AN UPSCATTERING SPECTRAL FORMATION MODEL FOR THE PROMPT EMISSION OF GAMMA-RAY BURSTS

Journal Article · Wed Jun 20 04:00:00 EDT 2012 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/752/2/116· OSTI ID:22037022

Titarchuk, Lev; Farinelli, Ruben; Frontera, Filippo ^[1]; Amati, Lorenzo ^[2]

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1. Dipartimento di Fisica, Universita di Ferrara, Via Saragat 1, 44122 Ferrara (Italy)
2. INAF-IASF Bologna, Via Gobetti 101, 40129 Bologna (Italy)

We propose a model for the spectral formation of gamma-ray burst (GRB) prompt emission, where the phenomenological Band function is usually applied to describe this emission. We suggest that the GRB prompt emission is mainly a result of two upscattering processes. The first process is the Comptonization of relatively cold soft photons of the star off electrons of a hot shell of plasma of temperature T{sub e} of the order of 10{sup 9} K (or kT{sub e} {approx} 100 keV) that moves subrelativistically with the bulk velocity V{sub b} substantially less than the speed of light c. In this phase, the Comptonization parameter Y is high and the interaction between a blackbody-like soft seed photon population and hot electrons leads to formation of a saturated Comptonization spectrum modified by the subrelativistic bulk outflow. The second process is an upscattering of the previously Comptonized spectrum by the plasma outflow once it becomes relativistic. This process gives rise to the high-energy power-law (PL) component above the peak in the EF(E) diagram where F(E) is the energy flux. The latter process can be described by a convolution of the Comptonized spectrum with a broken-PL Green function. Possible physical scenarios for this second upscattering process are discussed. In the framework of our model, we give an interpretation of the Amati relation between the intrinsic spectral peak photon energy and radiated energy or luminosity, and we propose a possible explanation of the GRB temporal variability.

• OSTI ID: 22037022
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 752; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ASTROPHYSICS
COSMIC ELECTRONS
COSMIC GAMMA BURSTS
COSMIC PHOTONS
ELECTRON TEMPERATURE
EMISSION SPECTRA
GAMMA ASTRONOMY
GAMMA SPECTRA
GREEN FUNCTION
KEV RANGE
LUMINOSITY
PHOTON EMISSION
RADIANT HEAT TRANSFER
RELATIVISTIC RANGE