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Neutron stars are unique cosmic laboratories for the exploration of matter under extreme conditions of density and neutron-proton asymmetry. Due to their enormous dynamic range, neutron stars display a myriad of exotic states of matter that…

Nuclear Theory · Physics 2018-05-18 J. Piekarewicz

The field of gamma-ray astronomy has experienced impressive progress over the last decade. Thanks to the advent of a new generation of imaging air Cherenkov telescopes (H.E.S.S., MAGIC, VERITAS) and thanks to the launch of the Fermi-LAT…

Instrumentation and Methods for Astrophysics · Physics 2016-07-20 Jürgen Knödlseder

Harnessing the sheer discovery potential of gravitational wave astronomy will require bold, deliberate, and sustained efforts to train and develop the requisite workforce. The next decade requires a strategic plan to build -- from the…

Neutron star binaries, which are among the most promising sources for the direct detection of gravitational waves (GW) by ground based detectors, are also potential electromagnetic (EM) emitters. Gravitational waves will provide a new…

General Relativity and Quantum Cosmology · Physics 2015-06-19 Shaon Ghosh , Gijs Nelemans

It remains an open question to what extent many of the astronomical sources of intense bursts of electromagnetic radiation are also strong emitters of non-photon messengers, in particular gravitational waves (GWs) and high-energy neutrinos…

High Energy Astrophysical Phenomena · Physics 2011-12-15 Imre Bartos , Chad Finley , Alessandra Corsi , Szabolcs Márka

With the discovery of a high-energy neutrino flux in the 0.1 PeV to PeV range from beyond the Earth's atmosphere with the IceCube detector, neutrino astronomy has achieved a major breakthrough in the exploration of the high-energy universe.…

High Energy Astrophysical Phenomena · Physics 2019-08-13 A. Kappes

An overview of the multi-messenger capabilities of the Pierre Auger Observatory is presented. The techniques and performance of searching for Ultra-High Energy neutrinos, photons and neutrons are described. Some of the most relevant results…

