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Wormholes and the cosmological constant
Abstract
We review Coleman’s wormhole mechanism for the vanishing of the cosmological constant. We show that in a minisuperspace model wormhole-connected universes dominate the path integral. We also provide evidence that the Euclidean path integral over geometries with spherical topology is unstable with respect to formation of infinitely many wormhole-connected 4-spheres. Consistency is restored by summing over all topologies, which leads to Coleman’s result. Coleman’s argument for determination of other parameters is reviewed and applied to the mass of the pion. A discouraging result is found that the pion mass is driven to zero. We also consider qualitatively the implications of the wormhole theory for cosmology. We argue that a small number of universes containing matter and energy may exist in contact with infinitely many cold and empty universes. Contact with the cold universes insures that the cosmological constant in the warm ones is zero
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In the Vilenkin-Linde tunneling wave function formalism, the Euclidean action enters with different sign, so probabilities are P ∼ exp(I).
“In a sense, the Euclidean action enters this formalism with different sign, so that one ends up with probabilities P ∼ exp(I).”
From Dimensionality, topology, energy, the cosmological constant and signature change (1996) · cites this paper as [36]
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Quantum Fields in Curved Space
Birrell, N. D., & Davies, P. C. W. (1982) · doi:10.1017/cbo9780511622632 · Cited by 8,354
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Research works printed but not linked: 20
- Linde, 1988, Phys. Lett., B200, 272, 10.1016/0370-2693(88)90770-8 · DOI
- Hawking, 1987, Phys. Lett., B195, 337, 10.1016/0370-2693(87)90028-1 · DOI
- Horowitz, 1984, Nucl. Phys., B238, 653
- Strominger, 1984, Phys. Rev. Lett., 52, 1733, 10.1103/PhysRevLett.52.1733 · DOI
- See also more recent work by S. Giddings and A. Strominger, Harvard preprint HUTP-87/A067;
- Lavrelashvili, 1987, JETP Lett., 46, 167
- Hawking, 1978, Nucl. Phys., B144, 349, 10.1016/0550-3213(78)90375-9 · DOI
- Hawking, 1984, Phys. Lett., B134, 403, 10.1016/0370-2693(84)91370-4 · DOI
- S. Coleman, Harvard preprint HUTP-88/A008
- S. Giddings and A. Strominger, Harvard preprint HUTP-88/A006
- T. Banks, I. Klebanov, L. Susskind, talk delivered by T. Banks at the Yerevan Conference on High Energy Physics, in preparation
- T. Banks, Santa Cruz preprint SCIPP-88/09, to be published in Nucl. Phys. B. The relation between this work and the present paper will be discussed in ref. [8]
- S. Giddings and A. Strominger, Harvard preprint HUTP-88/A036
- S. Coleman, Harvard preprint HUTP-88/A022
- Gibbons, 1978, Nucl. Phys., B138, 141, 10.1016/0550-3213(78)90161-X · DOI · Paper page
- Hartle, 1983, Phys. Rev., D28, 2960
- Vilenkin, 1988, Phys. Rev., D37, 888
- B. Grinstein and M. Wise, Caltech preprint CALT-68-1505
- Candelas, 1983, Nucl. Phys., B237, 397
- J. Halliwell, ITP Santa Barbara preprint NSF-ITP-88-25
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Weinberg, S. (1989) · Reviews of Modern Physics · doi:10.1103/revmodphys.61.1 · Cited by 7,341
QUANTUM GRAVITY AND MINIMUM LENGTH
GARAY, L. J. (1995) · International Journal of Modern Physics A · doi:10.1142/s0217751x95000085 · Cited by 1,371
Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology
Hebecker, A., Mikhail, T., & Soler, P. (2018) · Frontiers in Astronomy and Space Sciences · doi:10.3389/fspas.2018.00035 · Cited by 136
Wormholes in spacetime and the constants of nature
Preskill, J. (1989) · Nuclear Physics B · doi:10.1016/0550-3213(89)90592-0 · Cited by 87
Can gravitational instantons really constrain axion inflation?
Hebecker, A., Mangat, P., Theisen, S., & Witkowski, L. T. (2017) · Journal of High Energy Physics · doi:10.1007/jhep02(2017)097 · Cited by 66
Lyons, A., & Hawking, S. W. (1991) · Physical Review D · doi:10.1103/physrevd.44.3802 · Cited by 25
Dimensionality, topology, energy, the cosmological constant and signature change
Embacher, F. (1996) · Classical and Quantum Gravity · doi:10.1088/0264-9381/13/5/012 · Cited by 6
Metadata
- Authors
- Klebanov, I., Susskind, L., & Banks, T.
- Venue
- Nuclear Physics B
- Publisher
- Elsevier BV
- Published
- 1989-05
- Volume
- 317
- Issue
- 3
- Pages
- 665-692
- ISSN
- 0550-3213
- Cited by
- 167
- References
- 1
- Language
- en
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