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[2] G.C. Agarwal, "Fundamentals of GRB Physics," Academic Press. [3] "Astrophysics of Gamma-Ray Bursts," Academic Resources.

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Understanding GRB Physics: Insights from G.C. Agarwal Gamma-Ray Bursts (GRBs) are the most luminous electromagnetic explosions in the universe, releasing more energy in a few seconds than the Sun will emit over its entire 10-billion-year lifetime. For students studying astrophysics or preparing for competitive entrance exams, comprehensive resources on this subject are crucial.

Gamma-ray bursts are transient flashes of gamma rays lasting from milliseconds to several minutes. They segregate into two broad classes by duration and spectral hardness: short GRBs (<2 s), often associated with compact-object mergers, and long GRBs (>2 s), linked to the collapse of massive stars (collapsars). Both classes release 10^49–10^54 erg in gamma rays, implying an extremely energetic central engine and relativistic motion.