Faraway matter as a possible substitute for dark matter

Autores
Carati, Andrea; Galgani, Luigi
Año de publicación
2011
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
A review is given of an attempt, made in two recent papers, to estimate the gravitational action of faraway matter on a test particle, in connection with the velocity dispersion in clusters of galaxies and with the rotation curves of spiral galaxies, respectively. Under the assumptions that faraway matter has a fractal distribution and that the gravitational action has a correlation length of the order of some kiloparsec, the gravitational action of faraway matter appears to be sufficient to explain the observations relative to such two phenomena, without invoking any local, dark matter contribution.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
faraway matter
dark matter
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/167651

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spelling Faraway matter as a possible substitute for dark matterCarati, AndreaGalgani, LuigiCiencias Astronómicasfaraway matterdark matterA review is given of an attempt, made in two recent papers, to estimate the gravitational action of faraway matter on a test particle, in connection with the velocity dispersion in clusters of galaxies and with the rotation curves of spiral galaxies, respectively. Under the assumptions that faraway matter has a fractal distribution and that the gravitational action has a correlation length of the order of some kiloparsec, the gravitational action of faraway matter appears to be sufficient to explain the observations relative to such two phenomena, without invoking any local, dark matter contribution.Facultad de Ciencias Astronómicas y Geofísicas2011-07info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf277-287http://sedici.unlp.edu.ar/handle/10915/167651enginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:44:40Zoai:sedici.unlp.edu.ar:10915/167651Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:44:40.821SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Faraway matter as a possible substitute for dark matter
title Faraway matter as a possible substitute for dark matter
spellingShingle Faraway matter as a possible substitute for dark matter
Carati, Andrea
Ciencias Astronómicas
faraway matter
dark matter
title_short Faraway matter as a possible substitute for dark matter
title_full Faraway matter as a possible substitute for dark matter
title_fullStr Faraway matter as a possible substitute for dark matter
title_full_unstemmed Faraway matter as a possible substitute for dark matter
title_sort Faraway matter as a possible substitute for dark matter
dc.creator.none.fl_str_mv Carati, Andrea
Galgani, Luigi
author Carati, Andrea
author_facet Carati, Andrea
Galgani, Luigi
author_role author
author2 Galgani, Luigi
author2_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
faraway matter
dark matter
topic Ciencias Astronómicas
faraway matter
dark matter
dc.description.none.fl_txt_mv A review is given of an attempt, made in two recent papers, to estimate the gravitational action of faraway matter on a test particle, in connection with the velocity dispersion in clusters of galaxies and with the rotation curves of spiral galaxies, respectively. Under the assumptions that faraway matter has a fractal distribution and that the gravitational action has a correlation length of the order of some kiloparsec, the gravitational action of faraway matter appears to be sufficient to explain the observations relative to such two phenomena, without invoking any local, dark matter contribution.
Facultad de Ciencias Astronómicas y Geofísicas
description A review is given of an attempt, made in two recent papers, to estimate the gravitational action of faraway matter on a test particle, in connection with the velocity dispersion in clusters of galaxies and with the rotation curves of spiral galaxies, respectively. Under the assumptions that faraway matter has a fractal distribution and that the gravitational action has a correlation length of the order of some kiloparsec, the gravitational action of faraway matter appears to be sufficient to explain the observations relative to such two phenomena, without invoking any local, dark matter contribution.
publishDate 2011
dc.date.none.fl_str_mv 2011-07
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url http://sedici.unlp.edu.ar/handle/10915/167651
dc.language.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
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277-287
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