Fire Drill'' system was designed to inject simulated supernova signals into the IceCube online system. We will discuss IceCube’s sensitivity to supernovae near the Milky Way, and describe the data challenges used to ensure the readiness of IceCube and its operators. We will also discuss the coordination of IceCube alerts and data challenges with SNEWS 2.0.
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- Title
- An End-to-End Test of the Sensitivity of IceCube to the Neutrino Burst from a Core-Collapse Supernova
- Creators
- Spencer Griswold - University of RochesterR. Abbasi - Loyola University ChicagoM. Ackermann - DESY, Zeuthen, GermanyJ. Adams - University of CanterburyJ. A. Aguilar - Université Libre de BruxellesM. Ahlers - University of CopenhagenM. Ahrens - Stockholm UniversityC. Alispach - Département de Physique NucléaireA. A. Alves - Karlsruhe Institute of Technology, Institute for Astroparticle Physics, Karlsruhe, GermanyN. M. Amin - University of DelawareR. An - Harvard UniversityK. Andeen - Marquette UniversityT. Anderson - Pennsylvania State UniversityG. Anton - Friedrich-Alexander-Universität Erlangen-NürnbergC. Argüelles - Harvard UniversityY. Ashida - Dept. of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin–Madison, Madison, WI, United StatesS. Axani - Massachusetts Institute of TechnologyX. Bai - South Dakota School of Mines and TechnologyA. V. Balagopal - Dept. of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin–Madison, Madison, WI, United StatesA. Barbano - Département de Physique NucléaireS. W. Barwick - University of California, IrvineB. Bastian - DESY, Zeuthen, GermanyV. Basu - Dept. of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin–Madison, Madison, WI, United StatesS. Baur - Université Libre de BruxellesR. Bay - University of California, BerkeleyJ. J. Beatty - The Ohio State UniversityK. H. Becker - University of WuppertalJ. Becker Tjus - Fakultät für Physik & Astronomie, Ruhr-Universität Bochum, Bochum, GermanyC. Bellenghi - Ludwig-Maximilians-Universität MünchenS. BenZvi - University of RochesterD. Berley - University of Maryland, College ParkE. Bernardini - Università di Padova, Padova, ItalyD. Z. Besson - National Research Nuclear University, Moscow Engineering Physics Institute (MEPhI), Moscow, Russian FederationG. Binder - Lawrence Berkeley National LaboratoryD. Bindig - University of WuppertalE. Blaufuss - University of Maryland, College ParkS. Blot - DESY, Zeuthen, GermanyM. Boddenberg - RWTH Aachen UniversityF. Bontempo - Karlsruhe Institute of Technology, Institute for Astroparticle Physics, Karlsruhe, GermanyJ. Borowka - RWTH Aachen UniversityS. Böser - Institute of Physics, University of Mainz, Mainz, GermanyO. Botner - Uppsala UniversityJ. Böttcher - RWTH Aachen UniversityE. Bourbeau - University of CopenhagenF. Bradascio - DESY, Zeuthen, GermanyJ. Braun - Dept. of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin–Madison, Madison, WI, United StatesS. Bron - Département de Physique NucléaireJ. Brostean-Kaiser - DESY, Zeuthen, GermanyS. Browne - Karlsruhe Institute of Technology, Institute of Experimental Particle Physics, Karlsruhe, GermanyA. Burgman - Uppsala UniversityR. T. Burley - Department of Physics, University of Adelaide, Adelaide, AustraliaR. S. Busse - University of MünsterM. A. Campana - Dept. of Physics, Drexel University, Philadelphia, PA, United StatesE. G. Carnie-Bronca - The University of AdelaideC. Chen - Georgia Institute of TechnologyD. Chirkin - Dept. of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin–Madison, Madison, WI, United StatesK. Choi - Sungkyunkwan UniversityB. A. Clark - Michigan State UniversityK. Clark - Queen's UniversityL. Classen - University of MünsterA. Coleman - University of DelawareG. H. Collin - Massachusetts Institute of TechnologyJ. M. Conrad - Massachusetts Institute of TechnologyP. Coppin - Vrije Universiteit BrusselP. Correa - Vrije Universiteit BrusselD. F. Cowen - Pennsylvania State UniversityR. Cross - University of RochesterC. Dappen - RWTH Aachen UniversityP. Dave - Georgia Institute of TechnologyC. De Clercq - Vrije Universiteit BrusselJ. J. DeLaunay - Pennsylvania State UniversityH. Dembinski - University of DelawareK. Deoskar - Stockholm UniversityS. De Ridder - Dept. of Physics and Astronomy, University of Gent, Gent, BelgiumA. Desai - Dept. of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin–Madison, Madison, WI, United StatesP. Desiati - Dept. of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin–Madison, Madison, WI, United StatesK. D. de Vries - Vrije Universiteit BrusselG. de Wasseige - Vrije Universiteit BrusselM. de With - Humboldt-Universität zu BerlinT. DeYoung - Michigan State UniversityS. Dharani - RWTH Aachen UniversityA. Diaz - Massachusetts Institute of TechnologyJ. C. Díaz-Vélez - University of Wisconsin–MadisonM. Dittmer - University of MünsterH. Dujmovic - Karlsruhe Institute of Technology, Institute for Astroparticle Physics, Karlsruhe, GermanyM. Dunkman - Pennsylvania State UniversityM. A. DuVernois - University of Wisconsin–MadisonE. Dvorak - South Dakota School of Mines and TechnologyT. Ehrhardt - Institute of Physics, University of Mainz, Mainz, GermanyP. Eller - Ludwig-Maximilians-Universität MünchenR. Engel - Karlsruhe Institute of Technology, Institute of Experimental Particle Physics, Karlsruhe, GermanyH. Erpenbeck - RWTH Aachen UniversityJ. Evans - University of Maryland, College ParkP. A. Evenson - University of DelawareK. L. Fan - University of Maryland, College ParkA. R. Fazely - Dept. of Physics, Southern University, Baton Rouge, LA, United StatesS. Fiedlschuster - Friedrich-Alexander-Universität Erlangen-NürnbergA. T. Fienberg - Pennsylvania State UniversityK. Filimonov - University of California, BerkeleyC. Finley - Stockholm University
- Publication Details
- Pos : proceedings of science, v 395, 1085
- Publisher
- SISSA Medialab
- Grant note
- Michigan State University (http://data.elsevier.com/vocabulary/SciValFunders/100007709) Helmholtz Association (http://data.elsevier.com/vocabulary/SciValFunders/501100009318) Fonds Wetenschappelijk Onderzoek (http://data.elsevier.com/vocabulary/SciValFunders/501100003130) Marsden Fund (http://data.elsevier.com/vocabulary/SciValFunders/501100009193) Bundesministerium für Bildung und Forschung (http://data.elsevier.com/vocabulary/SciValFunders/501100002347) U.S. National Science Foundation-Physics Division Knut och Alice Wallenbergs Stiftelse (http://data.elsevier.com/vocabulary/SciValFunders/501100004063) Extreme Science and Engineering Discovery Environment Natural Sciences and Engineering Research Council of Canada (http://data.elsevier.com/vocabulary/SciValFunders/501100000038) Villum Fonden and Carlsberg Foundation
- Resource Type
- Conference proceeding
- Language
- English
- Academic Unit
- Physics
- Scopus ID
- 2-s2.0-85145020299
- Other Identifier
- 991022237859304721