IceCube-Gen2: the window to the extreme Universe

Abstract The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a wealth of information about the Universe. However, at PeV (10 15 eV) energies and above, most of the Universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explor...

Full description

Bibliographic Details
Published in:Journal of Physics G: Nuclear and Particle Physics
Main Authors: Aartsen, M G, Abbasi, R, Ackermann, M, Adams, J, Aguilar, J A, Ahlers, M, Ahrens, M, Alispach, C, Allison, P, Amin, N M, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Arlen, T C, Auffenberg, J, Axani, S, Bagherpour, H, Bai, X, Balagopal V, A, Barbano, A, Bartos, I, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, J J, Becker, K-H, Tjus, J Becker, BenZvi, S, Berley, D, Bernardini, E, Besson, D Z, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Bohmer, M, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J
Format: Article in Journal/Newspaper
Language:unknown
Published: IOP Publishing 2021
Subjects:
Online Access:http://dx.doi.org/10.1088/1361-6471/abbd48
https://iopscience.iop.org/article/10.1088/1361-6471/abbd48
https://iopscience.iop.org/article/10.1088/1361-6471/abbd48/pdf
id crioppubl:10.1088/1361-6471/abbd48
record_format openpolar
spelling crioppubl:10.1088/1361-6471/abbd48 2024-09-30T14:43:49+00:00 IceCube-Gen2: the window to the extreme Universe Aartsen, M G Abbasi, R Ackermann, M Adams, J Aguilar, J A Ahlers, M Ahrens, M Alispach, C Allison, P Amin, N M Andeen, K Anderson, T Ansseau, I Anton, G Argüelles, C Arlen, T C Auffenberg, J Axani, S Bagherpour, H Bai, X Balagopal V, A Barbano, A Bartos, I Bastian, B Basu, V Baum, V Baur, S Bay, R Beatty, J J Becker, K-H Tjus, J Becker BenZvi, S Berley, D Bernardini, E Besson, D Z Binder, G Bindig, D Blaufuss, E Blot, S Bohm, C Bohmer, M Böser, S Botner, O Böttcher, J Bourbeau, E Bourbeau, J Bradascio, F Braun, J Bron, S Brostean-Kaiser, J 2021 http://dx.doi.org/10.1088/1361-6471/abbd48 https://iopscience.iop.org/article/10.1088/1361-6471/abbd48 https://iopscience.iop.org/article/10.1088/1361-6471/abbd48/pdf unknown IOP Publishing https://iopscience.iop.org/page/copyright https://iopscience.iop.org/info/page/text-and-data-mining Journal of Physics G: Nuclear and Particle Physics volume 48, issue 6, page 060501 ISSN 0954-3899 1361-6471 journal-article 2021 crioppubl https://doi.org/10.1088/1361-6471/abbd48 2024-09-17T04:17:59Z Abstract The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a wealth of information about the Universe. However, at PeV (10 15 eV) energies and above, most of the Universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the Universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. These energetic particles have millions of times higher energies than those produced in the most powerful particle accelerators on Earth. As neutrinos can escape from regions otherwise opaque to radiation, they allow an unique view deep into exploding stars and the vicinity of the event horizons of black holes. The discovery of cosmic neutrinos with IceCube has opened this new window on the Universe. IceCube has been successful in finding first evidence for cosmic particle acceleration in the jet of an active galactic nucleus. Yet, ultimately, its sensitivity is too limited to detect even the brightest neutrino sources with high significance, or to detect populations of less luminous sources. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the Universe at the highest energies. IceCube-Gen2 is designed to: (a) Resolve the high-energy neutrino sky from TeV to EeV energies (b) Investigate cosmic particle acceleration through multi-messenger observations (c) Reveal the sources and propagation of the highest energy particles in the Universe (d) Probe fundamental physics with high-energy neutrinos IceCube-Gen2 will enhance the existing IceCube detector at the South Pole. It will increase the annual rate of observed cosmic neutrinos by a factor of ten compared to IceCube, and will be able to detect sources five times fainter than its predecessor. Furthermore, through the addition of a radio array, IceCube-Gen2 will extend the energy range ... Article in Journal/Newspaper South pole IOP Publishing South Pole Journal of Physics G: Nuclear and Particle Physics 48 6 060501
institution Open Polar
collection IOP Publishing
op_collection_id crioppubl
language unknown
