Global emergent time, how does Tomita flow work?

  • #61
The Tomita flow, and thermal time, came up in one of the Loops parallel session talks that I think of at the moment: one by Goffredo Chirco. There may be others.
The parallel session abstracts are here:
http://www.perimeterinstitute.ca/sites/perimeter-www.pi.local/files/conferences/attachments/Parallel%20Session%20Abstracts_7.pdf

To find the videos, I can use the index I just posted in the "Loops 2013 talks" thread:
https://www.physicsforums.com/showthread.php?p=4461021#post4461021
Looking down the alphabetical list for speaker's name you see:
Goffredo Chirco, Aix-Marseille University http://pirsa.org/13070085 (0)

Conveniently, the starting time is minute zero, so we get the talk as soon as we click on the link and select flash. There is no need to wait for buffering before we start.

The KMS condition, which is essential to thermal time, also came up in this talk:
Daniele Pranzetti, Albert Einstein Institute http://pirsa.org/13070054 (0)
The paper this was based on also treats Tomita time, but that part wasn't covered in the 20-minute version.These are two outstanding talks. I wonder what others in the Loops 2013 collection deal with Tomita time. Can anybody suggest others?

The basic reason it's so interesting is that this is a global time which is observer-independent.
Instead of depending on a choice of observer, it depends on the process whose quantum state is known. That is, a vector in a boundary Hilbert space that contains information about past during and future. And more or less equivalently thanks to Israel Gelfand, a positive functional defined on the C* algebra of the process. Here "state" does not mean "state at a given instant of time". The state is a quantum description of what can be known about an entire process occurring in an enclosed spacetime region.

The state gives rise to time. It is with this tomita global time that the researchers propose to work out a general covariant QFT and a general covariant statistical mechanics. this is new because up to now these constructs have been formulated using some postulated background or observer-dependent time.

EDIT: when you click on the link for Chirco it will say that the first talk is by Bianca Dittrich, but she gave her talk in a different session and the first is actually the one you want.
 
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  • #62
I googled "tomita flow modular flow" and you are the one of the top Google finds. Would you like to comment on whether modular flow in footnote 16 on p42 of http://arxiv.org/abs/1305.3182 is Tomita flow? Bianchi is cited in ref 16 and 63. One of the authors is an "LQG guy" :p

Footnote 16 on p42, "These unitary operators implement an evolution for an internal time . This time flow is called the modular flow [29]."

Also footnote 3 on p4, "The simplest example is given by considering a global thermal state, with temperature T, and taking V to be the whole space. Then, the modular Hamiltonian is simply the ordinary (local) Hamiltonian divided by T, as is evident from eq. (1.5), and so H simply generates ordinary time translations."

marcus said:
A recent paper by Robert Oeckl on the Boundary Formulation of QT interestingly refers to the (M,ω) picture, suggesting that he, too, may be looking at it as a possible way to go.
http://arxiv.org/abs/1212.5571
A positive formalism for quantum theory in the general boundary formulation
Robert Oeckl (CCM-UNAM)
(Submitted on 21 Dec 2012)
We introduce a new "positive formalism" for encoding quantum theories in the general boundary formulation, somewhat analogous to the mixed state formalism of the standard formulation. This makes the probability interpretation more natural and elegant, eliminates operationally irrelevant structure and opens the general boundary formulation to quantum information theory.
28 pages

to clarify the relevance here is a quote from end of section 2 on page 4:
"...The time-evolution operator U ̃ restricted to self-adjoint operators produces self-adjoint operators. Moreover, it is positive, i.e., it maps positive operators to positive operators. It also conserves the trace so that it maps mixed states to mixed states. These considerations suggest that positivity and order structure should play a more prominent role at a foundational level than say the Hilbert space structure of H or the algebra structure of the operators on it from which they are usually derived.
Algebraic quantum field theory [7] is a great example of the fruitfulness of taking serious some of these issues. There, one abandons in fact the notion of Hilbert spaces in favor of more flexible structures built on C∗-algebras. Also, positivity plays a crucial role there in the concept of state."

From marcus's quote, Oeckl does mention algebraic quantum field theory, which is exactly http://arxiv.org/abs/1305.3182's ref [29], cited for modular flow.

Also http://www.staff.science.uu.nl/~henri105/ comments at http://mathoverflow.net/questions/5...atization-of-time-other-than-perhaps-entropy: "In algebraic quantum field theory, time evolution can be identified with the modular flow of Tomita-Takesaki theory." He says it's the Bisognano-Wichman theorem.

