Penrose's Gravitationally Induced State Reduction

In summary, Penrose argues that the states to which a "superposition" will reduce are solutions to the coupled system consisting of the Schrodinger equation including...gravitation. He claims that the reduction of state is practically instantaneous due to the huge gravitational stresses involved. However, he does not provide any details of this 'new rigorous' idea.
  • #1
George Jones
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Endnote 30.37 of Penrose's book The Road to Reality briefly outlines what Penrose calls "a more rigous justification" for his graviationally induced state reduction. The endnote concludes with "Details of this argument will be published later."

Penrose also alludes to this argument in a popular-level talk he gave at the Perimeter Institude.

Does anyone know if the argument has been published? It is not on the arxiv, nor can find it using scholar.google.com.

Regards,
George
 
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  • #2
George Jones said:
...

Penrose also alludes to this argument in a popular-level talk he gave at the Perimeter Institude.

Does anyone know if the argument has been published? It is not on the arxiv, nor can find it using scholar.google.com.

Regards,
George

I have read mention of it, and know vaguely what you refer to, but I don't know of a rigorous exposition of the idea by Penrose.

Is it your impression that a rigorous presentation would involve re-working the foundations of quantum mechanics? (that may be a silly question, I don't understand the issues well enough to know if it is a good question)

I hope someone else can come up with an online source that elaborates on this---fraid I can't.
 
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  • #3
Just Google on "Penrose" and "FELIX" and you'll get all kinds of links. His idea is that superposition of physical objects causes gravitational stresses in space-time, and that the larger the object, the greater the stress, and therefore the sooner the superposition must resolve, in accordance with the Heisenberg uncertainty principle. Superposition of macroscopic objects like Schrodinger's cat would create huge stresses, involving such a great amount of energy that the reduction of state would be practically instantaneous.

Here are some on-line lectures by Penrose on the subject.
http://www.rdegraaf.nl/index.asp?sND_ID=842142
 
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  • #4
Marcus: Penrose certainly believes that quantum theory needs a thorough reworking, but that is not what my question is about.

turbo-1: I was asking about something much more specific.

Thank you both for replying.

I have had a passing interest in Penrose's work for about eight months. The original reference for his ideas about gravity's role is

R. Penrose, "On Gravity's Role in Quantum State Reduction," General Relativity and Gravitation, 28(5), 1996, pp. 581-600.

This is reprinted as Chapter 13 of Physics Meets Philosophy at the Planck Scale.

Here's my take on his ideas about gravitationally induced state reduction.

Consider a single (extended) massive particle at rest, and two possible spatial positions of the particle, i.e., the particle is either "over here" (H) or "over there". Suppose the quantum states for "over here" and "over there" are stationary states [itex]\left| \Psi_{1} \right>[/itex] and [itex]\left| \Psi_{2} \right>[/itex], respectively. If the the same gravitational potential energy is associated with both positions (no change in "height"), the stationary states have the same energy [itex]E[/itex].

So,

[tex]i \hbar \frac{\partial}{\partial t} \left| \Psi_{1} \right> = E \left| \Psi_{1} \right>[/tex]

and

[tex]i \hbar \frac{\partial}{\partial t} \left| \Psi_{2} \right> = E \left| \Psi_{2} \right>.[/tex]

Now, suppose that the quantum state of the mass is the superposition

[tex]\left| \Psi \right> = c_{1} \left| \Psi_{1} \right> + c_{2} \left| \Psi_{1} \right>[/tex]

of "over here" and "over there". It would appear that [itex]\left| \Psi \right>[/itex] is also a stationary state with energy [itex]E[/itex], but Penrose says "Not so fast!"

The states [itex]\left| \Psi_{1} \right>[/itex] and [itex]\left| \Psi_{2} \right>[/itex] refer to different spacetimes - the spacetime for the "over here" state is curved over here, because the mass is over here, while the spacetime for the "over there" state is curved over there. Consequently, [itex]\partial / \partial t[/itex] for the "over here" spacetime and, [itex]\partial / \partial t[/itex] for the "over there" spacetime are different as timelike vectors and as quantum operators. Thus, the superposition is ill-defined.

