6,936 research outputs found
Origin of GRB Afterglows in the Model of Galactic Neutron Stars
The launch of the Beppo-Sax satellite gave a unique opportunity to
investigate gamma ray bursts (GRB) in different spectral regions. The large
diversity of the afterglow behavior creates additional problems for the
cosmological model with a fireball. Formation of the afterglow giving the
observed diversity of properties is suggested in the Galactic neutron star
model of GRBs. It is based on the transient accretion disc formation around the
neutron star with a low-mass brown companion irradiated by the neutron star.Comment: Talk at the Workshop "Gamma-Ray Bursts in the Afterglow Era", Rome,
November 3-6. To appear in A&A Supp
High Velocity Neutron Stars as a Result of Asymmetric Neutrino Emission
Formation of a neutron star is accompanied by neutrino emission carring about
10% of the rest energy of the star. Toroidal field produced by twisting of a
dipole field in differentially rotating star is antisymmetric. Its summation
with antisymmetric toroidal field results in braking of mirror symmetry of the
magnetic field . For large magnetic field the neutron decay rate depends on its
strength. Neutrino is emitted more in one direction leading to flux asymmetry
and recoil of the neutron star. Estimations show that the neutron star can
reach velocities km/s for 3% asymmetry of the neutrino flux.Comment: Latex, no figures, 5 page
Gamma Ray Bursts statistical properties and limitations on the physical model
The present common view about GRB origin is related to cosmology. There are
two evidences in favour of this interpretation. The first is connected with
statistics, the second is based on measurements of the redshifts in the GRB
optical afterglows. Red shifts in optical afterglows had been observed only in
long GRB. Statistical errors, and possibility of galactic origin of short GRB
is discussed; their connection with Soft Gamma Repeaters (SGR) is analyzed.Comment: 4 pages, submitted to the Proc. of the XX Texas Symposiu
- …