Faraway matter as a possible substitute for dark matter
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...
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I19-R120-10915-1676512024-07-01T20:02:17Z http://sedici.unlp.edu.ar/handle/10915/167651 Faraway matter as a possible substitute for dark matter Carati, Andrea Galgani, Luigi 2011-07 2012 2024-07-01T17:07:20Z en Ciencias Astronómicas faraway matter dark matter 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 Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 277-287 |
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Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Ciencias Astronómicas faraway matter dark matter |
spellingShingle |
Ciencias Astronómicas faraway matter dark matter Carati, Andrea Galgani, Luigi Faraway matter as a possible substitute for dark matter |
topic_facet |
Ciencias Astronómicas faraway matter dark matter |
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. |
format |
Objeto de conferencia Objeto de conferencia |
author |
Carati, Andrea Galgani, Luigi |
author_facet |
Carati, Andrea Galgani, Luigi |
author_sort |
Carati, Andrea |
title |
Faraway matter as a possible substitute for 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 |
publishDate |
2011 |
url |
http://sedici.unlp.edu.ar/handle/10915/167651 |
work_keys_str_mv |
AT caratiandrea farawaymatterasapossiblesubstitutefordarkmatter AT galganiluigi farawaymatterasapossiblesubstitutefordarkmatter |
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1807223540479426560 |