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相关论文: Gravitational Wave Memory from the Relativistic Je…

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Gravitational wave (GW) memory, a permanent distortion of the space-time metric, is anticipated during the acceleration of relativistic jets in gamma-ray bursts (GRBs). While the precise mechanism behind GRBs is not yet fully understood,…

高能天体物理现象 · 物理学 2025-09-23 Yusuke Sakai , Ryo Yamazaki , Yoshihiro Okutani , Satsuki Ueno , Norichika Sago , Marco Meyer-Conde , Hirotaka Takahashi

Gamma-Ray Bursts (GRBs) are now considered as relativistic jets. We analyze the gravitational waves from the acceleration stage of the GRB jets. We show that (i) the point mass approximation is not appropriate if the opening half-angle of…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Norichika Sago , Kunihito Ioka , Takashi Nakamura , Ryo Yamazaki

Ultrarelativistic gamma-ray burst (GRB) jets are strong gravitational wave (GW) sources with memory-type signals. The plateau (or shallow decay) phases driven by the energy injection might appear in the early X-ray afterglows of GRBs. In…

高能天体物理现象 · 物理学 2023-03-08 Bao-Quan Huang , Tong Liu , Li Xue , Yan-Qing Qi

We discuss the gravitational wave background (GWB) from a cosmological population of gamma-ray bursts (GRBs). Among various emission mechanisms for the gravitational waves (GWs), we pay a particular attention to the vast anisotropic…

天体物理学 · 物理学 2009-11-13 Takashi Hiramatsu , Kei Kotake , Hideaki Kudoh , Atsushi Taruya

We study the gravitational wave (GW) production induced by the asymmetric jets of gamma-ray bursts (GRBs). The asymmetric jets result in a recoil force acted on the central compact object, whose motion leads to emission of GW. Under…

高能天体物理现象 · 物理学 2018-07-25 Shuang Du , Xiao-Dong Li , Yi-Ming Hu , Fang-Kun Peng , Miao Li

It is believed that the relativistic jets of gamma-ray bursts (GRBs) should initially propagate through a heavy envelope of the massive progenitor stars or through a merger ejecta formed from the compact binary mergers. The interaction of a…

高能天体物理现象 · 物理学 2020-09-09 Yun-Wei Yu

We focus on understanding the beaming of gravitational radiation from gamma ray bursts (GRBs) by approximating GRBs as linearly accelerated point masses. For accelerated point masses, it is known that gravitational radiation is beamed…

高能天体物理现象 · 物理学 2016-10-03 Andrew L. Miller , Thulsi Wickramasinghe

Gravitational waves (GWs) produce small distortions in the observable distribution of stars in the sky. We describe the characteristic pattern of astrometric deflections created by a specific gravitational waveform called a burst with…

广义相对论与量子宇宙学 · 物理学 2020-07-27 Dustin R. Madison

While the possible roles of GRBs' progenitors as Gravitational Waves (GW) sources have been extensively studied, little attention has been given to the jet itself as a GW source. We expect the jet's acceleration to produce a GW Memory…

高能天体物理现象 · 物理学 2014-01-21 Ofek Birnholtz , Tsvi Piran

Gamma-ray Bursts (GRBs) are bursts of $\gamma$-rays generated from relativistic jets launched from catastrophic events such as massive star core collapse or binary compact star coalescence. Previous studies suggested that GRB emission is…

高能天体物理现象 · 物理学 2016-03-29 Bin-Bin Zhang , Bing Zhang , Alberto J. Castro-Tirado

Gravitational-wave memory is a low-frequency, non-oscillatory signal that provides a promising probe of strong-field gravity. We present the first computation of memory from full inspiral--merger--ringdown waveforms in a theory beyond GR,…

广义相对论与量子宇宙学 · 物理学 2026-05-11 Silvia Gasparotto

The acceleration of a jet to relativistic velocities produces a unique memory type gravitational waves (GW) signal: {\it Jet-GW}. I discuss here resent result concerning properties of these GWs and consider their detectability in current…

高能天体物理现象 · 物理学 2022-10-07 Tsvi Piran

Non-spherical rapid acceleration of mass (or energy) to a relativistic velocity is a natural source of gravitational radiation. Such conditions arise in both long and short gamma-ray bursts whose central engine ejects relativistic jets. The…

高能天体物理现象 · 物理学 2021-11-10 Elly Leiderschneider , Tsvi Piran

We study the motion of a gyroscope located far away from an isolated gravitational source in an asymptotically flat spacetime. As seen from a local frame tied to distant stars, the gyroscope precesses when gravitational waves cross its…

高能物理 - 理论 · 物理学 2023-11-10 Ali Seraj , Blagoje Oblak

We provide a comprehensive review of major developments in our understanding of gamma-ray bursts, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered. We describe the…

高能天体物理现象 · 物理学 2015-06-03 Pawan Kumar , Bing Zhang

We considered a model for the prompt phase of Gamma-Ray Burst (GRB) emission arising from a magnetized jet undergoing gradual energy dissipation due to magnetic reconnection. The dissipated magnetic energy is translated to bulk kinetic…

高能天体物理现象 · 物理学 2017-05-03 Paz Beniamini , Dimitrios Giannios

Nonlinear gravitational wave memory is a surprise of theoretical physics. Whereas it is understood that a gravitational wave induces oscillatory squeezing and stretching motion in a collection of freely-falling test masses, it is unexpected…

广义相对论与量子宇宙学 · 物理学 2025-06-27 Robert R. Caldwell

Gamma ray bursts (GRBs) are short and intense pulses of $\gamma$-rays arriving from random directions in the sky. Several years ago Amelino-Camelia et al. pointed out that a comparison of time of arrival of photons at different energies…

天体物理学 · 物理学 2009-11-10 Tsvi Piran

In this article, we examine entangled quantum probes in geodesic trajectories in a flat background with a gravitational wave (GW) burst. In particular, these quantum probes are prepared initially either in the symmetric or anti-symmetric…

广义相对论与量子宇宙学 · 物理学 2025-01-30 Subhajit Barman , Indranil Chakraborty , Sajal Mukherjee

The detectability of gravitational wave (GW) radiation from accretion disks is discussed based on various astrophysical contexts. In order to emit GW radiation, the disk shape should lose axial symmetry. We point out that a significant…

天体物理学 · 物理学 2015-06-24 S. Mineshige , T. Hosokawa , M. Machida , R. Matsumoto
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