3 research outputs found
Gamma ray bursts from superconducting cosmic strings
Cusps of superconducting strings can serve as GRB engines. A powerful beamed
pulse of electromagnetic radiation from a cusp produces a jet of accelerated
particles, whose propagation is terminated by the shock responsible for GRB. A
single free parameter, the string scale of symmetry breaking , together with reasonable assumptions about the magnitude of cosmic
magnetic fields and the fraction of volume that they occupy, explains the GRB
rate, duration and fluence, as well as the observed ranges of these quantities.
The wiggles on the string can drive the short-time structures of GRB. This
model predicts that GRBs are accompanied by strong bursts of gravitational
radiation which should be detectable by LIGO, VIRGO and LISA detectors. Another
prediction is the diffuse X- and gamma-ray radiation at 8 MeV - 100 GeV with a
spectrum and flux comparable to the observed. The weakness of the model is the
prediction of too low rate of GRBs from galaxies, as compared with
observations. This suggests that either the capture rate of string loops by
galaxies is underestimated in our model, or that GRBs from cusps are
responsible for only a subset of the observed GRBs not associated with
galaxies.Comment: 29 pages, Revtex. This is a substantially expanded and revised
version of our earlier paper astro-ph/0001213. Final version, to appear in
Phys. Rev.