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Автор Shuichiro Yokoyama
Дата выпуска 2011-11-01
dc.description We investigate the halo bias in the case where the primordial curvature fluctuations, Φ, are sourced from both a Gaussian random field and a Gaussian-squared field, as Φ(x) = φ(x)+ψ(x)<sup>2</sup>−⟨ψ(x)<sup>2</sup>ångle, so-called ``ungaussiton model''. We employ the peak-background split formula and find a new scale-dependence in the halo bias induced from the Gaussian-squared field.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Scale-dependent bias from the primordial non-Gaussianity with a Gaussian-squared field
Тип paper
DOI 10.1088/1475-7516/2011/11/001
Electronic ISSN 1475-7516
Журнал Journal of Cosmology and Astroparticle Physics
Том 2011
Первая страница 1
Последняя страница 001
Аффилиация Shuichiro Yokoyama; Department of Physics and Astrophysics, Nagoya University, Aichi 464-8602, Japan
Выпуск 11

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