4.7 Article

Coupling matter in modified Q gravity

期刊

PHYSICAL REVIEW D
卷 98, 期 8, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.98.084043

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资金

  1. Fundacao para a Ciencia e a Tecnologia (FCT, Portugal) through an Investigador FCT Research Contract [IF/00859/2012]
  2. Ramon y Cajal Contract (Spain) [RYC-2013-13019]
  3. FCT [SFRH/BPD/102958/2014, UID/FIS/04434/2013, PEst-OE/FIS/UI2751/2014, PTDC/FIS-OUT/29048/2017]
  4. Spanish Projects [FIS2014-57387-C3-1-P, FIS2017-84440-C2-1-P]
  5. project H2020-MSCA-RISE-2017 [FunFiCO-777740]
  6. Generalitat Valenciana [SEJI/2017/042]
  7. Consolider Program CPANPHY [1205388]
  8. Severo Ochoa grant (Spain) [SEV-2014-0398]
  9. COST (European Cooperation in Science and Technology) [CA15117]

向作者/读者索取更多资源

We present a novel theory of gravity by considering an extension of symmetric teleparallel gravity. This is done by introducing, in the framework of the metric-affine formalism, a new class of theories where the nonmetricity Q is nonminimally coupled to the matter Lagrangian. More specifically, we consider a Lagrangian of the form L similar to f(1)(Q) + f(2)(Q)L-M, where f(1) and f(2) are generic functions of Q, and L-M is the matter Lagrangian. This nonminimal coupling entails the nonconservation of the energy-momentum tensor, and consequently the appearance of an extra force. The formulation of the gravity sector in terms of the Q instead of the curvature may result in subtle improvements of the theory. In the context of nonminimal matter couplings, we are therefore motivated to explore whether the new geometrical formulation in terms of the Q, when implemented also in the matter sector, would allow more universally consistent and viable realizations of the nonminimal coupling. Furthermore, we consider several cosmological applications by presenting the evolution equations and imposing specific functional forms of the functions f(1)(Q) and f(2)(Q), such as power-law and exponential dependencies of the nonminimal couplings. Cosmological solutions are considered in two general classes of models, and found to feature accelerating expansion at late times.

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