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Hi Ruta, thanks for joining the conversation. Nice to hear from you! You quoted Rovelli's September 2012 paper, in which he defines and uses several types of TIME.
I had better copy the abstract and the passage to give context to what you were quoting. Certainly one does not have to have a 4D block universe with a physically meaningful time coordinate being one of the dimensions merely in order to model change with the passage of time. You in particular would be expected to know this better than many others, including myself.
But here in this paper we have no lack of times: proper time, and thermal time, and a local version involving a local hamiltonian.
You have many choices for what fluctuation can mean, of course, since you have several opportunities to describe things as changing with the passage of time.
I think in that page 1 paragraph it is meant in a general sense without specifying the particular time-evolution. But anyway I will copy the material to get it all together where we can look at it:
http://arxiv.org/abs/1209.0065
General relativistic statistical mechanics
Carlo Rovelli
(Submitted on 1 Sep 2012)
Understanding thermodynamics and statistical mechanics in the full general relativistic context is an open problem. I give tentative definitions of equilibrium state, mean values, mean geometry, entropy and temperature, which reduce to the conventional ones in the non-relativistic limit, but remain valid for a general covariant theory. The formalism extends to quantum theory. The construction builds on the idea of thermal time, on a notion of locality for this time, and on the distinction between global and local temperature. The last is the temperature measured by a local thermometer, and is given by kT = [STRIKE]h[/STRIKE] dτ/ds, with k the Boltzmann constant, [STRIKE]h[/STRIKE] the Planck constant, ds proper time and dτ the equilibrium thermal time.
9 pages. A tentative second step in the thermal time direction, 10 years after the paper with Connes. The aim is the full thermodynamics of gravity. The language of the paper is a bit technical: look at the Appendix first.
==1209.0065 page 1 excerpt==
Thermodynamics and statistical mechanics are powerful and vastly general tools. But their usual formulation works only in the non-general-relativistic limit. Can they be extended to fully general relativistic systems?
The problem can be posed in physical terms: we do not know the position of each molecule of a gas, or the value of the electromagnetic field at each point in a hot cavity, as these fluctuate thermally, but we can give a statistical description of their properties. For the same reason, we do not know the exact value of the gravitational field, which is to say the exact form of the spacetime geometry around us, since nothing forbids it from fluctuating like any other field to which it is coupled. Is there a theoretical tool for describing these fluctuations?
The problem should not be confused with thermodynamics and statistical mechanics on curved spacetime. The difference is the same as the distinction between the dynamics of matter on a given curved geometry versus the dynamics of geometry itself, or the dynamics of charged particles versus dynamics of the electromagnetic field. Thermodynamics on curved spacetime is well understood (see the classic [1]) and statistical mechanics on curved spacetimes is an interesting domain (for a recent intriguing perspective see [2]). The problem is also distinct from “stochastic gravity” [3, 4], where metric fluctuations are generated by a Einstein-Langevin equation and related to semiclassical effects of quantum theory. Here, instead, the problem is the just the thermal behavior of conventional gravity.1
A number of puzzling relations between gravity and thermodynamics (or gravity, thermodynamics and quantum theory) have been extensively discussed in the literature [5–14]. Among the most intriguing are probably Jacobson’s celebrated derivation of the Einstein equations from the entropy-area relation [15, 16], and Penrose Weil-curvature hypothesis [17, 18]. These are very suggestive, but perhaps their significance cannot be evaluated until we better understand standard general covariant thermodynamics.
==endquote==[/QUOTE]
Well you are quoting Rovelli so your question is what does HE mean, so you could write and ask him. But I will venture to suggest that what he means is the spacetime geometry cbanges with the passage of time.RUTA said:What can it mean to say "spacetime fluctuates"...?
I had better copy the abstract and the passage to give context to what you were quoting. Certainly one does not have to have a 4D block universe with a physically meaningful time coordinate being one of the dimensions merely in order to model change with the passage of time. You in particular would be expected to know this better than many others, including myself.
You have many choices for what fluctuation can mean, of course, since you have several opportunities to describe things as changing with the passage of time.
I think in that page 1 paragraph it is meant in a general sense without specifying the particular time-evolution. But anyway I will copy the material to get it all together where we can look at it:
http://arxiv.org/abs/1209.0065
General relativistic statistical mechanics
Carlo Rovelli
(Submitted on 1 Sep 2012)
Understanding thermodynamics and statistical mechanics in the full general relativistic context is an open problem. I give tentative definitions of equilibrium state, mean values, mean geometry, entropy and temperature, which reduce to the conventional ones in the non-relativistic limit, but remain valid for a general covariant theory. The formalism extends to quantum theory. The construction builds on the idea of thermal time, on a notion of locality for this time, and on the distinction between global and local temperature. The last is the temperature measured by a local thermometer, and is given by kT = [STRIKE]h[/STRIKE] dτ/ds, with k the Boltzmann constant, [STRIKE]h[/STRIKE] the Planck constant, ds proper time and dτ the equilibrium thermal time.
9 pages. A tentative second step in the thermal time direction, 10 years after the paper with Connes. The aim is the full thermodynamics of gravity. The language of the paper is a bit technical: look at the Appendix first.
==1209.0065 page 1 excerpt==
Thermodynamics and statistical mechanics are powerful and vastly general tools. But their usual formulation works only in the non-general-relativistic limit. Can they be extended to fully general relativistic systems?
The problem can be posed in physical terms: we do not know the position of each molecule of a gas, or the value of the electromagnetic field at each point in a hot cavity, as these fluctuate thermally, but we can give a statistical description of their properties. For the same reason, we do not know the exact value of the gravitational field, which is to say the exact form of the spacetime geometry around us, since nothing forbids it from fluctuating like any other field to which it is coupled. Is there a theoretical tool for describing these fluctuations?
The problem should not be confused with thermodynamics and statistical mechanics on curved spacetime. The difference is the same as the distinction between the dynamics of matter on a given curved geometry versus the dynamics of geometry itself, or the dynamics of charged particles versus dynamics of the electromagnetic field. Thermodynamics on curved spacetime is well understood (see the classic [1]) and statistical mechanics on curved spacetimes is an interesting domain (for a recent intriguing perspective see [2]). The problem is also distinct from “stochastic gravity” [3, 4], where metric fluctuations are generated by a Einstein-Langevin equation and related to semiclassical effects of quantum theory. Here, instead, the problem is the just the thermal behavior of conventional gravity.1
A number of puzzling relations between gravity and thermodynamics (or gravity, thermodynamics and quantum theory) have been extensively discussed in the literature [5–14]. Among the most intriguing are probably Jacobson’s celebrated derivation of the Einstein equations from the entropy-area relation [15, 16], and Penrose Weil-curvature hypothesis [17, 18]. These are very suggestive, but perhaps their significance cannot be evaluated until we better understand standard general covariant thermodynamics.
==endquote==[/QUOTE]
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