FRW and domain walls in higher spin gravity

Abstract We present exact solutions to Vasiliev’s bosonic higher spin gravity equations in four dimensions with positive and negative cosmological constant that admit an interpretation in terms of domain walls, quasi-instantons and Friedman-Robertson-Walker (FRW) backgrounds. Their isometry algebras...

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Main Authors: R. Aros, C. Iazeolla, J. Noreña, E. Sezgin, P. Sundell, Y. Yin
Format: Article
Language:English
Published: SpringerOpen 2018-03-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP03(2018)153
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spelling doaj-24461aee99714b7e9be817deac20f4ff2020-11-25T00:54:42ZengSpringerOpenJournal of High Energy Physics1029-84792018-03-012018315710.1007/JHEP03(2018)153FRW and domain walls in higher spin gravityR. Aros0C. Iazeolla1J. Noreña2E. Sezgin3P. Sundell4Y. Yin5Departamento de Ciencias Físicas, Universidad Andres BelloNSR Physics Department, G. Marconi UniversityInstituto de Física, Pontificia Universidad Católica de ValparaísoMitchell Institute for Fundamental Physics and Astronomy, Texas A&M UniversityDepartamento de Ciencias Físicas, Universidad Andres BelloDepartamento de Ciencias Físicas, Universidad Andres BelloAbstract We present exact solutions to Vasiliev’s bosonic higher spin gravity equations in four dimensions with positive and negative cosmological constant that admit an interpretation in terms of domain walls, quasi-instantons and Friedman-Robertson-Walker (FRW) backgrounds. Their isometry algebras are infinite dimensional higher-spin extensions of spacetime isometries generated by six Killing vectors. The solutions presented are obtained by using a method of holomorphic factorization in noncommutative twistor space and gauge functions. In interpreting the solutions in terms of Fronsdal-type fields in space-time, a field-dependent higher spin transformation is required, which is implemented at leading order. To this order, the scalar field solves Klein-Gordon equation with conformal mass in (A)dS 4 . We interpret the FRW solution with de Sitter asymptotics in the context of inflationary cosmology and we expect that the domain wall and FRW solutions are associated with spontaneously broken scaling symmetries in their holographic description. We observe that the factorization method provides a convenient framework for setting up a perturbation theory around the exact solutions, and we propose that the nonlinear completion of particle excitations over FRW and domain wall solutions requires black hole-like states.http://link.springer.com/article/10.1007/JHEP03(2018)153Cosmology of Theories beyond the SMHigher Spin GravityHigher Spin Symmetry
collection DOAJ
language English
format Article
sources DOAJ
author R. Aros
C. Iazeolla
J. Noreña
E. Sezgin
P. Sundell
Y. Yin
spellingShingle R. Aros
C. Iazeolla
J. Noreña
E. Sezgin
P. Sundell
Y. Yin
FRW and domain walls in higher spin gravity
Journal of High Energy Physics
Cosmology of Theories beyond the SM
Higher Spin Gravity
Higher Spin Symmetry
author_facet R. Aros
C. Iazeolla
J. Noreña
E. Sezgin
P. Sundell
Y. Yin
author_sort R. Aros
title FRW and domain walls in higher spin gravity
title_short FRW and domain walls in higher spin gravity
title_full FRW and domain walls in higher spin gravity
title_fullStr FRW and domain walls in higher spin gravity
title_full_unstemmed FRW and domain walls in higher spin gravity
title_sort frw and domain walls in higher spin gravity
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-03-01
description Abstract We present exact solutions to Vasiliev’s bosonic higher spin gravity equations in four dimensions with positive and negative cosmological constant that admit an interpretation in terms of domain walls, quasi-instantons and Friedman-Robertson-Walker (FRW) backgrounds. Their isometry algebras are infinite dimensional higher-spin extensions of spacetime isometries generated by six Killing vectors. The solutions presented are obtained by using a method of holomorphic factorization in noncommutative twistor space and gauge functions. In interpreting the solutions in terms of Fronsdal-type fields in space-time, a field-dependent higher spin transformation is required, which is implemented at leading order. To this order, the scalar field solves Klein-Gordon equation with conformal mass in (A)dS 4 . We interpret the FRW solution with de Sitter asymptotics in the context of inflationary cosmology and we expect that the domain wall and FRW solutions are associated with spontaneously broken scaling symmetries in their holographic description. We observe that the factorization method provides a convenient framework for setting up a perturbation theory around the exact solutions, and we propose that the nonlinear completion of particle excitations over FRW and domain wall solutions requires black hole-like states.
topic Cosmology of Theories beyond the SM
Higher Spin Gravity
Higher Spin Symmetry
url http://link.springer.com/article/10.1007/JHEP03(2018)153
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