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dc.creatorAndo, Shin’ichiro-
dc.creatorBaret, Bruny-
dc.creatorBartos, Imre-
dc.creatorBouhou, Boutayeb-
dc.creatorChassande Mottin, Eric-
dc.creatorCorsi, Alessandra-
dc.creatorDi Palma, Irene-
dc.creatorDietz, Alexander-
dc.creatorDonzaud, Corinne-
dc.creatorEichler, David-
dc.creatorFinley, Chad-
dc.creatorGuetta, Dafne-
dc.creatorHalzen, Francis-
dc.creatorJones, Gareth-
dc.creatorKandhasamy, Shivaraj-
dc.creatorKotake, Kei-
dc.creatorKouchner, Antoine-
dc.creatorMandic, Vuk-
dc.creatorMarka, Szabolcs-
dc.creatorMarka, Zsuzsa-
dc.creatorMoscoso, Luciano-
dc.creatorPapa, Maria Alessandra-
dc.creatorPiran, Tsvi-
dc.creatorPradier, Thierry-
dc.creatorRomero, Gustavo Esteban-
dc.creatorSutton, Patrick-
dc.creatorThrane, Eric-
dc.creatorVan Elewyck, Veronique-
dc.creatorWaxman, Eli-
dc.date2016-03-18T19:11:23Z-
dc.date2016-03-18T19:11:23Z-
dc.date2013-10-
dc.date2016-03-30 10:35:44.97925-03-
dc.date.accessioned2019-04-29T15:49:49Z-
dc.date.available2019-04-29T15:49:49Z-
dc.date.issued2013-10-
dc.identifierAndo, Shin’ichiro; Baret, Bruny ; Bartos, Imre; Bouhou, Boutayeb ; Chassande Mottin, Eric; et al.; Multimessenger astronomy with gravitational waves and high-energy neutrinos; American Physical Society; Reviews Of Modern Physics; 85; 4; 10-2013; 1401-1401-
dc.identifier0034-6861-
dc.identifierhttp://hdl.handle.net/11336/4866-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/303161-
dc.descriptionMany of the astrophysical sources and violent phenomena observed in our Universe are potential emitters of gravitational waves and high-energy cosmic radiation, including photons, hadrons, and presumably also neutrinos. Both gravitational waves (GW) and high-energy neutrinos (HEN) are cosmic messengers that may escape much denser media than photons. They travel unaffected over cosmological distances, carrying information from the inner regions of the astrophysical engines from which they are emitted (and from which photons and charged cosmic rays cannot reach us). For the same reasons, such messengers could also reveal new, hidden sources that have not been observed by conventional photon-based astronomy. Coincident observation of GWs and HENs may thus play a critical role in multimessenger astronomy. This is particularly true at the present time owing to the advent of a new generation of dedicated detectors: the neutrino telescopes IceCube at the South Pole and ANTARES in the Mediterranean Sea, as well as the GW interferometers Virgo in Italy and LIGO in the United States. Starting from 2007, several periods of concomitant data taking involving these detectors have been conducted. More joint data sets are expected with the next generation of advanced detectors that are to be operational by 2015, with other detectors, such as KAGRA in Japan, joining in the future. Combining information from these independent detectors can provide original ways of constraining the physical processes driving the sources and also help confirm the astrophysical origin of a GW or HEN signal in case of coincident observation. Given the complexity of the instruments, a successful joint analysis of this combined GW and HEN observational data set will be possible only if the expertise and knowledge of the data is shared between the two communities. This Colloquium aims at providing an overview of both theoretical and experimental state of the art and perspectives for GW and HEN multimessenger astronomy.-
dc.descriptionFil: Ando, Shin’ichiro. Gravitation AstroParticle Physics Amsterdam Institute (GRAPPA); Países Bajos-
dc.descriptionFil: Baret, Bruny . AstroParticule et Cosmologie (APC), CNRS; Francia-
