Can a changing α explain the supernovae results?

被引:45
作者
Barrow, JD
Magueijo, J
机构
[1] Univ Cambridge, Ctr Math Sci, Dept Appl Math & Theoret Phys, Cambridge CB3 0LA, England
[2] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Theoret Phys Grp, London SW7 2BZ, England
关键词
cosmology : observations; cosmology : theory; early universe;
D O I
10.1086/312572
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that the supernovae results, which imply that there is evidence for an accelerating universe, may be closely related to the recent discovery of redshift dependence in the fine-structure constant or. The link is a class of varying speed-of-light (VSL) theories that contain cosmological solutions that are similar to quintessence. During the radiation-dominated epoch, the cosmological constant Lambda is prevented from dominating the universe by the usual VSL mechanism. In the matter-dominated epoch, the varying-e effects switch off, allowing Lambda to eventually surface and lead to an accelerating universe. By the time this happens, the residual variations in c imply a changing or at a rate that is in a,agreement with observations.
引用
收藏
页码:L87 / L90
页数:4
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