Dmitry67
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Question
How holographic principle is defined if we don't use null surfaces of the region - but regular ones, timelike? So normal boundaries we use (a box, a sphere...)
The problem I see: when 'region' is spacially extended, the position of the boundary (and the very notion of the region) becomes frame-dependent (in SR)
It is even worse in GR and very curved spaces. Talking about the Dark Energy and expansion (this is why I am asking this question) I don't see how 'region' can be bigger than a Hubble volume.
P.S. I assume that Dark Energy is enropic force associated with entropy of geometry of our spacetime?
If our space is so surprisingly flat, then it should tend to transform into more chaotic state...
How holographic principle is defined if we don't use null surfaces of the region - but regular ones, timelike? So normal boundaries we use (a box, a sphere...)
The problem I see: when 'region' is spacially extended, the position of the boundary (and the very notion of the region) becomes frame-dependent (in SR)
It is even worse in GR and very curved spaces. Talking about the Dark Energy and expansion (this is why I am asking this question) I don't see how 'region' can be bigger than a Hubble volume.
P.S. I assume that Dark Energy is enropic force associated with entropy of geometry of our spacetime?
If our space is so surprisingly flat, then it should tend to transform into more chaotic state...
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