The Effective Field Theory of nonsingular cosmology

被引:109
|
作者
Cai, Yong [1 ]
Wan, Youping [1 ,2 ]
Li, Hai-Guang [1 ]
Qiu, Taotao [3 ,4 ]
Piao, Yun-Song [1 ,5 ]
机构
[1] Univ Chinese Acad Sci, Sch Phys, Beijing 100049, Peoples R China
[2] Univ Sci & Technol China, Chinese Acad Sci, CAS Key Lab Res Galaxies & Cosmol, Dept Astron, Hefei 230026, Anhui, Peoples R China
[3] Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China
[4] Cent China Normal Univ, Key Lab Quark & Lepton Phys MOE, Wuhan 430079, Peoples R China
[5] Chinese Acad Sci, Inst Theoret Phys, POB 2735, Beijing 100190, Peoples R China
来源
关键词
Spacetime Singularities; Classical Theories of Gravity; Cosmology of Theories beyond the SM; ART; INFLATION; UNIVERSE;
D O I
10.1007/JHEP01(2017)090
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this paper, we explore the nonsingular cosmology within the framework of the E ff ective Field Theory (EFT) of cosmological perturbations. Due to the recently proved no-go theorem, any nonsingular cosmological models based on the cubic Galileon su ff er from pathologies. We show how the EFT could help us clarify the origin of the no-go theorem, and o ff er us solutions to break the no-go. Particularly, we point out that the gradient instability can be removed by using some spatial derivative operators in EFT. Based on the EFT description, we obtain a realistic healthy nonsingular cosmological model, and show the perturbation spectrum can be consistent with the observations.
引用
收藏
页数:18
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