On the Status of Highly Entropic Objects

Details On the Status of Highly Entropic Objects On the Status of Highly Entropic Objects

2003-09-23

arxiv.org/abs/hep-th/0309218v3

Phys.Rev. D69 (2004) 024014

Physics

High Energy Physics

High Energy Physics - Theory

6 pages, RevTex, a few editorial changes

Scientific paper

10.1103/PhysRevD.69.024014

It has been proposed that the entropy of any object must satisfy fundamental (holographic or Bekenstein) bounds set by the object's size and perhaps its energy. However, most discussions of these bounds have ignored the possibility that objects violating the putative bounds could themselves become important components of Hawking radiation. We show that this possibility cannot a priori be neglected in existing derivations of the bounds. Thus this effect could potentially invalidate these derivations; but it might also lead to observational evidence for the bounds themselves.

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