Observational Constraints on the Acceleration Discrepancy Problem

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dc.creatorMcGaugh, Stacy
dc.date2006-06-14
dc.date.accessioned2026-07-07T07:12:12Z
dc.date.available2026-07-07T07:12:12Z
dc.descriptionI review the data relating to the appearance of the missing mass problem at a particular acceleration scale. Rotation curves are examined in detail, with emphasis on the empirical connection between baryonic and total mass distributions. Other lines of evidence are also considered, including disk stability, dwarf spheroidals, giant ellipticals, clusters of galaxies, the microwave background, BBN, and the growth of large scale structure.
dc.description55 pages (all figures). Annotated slides from invited review for the Alternative Gravities & Dark Matter Workshop
dc.identifierhttps://arxiv.org/abs/astro-ph/0606351
dc.identifierhttp://arxiv.org/abs/astro-ph/0606351
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/112001
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleObservational Constraints on the Acceleration Discrepancy Problem
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