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Trace anomaly driven inflation
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For even-dimensional homogeneous and isotropic FRW cosmologies, the trace anomaly for conformal quantum fields is known.
“For example, for even-dimensional homogeneous and isotropic FRW cosmologies, the trace anomaly for conformal quantum fields is known [178,179].”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [178]
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Cites
Anti de Sitter space and holography
Witten, E. (1998) · Advances in Theoretical and Mathematical Physics · doi:10.4310/atmp.1998.v2.n2.a2 · Cited by 13,070
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
Gauge theory correlators from non-critical string theory
Gubser, S. S., Klebanov, I. R., & Polyakov, A. M. (1998) · Physics Letters B · doi:10.1016/s0370-2693(98)00377-3 · Cited by 9,307
Quantum Fields in Curved Space
Birrell, N. D., & Davies, P. C. W. (1982) · doi:10.1017/cbo9780511622632 · Cited by 8,354
A new type of isotropic cosmological models without singularity
Starobinsky, A. A. (1980) · Physics Letters B · doi:10.1016/0370-2693(80)90670-x · Cited by 7,677
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
Hartle, J. B., & Hawking, S. W. (1983) · Physical Review D · doi:10.1103/physrevd.28.2960 · Cited by 3,027
Self-citationGravitational 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
Supercooled phase transitions in the very early universe
Hawking, S. W., & Moss, I. L. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)90946-7 · Cited by 816
Self-citationSurface terms as counterterms in the AdS-CFT correspondence
Emparan, R., Johnson, C. V., & Myers, R. C. (1999) · Physical Review D · doi:10.1103/physrevd.60.104001 · Cited by 703
Flagged first, then by citations
Research works printed but not linked: 42
- P. de Bernardis, 2000, Nature (London), 404, 955, 10.1038/35010035 · DOI
- G.F. Mazenko, 1985, Phys. Rev. D, 31, 273, 10.1103/PhysRevD.31.273 · DOI
- A.D. Linde, 1983, Phys. Lett., 129B, 177, 10.1016/0370-2693(83)90837-7 · DOI · Paper page
- A.D. Linde, 1996, Phys. Rev. D, 54, 2504, 10.1103/PhysRevD.54.2504 · DOI
- S.W. Hawking, 1998, Phys. Lett. B, 425, 25, 10.1016/S0370-2693(98)00234-2 · DOI · Paper page
- C. Bennett, 1996, Astrophys. J. Lett., 464, L1, 10.1086/310075 · DOI
- D.M. Capper, 1974, Nuovo Cimento A, 23, 173, 10.1007/BF02748300 · DOI
- M.J. Duff, 1994, Class. Quantum Grav., 11, 1387, 10.1088/0264-9381/11/6/004 · DOI
- J.S. Dowker, 1976, Phys. Rev. D, 13, 3224, 10.1103/PhysRevD.13.3224 · DOI
- M.V. Fischetti, 1979, Phys. Rev. D, 20, 1757, 10.1103/PhysRevD.20.1757 · DOI · Paper page
- A. Vilenkin, 1985, Phys. Rev. D, 32, 2511, 10.1103/PhysRevD.32.2511 · DOI
- A.A. Starobinsky, 1981, JETP Lett., 34, 438
- A.A. Starobinsky, 1983, Sov. Astron. Lett., 9, 302
- J. Maldacena, 1998, Adv. Theor. Math. Phys., 2, 231, 10.4310/ATMP.1998.v2.n2.a1 · DOI · Paper page
- E. Tomboulis, 1977, Phys. Lett., 70B, 361, 10.1016/0370-2693(77)90678-5 · DOI
- L. Randall, 1999, Phys. Rev. Lett., 83, 4690, 10.1103/PhysRevLett.83.4690 · DOI · Paper page
