Death of baryonic dark matter

The nature of the dark matter in the Halo of our Galaxy remains a mystery. Arguments are presented that the dark matter does not consist of ordinary s tellar or substellar objects, i.e., the dark matter is not made of faint st ars, brown dwarfs, white dwarfs, or neutron stars. In fact, faint stars and brown dwarfs constitute no more than a few percent of the mass of our Gala xy, and stellar remnants must satisfy Omega(WD) less than or equal to 3 x 1 0(-3) h(-1,) where h is the Hubble constant in units of 100 km s(-1) Mpc(-1 ). On theoretical grounds one is then pushed to more exotic explanations. I ndeed a nonbaryonic component in the Halo seems to be required. (C) 2000 El sevier Science B.V. All rights reserved.