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Scale-invariance in gravity and implications for the cosmological constant

Bryan Kelleher 2004 Class. Quantum Grav. 21 2623-2639   doi: 10.1088/0264-9381/21/11/008  Help

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Bryan Kelleher
Physics Department, University College, Cork, Republic of Ireland
E-mail: bk@physics.ucc.ie

Abstract. Recently, a scale invariant theory was constructed by imposing a conformal symmetry on general relativity. The imposition of this symmetry changed the configuration space from superspace—the space of all Riemannian 3-metrics modulo diffeomorphisms—to conformal superspace—the space of all Riemannian 3-metrics modulo diffeomorphisms and conformal transformations. However, despite numerous attractive features, the theory suffers from at least one major problem: the volume of the universe is no longer a dynamical variable. In attempting to resolve this problem a new theory is found which has several surprising and attractive features from both quantization and cosmological perspectives. Furthermore, it is an extremely restrictive theory and thus may provide testable predictions quickly and easily. One particularly interesting feature of the theory is the resolution of the cosmological constant problem.

PACS numbers: 04.20.Cv, 04.20.Fy, 11.10.Ef

Print publication: Issue 11 (7 June 2004)
Received 21 October 2003
Published 26 April 2004

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