English
Related papers

Related papers: Multi-Messenger Searches in Astrophysics

200 papers

Binary neutron star mergers observations are a unique way to constrain fundamental physics and astrophysics at the extreme. The interpretation of gravitational-wave events and their electromagnetic counterparts crucially relies on…

High Energy Astrophysical Phenomena · Physics 2020-11-18 Sebastiano Bernuzzi

Neutrino astrophysics offers new perspectives on the Universe investigation: high energy neutrinos, produced by the most energetic phenomena in our Galaxy and in the Universe, carry complementary (if not exclusive) information about the…

High Energy Astrophysical Phenomena · Physics 2010-02-11 T. Chiarusi , M. Spurio

The current status of searches for ultra-high energy neutrinos and photons using air showers is reviewed. Regarding both physics and observational aspects, possible future research directions are indicated.

High Energy Astrophysical Phenomena · Physics 2019-08-15 J. Alvarez-Muniz , M. Risse , G. I. Rubtsov , B. T. Stokes

This century has seen a dramatic increase in observational possibilities of the physics of the universe. Several of the very recent new developments with emphasis on the particle physics aspect and in particular Gamma-Gamma interactions are…

High Energy Physics - Phenomenology · Physics 2007-05-23 H. Meyer

The recent milestones in multi-messenger astronomy have opened new ways to study the Unverse. The unprecedented gravitational wave (GW) follow-up campaigns established the power that the combination of different messengers has to identify…

The discovery of gravitational waves, high-energy neutrinos or the very-high-energy counterpart of gamma-ray bursts has revolutionized the high-energy and transient astrophysics community. The development of new instruments and analysis…

High Energy Astrophysical Phenomena · Physics 2021-06-09 Ž. Bošnjak , A. M. Brown , A. Carosi , M. Chernyakova , P. Cristofari , F. Longo , A. López-Oramas , M. Santander , K. Satalecka , F. Schüssler , O. Sergijenko , A. Stamerra , I. Agudo , R. Alves Batista , E. Amato , E. O. Anguner , L. A. Antonelli , M. Backes , Csaba Balazs , L. Baroncelli , J. Becker Tjus , C. Bigongiari , E. Bissaldi , C. Boisson , J. Bolmont , M. Böttcher , P. Bordas , C. Braiding , J. Bregeon , N. Bucciantini , A. Bulgarelli , M. Burton , F. Cangemi , P. Caraveo , M. Cardillo , S. Caroff , S. Casanova , S. Chaty , J. G. Coelho , G. Cotter , A. D'Aì , F. D'Ammando , E. M. de Gouveia Dal Pino , D. della Volpe , D. de Martino , T. Di Girolamo , A. Di Piano , A. Djannati-Ataï , V. Dwarkadas , E. de Ona Wilhelmi , R. C. Dos Anjos , G. Emery , E. Fedorova , S. Fegan , A. Fiasson , V. Fioretti , M. D. Filipovic , D. Gaggero , G. Galanti , D. Gasparrini , G. Ghirlanda , P. Goldoni , J. Granot , J. G. Green , M. Heller , B. Hnatyk , R. Hnatyk , D. Horan , T. Hovatta , S. Inoue , M. Jamrozy , D. Kantzas , B. Khélifi , N. Komin , A. Lamastra , N. La Palombara , J. P. Lenain , E. Lindfors , I. Liodakis , S. Lombardi , F. Lucarelli , P. L. Luque-Escamilla , P. Majumdar , A. Marcowith , S. Markoff , J. Marti , M. Martinez , D. Mazin , S. McKeague , S. Mereghetti , E. Mestre , T. Montaruli , G. Morlino , A. Morselli , C. Mundell , T. Murach , L. Nava , A. Nayerhoda , L. Nicastro , J. Niemiec , M. Nikolajuk , B. Olmi , R. Ong , M. Orienti , J. P. Osborne , Josep M. Paredes , G. Pareschi , N. Parmiggiani , B. Patricelli , A. Pe'er , G. Piano , G. Pühlhofer , M. Punch , O. Reimer , M. Ribó , G. Rodriguez , J. Rodriguez , P. Romano , G. Romeo , M. Roncadelli , G. Rowell , B. Rudak , I. Sadeh , F. Salesa Greus , F. G. Saturni , U. Sawangwit , M. Seglar-Arroyo , R. C. Shellard , H. Sol , R. Starling , T. Stolarczyk , G. Tagliaferri , F. Tavecchio , L. Tibaldo , V. Testa , S. Vercellone , A. Viana , J. Vink , V. Vitale , S. D. Vergani , S. Vorobiov , A. Wierzcholska , L. Yang , D. Zavrtanik , V. Zhdanov

