SciPost Phys. 9, 036 (2020) ·
published 11 September 2020

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A classical solution where the (scalar) field value moves by an ${\cal O}(1)$
range in Planck units is believed to signal the breakdown of Effective Field
Theory (EFT). One heuristic argument for this is that such a field will have
enough energy to be inside its own Schwarzschild radius, and will result in
collapse. In this paper, we consider an inverse problem: what kind of field
ranges arise during the gravitational collapse of a classical field? Despite
the fact that collapse has been studied for almost a hundred years, most of the
discussion is phrased in terms of fluid stress tensors, and not fields. An
exception is the scalar collapse made famous by Choptuik. We reconsider
Choptuiklike systems, but with the emphasis now on the evolution of the
scalar. We give strong evidence that generic spherically symmetric collapse of
a massless scalar field leads to superPlanckian field movement. But we also
note that in every such supercritical collapse scenario, the large field range
is hidden behind an apparent horizon. We also discuss how the familiar perfect
fluid models for collapse like OppenheimerSnyder and Vaidya should be viewed
in light of our results.
SciPost Phys. 7, 057 (2019) ·
published 29 October 2019

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In AdS/CFT, the nonuniqueness of the reconstructed bulk from boundary
subregions has motivated the notion of code subspaces. We present some closely
related structures that arise in flat space. A useful organizing idea is that
of an $asymptotic$ causal diamond (ACD): a causal diamond attached to the
conformal boundary of Minkowski space. The space of ACDs is defined by pairs of
points, one each on the future and past null boundaries, ${\cal I}^{\pm}$. We
observe that for flat space with an IR cutoff, this space (a) encodes a
preferred class of boundary subregions, (b) is a plausible way to capture
holographic data for local bulk reconstruction, (c) has a natural
interpretation as the kinematic space for holography, (d) leads to a
holographic entanglement entropy in flat space that matches previous
definitions and satisfies strong subadditivity, and, (e) has a bulk
union/intersection structure isomorphic to the one that motivated the
introduction of quantum error correction in AdS/CFT. By sliding the cutoff, we
also note one substantive way in which flat space holography differs from that
in AdS. Even though our discussion is centered around flat space (and AdS), we
note that there are notions of ACDs in other spacetimes as well. They could
provide a covariant way to abstractly characterize tensor subfactors of
Hilbert spaces of holographic theories.
Submissions
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