Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein Theory

We will confront some static spherically symmetric vacuum Brans-Dicke solutions in the Jordan and Einstein Frames with the Robertson parameters. While the regular solution in the vacuum Einstein theory is just the Schwarzschild black hole, the same in the Jordan frame Brans-Dicke theory is shown to...

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Main Authors: Alina Khaybullina, Ramil Izmailov, Kamal K. Nandi, Carlo Cattani
Format: Article
Language:English
Published: Hindawi Limited 2013-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2013/367029
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spelling doaj-fef854f6fa4a4ed2849e46b37cd6a73b2020-11-24T21:13:30ZengHindawi LimitedAdvances in High Energy Physics1687-73571687-73652013-01-01201310.1155/2013/367029367029Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein TheoryAlina Khaybullina0Ramil Izmailov1Kamal K. Nandi2Carlo Cattani3Ya.B. Zel'dovich International Center for Astrophysics, BSPU, Ufa 450000, RussiaYa.B. Zel'dovich International Center for Astrophysics, BSPU, Ufa 450000, RussiaYa.B. Zel'dovich International Center for Astrophysics, BSPU, Ufa 450000, RussiaYa.B. Zel'dovich International Center for Astrophysics, BSPU, Ufa 450000, RussiaWe will confront some static spherically symmetric vacuum Brans-Dicke solutions in the Jordan and Einstein Frames with the Robertson parameters. While the regular solution in the vacuum Einstein theory is just the Schwarzschild black hole, the same in the Jordan frame Brans-Dicke theory is shown to represent not a black hole but a traversable wormhole. But, in this case, the valid range of ω becomes too narrow to yield the observed weak field Robertson parameters at the positive mass mouth. The corresponding solution in the Einstein frame also provides a regular wormhole, and it yields the correct parametric values but only up to “one and half order.” We argue that a second-order contribution can in principle distinguish between the signatures of the regular wormhole and the singular Buchdahl solution in the Einstein frame. Thus, at the level of regular solutions, Brans-Dicke theory in each frame predicts effects very different from those of Einstein's theory. To our knowledge, these theoretical distinctions seem not to have received adequate attention so far.http://dx.doi.org/10.1155/2013/367029
collection DOAJ
language English
format Article
sources DOAJ
author Alina Khaybullina
Ramil Izmailov
Kamal K. Nandi
Carlo Cattani
spellingShingle Alina Khaybullina
Ramil Izmailov
Kamal K. Nandi
Carlo Cattani
Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein Theory
Advances in High Energy Physics
author_facet Alina Khaybullina
Ramil Izmailov
Kamal K. Nandi
Carlo Cattani
author_sort Alina Khaybullina
title Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein Theory
title_short Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein Theory
title_full Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein Theory
title_fullStr Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein Theory
title_full_unstemmed Regular Solutions in Vacuum Brans-Dicke Theory Compared to Vacuum Einstein Theory
title_sort regular solutions in vacuum brans-dicke theory compared to vacuum einstein theory
publisher Hindawi Limited
series Advances in High Energy Physics
issn 1687-7357
1687-7365
publishDate 2013-01-01
description We will confront some static spherically symmetric vacuum Brans-Dicke solutions in the Jordan and Einstein Frames with the Robertson parameters. While the regular solution in the vacuum Einstein theory is just the Schwarzschild black hole, the same in the Jordan frame Brans-Dicke theory is shown to represent not a black hole but a traversable wormhole. But, in this case, the valid range of ω becomes too narrow to yield the observed weak field Robertson parameters at the positive mass mouth. The corresponding solution in the Einstein frame also provides a regular wormhole, and it yields the correct parametric values but only up to “one and half order.” We argue that a second-order contribution can in principle distinguish between the signatures of the regular wormhole and the singular Buchdahl solution in the Einstein frame. Thus, at the level of regular solutions, Brans-Dicke theory in each frame predicts effects very different from those of Einstein's theory. To our knowledge, these theoretical distinctions seem not to have received adequate attention so far.
url http://dx.doi.org/10.1155/2013/367029
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