Effect upon universal order of Hubble expansion
- Autores
- Frieden, B. R.; Plastino, Ángel Luis; Plastino, Ángel Ricardo
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The level of order R in a spherical system of radius r0 with a probability amplitude function ψ(x),x=r,θ,φ obeys R=(12)r02I, where I=4∫dx|∇ψ|2 is its Fisher information level. We show that a flat space universe obeying the RobertsonWalker metric has an invariant value of the order as it undergoes either uniform Hubble expansion or contraction. This means that Hubble expansion per se does not cause a loss of universal order as time progresses. Instead, coarse graining processes characterizing decoherence and friction might cause a loss of order. Alternatively, looking backward in time, i.e. under Hubble contraction, as the big bang is approached and the Hubble radius r0 approaches small values, the structure in the amplitude function ψ(x) becomes ever more densely packed, increasing all local slopes ∇ψ and causing the Fisher information I to approach unboundedly large values. As a speculation, this ever-well locates the initial position of the universe in a larger, multiverse. © 2011 Elsevier B.V. All rights reserved.
Fil: Frieden, B. R.. University of Arizona; Estados Unidos
Fil: Plastino, Ángel Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Plastino, Ángel Ricardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de La Plata. Centro Regional de Estudios Genómicos; Argentina. Universidad de Granada; España - Materia
-
Coarse Graining
Fisher Information
Hubble Expansion
Order And Complexity - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/76031
Ver los metadatos del registro completo
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Effect upon universal order of Hubble expansionFrieden, B. R.Plastino, Ángel LuisPlastino, Ángel RicardoCoarse GrainingFisher InformationHubble ExpansionOrder And Complexityhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The level of order R in a spherical system of radius r0 with a probability amplitude function ψ(x),x=r,θ,φ obeys R=(12)r02I, where I=4∫dx|∇ψ|2 is its Fisher information level. We show that a flat space universe obeying the RobertsonWalker metric has an invariant value of the order as it undergoes either uniform Hubble expansion or contraction. This means that Hubble expansion per se does not cause a loss of universal order as time progresses. Instead, coarse graining processes characterizing decoherence and friction might cause a loss of order. Alternatively, looking backward in time, i.e. under Hubble contraction, as the big bang is approached and the Hubble radius r0 approaches small values, the structure in the amplitude function ψ(x) becomes ever more densely packed, increasing all local slopes ∇ψ and causing the Fisher information I to approach unboundedly large values. As a speculation, this ever-well locates the initial position of the universe in a larger, multiverse. © 2011 Elsevier B.V. All rights reserved.Fil: Frieden, B. R.. University of Arizona; Estados UnidosFil: Plastino, Ángel Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Plastino, Ángel Ricardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de La Plata. Centro Regional de Estudios Genómicos; Argentina. Universidad de Granada; EspañaElsevier Science2012-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/76031Frieden, B. R.; Plastino, Ángel Luis; Plastino, Ángel Ricardo; Effect upon universal order of Hubble expansion; Elsevier Science; Physica A: Statistical Mechanics and its Applications; 391; 1-2; 1-2012; 410-4130378-4371CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.physa.2011.08.005info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S037843711100611Xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:33:20Zoai:ri.conicet.gov.ar:11336/76031instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:33:21.202CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Effect upon universal order of Hubble expansion |
| title |
Effect upon universal order of Hubble expansion |
| spellingShingle |
Effect upon universal order of Hubble expansion Frieden, B. R. Coarse Graining Fisher Information Hubble Expansion Order And Complexity |
| title_short |
Effect upon universal order of Hubble expansion |
| title_full |
Effect upon universal order of Hubble expansion |
| title_fullStr |
Effect upon universal order of Hubble expansion |
| title_full_unstemmed |
Effect upon universal order of Hubble expansion |
| title_sort |
Effect upon universal order of Hubble expansion |
| dc.creator.none.fl_str_mv |
Frieden, B. R. Plastino, Ángel Luis Plastino, Ángel Ricardo |
| author |
Frieden, B. R. |
| author_facet |
Frieden, B. R. Plastino, Ángel Luis Plastino, Ángel Ricardo |
| author_role |
author |
| author2 |
Plastino, Ángel Luis Plastino, Ángel Ricardo |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Coarse Graining Fisher Information Hubble Expansion Order And Complexity |
| topic |
Coarse Graining Fisher Information Hubble Expansion Order And Complexity |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The level of order R in a spherical system of radius r0 with a probability amplitude function ψ(x),x=r,θ,φ obeys R=(12)r02I, where I=4∫dx|∇ψ|2 is its Fisher information level. We show that a flat space universe obeying the RobertsonWalker metric has an invariant value of the order as it undergoes either uniform Hubble expansion or contraction. This means that Hubble expansion per se does not cause a loss of universal order as time progresses. Instead, coarse graining processes characterizing decoherence and friction might cause a loss of order. Alternatively, looking backward in time, i.e. under Hubble contraction, as the big bang is approached and the Hubble radius r0 approaches small values, the structure in the amplitude function ψ(x) becomes ever more densely packed, increasing all local slopes ∇ψ and causing the Fisher information I to approach unboundedly large values. As a speculation, this ever-well locates the initial position of the universe in a larger, multiverse. © 2011 Elsevier B.V. All rights reserved. Fil: Frieden, B. R.. University of Arizona; Estados Unidos Fil: Plastino, Ángel Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Plastino, Ángel Ricardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de La Plata. Centro Regional de Estudios Genómicos; Argentina. Universidad de Granada; España |
| description |
The level of order R in a spherical system of radius r0 with a probability amplitude function ψ(x),x=r,θ,φ obeys R=(12)r02I, where I=4∫dx|∇ψ|2 is its Fisher information level. We show that a flat space universe obeying the RobertsonWalker metric has an invariant value of the order as it undergoes either uniform Hubble expansion or contraction. This means that Hubble expansion per se does not cause a loss of universal order as time progresses. Instead, coarse graining processes characterizing decoherence and friction might cause a loss of order. Alternatively, looking backward in time, i.e. under Hubble contraction, as the big bang is approached and the Hubble radius r0 approaches small values, the structure in the amplitude function ψ(x) becomes ever more densely packed, increasing all local slopes ∇ψ and causing the Fisher information I to approach unboundedly large values. As a speculation, this ever-well locates the initial position of the universe in a larger, multiverse. © 2011 Elsevier B.V. All rights reserved. |
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2012 |
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2012-01 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/76031 Frieden, B. R.; Plastino, Ángel Luis; Plastino, Ángel Ricardo; Effect upon universal order of Hubble expansion; Elsevier Science; Physica A: Statistical Mechanics and its Applications; 391; 1-2; 1-2012; 410-413 0378-4371 CONICET Digital CONICET |
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http://hdl.handle.net/11336/76031 |
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Frieden, B. R.; Plastino, Ángel Luis; Plastino, Ángel Ricardo; Effect upon universal order of Hubble expansion; Elsevier Science; Physica A: Statistical Mechanics and its Applications; 391; 1-2; 1-2012; 410-413 0378-4371 CONICET Digital CONICET |
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eng |
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