Two years ago, the astronomical community witnessed a historical breakthrough observation: the detection of a short Gamma-Ray Burst (GRB) by gamma-ray instruments in coincidence with the detection of a Gravitation Wave (GW) signal produced…

High Energy Astrophysical Phenomena · Physics 2019-09-16 Elisabetta Bissaldi

The present work discusses the development of the radio technique for detection of ultra-high energy air-showers induced by cosmic radiation, and the prospects of its application in the future multi-messenger activities, particularly for…

Instrumentation and Methods for Astrophysics · Physics 2019-05-22 D. Kostunin

Selected results obtained in major observational sky surveys (DSS, 2MASS, 2dF, SDSS) and deep field observations (HDF, GOODS, HUDF, etc.) are reviewed. Modern surveys provide information on the characteristics and space distribution of…

Astrophysics · Physics 2009-11-11 V. P. Reshetnikov

With the advanced gravitational wave detectors coming on line in the next 5 years, we expect to make the first detections of gravitational waves from astrophysical sources, and study the properties of the waves themselves as tests of…

General Relativity and Quantum Cosmology · Physics 2019-08-15 Alan J. Weinstein

With the new discoveries enabled thanks to the recent space missions, stellar physics is going through a revolution. However, these discoveries opened the door to many new questions that require more observations. The European Space…

Instrumentation and Methods for Astrophysics · Physics 2024-10-28 Savita Mathur , Ângela R. G. Santos

Modern astrophysics is undergoing a revolution. As detector technology has advanced, and astronomers have been able to study the sky with finer temporal detail, a rich diversity of sources which vary on timescales from years down to a few…

High Energy Astrophysical Phenomena · Physics 2018-11-02 D. R. Lorimer

The conventional view of stellar-mass binary black hole (sBBH) mergers is that there should not be enough matter present to produce a detectable electromagnetic transient. However, there ARE a number of mechanisms for producing such a…

High Energy Astrophysical Phenomena · Physics 2019-03-28 K. E. Saavik Ford , Federico Fraschetti , Chris Fryer , Steven L. Liebling , Rosalba Perna , Peter Shawhan , Péter Veres , Bing Zhang

We review some aspects of the current state of data-intensive astronomy, its methods, and some outstanding data analysis challenges. Astronomy is at the forefront of "big data" science, with exponentially growing data volumes and data…

Instrumentation and Methods for Astrophysics · Physics 2014-11-04 G. Longo , M. Brescia , S. G. Djorgovski , S. Cavuoti , C. Donalek

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

Rotating and oscillating neutron stars can give rise to long-lived Continuous Gravitational Waves (CGWs). Despite many years of searching, the detection of such a CGW signal remains elusive. In this article we describe the main…

High Energy Astrophysical Phenomena · Physics 2024-03-05 D. I. Jones , K. Riles

Experience suggests that structural issues in how institutional Astrophysics approaches data-driven science and the development of discovery technology may be hampering the community's ability to respond effectively to a rapidly changing…

Gamma-ray Bursts (GRBs) are relativistic cosmological beacons of transient high energy radiation whose afterglows span the electromagnetic spectrum. Theoretical expectations of correlated neutrino emission position GRBs at an astrophysical…

High Energy Astrophysical Phenomena · Physics 2009-11-05 Michael Stamatikos