1990
DOI: 10.1007/bf00671323
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Quantum corrections to the spacetime metric from geometric phase space quantization

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Cited by 63 publications
(57 citation statements)
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“…The resolution of classical singularities under the assumption of a maximal acceleration has been studied using canonical methods for Rindler [24], Schwarzschild [25], Reissner-Nordstrom [26], Kerr-Newman [27] and Friedman-Lemaître [28] metrics. Here we consider a simple homogeneous and isotropic cosmological model, with vanishing spatial curvature and pressure.…”
Section: Cosmologymentioning
confidence: 99%
“…The resolution of classical singularities under the assumption of a maximal acceleration has been studied using canonical methods for Rindler [24], Schwarzschild [25], Reissner-Nordstrom [26], Kerr-Newman [27] and Friedman-Lemaître [28] metrics. Here we consider a simple homogeneous and isotropic cosmological model, with vanishing spatial curvature and pressure.…”
Section: Cosmologymentioning
confidence: 99%
“…The starting point of our consideration will be the classical model of a relativistic particle with maximal proper acceleration [12][13][14]. Upon quantizing this model the equations for the wave functions can be treat as the dynamical equations for the corresponding field function.…”
Section: Introductionmentioning
confidence: 99%
“…In all these works space-time is endowed with a causal structure in which the proper accelerations of massive particles are limited. This is achieved by means of an embedding procedure pioneered in [20] and discussed at length in [16], [21] . The procedure stipulates that the line element experienced by an accelerating particle is represented by…”
mentioning
confidence: 99%
“…[1], [2], [16]. Though the effective potentials experienced by classical and quantum particles are different, their effects are similar.…”
mentioning
confidence: 99%