Constraints on self-interacting dark matter
- Department of Physics, Ohio State University, Columbus, Ohio 43210 (United States)
- Bartol Research Institute, University of Delaware, Newark, Delaware 19716 (United States)
We consider the growth of density perturbations in the presence of self-interacting dark matter (SIDM), proposed by Carlson, Machacek, & Hall. We determine the range of values for the coupling constant {lambda} and the particle mass {ital m}{prime}, for which the power spectrum lies in the {open_quote}{open_quote}allowed{close_quote}{close_quote} range based on constraints from the {ital IRAS} galaxy survey and damped Ly{alpha} systems. Our results show that no combination of parameters can meet both limits. We consider constraints on the 2{leftrightarrow}2 scatterings which keep the SIDM particles in pressure equilibrium, and we show that if such interactions maintain pressure equilibrium down to the present, they will be strong enough to disrupt galaxy mergers and may lead to stripping of galaxy halos as galaxies move through the dark matter background of these particles. Hence, we also investigate the evolution of large-scale structure in the SIDM model when the particles drop out of pressure equilibrium at some higher redshift. The resulting free streaming leads to an additional suppression of small-scale perturbations, but it does not significantly affect our results. {copyright} {ital 1995 The American Astronomical Society.}
- Research Organization:
- The Ohio State Univ., Columbus, OH (United States)
- DOE Contract Number:
- AC02-76ER01545
- OSTI ID:
- 279462
- Journal Information:
- Astrophysical Journal, Vol. 452, Issue 2; Other Information: PBD: Oct 1995
- Country of Publication:
- United States
- Language:
- English
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