On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 Gravity

Corda, Mosquera Cuesta, and Lorduy Gòmez have shown that spherically symmetric stationary states can be used as a model for galaxies in the framework of the linearized R2 gravity. Those states could represent a partial solution to the Dark Matter Problem. Here, we discuss an improvement of this work...

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Main Authors: Rishabh Jain, Burra G. Sidharth, Christian Corda
Format: Article
Language:English
Published: Wiley 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/2601741
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author Rishabh Jain
Burra G. Sidharth
Christian Corda
author_facet Rishabh Jain
Burra G. Sidharth
Christian Corda
author_sort Rishabh Jain
collection DOAJ
description Corda, Mosquera Cuesta, and Lorduy Gòmez have shown that spherically symmetric stationary states can be used as a model for galaxies in the framework of the linearized R2 gravity. Those states could represent a partial solution to the Dark Matter Problem. Here, we discuss an improvement of this work. In fact, as the star density is a functional of the invariants of the associated Vlasov equation, we show that any of these invariants is in its turn a functional of the local energy and the angular momentum. As a consequence, the star density depends only on these two integrals of the Vlasov system. This result is known as the “Jeans theorem.” In addition, we find an analogy of the historical Tolman–Oppenheimer–Volkoff equation for the system considered in this paper. For the sake of completeness, in the final section of the paper, we consider two additional models which argue that Dark Matter could not be an essential element.
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spelling doaj-art-346dc47d72e543678990cf0b90212b8c2025-02-03T07:24:46ZengWileyAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/26017412601741On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 GravityRishabh Jain0Burra G. Sidharth1Christian Corda2Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USAInternational Institute for Applicable Mathematics & Information Sciences (IIAMIS), Hyderabad, IndiaResearch Institute for Astronomy and Astrophysics of Maragha (RIAAM), P.O. Box 55134-441, Maragha, IranCorda, Mosquera Cuesta, and Lorduy Gòmez have shown that spherically symmetric stationary states can be used as a model for galaxies in the framework of the linearized R2 gravity. Those states could represent a partial solution to the Dark Matter Problem. Here, we discuss an improvement of this work. In fact, as the star density is a functional of the invariants of the associated Vlasov equation, we show that any of these invariants is in its turn a functional of the local energy and the angular momentum. As a consequence, the star density depends only on these two integrals of the Vlasov system. This result is known as the “Jeans theorem.” In addition, we find an analogy of the historical Tolman–Oppenheimer–Volkoff equation for the system considered in this paper. For the sake of completeness, in the final section of the paper, we consider two additional models which argue that Dark Matter could not be an essential element.http://dx.doi.org/10.1155/2016/2601741
spellingShingle Rishabh Jain
Burra G. Sidharth
Christian Corda
On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 Gravity
Advances in High Energy Physics
title On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 Gravity
title_full On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 Gravity
title_fullStr On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 Gravity
title_full_unstemmed On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 Gravity
title_short On the Jeans Theorem and the “Tolman–Oppenheimer–Volkoff Equation” in R2 Gravity
title_sort on the jeans theorem and the tolman oppenheimer volkoff equation in r2 gravity
url http://dx.doi.org/10.1155/2016/2601741
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