| Peer-Reviewed

Anisotropic Distribution of Space Pulsar Velocities

Received: 22 September 2014     Accepted: 25 September 2014     Published: 29 October 2014
Views:       Downloads:
Abstract

On the base of new data it is shown that the observed proper motions and directions of the tangential velocities of pulsars manifest the extremely anisotropic distributions. These anisotropies cannot be explained by the structure of our Galaxy or by various types of solar motions. They can be caused by the cosmological vector potential and the action of the new force. This force must be stronger in higher magnetic fields. The positive correlation between tangential velocities Vt and surface magnetic fields of pulsars Bs is seen indeed. It is shown that the new force can provide pulsar velocities up to several thousands of km/sec.

Published in American Journal of Astronomy and Astrophysics (Volume 2, Issue 6-1)

This article belongs to the Special Issue Global Anisotropy, Theory of Byuon, New Force, New Power System, Propulsion, Space Flights

DOI 10.11648/j.ajaa.s.2014020601.14
Page(s) 29-31
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), 2014. Published by Science Publishing Group

Keywords

Pulsars, Proper Motions, Magnetic Fields, New Force

References
[1] R.N.Manchester, G.B.Hobbs, A.Teoh, and M.Hobbs. The Australia Telescope National Facility Pulsar Catalogue. Astron.J., vol.129, pp.1993-2006, 2005.
[2] Z.Arzoumanian, D.F.Chernoff, and J.M.Cordes. The Velocity Distribution of Isolated Radio Pulsars Astrophys.J.,vol.289-301, pp.568, 2002.
[3] D. Lai. Neutron star kicks and supernova asymmetry..In Cosmic Explosions in Three Dimensions: Asymmetries in Supernovae and Gamma-Ray Bursts, Ed. by P. Hoflich, P. Kumar, and J. C. Wheeler (Cambridge Univ. Press, Cambridge, 2004), p. 276; astro-ph/0312542.
[4] Yu.A.Baurov, A.A.Shpitalnaya, and I.F.Malov. Global Anisotropy of Physical Space and Velocities of Pulsars. Int. J.of Pure and Applied Physics. vol..1, №1, pp..71-82, 2005.
[5] V. D. Pal’shin and A. I. Tsygan. Acceleration of binary X-ray sources by their radiation. Astron. Lett., vol. 24, pp.131-133,1998.
[6] Yu.A.Baurov. On the structure of physical vacuum and a new interaction in Nature (Theory, Experiment and Applications), Nova Science, NY, 2000.
[7] I.F.Malov, Yu.A.Baurov. On the Distribution of Radio Pulsars Velocities.Int. J. of Pure and Applied Physics. vol.2, №3, pp.273-280, 2006.
Cite This Article
  • APA Style

    Igor Fedorovich Malov. (2014). Anisotropic Distribution of Space Pulsar Velocities. American Journal of Astronomy and Astrophysics, 2(6-1), 29-31. https://doi.org/10.11648/j.ajaa.s.2014020601.14

    Copy | Download

    ACS Style

    Igor Fedorovich Malov. Anisotropic Distribution of Space Pulsar Velocities. Am. J. Astron. Astrophys. 2014, 2(6-1), 29-31. doi: 10.11648/j.ajaa.s.2014020601.14

    Copy | Download

    AMA Style

    Igor Fedorovich Malov. Anisotropic Distribution of Space Pulsar Velocities. Am J Astron Astrophys. 2014;2(6-1):29-31. doi: 10.11648/j.ajaa.s.2014020601.14

    Copy | Download

  • @article{10.11648/j.ajaa.s.2014020601.14,
      author = {Igor Fedorovich Malov},
      title = {Anisotropic Distribution of Space Pulsar Velocities},
      journal = {American Journal of Astronomy and Astrophysics},
      volume = {2},
      number = {6-1},
      pages = {29-31},
      doi = {10.11648/j.ajaa.s.2014020601.14},
      url = {https://doi.org/10.11648/j.ajaa.s.2014020601.14},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.s.2014020601.14},
      abstract = {On the base of new data it is shown that the observed proper motions and directions of the tangential velocities of pulsars manifest the extremely anisotropic distributions. These anisotropies cannot be explained by the structure of our Galaxy or by various types of solar motions. They can be caused by the cosmological vector potential and the action of the new force. This force must be stronger in higher magnetic fields. The positive correlation between tangential velocities Vt and surface magnetic fields of pulsars Bs is seen indeed. It is shown that the new force can provide pulsar velocities up to several thousands of km/sec.},
     year = {2014}
    }
    

    Copy | Download

  • TY  - JOUR
    T1  - Anisotropic Distribution of Space Pulsar Velocities
    AU  - Igor Fedorovich Malov
    Y1  - 2014/10/29
    PY  - 2014
    N1  - https://doi.org/10.11648/j.ajaa.s.2014020601.14
    DO  - 10.11648/j.ajaa.s.2014020601.14
    T2  - American Journal of Astronomy and Astrophysics
    JF  - American Journal of Astronomy and Astrophysics
    JO  - American Journal of Astronomy and Astrophysics
    SP  - 29
    EP  - 31
    PB  - Science Publishing Group
    SN  - 2376-4686
    UR  - https://doi.org/10.11648/j.ajaa.s.2014020601.14
    AB  - On the base of new data it is shown that the observed proper motions and directions of the tangential velocities of pulsars manifest the extremely anisotropic distributions. These anisotropies cannot be explained by the structure of our Galaxy or by various types of solar motions. They can be caused by the cosmological vector potential and the action of the new force. This force must be stronger in higher magnetic fields. The positive correlation between tangential velocities Vt and surface magnetic fields of pulsars Bs is seen indeed. It is shown that the new force can provide pulsar velocities up to several thousands of km/sec.
    VL  - 2
    IS  - 6-1
    ER  - 

    Copy | Download

Author Information
  • P. N. Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Russia

  • Sections