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Inflationary Universe, Primordial Sound Waves and Galaxy Formation

Published online by Cambridge University Press:  04 August 2017

V. N. Lukash  and
I. D. Novikov
V. N. Lukash
Affiliation:
Space Research Institute, Moscow
I. D. Novikov
Affiliation:
Space Research Institute, Moscow

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At present cosmology experiences a qualitatively new state of its development. Up to now cosmological theory successfully extrapolated to the past the Universe we observe now. This extrapolation was reliable up to the temperatures T ∼1010K. The endeavors to advance nearer to the singularity imply that even cardinally new hypotheses in the elementary particle physics (e.g. Hagerdorn's hypothesis) brought about the relatively insignificant variations in cosmology—the Universe expansion rate obeyed the power law as before, the main features of the cosmological model (homogeneity, singularity, the existence of horizone, etc.) remained unchanged.

References

1. Doroshkevich, A.G., Lukash, V.N., Novikov, I.D., Zh. Eksp. Teor. Fiz. 64, 1457, (1973).Google Scholar
2. Collins, C.B., Hawking, S.Q., Astroph. J. 180, 317 (1973).CrossRefGoogle Scholar
3. Zeldovich, Ya.B., Mon. Not. R. Astron. Soc. 160, 1L (1972).CrossRefGoogle Scholar
4. Dimopoulos, S., Proc. of IAU Symposium 104 “Early Evolution of the Universe and Its Present Structure,” Crete, Greece, Aug 30-Sep 2 (1982).Google Scholar
5. Sato, K., Proc. of IAU Symposium 104 “Early Evolution of the Universe and Its Present Structure,” Crete, Greece, Aug 30-Sep 2 (1982).Google Scholar
6. Bludman, S., Proc. of IAU Symposium 104 “Early Evolution of the Universe and Its Present Structure,” Crete, Greece, Aug 30-Sep 2 1982, (1983) p. 447.Google Scholar
7. Guth, A.H., Phys. Rev. D23, 347 (1981).Google Scholar
8. Dolgov, A.D., Zeldovich, Ya.B., Rev. Mod. Phys. 53, 3 (1981).Google Scholar
9. Turner, M., Proc. of IAU Symposium 104 “Early Evolution of the Universe and Its Present Structure,” Crete, Greece, Aug 30-Sep 2 (1982).Google Scholar
10. Linde, A.D., Phys. Lett. 108B, 389 (1982).CrossRefGoogle Scholar
11. Starobinski, A. A., Phys. Lett. 91B, 99 (1980).CrossRefGoogle Scholar
12. Grishchuk, L.P., Zeldovich, Ya.B., Proc. of 2nd Seminar “Quantum Gravity,” Moscow, Oct 13–15 (1981).Google Scholar
13. Starobinski, A.A., Pis ma Zh. Eksp. Teor. Fiz. 30, 719 (1979).Google Scholar
14. Lukash, V.N., Zh. Eksp. Teor. Fiz. 79, 1601 (1980).Google Scholar
15. Bardeen, J.M., Proc. of Nuffield Workshop on the Very Early Universe (<1 sec), Cambridge, June 21-July 9 (1982).Google Scholar
16. Guth, A.H., Proc. of Nuffield Workshop on the Very Early Universe (<1 sec), Cambridge, June 21-July 9 (1982).Google Scholar
17. Hawking, S.W., Proc. of Nuffield Workshop on the Very Early Universe (<1 sec), Cambridge, June 21-July 9 (1982).Google Scholar
18. Starobinski, A.A., Proc. of Nuffield Workshop on the Very Early Universe (<1 sec), Cambridge, June 21-July 9 (1982).Google Scholar
19. Steinhardt, P.J., Proc. of Nuffield Workshop on the Very Early Universe (<1 sec), Cambridge, June 21-July 9 (1982).Google Scholar
20. Lifshitz, E.M., Zh. Eksp Teor. Fiz. 16, 587 (1946).Google Scholar
21. Lukash, V.N., Pis 'ma Zh. Eksp. Teor. Fiz. 31, 631 (1980).Google Scholar
22. Kompaneets, D.A., Lukash, V.N., Novikov, I.D., Astron. Zh. 59, 424 (1982).Google Scholar
23. Lukash, V.N., Novikov, I.D., Proc. of Nuffield Workshop on the Very Early Universe (<1 sec), Cambridge, June 21-July 9 (1982).Google Scholar
24. Grishchuk, L.P., Zh. Eksp. Teor. Fiz. 67, 825 (1974).Google Scholar
25. Veryaskin, A.V., Rubakov, V.A., Sazhin, M.V., submitted to Phys. Lett. B (1982).Google Scholar