Incidentally, the Blanco et al paper actually does link (at linear level) the Einstein Equations with "E=TdS". So it's like a holographic version of the Jacobson derivation, as van Raamsdonk's http://arxiv.org/abs/1308.3716 "Entanglement Thermodynamics" stresses. (In the Blanco et al paper, E is the "modular energy".)
 
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  • #63
Atyy, a quote from recent Chirco et al paper nicely clears up the terminology. There are variants in terminology (just as you suggest) depending on where the speaker comes from. In mathematics, it's Tomita, in QFT it's modular.

==quote Chirco et al http://arxiv.org/abs/1309.0777 page 4== (link corrected at Atyy's suggestion)
...is called the thermal Hamiltonian. The conjugate flow parameter τ is called thermal time [6, 8]. For a non-relativistic system it is simply related to the non-relativistic time t by

τ=t/β

where β is the inverse temperature. In mathematics, the thermal time flow is called the Tomita flow [19]; the thermal hamiltonian is called the modular Hamiltonian in quantum field theory [20, 21], and the entanglement Hamiltonian in the condensed matter context [22]. For a recent discussion of this quantity in quantum gravity see also [23].

==endquote==
The reference [20] is to R. Haag, “Local quantum physics: Fields, particles, algebras”, Springer (1992)
That is, to the same standard QFT text that Blanco et al paper you found cites ([29]) in connection with what QFT people call modular flow.
atyy said:
I googled "tomita flow modular flow" and you are the one of the top Google finds. Would you like to comment on whether modular flow in footnote 16 on p42 of http://arxiv.org/abs/1305.3182 is Tomita flow? Bianchi is cited in ref 16 and 63. One of the authors is an "LQG guy" :p

Footnote 16 on p42, "These unitary operators implement an evolution for an internal time . This time flow is called the modular flow [29]."
...
Yes! [29] R. Haag, “Local quantum physics: Fields, particles, algebras”, Berlin, Germany: Springer (1992) (Texts and monographs in physics).

Over and beyond just noting the overlap in terminology, you are pointing out a whole bunch of interesting connections.

EDIT: Atyy, I appreciate your catching my typo error in the above Chirco paper link. I could still edit, so I corrected it.
 
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  • #64
Thanks marcus! The link for the Chirco paper is http://arxiv.org/abs/1309.0777

So does AdS/CFT instantiate Connes-Rovelli thermal time? There appears to be a derivation of the Einstein equation at linear level from "entanglement thermodynamics" dE=dS where E refers to the modular Hamiltonian that Chirco et al say is the thermal Hamiltonian in their language and the entanglement Hamiltonian in condensed matter.

The AdS/CFT papers are
http://arxiv.org/abs/1305.3182
http://arxiv.org/abs/1308.3716
http://arxiv.org/abs/1304.7100
The first two are most relevant to Tomita flow because they use the modular Hamiltonian. There's definitely the idea that these are the AdS/CFT version of Jacobson's derivation, which I think inspired Rovelli too. Edit: In fact, Connes-Rovelli thermal time preceded Jacobson's derivation.

It also makes me wonder whether Bianchi's black hole entropy is really the black hole entropy or whether he actually calculated the entangelement entropy of some other region bounded by an extremal surface - since the Ryu-Takayanagi formula says those have the same form as the BH entropy. The best way to probe the black hole interior in AdS/CFT so far seems to have been to use the Ryu-Takayanagi formula in a non-stationary spacetime since the minimal surfaces penetrate the black hole in those cases. But I believe there is no tight link between the Ryu-Takayanagi formula and the BH entropy of black holes at this time, although it seems there should be one.

marcus said:
==quote Chirco et al http://arxiv.org/abs/1309.0777 page 4== (link corrected at Atyy's suggestion)
...is called the thermal Hamiltonian. The conjugate flow parameter τ is called thermal time [6, 8]. For a non-relativistic system it is simply related to the non-relativistic time t by

τ=t/β

where β is the inverse temperature. In mathematics, the thermal time flow is called the Tomita flow [19]; the thermal hamiltonian is called the modular Hamiltonian in quantum field theory [20, 21], and the entanglement Hamiltonian in the condensed matter context [22]. For a recent discussion of this quantity in quantum gravity see also [23].

