CLOSED FRIEDMANN MODEL IN A MODIFIED GRAVITATIONAL THEORY
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Abstract
We consider a closed Friedmann model in modified theory of gravity (including the Riemann tensor). The dependence of the scale factor on time for a hot ultrarelativistic case (p=ε/3). In this case the exponent of the Riemann tensor chosen as α = 1/2. If we set the parameter A = sqrt(6) , then, we obtain a solution in which there is no physical singularity. A similar solution was obtained at A = sqrt(3).
References
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2. Ya.B. Zel'dovich and I.D. Novikov, Stroyeniye i evolyutsiya Vselennoy, (Moscow, Nauka, 1975), 736s. (in Russ).
3. S. Khoking ,Dzh. Ellips, Krupnomasshtabnaya struktura prostranstva, (Moscow, Mir, 1977), 436 s. (in Russ).
4. A.D. Linde, Fizika elementarnykh chastits i inflyatsionnaya kosmologiya, (Moscow, Nauka, 1990).
5. V.L. Ginsburg, UFN, 134, 469 – 517 (1981). (in Russ).
6. V.I. Gurovich and A.A. Starabinskiy, ZHETF, 1683 – 1699 (1977). (in Russ)
7. Ya.B. Zel'dovich, UFN,133, 479 -503 (1981). (in Russ)
8. V.F. Mukhanov, G.V. Chibisov, Pis'ma v ZHETF, 33 (1981). (in Russ)
9. O.Sh. Sharshekeyev Modeli metagalaktiki, polya Shvartsshil'da OTO modifitsirovannaya teoriya gravitatsii, (Frunze, Mektep,1980), 116. (in Russ)
10. L.D. Landau, Ye.I. Lifshits, Teoriya polya, (Moscow, Nauka, 1973), 504s. (in Russ)
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Published
2011-12-20
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Section
Theoretical Physics. Nuclear and Elementary Particle Physics. Astrophysics
