Advancing the Landscape of Multimessenger Science in the Next Decade

Engel, Kristi; Lewis, Tiffany R.; Muzio, Marco Stein; Venters, Tonia M.; Ahlers, M.; Albert, A.; Allen, Alice; Solares, Hugo Alberto Ayala; Anandagoda, Samalka; Andersen, T. C.; Antier, S.; Alvarez-Castillo, David; Bar, Olaf; Beznosko, Dmitri; Bibrzyck, Łukasz; Brazier, A.; Brisbois, C.; Brose, Robert; Brown, Duncan; Bulla, Mattia; Burgess, J. Michael; Burns, E.; Chirenti, Cecilia; Ciprini, S.; Clay, R. W.; Coughlin, M. W.; Cummings, Austin; D’Elia, V.; Dai, Shi; Dietrich, Tim; Lalla, N. Di; Dingus, B. L.; Durocher, Mora; Eser, Johannes; Filipović, Miroslav; Fleischhack, Henrike; Foucart, François; Frontczak, Michał; Fryer, Christopher L.; Gamble, Ronald; Gasparrini, D.; Giardino, Marco; Goodman, J. A.; Harding, J. Patrick; Hare, Jeremy; Holley‐Bockelmann, Kelly; Homola, P.; Hughes, Kaeli A.; Humensky, Brian; Inoue, Y.; Jaffe, T. R.; Kargaltsev, Oleg; Kierans, Carolyn; Kneller, James P.; Leto, C.; Lucarelli, F.; Martínez-Huerta, H.; Maselli, A.; Meli, A.; Meyers, P. M.; Mueller, G.; Nasipak, Zachary; Negro, Michela; Niedźwiecki, Michał; Noble, Scott C.; Omodei, N.; Osłowski, S.; Perri, M.; Piekarczyk, Marcin; Pittori, C.; Polenta, G.; Prechelt, Remy; Principe, G.; Racusin, J. L.; Rzecki, Krzysztof; Sambruna, R. M.; Schlieder, Joshua E.; Shoemaker, D. H.; Smale, A. P.; Sośnicki, Tomasz; Stein, Robert J.; Stuglik, Sławomir; Teuben, Peter; Thorpe, James; Verbiest, J. P. W.; Verrecchia, Franceso; Vitale, Salvatore; Wadiasingh, Zorawar; Wibig, T.; Willox, Elijah; Wilson-Hodge, C.; Wood, J.; Ye, Hui; Zhang, Haocheng

doi:10.48550/arxiv.2203.10074

Cited by 4 publications

(3 citation statements)

References 793 publications

(940 reference statements)

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“…Optical Cherenkov signal detection continues to be an important means of identifying neutrinoinduced signals, as evident from the international efforts of IceCube, Baikal-GVD, KM3NeT, and P-ONE. The planned IceCube-Gen2 (132) will expand IceCube's optical Cherenkov detection volume to 8 km 3 .…”

Section: Neutrino Detection For E > 10 Pevmentioning

confidence: 99%

“…As neutral particles with only weak interactions, neutrinos are important messengers from energetic astrophysical processes. They can escape astrophysical sources and travel without deflection through environments with magnetic fields to reveal their origins in a way that is complementary to the information carried by cosmic rays and electromagnetic radiation, and now by gravitational waves (3). Along with electromagnetic scattering of electrons, weak scattering of neutrinos and antineutrinos can be used to probe the structure of nucleons and nuclei (4,5).…”

Section: Introductionmentioning

confidence: 99%

See 1 more Smart Citation

High-Energy to Ultrahigh-Energy Neutrino Interactions

Reno

2023

Annu. Rev. Nucl. Part. Sci.

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The cross sections for neutrino interactions with nucleons have been measured directly in accelerator experiments and through the zenith-angle and energy dependence of neutrino events at the IceCube Neutrino Observatory. Fluxes of high-energy neutrinos are produced at the Large Hadron Collider and by cosmic rays in the atmosphere. High-energy neutrinos also come from astrophysical and cosmic sources. The theory of neutrino interactions is reviewed. Current cross-section measurements and prospects for the future are discussed. The focus here is on neutrino interactions for energies larger than 1 TeV. Expected final online publication date for the Annual Review of Nuclear and Particle Science, Volume 73 is September 2023. Please see http://www.annualreviews.org/page/journal/pubdates for revised estimates.

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Section: Neutrino Detection For E > 10 Pevmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

High-Energy to Ultrahigh-Energy Neutrino Interactions

Reno

2023

Annu. Rev. Nucl. Part. Sci.

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“…Firstly, the LIGO-Virgo-KAGRA (LVK) O4 run is currently underway and will continue until 2025, followed shortly thereafter by their O5 run from 2027 to 2030 [18]. At the same time, all-sky gamma-ray telescopes, such as Fermi and Swift, are still operating but may be decomissioned in the early 2030s, leaving a GeV-gap gamma-ray sky monitoring [19]. During this golden era for multimessenger science, RNO-G will be the only facility able to provide UHE neutrino follow-up to alerts.…”

Section: Marco Stein Muziomentioning

confidence: 99%

Multimessenger Potential of the Radio Neutrino Observatory in Greenland

A.¹,

Allison²,

Besson³

et al. 2023

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)

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The Radio Neutrino Observatory in Greenland (RNO-G) is the only ultrahigh energy (UHE, ≳30 PeV) neutrino monitor of the Northern sky and will soon be the world's most sensitive high-uptime detector of UHE neutrinos. Because of this, RNO-G represents an important piece of the multimessenger landscape over the next decade. In this talk, we will highlight RNO-G's multimessenger capabilities and its potential to provide key information in the search for the most extreme astrophysical accelerators. In particular, we will highlight opportunities enabled by RNO-G's unique field-of-view, its potential to constrain the sources of UHE cosmic rays, and its complementarity with IceCube at lower energies.

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Constraining the ellipticity and frequency of binary neutron star remnant via its gravitational-wave and electromagnetic radiations

Yuan

Fan

Lü

2023

Monthly Notices of the Royal Astronomical Society

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The nature of the merger remnant of binary neutron star (BNS) remains an open question. From the theoretical point of view, one possible outcome is a supra-massive neutron star (SMNS), which is supported by rigid rotation and through its survival of hundreds of seconds before collapsing into a black hole (BH). If this is the case, the SMNS can emit continuous gravitational waves (GW) and electromagnetic (EM) radiation, particularly in the X-ray band. In this work, the ellipticity and initial frequency of SMNS are constrained with a Bayesian framework using simulated X-ray and GW signals, which could be detected by The Transient High Energy Sky and Early Universe Surveyor (THESEUS) and Einstein Telescope (ET), respectively. We found that only considering the X-ray emission can not completely constrain the initial frequency and ellipticity of the SMNS, but it can reduce the ranges of the parameters. Afterwards, we can use the posterior distribution of the X-ray parameter estimates as a prior for the GW parameter estimates. It was found that the 95% credible region of the joint X-ray–GW analysis was about 105 times smaller than that of the X-ray analysis alone.

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Advancing the Landscape of Multimessenger Science in the Next Decade

Cited by 4 publications

References 793 publications

High-Energy to Ultrahigh-Energy Neutrino Interactions

High-Energy to Ultrahigh-Energy Neutrino Interactions

Multimessenger Potential of the Radio Neutrino Observatory in Greenland

Constraining the ellipticity and frequency of binary neutron star remnant via its gravitational-wave and electromagnetic radiations

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