==endquote==

Chirco's ref 23 is Bianchi-Myers! http://arxiv.org/abs/1212.5183 which indeed has a long discussion on the modular Hamiltonian.

Physics Monkey said:
Presumably if Tomita time is going to be useful, it should agree with usual notions in the right limit. Has it been checked that this time gives the usual global time evolution in, for example, asymptotically AdS spaces?

Also, we know that the Cauchy problem is not well posed in AdS because of the need for boundary conditions. Is this freedom apparent in Tomita time? Are there other freedoms?

marcus said:
It gives the right limit in several interesting cases. I don't know about asymptotic AdS.

Confirming cases are listed and discussed in the 1994 paper by Alain Connes and Carlo Rovelli.

I gave the link in post #2 of this thread.

The RATIO of T-time to local observer time can be given a physical meaning, which is kind of interesting---a general relativistic temperature identified by Tolman around 1930. There's a link to the Smerlak Rovelli paper about that also in post #2, I think.
https://www.physicsforums.com/showthread.php?p=4209223#post4209223

Physics Monkey asked essentially the same question in post #49. Are we now in a position to answer Physics Monkey's question in more detail? Incidentally, the entanglement Hamiltonian is very common in condensed matter physics, where it's associated with the Renyi entropies. I'd never associated it with Tomita flow which I'd seen many times in marcus's posts! Duh!

For example, it's used by Swingle, McMinis and Tubman in their eq 3.8 http://arxiv.org/abs/1211.0006 :smile:
 
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  • #65
http://arxiv.org/abs/1102.0440
Towards a derivation of holographic entanglement entropy
Horacio Casini, Marina Huerta, Robert C. Myers

Explicitly mentions and uses the modular flow!

The warm-up Rindler wedge example in section 2.1 is exactly (I think) the same as Connes and Rovelli's http://arxiv.org/abs/gr-qc/9406019 section 4.3.

From Casini et al's section 2.1: "One well-known example is given by Rindler space R ... In this case for any QFT, the modular Hamiltonian is just the boost generator in the X1 direction. This result is commonly known as the Bisognano-Wichmann theorem [25]. ... Interpreted in the sense of Unruh [26], the state in R is thermal ... With this choice, the Rindler state is thermal with respect to Hτ, the Hamiltonian generating τ translations, with a temperature ... With this notation, the modular flow (2.6) on R simply corresponds to the time translation ... and the modular Hamiltonian HR is simply related to Hτ with ..."
 
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  • #66
And here are a couple of condensed matter theorists talking about Tomita flow!

http://arxiv.org/abs/1109.1283
A geometric proof of the equality between entanglement and edge spectra
Brian Swingle, T. Senthil

"Remarkably, the entanglement Hamiltonian is the generator of a geometric flow in spacetime, and this flow may be interpreted as time evolution in Rindler space. The reduced density matrix of the half space is then a simple thermal state with respect to time evolution in Rindler space."

It looks like their main reference is to J. J. Bisognano and E. H. Wichmann, 17, 303 (1976), ISSN 00222488.
 
  • #67
A major question in my mind is related to the issue of infinities and their role in the physics. I am accustomed to finite (but large) dimensional algebras in which the "modular flow" is really a very simple object generated by some ordinary matrices. I also have the prejudice that anything physical should be describable in a finite language like this. For example, all physical measurements with quantum fields can be described in this language.

On the other hand, my understanding is that the mathematically non-trivial aspects of modular flow in the operator algebra context are all associated with "weird" infinite algebras. So I don't see how there can be physics in such an infinite object. In fact, I have this same objection to much of old school loop gravity, which seemed way too infinite to be right.

Of course, this is mostly my vague feelings and superstitions.
 
  • #68
http://arxiv.org/abs/1310.6335
State-Dependent Bulk-Boundary Maps and Black Hole Complementarity
Kyriakos Papadodimas, Suvrat Raju
Finally, we explore an intriguing link between our construction of interior operators and Tomita-Takesaki theory.
 
  • #69
I arrive late in this thread (mainly via the other "QBist" thread) and I'm trying to get a couple of things straightened out...

From Marcus's summaries about Tomita time, and also some of the references he cites, I understand that:
##S## is an anti-linear operator.
However, then Marcus (and others) speak of an adjoint ##S^*## of an operator ##S## via a definition like:
$$
(\phi, S^* \psi) ~\equiv~ (S\phi, \psi) ~.
$$ However, in Weinberg vol1, p51, eq(2.2.7), he defines the adjoint of an anti-linear operator via:
$$
(\phi, S^* \psi) ~\equiv~ (S\phi, \psi)^* ~=~ (\psi, S\phi) ~.
$$ Weinberg's motivation for his definition is that one can then write ##A^* = A^{-1}## regardless of whether ##A## is linear or antilinear.

