Non-linear extension of non-metricity scalar for MOND

DOI10.1016/J.PHYSLETB.2020.135970zbMath1475.83111arXiv2004.00888OpenAlexW3014638712MaRDI QIDQ820445

Mudit Garg, Lavinia Heisenberg, Fabio D'Ambrosio

Publication date: 27 September 2021

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2004.00888

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) General theory of nonlinear incidence geometry (51B05) Dark matter and dark energy (83C56)

Related Items (7)

Constraint on the equation of state parameter (\(\omega\)) in non-minimally coupled \(f(Q)\) gravity ⋮ Scalar field cosmology with powerlaw and hybrid expansion law in symmetric teleparallel gravity ⋮ Anisotropic Strange Star Model Beyond Standard Maximum Mass Limit by Gravitational Decoupling in f(Q)$f(Q)$ Gravity ⋮ Hamiltonian Analysis of f(Q)$f(\mathbb {Q})$ Gravity and the Failure of the Dirac–Bergmann Algorithm for Teleparallel Theories of Gravity ⋮ First evidence that non-metricity \(f(Q)\) gravity could challenge \(\Lambda\)CDM ⋮ Anisotropic compact stars admitting Karmarkar condition in \(f(\mathcal{Q})\) theory ⋮ Late-time cosmology with phantom dark-energy in f(Q) gravity

Cites Work

• New kinetic interactions for massive gravity?
• Gravitational polarization and the phenomenology of MOND

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