{ "id": "1511.01096", "version": "v1", "published": "2015-11-03T21:00:02.000Z", "updated": "2015-11-03T21:00:02.000Z", "title": "Precision measurement of the local bias of dark matter halos", "authors": [ "Titouan Lazeyras", "Christian Wagner", "Tobias Baldauf", "Fabian Schmidt" ], "comment": "23 pages, 8 figures", "categories": [ "astro-ph.CO" ], "abstract": "We present accurate measurements of the linear, quadratic, and cubic local bias of dark matter halos, using curved \"separate universe\" N-body simulations which effectively incorporate an infinite-wavelength overdensity. This can be seen as an exact implementation of the peak-background split argument. We compare the results with the linear and quadratic bias measured from the halo-matter power spectrum and bispectrum, and find good agreement. On the other hand, the standard peak-background split applied to the Sheth & Tormen (1999) and Tinker et al. (2008) halo mass functions matches the measured linear bias parameter only at the level of 10%. The prediction from the excursion set-peaks approach performs much better, which can be attributed to the stochastic moving barrier employed in the excursion set-peaks prediction. We also provide convenient fitting formulas for the nonlinear bias parameters $b_2(b_1)$ and $b_3(b_1)$.", "revisions": [ { "version": "v1", "updated": "2015-11-03T21:00:02.000Z" } ], "analyses": { "keywords": [ "dark matter halos", "precision measurement", "halo mass functions matches", "excursion set-peaks approach performs", "peak-background split" ], "publication": { "doi": "10.1088/1475-7516/2016/02/018", "journal": "Journal of Cosmology and Astro-Particle Physics", "year": 2016, "month": "Feb", "volume": 2016, "number": 2, "pages": "018" }, "note": { "typesetting": "TeX", "pages": 23, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2016JCAP...02..018L", "inspire": 1402741 } } }