Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...357..161m&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 357, July 1, 1990, p. 161-174. Research supported by the Alfred P. Sloan Fo
Astronomy and Astrophysics
Astrophysics
10
Energy Spectra, Gamma Ray Bursts, Neutron Stars, Plasma Oscillations, Relativistic Plasmas, Stellar Magnetospheres, Compton Effect, Particle Acceleration, Plasma-Particle Interactions, Polar Caps, Thermal Radiation
Scientific paper
Several mechanisms for the primary release of energy in gamma-ray bursts (GRBs) may result in the excitation of relativistic, magnetospheric plasma oscillations above the polar cap of a neutron star. This paper presents a survey of detailed calculations of the inverse Compton scattering interaction between the sinusoidally accelerated particles in relativistic, magnetospheric plasma oscillations and the self-consistently determined thermal radiation from the stellar surface. The upscattered photons are boosted to gamma-ray energies and a Monte Carlo simulation is used to obtain the spectrum for different viewing angles relative to the magnetic field in the oscillating region. It is shown that several GRB spectral characteristics may be understood in the context of a model wherein the overall spectrum changes with aspect angle as a result of the superposition of four components with different angular distributions.
No associations
LandOfFree
Gamma-ray bursts from magnetospheric plasma oscillations. II - Model spectra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Gamma-ray bursts from magnetospheric plasma oscillations. II - Model spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-ray bursts from magnetospheric plasma oscillations. II - Model spectra will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1092488