Resonant Compton scattering in models of gamma-ray burst sources

Conference · Wed Jan 01 04:00:00 EST 1992

OSTI ID:5306209

Vitello, P A

We consider here the spectra produced from the resonant Compton scattering of blackbody and power-law photons by a beam of relativistic electrons/positrons. The beam is assumed to be directed radially outward along the magnetic axis of a highly magnitized neutron star. We assume a dipole magnetic field geometry, and include the effects of magnetic Compton scattering energy losses on the particles in the beam during transport. A range of surface intensities for a magnetic field of 2 {times} 10{sup 12} Gauss are studied for a power-law electron/positron source functions of index {Gamma}. The calculated scattered photon spectra are similar to observed gamma-ray burst spectra with a spectral index {alpha} which breaks from {alpha} {approx equal} 1 to {alpha} {approx equal} {Gamma}.

• Research Organization: Lawrence Livermore National Lab., CA (United States)
• Sponsoring Organization: DOE; USDOE, Washington, DC (United States)
• DOE Contract Number: W-7405-ENG-48
• OSTI ID: 5306209
• Report Number(s): UCRL-JC-110087; CONF-9110310--4; ON: DE92010720
• Country of Publication: United States
• Language: English

Related Subjects

661100 -- Classical & Quantum Mechanics-- (1992-)
661300* -- Other Aspects of Physical Science-- (1992-)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BASIC INTERACTIONS
BEAMS
COMPTON EFFECT
COSMIC GAMMA BURSTS
COSMIC RADIATION
CROSS SECTIONS
DIPOLES
ELASTIC SCATTERING
ELECTROMAGNETIC INTERACTIONS
ELECTRON BEAMS
ENERGY LOSSES
INTERACTIONS
IONIZING RADIATIONS
LEPTON BEAMS
LOSSES
MAGNETIC DIPOLES
MULTIPOLES
NEUTRON STARS
PARTICLE BEAMS
PRIMARY COSMIC RADIATION
RADIATIONS
SCATTERING
STARS