The DOI matches its Crossref record; 6 of the 6 references it cites were found in a registry or an index.
Open universe from inflation
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Inflation in the string theory landscape scenario is eternal.
“This is an important consideration, because inflation in the string theory landscape scenario is eternal [37,38].”
From Creation of a compact topologically nontrivial inflationary universe (2004) · cites this paper as [38]
The Introduction and Concluding Remarks describe an open-universe model with old and new inflation, not a string-theory landscape scenario. The Concluding Remarks say that eternal inflation backward in time seems inconsistent with a finite bubble-nucleation rate, but do not establish whether inflation in a landscape scenario is eternal. Searched for string-theory landscape, eternal inflation, and future-directed inflation. (LLM, conf=0.76)
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Citations
Cites
Inflationary universe: A possible solution to the horizon and flatness problems
Guth, A. H. (1981) · Physical Review D · doi:10.1103/physrevd.23.347 · Cited by 9,983
Quantum Fields in Curved Space
Birrell, N. D., & Davies, P. C. W. (1982) · doi:10.1017/cbo9780511622632 · Cited by 8,354
Linde, A. D. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)91219-9 · Cited by 6,405
Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
Albrecht, A., & Steinhardt, P. J. (1982) · Physical Review Letters · doi:10.1103/physrevlett.48.1220 · Cited by 4,981
Gravitational effects on and of vacuum decay
Coleman, S., & De Luccia, F. (1980) · Physical Review D · doi:10.1103/physrevd.21.3305 · Cited by 1,537 · cited 12×
“There are two unsettling aspects of the Coleman-de Luccia instanton.”
BackgroundResultInfluentialCould the universe have recovered from a slow first-order phase transition?
Guth, A. H., & Weinberg, E. J. (1983) · Nuclear Physics B · doi:10.1016/0550-3213(83)90307-3 · Cited by 576
Flagged first, then by citations
Research works printed but not linked: 36
- J. R. Gott III, 1982, Nature (London), 295, 304, 10.1038/295304a0 · DOI
- J. R. Gott, 1984, Phys. Lett., 136B, 157, 10.1016/0370-2693(84)91171-7 · DOI
- A. Linde, 1983, Phys. Lett., 129B, 177, 10.1016/0370-2693(83)90837-7 · DOI · Paper page
- R. Carlitz, 1987, Phys. Rev. D, 36, 2327, 10.1103/PhysRevD.36.2327 · DOI
- D. Lyth, 1990, Phys. Lett. B, 252, 336, 10.1016/0370-2693(90)90548-K · DOI
- B. Ratra, 1995, Phys. Rev. D, 52, 1837, 10.1103/PhysRevD.52.1837 · DOI
- B. Ratra, 1994, Astrophys. J. Lett., 432, L5, 10.1086/187498 · DOI
- V. Rubakov, 1984, Nucl. Phys., B245, 481, 10.1016/0550-3213(84)90443-7 · DOI
- T. Vachaspati, 1991, Phys. Rev. D, 43, 3846, 10.1103/PhysRevD.43.3846 · DOI
- J. Garriga, 1992, Phys. Rev. D, 45, 3469, 10.1103/PhysRevD.45.3469 · DOI
- M. Sasaki, 1993, Prog. Theor. Phys., 90, 1019, 10.1143/ptp/90.5.1019 · DOI
- M. Sasaki, 1993, Phys. Lett. B, 317, 510, 10.1016/0370-2693(93)91364-S · DOI
- T. Tanaka, 1994, Phys. Rev. D, 50, 6444, 10.1103/PhysRevD.50.6444 · DOI
- S. Coleman, 1977, Phys. Rev. D, 15, 2929, 10.1103/PhysRevD.15.2929 · DOI · Paper page
- S. Coleman, 1977, Phys. Rev. D, 16, 1248, 10.1103/PhysRevD.16.1248 · DOI
- C. Callan, 1977, Phys. Rev. D, 16, 1763, 10.1103/PhysRevB.16.1763 · DOI
- L. Jensen, 1984, Nucl. Phys., B237, 176, 10.1016/0550-3213(84)90021-X · DOI
- A. S. Goncharov, 1986, Sov. J. Part. Nucl., 17, 369
- A. Linde, 1992, Nucl. Phys., B372, 421, 10.1016/0550-3213(92)90326-7 · DOI
