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Astronomy Reports

, Volume 62, Issue 12, pp 905–910 | Cite as

Relativistic Behavior and Equitemporal Surfaces in Ultra-Relativistic Prompt Emission Phase of Gamma-Ray Bursts

  • R. Moradi
  • R. Ruffini
  • C. L. Bianco
  • Y.-C. Chen
  • M. Karlica
  • J. D. Melon Fuksman
  • D. Primorac
  • J. A. Rueda
  • S. Shakeri
  • Y. Wang
  • S. S. Xue
Article
  • 9 Downloads

Abstract

In this work we study a role of baryon load and interstellarmediumdensity to explain the nature of peaks in the ultra-relativistic prompt emission (UPE) phase of Gamma-ray Bursts (GRBs). We study the behavior of their Γ Lorenz factor fromthe moment of transparency all the way up to interstellarmedium. We finally study the characteristic of equitemporal surfaces in the UPE phase.

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Copyright information

© Pleiades Publishing, Ltd. 2018

Authors and Affiliations

  • R. Moradi
    • 1
    • 2
  • R. Ruffini
    • 1
    • 2
  • C. L. Bianco
    • 1
    • 2
  • Y.-C. Chen
    • 1
    • 2
  • M. Karlica
    • 1
    • 2
  • J. D. Melon Fuksman
    • 1
    • 2
  • D. Primorac
    • 1
    • 2
  • J. A. Rueda
    • 1
    • 2
  • S. Shakeri
    • 3
  • Y. Wang
    • 1
    • 2
  • S. S. Xue
    • 1
    • 2
  1. 1.ICRANetPescaraItaly
  2. 2.ICRA and University of Rome “Sapienza”Physics DepartmentRomeItaly
  3. 3.School of AstronomyInstitute for Research in Fundamental Sciences (IPM)TehranIran

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