Relaxing the cosmological constant
A non-zero cosmological constant allows massless gravitons to self-interact via a coupling of dimension three. If the cosmological constant is positive then the background geometry will subject gravitons to an enormous redshift. These two facts are together responsible for the severe infrared diverg...
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| Published in | Physics letters. B Vol. 301; no. 4; pp. 351 - 357 |
|---|---|
| Main Authors | , |
| Format | Journal Article |
| Language | English |
| Published |
Amsterdam
Elsevier B.V
11.03.1993
Elsevier Science |
| Subjects | |
| Online Access | Get full text |
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| Abstract | A non-zero cosmological constant allows massless gravitons to self-interact via a coupling of dimension three. If the cosmological constant is positive then the background geometry will subject gravitons to an enormous redshift. These two facts are together responsible for the severe infrared divergences which detailed, explicit calculations [N.C. Tsamis and R.P. Woodard, Strong infrared effects in quantum gravity, preprint CRETE-92-17, UFIFT-92-24] reveal in loop corrections to the gravitational force law. We argue that, as a result, the cosmological interaction has a finite lifetime. Furthermore, this lifetime is consistent with inflation. |
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| AbstractList | A non-zero cosmological constant allows massless gravitons to self-interact via a coupling of dimension three. If the cosmological constant is positive then the background geometry will subject gravitons to an enormous redshift. These two facts are together responsible for the severe infrared divergences which detailed, explicit calculations [N.C. Tsamis and R.P. Woodard, Strong infrared effects in quantum gravity, preprint CRETE-92-17, UFIFT-92-24] reveal in loop corrections to the gravitational force law. We argue that, as a result, the cosmological interaction has a finite lifetime. Furthermore, this lifetime is consistent with inflation. |
| Author | Woodard, R.P. Tsamis, N.C. |
| Author_xml | – sequence: 1 givenname: N.C. surname: Tsamis fullname: Tsamis, N.C. email: TSAMIS@IESL.FORTH.GR organization: Department of Physics, University of Crete, GR-71409 Iraklion, Crete, Greece – sequence: 2 givenname: R.P. surname: Woodard fullname: Woodard, R.P. email: WOODARD@UFHEPA.PHYS.UFL.EDU organization: Department of Physics, University of Florida, Gainesville, FL 32611, USA |
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| Cites_doi | 10.1103/RevModPhys.61.1 10.1016/0370-2693(87)90593-4 10.1016/0370-2693(91)91790-3 10.1103/PhysRev.52.54 10.1016/0370-2693(91)91711-4 10.1016/0370-2693(92)91174-8 10.1103/PhysRev.138.B988 10.1103/PhysRev.133.B1549 10.1016/0550-3213(82)90049-9 |
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| SubjectTerms | Exact sciences and technology Physics Quantum chromodynamics Specific theories and interaction models; particle systematics The physics of elementary particles and fields |
| Title | Relaxing the cosmological constant |
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