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The global structure of the universe and the distribution of quasi-stellar objects
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Claims the paper makes
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In all known cases, the probability of creation of a low energy density inflationary universe is exponentially suppressed.
“In our opinion, however, the last 20 years of the debates on the probability of quantum creation a closed universe or an infinite open universe [15,16,17,19,21] demonstrated that in all known cases the probability of creation of a low energy density inflationary universe is exponentially suppressed.”
From Creation of a compact topologically nontrivial inflationary universe (2004) · cites this paper as [16]
If inflation can occur only at an energy density V much smaller than the Planck density, then the probability of quantum creation of a closed or infinitely large open inflationary universe is exponentially suppressed for all known choices of the wave function of the universe.
“If inflation can occur only at the energy density V much smaller than the Planck density, which is the case for many inflationary models based on string theory, then the probability of quantum creation of a closed or an infinitely large open inflationary universe is exponentially suppressed for all known choices of the wave function of the universe.”
From Creation of a compact topologically nontrivial inflationary universe (2004) · cites this paper as [16]
The probability of quantum creation of a closed inflationary universe is exponentially suppressed by P ~ exp(-24π^2/V(φ)).
“An investigation of this issue using Euclidean approach to quantum cosmology suggested [15,16] that the probability of quantum creation of a closed inflationary universe is exponentially suppressed by a factor of P ∼ exp - 24π 2 V (φ) .(1)”
From Creation of a compact topologically nontrivial inflationary universe (2004) · cites this paper as [16]
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No references could be resolved yet.
Research works printed but not linked: 9
- J. N. Bachall et al., Ap. J. Letters,157, L 77, 1969. · DOI
- G. R. Burbidge andE. M. Burbidge, Nature,224, 21, 1969 and lit. quoted there.M. B. Bell, Nature,224, 229, 1969.C. L. Cowan, Nature,224, 665, 1969. · DOI
- S. H. Plagemann et al., Nature,224, 875, 1969. · DOI
- O. Heckmann andE. Schücking, a) in “Handbuch der Physik” LIII, p. 515 (Springer, 1959); b) in “Gravitation, an introduction to current research” (ed. L. Witten), p. 438 (J. Wiley, New York, 1962).
- J. A. Wolf, Spaces of constant curvature (McGraw-Hill, 1967).W. Rinow, Die innere Geometrie der metrischen Raume (Springer, 1961) and lit. quoted there.
- A. R. Sandage, Observatory,88, 91, 1968.
- M. Süveges, Acta Phys. Hung.,20, 273, 1966.W. Kundt, in “Springer Tracts in Modern Physics”, Vol. 47, p. 124, 1968.Ja. B. Zeldovich andI. D. Novikov, Relativistic Astrophysics (in Russian), Moscow 1967. Appendix VII. · DOI
- A. Einstein andE. Straus, Rev. Mod. Phys.,17, 120, 1940. · DOI
- Ch. W. Misner, Phys. Rev. Letters,22, 1071, 1969. · DOI · Paper page
Cited by
Sorted by citations
Creation of a compact topologically nontrivial inflationary universe
Linde, A. (2004) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2004/10/004 · Cited by 158
Metadata
- Authors
- Paál, G.
- Venue
- Acta Physica Academiae Scientiarum Hungaricae
- Published
- 1971-03
- Volume
- 30
- Issue
- 1
- Pages
- 51-54
- ISSN
- 0001-6705
- Cited by
- 11
- References
- 0
- Language
- en
- Licence
- www.springer.com/tdm (tdm)
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