Resolving cosmological singularities

被引:99
作者
Chamseddine, Ali H. [1 ,2 ]
Mukhanov, Viatcheslav [3 ,4 ,5 ]
机构
[1] Amer Univ Beirut, Phys Dept, Beirut, Lebanon
[2] IHES, F-91440 Bures Sur Yvette, France
[3] Niels Bohr Int Acad, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
[4] Ludwig Maxmillians Univ, Theoret Phys, Theresienstr 37, D-80333 Munich, Germany
[5] MPI Phys, Foehringer Ring 6, D-80850 Munich, Germany
基金
美国国家科学基金会;
关键词
cosmic singularity; modified gravity; COLLAPSE;
D O I
10.1088/1475-7516/2017/03/009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We find a simple modification of the longitudinal mode in General Relativity which incorporates the idea of limiting curvature. In this case the singularities in contracting Friedmann and Kasner universes are avoided, and instead, the universe has a regular bounce which takes place during the time inversely proportional to the square root of the limiting curvature. Away from the bounce, corrections to General Relativity are negligible. In addition the non-singluar modification of General Relativity delivers for free a realistic candidate for Dark Matter.
引用
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页数:12
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