description Abstract The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a wealth of information about the Universe. However, at PeV (10 15 eV) energies and above, most of the Universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the Universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. These energetic particles have millions of times higher energies than those produced in the most powerful particle accelerators on Earth. As neutrinos can escape from regions otherwise opaque to radiation, they allow an unique view deep into exploding stars and the vicinity of the event horizons of black holes. The discovery of cosmic neutrinos with IceCube has opened this new window on the Universe. IceCube has been successful in finding first evidence for cosmic particle acceleration in the jet of an active galactic nucleus. Yet, ultimately, its sensitivity is too limited to detect even the brightest neutrino sources with high significance, or to detect populations of less luminous sources. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the Universe at the highest energies. IceCube-Gen2 is designed to: (a) Resolve the high-energy neutrino sky from TeV to EeV energies (b) Investigate cosmic particle acceleration through multi-messenger observations (c) Reveal the sources and propagation of the highest energy particles in the Universe (d) Probe fundamental physics with high-energy neutrinos IceCube-Gen2 will enhance the existing IceCube detector at the South Pole. It will increase the annual rate of observed cosmic neutrinos by a factor of ten compared to IceCube, and will be able to detect sources five times fainter than its predecessor. Furthermore, through the addition of a radio array, IceCube-Gen2 will extend the energy range ...
format Article in Journal/Newspaper
author Aartsen, M G
Abbasi, R
Ackermann, M
Adams, J
Aguilar, J A
Ahlers, M
Ahrens, M
Alispach, C
Allison, P
Amin, N M
Andeen, K
Anderson, T
Ansseau, I
Anton, G
Argüelles, C
Arlen, T C
Auffenberg, J
Axani, S
Bagherpour, H
Bai, X
Balagopal V, A
Barbano, A
Bartos, I
Bastian, B
Basu, V
Baum, V
Baur, S
Bay, R
Beatty, J J
Becker, K-H
Tjus, J Becker
BenZvi, S
Berley, D
Bernardini, E
Besson, D Z
Binder, G
Bindig, D
Blaufuss, E
Blot, S
Bohm, C
Bohmer, M
Böser, S
Botner, O
Böttcher, J
Bourbeau, E
Bourbeau, J
Bradascio, F
Braun, J
Bron, S
Brostean-Kaiser, J
spellingShingle Aartsen, M G
Abbasi, R
Ackermann, M
Adams, J
Aguilar, J A
Ahlers, M
Ahrens, M
Alispach, C
Allison, P
Amin, N M
Andeen, K
Anderson, T
Ansseau, I
Anton, G
Argüelles, C
Arlen, T C
Auffenberg, J
Axani, S
Bagherpour, H
Bai, X
Balagopal V, A
Barbano, A
Bartos, I
Bastian, B
Basu, V
Baum, V
Baur, S
Bay, R
Beatty, J J
Becker, K-H
Tjus, J Becker
BenZvi, S
Berley, D
Bernardini, E
Besson, D Z
Binder, G
Bindig, D
Blaufuss, E
Blot, S
Bohm, C
Bohmer, M
Böser, S
Botner, O
Böttcher, J
Bourbeau, E
Bourbeau, J
Bradascio, F
Braun, J
Bron, S
Brostean-Kaiser, J
IceCube-Gen2: the window to the extreme Universe
author_facet Aartsen, M G
Abbasi, R
Ackermann, M
Adams, J
Aguilar, J A
Ahlers, M
Ahrens, M
Alispach, C
Allison, P
Amin, N M
Andeen, K
Anderson, T
Ansseau, I
Anton, G
Argüelles, C
Arlen, T C
Auffenberg, J
Axani, S
Bagherpour, H
Bai, X
Balagopal V, A
Barbano, A
Bartos, I
Bastian, B
Basu, V
Baum, V
Baur, S
Bay, R
Beatty, J J
Becker, K-H
Tjus, J Becker
BenZvi, S
Berley, D
Bernardini, E
Besson, D Z
Binder, G
Bindig, D
Blaufuss, E
Blot, S
Bohm, C
Bohmer, M
Böser, S
Botner, O
Böttcher, J
Bourbeau, E
Bourbeau, J
Bradascio, F
Braun, J
Bron, S
Brostean-Kaiser, J
author_sort Aartsen, M G
title IceCube-Gen2: the window to the extreme Universe
title_short IceCube-Gen2: the window to the extreme Universe
title_full IceCube-Gen2: the window to the extreme Universe
title_fullStr IceCube-Gen2: the window to the extreme Universe
title_full_unstemmed IceCube-Gen2: the window to the extreme Universe
title_sort icecube-gen2: the window to the extreme universe
publisher IOP Publishing
publishDate 2021
url http://dx.doi.org/10.1088/1361-6471/abbd48
https://iopscience.iop.org/article/10.1088/1361-6471/abbd48
https://iopscience.iop.org/article/10.1088/1361-6471/abbd48/pdf
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source Journal of Physics G: Nuclear and Particle Physics
volume 48, issue 6, page 060501
ISSN 0954-3899 1361-6471
op_rights https://iopscience.iop.org/page/copyright
https://iopscience.iop.org/info/page/text-and-data-mining
op_doi https://doi.org/10.1088/1361-6471/abbd48
container_title Journal of Physics G: Nuclear and Particle Physics
container_volume 48
container_issue 6
container_start_page 060501
_version_ 1811645447622623232