Naty1 said:
Hi MiljenkoM, I don't really understand all of your post #10..
Hi, Naty1... I'll try to make my points more clear in this post, and if you have any questions after, please ask.
Naty1 said:
Do you agree this is or is not accurate:
Would it be fair to describe the Unruh effect by saying that from the perspective of an accelerated observer, some virtual particles in an inertial frame become real particles in the accelerated frame?
I think its fine...its one explanation; but there could well be other intepretations.
Well, there is parse nothing particularly wrong with putting it like that, but I don't think it is very accurate description of effect. It raises a lot of questions if you put it like that, for example: why
only some virtual particles, how do you decide which? Now, the main problem with this is that you are using classical concept of particles that involves poin-like objects moving along trajectories. Now we know that this concept does not actually apply on subatomic scales. As you know, one needs QFT in which basic object are not particles but quantum fields. Quantum states of the fields are interpreted in terms of corresponding particles. Experiments are than described as computing probabilities for specific field configuration and so on...
As I sad in my previous post, I got a feeling that OP was thinking that mode functions are wave functions of particles, and that Bogoliubov transformations are turning one particle into another...
Since Unruh is quantum
field effect, I don't see any point in making it
"particle" effect.
Naty1 said:
MY limited understanding is that the Rindler horizon associated with the Unruh effect and a Schwarzschild horizon, for example, associated with a black hole are pretty much equivalent descriptions regarding the appearance of 'thermal radiation' ...
but I do not know all the math so am happy to learn more.
Agreed, horizon is crucial in derivation of Hawking radiation. Consider for example neutron star, whose radious may be close to Schwarzschild radius but now there is no horizont, and neutron stars as far as I know do not emit Hawking radiation. But with Unruh effect horizon is only crucial for thermal spectrum of detected particles. You can set for example mind experiment with model detector that is accelerating only for finite time, than there is no horizon, all the photons will eventually catch up with detector. And you'll find out that transition probability for detector ≠0, meaning, it is detecting particles but with different spectrum than thermal spectrum [arXiv: gr-qc/0306022v2]. BTW how do you set a link in this forum?
Naty1 said:
This description SUGGESTS something different between the Unruh and Black Hole situation, but other than the fact that in the Unruh effect the horizon is way distant [maybe infinity, I'm not positive] and the Black Holes horizon is right nearby,
I'm unsure what else may be different.
Horizon for accelerating observer is 1/
a away from him, where
a is acceleration, but I don't think this is important.
Main difference is that Unruh effect is flat space effect, and Hawking is curved space.
Now you can draw analogy between this two affects. First you need to find analog to Minkowski vacuum state, state that is regular throughout Schwarzschild spacetime, and this state is called Hartle-Hawking vacuum. State that is analog to Rindler vacuum (vacuum defined by accelerating observer) in case of black hole is called Boulware vacuum. And now by analogy with Unruh effect you find that Hartle-Hawking vacuum is thermal state, same as you will find that Minkowski vacuum is thermal state in Unruh effect.
Now, my point in post #10 was that Unruh and Hawking effect are not infect analog, where one in flat spacetime, other in curved. And way to illustrate this is to look at Kerr black hole, where there is no Hartle-Hawking vacuum, and you can't draw analogy to Unruh effect, but nevertheless there is emission of particles from black hole (Hawking effect).