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Desjacques, V; Seljak, U; Iliev, I T (2010). Effect of primordial non-Gaussianity on halo bias and mass function. In: Invisible Universe International Conference, Paris, FR, 29 June 2010 - 03 July 2010, 826-835.

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Abstract

We discuss the effect of quadratic and cubic local non-Gaussianity on the mass function and bias of dark matter halos extracted from cosmological N-body simulations. This type of non-Gaussianity induces a k-dependent bias in the large-scale clustering of rare objects. While we find that at low wavenumbers k<0.03 hMpc-1 the theory and the simulations agree well with each other for biased halos with b(M)>1.5, including a scale independent correction to the non-Gaussian bias improves the agreement on small scales where the k-dependent effect becomes rapidly negligible. Using available large-scale structure data, we obtain a limit on the size of the cubic nonlinear parameter of -3.5×105< gNL<8.2×105. Future observations shall improve this bound by 1-2 orders of magnitude.

Item Type:Conference or Workshop Item (Paper), not refereed, original work
Communities & Collections:07 Faculty of Science > Institute of Theoretical Physics
DDC:530 Physics
Language:English
Event End Date:03 July 2010
Deposited On:03 Mar 2011 16:52
Last Modified:28 Nov 2013 02:00
Publisher:American Institute of Physics
Series Name:AIP Conference Proceedings
Number:1241
ISSN:0094-243X (P) 1551-7616 (E)
ISBN:10.1063/1.3462723
Publisher DOI:10.1063/1.3462723
Related URLs:http://opac.nebis.ch/F/?local_base=NEBIS&con_lng=GER&func=find-b&find_code=SYS&request=006196849
http://universe2009.obspm.fr/ (Organisation)
Citations:Web of Science®
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