When Anisotropy of Vacuum Set the Space Isotropy

A. G. Syromyatnikov

doi:doi:10.11648/j.ijhep.s.2016030101.12

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When Anisotropy of Vacuum Set the Space Isotropy

A. G. Syromyatnikov

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

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), 2024. 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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TY  - JOUR
T1  - When Anisotropy of Vacuum Set the Space Isotropy
AU  - A. G. Syromyatnikov
Y1  - 2016/03/14
PY  - 2016
N1  - https://doi.org/10.11648/j.ijhep.s.2016030101.12
DO  - 10.11648/j.ijhep.s.2016030101.12
T2  - International Journal of High Energy Physics
JF  - International Journal of High Energy Physics
JO  - International Journal of High Energy Physics
SP  - 9
EP  - 14
PB  - Science Publishing Group
SN  - 2376-7448
UR  - https://doi.org/10.11648/j.ijhep.s.2016030101.12
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
IS  - 1-1
ER  -

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Author Information

A. G. Syromyatnikov

Department of Physics, St. Petersburg University, Universitetskaya nab., St. Petersburg, Russia

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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

Copy | Download

@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}
}

Copy | Download

TY  - JOUR
T1  - When Anisotropy of Vacuum Set the Space Isotropy
AU  - A. G. Syromyatnikov
Y1  - 2016/03/14
PY  - 2016
N1  - https://doi.org/10.11648/j.ijhep.s.2016030101.12
DO  - 10.11648/j.ijhep.s.2016030101.12
T2  - International Journal of High Energy Physics
JF  - International Journal of High Energy Physics
JO  - International Journal of High Energy Physics
SP  - 9
EP  - 14
PB  - Science Publishing Group
SN  - 2376-7448
UR  - https://doi.org/10.11648/j.ijhep.s.2016030101.12
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
IS  - 1-1
ER  -

Copy | Download