%0 Journal Article
%T On the Gamma-Ray Bursts Origin
%A A. G. Syromyatnikov
%J International Journal of Astronomy and Astrophysics
%P 425-434
%@ 2161-4725
%D 2016
%I Scientific Research Publishing
%R 10.4236/ijaa.2016.64034
%X <p style=\"margin-left:10.0pt;\">
	<span style=\"font-family:;\" \"=\"\">Gamma-ray (GRBs) and X-ray Bursts are millisecond-10 and 1000 seconds</span><span style=\"font-family:;\" \"=\"\">-</span><span style=\"font-family:;\" \"=\"\">long</span><span style=\"font-family:;\" \"=\"\"> events of unknown origin. Recent simulations of the
merger of binary neutron star <span>systems do not
generate a magnetically dominated called funnel nor a
relativistic</span> outflow. New models for the detection the afterglow of GRB
121024A, measured 0.15 <span>days after the burst,
invoke anisotropy as required to produce the complex</span> micro<span>physics </span><span>of
realistic shocks in relativistic jets</span><span>.
On the other hand the non-thermal</span> gamma-rays are supposed to be produced
by a fireball of relativistic <span style=\"white-space:normal;\">e</span><sup style=\"white-space:normal;\"><span style=\"white-space:nowrap;\">&amp;minus;</span></sup>e<sup>+</sup> pairs that are created
by annihilation of neutrino-antineutrino pairs in the vicinity of the hot,
merged object. It is also known that in a system of a large number of fermions
with pair</span><span style=\"font-family:;\" \"=\"\">s,</span><span style=\"font-family:;\" \"=\"\"> gravitational interaction occur</span><span style=\"font-family:;\" \"=\"\">s</span><span style=\"font-family:;\" \"=\"\"> a spontaneous breaking of the vacuum spatial symmetry, accompanied by
gravitational mass defect. If spherical symmetry is broken, as in the known
case of the merger scenario where a rapidly rotating disk can be formed and
material is pulled away from rotation axis by centrifugal forces, then a
baryon-free funnel along the rotation axes may allow relativistic beam of</span><span style=\"font-family:;\" \"=\"\"> </span><i><span style=\"line-height:99%;font-family:;\" \"=\"\">¦Ã</span></i><span style=\"font-family:;\" \"=\"\">¡¯s and e<sup><span style=\"white-space:nowrap;\">&amp;minus;</span></sup><span>e<sup>+</sup> to escape. It might lead to matter ejection with Lorentz
factors of ~10<sup>2</sup> </span></span><span style=\"font-family:;\" \"=\"\">-</span><span style=\"font-family:;\" \"=\"\"> 10</span><sup><span style=\"font-family:;\" \"=\"\">3</span></sup><span style=\"font-family:;\" \"=\"\"> which are <span>in the
right range to enable copious gamma production during shock interaction</span> with ambient interstellar gas. Here we show that the space rays generation
mechanism on a method of direct transformation of intergalactic gamma-rays to
the proton <span>current on spin shock-waves
%K Gamma-Ray Bursts
%K Spin Density Waves
%K Spin Shock Waves
%K Gravitational Mass  Defect
%U http://www.scirp.org/journal/PaperInformation.aspx?PaperID=72885