12
Halo Mass and Velocity functions

Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

  • Upload
    others

  • View
    0

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Halo Mass and Velocity functions

Page 2: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Functional form for mass function:

Average matter density:

Numerical factor:

rms density fluctuation:

Page 3: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Warren et al 2006

Page 4: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Tinker etal 2008

Halo mass function at z=0

Note the vertical axis scaling: the main trend of the mass function - dn/dM∼M-2 -

has been taken away. We are looking at the deviations from the power-law.

Page 5: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Nearly universal shape of mass function when we plot

Page 6: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Read et al 2007

Evolution of the mass function with redshift

Page 7: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Evolution of the mass function with redshift

Symbols are from N-body simulations for distinct halos defined using Spherical Overdensity algorithm

Full curves are for the Sheth-Torman approximation

Page 8: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend
Page 9: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend
Page 10: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Halo Velocity function

For each halo we find mass within given radius M(<r) and then find maximum of circular velocity

Page 11: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Halo Velocity function

Page 12: Halo Mass and Velocity functions - NMSU Astronomyastronomy.nmsu.edu/aklypin/COSMOLOGY/HaloMassFunction.pdf · Halo mass function at z=0 Note the vertical axis scaling: the main trend

Halo Velocity function