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IceCube search for neutrinos from GRB 221009A
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2023 (English)In: Proceedings of 38th International Cosmic Ray Conference (ICRC 2023), Sissa Medialab Srl , 2023, article id 1511Conference paper, Published paper (Refereed)
Abstract [en]

 GRB 221009A is the brightest Gamma Ray Burst (GRB) ever observed. The observed extremelyhigh flux of high and very-high-energy photons provide a unique opportunity to probe the predictedneutrino counterpart to the electromagnetic emission. We have used a variety of methods to searchfor neutrinos in coincidence with the GRB over several time windows during the precursor, promptand afterglow phases of the GRB. MeV scale neutrinos are studied using photo-multiplier ratescalers which are normally used to search for galactic core-collapse supernovae neutrinos. GeVneutrinos are searched starting with DeepCore triggers. These events don’t have directionallocalization, but instead can indicate an excess in the rate of events. 10 GeV - 1 TeV and >TeVneutrinos are searched using traditional neutrino point source methods which take into accountthe direction and time of events with DeepCore and the entire IceCube detector respectively. The>TeV results include both a fast-response analysis conducted by IceCube in real-time with timewindows of T0 − 1 to T0 + 2 hours and T0 ± 1 day around the time of GRB 221009A, as well asan offline analysis with 3 new time windows up to a time window of T0 − 1 to T0 + 14 days, thelongest time period we consider. The combination of observations by IceCube covers 9 ordersof magnitude in neutrino energy, from MeV to PeV, placing upper limits across the range forpredicted neutrino emission.

Place, publisher, year, edition, pages
Sissa Medialab Srl , 2023. article id 1511
Series
PoS proceedings of science, E-ISSN 1824-8039 ; 444
Keywords [en]
Neutrinos, gamma-ray burst
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Physics
Identifiers
URN: urn:nbn:se:uu:diva-535302DOI: 10.22323/1.444.1511OAI: oai:DiVA.org:uu-535302DiVA, id: diva2:1885473
Conference
The 38th International Cosmic Ray Conference, Nagoya, Japan, 26 July- 3 August, 2023
Available from: 2024-07-23 Created: 2024-07-23 Last updated: 2024-08-01Bibliographically approved
In thesis
1. Searching for IceCube Neutrinos from the Death of Stars and Beyond: From MeV to PeV Energies
Open this publication in new window or tab >>Searching for IceCube Neutrinos from the Death of Stars and Beyond: From MeV to PeV Energies
2024 (English)Doctoral thesis, comprehensive summary (Other academic)
Abstract [en]

The stellar death and its aftermath are compelling systems to study due to their extreme conditions and a rich array of observable messengers, such as photons, gravitational waves, and neutrinos. Neutrinos, as messengers of these systems, are particularly interesting due to their ability to traverse space unimpeded by interstellar debris, magnetic fields, or photons, thus preserving important information about the source, with different sites of production that influence the neutrino energy from nuclear processes in very dense and hot environments producing thermal MeV energy neutrinos to cosmic acceleration sites, where matter collides in shocks, producing high energy neutrinos in the O(>GeV-TeV). These neutrinos can be observed by neutrino telescopes such as the IceCube Neutrino Observatory, which has sensitivity for neutrinos from the MeV to >PeV energy ranges. In this thesis, we performed several searches, focusing on MeV neutrinos from Gamma Ray Bursts and Neutron Star Mergers, making use of information from other messengers such as photons and gravitational waves to inform our search, and >GeV neutrinos from Core-Collapse Supernovae. We produced MeV neutrino flux limits for GRB 221009A and provided detection horizon limits for >GeV neutrinos from Core-Collapse Supernovae. We also introduced a novel methodology for producing model-independent MeV neutrino flux and luminosity limits, developed a new IceCube MeV energy real-time fast analysis for the follow-up of external alerts from other observatories, and demonstrated how to search for MeV neutrinos correlated with gravitational waves.

Place, publisher, year, edition, pages
Uppsala: Acta Universitatis Upsaliensis, 2024. p. 121
Series
Digital Comprehensive Summaries of Uppsala Dissertations from the Faculty of Science and Technology, ISSN 1651-6214 ; 2426
Keywords
Neutrinos, Gravitational Waves, Neutron Star Mergers, Core-Collapse Supernova, Supernovae, High-Energy Neutrinos, Low-Energy Neutrinos, Astrophysical Neutrinos
National Category
Astronomy, Astrophysics and Cosmology Subatomic Physics
Research subject
Physics
Identifiers
urn:nbn:se:uu:diva-535303 (URN)978-91-513-2185-1 (ISBN)
Public defence
2024-09-19, Häggsalen, Ångströmlaboratoriet, Lägerhyddsvägen 1, Uppsala, 13:15 (English)
Opponent
Supervisors
Available from: 2024-08-27 Created: 2024-08-01 Last updated: 2024-08-27

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Beise, JakobBotner, OlgaColeman, AlanGlaser, ChristianGlüsenkamp, ThorstenHallgren, AllanHeyer, NilsO'Sullivan, ErinPérez de los Heros, CarlosPontén, AxelSharma, AnkurValtonen-Mattila, Nora

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Beise, JakobBotner, OlgaColeman, AlanGlaser, ChristianGlüsenkamp, ThorstenHallgren, AllanHeyer, NilsO'Sullivan, ErinPérez de los Heros, CarlosPontén, AxelSharma, AnkurValtonen-Mattila, Nora
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