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Short gamma-ray bursts are associated with binary neutron star mergers, which are multimessenger astronomical events that have been observed both in gravitational waves and in the multiband electromagnetic spectrum. Depending on the masses…

High Energy Astrophysical Phenomena · Physics 2023-01-10 Cecilia Chirenti , Simone Dichiara , Amy Lien , M. Coleman Miller , Robert Preece

Short gamma-ray bursts (GRBs) are explosive transients caused by binary mergers of compact objects containing at least one neutron star. Multi-wavelength afterglow observations provide constraints on the physical parameters of the jet, its…

Recent discovery of the afterglow emission from short gamma-ray bursts suggests that binary neutron star or black hole-neutron star binary mergers are the likely progenitors of these short bursts. The accretion of neutron star material and…

Astrophysics · Physics 2011-02-11 Soebur Razzaque , Peter Meszaros

Double neutron star mergers are strong sources of gravitational waves. The upcoming advanced gravitational wave detectors are expected to make the first detection of gravitational wave bursts (GWBs) associated with these sources. Proposed…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Bing Zhang

The joint detection of gravitational waves (GWs) and $\gamma$-rays from a binary neutron-star (NS) merger provided a unique view of off-axis GRBs and an independent measurement of the NS merger rate. Comparing the observations of GRB170817…

High Energy Astrophysical Phenomena · Physics 2018-12-12 Paz Beniamini , Maria Petropoulou , Rodolfo Barniol Duran , Dimitrios Giannios

We explore the intriguing possibility of employing future ground-based gravitational-wave interferometers to detect the inspiral of binary neutron stars sufficiently early to alert electromagnetic observatories so that a gamma-ray burst…

High Energy Astrophysical Phenomena · Physics 2018-12-18 Sarp Akcay

The progenitors of gamma-ray bursts (GRBs) have long been an unresolved issue. GRB 230307A stands out as an exceptionally bright event, belonging to the long-duration GRBs but also exhibiting a late emission component reminiscent of a…

High Energy Astrophysical Phenomena · Physics 2024-10-01 Junping Chen , Rong-Feng Shen , Wen-Jun Tan , Chen-Wei Wang , Shao-Lin Xiong , Run-Chao Chen , Bin-Bin Zhang

On August 17, 2017 the LIGO-Virgo collaboration detected for the first time gravitational waves from the binary merger of two neutron stars (GW170817). Unlike the merger of two black holes, the associated electromagnetic radiation was also…

Nuclear Theory · Physics 2019-05-01 J. Piekarewicz

Astrophysical transient events like Gamma Ray Bursts (GRBs) have always been promising candidates for multi-messenger astronomy, with electromagnetic and gravitational wave signals having already been observed in GRBs such as GRB 170817A.…

High Energy Astrophysical Phenomena · Physics 2023-08-01 Karlijn Kruiswijk , Gwenhaël de Wasseige

The ANTARES telescope has the opportunity to detect transient neutrino sources, such as gamma-ray bursts (GRBs), core-collapse supernovae (SNe), flares of active galactic nuclei (AGNs)... To enhance the sensitivity to these sources, we are…

The gravitational wave GW170817 from a binary neutron star merger and the simultaneous electromagnetic detection of the GRB170817A by Fermi Gamma-Ray Space Telescope, opened a new era in the multi-messenger astronomy. Furthermore, the GRBs…

High Energy Astrophysical Phenomena · Physics 2024-07-16 Alessandro Drago , Simone Bini , Mariangela Cestelli Guidi , Augusto Marcelli , Valerio Bocci , Emanuele Pace

The recent localization of some short-hard gamma ray bursts (GRBs) in galaxies with low star formation rates has lent support to the suggestion that these events result from compact object binary mergers. We discuss how new simulations in…

Astrophysics · Physics 2009-11-11 Joshua A. Faber , Thomas W. Baumgarte , Stuart L. Shapiro , Keisuke Taniguchi

