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
Views 1032      Downloads 119
Marius Arghirescu, State Office for Inventions and Trademarks, Bucharest, Romania
Article Tools
Follow on us
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.
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
Copyright © 2018 Authors retain the copyright of this article.
This article is an open access article distributed under the Creative Commons Attribution License ( which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Sinha, K. P., Sudarshan, E. C. G., „The superfluid as a source of all interactions”, Found. of Physics, Vol. 8, Issue 11–12, Dec. (1978), pp. 823–831.
Arghirescu, M., “The Cold Genesis”, Ed. Invel- Multimedia, 2011; viXra, 1104. 0043, (2012).
Arghirescu, M., “The Cold Genesis of Matter and Fields”, Ed. SciencePG, (2015).
Arghirescu, M., ‘A Quasi-Unitary Pre-Quantum theory of Particles and Fields and some Theoretical Implications’, IJHEP, july, 80-103, (2015).
Anderson, C. D., ‘The Positive Electron’, Phys. Rev. 43, 491, 15 March (1933).
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.
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.
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.
J. I. Rivas, A. Camacho, ‘Bose-Einstein condensates in a homogeneous gravitational field’, arXiv: 1101. 1263v1 [cond-mat. quant-gas] 6 Jan (2011).
Elizabeth A. Donley, N. R., Claussen, S. L. et al. ‘Dynamics of collapsing and exploding Bose-Einstein condensates’, arXiv: cond-mat/0105019v3, June (2001).
Claussen N. R., Kokkelmans S. J. J. M. F., Thompson S. T., Donley E. A., Hodby, E., Wieman C. E. Phys. Rev. A 67 060701(R), (2003).
Bӧhmer C. G., Harko T., ‘Can dark matter be a Bose- Einstein condensate?’, arXiv:0705.4158v4 [astro-ph] 21 Jun (2007)
Alfaro J., Espriu D., Gabbanelli L., ‘Bose-Einstein graviton condensate in a Schwarzschild black hole’, IOP Journal, Vol. 35, No. 1, Nov. (2017); arXiv: 1609. 01639v1 [gr-qc] 6, Sept. (2016).
A. D. Linde, Phys. Lett. B 86, 39 (1979).
Dallilar Y., Eikenberry S. S., Garner A., ‘A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni’, Science Vol. 358, Issue 6368, 08 Dec. (2017), pp. 1299-1302
D.W.Liu et al., [Super Kamiokande Collaboration], Phys.Rev.Lett.93, 021802(2004); arXiv: hep-ex/0402015.
Nieuwenhuizen, T. M., ‘Dirac neutrino mass from a neutrino dark matter model for the galaxy cluster Abell 1689’, Journal of Physics: Conference Series, 701 (1): 012022, (2016); arXiv: 1510. 06958.
Science Publishing Group
1 Rockefeller Plaza,
10th and 11th Floors,
New York, NY 10020
Tel: (001)347-983-5186