Kinematical properties of time-like trajectories in \(R\pm\mu^4/R\) theory of gravity
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Publication:267266
DOI10.1007/S10773-015-2651-XzbMath1337.83017OpenAlexW2221308323MaRDI QIDQ267266
Publication date: 8 April 2016
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-015-2651-x
Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Equations of motion in general relativity and gravitational theory (83C10)
Cites Work
- Static spherically symmetric solution of \((R \pm \mu ^{4}/R)\) gravity
- Can modified gravity explain accelerated cosmic expansion?
- \(1/R\) gravity and scalar-tensor gravity
- Are<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Dark Energy Models Cosmologically Viable?
- The Newtonian limit of metric gravity theories with quadratic Lagrangians
- Cosmological parameters from SDSS and WMAP
- CURVATURE QUINTESSENCE
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- Spherical symmetry in f ( R )-gravity
- Brane-world gravity
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