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Related papers: Kilonova and Optical Afterglow from Binary Neutron…

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In this letter we focus on the peculiar case of a coalescing compact-object binary whose chirp mass is compatible both with a neutron star-neutron star and black hole-neutron star system, with the black hole in the $\sim 3-5M_\odot$ range…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Claudio Barbieri , Om Sharan Salafia , Monica Colpi , Giancarlo Ghirlanda , Albino Perego , Alberto Colombo

Current and future optical and near-infrared wide-field surveys have the potential of finding kilonovae, the optical and infrared counterparts to neutron star mergers, independently of gravitational-wave or high-energy gamma-ray burst…

The gamma-ray burst that followed the first detection of gravitational waves from the merger of a Binary Neutron Stars and its low energy counterparts were in many respects unusual and challenge our understanding of mechanisms involved in…

High Energy Astrophysical Phenomena · Physics 2018-11-20 Houri Ziaeepour

Kilonovae (KNe) are one of the fastest types of optical transients known, cooling rapidly in the first few days following their neutron-star merger origin. We show here that KN spectral features go through rapid recombination transitions,…

High Energy Astrophysical Phenomena · Physics 2024-08-14 Albert Sneppen , Darach Watson , James H. Gillanders , Kasper E. Heintz

Mergers of black hole-neutron star (BHNS) binaries have now been observed by GW detectors with the recent announcement of GW200105 and GW200115. Such observations not only provide confirmation that these systems exist, but will also give…

Recent observations indicate that in a large fraction of binary neutron star (BNS) mergers a long-lived neutron star (NS) may be formed rather than a black hole. Unambiguous electromagnetic (EM) signatures of such a scenario would strongly…

High Energy Astrophysical Phenomena · Physics 2016-03-16 Daniel M. Siegel , Riccardo Ciolfi

We present UV, optical, and NIR photometry of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo, the binary neutron star merger GW170817. Our data set extends from the discovery of the optical…

High Energy Astrophysical Phenomena · Physics 2017-10-17 P. S. Cowperthwaite , E. Berger , V. A. Villar , B. D. Metzger , M. Nicholl , R. Chornock , P. K. Blanchard , W. Fong , R. Margutti , M. Soares-Santos , K. D. Alexander , S. Allam , J. Annis , D. Brout , D. A. Brown , R. E. Butler , H. -Y. Chen , H. T. Diehl , Z. Doctor , M. R. Drout , T. Eftekhari , B. Farr , D. A. Finley , R. J. Foley , J. A. Frieman , C. L. Fryer , J. García-Bellido , M. S. S. Gill , J. Guillochon , K. Herner , D. E. Holz , D. Kasen , R. Kessler , J. Marriner , T. Matheson , E. H. Neilsen, , E. Quataert , A. Palmese , A. Rest , M. Sako , D. M. Scolnic , N. Smith , D. L. Tucker , P. K. G. Williams , E. Balbinot , J. L. Carlin , E. R. Cook , F. Durret , T. S. Li , P. A. A. Lopes , A. C. C. Lourenço , J. L. Marshall , G. E. Medina , J. Muir , R. R. Muñoz , M. Sauseda , D. J. Schlegel , L. F. Secco , A. K. Vivas , W. Wester , A. Zenteno , Y. Zhang , T. M. C. Abbott , M. Banerji , K. Bechtol , A. Benoit-Lévy , E. Bertin , E. Buckley-Geer , D. L. Burke , D. Capozzi , A. Carnero Rosell , M. Carrasco Kind , F. J. Castander , M. Crocce , C. E. Cunha , C. B. D'Andrea , L. N. da Costa , C. Davis , D. L. DePoy , S. Desai , J. P. Dietrich , A. Drlica-Wagner , T. F. Eifler , A. E. Evrard , E. Fernandez , B. Flaugher , P. Fosalba , E. Gaztanaga , D. W. Gerdes , T. Giannantonio , D. A. Goldstein , D. Gruen , R. A. Gruendl , G. Gutierrez , K. Honscheid , B. Jain , D. J. James , T. Jeltema , M. W. G. Johnson , M. D. Johnson , S. Kent , E. Krause , R. Kron , K. Kuehn , N. Kuropatkin , O. Lahav , M. Lima , H. Lin , M. A. G. Maia , M. March , P. Martini , R. G. McMahon , F. Menanteau , C. J. Miller , R. Miquel , J. J. Mohr , E. Neilsen , R. C. Nichol , R. L. C. Ogando , A. A. Plazas , N. Roe , A. K. Romer , A. Roodman , E. S. Rykoff , E. Sanchez , V. Scarpine , R. Schindler , M. Schubnell , I. Sevilla-Noarbe , M. Smith , R. C. Smith , F. Sobreira , E. Suchyta , M. E. C. Swanson , G. Tarle , D. Thomas , R. C. Thomas , M. A. Troxel , V. Vikram , A. R. Walker , R. H. Wechsler , J. Weller , B. Yanny , J. Zuntz

