Unraveling the Enigma: Exploring the Diverse Facets of Gamma-Ray Burst Emission

A special issue of Galaxies (ISSN 2075-4434).

Deadline for manuscript submissions: 20 September 2024 | Viewed by 110

Special Issue Editor


E-Mail Website
Guest Editor
Department of Physics, Hiroshima University, Hiroshima 739-8526, Japan
Interests: gamma-ray bursts; clusters of galaxies; Cherenkov telescope; galactic center

Special Issue Information

Dear Colleagues,

Gamma-ray bursts (GRBs), the most energetic and mysterious explosions in the universe, continue to captivate the scientific community with their enigmatic origins and profound implications for astrophysics. The aim of this Special Issue is to delve into the forefront of GRB research, shedding light on the diverse aspects of their emission mechanisms, properties, and the profound astrophysical phenomena associated with these high-energy events.

This Special Issue seeks to explore the underlying physics governing the emission processes of GRBs, addressing key questions such as the nature of the progenitor systems, the mechanisms responsible for the extreme energy release, and the interactions with the surrounding environment. We invite contributions that span observational, theoretical, and computational approaches to decipher the intricacies of GRB emissions, aiming to advance our understanding of these cosmic fireworks.

The scope of this issue encompasses a wide array of topics, including but not limited to the identification and characterization of different GRB classes, the role of magnetic fields in the emission process, and the connection between GRBs and other astrophysical phenomena such as supernovae and compact object mergers. We encourage submissions that leverage multi-messenger observations, incorporating data from satellites, ground-based telescopes, and emerging gravitational wave detectors to provide a comprehensive view of GRB events.

Researchers and experts in the field are invited to contribute their latest findings, theories, and observational insights, fostering a collaborative platform for the exchange of ideas and advancements in our quest to unravel the mysteries of GRB emissions. Through this Special Issue, we aim to consolidate the current state of knowledge, identify key challenges, and pave the way for future breakthroughs in understanding the astrophysical processes underlying the emission of gamma-ray bursts.

Dr. Helen Poon
Guest Editor

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Galaxies is an international peer-reviewed open access semimonthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 1400 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • gamma-ray bursts
  • high energy
  • observations
  • theory
  • multiwavelength

Published Papers

This special issue is now open for submission.
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