Generalized Poisson distributions for systems with two-particle interactions

Autores
Hameeda, Mir; Plastino, Ángelo; Rocca, Mario Carlos
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In a cosmological context, observational best fits for galaxies’ distributions in the Universe have been tackled by recourse to different distribution functions. We provide here arguments favoring the formulation of a rather general distribution function (DF), of Poisson origin, describing galaxy clustering. The DF should be useful irrespective of distances or temperatures. We will be discussing distribution function for gravitational interactions.
Fil: Hameeda, Mir. Kasmir University; India. Inter University Centre for Astronomy and Astrophysics; India. Damghan University; Irán
Fil: Plastino, Ángelo. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina
Fil: Rocca, Mario Carlos. 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. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina
Materia
Gravitational interactions
Distribution functions
Galaxy clusters
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/181371
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/181371
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Generalized Poisson distributions for systems with two-particle interactionsHameeda, MirPlastino, ÁngeloRocca, Mario CarlosGravitational interactionsDistribution functionsGalaxy clustershttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In a cosmological context, observational best fits for galaxies’ distributions in the Universe have been tackled by recourse to different distribution functions. We provide here arguments favoring the formulation of a rather general distribution function (DF), of Poisson origin, describing galaxy clustering. The DF should be useful irrespective of distances or temperatures. We will be discussing distribution function for gravitational interactions.Fil: Hameeda, Mir. Kasmir University; India. Inter University Centre for Astronomy and Astrophysics; India. Damghan University; IránFil: Plastino, Ángelo. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; ArgentinaFil: Rocca, Mario Carlos. 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. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; ArgentinaIOP Publishing2021-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/181371Hameeda, Mir; Plastino, Ángelo; Rocca, Mario Carlos; Generalized Poisson distributions for systems with two-particle interactions; IOP Publishing; IOP SciNotes; 2; 1; 3-2021; 1-82633-1357CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/2633-1357/abec9finfo:eu-repo/semantics/altIdentifier/doi/10.1088/2633-1357/abec9finfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-11-12T09:51:41Zoai:ri.conicet.gov.ar:11336/181371instacron: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:34982025-11-12 09:51:41.428CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Generalized Poisson distributions for systems with two-particle interactions
title Generalized Poisson distributions for systems with two-particle interactions
spellingShingle Generalized Poisson distributions for systems with two-particle interactions
Hameeda, Mir
Gravitational interactions
Distribution functions
Galaxy clusters
title_short Generalized Poisson distributions for systems with two-particle interactions
title_full Generalized Poisson distributions for systems with two-particle interactions
title_fullStr Generalized Poisson distributions for systems with two-particle interactions
title_full_unstemmed Generalized Poisson distributions for systems with two-particle interactions
title_sort Generalized Poisson distributions for systems with two-particle interactions
dc.creator.none.fl_str_mv Hameeda, Mir
Plastino, Ángelo
Rocca, Mario Carlos
author Hameeda, Mir
author_facet Hameeda, Mir
Plastino, Ángelo
Rocca, Mario Carlos
author_role author
author2 Plastino, Ángelo
Rocca, Mario Carlos
author2_role author
author
dc.subject.none.fl_str_mv Gravitational interactions
Distribution functions
Galaxy clusters
topic Gravitational interactions
Distribution functions
Galaxy clusters
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In a cosmological context, observational best fits for galaxies’ distributions in the Universe have been tackled by recourse to different distribution functions. We provide here arguments favoring the formulation of a rather general distribution function (DF), of Poisson origin, describing galaxy clustering. The DF should be useful irrespective of distances or temperatures. We will be discussing distribution function for gravitational interactions.
Fil: Hameeda, Mir. Kasmir University; India. Inter University Centre for Astronomy and Astrophysics; India. Damghan University; Irán
Fil: Plastino, Ángelo. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina
Fil: Rocca, Mario Carlos. 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. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina
description In a cosmological context, observational best fits for galaxies’ distributions in the Universe have been tackled by recourse to different distribution functions. We provide here arguments favoring the formulation of a rather general distribution function (DF), of Poisson origin, describing galaxy clustering. The DF should be useful irrespective of distances or temperatures. We will be discussing distribution function for gravitational interactions.
publishDate 2021
dc.date.none.fl_str_mv 2021-03
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/181371
Hameeda, Mir; Plastino, Ángelo; Rocca, Mario Carlos; Generalized Poisson distributions for systems with two-particle interactions; IOP Publishing; IOP SciNotes; 2; 1; 3-2021; 1-8
2633-1357
CONICET Digital
CONICET
url http://hdl.handle.net/11336/181371
identifier_str_mv Hameeda, Mir; Plastino, Ángelo; Rocca, Mario Carlos; Generalized Poisson distributions for systems with two-particle interactions; IOP Publishing; IOP SciNotes; 2; 1; 3-2021; 1-8
2633-1357
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/2633-1357/abec9f
info:eu-repo/semantics/altIdentifier/doi/10.1088/2633-1357/abec9f
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1848598151830700032
score 13.24909

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