A test of the Copernican principle

被引:132
作者
Caldwell, R. R. [1 ]
Stebbins, A. [2 ]
机构
[1] Dartmouth Coll, Dept Phys & Astron, Wilder Lab 6127, Hanover, NH 03755 USA
[2] Fermilab Natl Accelerator Lab, Theoret Astrophys Grp, Batavia, IL 60510 USA
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevLett.100.191302
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The blackbody nature of the cosmic microwave background (CMB) radiation spectrum is used in a modern test of the Copernican principle. The reionized universe serves as a mirror to reflect CMB photons, thereby permitting a view of ourselves and the local gravitational potential. By comparing with measurements of the CMB spectrum, a limit is placed on the possibility that we occupy a privileged location, residing at the center of a large void. The Hubble diagram inferred from lines of sight originating at the center of the void may be misinterpreted to indicate cosmic acceleration. Current limits on spectral distortions are shown to exclude the largest voids which mimic cosmic acceleration. More sensitive measurements of the CMB spectrum could prove the existence of such a void or confirm the validity of the Copernican principle.
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页数:4
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