Spinor model of a perfect fluid

• Authors: Bijan Saha
• Languages of publication: EN

Abstracts

EN

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

EN

spinor field; perfect fluid; dark energy

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2010
• Volume: 8
• Issue: 6
• Pages: 920-923

Dates

published

1 - 12 - 2010

online

5 - 9 - 2010

Contributors

author

Bijan Saha

• Laboratory of Information Technologies, Joint Institute for Nuclear Research, Dubna, 141980, Dubna, Moscow region, Russia

References

• [1] B. Saha, Phys. Rev. D. 64, 123501 (2001) http://dx.doi.org/10.1103/PhysRevD.64.123501
• [2] B. Saha, T. Boyadjiev, Phys. Rev. D. 69, 124010 (2004) http://dx.doi.org/10.1103/PhysRevD.69.124010
• [3] B. Saha, Phys. Part. Nuclei 37, S13 (2006) http://dx.doi.org/10.1134/S1063779606070021[Crossref]
• [4] B. Saha, Phys. Rev. D. 74, 124030 (2006) http://dx.doi.org/10.1103/PhysRevD.74.124030
• [5] B. Saha, Phys. Rev. D. 69, 124006 (2004) http://dx.doi.org/10.1103/PhysRevD.69.124006
• [6] V. G. Krechet, M. L. Fel’chenkov, G. N. Shikin, Gravitation and Cosmology 14, 292 (2008) http://dx.doi.org/10.1134/S0202289308030134[Crossref]
• [7] B. Saha, arXiv:gr-qc/0701059 [WoS]
• [8] B. Saha, Int. J. Theor. Phys. 45, 983 (2006) http://dx.doi.org/10.1007/s10773-006-9089-0[Crossref]

Identifiers

DOI

10.2478/s11534-010-0019-7