Gravitational waves from coalescence of a Binary Neutron Star (BNS) and its accompagning short Gamma-Ray Burst GW/GRB~170817A confirmed the presumed origin of these puzzeling transients and opened up the way for relating properties of short…

High Energy Astrophysical Phenomena · Physics 2019-07-23 Houri Ziaeepour

The detection of GW170817 in gravitational waves and gamma rays revealed that short gamma-ray bursts are associated with the merger of neutron-stars. Gamma rays are thought to result from the formation of collimated jets, but the details of…

High Energy Astrophysical Phenomena · Physics 2020-06-10 Amanda Farah , Reed Essick , Zoheyr Doctor , Maya Fishbach , Daniel E. Holz

Based on different neutron star-white dwarf (NS-WD) population models, we investigate the prospects of gravitational-wave (GW) detections for NS-WD mergers, with the help of early warnings from two space-borne decihertz GW observatories,…

High Energy Astrophysical Phenomena · Physics 2024-02-15 Yacheng Kang , Chang Liu , Jin-Ping Zhu , Yong Gao , Lijing Shao , Bing Zhang , Hui Sun , Yi-Han Iris Yin , Bin-Bin Zhang

{\it Fermi}/GBM (Gamma-ray Burst Monitor) and INTEGRAL (the International Gamma-ray Astrophysics Laboratory) reported the detection of the $\gamma$-ray counterpart, GRB 170817A, to the LIGO (Light Interferometer Gravitational-wave…

High Energy Astrophysical Phenomena · Physics 2018-05-16 Gavin P Lamb , Shiho Kobayashi

The collapsar model was proposed to explain the long-duration gamma-ray bursts (GRBs), while the short GRBs are associated with the mergers of compact objects. In the first case, mainly the energetics of the events is consistent with the…

High Energy Astrophysical Phenomena · Physics 2018-05-10 Agnieszka Janiuk , Kostas Sapountzis

The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, the short gamma-ray burst GRB~170817A, heralded the birth of…