- T. S. Bunch, 1978, Proc. R. Soc. London, A360, 117, 10.1098/rspa.1978.0060 · DOI
- B. Allen, 1985, Phys. Rev. D, 32, 3136, 10.1103/PhysRevD.32.3136 · DOI
- B. Rhatra, 1985, Phys. Rev. D, 31, 1931, 10.1103/PhysRevD.31.1931 · DOI
- D. Lyth, 1985, Phys. Rev. D, 31, 1792, 10.1103/PhysRevD.31.1792 · DOI
- M. Bander, 1966, Rev. Mod. Phys., 38, 346, 10.1103/RevModPhys.38.346 · DOI · Paper page
- A. Z. Dolginov, 1960, Sov. Phys. JETP, 10, 1022
- J. Bardeen, 1980, Phys. Rev. D, 22, 1882, 10.1103/PhysRevD.22.1882 · DOI · Paper page
- L. Abbott, 1986, Astrophys. J., 308, 462, 10.1086/164525 · DOI
- V. Mukhanov, 1992, Phys. Rep., 215, 203, 10.1016/0370-1573(92)90044-Z · DOI · Paper page
- H. Kodama, 1984, Prog. Theor. Phys. Suppl., 78, 1, 10.1143/PTPS.78.1 · DOI
- S. Hawking, 1982, Phys. Lett., 115B, 295, 10.1016/0370-2693(82)90373-2 · DOI
- A. A. Starobinsky, 1982, Phys. Lett., 117B, 175, 10.1016/0370-2693(82)90541-X · DOI
- A. H. Guth, 1982, Phys. Rev. Lett., 49, 1110, 10.1103/PhysRevLett.49.1110 · DOI
- J. Bardeen, 1983, Phys. Rev. D, 28, 679, 10.1103/PhysRevD.28.679 · DOI · Paper page
- A. Vilenkin, 1992, Phys. Rev. D, 46, 3255, 10.1103/PhysRevD.46.2355 · DOI
- A. Borde, 1994, Phys. Rev. Lett., 72, 3305, 10.1103/PhysRevLett.72.3305 · DOI · Paper page
- K. Yamamoto, 1995, Phys. Rev. D, 51, 2968, 10.1103/PhysRevD.51.2968 · DOI
Cited by
Sorted by citations
The evidence for a spatially flat Universe
Efstathiou, G., & Gratton, S. (2020) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1093/mnrasl/slaa093 · Cited by 203
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
Garriga, J., & Vilenkin, A. (1998) · Physical Review D · doi:10.1103/physrevd.57.2230 · Cited by 154
The galaxy power spectrum take on spatial curvature and cosmic concordance
Vagnozzi, S., Di Valentino, E., Gariazzo, S., Melchiorri, A., Mena, O., & Silk, J. (2021) · Physics of the Dark Universe · doi:10.1016/j.dark.2021.100851 · Cited by 138
Can the Universe create itself?
Gott, J. R., & Li, L.-X. (1998) · Physical Review D · doi:10.1103/physrevd.58.023501 · Cited by 127
Holographic framework for eternal inflation
Freivogel, B., Sekino, Y., Susskind, L., & Yeh, C.-P. (2006) · Physical Review D · doi:10.1103/physrevd.74.086003 · Cited by 117
Steady state eternal inflation
Aguirre, A., & Gratton, S. (2002) · Physical Review D · doi:10.1103/physrevd.65.083507 · Cited by 68
Curvature constraints from large scale structure
Dio, E. D., Montanari, F., Raccanelli, A., Durrer, R., Kamionkowski, M., & Lesgourgues, J. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/06/013 · Cited by 61
Quantum cosmology and open universes
Coule, D. H., & Martin, J. (2000) · Physical Review D · doi:10.1103/physrevd.61.063501 · Cited by 60
A critical review of inflation
Turok, N. (2002) · Classical and Quantum Gravity · doi:10.1088/0264-9381/19/13/305 · Cited by 58
Self-citationObservable effects of anisotropic bubble nucleation
Blanco-Pillado, J. J., & Salem, M. P. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/07/007 · Cited by 44
Abdalla, E., Abellán, G. F., Aboubrahim, A., Agnello, A., Akarsu, Ö., Akrami, Y., Alestas, G., Aloni, D., Amendola, L., Anchordoqui, L. A., et al. (2022) · Journal of High Energy Astrophysics · doi:10.1016/j.jheap.2022.04.002 · Cited by 37
Metadata
- Authors
- Bucher, M., Goldhaber, A. S., & Turok, N.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1995-09-15
- Volume
- 52
- Issue
- 6
- Pages
- 3314-3337
- ISSN
- 0556-2821
- Cited by
- 281
- References
- 6
- Language
- en
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