dc.descriptionFil: Bartos, Imre. Department of Physics, Columbia University; Estados Unidos-
dc.descriptionFil: Bouhou, Boutayeb . AstroParticule et Cosmologie (APC), CNRS; Francia-
dc.descriptionFil: Chassande Mottin, Eric. AstroParticule et Cosmologie (APC) , CNRS; Francia-
dc.descriptionFil: Corsi, Alessandra. Physics Department, George Washington University; Estados Unidos-
dc.descriptionFil: Di Palma, Irene . Albert-Einstein-Institut, Max-Planck-Institut fur Gravitationsphysik; Alemania-
dc.descriptionFil: Dietz, Alexander . Department of Physics and Astronomy of the University of Mississippi; Estados Unidos-
dc.descriptionFil: Donzaud, Corinne . AstroParticule et Cosmologie (APC), CNRS; Francia-
dc.descriptionFil: Eichler, David . Department of Physics, Ben Gurion University; Israel-
dc.descriptionFil: Finley, Chad . Oskar Klein Centre & Dept. of Physics, Stockholm University,; Suecia-
dc.descriptionFil: Guetta, Dafne . Department of Physics and Optical Engineering; Israel-
dc.descriptionFil: Halzen, Francis . Department of Physics, University of Wisconsin; Estados Unidos-
dc.descriptionFil: Jones, Gareth . School of Physics and Astronomy, Cardiff University; Reino Unido-
dc.descriptionFil: Kandhasamy, Shivaraj . University of Minnesota, Minneapolis; Estados Unidos-
dc.descriptionFil: Kotake, Kei . Division of Theoretical Astronomy, National Astronomical Observatory of Japan; Japón-
dc.descriptionFil: Kouchner, Antoine . AstroParticule et Cosmologie (APC), CNRS; Francia-
dc.descriptionFil: Mandic, Vuk . University of Minnesota, Minneapolis; Estados Unidos-
dc.descriptionFil: Marka, Szabolcs . Department of Physics, Columbia University; Estados Unidos-
dc.descriptionFil: Marka, Zsuzsa . Department of Physics, Columbia University; Estados Unidos-
dc.descriptionFil: Moscoso, Luciano . AstroParticule et Cosmologie (APC), CNRS; Francia-
dc.descriptionFil: Papa, Maria Alessandra . Albert-Einstein-Institut, Max-Planck-Institut fur Gravitationsphysik; Alemania-
dc.descriptionFil: Piran, Tsvi . Racah Institute of Physics, Hebrew University of Jerusalem; Israel-
dc.descriptionFil: Pradier, Thierry . Universite de Strasbourg & Institut Pluridisciplinaire Hubert Curien,Strasbourg; Francia-
dc.descriptionFil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina-
dc.descriptionFil: Sutton, Patrick . School of Physics and Astronomy, Cardiff University; Reino Unido-
dc.descriptionFil: Thrane, Eric . University of Minnesota, Minneapolis; Estados Unidos-
dc.descriptionFil: Van Elewyck, Veronique. AstroParticule et Cosmologie (APC), CNRS; Francia-
dc.descriptionFil: Waxman, Eli . Department of Particle Physics & Astrophysics, The Weizmann Institute of Science; Israel-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherAmerican Physical Society-
dc.relationinfo:eu-repo/semantics/altIdentifier/arxiv/1203.5192-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/RevModPhys.85.1401-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1203.5192-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/10.1103/RevModPhys.85.1401-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://journals.aps.org/rmp/abstract/10.1103/RevModPhys.85.1401-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.subjectGravitational wave detectors-
dc.subjectGravitational radiation-
dc.subjectNeutrino muons-
dc.subjectCosmic ray detectors-
dc.subjectCosmic rays-
dc.subjectNeutrino pions-
dc.subjectParticle detectors-
dc.subjectMagnetic fields-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleMultimessenger astronomy with gravitational waves and high-energy neutrinos-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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