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The early optical afterglow emission of several gamma-ray bursts (GRBs) shows a high linear polarization degree (PD) of tens of percent, suggesting an ordered magnetic field in the emission region. The light curves are consistent with being…

High Energy Astrophysical Phenomena · Physics 2017-08-09 Wei Deng , Bing Zhang , Hui Li , James M. Stone

In this study, the light curves and spectrum of the photospheric thermal radiation from ultrarelativistic gamma-ray burst (GRB) jets are calculated using 2D relativistic hydrodynamic simulations of jets from a collapsar. As the jet…

High Energy Astrophysical Phenomena · Physics 2011-04-13 Akira Mizuta , Shigehiro Nagataki , Junichi Aoi

We report on observations of correlated behavior between the prompt gamma-ray and optical emission from GRB 080319B, which confirm that (i) they occurred within the same astrophysical source region and (ii) their respective radiation…

Astrophysical observations provide a unique opportunity to test possible signatures of Lorentz Invariance Violation (LIV), due to the high energies and long distances involved. In quantum theory of gravity, one may expect the modification…

Cosmology and Nongalactic Astrophysics · Physics 2020-03-04 Yu Pan , Jingzhao Qi , Shuo Cao , Tonghua Liu , Yuting Liu , Shuaibo Geng , Yujie Lian , Zong-Hong Zhu

Gamma-ray bursts (GRBs) are intense pulses of high-energy emission associated with massive stars' death or compact objects' coalescence. Their multi-wavelength observations help verify the reliability of the standard fireball model. We…

High Energy Astrophysical Phenomena · Physics 2024-11-19 M. G. Dainotti , S. Bhardwaj , E. Bissaldi , N. Fraija , S. Sourav , A. Galvan-Gamez

In this paper we examine gamma-ray and optical data of GRB 091024, a gamma-ray burst (GRB) with an extremely long duration of T90~1020 s, as observed with the Fermi Gamma-Ray Burst Monitor (GBM). We present spectral analysis of all three…

In this paper, we propose a novel minimal physical model to elucidate the long-term stochastic variability of blazars. The model is built on the realistic background of magnetized plasma jets dissipating energy through a turbulent cascade…

High Energy Astrophysical Phenomena · Physics 2024-08-06 Nan Ding , Yunyong Tang , Qiusheng Gu , Rui Xue , Yongyun Chen

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…

High Energy Astrophysical Phenomena · Physics 2017-05-03 Paz Beniamini , Dimitrios Giannios

The relative-space-time-transformation (RSTT) paradigm and the interpretation of the burst-structure (IBS) paradigm are applied to probe the origin of the time variability of GRBs. Again GRB 991216 is used as a prototypical case, thanks to…

Astrophysics · Physics 2007-05-23 R. Ruffini , C. L. Bianco , P. Chardonnet , F. Fraschetti , S. -S. Xue

We use a sample of radio-loud active galactic nuclei (AGNs) with measured black hole masses to explore the jet formation mechanisms in these sources. Based on the K\"{o}nigl's inhomogeneous jet model, the jet parameters, such as the bulk…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Bo Chai , Xinwu Cao , Minfeng Gu

Astrophysical models for the high-energy emission of blazars are reviewed. Blazars ejecting relativistic radio jets at small angles to the line-of-sight are the only type of active galactic nuclei (AGN) discovered above 100 MeV. The…

Astrophysics · Physics 2007-05-23 Karl Mannheim

Motivated by GW170817 we examine constraints that observations put on the angular structure of long gamma-ray burst (GRB) jets. First, the relatively narrow observed distribution of $E_{X}/E_{\gamma}$ (the isotropic equivalent early X-ray…

High Energy Astrophysical Phenomena · Physics 2018-12-12 Paz Beniamini , Ehud Nakar

Gamma-ray bursts (GRBs) are classified into long and short populations (i.e., LGRBs and SGRBs) based on the observed bimodal distribution of duration $T_{90}$. Multimessenger observations indicated that most SGRBs and LGRBs should be…

High Energy Astrophysical Phenomena · Physics 2022-09-21 Yun-Feng Wei , Tong Liu

We investigate the nature of the mass-metallicity (M-Z) relation for long gamma-ray burst (LGRB) host galaxies. Recent studies suggest that the M-Z relation for local LGRB host galaxies may be systematically offset towards lower…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Daniel Kocevski , Andrew A. West

Ultrarelativistic jets are believed to play an important role in producing prompt emission and afterglow of gamma-ray bursts (GRBs), but the nature of the jet is poorly known owing to the lack of decisive features observed in the prompt…

High Energy Astrophysical Phenomena · Physics 2024-09-25 Zhen Zhang , Haoxiang Lin , Zhuo Li , Shao-Lin Xiong , Yan-Qiu Zhang , Qinyuan Zhang , Shu-Xu Yi , Xilu Wang

We constrain the possibility of a non-trivial refractive index in free space corresponding to an energy-dependent velocity of light: c(E) \simeq c_0 (1 - E/M), where M is a mass scale that might represent effect of quantum-gravitational…

The nature of the central engines of gamma-ray bursts (GRBs) and the composition of their relativistic jets are still under debate. If the jets are Poynting flux dominated rather than baryon dominated, a coherent radio flare from magnetic…

Gamma-ray astronomy has become one of the main experimental ways to test the modified dispersion relations (MDRs) of photons in vacuum, obtained in some attempts to formulate a theory of Quantum Gravity. The MDRs in use imply time delays…

High Energy Astrophysical Phenomena · Physics 2022-05-11 J. Bolmont , S. Caroff , M. Gaug , A. Gent , A. Jacholkowska , D. Kerszberg , C. Levy , T. Lin , M. Martinez , L. Nogues , A. N. Otte , C. Perennes , M. Ronco , T. Terzić

Gamma-ray bursts (GRBs) are bright extragalactic flashes of gamma-ray radiation and briefly the most energetic explosions in the Universe. Their catastrophic origin (the merger of compact objects or the collapse of massive stars) drives the…

The essence of the ``Supercritical Pile'' model is a process for converting the energy stored in the relativistic protons of a Relativistic Blast Wave (RBW) of Lorentz factor $\Gamma$ into electron -- positron pairs of similar Lorentz…

Astrophysics · Physics 2009-11-10 Demosthenes Kazanas , Markos Georganopoulos , Apostolos Mastichiadis