Gravitationall lensing evidence against extended dark matter halos

It is generally thought that galaxies are embedded in dark matter halos extending
well beyond their luminous matter. The existence of these galactic halos is mainly
derived from the larger than expected velocities of stars and gas in the outskirts of
spiral galaxies. Much less is known about dark matter around early-type (elliptical
or lenticular) galaxies. We use gravitational lensing to derive the masses of early-type
galaxies deflecting light of background quasars. This provides a robust measurement of
the total mass within the Einstein ring, a circle whose diameter is comparable to the
separation of the different quasar images. We find that the mass-to-light ratio of the
lensing galaxies does not depend on radius, from inner galactic regions out to several
half-light radii. Moreover, its value does not exceed the value predicted by stellar
population models by more than a factor two, which may be explained by baryonic
dark matter alone, without any need for exotic matter. Our results thus suggest that,
if dark matter is present in early-type galaxies, its amount does not exceed the amount
of luminous matter and its density follows that of luminous matter, in sharp contrast
to what is found from rotation curves of spiral galaxies.