Can black hole entropy be observer-dependent?

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The discussion centers on the philosophical implications of an infinite series of cause-and-effect events leading to the present moment, questioning how such an infinity could be traversed. Participants express skepticism about the notion that every effect must have a cause, especially in light of quantum mechanics, which suggests randomness in certain occurrences. The conversation also touches on the nature of time, with some arguing that time may be an emergent property rather than a fundamental aspect of reality. The Big Bang theory is clarified, emphasizing that it does not assert something came from nothing, but rather that its mechanics are not fully understood. Ultimately, the dialogue reflects a blend of scientific inquiry and philosophical speculation regarding the origins and nature of time and causality.
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In previous post I mentioned some articles about entropy in general relativity and for possible entertainment or simply to give a bit of the flavor will quote a passage from Don Marolf's 2004 paper

==quote http://arxiv.org/abs/hep-th/0410168 from conclusions==
the realization that observers remaining outside a black hole associate a different (and, at least in interesting cases, smaller) flux of entropy across the horizon with a given physical process than do observers who themselves cross the horizon during the process. In particular, this second mechanism was explored using both analytic and numerical techniques in a simple toy model. We note that similar effects have been reported35 for calculations involving quantum teleportation experiments in non-inertial frames. Our observations are also in accord with general remarks36,37 that, in analogy with energy, entropy should be a subtle concept in General Relativity.
We have concentrated here on this new observer-dependence in the concept of entropy
. It is tempting to speculate that this observation will have further interesting implications for the thermodynamics of black holes. For example, the point here that the two classes of observers assign different values to the entropy flux across the horizon seems to be in tune with the point of view (see, e.g., Refs. 38,39,40,41,42) that the Bekenstein-Hawking entropy of a black hole does not count the number of black hole microstates, but rather refers to some property of these states relative to observers who…

==endquote==
 

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