Black Holes Hint towards De Sitter Matrix Theory - INSPIRE

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Black Holes Hint towards De Sitter Matrix Theory

Leonard Susskind
(
- Stanford U., Phys. Dept. and
- Google Inc.
)

Sep 3, 2021

43 pages

Published in:

Universe 9 (2023) 8, 368

Published: Aug 11, 2023

e-Print:

2109.01322 [hep-th]

DOI:

10.3390/universe9080368

View in:

ADS Abstract Service

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Abstract: (MDPI)

De Sitter black holes and other non-perturbative configurations can be used to probe the holographic degrees of freedom of de Sitter space. For small black holes, evidence was first provided in the seminal work of Banks, Fiol, and Morrise and follow-ups by Banks and Fischler, showing that dS is described by a form of matrix theory. For large black holes, the evidence provided here is new: Gravitational calculations and matrix theory calculations of the rates of exponentially rare fluctuations match one another in surprising detail. The occurrences of Nariai geometry and the “inside-out” transition are particularly interesting examples, which I explain in this paper.

Note:

43 pages, 11 figures

black holes
de Sitter
matrix
black hole: de Sitter
matrix model
holography
fluctuation
nonperturbative
Nariai
entropy: entanglement

References(13)

Figures(11)

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Lisa Dyson
(
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)
,
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(
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)
,
Leonard Susskind
(
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)

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(
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)
,
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(
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)
,
Alexander Morisse
(
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)

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Addendum to Fast Scramblers

Leonard Susskind
(
- Stanford U., ITP and
- Stanford U., Phys. Dept.
)

e-Print:
- 1101.6048

Holographic Space-time, Newton's Law and the Dynamics of Black Holes

Tom Banks
(
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)
,
Willy Fischler
(
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- Texas U., TCC
)

e-Print:
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•
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•
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(
- Stanford U., Phys. Dept.
)

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•
e-Print:
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•
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