Multipoint propagators for non-Gaussian initial conditions

被引:32
作者
Bernardeau, Francis [1 ]
Crocce, Martin [2 ]
Sefusatti, Emiliano [1 ]
机构
[1] CEA Saclay, Inst Phys Theor, CEA DSM IPhT, Unite Rech Associee CNRS, F-91191 Gif Sur Yvette, France
[2] IEEC CSIC, Inst Ciencies Espai, Fac Ciencies, Barcelona 08193, Spain
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 08期
关键词
LARGE-SCALE STRUCTURE; ACOUSTIC-OSCILLATIONS; NONLINEAR EVOLUTION; CONSTRAINTS;
D O I
10.1103/PhysRevD.82.083507
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show here how renormalized perturbation theory calculations applied to the quasilinear growth of the large-scale structure can be carried on in presence of primordial non-Gaussian (PNG) initial conditions. It is explicitly demonstrated that the series reordering scheme proposed in Bernardeau, Crocce, and Scoccimarro [Phys. Rev. D 78, 103521 (2008)] is preserved for non-Gaussian initial conditions. This scheme applies to the power spectrum and higher-order spectra and is based on a reorganization of the contributing terms into the sum of products of multipoint propagators. In case of PNG, new contributing terms appear, the importance of which is discussed in the context of current PNG models. The properties of the building blocks of such resummation schemes, the multipoint propagators, are then investigated. It is first remarked that their expressions are left unchanged at one-loop order irrespective of statistical properties of the initial field. We furthermore show that the high-momentum limit of each of these propagators can be explicitly computed even for arbitrary initial conditions. They are found to be damped by an exponential cutoff whose expression is directly related to the moment generating function of the one-dimensional displacement field. This extends what had been established for multipoint propagators for Gaussian initial conditions. Numerical forms of the cutoff are shown for the so-called local model of PNG.
引用
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页数:14
相关论文
共 31 条
[1]   Primordial bispectrum information from CMB polarization [J].
Babich, D ;
Zaldarriaga, M .
PHYSICAL REVIEW D, 2004, 70 (08)
[2]   Signatures of primordial non-Gaussianities in the matter power-spectrum and bispectrum: the time-RG approach [J].
Bartolo, Nicola ;
Beltran Almeida, Juan P. ;
Matarrese, Sabino ;
Pietroni, Massimo ;
Riotto, Antonio .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2010, (03)
[3]  
Bell ET., 1934, Am Math Mon, V41, P411, DOI [DOI 10.1080/00029890.1934.11987615, 10.1080/00029890.1934.11987615]
[4]   Large-scale structure of the Universe and cosmological perturbation theory [J].
Bernardeau, F ;
Colombi, S ;
Gaztañaga, E ;
Scoccimarro, R .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2002, 367 (1-3) :1-248
[5]   Multipoint propagators in cosmological gravitational instability [J].
Bernardeau, Francis ;
Crocce, Martin ;
Scoccimarro, Roman .
PHYSICAL REVIEW D, 2008, 78 (10)
[6]   Propagators in Lagrangian space [J].
Bernardeau, Francis ;
Valageas, Patrick .
PHYSICAL REVIEW D, 2008, 78 (08)
[7]   Memory of initial conditions in gravitational clustering [J].
Crocce, M ;
Scoccimarro, R .
PHYSICAL REVIEW D, 2006, 73 (06)
[8]   Renormalized cosmological perturbation theory [J].
Crocce, M ;
Scoccimarro, R .
PHYSICAL REVIEW D, 2006, 73 (06)
[9]   Nonlinear evolution of baryon acoustic oscillations [J].
Crocce, Martin ;
Scoccimarro, Roman .
PHYSICAL REVIEW D, 2008, 77 (02)
[10]   Primordial non-Gaussianity from the large-scale structure [J].
Desjacques, V. ;
Seljak, U. .
CLASSICAL AND QUANTUM GRAVITY, 2010, 27 (12) :1-29