- S.W. Hawking, 2000, Phys. Rev. D, 62, 043501, 10.1103/PhysRevD.62.043501 · DOI
- M. Henningson, 1998, J. High Energy Phys., 07, 023, 10.1088/1126-6708/1998/07/023 · DOI · Paper page
- G.W. Gibbons, 1978, Nucl. Phys., B146, 90, 10.1016/0550-3213(78)90434-0 · DOI · Paper page
- H. Osborn, 2000, Nucl. Phys., B571, 287, 10.1016/S0550-3213(99)00775-0 · DOI
- A. Higuchi, 1987, J. Math. Phys., 28, 1553, 10.1063/1.527513 · DOI
- G.W. Gibbons, 1977, Phys. Rev. D, 15, 2752, 10.1103/PhysRevD.15.2752 · DOI · Paper page
- A. Tseytlin, 1998, Nucl. Phys., B533, 88
- M. Henningson, 2000, Fortschr. Phys., 48, 125, 10.1002/(SICI)1521-3978(20001)48:1/3<125::AID-PROP125>3.0.CO;2-B · DOI
- V. Balasubramanian, 1999, Commun. Math. Phys., 208, 413, 10.1007/s002200050764 · DOI · Paper page
- P. Kraus, 1999, Nucl. Phys., B563, 259, 10.1016/S0550-3213(99)00549-0 · DOI · Paper page
- S.W. Hawking, 1982, Phys. Lett., 115B, 295, 10.1016/0370-2693(82)90373-2 · DOI
- S. Coleman, 1969, Theory and Phenomenology in Particle Physics
- S. Gratton, 1999, Phys. Rev. D, 60, 123507, 10.1103/PhysRevD.60.123507 · DOI
- T. Hertog, 2000, Phys. Rev. D, 62, 083514, 10.1103/PhysRevD.62.083514 · DOI
- S. Nojiri, 2000, Phys. Rev. D, 62, 064006, 10.1103/PhysRevD.62.064006 · DOI
- S. Nojiri, 2000, Phys. Lett. B, 484, 119, 10.1016/S0370-2693(00)00629-8 · DOI
- S. Nojiri, 2000, Phys. Rev. D, 62, 104003, 10.1103/PhysRevD.62.104003 · DOI
- L. Anchordoqui, 2000, J. High Energy Phys., 10, 050, 10.1088/1126-6708/2000/10/050 · DOI
- H.A. Chamblin, 1999, Nucl. Phys., B562, 133, 10.1016/S0550-3213(99)00520-9 · DOI
- S. Mukohyama, 2000, Phys. Rev. D, 62, 084015, 10.1103/PhysRevD.62.084015 · DOI
- H. Kodama, 2000, Phys. Rev. D, 62, 064022, 10.1103/PhysRevD.62.064022 · DOI
- R. Maartens, 2000, Phys. Rev. D, 62, 084023, 10.1103/PhysRevD.62.084023 · DOI
- D. Langlois, 2000, Phys. Rev. D, 62, 126012, 10.1103/PhysRevD.62.126012 · DOI
- C. van de Bruck, 2000, Phys. Rev. D, 62, 123515, 10.1103/PhysRevD.62.123515 · DOI
- K. Koyama, 2000, Phys. Rev. D, 62, 123502, 10.1103/PhysRevD.62.123502 · DOI
- B. Whitt, 1984, Phys. Lett., 145B, 176, 10.1016/0370-2693(84)90332-0 · DOI
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Testing general relativity in cosmology
Ishak, M. (2019) · Living Reviews in Relativity · doi:10.1007/s41114-018-0017-4 · Cited by 449
Induced quantum metric fluctuations and the validity of semiclassical gravity
Hu, B. L., Roura, A., & Verdaguer, E. (2004) · Physical Review D · doi:10.1103/physrevd.70.044002 · Cited by 82
A critical review of inflation
Turok, N. (2002) · Classical and Quantum Gravity · doi:10.1088/0264-9381/19/13/305 · Cited by 58
Three-Dimensional Quantum Black Holes: A Primer
Panella, E., Pedraza, J. F., & Svesko, A. (2024) · Universe · doi:10.3390/universe10090358 · Cited by 24
Metadata
- Authors
- Hawking, S. W., Hertog, T., & Reall, H. S.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2001-03-05
- Volume
- 63
- Issue
- 8
- ISSN
- 0556-2821
- 1089-4918
- Cited by
- 148
- References
- 11
- Language
- en
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