Do Newtonian large-scale structure simulations fail to include relativistic effects?

被引:14
|
作者
Faraoni, Valerio [1 ,2 ]
Lapierre-Leonard, Marianne [1 ]
Prain, Angus [1 ,2 ]
机构
[1] Bishops Univ, Dept Phys, Sherbrooke, PQ J1M 1Z7, Canada
[2] Bishops Univ, STAR Res Cluster, Sherbrooke, PQ J1M 1Z7, Canada
来源
PHYSICAL REVIEW D | 2015年 / 92卷 / 02期
基金
加拿大自然科学与工程研究理事会;
关键词
ENERGY; TESTS;
D O I
10.1103/PhysRevD.92.023511
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Newtonian simulations describing the formation of large-scale structures do not include relativistic effects. A new approach to this problem is proposed, which consists of splitting the Hawking-Hayward quasilocal energy of a closed spacelike 2-surface into a "Newtonian" part due to local perturbations and a "relativistic" part due to the cosmology. It is found that the Newtonian part dominates over the relativistic one as time evolves, lending support to the validity of Newtonian simulations.
引用
收藏
页数:8
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