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Multimessenger astronomy incorporating gravitational radiation is a new and exciting field that will potentially provide significant results and exciting challenges in the near future. With advanced interferometric gravitational wave…

General Relativity and Quantum Cosmology · Physics 2019-08-13 N. L. Christensen

Observations with next-generation ground-based detectors further enhanced with multi-messenger (electromagnetic and neutrino) detections will allow us to probe new extreme astrophysics. Target sources included: core-collapse supernovae,…

A budget neutral strategy is proposed for NSF to lead the implementation of multimessenger astronomy and astrophysics, as outlined in the Astro2010 Decadal Survey. The emerging capabilities for simultaneous measurements of physical and…

Instrumentation and Methods for Astrophysics · Physics 2012-03-08 Maurice H. P. M. van Putten , Graziano Rossi

The observational evidence for the inflationary cosmology with baryosynthesis and dark matter/energy can be viewed as the messenger for new physics, which governed the Universe origin, evolution and structure. To specify the physics beyond…

High Energy Physics - Phenomenology · Physics 2021-02-03 Maxim Yu. Khlopov

Multi-messenger astronomy, the coordinated observation of different classes of signals originating from the same astrophysical event, provides a wealth of information about astrophysical processes with far-reaching implications. So far, the…

Instrumentation and Methods for Astrophysics · Physics 2021-03-02 Conner Dailey , Colin Bradley , Derek F. Jackson Kimball , Ibrahim Sulai , Szymon Pustelny , Arne Wickenbrock , Andrei Derevianko

Multimessenger observations may hold the key to learn about the most energetic sources in the universe. The recent construction of large scale observatories opened new possibilities in testing non thermal cosmic processes with alternative…

High Energy Astrophysical Phenomena · Physics 2019-06-05 Dafne Guetta

The multi-messenger exploration of dark matter and physics beyond the Standard Model has emerged as a central direction in modern astro-particle physics, particularly following the discovery of gravitational waves. In this work, we present…

In the quest for high-energy neutrino sources, the Astrophysical Multimessenger Observatory Network (AMON) has implemented a new search by combining data from the High Altitude Water Cherenkov (HAWC) observatory and the Astronomy with a…

High Energy Astrophysical Phenomena · Physics 2023-03-15 H. A. Ayala Solares , S. Coutu , D. Cowen , D. B. Fox , T. Grégoire , F. McBride , M. Mostafá , K. Murase , S. Wissel , A. Albert , S. Alves , M. André , M. Ardid , S. Ardid , J. -J. Aubert , J. Aublin , B. Baret , S. Basa , B. Belhorma , M. Bendahman , F. Benfenati , V. Bertin , S. Biagi , M. Bissinger , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Brânzaş , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , A. Capone , L. Caramete , J. Carr , V. Carretero , S. Celli , M. Chabab , T. N. Chau , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , J. A. B. Coelho , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , A. F. Díaz , G. de Wasseige , B. De Martino , C. Distefano , I. Di Palma , A. Domi , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , T. van Eeden , D. van Eijk , N. El Khayati , A. Enzenhöfer , P. Fermani , G. Ferrara , F. Filippini , L. Fusco , J. García , P. Gay , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , F. Huang , G. Illuminati , C. W. James , B. Jisse-Jung , M. de Jong , P. de Jong , M. Kadler , O. Kalekin , U. Katz , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , M. Lamoureux , R. Le Breton , D. Lefèvre , E. Leonora , G. Levi , S. Le Stum , D. Lopez-Coto , S. Loucatos , L. Maderer , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , K. Melis , P. Migliozzi , A. Moussa , R. Muller , L. Nauta , S. Navas , E. Nezri , B. Ó Fearraigh , A. Păaun , G. E. Păvălaş , C. Pellegrino , M. Perrin-Terrin , V. Pestel , P. Piattelli , C. Pieterse , C. Poirè , V. Popa , T. Pradier , N. Randazzo , D. Real , S. Reck , G. Riccobene , A. Romanov , A. Sánchez-Losa , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , J. Schumann , F. Schüssler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , S. J. Tingay , B. Vallage , V. Van Elewyck , F. Versari , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zúñiga , A. Albert , C. Alvarez , J. C. Arteaga-Velázquez , R. Babu , E. Belmont-Moreno , K. S. Caballero-Mora , T. Capistrán , A. Carramiñana , S. Casanova , U. Cotti , O. Chaparro-Amaro , J. Cotzomi , S. Coutiño de León , E. De la Fuente , C. de León , R. Diaz Hernandez , M. A. DuVernois , M. Durocher , J. C. Díaz-Vélez , K. Engel , C. Espinoza , K. L. Fan , M. Fernández Alonso , N. Fraija , J. A. García-González , F. Garfias , M. M. González , J. A. Goodman , J. P. Harding , S. Hernandez , D. Huang , F. Hueyotl-Zahuantitla , P. Hüntemeyer , A. Iriarte , V. Joshi , S. Kaufmann , A. Lara , H. León Vargas , J. T. Linnemann , A. L. Longinotti , G. Luis-Raya , K. Malone , O. Martinez , I. Martinez-Castellanos , J. Martínez-Castro , J. A. Matthews , P. Miranda-Romagnoli , J. A. Morales-Soto , E. Moreno , A. Nayerhoda , L. Nellen , M. U. Nisa , R. Noriega-Papaqui , N. Omodei , A. Peisker , Y. Pérez Araujo , E. G. Pérez-Pérez , C. D. Rho , D. Rosa-González , E. Ruiz-Velasco , H. Salazar , F. Salesa Greus , A. Sandoval , M. Schneider , A. J. Smith , Y. Son , R. W. Springer , O. Tibolla , K. Tollefson , I. Torres , R. Torres-Escobedo , R. Turner , F. Ureña-Mena , E. Varela , X. Wang , K. Whitaker , E. Willox , A. Zepeda , H. Zhou

