Relative space-time transformations in GRBs

Details Relative space-time transformations in GRBs Relative space-time transformations in GRBs

2001-06-28

arxiv.org/abs/astro-ph/0106531v1

Astrophys.J. 555 (2001) L107-L111

Astronomy and Astrophysics

Astrophysics

AASTeX, 10 pages, 2 figures, to appear in Ap. J. Lett

Scientific paper

10.1086/323175

The GRB 991216 and its relevant data acquired from the BATSE experiment and RXTE and Chandra satellites are used as a prototypical case to test the theory linking the origin of gamma ray bursts (GRBs) to the process of vacuum polarization occurring during the formation phase of a black hole endowed with electromagnetic structure (EMBH). The relative space-time transformation paradigm (RSTT paradigm) is presented. It relates the observed signals of GRBs to their past light cones, defining the events on the worldline of the source essential for the interpretation of the data. Since GRBs present regimes with unprecedently large Lorentz $\gamma$ factor, also sharply varying with time, particular attention is given to the constitutive equations relating the four time variables: the comoving time, the laboratory time, the arrival time at the detector, duly corrected by the cosmological effects. This paradigm is at the very foundation of any possible interpretation of the data of GRBs.

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