So what's going on with the ##S## operator used in Tomita time? Is it a typo, or an intentionally different definition of "adjoint" for antilinear operators compared to Weinberg's ? I presume it's intentionally different, else the Tomita ##Q## operator would trivially be the identity, (right?).
 
  • #70
Papadodimas and Raju http://arxiv.org/abs/1310.6335 give the same definition of the adjoint as Weinberg in their discussion of Tomita-Takesaki theory (p57 and p86).
 
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  • #71
Could simply be a matter of mathematical conventions. If someone would like to write a brief summary of the Tomita flow in context of C* quantum formalism, and use Weinberg's conventions, I'd be delighted to go along with their notation. There's nothing sacred about the particular way that Alain Connes and Carlo Rovelli did it in their 1994 paper http://arxiv.org/abs/gr-qc/9406019 , or that section of the Princeton Companion to Mathematics that I linked to. Nice to have some explicit summary posted here in thread as well as backup sources available online though.

I'm not sure how useful that section of the Princeton Companion actually is, but here's the link FWIW:
http://books.google.com/books?id=ZO...6AEwAw#v=onepage&q=minoru tomita math&f=false
Maybe we need a fresh new one page in-thread summary and new backup source links.
 
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  • #72
Rep, I really like your bringing up Derek Wise' thing about lifting to "observer space" and the general idea of reality with no "official" spacetime still being real and representable.

So the question now for me, about the C* formulation, is could it be useful in implementing that Wise-Gielen idea. So I want to keep that in sight.

Maybe * algebra can be used to build a quantum version of Wise-Gielen observer space.

Correct me if I am mistaken (Rep and Atyy too!) but I think so far Wise-Gielen is purely classical.

Also I think Rovelli C* picture has a shortcoming in the following sense: I do not see a way in that context to realize anyone particular observer's construction of space or of spacetime, or, say, of his past lightcone. There may BE an obvious way, but I don't see it.

Suppose the C* picture needs further elaboration so that it contains something that is not an official spacetime but which verges on looking like a bundle of observers.
Could we give the C* picture something extra that sort of looks like it is enough like spacetime to allow us to work with it and do spacetime things.

As it is, the C* picture is just a normed algebra of measurements with maybe a time-flow defined on them. It is pretty vague. I'm worried. Maybe we should go back to the QB thread. Maybe there is no immediately obvious way to apply the C* picture to the idea in the other thread.
 
  • #73
marcus said:
Rep,
:biggrin:

Evo sometimes abbreviates my name to "Strange", but that can create ambiguities in different contexts.

Maybe * algebra can be used to build a quantum version of Wise-Gielen observer space.
Correct me if I am mistaken (Rep and Atyy too!) but I think so far Wise-Gielen is purely classical.
That's the impression I got too.

Also I think Rovelli C* picture has a shortcoming in the following sense: I do not see a way in that context to realize anyone particular observer's construction of space or of spacetime, or, say, of his past lightcone. There may BE an obvious way, but I don't see it. [...]
I had envisaged a (representation of) an algebra of observables ##A## associated to an inertial observer. That observer constructs a spacetime as a homogeneous space for the associated group. For multiple observers, we construct tensor products like ##A\otimes A##, and hence products of their respective spacetimes . (Think: products of symplectic phase spaces in classical mechanics.) But there must be more to it than that if we are to accommodate mutual accelerations associated with interactions, etc.

So yes, for this part of the discussion we should go back to the other (QBist) thread. I'll resume that later. I only came over here to clarify the Tomita-time construction, so I need to study the references that you and atyy mentioned above.
 
  • #74
marcus said:
[...] If someone would like to write a brief summary of the Tomita flow in context of C* quantum formalism, and use Weinberg's conventions, I'd be delighted to go along with their notation. There's nothing sacred about the particular way that Alain Connes and Carlo Rovelli did it in their 1994 paper http://arxiv.org/abs/gr-qc/9406019 , or that section of the Princeton Companion to Mathematics that I linked to.[...]
Now that I've read and pondered some more on Tomita-time, and thermal time, I begin to think that the antiunitary ##J## part of the operator ##S = J \Delta^{1/2}## is a mere red herring for these purposes.