High Energy Astrophysical Phenomena · Physics 2026-04-13 S. Abe , J. Abhir , A. Abhishek , F. Acero , A. Acharyya , R. Adam , A. Aguasca-Cabot , I. Agudo , I. Albanese , J. Alfaro , C. Alispach , R. Alves Batista , E. Amato , G. Ambrosi , D. Ambrosino , F. Ambrosino , L. Angel , C. Aramo , A. Arbet-Engels , C. Arcaro , C. Arena , T. T. H. Arnesen , K. Asano , H. Ashkar , C. Bakshi , C. Balazs , M. Balbo , A. Baquero Larriva , V. Barbosa Martins , J. A. Barrio , C. Bartolini , I. Batkovic , R. Batzofin , N. Bavdaz , J. Becerra Gonzalez , G. Beck , W. Benbow , E. Bernardini , M. G. Bernardini , J. Bernete , A. Berti , B. Bertucci , V. Beshley , P. Bhattacharjee , S. Bhattacharyya , C. Bigongiari , A. Biland , E. Bissaldi , M. Bla\ na , O. Blanch , J. Blazek , C. Boisson , G. Bonnoli , Z. Bosnjak , E. Bottacini , M. Bottcher , E. Bronzini , G. Brunelli , J. Buces Saez , A. Bulgarelli , T. Bulik , L. Burmistrov , P. G. Calisse , A. Campoy-Ordaz , B. K. Cantlay , G. Capasso , A. Caproni , R. Capuzzo-Dolcetta , M. Cardillo , S. Caroff , A. Carosi , E. Carquin , S. Casanova , E. Cascone , F. Cassol , G. Castignani , F. Catalani , D. Cerasole , M. Cerruti , P. M. Chadwick , S. Chaty , A. W. Chen , Y. Chen , M. Chernyakova , A. Chiavassa , G. Chon , J. Chudoba , L. Chytka , G. M. Cicciari , A. Cifuentes Santos , C. H. Coimbra Araujo , J. L. Contreras , B. Cornejo , J. Cortina , A. Costa , G. Cotter , P. Cristofari , O. Cuevas , Z. Curtis-Ginsberg , G. D'Amico , F. D'Ammando , P. D'Avanzo , P. Da Vela , L. David , F. Dazzi , M. de Bony de Lavergne , V. De Caprio , E. M. de Gouveia Dal Pino , B. De Lotto , M. de Naurois , V. de Souza , L. del Peral , M. V. del Valle , C. Delgado , D. della Volpe , D. Depaoli , A. Dettlaff , L. Di Bella , T. Di Girolamo , A. Di Piano , F. Di Pierro , R. Di Tria , L. Di Venere , R. Dima , A. Dinesh , E. Do Souto Espiñeira , D. Dominis Prester , A. Donini , D. Dorner , J. Dorner , M. Doro , L. Ducci , V. V. Dwarkadas , J. Ebr , C. Eckner , K. Egberts , L. Eisenberger , D. Elsasser , G. Emery , C. Escanuela Nieves , P. Escarate , M. Escobar Godoy , J. Escudero Pedrosa , P. Esposito , D. Falceta-Goncalves , E. Fedorova , S. Fegan , K. Feijen , Q. Feng , G. Ferrand , E. Fiandrini , A. Fiasson , M. Filipovic , V. Fioretti , L. Foffano , G. Fontaine , Y. Fukazawa , Y. Fukui , G. Galanti , G. Galaz , S. Gallozzi , V. Gammaldi , M. Garczarczyk , C. Gasbarra , D. Gasparrini , M. Gaug , G. Ghirlanda , J. G. Giesbrecht Formiga Paiva , N. Giglietto , F. Giordano , M. Giroletti , R. Giuffrida , J. -F. Glicenstein , P. Goldoni , J. M. Gonzalez , J. Goulart Coelho , T. Gradetzke , J. Granot , R. Grau , D. Green , J. G. Green , J. Grube , J. Hackfeld , D. Hadasch , A. Hahn , P. Hamal , W. Hanlon , S. Hara , V. M. Harvey , T. Hassan , K. Hayashi , L. Heckmann , N. Hiroshima , B. Hnatyk , R. Hnatyk , D. Horan , P. Horvath , D. Hrupec , S. Hussain , M. Iarlori , T. Inada , F. Incardona , S. Inoue , F. Iocco , A. Iuliano , Jahanvi , M. Jamrozy , P. Janecek , F. Jankowsky , C. Jarnot , I. Jaroschewski , P. Jean , V. Jilek , J. Jimenez Quiles , W. Jin , E. Joshi , J. Jurysek , V. Karas , H. Katagiri , J. Kataoka , S. Kaufmann , T. Keita , D. Kerszberg , M. Kherlakian , D. B. Kieda , R. Kissmann , T. Kleiner , Y. Kobayashi , K. Kohri , D. Kolar , N. Komin , A. Kong , K. Kosack , D. Kostunin , G. Kowal , H. Kubo , J. Kushida , A. La Barbera , N. La Palombara , B. Lacave , M. Lainez , A. Lamastra , J. Lapington , S. Lazarevic , J. -P. Lenain , F. Leone , E. Leonora , G. Leto , E. Lindfors , S. Lombardi , F. Longo , R. Lopez-Coto , M. Lopez-Moya , A. Lopez-Oramas , J. Lozano Bahilo , P. L. Luque-Escamilla , E. Lyard , O. Macias , P. Majumdar , M. Makariev , D. Mandat , S. Mangano , A. Marchetti , M. Mariotti , S. Markoff , I. Marquez , G. Marsella , O. Martinez , G. Maurin , D. Mazin , D. Melkumyan , S. Menon , E. Mestre , D. M. -A. Meyer , D. Miceli , M. Miceli , M. Michailidis , T. Miener , J. M. Miranda , R. Moderski , M. Molero , C. Molfese , E. Molina , K. Morik , A. Morselli , E. Moulin , A. L. Muller , K. Munari , T. Murach , A. Muraczewski , H. Muraishi , T. Nakamori , R. Nemmen , J. Niemiec , D. Nieto , M. Nievas Rosillo , L. Nikolic , K. Noda , D. Nosek , V. Novotny , S. Nozaki , A. Okumura , R. A. Ong , R. Orito , M. Orlandini , E. Orlando , S. Orlando , J. Otero-Santos , I. Oya , M. Ozlati Moghadam , A. Pagliaro , M. Palatiello , A. Pandey , G. Panebianco , D. Paneque , F. R. Pantaleo , J. M. Paredes , B. Patricelli , A. Pe'er , M. Pech , M. Pecimotika , M. Peresano , E. Peretti , J. Perez-Romero , G. Peron , F. Perrotta , M. Persic , O. Petruk , F. Pfeifle , E. Pietropaolo , M. Pihet , L. Pinchbeck , F. Pintore , G. Pirola , C. Pittori , F. Podobnik , M. Pohl , V. Pollet , G. Ponti , E. Prandini , G. Principe , M. Prouza , E. Pueschel , G. Puhlhofer , M. L. Pumo , M. Punch , A. Quirrenbach , S. Raino , R. Rando , S. Recchia , A. Reimer , O. Reimer , I. Reis , A. Reisenegger , W. Rhode , M. Ribo , C. Ricci , T. Richtler , J. Rico , L. Riitano , V. Rizi , E. Roache , G. Rodriguez Fernandez , P. Romano , G. Romeo , J. Rosado , A. Rosales de Leon , A. Roy , I. Sadeh , L. Saha , T. Saito , M. Sanchez-Conde , P. Sangiorgi , H. Sano , R. Santos-Lima , V. Sapienza , S. Sarkar , F. G. Saturni , A. Scherer , F. Schiavone , P. Schipani , P. Schovanek , F. Schussler , O. Sergijenko , H. Siejkowski , A. Simongini , V. Sliusar , A. Slowikowska , I. Sofia , H. Sol , S. Spinello , A. Stamerra , T. Starecki , R. Starling , T. Stolarczyk , Y. Suda , A. Sunny , T. Suomijarvi , R. Takeishi , S. J. Tanaka , F. Tavecchio , T. Tavernier , Y. Terada , M. Teshima , V. Testa , W. W. Tian , Y. Tian , L. Tibaldo , O. Tibolla , S. J. Tingay , C. J. Todero Peixoto , F. Tombesi , D. Tonev , F. Torradeflot , D. F. Torres , N. Tothill , G. Tovmassian , G. Tripodo , A. Trois , A. Tsiahina , A. Tutone , L. Vaclavek , M. Vacula , C. van Eldik , J. Vandenbroucke , V. Vassiliev , M. Vazquez Acosta , M. Vecchi , S. Vercellone , S. D. Vergani , I. Viale , A. Viana , A. Vigliano , J. Vignatti , C. F. Vigorito , J. Villanueva , E. Visentin , V. Voitsekhovskyi , S. Vorobiov , I. Vovk , T. Vuillaume , R. Walter , M. Wechakama , M. White , A. Wierzcholska , M. Will , F. Wohlleben , A. Wolter , F. Xotta , T. Yamamoto , R. Yamazaki , T. Yoshikoshi , M. Zacharias , G. Zaharijas , R. Zanmar Sanchez , D. Zavrtanik , M. Zavrtanik , A. Zech , V. I. Zhdanov , J. Zuriaga-Puig

We carried out a systematic search of precursors on the sample of short GRBs observed by Swift. We found that ~8-10% of short GRBs display such early episode of emission. One burst (GRB 090510) shows two precursor events, the former ~13 s…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Eleonora Troja , Stephan Rosswog , Neil Gehrels

Bimodal distribution of the observed duration of gamma-ray bursts (GRBs) has led to two distinct progenitors; compact star mergers, either two neutron stars (NSs) or a NS and a black hole (BH), for short GRBs (SGRBs), and so-called…

High Energy Astrophysical Phenomena · Physics 2023-05-25 Petrosian Vah/'e , Maria Giovanna Dainotti