
TL;DR
This paper reviews various formulations of the holographic principle, analyzing their validity in quantum gravity, and concludes that only the weak form, which constrains boundary information, is likely to hold in the full theory.
Contribution
It classifies and critically assesses different holographic principles, highlighting the limitations of strong and null forms and emphasizing the robustness of the weak form in quantum gravity.
Findings
Only the weak holographic form is supported by generalized second law arguments.
Strong forms face counterexamples at semiclassical level.
Null forms are limited to matter entropy, with difficulties including gravitational degrees of freedom.
Abstract
We review the different proposals which have so far been made for the holographic principle and the related entropy bounds and classify them into the strong, null and weak forms. These are analyzed, with the aim of discovering which may hold at the level of the full quantum theory of gravity. We find that only the weak forms, which constrain the information available to observers on boundaries, are implied by arguments using the generalized second law. The strong forms, which go further and posit a bound on the entropy in spacelike regions bounded by surfaces, are found to suffer from serious problems, which give rise to counterexamples already at the semiclassical level. The null form, proposed by Fischler, Susskind, Bousso and others, in which the bound is on the entropy of certain null surfaces, appears adequate at the level of a bound on the entropy of matter in a single background…
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