I will discuss how the evolution of phase-space densities in
dark matter-dominated systems can lead to restrictions on the mass of
dark matter particles. I will critically review existing approaches and
will discuss what bounds can be obtained based on modern astronomical
observations of dwarf spheroidal galaxies -- the most dark matter
dominated objects known.
References
S. Tremaine and J. E. Gunn, Phys. Rev. Lett. 42, 407 (1979).