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dc.contributor.authorEdmonds, D.en_US
dc.contributor.authorFarrah, D.en_US
dc.contributor.authorMinic, D.en_US
dc.contributor.authorNg, Y. J.en_US
dc.contributor.authorTakeuchi, T.en_US
dc.date.accessioned2018-02-19T08:15:08Z
dc.date.available2018-02-19T08:15:08Z
dc.identifier.urihttp://hdl.handle.net/10919/82164
dc.description.abstractModified Dark Matter (MDM) is a phenomenological model of dark matter, inspired by gravitational thermodynamics, that naturally accounts for the universal acceleration constant observed in galactic rotation curve data; a critical acceleration related to the cosmological constant, $\Lambda$, appears as a phenomenological manifestation of MDM. We show that the resulting mass profiles, which are sensitve to $\Lambda$, are consistent with observations at the galactic and galaxy cluster scales. Our results suggest that dark matter mass profiles contain information about the cosmological constant in a non-trivial way.en_US
dc.relation.urihttp://arxiv.org/abs/1801.00160v1en_US
dc.subjectastro-ph.COen_US
dc.subjectastro-ph.COen_US
dc.subjecthep-phen_US
dc.subjecthep-then_US
dc.titleModified Dark Matter in Galaxies and Galaxy Clustersen_US
dc.typeArticle - Refereed
dc.description.notesTo be published in the Proceedings of the Bahamas Advanced Study Institute and Conferences (BASIC)en_US
dc.description.notesTo be published in the Proceedings of the Bahamas Advanced Study Institute and Conferences (BASIC)en_US
dc.identifier.orcidTakeuchi, T [0000-0002-3594-5149]en_US
pubs.organisational-group/Virginia Tech
pubs.organisational-group/Virginia Tech/All T&R Faculty
pubs.organisational-group/Virginia Tech/Science
pubs.organisational-group/Virginia Tech/Science/COS T&R Faculty
pubs.organisational-group/Virginia Tech/Science/Physics


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