Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G
International audience Binary neutron star (BNS) mergers can be sources of ultrahigh-energy (UHE) cosmic rays and potential emitters of UHE neutrinos. The upcoming and current radio neutrino detectors like the Giant Radio Array for Neutrino Detection (GRAND), IceCube-Gen2 Radio, and the Radio Neutri...
Main Authors: | , , , , |
---|---|
Other Authors: | , |
Format: | Report |
Language: | English |
Published: |
HAL CCSD
2024
|
Subjects: | |
Online Access: | https://hal.science/hal-04650457 |
id |
ftinsu:oai:HAL:hal-04650457v1 |
---|---|
record_format |
openpolar |
spelling |
ftinsu:oai:HAL:hal-04650457v1 2024-09-09T19:43:30+00:00 Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G Mukhopadhyay, Mainak Kotera, Kumiko Wissel, Stephanie Murase, Kohta Kimura, Shigeo S Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) 2024-07-16 https://hal.science/hal-04650457 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2406.19440 hal-04650457 https://hal.science/hal-04650457 ARXIV: 2406.19440 INSPIRE: 2803112 https://hal.science/hal-04650457 2024 neutrino detector UHE network neutron star binary gravitational radiation detector multimessenger observatory burst stacking gravitational radiation sensitivity trigger Einstein Telescope cosmic radiation [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] info:eu-repo/semantics/preprint Preprints, Working Papers, . 2024 ftinsu 2024-07-24T23:44:29Z International audience Binary neutron star (BNS) mergers can be sources of ultrahigh-energy (UHE) cosmic rays and potential emitters of UHE neutrinos. The upcoming and current radio neutrino detectors like the Giant Radio Array for Neutrino Detection (GRAND), IceCube-Gen2 Radio, and the Radio Neutrino Observatory in Greenland (RNO-G) are projected to reach the required sensitivities to search for these neutrinos. In particular, in conjunction with the next-generation of gravitational wave (GW) detectors like Cosmic Explorer (CE) and Einstein Telescope (ET), GW-triggered stacking searches can be performed with the UHE neutrino detectors. In this work, we explore the prospects of such searches by implementing in our analysis an upper distance limit based on the sky-localization capabilities of the GW detectors from which meaningful triggers can be collected. We find that if each GW burst is associated with a total isotropic-equivalent energy of $\sim 10^{50} - 10^{51}$ erg emitted in UHE neutrinos, along with a corresponding beaming fraction of $1$%, GRAND and IceCube-Gen2 Radio have a large probability ($\sim 99$%) to detect a coincident neutrino event using the joint combination of CE+ET in a timescale of less than 15 years of operation for our fiducial choice of parameters. In case of nondetections, the parameter spaces can be constrained at $3\sigma$ level in similar timescales of operation. We also highlight and discuss the prospects of such joint radio neutrino detector network, their importance, and their role in facilitating synergic GW and neutrino observations in the next era of multimessenger astrophysics. Report Greenland Institut national des sciences de l'Univers: HAL-INSU Greenland |
institution |
Open Polar |
collection |
Institut national des sciences de l'Univers: HAL-INSU |
op_collection_id |
ftinsu |
language |
English |
topic |
neutrino detector UHE network neutron star binary gravitational radiation detector multimessenger observatory burst stacking gravitational radiation sensitivity trigger Einstein Telescope cosmic radiation [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] |
spellingShingle |
neutrino detector UHE network neutron star binary gravitational radiation detector multimessenger observatory burst stacking gravitational radiation sensitivity trigger Einstein Telescope cosmic radiation [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] Mukhopadhyay, Mainak Kotera, Kumiko Wissel, Stephanie Murase, Kohta Kimura, Shigeo S Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G |
topic_facet |
neutrino detector UHE network neutron star binary gravitational radiation detector multimessenger observatory burst stacking gravitational radiation sensitivity trigger Einstein Telescope cosmic radiation [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] |
description |
International audience Binary neutron star (BNS) mergers can be sources of ultrahigh-energy (UHE) cosmic rays and potential emitters of UHE neutrinos. The upcoming and current radio neutrino detectors like the Giant Radio Array for Neutrino Detection (GRAND), IceCube-Gen2 Radio, and the Radio Neutrino Observatory in Greenland (RNO-G) are projected to reach the required sensitivities to search for these neutrinos. In particular, in conjunction with the next-generation of gravitational wave (GW) detectors like Cosmic Explorer (CE) and Einstein Telescope (ET), GW-triggered stacking searches can be performed with the UHE neutrino detectors. In this work, we explore the prospects of such searches by implementing in our analysis an upper distance limit based on the sky-localization capabilities of the GW detectors from which meaningful triggers can be collected. We find that if each GW burst is associated with a total isotropic-equivalent energy of $\sim 10^{50} - 10^{51}$ erg emitted in UHE neutrinos, along with a corresponding beaming fraction of $1$%, GRAND and IceCube-Gen2 Radio have a large probability ($\sim 99$%) to detect a coincident neutrino event using the joint combination of CE+ET in a timescale of less than 15 years of operation for our fiducial choice of parameters. In case of nondetections, the parameter spaces can be constrained at $3\sigma$ level in similar timescales of operation. We also highlight and discuss the prospects of such joint radio neutrino detector network, their importance, and their role in facilitating synergic GW and neutrino observations in the next era of multimessenger astrophysics. |
author2 |
Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) |
format |
Report |
author |
Mukhopadhyay, Mainak Kotera, Kumiko Wissel, Stephanie Murase, Kohta Kimura, Shigeo S |
author_facet |
Mukhopadhyay, Mainak Kotera, Kumiko Wissel, Stephanie Murase, Kohta Kimura, Shigeo S |
author_sort |
Mukhopadhyay, Mainak |
title |
Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G |
title_short |
Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G |
title_full |
Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G |
title_fullStr |
Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G |
title_full_unstemmed |
Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G |
title_sort |
ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: grand, icecube-gen2 radio, and rno-g |
publisher |
HAL CCSD |
publishDate |
2024 |
url |
https://hal.science/hal-04650457 |
geographic |
Greenland |
geographic_facet |
Greenland |
genre |
Greenland |
genre_facet |
Greenland |
op_source |
https://hal.science/hal-04650457 2024 |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2406.19440 hal-04650457 https://hal.science/hal-04650457 ARXIV: 2406.19440 INSPIRE: 2803112 |
_version_ |
1809912983554359296 |