High Energy Astrophysical Phenomena · Physics 2019-04-29 The Pierre Auger Collaboration , A. Aab , P. Abreu , M. Aglietta , I. F. M. Albuquerque , J. M. Albury , I. Allekotte , A. Almela , J. Alvarez Castillo , J. Alvarez-Muñiz , G. A. Anastasi , L. Anchordoqui , B. Andrada , S. Andringa , C. Aramo , H. Asorey , P. Assis , G. Avila , A. M. Badescu , A. Bakalova , A. Balaceanu , F. Barbato , R. J. Barreira Luz , S. Baur , K. H. Becker , J. A. Bellido , C. Berat , M. E. Bertaina , X. Bertou , P. L. Biermann , J. Biteau , S. G. Blaess , A. Blanco , J. Blazek , C. Bleve , M. Boháčová , D. Boncioli , C. Bonifazi , N. Borodai , A. M. Botti , J. Brack , T. Bretz , A. Bridgeman , F. L. Briechle , P. Buchholz , A. Bueno , S. Buitink , M. Buscemi , K. S. Caballero-Mora , L. Caccianiga , L. Calcagni , A. Cancio , F. Canfora , J. M. Carceller , R. Caruso , A. Castellina , F. Catalani , G. Cataldi , L. Cazon , M. Cerda , J. A. Chinellato , J. Chudoba , L. Chytka , R. W. Clay , A. C. Cobos Cerutti , R. Colalillo , A. Coleman , M. R. Coluccia , R. Conceição , A. Condorelli , G. Consolati , F. Contreras , F. Convenga , M. J. Cooper , S. Coutu , C. E. Covault , B. Daniel , S. Dasso , K. Daumiller , B. R. Dawson , J. A. Day , R. M. de Almeida , S. J. de Jong , G. De Mauro , J. R. T. de Mello Neto , I. De Mitri , J. de Oliveira , F. O. de Oliveira Salles , V. de Souza , J. Debatin , M. del Río , O. Deligny , N. Dhital , M. L. Díaz Castro , F. Diogo , C. Dobrigkeit , J. C. D'Olivo , Q. Dorosti , R. C. dos Anjos , M. T. Dova , A. Dundovic , J. Ebr , R. Engel , M. Erdmann , C. O. Escobar , A. Etchegoyen , H. Falcke , J. Farmer , G. Farrar , A. C. Fauth , N. Fazzini , F. Feldbusch , F. Fenu , L. P. Ferreyro , J. M. Figueira , A. Filipčič , M. M. Freire , T. Fujii , A. Fuster , B. García , H. Gemmeke , A. Gherghel-Lascu , P. L. Ghia , U. Giaccari , M. Giammarchi , M. Giller , D. Głas , J. Glombitza , F. Gobbi , G. Golup , M. Gómez Berisso , P. F. Gómez Vitale , J. P. Gongora , N. González , I. Goos , D. Góra , A. Gorgi , M. Gottowik , T. D. Grubb , F. Guarino , G. P. Guedes , E. Guido , R. Halliday , M. R. Hampel , P. Hansen , D. Harari , T. A. Harrison , V. M. Harvey , A. Haungs , T. Hebbeker , D. Heck , P. Heimann , G. C. Hill , C. Hojvat , E. M. Holt , P. Homola , J. R. Hörandel , P. Horvath , M. Hrabovský , T. Huege , J. Hulsman , A. Insolia , P. G. Isar , I. Jandt , J. A. Johnsen , M. Josebachuili , J. Jurysek , A. Kääpä , K. H. Kampert , B. Keilhauer , N. Kemmerich , J. Kemp , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Krause , D. Kuempel , G. Kukec Mezek , A. Kuotb Awad , B. L. Lago , D. LaHurd , R. G. Lang , R. Legumina , M. A. Leigui de Oliveira , V. Lenok , A. Letessier-Selvon , I. Lhenry-Yvon , O. C. Lippmann , D. Lo Presti , L. Lopes , R. López , A. López Casado , R. Lorek , Q. Luce , A. Lucero , M. Malacari , G. Mancarella , D. Mandat , B. C. Manning , P. Mantsch , A. G. Mariazzi , I. C. Mariş , G. Marsella , D. Martello , H. Martinez , O. Martínez Bravo , M. Mastrodicasa , H. J. Mathes , S. Mathys , J. Matthews , G. Matthiae , E. Mayotte , P. O. Mazur , G. Medina-Tanco , D. Melo , A. Menshikov , K. -D. Merenda , S. Michal , M. I. Micheletti , L. Middendorf , L. Miramonti , B. Mitrica , D. Mockler , S. Mollerach , F. Montanet , C. Morello , G. Morlino , M. Mostafá , A. L. Müller , M. A. Muller , S. Müller , R. Mussa , L. Nellen , P. H. Nguyen , M. Niculescu-Oglinzanu , M. Niechciol , D. Nitz , D. Nosek , V. Novotny , L. Nožka , A Nucita , L. A. Núñez , F. Oikonomou , A. Olinto , M. Palatka , J. Pallotta , M. P. Panetta , P. Papenbreer , G. Parente , A. Parra , M. Pech , F. Pedreira , J. Pękala , R. Pelayo , J. Peña-Rodriguez , L. A. S. Pereira , M. Perlin , L. Perrone , C. Peters , S. Petrera , J. Phuntsok , T. Pierog , M. Pimenta , V. Pirronello , M. Platino , J. Poh , B. Pont , C. Porowski , R. R. Prado , P. Privitera , M. Prouza , A. Puyleart , S. Querchfeld , S. Quinn , R. Ramos-Pollan , J. Rautenberg , D. Ravignani , M. Reininghaus , J. Ridky , F. Riehn , M. Risse , P. Ristori , V. Rizi , W. Rodrigues de Carvalho , J. Rodriguez Rojo , M. J. Roncoroni , M. Roth , E. Roulet , A. C. Rovero , P. Ruehl , S. J. Saffi , A. Saftoiu , F. Salamida , H. Salazar , G. Salina , J. D. Sanabria Gomez , F. Sánchez , E. M. Santos , E. Santos , F. Sarazin , R. Sarmento , C. Sarmiento-Cano , R. Sato , P. Savina , M. Schauer , V. Scherini , H. Schieler , M. Schimassek , M. Schimp , F. Schlüter , D. Schmidt , O. Scholten , P. Schovánek , F. G. Schröder , S. Schröder , J. Schumacher , S. J. Sciutto , M. Scornavacche , R. C. Shellard , G. Sigl , G. Silli , O. Sima , R. Šmída , G. R. Snow , P. Sommers , J. F. Soriano , J. Souchard , R. Squartini , D. Stanca , S. Stanič , J. Stasielak , P. Stassi , M. Stolpovskiy , A. Streich , F. Suarez , M. Suárez-Durán , T. Sudholz , T. Suomijärvi , A. D. Supanitsky , J. Šupík , Z. Szadkowski , A. Taboada , O. A. Taborda , A. Tapia , C. Timmermans , C. J. Todero Peixoto , B. Tomé , G. Torralba Elipe , A. Travaini , P. Travnicek , M. Trini , M. Tueros , R. Ulrich , M. Unger , M. Urban , J. F. Valdés Galicia , I. Valiño , L. Valore , P. van Bodegom , A. M. van den Berg , A. van Vliet , E. Varela , B. Vargas Cárdenas , D. Veberič , C. Ventura , I. D. Vergara Quispe , V. Verzi , J. Vicha , L. Villaseñor , J. Vink , S. Vorobiov , H. Wahlberg , A. A. Watson , M. Weber , A. Weindl , M. Wiedeński , L. Wiencke , H. Wilczyński , T. Winchen , M. Wirtz , D. Wittkowski , B. Wundheiler , L. Yang , A. Yushkov , E. Zas , D. Zavrtanik , M. Zavrtanik , L. Zehrer , A. Zepeda , B. Zimmermann , M. Ziolkowski , Z. Zong , F. Zuccarello

