Observing the dimensionality of our parent vacuum

It seems generic to have vacua with lower dimensionality than ours. We consider the possibility that the observable universe originated in a transition from one of these vacua. Such a universe has anisotropic spatial curvature. This may be directly observable through its late-time effects on the CMB...

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Main Authors: Graham, Peter W., Harnik, Roni, Rajendran, Surjeet
Other Authors: Massachusetts Institute of Technology. Center for Theoretical Physics
Format: Article
Language:en_US
Published: American Physical Society 2011
Online Access:http://hdl.handle.net/1721.1/60577
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author Graham, Peter W.
Harnik, Roni
Rajendran, Surjeet
author2 Massachusetts Institute of Technology. Center for Theoretical Physics
author_facet Massachusetts Institute of Technology. Center for Theoretical Physics
Graham, Peter W.
Harnik, Roni
Rajendran, Surjeet
author_sort Graham, Peter W.
collection MIT
description It seems generic to have vacua with lower dimensionality than ours. We consider the possibility that the observable universe originated in a transition from one of these vacua. Such a universe has anisotropic spatial curvature. This may be directly observable through its late-time effects on the CMB if the last period of slow-roll inflation was not too long. These affect the entire sky, leading to correlations which persist up to the highest CMB multipoles, thus allowing a conclusive detection above cosmic variance. Further, this anisotropic curvature causes different dimensions to expand at different rates. This leads to other potentially observable signals including a quadrupolar anisotropy in the CMB which limits the size of the curvature. Conversely, if isotropic curvature is observed it may be evidence that our parent vacuum was at least 3+1 dimensional. Such signals could reveal our history of decompactification, providing evidence for the existence of vastly different vacua.
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spelling mit-1721.1/605772022-09-29T19:03:43Z Observing the dimensionality of our parent vacuum Graham, Peter W. Harnik, Roni Rajendran, Surjeet Massachusetts Institute of Technology. Center for Theoretical Physics Massachusetts Institute of Technology. Department of Physics Rajendran, Surjeet Rajendran, Surjeet It seems generic to have vacua with lower dimensionality than ours. We consider the possibility that the observable universe originated in a transition from one of these vacua. Such a universe has anisotropic spatial curvature. This may be directly observable through its late-time effects on the CMB if the last period of slow-roll inflation was not too long. These affect the entire sky, leading to correlations which persist up to the highest CMB multipoles, thus allowing a conclusive detection above cosmic variance. Further, this anisotropic curvature causes different dimensions to expand at different rates. This leads to other potentially observable signals including a quadrupolar anisotropy in the CMB which limits the size of the curvature. Conversely, if isotropic curvature is observed it may be evidence that our parent vacuum was at least 3+1 dimensional. Such signals could reveal our history of decompactification, providing evidence for the existence of vastly different vacua. United States. Dept. of Energy. Office of Nuclear Physics (Grant No. DE-FG02-94ER40818) National Science Foundation (U.S.) (Grant No. PHY-0600465) 2011-01-14T18:30:38Z 2011-01-14T18:30:38Z 2010-09 2010-03 Article http://purl.org/eprint/type/JournalArticle 1550-7998 1550-2368 http://hdl.handle.net/1721.1/60577 Graham, Peter W., Roni Harnik, and Surgeet Fajendran. "Observing the dimensionality of our parent vacuum." Physical Review D 82.6 (201): 063524. © 2010 The American Physical Society en_US http://dx.doi.org/10.1103/PhysRevD.82.063524 Physical Review D Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Physical Society APS
spellingShingle Graham, Peter W.
Harnik, Roni
Rajendran, Surjeet
Observing the dimensionality of our parent vacuum
title Observing the dimensionality of our parent vacuum
title_full Observing the dimensionality of our parent vacuum
title_fullStr Observing the dimensionality of our parent vacuum
title_full_unstemmed Observing the dimensionality of our parent vacuum
title_short Observing the dimensionality of our parent vacuum
title_sort observing the dimensionality of our parent vacuum
url http://hdl.handle.net/1721.1/60577
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