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Wiersema, K., Covino, S., Toma, K., van der Horst, A.J., et al. (2014) Circular Polarization in the Optical Afterglow of GRB 121024A. Nature, 509, 201-204.
https://doi.org/10.1038/nature13237

has been cited by the following article:

  • TITLE: On the Gamma-Ray Bursts Origin

    AUTHORS: A. G. Syromyatnikov

    KEYWORDS: Gamma-Ray Bursts, Spin Density Waves, Spin Shock Waves, Gravitational Mass Defect

    JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.6 No.4, December 21, 2016

    ABSTRACT: Gamma-ray (GRBs) and X-ray Bursts are millisecond-10 and 1000 seconds-longevents of unknown origin. Recent simulations of the merger of binary neutron starsystems do not generate a magnetically dominated called funnel nor a relativisticoutflow. New models for the detection the afterglow of GRB 121024A, measured 0.15days after the burst, invoke anisotropy as required to produce the complexmicrophysicsof realistic shocks in relativistic jets. On the other hand the non-thermalgamma-rays are supposed to be produced by a fireball of relativistice?e+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 pairs,gravitational interaction occursa 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 ofγ’s and e?e+to escape. It might lead to matter ejection with Lorentz factors of ~102-103which arein the right range to enable copious gamma production during shock interactionwith ambient interstellar gas. Here we show that the space rays generation mechanism on a method of direct transformation of intergalactic gamma-rays to the protoncurrent on spin shock-waves ensure precise agreement between generated protoncurrents (spin shock waves theory) with the angular distribution data of Galacticgamma-rays as well as for the individual pulses of gamma-/X-ray bursts. There is a precise confirmation of the generated currents (theory) with the burst radiation data characterized by the standard deviation of ±1% in intensity in relative units within the sensitivity of the equipment. Thus, it was found that the spin angular momentum conservation law (equation of dynamics of spin shock waves) in the X-ray/gammaranges is fulfilled exactly in real time. The next step involves setting the inverseproblem of determining the wave function disturbance on the differential of measured smoothing pulses. In the asymptotic large times the problem is reduced to the solutions of the functional equation with shift of the argument. This will give additional information about the change speed of the wave, as well as on the interaction.