This review describes telescopes designed to study neutrinos from astrophysical sources. These sources include the Sun and Supernovae emitting neutrino energies up to tens of MeV, atmospheric neutrino sources caused by cosmic ray…

Astrophysics · Physics 2008-11-26 A. B. McDonald , C. Spiering , S. Schoenert , E. T. Kearns , T. Kajita

Ongoing experimental efforts to detect cosmic sources of high energy neutrinos are guided by the expectation that astrophysical accelerators of cosmic ray protons would also generate neutrinos through interactions with ambient matter and/or…

Astrophysics · Physics 2014-10-13 Luis A. Anchordoqui , Dan Hooper , Subir Sarkar , Andrew M. Taylor

Cataclysmic cosmic events can be plausible sources of both gravitational waves (GW) and high-energy neutrinos (HEN). Both GW and HEN are alternative cosmic messengers that may escape very dense media and travel unaffected over cosmological…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 V. Van Elewyck

Cosmic high energy neutrinos are inextricably linked to the origin of cosmic rays which is one of the major unresolved questions in astrophysics. In particular, the highest energy cosmic rays observed possess macroscopic energies and their…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Sigl

We summarize recent results of the observations of high (1 TeV-100 PeV) and ultrahigh ($\geq 100$ PeV) energy neutrinos, including the detection of a diffuse cosmic high-energy neutrino background, the identification of the first neutrino…

High Energy Astrophysical Phenomena · Physics 2026-05-13 Ke Fang , Kohta Murase

The gamma-ray survey of the sky by the Fermi Gamma-ray Space Telescope offers both opportunities and challenges for multiwavelength and multi-messenger studies. Gamma-ray bursts, pulsars, binary sources, flaring Active Galactic Nuclei, and…

