Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity

We compare the initial value formulation of the low-energy limit of (nonprojectable) Hořava gravity to that of Einstein-æther theory when the æther is assumed to be hypersurface orthogonal at the level of the field equations. This comparison clearly highlights a crucial difference in the causal stru...

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Main Authors: Bhattacharyya, Jishnu, Coates, Andrew, Colombo, Mattia, Sotiriou, Thomas P.
Format: Article
Published: American Physical Society 2016
Online Access:https://eprints.nottingham.ac.uk/39494/
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author Bhattacharyya, Jishnu
Coates, Andrew
Colombo, Mattia
Sotiriou, Thomas P.
author_facet Bhattacharyya, Jishnu
Coates, Andrew
Colombo, Mattia
Sotiriou, Thomas P.
author_sort Bhattacharyya, Jishnu
building Nottingham Research Data Repository
collection Online Access
description We compare the initial value formulation of the low-energy limit of (nonprojectable) Hořava gravity to that of Einstein-æther theory when the æther is assumed to be hypersurface orthogonal at the level of the field equations. This comparison clearly highlights a crucial difference in the causal structure of the two theories at the nonperturbative level: in Hořava gravity evolution equations include an elliptic equation that is not a constraint relating initial data but needs to be imposed on each slice of the foliation. This feature is absent in Einstein-æther theory. We discuss its physical significance in Hořava gravity. We also focus on spherical symmetry, and we revisit existing collapse simulations in Einstein-æther theory. We argue that they have likely already uncovered the dynamical formation of a universal horizon and that they can act as evidence that this horizon is indeed a Cauchy horizon in Hořava gravity.
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spelling nottingham-394942020-05-04T17:40:44Z https://eprints.nottingham.ac.uk/39494/ Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity Bhattacharyya, Jishnu Coates, Andrew Colombo, Mattia Sotiriou, Thomas P. We compare the initial value formulation of the low-energy limit of (nonprojectable) Hořava gravity to that of Einstein-æther theory when the æther is assumed to be hypersurface orthogonal at the level of the field equations. This comparison clearly highlights a crucial difference in the causal structure of the two theories at the nonperturbative level: in Hořava gravity evolution equations include an elliptic equation that is not a constraint relating initial data but needs to be imposed on each slice of the foliation. This feature is absent in Einstein-æther theory. We discuss its physical significance in Hořava gravity. We also focus on spherical symmetry, and we revisit existing collapse simulations in Einstein-æther theory. We argue that they have likely already uncovered the dynamical formation of a universal horizon and that they can act as evidence that this horizon is indeed a Cauchy horizon in Hořava gravity. American Physical Society 2016-03-23 Article PeerReviewed Bhattacharyya, Jishnu, Coates, Andrew, Colombo, Mattia and Sotiriou, Thomas P. (2016) Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity. Physical Review D, 93 (6). 64056/1-64056/10. ISSN 2470-0029 http://dx.doi.org/10.1103/PhysRevD.93.064056 doi:10.1103/PhysRevD.93.064056 doi:10.1103/PhysRevD.93.064056
spellingShingle Bhattacharyya, Jishnu
Coates, Andrew
Colombo, Mattia
Sotiriou, Thomas P.
Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity
title Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity
title_full Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity
title_fullStr Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity
title_full_unstemmed Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity
title_short Evolution and spherical collapse in Einstein-Æther theory and Hořava gravity
title_sort evolution and spherical collapse in einstein-æther theory and hořava gravity
url https://eprints.nottingham.ac.uk/39494/
https://eprints.nottingham.ac.uk/39494/
https://eprints.nottingham.ac.uk/39494/