The Cosmological Dependence of Galactic Specific Angular Momenta

Abstract

Hydrodynamical simulations of galaxy formation in spatially flat Cold Dark Matter (CDM) cosmologies with and without a cosmological constant (Lambda) are described. A simple star formation algorithm is employed and radiative cooling is allowed only after redshift z=1 so that enough hot gas is available to form large, rapidly rotating stellar discs if angular momentum is approximately conserved during collapse. The specific angular momenta of the final galaxies are found to be sensitive to the assumed background cosmology. This dependence arises from the different angular momenta contained in the haloes at the epoch when the gas begins to collapse and the inhomogeneity of the subsequent halo evolution. In the Lambda-dominated cosmology, the ratio of stellar specific angular momentum to that of the dark matter halo (measured at the virial radius) has a median value of ~0.24 at z=0. The corresponding quantity for the Lambda=0 cosmology is over 3 times lower. It is concluded that the observed frequency and angular momenta of disc galaxies pose significant problems for spatially flat CDM models with Lambda=0 but may be consistent with a Lambda-dominated CDM universe.

5 pages, 5 figures, submitted to MNRAS

References in corpus (4)

• The Formation of Galactic Disks
• The Deuterium Abundance Towards Q1009+2956
• Formation of disk galaxies: feedback and the angular momentum problem
• Constraints on Omega_Lambda and Omega_m from Distant Type 1a Supernovae and Cosmic Microwave Background Anisotropies

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