MACHOs: The Plot Thickens

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dc.creatorTurner, Michael S.
dc.creatorGates, Evalyn I.
dc.creatorGyuk, Geza
dc.date1996-01-29
dc.date.accessioned2026-07-07T02:20:49Z
dc.date.available2026-07-07T02:20:49Z
dc.descriptionWe discuss the implications of the recent upward revision of the LMC microlensing rate by the MACHO Collaboration. We conclude: (i) A good case for the existence of baryonic dark matter in the halo has been made; (ii) The case for the existence of cold dark matter is unaffected and still compelling; and (iii) The Galactic halo is still an excellent place to search for cold dark matter particles (e.g., axions or neutralinos).
dc.description6 pages, two figures, postscript
dc.identifierhttps://arxiv.org/abs/astro-ph/9601168
dc.identifierhttp://arxiv.org/abs/astro-ph/9601168
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10343
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleMACHOs: The Plot Thickens
dc.typetext

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