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The cosmological constant and the dimensionality of space-time
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As a consequence of the procedure, Λ effectively becomes dependent not only on the dimension but on the particular configuration itself.
“As a consequence of the procedure we suggest, Λ effectively becomes dependent not only on the dimension (as was anticipated before [7]) but on the particular configuration itself.”
From Dimensionality, topology, energy, the cosmological constant and signature change (1996) · cites this paper as [7]
Our approach, like Gasperini's, will predict n=4 as the lowest possible value, whereas minimization at constant Λ would lead to n→∞.
“As far as the dimension is concerned, our approach (like Gasperini's [7]) will predict n = 4 as the lowest possible value, whereas minimization at constant Λ would lead to n → ∞.”
From Dimensionality, topology, energy, the cosmological constant and signature change (1996) · cites this paper as [7]
Gasperini's approach holds that the energy U contained in the Euclidean n-geometry of an instanton is conserved under dimensional transitions.
“Our last comments concerns the approach suggested by Gasperini [7], that the energy U contained in the Euclidean n-geometry of an instanton is conserved under dimensional transitions.”
From Dimensionality, topology, energy, the cosmological constant and signature change (1996) · cites this paper as [7]
This is quite similar to the reasoning of Gasperini.
“This is quite similar to the reasoning of Gasperini [7].”
From Dimensionality, topology, energy, the cosmological constant and signature change (1996) · cites this paper as [7]
Citations
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No references could be resolved yet.
Research works printed but not linked: 10
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- Klebanov, 1989, Nucl. Phys. B, 317, 665, 10.1016/0550-3213(89)90538-5 · DOI · Paper page
- Rubakov, 1988, Phys. Lett. B, 214, 503, 10.1016/0370-2693(88)90108-6 · DOI
- Adler, 1989, Phys. Rev. Lett., 62, 373, 10.1103/PhysRevLett.62.373 · DOI
- Hawking, 1984, Phys. Lett. B, 134, 403, 10.1016/0370-2693(84)91370-4 · DOI
- Baum, 1983, Phys. Lett. B, 133, 185, 10.1016/0370-2693(83)90556-7 · DOI
- Myers, 1988, Baby universes in higher dimensional theories, NSF-ITP-88-156
- Volovich, 1989, Phys. Lett. B, 219, 66, 10.1016/0370-2693(89)90839-3 · DOI · Paper page
- Aurilia, 1980, Nucl. Phys. B, 176, 509, 10.1016/0550-3213(80)90466-6 · DOI
- Hawking, 1978, Phys. Rev. D, 18, 1747, 10.1103/PhysRevD.18.1747 · DOI
Cited by
Sorted by citations
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
- Gasperini, M.
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 1989-06
- Volume
- 224
- Issue
- 1-2
- Pages
- 49-52
- ISSN
- 0370-2693
- Cited by
- 7
- References
- 0
- Language
- en
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