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相关论文: Radio precursors to neutron star binary mergings

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We discuss possible radio bursts which can be generated during binary neutron stars mergers associated with short gamma-ray bursts. Low-frequency radio band appear to be advantageous due to the time delay of a radio signal propagating in…

高能天体物理现象 · 物理学 2010-04-30 K. A. Postnov , M. S. Pshirkov

LOFAR, the Low Frequency Array, is an innovative new radio telescope currently under construction in the Netherlands. With its continuous monitoring of the radio sky we expect LOFAR will detect many new transient events, including GRB…

天体物理仪器与方法 · 物理学 2011-03-28 Joeri van Leeuwen , The LOFAR Transients Key Science Project

The prompt emission in long gamma-ray bursts arises from within relativistic outflows created during the collapse of massive stars, and the mechanism by which radiation is produced may be either magnetically- or matter-dominated. In this…

高能天体物理现象 · 物理学 2020-05-06 R. L. C. Starling , . A. Rowlinson , A. J. van der Horst , R. A. M. J. Wijers

Both observational and theoretical rates of binary neutron star coalescence give low prospects for detection of a single event by the initial LIGO/VIRGO interferometers. However, by utilizing at the best all the a priori information on the…

天体物理学 · 物理学 2007-05-23 S. Bonazzola , E. Gourgoulhon

We describe the possible electromagnetic signals expected from the magnetospheric interactions of a neutron star binary prior to merger. We find that both radio and X-ray signals of detectable strength are possible. We discuss possible…

天体物理学 · 物理学 2009-10-31 Brad M. S. Hansen , Maxim Lyutikov

The first detection of a binary neutron star merger, GW170817, and an associated short gamma-ray burst confirmed that neutron star mergers are responsible for at least some of these bursts. The prompt gamma ray emission from these events is…

高能天体物理现象 · 物理学 2018-05-11 Daniel Williams , James A. Clark , Andrew R. Williamson , Ik Siong Heng

The composition of relativistic gamma-ray burst (GRB) jets and their emission mechanisms are still debated, and they could be matter or magnetically dominated. One way to distinguish these mechanisms arises because a Poynting flux dominated…

Observations of short gamma-ray bursts indicate ongoing energy injection following the prompt emission, with the most likely candidate being the birth of a rapidly rotating, highly magnetised neutron star. We utilise X-ray observations of…

高能天体物理现象 · 物理学 2016-03-09 Paul D Lasky , Kostas Glampedakis

Fast radio bursts (FRBs) at cosmological distances have recently been discovered, whose duration is about milliseconds. We argue that the observed short duration is difficult to explain by giant flares of soft gamma-ray repeaters, though…

高能天体物理现象 · 物理学 2015-06-16 Tomonori Totani

We discuss a multimessenger strategy to detect radio pulses from Galactic binary neutron stars in a very tight orbit with the period shorter than 10 min. On one hand, all-sky surveys by radio instruments are inefficient for detecting faint…

高能天体物理现象 · 物理学 2018-12-31 Koutarou Kyutoku , Yuki Nishino , Naoki Seto

As a new kind of radio transient sources detected at $\sim 1.4$ GHz, fast radio bursts are specially characterized by their short durations and high intensities. Although only ten events are detected so far, fast radio bursts may actually…

高能天体物理现象 · 物理学 2015-12-22 Y. F. Huang , J. J. Geng

Fast radio bursts are mysterious millisecond-duration transients prevalent in the radio sky. Rapid accumulation of data in recent years has facilitated an understanding of the underlying physical mechanisms of these events. Knowledge gained…

高能天体物理现象 · 物理学 2020-11-11 Bing Zhang

The multi-messenger observation of gamma-ray burst (GRB)\,170817A from the nearby binary neutron-star merger GW170817 demonstrated that low-energy $\gamma$-ray emission can be observed at relatively large angles from GRB jet axes. If such…

高能天体物理现象 · 物理学 2019-03-20 Imre Bartos , Kyung-hwan Lee , Alessandra Corsi , Zsuzsa Marka , Szabolcs Marka

It is an open question whether and how gravitational wave events involving neutron stars can be preceded by electromagnetic counterparts. This work shows that the collision of two neutron stars with magnetic fields well below magnetar-level…

高能天体物理现象 · 物理学 2023-06-21 Elias R. Most , Alexander A. Philippov

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…

高能天体物理现象 · 物理学 2023-01-10 Cecilia Chirenti , Simone Dichiara , Amy Lien , M. Coleman Miller , Robert Preece

Coalescing neutron star binaries are believed to be the most reliable sources for ground-based detectors of gravitational waves and likely progenitors of short gamma-ray bursts. In the process of coalescence, magnetic fields of neutron…

高能天体物理现象 · 物理学 2015-05-14 K. A. Postnov , A. G. Kuranov

We investigate pre-merger coherent radio emission from neutron star mergers arising due to the magnetospheric interaction between compact objects. We consider two plausible radiation mechanisms, and show that if one neutron star has a…

高能天体物理现象 · 物理学 2022-12-21 A. J. Cooper , O. Gupta , Z. Wadiasingh , R. A. M. J. Wijers , O. M. Boersma , I. Andreoni , A. Rowlinson , K. Gourdji

The LOw FRequency ARray - LOFAR is a new radio telescope that is moving the science of radio pulsars and transients into a new phase. Its design places emphasis on digital hardware and flexible software instead of mechanical solutions.…

天体物理仪器与方法 · 物理学 2012-07-03 Maciej Serylak , Aris Karastergiou , Chris Williams , Wes Armour , LOFAR Pulsar Working Group

As evidenced by the coincident detections of GW170817 and GRB 170817A, short gamma-ray bursts are likely associated with neutron star-neutron star merger events. Although rare, some bursts display episodes of early emission, with precursor…

高能天体物理现象 · 物理学 2020-04-15 Arthur G. Suvorov , Kostas D. Kokkotas

The merger of a neutron star binary may result in the formation of a rapidly-spinning magnetar. The magnetar can potentially survive for seconds or longer as a supramassive neutron star before collapsing to a black hole if, indeed, it…

高能天体物理现象 · 物理学 2016-11-09 Wen-fai Fong , Brian D. Metzger , Edo Berger , Feryal Ozel
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