HALOFIT: nonlinear distribution of cosmological mass and galaxies

Peacock, J A and Smith, R E (2014) HALOFIT: nonlinear distribution of cosmological mass and galaxies. Astrophysical Source Code Library (ASLC), The Royal Observatory, Edinburgh.

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Abstract

HALOFIT provides an explanatory framework for galaxy bias and clustering and has been incorporated into CMB packages such as CMBFAST (ascl:9909.004) and CAMB (ascl:1102.026). It attains a reasonable level of precision, though the halo model does not match N-body data perfectly. The code is written in Fortran 77. HALOFIT tends to underpredict the power on the smallest scales in standard LCDM universes (although HALOFIT was designed to work for a much wider range of power spectra); its accuracy can be improved by using a supplied correction.

Item Type: Other
Schools and Departments: School of Mathematical and Physical Sciences > Physics and Astronomy
Subjects: Q Science > QB Astronomy
Related URLs:
Depositing User: Billy Wichaidit
Date Deposited: 12 Sep 2017 15:15
Last Modified: 12 Sep 2017 15:15
URI: http://sro.sussex.ac.uk/id/eprint/70124

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