Geodesic
Oscillating universe in the case $p\neq0$
Teoretičeskaâ i matematičeskaâ fizika, Tome 58 (1984) no. 2, pp. 163-168

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Markov [1,2] has considered a perpetually oscillating universe under a special assumption concerning the parameters of the model: $n=m=1$, $\Lambda'=2\rho_{\rm PI}$. He considered the case of dust, $T_{\mu\nu}=\rho c^2{\delta_\mu}^0 {\delta_\nu}^0$ with pressure $p=0$. The present paper investigates the variant with $p\ne0$, and there is also a discussion of a model in which the requirement $T_{\mu;\nu}^\nu =0$ is satisfied. 
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     author = {\`E. G. Aman and M. A. Markov},
     title = {Oscillating universe in the case $p\neq0$},
     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
     pages = {163--168},
     publisher = {mathdoc},
     volume = {58},
     number = {2},
     year = {1984},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/TMF_1984_58_2_a0/}
}
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È. G. Aman; M. A. Markov. Oscillating universe in the case $p\neq0$. Teoretičeskaâ i matematičeskaâ fizika, Tome 58 (1984) no. 2, pp. 163-168. http://geodesic.mathdoc.fr/item/TMF_1984_58_2_a0/