The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field
International Journal of High Energy Physics
Volume 5, Issue 1, June 2018, Pages: 55-62
Received: May 13, 2018; Accepted: May 29, 2018; Published: Jun. 13, 2018
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Author
Marius Arghirescu, State Office for Inventions and Trademarks, Bucharest, Romania
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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.
Keywords
Bose-Einstein Condensate, Bosonic Cluster, Elementary Particles, Magnetic Field Confining, Black Hole, Magnetar
To cite this article
Marius Arghirescu, The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field, International Journal of High Energy Physics. Vol. 5, No. 1, 2018, pp. 55-62. doi: 10.11648/j.ijhep.20180501.16
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Copyright © 2018 Authors retain the copyright of this article.
This article is an open access article distributed under the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/) which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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