The generic idea behind the thermal time construction starts with an arbitrarily-chosen fiducial (aka cyclic) state operator ##\omega##. As a state operator, it satisfies ##\omega^* = \omega## (hence all its eigenvalues are real). Also, its eigenvalues are all nonnegative.

The operator ##\Delta## is simply ##\omega##. The operator ##\omega^{1/2}## makes sense (simply take the square roots of the eigenvalues). Similarly, the operator ##U(t) := \omega^{it}## also makes sense by similarly raising the eigenvalues to that power.

The original state operator ##\omega## is obviously invariant under conjugation by ##U(t)##, i.e., ##U(t) \, \omega \, U(-t) \;=\; \omega##, etc.

However, if ##\omega## is a pure state then one and only one of its eigenvalues is 1 while the others are zero (cf. Ballentine p52). In that case ##\omega^n = \omega##, where ##n## is any complex number. Therefore, the "flow" represented by the ##U(t)## is trivial (the identity) if ##\omega## is pure, but can be nontrivial if ##\omega## is nonpure -- which is the case for the usual thermal (Gibbs) state ##\omega = \exp (-\beta H)## .

The Tomita construction seems to start from any antilinear operator ##S##, performs a "polar" decomposition of it, obtaining a corresponding ##\Delta## thereby which can be used as the fiducial state operator. But so what? For a given algebra, how is ##S## picked out? And is this essentially equivalent to picking out a fiducial state operator ##\omega##, as is usually done? I don't see what the fuss is all about. What am I missing?
 
  • #75
Usual QM is hamiltonian dependent. Once you have H you know how operators evolve with time in the Heisenberg picture.
To study KMS condition we compute the average value ##\langle \alpha_t(A) B \rangle ## in the state exp(-H).

With Tomita machinery no Hamiltonian to begin with but things are state dependent.
given a density matrix ## \rho## we send ##A\rho## to ## S(A \rho) =A^*\rho## then Tomita theorem associates ## \rho## to a KMS flow ## \sigma_{\rho}(s)## (we compute ##\langle \sigma_{\rho}(s) (A) B \rangle## in the state ##\rho##
You see that S is not picked among others. One ##\rho##, one Tomita flow.
Could you tell me why in ##S = J \Delta## Connes calls J the phase of S and ##\Delta## the modulus of S?
 
  • #76
naima said:
[...]
You see that S is not picked among others. One ##\rho##, one Tomita flow.
Yes, that's the impression I got. But I find it quite weird to rely on such a thing for time-flow, since the flow becomes trivial if the state is pure.

Could you tell me why in ##S = J \Delta## Connes calls J the phase of S and ##\Delta## the modulus of S?
I haven't read much of Connes, but I guess the terminology just follows the standard terminology in linear algebra and functional analysis. E.g., in Lax's textbook on Linear Algebra, there's a "polar decomposition" theorem 22 on p139, which says:
Lax said:
Let ##Z## be a linear mapping of a complex Euclidean space into itself. Then ##Z## can be factored as $$Z = RU ~,$$where ##R## is a nonnnegative self-adjoint mapping, and ##U## is unitary.
So the terminology of calling ##R## a "modulus" and ##U## a "phase" is just a generalization of terms used in polar decomposition of a complex number: ##z = r e^{i\theta}##.

Looking at Lax's proof, I think it goes through similarly, if ##Z## is anti-linear instead. In that case the decomposition is of the form ##Z = RJ## where now ##J## is anti-unitary. So calling it a "phase" is perhaps an abuse of terminology, but mathematicans love to call different things by the same name. :biggrin:
 
  • #77
Too many assumptions for my comfort zone.
 
  • #78
Chronos said:
Too many assumptions for my comfort zone.
Can you elaborate? (I'm kinda struggling with this stuff.) :frown:
 
  • #79
strangerep said:
Yes, that's the impression I got. But I find it quite weird to rely on such a thing for time-flow, since the flow becomes trivial if the state is pure.

When the state is almost pure his entropy is very small. As the one-parameter s grows the operators seem to be frozen.
Rovelli wrote once that the time flow is a product of our ignorance (entropy). the sentence is mysterious but in this point of view it may be taken into account.

I think that Marcus was wrong with:
marcus said:
Tomita time is an intrinsic observer-independent time variable available to us for fully general relativistic analysis.
Being state dependent how could it be observer-independent?

