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The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field

Received: 13 May 2018     Accepted: 29 May 2018     Published: 13 June 2018
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Abstract

In the paper - based on a previous work regarding the cold particles forming process as collapsed cold clusters of gammons- considered as pairs: g* = (e-e+) of axially coupled electrons with opposed charges, is analyzed the possibility of gammons pre-cluster forming from a Bose-Einstein condensate formed in the magnetic and in the gravitational field of a star. By known relations of a BEC forming, it is argued that- in the magnetic field of a star, the forming of a gammonic BEC with particles density N0 corresponding to those of a pre-cluster of gammons which may generates a particle-like stable cluster, may occurs- for a transition temperature TBE » 103K, in a specific interval of field intensity and of temperature: B = (2.2x106 ¸ 8.3x107) T and Tp = (4.8x10-11 ¸ 1.8x10-10) K. The possible mechanism of the formed BEC transforming into pre-clusters of gammons which may become particle-like collapsed BEC, is a pearlitization mechanism, resulted as fragmentation of the formed BEC. It is argued that the particles forming from chiral quantum vacuum fluctuations is possible at T ®0K, either by a vortexial, magnetic-like field corresponding to B ³ 104 T or by already formed gammons, in a “step-by-step” process.

Published in International Journal of High Energy Physics (Volume 5, Issue 1)
DOI 10.11648/j.ijhep.20180501.16
Page(s) 55-62
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), 2018. Published by Science Publishing Group

Keywords

Bose-Einstein Condensate, Bosonic Cluster, Elementary Particles, Magnetic Field Confining, Black Hole, Magnetar

References
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[4] Arghirescu, M., ‘A Quasi-Unitary Pre-Quantum theory of Particles and Fields and some Theoretical Implications’, IJHEP, july, 80-103, (2015).
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[6] Arghirescu, M., ‘A preonic quasi-crystal quark model based on a cold genesis theory and on the experimentally evidenced neutral boson of 34 me’, Global Journal of Physics Vol. 5, No 1, (2016), pp. 496-504.
[7] Arghirescu M., ‘The Explaining of the Elementary Particles Cold Genesis by a Preonic Quasi-Crystal Model of Quarks and a Pre-Quantum Theory of Fields’, IJHEP, Vol. 5, No. 1, (2018), pp. 12-22.
[8] Perez Rojas H., Villegas-Lelovski L., ‘Bose-Einstein Condensation in a Constant Magnetic Field’, Brazilian Journ. of Phys., vol. 30, no. 2, June, (2000), pp. 410-418.
[9] J. I. Rivas, A. Camacho, ‘Bose-Einstein condensates in a homogeneous gravitational field’, arXiv: 1101. 1263v1 [cond-mat. quant-gas] 6 Jan (2011).
[10] Elizabeth A. Donley, N. R., Claussen, S. L. et al. ‘Dynamics of collapsing and exploding Bose-Einstein condensates’, arXiv: cond-mat/0105019v3, June (2001).
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    Marius Arghirescu. (2018). The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field. International Journal of High Energy Physics, 5(1), 55-62. https://doi.org/10.11648/j.ijhep.20180501.16

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    ACS Style

    Marius Arghirescu. The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field. Int. J. High Energy Phys. 2018, 5(1), 55-62. doi: 10.11648/j.ijhep.20180501.16

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    AMA Style

    Marius Arghirescu. The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field. Int J High Energy Phys. 2018;5(1):55-62. doi: 10.11648/j.ijhep.20180501.16

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  • @article{10.11648/j.ijhep.20180501.16,
      author = {Marius Arghirescu},
      title = {The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field},
      journal = {International Journal of High Energy Physics},
      volume = {5},
      number = {1},
      pages = {55-62},
      doi = {10.11648/j.ijhep.20180501.16},
      url = {https://doi.org/10.11648/j.ijhep.20180501.16},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijhep.20180501.16},
      abstract = {In the paper - based on a previous work regarding the cold particles forming process as collapsed cold clusters of gammons- considered as pairs: g* = (e-e+) of axially coupled electrons with opposed charges, is analyzed the possibility of gammons pre-cluster forming from a Bose-Einstein condensate formed in the magnetic and in the gravitational field of a star. By known relations of a BEC forming, it is argued that- in the magnetic field of a star, the forming of a gammonic BEC with particles density N0 corresponding to those of a pre-cluster of gammons which may generates a particle-like stable cluster, may occurs- for a transition temperature TBE » 103K, in a specific interval of field intensity and of temperature: B = (2.2x106 ¸ 8.3x107) T and Tp = (4.8x10-11 ¸ 1.8x10-10) K. The possible mechanism of the formed BEC transforming into pre-clusters of gammons which may become particle-like collapsed BEC, is a pearlitization mechanism, resulted as fragmentation of the formed BEC. It is argued that the particles forming from chiral quantum vacuum fluctuations is possible at T ®0K, either by a vortexial, magnetic-like field corresponding to B ³ 104 T or by already formed gammons, in a “step-by-step” process.},
     year = {2018}
    }
    

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    T1  - The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field
    AU  - Marius Arghirescu
    Y1  - 2018/06/13
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    DO  - 10.11648/j.ijhep.20180501.16
    T2  - International Journal of High Energy Physics
    JF  - International Journal of High Energy Physics
    JO  - International Journal of High Energy Physics
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    PB  - Science Publishing Group
    SN  - 2376-7448
    UR  - https://doi.org/10.11648/j.ijhep.20180501.16
    AB  - In the paper - based on a previous work regarding the cold particles forming process as collapsed cold clusters of gammons- considered as pairs: g* = (e-e+) of axially coupled electrons with opposed charges, is analyzed the possibility of gammons pre-cluster forming from a Bose-Einstein condensate formed in the magnetic and in the gravitational field of a star. By known relations of a BEC forming, it is argued that- in the magnetic field of a star, the forming of a gammonic BEC with particles density N0 corresponding to those of a pre-cluster of gammons which may generates a particle-like stable cluster, may occurs- for a transition temperature TBE » 103K, in a specific interval of field intensity and of temperature: B = (2.2x106 ¸ 8.3x107) T and Tp = (4.8x10-11 ¸ 1.8x10-10) K. The possible mechanism of the formed BEC transforming into pre-clusters of gammons which may become particle-like collapsed BEC, is a pearlitization mechanism, resulted as fragmentation of the formed BEC. It is argued that the particles forming from chiral quantum vacuum fluctuations is possible at T ®0K, either by a vortexial, magnetic-like field corresponding to B ³ 104 T or by already formed gammons, in a “step-by-step” process.
    VL  - 5
    IS  - 1
    ER  - 

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