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Gamma-Ray Bursts

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arxiv astro-ph/0605208 v5 pith:PYX5RIN5 submitted 2006-05-09 astro-ph hep-ph

P. Meszaros This is my paper · ORCID
classification astro-phhep-ph
keywords burstsgamma-rayafterglowbreakthroughsburstdebatedecadesdiscovery
verification ladder T0 review T1 audit T2 compute T3 formal

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Gamma-ray bursts are the most luminous explosions in the Universe, and their origin and mechanism are the focus of intense research and debate. More than three decades after their discovery, and after pioneering breakthroughs from space and ground experiments, their study is entering a new phase with the recently launched Swift satellite. The interplay between these observations and theoretical models of the prompt gamma ray burst and its afterglow is reviewed.

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Cited by 13 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Time varying polarized gamma-rays from GRB 160821A: evidence for ordered magnetic fields

    astro-ph.HE 2019-08 conditional novelty 8.0 of 10

    GRB 160821A shows 66% linear polarization that changes its angle twice, implying ordered magnetic fields in the gamma-ray burst jet.

  2. Detectability of Gravitational-wave counterparts of EP-FXTs observed during the O4b LIGO-Virgo-KAGRA Observing Run

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    No gravitational-wave counterpart is statistically associated with any of 47 Einstein Probe fast X-ray transients in the O4b run; 90% exclusion distances of ~178 Mpc (BNS) and ~349 Mpc (NSBH) disfavor nearby compact-b...

  3. Ultra high-energy cosmic rays from relativistic outflows in accretion induced collapse of white dwarfs

    astro-ph.HE 2026-05 unverdicted novelty 6.0 of 10

    Relativistic outflows in accretion-induced collapse of white dwarfs are modeled as sources of UHECRs, contributing a few 10^43-10^45 erg Mpc^{-3} yr^{-1} assuming iron-like nuclei and sufficient event rates.

  4. Carpet-3 detection of a photon-like air shower with estimated primary energy above 100 TeV in a spatial and temporal coincidence with GRB 221009A

    astro-ph.HE 2025-02 conditional novelty 6.0 of 10

    Carpet-3 reports a photon-like air shower with estimated energy around 300 TeV arriving from the direction of GRB 221009A about 75 minutes after the trigger, with a coincidence probability of about 0.9 percent.

  5. Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH

    astro-ph.HE 2019-09 conditional novelty 6.0 of 10

    Neutrino self-interactions inside neutrino-cooled accretion disks are argued to push flavors toward equipartition, reducing the neutrino-antineutrino annihilation energy deposition around black holes by a factor up to...

  6. Early Multiwavelength Observations of AT 2026fgk: The Luminous Afterglow to Sub-luminous GRB 260310A, Identified Independently of a Gamma-ray Trigger

    astro-ph.HE 2026-06 accept novelty 5.0 of 10

    First blind optical identification of a z=0.153 sub-luminous GRB afterglow with Ic-BL SN, yielding a volumetric rate consistent with on-axis high-luminosity long GRBs.

  7. Trapped fireshell (halo) of photons and pairs around black-hole horizon: source for ultra-high-energy particles

    astro-ph.HE 2025-12 reject novelty 5.0 of 10

    The paper predicts a Klein-Nishina 'runaway' that accelerates electrons and protons to ultra-high energies inside a gravitationally trapped photon-pair halo, with a time-declining UHE luminosity.

  8. Picolensing as a Probe of Primordial Black Hole Dark Matter

    astro-ph.HE 2024-11 conditional novelty 5.0 of 10

    Asteroid-mass primordial black hole dark matter could be probed by picolensing of gamma-ray bursts, but only with detector separations of at least Earth-L2 distance once realistic GRB size uncertainties are included.

  9. Extending the Comisso-Asenjo Energy Extraction Mechanism to Pure Lovelock Gravity

    gr-qc 2026-07 conditional novelty 4.0 of 10

    For rotating pure Lovelock black holes in 6–9 dimensions, magnetic reconnection extracts more rotational energy as dimension grows, with the 9-dimensional case most efficient and sometimes outpacing the Blandford-Znaj...

  10. Short-duration gamma-ray bursts from Kerr-Newman black hole mergers

    astro-ph.HE 2024-11 reject novelty 4.0 of 10

    A Kerr-Newman black hole produced by a binary black hole merger, with a magnetized disk, can power a short gamma-ray burst via the Blandford-Znajek mechanism, and the model is applied to GW150914.

  11. The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range

    gr-qc 2019-08 accept novelty 3.0 of 10

    A Decihertz Observatory would fill the gap between LISA and ground detectors, enabling early-warning multimessenger astronomy and measurements of intermediate-mass black hole populations.

  12. Early Optical Follow-up of Gamma-Ray Bursts: The Critical Role of Robotic Telescopes

    astro-ph.HE 2026-06 unverdicted novelty 2.0 of 10

    A review of early optical GRB features including prompt emission, reverse shocks, and afterglow onset, highlighting robotic telescopes' role in constraining jet Lorentz factors and magnetization.

  13. A review of long lasting activities of the central engine of gamma-ray bursts

    astro-ph.HE 2025-01 unverdicted novelty 1.0 of 10

    A review of ultra-long gamma-ray bursts and X-ray plateau phases as evidence that the central engine keeps working long after the first flash.

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