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In the recent analysis by Mielczarek, Linsefors, and Barrau, the key parameter is ρc the highest density achieved in the bounce. The extremes (negative and then positive) of the Hubble rate occur symmetrically at density ρc/2
In the contraction preceding bounce, as the density approaches ρc/2, lightcones narrow down and the geometry becomes in a sense less Lorentzian. Interaction between neighboring points is suppressed.
Precisely at density ρc/2 the geometry FREEZES into a Euclidean phase consisting of a bundle of parallel timelines. Spatial derivatives are suppressed.
However density continues to rise, reaching ρc, where it rebounds and declines back down to ρc/2. During that Euclidean phase of extreme condensation with interaction turned off, I would say that time does not exist. I cannot imagine how a clock could be constructed under such circumstances, an oscillator or similar cyclical process with a counter recording the cycles. That is the operational meaning of time. If you cannot imagine measuring time, nothing corresponding to that idea exists.
Instead, the excursion of density, from ρc/2 up to ρc, and back down again, can (if you wish) serve to parametrize the bundle of timelines which spacetime has momentarily become.
The interesting thing, which is the focus of the MLB paper, is the MELTING of this Euclidean timeless phase that occurs after the bounce starting at ρc/2 and restores the Lorentzian signature.
MLB call the 3d hypersurface at ρc/2 the "silent surface" and they suggest this would be a good place to impose initial conditions and to analyze the power spectrum of quantum fluctuations. Up to that point, interactions have been turned off so neighboring points are "deaf" to each other. I suppose that is the basic reason they speak of it as "silence". This isolation or spatial disconnectedness is reminiscent of the classical 1970 finding by three Russian physicists (B, K, and L) formerly members of Lev Landau's group.
http://arxiv.org/abs/1411.0272v1
Silent initial conditions for cosmological perturbations with a change of space-time signature
Jakub Mielczarek, Linda Linsefors, Aurelien Barrau
(Submitted on 2 Nov 2014)
Recent calculations in loop quantum cosmology suggest that a transition from a Lorentzian to an Euclidean space-time might take place in the very early Universe. The transition point leads to a state of silence, characterized by a vanishing speed of light. This behavior can be interpreted as a decoupling of different space points, similar to the one characterizing the BKL phase.
In this study, we address the issue of imposing initial conditions for the cosmological perturbations at the transition point between the Lorentzian and Euclidean phases. Motivated by the decoupling of space points, initial conditions characterized by a lack of correlations are investigated. We show that the "white noise" initial conditions are supported by the analysis of the vacuum state in the Euclidean regime adjacent to the state of silence...
12 pages, 8 figures
In the contraction preceding bounce, as the density approaches ρc/2, lightcones narrow down and the geometry becomes in a sense less Lorentzian. Interaction between neighboring points is suppressed.
Precisely at density ρc/2 the geometry FREEZES into a Euclidean phase consisting of a bundle of parallel timelines. Spatial derivatives are suppressed.
However density continues to rise, reaching ρc, where it rebounds and declines back down to ρc/2. During that Euclidean phase of extreme condensation with interaction turned off, I would say that time does not exist. I cannot imagine how a clock could be constructed under such circumstances, an oscillator or similar cyclical process with a counter recording the cycles. That is the operational meaning of time. If you cannot imagine measuring time, nothing corresponding to that idea exists.
Instead, the excursion of density, from ρc/2 up to ρc, and back down again, can (if you wish) serve to parametrize the bundle of timelines which spacetime has momentarily become.
The interesting thing, which is the focus of the MLB paper, is the MELTING of this Euclidean timeless phase that occurs after the bounce starting at ρc/2 and restores the Lorentzian signature.
MLB call the 3d hypersurface at ρc/2 the "silent surface" and they suggest this would be a good place to impose initial conditions and to analyze the power spectrum of quantum fluctuations. Up to that point, interactions have been turned off so neighboring points are "deaf" to each other. I suppose that is the basic reason they speak of it as "silence". This isolation or spatial disconnectedness is reminiscent of the classical 1970 finding by three Russian physicists (B, K, and L) formerly members of Lev Landau's group.
http://arxiv.org/abs/1411.0272v1
Silent initial conditions for cosmological perturbations with a change of space-time signature
Jakub Mielczarek, Linda Linsefors, Aurelien Barrau
(Submitted on 2 Nov 2014)
Recent calculations in loop quantum cosmology suggest that a transition from a Lorentzian to an Euclidean space-time might take place in the very early Universe. The transition point leads to a state of silence, characterized by a vanishing speed of light. This behavior can be interpreted as a decoupling of different space points, similar to the one characterizing the BKL phase.
In this study, we address the issue of imposing initial conditions for the cosmological perturbations at the transition point between the Lorentzian and Euclidean phases. Motivated by the decoupling of space points, initial conditions characterized by a lack of correlations are investigated. We show that the "white noise" initial conditions are supported by the analysis of the vacuum state in the Euclidean regime adjacent to the state of silence...
12 pages, 8 figures
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