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

Marius Arghirescu

doi:doi:10.11648/j.ijhep.20180501.16

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

Marius Arghirescu

Published in International Journal of High Energy Physics (Volume 5, Issue 1)

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 T_BE » 10³K, in a specific interval of field intensity and of temperature: B = (2.2x10⁶ ¸ 8.3x10⁷) T and T_p = (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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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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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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TY  - JOUR
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
PY  - 2018
N1  - https://doi.org/10.11648/j.ijhep.20180501.16
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
SP  - 55
EP  - 62
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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Marius Arghirescu

State Office for Inventions and Trademarks, Bucharest, Romania

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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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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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TY  - JOUR
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
PY  - 2018
N1  - https://doi.org/10.11648/j.ijhep.20180501.16
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
SP  - 55
EP  - 62
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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