Dilatons, flatness, and the cosmological constant
- 15 January 1988
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 37 (2) , 333-337
- https://doi.org/10.1103/physrevd.37.333
Abstract
Symmetries that exist for some theories when considering small perturbations around some special backgrounds, which include flat but not de Sitter space and, among cosmological solutions spatially flat but generally not k=±1 Robertson-Walker solutions, are studied. The models examined include theories of nonconformally coupled massless fields, Brans-Dicke theories, and some supergravity theories with a dilaton field. The uses and possible consequences of these symmetries, among them the fact that they should help define the quantum vacuum in certain cosmologies, are discussed. Possible mechanisms which may solve the cosmological and flatness problems in which these symmetries play a role are also discussed.Keywords
This publication has 14 references indexed in Scilit:
- Spacetimes with cosmological constant and a conformal Killing field have constant curvatureClassical and Quantum Gravity, 1987
- Background symmetry and the flatness problemPhysics Letters B, 1986
- Quantum instability of de Sitter spacetimePhysical Review D, 1985
- No-scale supersymmetric GUTsNuclear Physics B, 1984
- No-scale supergravity models with a planck mass gravitinoPhysics Letters B, 1984
- Phenomenological SU(1, 1) supergravityNuclear Physics B, 1984
- No-scale supersymmetric standard modelPhysics Letters B, 1984
- Some Properties of a Cosmological Solution in the Brans-Dicke TheoryPhysical Review Letters, 1978
- Limits of spacetimesCommunications in Mathematical Physics, 1969
- Mach's Principle and a Relativistic Theory of GravitationPhysical Review B, 1961