Generalizing the MOND description of rotation curves

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dc.creatorCosta, Sandro S. e
dc.creatorOpher, R.
dc.date2001-12-19
dc.date.accessioned2026-07-07T02:02:01Z
dc.date.available2026-07-07T02:02:01Z
dc.descriptionWe present new mathematical alternatives for explaining rotation curves of spiral galaxies in the MOND context. For given total masses, it is shown that various mathematical alternatives to MOND, while predicting flat rotation curves for large galactic radii, predict curves with different peculiar features for smaller radii. They are thus testable against observational data.
dc.descriptionelsart style (uses packages graphics and amssymb), 9 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0112454
dc.identifierhttp://arxiv.org/abs/astro-ph/0112454
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3952
dc.subjectAstrophysics
dc.titleGeneralizing the MOND description of rotation curves
dc.typetext

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