Simplest curvaton model

被引:23
作者
Bartolo, N
Liddle, AR
机构
[1] Dipartimento Fis Padova G Galilei, I-35131 Padua, Italy
[2] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy
[3] Univ Sussex, Ctr Astron, Brighton BN1 9QJ, E Sussex, England
来源
PHYSICAL REVIEW D | 2002年 / 65卷 / 12期
关键词
D O I
10.1103/PhysRevD.65.121301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyze the simplest possible realization of the curvaton scenario, where a nearly scale-invariant spectrum of adiabatic perturbations is generated by conversion of an isocurvature perturbation generated during inflation, rather than the usual inflationary mechanism. We explicitly evaluate all the constraints on the model, under both the assumptions of prompt and delayed reheating, and we outline the viable parameter space.
引用
收藏
页数:5
相关论文
共 10 条
[1]  
BARTOLO N, 2001, PHYS REV D, V6408, P3504
[2]   Adiabatic CMB perturbations in pre-Big-Bang string cosmology [J].
Enqvist, K ;
Sloth, MS .
NUCLEAR PHYSICS B, 2002, 626 (1-2) :395-409
[3]  
Kolb E. W., 1990, The Early Universe, DOI [10.1201/9780429492860, DOI 10.1201/9780429492860]
[4]  
Liddle A.R., 2000, COSMOLOGICAL INFLATI
[5]   Non-Gaussian isocurvature perturbations from inflation [J].
Linde, A ;
Mukhanov, V .
PHYSICAL REVIEW D, 1997, 56 (02) :R535-R539
[6]   Generating the curvature perturbation without an inflaton [J].
Lyth, DH ;
Wands, D .
PHYSICS LETTERS B, 2002, 524 (1-2) :5-14
[7]   ISOCURVATURE BARYON PERTURBATIONS AND INFLATION [J].
MOLLERACH, S .
PHYSICAL REVIEW D, 1990, 42 (02) :313-325
[8]   Effects of cosmological moduli fields on cosmic microwave background [J].
Moroi, T ;
Takahashi, T .
PHYSICS LETTERS B, 2001, 522 (3-4) :215-221
[9]  
WANG X, ASTROPH0105091
[10]  
WANG XN, IN PRESS PHYS REV D