1995
DOI: 10.1016/0550-3213(95)00222-e
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The Chern-Simons invariant as the natural time variable for classical and quantum cosmology

Abstract: We propose that the Chern-Simons invariant of the Ashtekar-Sen connection (or its imaginary part in the Lorentzian case) is the natural internal time coordinate for classical and quantum cosmology. The reasons for this are: 1) It is a function on the gauge and di eomorphism invariant con guration space, whose gradient is orthogonal to the two p h ysical degrees of freedom, in the metric de ned by the Ashtekar formulation of general relativity.2) The imaginary part of the Chern-Simons form reduces in the limit … Show more

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Cited by 72 publications
(127 citation statements)
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“…Recently Smolin and Soo argued that since the proper arena of the dynamics is the phase space rather than the spacetime and in a canonical quantum theory the carrying space of the wave functions is the configuration space, we should find a natural time variable in the configuration space and not in the spacetime. For such a natural time variable in the configuration space they suggested the imaginary part of the Chern-Simons functional built from the complex Ashtekar connection [13]. Although the quantum dynamics must be formulated in the configuration space (or on the phase space endowed with an appropriate polarization), we think that in the classical theory time in the phase space or configuration space (i.e.…”
Section: Introductionmentioning
confidence: 99%
“…Recently Smolin and Soo argued that since the proper arena of the dynamics is the phase space rather than the spacetime and in a canonical quantum theory the carrying space of the wave functions is the configuration space, we should find a natural time variable in the configuration space and not in the spacetime. For such a natural time variable in the configuration space they suggested the imaginary part of the Chern-Simons functional built from the complex Ashtekar connection [13]. Although the quantum dynamics must be formulated in the configuration space (or on the phase space endowed with an appropriate polarization), we think that in the classical theory time in the phase space or configuration space (i.e.…”
Section: Introductionmentioning
confidence: 99%
“…These reduce, in the limit of vanishing slow role parameter,V /V , to the Chern-Simons invariant of the Ashtekar connection. This is good, as the latter is known to be the Hamilton-Jacobi function for deSitter spacetime [9,13,12,14]. By exponentiating the actions of these solutions, one obtains a semiclassical state that reduces in the same limit to the Kodama state.…”
Section: Introductionmentioning
confidence: 87%
“…Furthermore, for constant cosmological constant, there is an exact solution to the quantum constraints that define the full quantum general relativity, discovered by Kodama [9], which has both an exact Planck scale description and a semiclassical interpretation in terms of deSitter spacetime. While there are open issues of interpretation concerning this state [10,11,19], it is also true that it can be used as the basis of both non-perturbative and semiclassical caclulations [12,13,14]. Furthermore, exact results in the loop representation have made possible an understanding of the temperature and entropy of deSitter spacetime [12,14] in terms of the kinematics of the quantum gravitational field.…”
Section: Introductionmentioning
confidence: 99%
“…Under a large gauge transformation characterized by winding number n, Y CS → Y CS + 4π 2 n [15], and the Chern-Simons state transforms as CS (A) → e inθ CS (A) [6]. The inclusion of matter perturbations reproduce standard quantum field theory on de Sitter background [16], while linearizing the quantum theory one recovers long-wavelength gravitons on de Sitter [11]. In this sense the Chern-Simons state is a genuine ground state of the theory.…”
mentioning
confidence: 88%