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- W1656586285 abstract "We study the mass and redshift dependence of the concentration parameter in Nbody simulations spanning masses from $10^{10} hMsun$ to $10^{15} hMsun$ and redshifts from 0 to 2. We present a series of fitting formulas that accurately describe the time evolution of the concentration-mass relation since z=2. Using arguments based on the spherical collapse model we study the behaviour of the scale length of the density profile during the assembly history of haloes, obtaining physical insights on the origin of the observed time evolution of the concentration mass relation. We present preliminary results of the implementation of this model in the prediction of the values of the concentration parameter for different masses and redshifts." @default.
- W1656586285 created "2016-06-24" @default.
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- W1656586285 date "2011-02-10" @default.
- W1656586285 modified "2023-10-16" @default.
- W1656586285 title "The Redshift Evolution of LCDM Halo Parameters" @default.
- W1656586285 cites W1892812743 @default.
- W1656586285 doi "https://doi.org/10.48550/arxiv.1102.2186" @default.
- W1656586285 hasPublicationYear "2011" @default.
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