Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies

In the case of barotropic FRW cosmologies, the Hubble parameter in conformal time is the solution of a simple Riccati equation of constant coefficients. We consider these cosmologies in the framework of nonrelativistic supersymmetry that has been effective in the area of supersymmetric quantum mecha...

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Veröffentlicht in:Symmetry, Integrability and Geometry: Methods and Applications
Datum:2011
Hauptverfasser: Rosu, H.C., Khmelnytskaya, K.V.
Format: Artikel
Sprache:Englisch
Veröffentlicht: Інститут математики НАН України 2011
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/146789
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Zitieren:Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies / H.C. Rosu, K.V. Khmelnytskaya // Symmetry, Integrability and Geometry: Methods and Applications. — 2011. — Т. 7. — Бібліогр.: 18 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Rosu, H.C.
Khmelnytskaya, K.V.
author_facet Rosu, H.C.
Khmelnytskaya, K.V.
citation_txt Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies / H.C. Rosu, K.V. Khmelnytskaya // Symmetry, Integrability and Geometry: Methods and Applications. — 2011. — Т. 7. — Бібліогр.: 18 назв. — англ.
collection DSpace DC
container_title Symmetry, Integrability and Geometry: Methods and Applications
description In the case of barotropic FRW cosmologies, the Hubble parameter in conformal time is the solution of a simple Riccati equation of constant coefficients. We consider these cosmologies in the framework of nonrelativistic supersymmetry that has been effective in the area of supersymmetric quantum mechanics. Recalling that Faraoni [Amer. J. Phys. 67 (1999), 732-734] showed how to reduce the barotropic FRW system of differential equations to simple harmonic oscillator differential equations, we set the latter equations in the supersymmetric approach and divide their solutions into two classes of 'bosonic' (nonsingular) and 'fermionic' (singular) cosmological zero-mode solutions. The fermionic equations can be considered as representing cosmologies of Stephani type, i.e., inhomogeneous and curvature-changing in the conformal time. We next apply the so-called shifted Riccati procedure by introducing a constant additive parameter, denoted by S, in the common Riccati solution of these supersymmetric partner cosmologies. This leads to barotropic Stephani cosmologies with periodic singularities in their spatial curvature indices that we call U and V cosmologies, the first being of bosonic type and the latter of fermionic type. We solve completely these cyclic singular cosmologies at the level of their zero modes showing that an acceptable shift parameter should be purely imaginary, which in turn introduces a parity-time (PT) property of the partner curvature indices.
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spelling Rosu, H.C.
Khmelnytskaya, K.V.
2019-02-11T15:16:03Z
2019-02-11T15:16:03Z
2011
Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies / H.C. Rosu, K.V. Khmelnytskaya // Symmetry, Integrability and Geometry: Methods and Applications. — 2011. — Т. 7. — Бібліогр.: 18 назв. — англ.
1815-0659
2010 Mathematics Subject Classification: 81Q60
DOI:10.3842/SIGMA.2011.013
https://nasplib.isofts.kiev.ua/handle/123456789/146789
In the case of barotropic FRW cosmologies, the Hubble parameter in conformal time is the solution of a simple Riccati equation of constant coefficients. We consider these cosmologies in the framework of nonrelativistic supersymmetry that has been effective in the area of supersymmetric quantum mechanics. Recalling that Faraoni [Amer. J. Phys. 67 (1999), 732-734] showed how to reduce the barotropic FRW system of differential equations to simple harmonic oscillator differential equations, we set the latter equations in the supersymmetric approach and divide their solutions into two classes of 'bosonic' (nonsingular) and 'fermionic' (singular) cosmological zero-mode solutions. The fermionic equations can be considered as representing cosmologies of Stephani type, i.e., inhomogeneous and curvature-changing in the conformal time. We next apply the so-called shifted Riccati procedure by introducing a constant additive parameter, denoted by S, in the common Riccati solution of these supersymmetric partner cosmologies. This leads to barotropic Stephani cosmologies with periodic singularities in their spatial curvature indices that we call U and V cosmologies, the first being of bosonic type and the latter of fermionic type. We solve completely these cyclic singular cosmologies at the level of their zero modes showing that an acceptable shift parameter should be purely imaginary, which in turn introduces a parity-time (PT) property of the partner curvature indices.
This paper is a contribution to the Proceedings of the Workshop “Supersymmetric Quantum Mechanics and Spectral Design” (July 18–30, 2010, Benasque, Spain). The full collection is available at http://www.emis.de/journals/SIGMA/SUSYQM2010.html.
 One of the authors (HCR) thanks the Organizing Committee for the kind invitation and the
 administration of the Benasque Center for their warm hospitality. We also thank the referees for their valuable comments.
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Інститут математики НАН України
Symmetry, Integrability and Geometry: Methods and Applications
Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
Article
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spellingShingle Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
Rosu, H.C.
Khmelnytskaya, K.V.
title Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
title_full Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
title_fullStr Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
title_full_unstemmed Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
title_short Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
title_sort shifted riccati procedure: application to conformal barotropic frw cosmologies
url https://nasplib.isofts.kiev.ua/handle/123456789/146789
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AT khmelnytskayakv shiftedriccatiprocedureapplicationtoconformalbarotropicfrwcosmologies