Future GW detector networks and EM observatories will provide a unique opportunity to observe the most luminous events in the Universe involving matter in extreme environs. They will address some of the key questions in physics and…

Neutron stars are compact and dense celestial objects that offer the unique opportunity to explore matter and its interactions under conditions that cannot be reproduced elsewhere in the Universe. Their extreme gravitational, rotational and…

High Energy Astrophysical Phenomena · Physics 2024-01-29 Stefano Ascenzi , Vanessa Graber , Nanda Rea

The recent discoveries of high-energy cosmic neutrinos and gravitational waves from astrophysical objects have led to the new era of multi-messenger astrophysics. In particular, electromagnetic follow-up observations triggered by these…

High Energy Astrophysical Phenomena · Physics 2019-10-25 Kohta Murase , Imre Bartos

The possible connection between high energy neutrinos in the energy region above 100 TeV and ultrahigh energy cosmic rays (UHECRs) at energies above $10^{19}$ eV motivates multi-messenger observation approaches involving neutrinos and the…

High Energy Astrophysical Phenomena · Physics 2023-09-25 Shigeru Yoshida

High-energy cosmic neutrinos carry unique information about the most energetic non-thermal sources in the Universe. This white paper describes the outstanding astrophysics questions that neutrino astronomy can address in the coming decade.…

The All-sky Medium Energy Gamma-ray Observatory (AMEGO) is a Probe-class mission concept that will provide essential contributions to multimessenger astrophysics in the next decade. AMEGO operates both as a Compton and pair telescope to…

Instrumentation and Methods for Astrophysics · Physics 2021-01-11 Carolyn A. Kierans , the AMEGO Team

Gravitational waves (GWs) are expected to play a crucial role in the development of multimessenger astrophysics. The combination of GW observations with other astrophysical triggers, such as from gamma-ray and X-ray satellites,…

General Relativity and Quantum Cosmology · Physics 2011-01-28 Eric Chassande-Mottin , Martin Hendry , Patrick J. Sutton , Szabolcs Márka

The precision era of multi-messenger astronomy, together with modern astrophysical, cosmological, and gravitational wave observations, increasingly points toward the existence of a ``dark" sector that cannot be explained within the…

Multi-messenger astrophysics is undergoing a transition towards low-latency searches based on signals that could not individually be established as discoveries. The rapid identification of signals is important in order to initiate timely…

High Energy Astrophysical Phenomena · Physics 2019-10-30 Imre Bartos , Doga Veske , Azadeh Keivani , Zsuzsa Marka , Stefan Countryman , Erik Blaufuss , Chad Finley , Szabolcs Marka

Coincident multimessenger observations of cosmic sources can offer numerous benefits, especially when used in the context of synergistic astrophysics. One significant advantage is enhancing the detection significance of separate detectors…

High Energy Astrophysical Phenomena · Physics 2025-05-12 Doğa Veske , Albert Zhang , Zsuzsa Márka , Szabolcs Márka