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When Anisotropy of Vacuum Set the Space Isotropy

Received: 19 June 2015     Accepted: 20 June 2015     Published: 14 March 2016
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Abstract

Results of some theoretical and experiment investigations of space-time anisotropy of Galactic gamma-rays angular distribution within the frame of the space rays generation mechanism on a method of direct transformation of intergalactic gamma-rays to the current on spin shock-waves are presented. However, the source anisotropy origin is unknown. Here I show that on Fermi telescope data brightness at the edge of the area, limited 20° Galactic longitude, twice higher the brightness of diffuse radiation. Thus the range of the observed distribution mapping of gamma rays from the Galactic longitude of theoretical (intensity of above-average level) in fact is limited above 20° strict accordance with the theory. I found that the Galactic gamma – ray angular anisotropy axis has following coordinates: longitude l = 96°, latitude ≈ 20°, that corresponds in the second equatorial coordinate system: right ascension α = 271°, declination δ ≈ 40 - supernova residuals Cygnus X-3 on periphery.

Published in International Journal of High Energy Physics (Volume 3, Issue 1-1)

This article belongs to the Special Issue Breaking of Space Symmetry in the Masses Spectrum Problem

DOI 10.11648/j.ijhep.s.2016030101.12
Page(s) 9-14
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2016. Published by Science Publishing Group

Keywords

Galaxy Gamma-Rays, Spin Shock-Waves, Eight Spin Shock Waves Model, Fermi Space Telescope

References
[1] SYROMYATNIKOV A. G., Vestnik Sanct Peterburgskogo universiteta. Ser. 4. Vip. 2 (2012) 108-112; SYROMYATNIKOV A. G., Vestnik Sanct Peterburgskogo universiteta. Ser. 4. Vol. 2 (60) Vip. 1 (2015) 88-92.
[2] Gamma-ray astronomy, Physical encyclopedia/HL. Ed. Prokhorov A. M., (Sov. Encyclopedia, Moscow, T1. Aaron-Bohm effect-long lines, 1988): web-site: http://en.wikipedia.org/wiki/Gamma-ray_burst.
[3] PROSHIN Yu. N., USEYNOV N. H., Magnetic break with spin rotation, UFN 165 No. 1 (1985) 41-87.
[4] Website (2015): glast.gsfc.nasa.gov: Diffuse Hard X-Ray/Gamma-Ray Emission from Galaxy and local group of galaxies Galactic Diffuse Emission: MIZUNOI T., TAKAHASHI T., TAKAHASHI H., KATAGIRI H., FUZUKAWA Y. and OHSUGI T. (Hiroshima Univ.); STANLEY D. Hunter, galactic diffuse gamma-ray emission, the EGRET Model, and GLAST, Science, July 23, 2004. NASA /GSFC Code 66/.
[5] SYROMYATNIKOV A. G., Physical effects in Conformal Gauge Theory of Gravitation (LAP Lambert Academic Publishing GmbH & Co. KG, Saarbrucken, Germany, 2012).
[6] SYROMYATNIKOV A. G., On some feature of possible torsion effects on observables at hadron colliders, Int. J. Geom. Meth. Mod. Phys (2015) (to be published) DOI: 10.1142/S0219887815500802.
[7] BAUROV Yu. A. et al., Phys. Lett. A. 311 (2003) 512.
[8] ARBUSOV B. A., JETP Lett. 42 Vip. 10 (1985) 430-432.
[9] BAUROV Yu. A., The anisotropy of cosmic rays and the global anisotropy of physical space, J. Mod. Phys. 3 (2012) 1744.
[10] BAUROV Yu. A., On the structure of physical vacuum and a new interaction in Nature (Theory, Experiment and Applications) (Nova Science, NY, 2000).
[11] SYROMYATNIKOV A. G., Vestnik Sanct Peterburgskogo universiteta. Ser. 4. Vip. 2 (2009) 410-425.
[12] SYROMYATNIKOV A. G., Sovremenny nauchny vestnik. Ser.: Physics. No4 (100) (2011) 33-44. (DOI: 10.17686/sced_rusnauka_2011-236).
[13] TEILOR J. H., MANCHESTER R. N. and LYNE A. G., Catalog of 558 Pulsars, Ap. J. Suppl. Series 88 (1993) 529–568.
[14] Supernova Catalogue (Moscow State University, Astronomy institute, 2015).
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  • APA Style

    A. G. Syromyatnikov. (2016). When Anisotropy of Vacuum Set the Space Isotropy. International Journal of High Energy Physics, 3(1-1), 9-14. https://doi.org/10.11648/j.ijhep.s.2016030101.12

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    ACS Style

    A. G. Syromyatnikov. When Anisotropy of Vacuum Set the Space Isotropy. Int. J. High Energy Phys. 2016, 3(1-1), 9-14. doi: 10.11648/j.ijhep.s.2016030101.12

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    AMA Style

    A. G. Syromyatnikov. When Anisotropy of Vacuum Set the Space Isotropy. Int J High Energy Phys. 2016;3(1-1):9-14. doi: 10.11648/j.ijhep.s.2016030101.12

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  • @article{10.11648/j.ijhep.s.2016030101.12,
      author = {A. G. Syromyatnikov},
      title = {When Anisotropy of Vacuum Set the Space Isotropy},
      journal = {International Journal of High Energy Physics},
      volume = {3},
      number = {1-1},
      pages = {9-14},
      doi = {10.11648/j.ijhep.s.2016030101.12},
      url = {https://doi.org/10.11648/j.ijhep.s.2016030101.12},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijhep.s.2016030101.12},
      abstract = {Results of some theoretical and experiment investigations of space-time anisotropy of Galactic gamma-rays angular distribution within the frame of the space rays generation mechanism on a method of direct transformation of intergalactic gamma-rays to the current on spin shock-waves are presented. However, the source anisotropy origin is unknown. Here I show that on Fermi telescope data brightness at the edge of the area, limited 20° Galactic longitude, twice higher the brightness of diffuse radiation. Thus the range of the observed distribution mapping of gamma rays from the Galactic longitude of theoretical (intensity of above-average level) in fact is limited above 20° strict accordance with the theory. I found that the Galactic gamma – ray angular anisotropy axis has following coordinates: longitude l = 96°, latitude ≈ 20°, that corresponds in the second equatorial coordinate system: right ascension α = 271°, declination δ ≈ 40 - supernova residuals Cygnus X-3 on periphery.},
     year = {2016}
    }
    

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    T1  - When Anisotropy of Vacuum Set the Space Isotropy
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    JF  - International Journal of High Energy Physics
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    AB  - Results of some theoretical and experiment investigations of space-time anisotropy of Galactic gamma-rays angular distribution within the frame of the space rays generation mechanism on a method of direct transformation of intergalactic gamma-rays to the current on spin shock-waves are presented. However, the source anisotropy origin is unknown. Here I show that on Fermi telescope data brightness at the edge of the area, limited 20° Galactic longitude, twice higher the brightness of diffuse radiation. Thus the range of the observed distribution mapping of gamma rays from the Galactic longitude of theoretical (intensity of above-average level) in fact is limited above 20° strict accordance with the theory. I found that the Galactic gamma – ray angular anisotropy axis has following coordinates: longitude l = 96°, latitude ≈ 20°, that corresponds in the second equatorial coordinate system: right ascension α = 271°, declination δ ≈ 40 - supernova residuals Cygnus X-3 on periphery.
    VL  - 3
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Author Information
  • Department of Physics, St. Petersburg University, Universitetskaya nab., St. Petersburg, Russia

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