Tree-like structure of eternal inflation: A solvable model - INSPIRE

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Tree-like structure of eternal inflation: A solvable model

Daniel Harlow
(
- Stanford U., ITP and
- Stanford U., Phys. Dept.
)
,
Stephen H. Shenker
(
- Stanford U., ITP and
- Stanford U., Phys. Dept.
)
,
Douglas Stanford
(
- Stanford U., ITP and
- Stanford U., Phys. Dept.
)
,
Leonard Susskind
(
- Stanford U., ITP and
- Stanford U., Phys. Dept.
)

Oct, 2011

24 pages

Published in:

Phys.Rev.D 85 (2012) 063516

e-Print:

1110.0496 [hep-th]

DOI:

10.1103/PhysRevD.85.063516

Report number:

SU-ITP-11-47

View in:

ADS Abstract Service

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Abstract: (arXiv)

In this paper we introduce a simple discrete stochastic model of eternal inflation that shares many of the most important features of the continuum theory as it is now understood. The model allows us to construct a multiverse and rigorously analyze its properties. Although simple and easy to solve, it has a rich mathematical structure underlying it. Despite the discreteness of the space-time the theory exhibits an unexpected non-perturbative analog of conformal symmetry that acts on the boundary of the geometry. The symmetry is rooted in the mathematical properties of trees, p-adic numbers, and ultrametric spaces; and in the physical property of detailed balance. We provide self-contained elementary explanations of the unfamiliar mathematical concepts, which have have also appeared in the study of the p-adic string. The symmetry acts on a huge collection of very low dimensional "multiverse fields" that are not associated with the usual perturbative degrees of freedom. They are connected with the late-time statistical distribution of bubble-universes in the multiverse. The conformal symmetry which acts on the multiverse fields is broken by the existence of terminal decays - to hats or crunches - but in a particularly simple way. We interpret this symmetry breaking as giving rise to an arrow of time. The model is used to calculate statistical correlations at late time and to discuss the measure problem. We show that the natural cutoff in the model is the analog of the so-called light-cone-time cutoff. Applying the model to the problem of the cosmological constant, we find agreement with earlier work.

Note:

39 pages plus appendices, with 11 figures. Journal version (PRD). A discussion of the arrow of time added, along with various other minor clarifications suggested by an anonymous referee. References also added

98.80.Jk
04.60.Kz
11.25.Hf
symmetry: conformal
model: stochastic
space-time: discrete
p-adic
multiverse
inflation

References(50)

Figures(11)

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