GRB 160821B is a short duration gamma-ray burst (GRB) detected and localized by the Neil Gehrels Swift Observatory in the outskirts of a spiral galaxy at z=0.1613, at a projected physical offset of 16 kpc from the galaxy's center. We…

The detection of the binary neutron star merger GW170817 and the associated electromagnetic (EM) counterpart, the "kilonova" (kN) AT2017gfo, opened a new era in multi-messenger astronomy. However, despite many efforts, it has been proven…

High Energy Astrophysical Phenomena · Physics 2021-05-26 A. Sagués Carracedo , M. Bulla , U. Feindt , A. Goobar

We predict linear polarization for a radioactively-powered kilonova following the merger of a black hole and a neutron star. Specifically, we perform 3-D Monte Carlo radiative transfer simulations for two different models, both featuring a…

High Energy Astrophysical Phenomena · Physics 2020-12-16 M. Bulla , K. Kyutoku , M. Tanaka , S. Covino , J. R. Bruten , T. Matsumoto , J. R. Maund , V. Testa , K. Wiersema

The ongoing LIGO-Virgo-KAGRA observing run O4 provides an opportunity to discover new multi-messenger events, including binary neutron star (BNS) mergers such as GW170817, and the highly anticipated first detection of a multi-messenger…

We investigate $r$-process nucleosynthesis and kilonova emission resulting from binary neutron star (BNS) mergers based on a three-dimensional (3D) general-relativistic magnetohydrodynamic (GRMHD) simulation of a hypermassive neutron star…

High Energy Astrophysical Phenomena · Physics 2022-11-16 Sanjana Curtis , Philipp Mösta , Zhenyu Wu , David Radice , Luke Roberts , Giacomo Ricigliano , Albino Perego

Detections of gravitational waves (GWs) may soon uncover the signal from the coalescence of a black hole - neutron star (BHNS) binary, that is expected to be accompanied by an electromagnetic (EM) signal. In this paper, we present a…

High Energy Astrophysical Phenomena · Physics 2020-01-29 C. Barbieri , O. S. Salafia , A. Perego , M. Colpi , G. Ghirlanda

Ejected material from neutron star mergers give rise to electromagnetic emission powered by radioactive decays of r-process nuclei, which is so called kilonova or macronova. While properties of the emission are largely affected by opacities…

The detection of GW170817 and the accompanying electromagnetic counterpart, AT2017gfo, have provided an important set of observational constraints for theoretical models of neutron star mergers, nucleosynthesis, and radiative transfer for…

The multi-messenger detection of GW170817 showed that binary neutron star (BNS) mergers are progenitors of (at least some) short gamma-ray bursts (GRBs), and that short GRB jets (and their afterglows) can have structures (and observational…

High Energy Astrophysical Phenomena · Physics 2023-07-04 Avery Eddins , Kyung-hwan Lee , Alessandra Corsi , Imre Bartos , Zsuzsanna Marka , Szabolcs Marka

We present optical spectra and light curves for three hydrogen-poor super-luminous supernovae followed by the Public ESO Spectroscopic Survey of Transient Objects (PESSTO). Time series spectroscopy from a few days after maximum light to 100…

Short gamma-ray burst (SGRB) GRB 170817A was found to be related to a binary neutron star (BNS) merger. It is uncertain whether all SGRBs are caused by BNS mergers, and also under what conditions a BNS merger can cause a SGRB. As BNS…

High Energy Astrophysical Phenomena · Physics 2022-04-06 Minori Shikauchi , Kipp Cannon , Haoxiang Lin , Tomonori Totani , J. Richard Shaw

The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of gamma-rays, a gravitational wave signal, and a transient optical/near-infrared source powered by the synthesis of large amounts…