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Using a set of high-resolution dark matter only cosmological simulations wefound a correlation between the dark matter halo mass M and its spin parameterlambda for objects forming at redshifts z > 10: the spin parameter decreaseswith increasing mass. However, halos forming at later times do not exhibit sucha strong correlation, in agreement with the findings of previous studies. Whilewe presented such a correlation in a previous study using the Bullock et al.(2001) spin parameter defintion we now defer to the classical definitionshowing that the results are independent of the definition.

A correlation between spin parameter and dark matter halo mass