It would be interesting to see how it is an emerging time.
 
  • #80
naima said:
When the state is almost pure his entropy is very small. As the one-parameter s grows the operators seem to be frozen.
Rovelli wrote once that the time flow is a product of our ignorance (entropy). [...]
Can you recall the reference? I'd like to read the context of Rovelli's remark.

Indeed, I have trouble making sense of it. Does it suggest that the less one knows about the global state, the faster time seems to flow?? And does this even sit consistently with Lorentz boosts and relative time dilation between different observers? It also seems to be in contradiction with known gravitational time dilation in which a clock in a stronger gravitational field runs slower.

Hmmm,... let's see,... an observer accelerating strongly knows less(?) than a weakly-accelerating observer. (I mean in terms of entanglement entropy associated with their Rindler horizons). So...
[Oops! Brain crash -- core dumped. I'll have to think about that further after I reboot.] :rolleyes:

I think that Marcus was wrong with:
Marcus said:
Tomita time is an intrinsic observer-independent time variable available to us for fully general relativistic analysis.
Being state dependent how could it be observer-independent?
I was under the impression that the state ##\omega## which generates Tomita time flow is analogous to the "fiducial vacuum state" from which Fock spaces are built (except that the latter is pure but the former is nonpure). So it's a "given". Then, just as inequivalent Fock spaces can arise from different choices of vacuum state, so different universes arise from different choices of ##\omega##.

But,... as you see,... I struggle with all this... :frown:

It would be interesting to see how it is an emerging time.
Yes -- emerging from what? Spin network states?
 
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  • #81
strangerep said:
Can you recall the reference? I'd like to read the context of Rovelli's remark.

Indeed, I have trouble making sense of it. Does it suggest that the less one knows about the global state, the faster time seems to flow?? And does this even sit consistently with Lorentz boosts and relative time dilation between different observers? It also seems to be in contradiction with known gravitational time dilation in which a clock in a stronger gravitational field runs slower.

It is a quotation from Rovelli's small book "what is time? What is space?"

He writes that he worked on a timeless theory that had no success around him unless he met Alain Connes (1982 Fields medal). he realized that his theory was a soecial case of Connes's theory. They wrote a paper together.

He says that the flow of time is an emerging effect of our ignorance. If we had a perfect knowledge of things they would seem to be frozen (i use here my proper words).
Take the zeno effect if you observe continuously a up spin it will freeze. nothing will happen to it. You must accept not to observe it for a while to see becoming down.
This may be in relation to the frozen flow associated to a pure state. Only decohered observers would see things moving. A finite time observer has only access to events inside the future cone of his birthday and the past cone of his death (the diamond) but his wave function may be nor null outside this region. This is the reason while entropy and temperature is associated to this diamond.

You will see here answers from Rovelli.
It is hard to imagine that what we (decohered observers) see is not what really happens but only WE see.

I do not know what is the physical meaning of the state which generate Tomita flow. is it a vacuum seen by the observer or the state of the observer?
 
  • #82
naima said:
You will see here answers from Rovelli.
Thanks. Normally, I don't read much of the FQXi comments (too much waffle), but Rovelli's responses are interesting (and also a lesson in how to remain polite).

I'll quote a few of Rovelli's remarks from your link which seem relevant to my other confusions above...

C. Rovelli said:
[...] it is important to recall that the thermal time hypothesis does not REPLACE dynamics. My entire point is that dynamics can be expressed as correlations between variables, and does not NEED a time to be specified. The thermal time is only the one needed to make sense of our sense of flowing time, it is not a time needed to compute how a simple physical system behaves. The last can be expressed in terms of correlations between a variable and a clock hand, without having to say which one is the time variable. Therefore the question about the flow of time defined by bodies at different temperature is a question about thermodynamics out of equilibrium.

[...]

[...] all temporal "effects" that are captured by ordinary mechanics have nothing to do with thermal time. They just have to do with the fact that there are laws that govern the relations among variables. The additional peculiar "flowing" of time is an "effect" which is not the same thing as temperature, but (if we believe the thermal time hypothesis) it emerges in a thermodynamcal/statistical situation only.

naima said:
I do not know what is the physical meaning of the state which generate Tomita flow. is it a vacuum seen by the observer or the state of the observer?
I'm not sure about that, but this extract from another of Rovelli's responses seems relevant (emboldening is mine):
C. Rovelli said:
[...] In a timeless world, a small subsystem (us) whose interaction with the rest of the universe is limited to a very small number of variables, and therefore who has no access to the exact state of the rest of the universe (that is, it has the same state for many different states of the universe), can be correlated with the rest of the world in such a way to have an imprecise information about the rest of the system (a way to express these notions precisely using Shannon information theory is in my work on relational quantum theory); then with respect to this subsystem a Tomita flow is defined; and this flow itself is the physical underpinning of the perception of the flow of time, whatever this perception is.

