What is the boost hamiltonian in the Unruh effect?

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Discussion Overview

The discussion revolves around the concept of the "boost Hamiltonian" in the context of the Unruh effect, exploring its implications in quantum field theory (QFT) on curved spacetime and the thermal state associated with accelerated observers. Participants examine theoretical frameworks, mathematical formulations, and related literature.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant references Jacobson's paper, noting that the Minkowski vacuum state is a thermal state with respect to the boost Hamiltonian at a certain temperature, but expresses confusion about the definition of the "boost Hamiltonian."
  • Another participant suggests a paper that may provide insights into the boost Hamiltonian, specifically pointing to sections related to horizon energy and boundary terms in general relativity.
  • A third participant discusses the relationship between Minkowski space and Rindler space, highlighting the boost Killing vector and its role in the thermal distribution derived from the boost Hamiltonian.
  • One participant mentions a paper on semiclassical QFT in curved spacetime, discussing the modes of the field and the application of the Bogoliubov machinery to the Unruh effect, questioning the existence of an analogous theory in statistical mechanics for curved spacetime.
  • Another participant reiterates the discussion on semiclassical QFT, emphasizing that the interpretation of thermal spectra does not require explicit calculations and relates the methodology of thermal field theory to Wick rotation in curved spacetime.
  • There is a mention of the Rindler observer carrying a particle detector that could detect particles associated with the field, indicating a practical aspect of the theoretical discussion.

Areas of Agreement / Disagreement

Participants express various viewpoints on the nature and implications of the boost Hamiltonian, with no consensus reached on its definition or the relationship to the Unruh effect. Multiple competing views and interpretations remain present throughout the discussion.

Contextual Notes

Participants reference complex mathematical formulations and theoretical constructs, including the use of Wick rotation and the Bogoliubov transformation, which may depend on specific assumptions or definitions not fully explored in the discussion.

naima
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I am reading this Jacobson's paper
he writes:
According to the Unruh effect the Minkowski vacuum state of quantum fields—or any state at
very short distances— is a thermal state with respect to the boost hamiltonian at temperature
T.
I know that the accelerated observer is in a thermal environment, but i do not see what is this "boost hamiltonian". Can you write it?
Thanks.
 
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This paper may offer insights:

http://arxiv.org/pdf/1205.5325v1.pdf
Horizon energy as the boost boundary term in general relativity and loop gravity
Try the last several paragraphs related to eq (9).

A Google search for 'boost Hamiltonian' brings up lots of hits.
 
Refer to the discussion of Rindler space at http://www.scholarpedia.org/article/Unruh_effect, specifically the coordinate transformation a few lines below eq. (1) which relates ##(t,z)## of Minkowski space to the ##(\tau,\xi)## of Rindler space. The boost Killing vector in the ##z## direction of Minkowski space is
$$ z \frac{\partial}{\partial t} + t \frac{\partial}{\partial z} = \frac{\partial}{\partial \tau}.~~~(*)$$
Examining the mode expansion eq. (2), we see that the modes are eigenfunctions of the boosts with eigenvalues ## i \Omega_k##. In the thermal expansion, we Wick rotate ##\tau## to ##i \beta##, with ##\beta## the inverse temperature, so the eigenvalues become real and positive. Then the thermal distribution (5) is recognized as what we would have computed from a theory where we used the boost (*) as the Hamiltonian.
 
Last edited:
Thanks
I found a good paper about the subject.
It describes the semiclassical QFT on curved spacetime. Here ##\phi## is a solution of the motion equation.
Its modes are "planes waves" a) in Minkowski b) in the wedges of accelerated observer.
The Bogoliubov machinery gives an elegant solution to the unruh effect.
It uses no explicit Wick rotation. Is there an analogous theory of statistical mecanics in curved space(time)?
What is the status in this theory or ##\phi## and its modes?
 
naima said:
Thanks
I found a good paper about the subject.
It describes the semiclassical QFT on curved spacetime. Here ##\phi## is a solution of the motion equation.
Its modes are "planes waves" a) in Minkowski b) in the wedges of accelerated observer.
The Bogoliubov machinery gives an elegant solution to the unruh effect.

The analysis there is completely standard and equivalent to that in the link I provided.

It uses no explicit Wick rotation. Is there an analogous theory of statistical mecanics in curved space(time)?

The interpretation of (2.37) as a thermal spectrum does not need an explicit calculation. Your original question asked how does one obtain the Planck spectrum from the "boost Hamiltonian", which is what I answered. According to the methodology of thermal field theory, one Wick rotates to imaginary time. One is left with QFT on a spacetime with Euclidean signature and the time variable is made periodic with period equal to the inverse temperature. One can do this in curved spacetime as well.

What is the status in this theory or ##\phi## and its modes?

The idea is that the Rindler observer would be carrying a particle detector that could detect ##\phi## particles.
 

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