CMBR anisotropy: Theoretical approaches

被引：4
作者：
Barbashov, B. M. [1 ]
Pervushin, V. N.
Zakharov, A. F.
Zinchuk, V. A.
机构：
[1] Joint Inst Nucl Res, Bogolyubov Lab Theoret Phys, Dubna 141980, Moscow Oblast, Russia
[2] Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
[3] Inst Theoret & Expt Phys, Moscow 117259, Russia
[4] Russian Acad Sci, PN Lebedev Phys Inst, Ctr Astro Space, Moscow, Russia
来源：
PHYSICS OF ATOMIC NUCLEI | 2007年 / 70卷 / 01期
基金：
中国国家自然科学基金;
关键词：
D O I：
10.1134/S1063778807010243
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
A version of the cosmological perturbation theory based on exact resolution of the energy constraint is developed. In this version, the conformal time is invariant with respect to the diffeomorphisms of general relativity, and the scalar perturbations are the potential ones in accordance with the Dirac minimal surface constraint. The exact resolution gives one a possibility to fulfill the Hamiltonian reduction and to explain the "CMBR primordial power spectrum" and other problems of modern cosmology by quantization of the energy constraint and cosmological creation of matter.
引用
收藏
页码：191 / 197
页数：7
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