Numerical evolution of cosmological scalar field perturbations

被引：0
|
作者：
Herrera-Martin, Antonio [1 ]
Arturo Urena-Lopez, L. [1 ]
机构：
[1] Univ Guanajuato, Dept Fis, DCI, Leon 37150, Guanajuato, Mexico
来源：
IX WORKSHOP OF THE GRAVITATION AND MATHEMATICAL PHYSICS DIVISION OF THE MEXICAN PHYSICAL SOCIETY | 2012年 / 1473卷
关键词：
Scalar field dark matter; linear perturbation theory; structure formation;
D O I：
10.1063/1.4748544
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We present preliminary results of the lattice evolution of a scalar field endowed with a parabolic potential, using a modified version of the numerical setting provided by the preheating code HLattice. The evolution of linear perturbations in this model is compared with the standard results of linear perturbations of cold dark matter. It is shown that, using appropriate definitions on the lattice, that both the unperturbed and perturbed fields have the same behavior as in the case of cold dark matter.
引用
收藏
页码：126 / 131
页数：6
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