Superpose anyway, and try to find a quantative measure of just how different the two [itex]\partial / \partial t[/itex] are. When taking the partial derivative with respect to [itex]t[/itex], spatial coordinates are held constant, so spatial variations cause changes in [itex]\partial / \partial t[/itex].

Thus, the spatial variation of some relevant quantity might serve as a measure of the ill-definedness of the superposition. What relevant quantity? For weak fields, maybe the difference between the Newtonian gravitation potentials for the two parts of the superposition, i.e., integrate over all space, the square (so plus and minus variations don't cancel) of the gradient (spatial variation) of the difference between the potentials.

Poisson's equation gives that this is proportional to the gravitational self-energy of the mass distribution that's left over when the two mass distributions are subtracted, which also seems like a good measure of just how different things are for the two spacetimes. This energy is then used to estimate, via the uncertainty principle, the time taken for state reduction.

It is here, I believe, that Penrose has had a new idea for further justification, and I was asking for details of this new "rigorous" idea.

Reduction to what state? Penrose claims that the states to which a "superposition" will reduce are solutions to the coupled system consisting of the Schrodinger equation including Newtonian gravitational potential energy together with Poisson's equation with the mass density represented by [itex]m \left| \psi \right|^2[/itex].

Penrose claims that this should be observable either by an experiment in space, or by a ground-based experiment being considered at the University of California. As Patrick Vanesch has said, if no decoherence is seen, everyone will interpret this as vindication for standard quantum mechanics. If decoherence is seen, then some people will claim that feedback with the environment is at work, not gravitationally induced state reduction.

http://arxiv.org/abs/quant-ph/0210001

Regards,
George
 
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  • #5
I'm sorry to point you to lectures instead of relevant papers. Your initial query was not specific enough for me to determine the level of detail you expected. Your follow-up post is quite detailed, and I can tell you that I have not seen a Penrose paper addressing the points you raise, and I have been Googling him fairly regularly for over a year since I have been working on a private model of quantum gravitation. Penrose believes that the marriage of quantum theory and GR will be an even-handed one, and that both will have to be adjusted. So far, my inclination is that GR will have to absorb the bulk of the modifications. I hope he comes up with the rigorous interpretation - I'm anxious to see it.
 
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  • #6
It should be noted that the idea of gravity-driven state collapse is not strictly Penrose's doing. It's been around for a while. In fact, Lagos Diosi came up with a virtually identical mechanism in the late 80s, several years before Penrose's Gen. Rel. Grav. paper.

There are also several recent publications that deal with this mechanism (the "Penrose-Diosi" formalism, as it's been called). These include:

Testing Gravity-Driven Collapse of the Wavefunction via Cosmogenic Neutrinos (Joy Christian)
http://arxiv.org/abs/quant-ph/0503001

Gravitationally-Induced Quantum Superpopsition Reduction with Large Extra Dimensions (J. R. Mureika)
http://arxiv.org/abs/gr-qc/0509082
 

Related to Penrose's Gravitationally Induced State Reduction

1. What is Penrose's Gravitationally Induced State Reduction?

Penrose's Gravitationally Induced State Reduction is a theory proposed by physicist Roger Penrose, which suggests that gravity plays a role in the collapse of the quantum wave function. This means that the act of measurement in quantum mechanics may be influenced by the presence of massive objects, such as planets or black holes.

2. How does Penrose's theory differ from other interpretations of quantum mechanics?

Penrose's theory differs from other interpretations of quantum mechanics, such as the Copenhagen interpretation, in that it proposes an objective and physical mechanism for the collapse of the wave function. It also suggests that the collapse is a continuous process rather than an instantaneous event.

3. Is there any evidence to support Penrose's theory?

Currently, there is no direct evidence to support Penrose's theory. However, some experiments have shown hints of a possible connection between gravity and quantum mechanics, and further research is being conducted to test this theory.

4. How does Penrose's theory relate to the concept of quantum entanglement?

Penrose's theory does not directly address quantum entanglement. However, some researchers have proposed that gravitational interactions between entangled particles may play a role in the collapse of the wave function.

5. What are the implications of Penrose's theory for our understanding of the universe?

If Penrose's theory is proven to be true, it would have significant implications for our understanding of the universe. It would provide a new perspective on the relationship between gravity and quantum mechanics and could potentially lead to a unified theory that combines these two fundamental theories of physics.

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