Experimental Limits on the Dark Matter Halo of the Galaxy from Gravitational Microlensing

Publication information:

C. Alcock, R. A. Allsman, T. S. Axelrod, D. P. Bennett, K. H. Cook, K. C. Freeman, K. Griest, J. A. Guern, M. J. Lehner, S. L. Marshall, H. -S. Park, S. Perlmutter, B. A. Peterson, M. R. Pratt, P. J. Quinn, A. W. Rodgers, C. W. Stubbs, and W. Sutherland. 1995. “Experimental Limits on the Dark Matter Halo of the Galaxy from Gravitational Microlensing”. Physical Review Letters, 74, Pp. 2867. doi:10.1103/PhysRevLett.74.2867

Abstract

We monitored 8.6×10⁶ stars in the Large Magellanic Cloud for 1.1 years and have found three events consistent with gravitational microlensing. We place strong constraints on Galactic halo lensing objects in the mass range 10^-4M_solar to 10^-1M_solar. Three events are fewer than expected for a standard spherical halo of objects in this mass range, but appear to exceed the number expected from known Galactic populations. Fitting a naive spherical halo model to our data yields a MACHO fraction f of massive compact halo objects (MACHOs), f = 0.19^+0.16_-0.10, a total MACHO mass (inside 50 kpc) of 7.6⁺⁶_-4×10¹⁰M_solar, and a microlensing optical depth 8.8⁺⁷_-5×10^-8 (68% C.L.).