Gravitational Microlensing and the Galactic Halo

Details Gravitational Microlensing and the Galactic Halo Gravitational Microlensing and the Galactic Halo

1995-08-17

arxiv.org/abs/astro-ph/9508071v1

Phys.Rev.D53:4138-4176,1996

Astronomy and Astrophysics

Astrophysics

19 pages, 13 multipart figures are available at ftp://astro.uchicago.edu/ftp/pub/astro/gyuk/

Scientific paper

10.1103/PhysRevD.53.4138

By means of extensive galactic modeling we study the implications of the more than eighty microlensing events that have now been observed for the composition of the dark halo of the Galaxy, as well as for other properties of the Galaxy. We take the Galaxy to be comprised of luminous and dark disk components, a bulge, and a dark halo consisting of both MACHOs and cold dark matter with each component being described by several observationally motivated parameters. We pare down an initial model space of millions of galactic models to viable models, those which are consistent with the observational data, including rotation curve, local projected mass density, and microlensing rates toward the LMC and bulge. On the basis of a conservative, minimal set of observational constraints an all-MACHO halo cannot yet be excluded, although in most viable models of the Galaxy the halo MACHO fraction is between 0\% and 30\%, consistent with expectations for a universe whose primary component is cold dark matter. An all-MACHO halo is required to be light, and when data on the local escape velocity and satellite-galaxy proper motions, which probe the extent of the dark halo, are taken into account, models which have a high MACHO mass fraction are ruled out. We also explore the possibility that there are no MACHOs in the halo. Finally, we point out several important tests that could definitively exclude an all-MACHO e.g., optical depth for microlensing which is less than $1.5\times 10^{-7}$ toward the LMC or greater than $3\times 10^{-6}$ toward the bulge.

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