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We perform a comparative analysis of nucleosynthesis yields from binary neutron star (BNS) mergers, black hole-neutron star (BHNS) mergers, and core-collapse supernovae (CCSNe) with the goal of determining which are the most dominant…

高能天体物理现象 · 物理学 2023-08-30 Nick Ekanger , Mukul Bhattacharya , Shunsaku Horiuchi

Long-duration GRB 211211A, which lacked an associated supernova at such a low redshift $z=0.076$, but was associated with a possible kilonova emission, has attracted great attention. The neutron star-white dwarf (NS-WD) merger is proposed…

高能天体物理现象 · 物理学 2025-07-28 Xiao-Xuan Liu , Hou-Jun Lü , Qiu-Hong Chen , Zhao-Wei Du , En-Wei Liang

Black hole - neutron star (BH-NS) mergers are a major target for ground-based gravitational wave (GW) observatories. A merger can also produce an electromagnetic counterpart (a kilonova) if it ejects neutron-rich matter that assembles into…

高能天体物理现象 · 物理学 2021-08-26 Siva Darbha , Daniel Kasen , Francois Foucart , Daniel J. Price

A kilonova signal is generally expected after a Black Hole - Neutron Star merger. The strength of the signal is related to the equation of state of neutron star matter and it increases with the stiffness of the latter. The recent results…

高能天体物理现象 · 物理学 2022-05-30 Francesco Di Clemente , Alessandro Drago , Giuseppe Pagliara

To date GW170817, produced by a binary neutron star (BNS) merger, is the only gravitational wave event with an electromagnetic (EM) counterpart. It was associated with a prompt short gamma-ray burst (GRB), an optical kilonova, and the…

Black hole-neutron star (BHNS) binaries are amongst promising candidates for the joint detection of electromagnetic (EM) signals with gravitational waves (GWs) and are expected to be detected in the near future. Here we study the effect of…

高能天体物理现象 · 物理学 2021-12-22 Mukul Bhattacharya , Pawan Kumar , George Smoot

We investigate the ability of the Large Synoptic Survey Telescope (LSST) to discover kilonovae (kNe) from binary neutron star (BNS) and neutron star-black hole (NSBH) mergers, focusing on serendipitous detections in the Wide-Fast-Deep (WFD)…

天体物理仪器与方法 · 物理学 2019-02-19 Christian N. Setzer , Rahul Biswas , Hiranya V. Peiris , Stephan Rosswog , Oleg Korobkin , Ryan T. Wollaeger

Mergers of black hole (BH) and neutron star (NS) binaries are expected to be observed by gravitational wave observatories in the coming years. Until now, LIGO has only set an upper limit on this merger rate. BH-NS binaries are expected to…

星系天体物理 · 物理学 2019-05-08 Giacomo Fragione , Abraham Loeb

Rapid identification of the optical counterparts of Neutron Star (NS) merger events discovered by gravitational wave detectors may require observing a large error region and sifting through a large number of transients to identify the…

We report the results of our follow-up campaign for the neutron star - black hole (NSBH) merger GW200115 detected during the O3 run of the Advanced LIGO and Advanced Virgo detectors. We obtained wide-field observations with the Deca-Degree…

We model the formation of black hole-neutron star (BH-NS) binaries via dynamical interactions in globular clusters. We find that in dense, massive clusters, 16-61% of the BH-NS binaries formed by interactions with existing BH binaries will…

高能天体物理现象 · 物理学 2015-06-11 Drew Clausen , Steinn Sigurdsson , David F. Chernoff

Simulations of neutron star-black hole (NSBH) binaries generally consider black holes with masses in the range $(5-10)M_\odot$, where we expect to find most stellar mass black holes. The existence of lower mass black holes, however, cannot…

高能天体物理现象 · 物理学 2019-06-05 F. Foucart , M. D. Duez , L. E. Kidder , S. Nissanke , H. P. Pfeiffer , M. A. Scheel

Within the next few years gravitational waves (GWs) from merging black holes (BHs) and neutron stars (NSs) may be directly detected, making a thorough theoretical understanding of these systems a high priority. As an additional motivation,…

高能天体物理现象 · 物理学 2013-03-08 Branson C. Stephens , William E. East , Frans Pretorius

The detection of a secular post-merger gravitational wave (GW) signal in a binary neutron star (BNS) merger serves as strong evidence for the formation of a long-lived post-merger neutron star (NS), which can help constrain the maximum mass…

广义相对论与量子宇宙学 · 物理学 2023-11-17 Yikang Chen , Bin Liu , Shunke Ai , Lin Lan , He Gao , Yong Yuan , Zong-Hong Zhu