High Energy Astrophysical Phenomena · Physics 2019-08-13 D. J. Thompson

The discovery by Advanced LIGO/Virgo of gravitational waves from the binary neutron star (NS) merger GW170817, and subsequently by astronomers of transient counterparts across the electromagnetic (EM) spectrum, has initiated the era of…

High Energy Astrophysical Phenomena · Physics 2017-10-18 Brian D. Metzger

Gamma-rays, the most energetic photons, carry information from the far reaches of extragalactic space with minimal interaction or loss of information. They bring messages about particle acceleration in environments so extreme they cannot be…

High Energy Astrophysical Phenomena · Physics 2022-03-15 Kristi Engel , Jordan Goodman , Petra Huentemeyer , Carolyn Kierans , Tiffany R. Lewis , Michela Negro , Marcos Santander , David A. Williams , Alice Allen , Tsuguo Aramaki , Rafael Alves Batista , Mathieu Benoit , Peter Bloser , Jennifer Bohon , Aleksey E. Bolotnikov , Isabella Brewer , Michael S. Briggs , Chad Brisbois , J. Michael Burgess , Eric Burns , Regina Caputo , Gabriella A. Carini , S. Bradley Cenko , Eric Charles , Stefano Ciprini , Valerio D'Elia , Tansu Daylan , James Distel , Axel Donath , Wade Duvall , Henrike Fleischhack , Corinne Fletcher , Wen Fe Fong , Dario Gasparrini , Marco Giardino , Adam Goldstein , Sean Griffin , J. Eric Grove , Rachel Hamburg , J. Patrick Harding , Jeremy Hare , Boyan Hristov , C. Michelle Hui , Tess Jaffe , Pete Jenke , Oleg Kargaltsev , Christopher M. Karwin , Matthew Kerr , Dongsung Kim , Daniel Kocevski , John Krizmanic , Ranjan Laha , Niccolo Di Lalla , Jason Legere , Cristina Leto , Richard Leys , Fabrizio Lucarelli , Israel Martinez-Castellanos , Alessandro Maselli , M. Nicola Mazziotta , Mark McConnell , Julie McEnery , Jessica Metcalfe , Manuel Meyer , Alexander A. Moiseev , Reshmi Mukherjee , Michela Negro , Keiichi Ogasawara , Nicola Omodei , Ivan Peric , Jeremy S. Perkins , Matteo Perri , Carlotta Pittori , Gianluca Polenta , Daniel Poulson , Robert Preece , Giacomo Principe , Judith L. Racusin , Oliver Roberts , Nicholas L. Rodd , Peter Shawhan , Thomas Shutt , Clio Sleator , Alan Smale , John Smedley , Jacob R. Smith , Jay Tasson , Peter Teuben , John Tomsick , Peter Veres , Francesco Verrecchia , Zorawar Wadiasingh , Colleen A. Wilson-Hodge , Joshua Wood , Richard S. Woolf , Hui Yang , Bing Zhang , Haocheng Zhang , Andreas Zoglauer

High precision astrometry provides the foundation to resolve many fundamental problems in astrophysics. The application of astrometric studies spans a wide range of fields, and has undergone enormous growth in recent years. This is as a…

Instrumentation and Methods for Astrophysics · Physics 2019-10-30 Maria Rioja , Richard Dodson

A world-wide array of highly sensitive interferometers stands poised to usher in a new era in astronomy with the first direct detection of gravitational waves. The data from these instruments will provide a unique perspective on extreme…

General Relativity and Quantum Cosmology · Physics 2013-02-27 Neil J. Cornish

Over the last two decades, we have intensified our search for a ghost particle, with the hope that it would provide us with information on the darkest places of our Universe. This quest has been conducted from the deep caves of the Earth,…

High Energy Astrophysical Phenomena · Physics 2023-10-02 Valentin Decoene

Gamma ray earthbound and satellite experiments have discovered, over the last years, many galactic and extra-galactic gamma ray sources. The detection of astrophysical neutrinos emitted by the same sources would imply that these…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 A. G. Tsirigotis , A. Leisos , S. E. Tzamarias
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