Pith. sign in

Arrow of Time in String Theory

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it
abstract

Inflation allows the problem of the Arrow of time to be understood as a question about the structure of spacetime: why was the intrinsic curvature of the earliest spatial sections so much better behaved than it might have been? This is really just the complement of a more familiar problem: what mechanism prevents the extrinsic curvature of the earliest spatial sections from diverging, as classical General Relativity suggests? We argue that the stringy version of "creation from nothing", sketched by Ooguri, Vafa, and Verlinde, solves both of these problems at once. The argument, while very simple, hinges on some of the deepest theorems in global differential geometry. These results imply that when a spatially toral spacetime is created from nothing, the earliest spatial sections are forced to be [quasi-classically] exactly locally isotropic. This local isotropy, in turn, forces the inflaton into its minimal-entropy state. The theory explains why the Arrow does not reverse in black holes or in a cosmic contraction, if any.

citation-role summary

background 1

citation-polarity summary

fields

gr-qc 1

years

2024 1

verdicts

CONDITIONAL 1

roles

background 1

polarities

background 1

representative citing papers

Intrinsic Torsion, Extrinsic Torsion, and the Hubble Parameter

gr-qc · 2024-12-12 · conditional · novelty 5.0

The second fundamental form of a spatial slice in a torsional spacetime is a sum of the Hubble term and an extrinsic torsion term, producing a negative bias in Hubble estimates when torsion is neglected.

citing papers explorer

Showing 1 of 1 citing paper.

  • Intrinsic Torsion, Extrinsic Torsion, and the Hubble Parameter gr-qc · 2024-12-12 · conditional · none · ref 58 · internal anchor

    The second fundamental form of a spatial slice in a torsional spacetime is a sum of the Hubble term and an extrinsic torsion term, producing a negative bias in Hubble estimates when torsion is neglected.