On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. Preliminary analysis of the GW data suggests that the event was likely due to the merger of a compact binary system formed by a BH…

太阳与恒星天体物理 · 物理学 2020-11-11 K. Ackley , L. Amati , C. Barbieri , F. E. Bauer , S. Benetti , M. G. Bernardini , K. Bhirombhakdi , M. T. Botticella , M. Branchesi , E. Brocato , S. H. Bruun , M. Bulla , S. Campana , E. Cappellaro , A. J. Castro-Tirado , K. C. Chambers , S. Chaty , T. -W. Chen , R. Ciolfi , A. Coleiro , C. M. Copperwheat , S. Covino , R. Cutter , F. D'Ammando , P. D'Avanzo , G. De Cesare , V. D'Elia , M. Della Valle , L. Denneau , M. De Pasquale , V. S. Dhillon , M. J. Dyer , N. Elias-Rosa , P. A. Evans , R. A. J. Eyles-Ferris , A. Fiore , M. Fraser , A. S. Fruchter , J. P. U. Fynbo , L. Galbany , C. Gall , D. K. Galloway , F. I. Getman , G. Ghirlanda , J. H. Gillanders , A. Gomboc , B. P. Gompertz , C. González-Fernández , S. González-Gaitán , A. Grado , G. Greco , M. Gromadzki , P. J. Groot , C. P. Gutiérrez , T. Heikkilä , K. E. Heintz , J. Hjorth , Y. -D. Hu , M. E. Huber , C. Inserra , L. Izzo , J. Japelj , A. Jerkstrand , Z. P. Jin , P. G. Jonker , E. Kankare , D. A. Kann , M. Kennedy , S. Kim , S. Klose , E. C. Kool , R. Kotak , H. Kuncarayakti , G. P. Lamb , G. Leloudas , A. J. Levan , F. Longo , T. B. Lowe , J. D. Lyman , E. Magnier , K. Maguire , E. Maiorano , I. Mandel , M. Mapelli , S. Mattila , O. R. McBrien , A. Melandri , M. J. Michałowski , B. Milvang-Jensen , S. Moran , L. Nicastro , M. Nicholl , A. Nicuesa Guelbenzu , L. Nuttal , S. R. Oates , P. T. O'Brien , F. Onori , E. Palazzi , B. Patricelli , A. Perego , M. A. P. Torres , D. A. Perley , E. Pian , G. Pignata , S. Piranomonte , S. Poshyachinda , A. Possenti , M. L. Pumo , J. Quirola-Vásquez , F. Ragosta , G. Ramsay , A. Rau , A. Rest , T. M. Reynolds , S. S. Rosetti , A. Rossi , S. Rosswog , N. B. Sabha , A. Sagués Carracedo , O. S. Salafia , L. Salmon , R. Salvaterra , S. Savaglio , L. Sbordone , P. Schady , P. Schipani , A. S. B. Schultz , T. Schweyer , S. J. Smartt , K. W. Smith , M. Smith , J. Sollerman , S. Srivastav , E. R. Stanway , R. L. C. Starling , D. Steeghs , G. Stratta , C. W. Stubbs , N. R. Tanvir , V. Testa , E. Thrane , J. L. Tonry , M. Turatto , K. Ulaczyk , A. J. van der Horst , S. D. Vergani , N. A. Walton , D. Watson , K. Wiersema , K. Wiik , L. Wyrzykowski , S. Yang , S. -X. Yi , D. R. Young

We present the first effort to aggregate, homogenize, and uniformly model the combined ultraviolet, optical, and near-infrared dataset for the electromagnetic counterpart of the binary neutron star merger GW170817. By assembling all of the…

Short gamma-ray bursts result from mergers of two neutron stars or from collapsars, but probably at a smaller rate. In the first case, a kilonova occurs while in the second case a Type Ic supernova is expected. } {Even if future…

高能天体物理现象 · 物理学 2019-01-29 Nidhal Guessoum , Hannachi Zitouni , Robert Mochkovitch

The historic first joint detection of both gravitational wave and electromagnetic emission from a binary neutron star merger cemented the association between short gamma-ray bursts (SGRBs) and compact object mergers, as well as providing a…

With the forth observing run of the LIGO-Virgo-KAGRA gravitational-wave network, which enabled the discovery of the kilonova (KN) counterpart to GW170817, ending with no new confirmed neutron star mergers, the intrinsic rate of these events…

高能天体物理现象 · 物理学 2026-02-17 Haille M. L. Perkins , Gautham Narayan , Brian D. Fields , Ved G. Shah , Genevieve Schroeder