General effective field theory of teleparallel gravity

被引:6
|
作者
Mylova, Maria [1 ]
Said, Jackson Levi [2 ,3 ]
Saridakis, Emmanuel N. [4 ,5 ,6 ]
机构
[1] Ewha Womans Univ, Cosmol, 52 Ewhayeodae Gil, Seoul, South Korea
[2] Univ Malta, Inst Space Sci & Astron, MSD-2080 Msida, Malta
[3] Univ Malta, Dept Phys, MSD-2080 Msida, Malta
[4] Natl Observ Athens, Lofos Nymfon, Athens 11852, Greece
[5] Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
[6] Univ Catolica Norte, Dept Matemat, Avda Angamos 0610, Antofagasta 1280, Chile
基金
新加坡国家研究基金会;
关键词
effective field theory; teleparallel gravity; cosmology; DARK ENERGY; EQUATIONS; TENSOR;
D O I
10.1088/1361-6382/accccc
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We construct the effective field theory (EFT) of the teleparallel equivalent of general relativity (TEGR). Firstly, we present the necessary field redefinitions of the scalar field and the tetrads. Then we provide all the terms at next-to-leading-order, containing the torsion tensor and its derivatives, and derivatives of the scalar field, accompanied by generic scalar-field-dependent couplings, where all operators are suppressed by a scale ?. Removing all redundant terms using the field redefinitions we result to the EFT of TEGR, which includes significantly more terms comparing to the EFT of general relativity (GR). Finally, we present an application in a cosmological framework. Interestingly enough, although GR and TEGR are completely equivalent at the level of classical equations, we find that their corresponding EFTs possess minor but non-zero differences. Hence, we do verify that at higher energies the excitation and the features of the extra degrees of freedom are slightly different in the two theories, thus making them theoretically distinguishable. Nevertheless, we mention that these differences are suppressed by the heavy mass scale ? and thus it is not guaranteed that they could be measured in future experiments and observations.
引用
收藏
页数:22
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