Ghost and Laplacian instabilities in teleparallel Horndeski gravity

被引:9
作者
Capozziello, Salvatore [1 ,2 ,3 ]
Caruana, Maria [4 ,5 ]
Said, Jackson Levi [4 ,5 ]
Sultana, Joseph [6 ]
机构
[1] Univ Napoli Federico II, Complesso Univ Monte S Angelo, Dipartimento Fis E Pancini, Via Cinthia 9 Edificio G, I-80126 Naples, Italy
[2] Ist Nazl Fis Nucl INFN, Complesso Univ Monte S Angelo, Sez Napoli, Via Cinthia 9 Edificio G, I-80126 Naples, Italy
[3] Scuola Super Meridionale, Largo San Marcellino 10, I-80138 Naples, Italy
[4] Univ Malta, Inst Space Sci & Astron, MSD-2080 Msida, Malta
[5] Univ Malta, Dept Phys, MSD-2080 Msida, Malta
[6] Univ Malta, Dept Math, MSD-2080 Msida, Malta
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2023年 / 03期
关键词
Cosmological perturbation theory in GR and beyond; modified gravity; gravitational waves; theory; Gravitational waves in GR and beyond; FIELD-EQUATIONS; TENSOR; INFLATION; TORSION;
D O I
10.1088/1475-7516/2023/03/060
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Teleparallel geometry offers a platform on which to build up theories of gravity where torsion rather than curvature mediates gravitational interaction. The teleparallel analogue of Horndeski gravity is an approach to teleparallel geometry where scalar-tensor theories are considered in this torsional framework. Teleparallel gravity is based on the tetrad formalism. This turns out to result in a more general formalism of Horndeski gravity. In other words, the class of teleparallel Horndeski gravity models is much broader than the standard metric one. In this work, we explore constraints on this wide range of models coming from ghost and Laplacian instabilities. The aim is to limit pathological branches of the theory by fundamental considerations. It is possible to conclude that a very large class of models results physically viable.
引用
收藏
页数:29
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