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
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/167651
Ver los metadatos del registro completo
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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:UNLP2025-10-15T11:36:26Zoai: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:13292025-10-15 11:36:26.402SEDICI (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 |
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2011-07 |
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info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Objeto de conferencia http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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eng |
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eng |
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