Cosmological consequences of the relativistic theory of gravitation with massive gravitons
Teoretičeskaâ i matematičeskaâ fizika, Tome 79 (1989) no. 2, pp. 307-313 Cet article a éte moissonné depuis la source Math-Net.Ru

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It is shown that introducing the non-zero graviton mass we can provide the solution of such standard cosmological scenario problems as singularity, horizon, flatness and concentration of relic monopoles.
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Yu. V. Chugreev. Cosmological consequences of the relativistic theory of gravitation with massive gravitons. Teoretičeskaâ i matematičeskaâ fizika, Tome 79 (1989) no. 2, pp. 307-313. http://geodesic.mathdoc.fr/item/TMF_1989_79_2_a13/

[1] Linde A. D., Rep. Progr. Phys., 47 (1984), 925–986 | DOI | MR

[2] Logunov A. A., Mestvirishvili M. A., Osnovy relyativistskoi teorii gravitatsii, MGU, M., 1986

[3] Guth A., Phys. Rev., D23 (1981), 347–356

[4] Loh E. D., Spillar E. J., Astrophys. J., 307:8 (1986), 1–4 | DOI

[5] Rindler W., Mon. Not. R. Astron. Soc., 116:6 (1956), 662–677 | DOI | MR

[6] Olivo-Melchiorri B., Melchiorri F., Riv. Nuovo Cim., 8:9 (1985), 1–35 | DOI

[7] Kibble T. W., J. Phys. A: Math. Gen., 9 (1976), 1387–1398 | DOI | Zbl

[8] Kibble T. W., Phys. Rep., 67 (1980), 183–199 | DOI | MR

[9] Zeldovich Ya. B., Khlopov M. Yu., UFN, 135:1 (1981), 45–78 | DOI | MR

[10] Prescill J. P., Phys. Rev. Lett., 43 (1979), 1365–1368 | DOI

[11] Dolgov A. D., Zeldovich Ya. B., UFN, 30:4 (1980), 559–614 | DOI

[12] Logunov A. A., Mestvirishvili M. A., Chugreev Yu. V., TMF, 74:1 (1988), 3–15 | MR

[13] Boulware D. G., Deser S., Phys. Rev., D6:12 (1972), 3368–3382

[14] Jun J.-H., Kang I., Phys. Rev., D34:4 (1986), 1005–1010 | MR

[15] Zeldovich Ya. B., ZhETF, 41:5(11) (1961), 1609–1615

[16] Weinberg S., The First Three Minutes, Basic Books Publ., N. Y., 1977 | MR

[17] Veinberg S., Gravitatsiya i kosmologiya, Mir, M., 1975

[18] Mestvirishvili M. A., Chugreev Yu. V., Fridmanovskaya model evolyutsii Vselennoi v RTG, MGU, M., 1988