Source: http://rgs.vniims.ru/abs/abs-16-228.html
Timestamp: 2019-04-23 02:22:44+00:00

Document:
Cosmological models with a generalized and modified Chaplygin gas equivalent to nonlinear scalar and spinor fields have been considered. Scale factors and field potentials have been found.
T. Multamaki, M. Manera, and E. Gazta naga, Phys. Rev. D 69, 023004 (2004).
M. Szydlowski and W. Czaja, Phys. Rev. D 69, 023506 (2004).
T. Barriero and A. A. Sen, Phys. Rev. D 70, 124013 (2004).
V. Bouhmadi-Lopez and P. V. Moniz, Phys. Rev. D 71, 063521 (2005).
G. N. Shikin, M. L. Fil'chenkov, and V. G. Krechet, Grav. Cosmol. 13, 241 (2007).
V. G. Krechet, M. L. Fil'chenkov and G. N. Shikin, Grav. Cosmol. 14, 292 (2008).
V. G. Krechet, M. L. Fil'chenkov and G. N. Shikin, Grav. Cosmol. 15, 37 (2009).
L. D. Landau and E. M. Lifshitz, Field Theory (Nauka, Moscow, 1973).
A. D. Dolgov, Ya. B. Zel'dovich, and M. V. Sazhin, Cosmology of the Early Universe (Moscow University Press, Moscow, 1988).
A. D. Linde, Elementary Particle Physics and Inflationary Cosmology (Nauka, Moscow, 1978).

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