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Open Physics

formerly Central European Journal of Physics

Editor-in-Chief: Seidel, Sally

Managing Editor: Lesna-Szreter, Paulina

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IMPACT FACTOR 2016 (Open Physics): 0.745
IMPACT FACTOR 2016 (Central European Journal of Physics): 0.765

CiteScore 2017: 0.83

SCImago Journal Rank (SJR) 2017: 0.241
Source Normalized Impact per Paper (SNIP) 2017: 0.537

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ISSN
2391-5471
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Volume 8, Issue 6

Issues

Volume 13 (2015)

Spinor model of a perfect fluid

Bijan Saha
  • Laboratory of Information Technologies, Joint Institute for Nuclear Research, Dubna, 141980, Dubna, Moscow region, Russia
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Published Online: 2010-09-05 | DOI: https://doi.org/10.2478/s11534-010-0019-7

Abstract

Different characteristics of matter influencing the evolution of the uUniverse haves been simulated by means of a nonlinear spinor field. We have considered two cases where the spinor field nonlinearity occurs either as a result of self-action or due to the interaction with a scalar field.

Keywords: spinor field; perfect fluid; dark energy

  • [1] B. Saha, Phys. Rev. D. 64, 123501 (2001) http://dx.doi.org/10.1103/PhysRevD.64.123501Google Scholar

  • [2] B. Saha, T. Boyadjiev, Phys. Rev. D. 69, 124010 (2004) http://dx.doi.org/10.1103/PhysRevD.69.124010Google Scholar

  • [3] B. Saha, Phys. Part. Nuclei 37, S13 (2006) http://dx.doi.org/10.1134/S1063779606070021CrossrefGoogle Scholar

  • [4] B. Saha, Phys. Rev. D. 74, 124030 (2006) http://dx.doi.org/10.1103/PhysRevD.74.124030Google Scholar

  • [5] B. Saha, Phys. Rev. D. 69, 124006 (2004) http://dx.doi.org/10.1103/PhysRevD.69.124006Google Scholar

  • [6] V. G. Krechet, M. L. Fel’chenkov, G. N. Shikin, Gravitation and Cosmology 14, 292 (2008) http://dx.doi.org/10.1134/S0202289308030134CrossrefGoogle Scholar

  • [7] B. Saha, arXiv:gr-qc/0701059 Web of ScienceGoogle Scholar

  • [8] B. Saha, Int. J. Theor. Phys. 45, 983 (2006) http://dx.doi.org/10.1007/s10773-006-9089-0CrossrefGoogle Scholar

About the article

Published Online: 2010-09-05

Published in Print: 2010-12-01


Citation Information: Open Physics, Volume 8, Issue 6, Pages 920–923, ISSN (Online) 2391-5471, DOI: https://doi.org/10.2478/s11534-010-0019-7.

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© 2010 Versita Warsaw. This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License. BY-NC-ND 3.0

Citing Articles

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[1]
Bijan Saha
Canadian Journal of Physics, 2016, Volume 94, Number 1, Page 116
[2]
Ratbay Myrzakulov, Diego Sáez-Gómez, and Petr Tsyba
International Journal of Geometric Methods in Modern Physics, 2015, Volume 12, Number 02, Page 1550023
[3]
Edward J. Kim, Seyen Kouwn, Phillial Oh, and Chan-Gyung Park
Journal of Cosmology and Astroparticle Physics, 2014, Volume 2014, Number 07, Page 001
[4]
Bijan Saha
Physics of Particles and Nuclei, 2014, Volume 45, Number 2, Page 349
[5]
Bijan Saha
International Journal of Theoretical Physics, 2014, Volume 53, Number 4, Page 1109
[6]
SEYEN KOUWN, JOOHAN LEE, TAE HOON LEE, and PHILLIAL OH
Modern Physics Letters A, 2013, Volume 28, Number 29, Page 1350121
[7]
Koblandy Yerzhanov, Kuralay Yesmakhanova, Petr Tsyba, Nurgissa Myrzakulov, Gulgasyl Nugmanova, and Ratbay Myrzakulov
Astrophysics and Space Science, 2012, Volume 341, Number 2, Page 681
[8]
Bijan Saha
International Journal of Theoretical Physics, 2012, Volume 51, Number 6, Page 1812

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