Finally, Marcus: if you're still reading this thread... Does the following Rovelli quote remind you of anything we were discussing recently? :biggrin:
C. Rovelli said:
[...] getting rid of space at the fundamental level is not very new. I think that what general relativity does is precisely so. It is the realization that the Newtonian "space" is nothing else that one of the physical fields that make up reality. Reality is not a space inside which things moves, but rather an ensemble of fields in interaction. So, my answer is that we must forget space and forget time. Forgetting space is easy; we have centuries of traditions that give us examples about how to think the world without a fundamental space. Forgetting time is more difficult, [...]
 
  • #83
I remember my first account here a couple of yrs ago- PF 'Existence of time'. My understanding is raw at that time(and still does today^^) and i have the sense that time can also be expressed not in the usual experience. Way back when i was a kid I used to play with clocks comparing and manipulating each one to a point of breaking. I'm very curious. Instead of imaging godzillas and voltrons. I'm often confined to such unusual questions. Crazy stuff like 'what if' time clocks were never invented and all we can see are movements and have a sense of measurement through uniformity of events e.g changes in location of the sun and passing of seasons, etc etc. In my attempt. I imagined myself as an outside observer. I was trying to deduced everything as a variable of movements/dynamics(my version of thinking of what is thermal today) confined from a reference of absolute stillness. I always thought that physicality of movement/vibration/thermal creates the experience of passing moment--- time in a sense that it is emergent, consequential and the uniformity of such events are what is measured.

I was surprised when i read the links. Brought back old memories.

----CR reply "is that dynamics can be expressed as correlations between variables, and does not NEED a time to be specified. The thermal time is only the one needed to make sense of our sense of flowing time, it is not a time needed to compute how a simple physical system behaves. The last can be expressed in terms of correlations between a variable and a clock hand, without having to say which one is the time variable. Therefore the question about the flow of time defined by bodies at different temperature is a question about thermodynamics out of equilibrium... ALL dynamical systems (classical) can be simply reformulated in a way that puts time on the same ground as the other variables, an din this case the dynamics is expressed by a "Wheeler-DeWitt-like" constraint.
 
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  • #84
strangerep said:
Indeed, I have trouble making sense of it. Does it suggest that the less one knows about the global state, the faster time seems to flow?? And does this even sit consistently with Lorentz boosts and relative time dilation between different observers? It also seems to be in contradiction with known gravitational time dilation in which a clock in a stronger gravitational field runs slower.

I also worked with Tomitas flow in the context of foliations on spacetime. Here it seems there is an interesting perspective. Connes used the flow to change from factor II foliations (as described by factor II von Neumann algebras) to factor III foliations. Both foliations are related by a postive, measurable function as density. But from the physical point of view, this function can be interpreted as probability function. Then your quote above will make sense.
 
  • #85
torsten said:
But from the physical point of view, this function can be interpreted as probability function. Then your quote above will make sense.

Could you elaborate for almost laymen?
 
  • #86
naima said:
Could you elaborate for almost laymen?

The space of leafs of a foliation is a complicated space. Consider for instance a curve covering the torus, the so-called Kronecker foliation of the torus. A continuous function over the leaf space of this foliation can be only the constant function (otherwise the function is not continuous).
Connes had now the brilliant idea to associate a von Neumann algebra of operators to the leaf space of a foliation. Then from the structure of this algebra, one can recover the properties of the foliation. The leaf space was the first example of a non-commutative space (and a motivation for the following constructions). In case of the Kronecker foliation of the torus, one obtains a factor II algebra for the leaf space.
But there are physically more interesting foliations, mainly foliations of hyperbolic manifolds having a factor III as leaf space. By using Tomitas theory, Connes constructed a new foliation (with factor II leaf space) from the factor III leaf space. It is a total space of the bundle of positive densities or equivalently the space of probability functions (after integration). The probability function is defined over the transverse bundle of the foliation, i.e. the space who labelled the leafs.
I hope it is now more understandable
 

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