Classical color fields as a dark matter candidate

• Authors: Vladimir Dzhunushaliev
• Languages of publication: EN

Abstracts

EN

A model of Dark Matter is proposed where the Dark Matter is a classical color field. The color fields are invisible as they may interact with colored elementary particles like the ’t Hooft-Polyakov monopole only. Comparison with the Universal Rotation Curve is carried out.

Keywords

EN

dark matter; universal rotation curve; classical gauge theory

Discipline

• 95.35.+d: Dark matter (stellar, interstellar, galactic, and cosmological)(see also 95.30.Cq Elementary particle processes; for brown dwarfs, see 97.20.Vs; for galactic halos, see 98.35.Gi or 98.62.Gq; for models of the early Universe, see 98.80.Cq)

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2007
• Volume: 5
• Issue: 3
• Pages: 342-350

Dates

published

1 - 9 - 2007

online

8 - 6 - 2007

Contributors

author

Vladimir Dzhunushaliev

• Departement of Physics and Microelectronics Engineering, Kyrgyz-Russian Slavic University, Bishkek, Kievskaya Str. 44, 720021, Kyrgyz Republic

References

• [1] F. Zwicky: “Die Rotverschiebung von extragalaktischen Nebeln”, Helv. Phys. Acta., Vol. 6, (1933), pp. 110–127.
• [2] D. Clowe, M. Bradac, A. H. Gonzalez, M. Markevitch, S. W. Randall, C. Jones and D. Zaritsky: “A direct empirical proof of the existence of dark matter”, Preprint: arXiv:astro-ph/0608407.
• [3] F. Combes, P. Boissé, A. Mazure and A. Blanchard: Galaxies and Cosmology, 2nd ed., Springer, New York, 2002.
• [4] J. Binney and S. Tremaine: Galactic Dynamics, Princeton University Press, 1994.
• [5] M. Milgrom: “A modification of the newtonian dynamics as a possible alternative to the hidden mass hypothesis”, Astrophys. J., Vol. 270, (1983), pp. 365–370. http://dx.doi.org/10.1086/161130[Crossref]
• [6] B. Sadoulet: “Deciphering the nature of dark matter”, Rev. Mod. Phys., Vol. 71, (1999), S197–S204. http://dx.doi.org/10.1103/RevModPhys.71.S197[Crossref]
• [7] Y. N. Obukhov: “Analogue of black string in the Yang-Mills gauge theory”, Int. J. Theor. Phys., Vol. 37, (1998), 1455–1468; V. D. Dzhunushaliev and D. Singleton: “Confining solutions of SU(3) Yang-Mills theory”, In: VV. Dvoeglazov (Ed.): Contribution to contemporary fundamental physics, Nova Science Publishers, 1999, pp. 336–346. http://dx.doi.org/10.1023/A:1026603516460[Crossref]
• [8] A. Actor: “Classical solutions of SU(2) Yang-Mills theories”, Rev. Mod. Phys., Vol. 51, (1979), pp. 461–525. http://dx.doi.org/10.1103/RevModPhys.51.461[Crossref]
• [9] E. Corrigan, D. I. Olive, D. B. Farlie and J. Nuyts: “Magnetic monopoles in SU(3) gauge theories”, Nucl. Phys., Vol. B106, (1976), pp. 475–492.
• [10] M. Persic, P. Salucci and F. Stel, “The Universal rotation curve of spiral galaxies: 1. The Dark matter connection”, Mon. Not. Roy. Astron. Soc., Vol. 281, (1996), pp. 27–47
• [11] V. Dzhunushaliev, “Color defects in a gauge condensate,” Preprint: arXiv:hepph/0605070.

Identifiers

DOI

10.2478/s11534-007-0028-3