Noether's stars in \(f(\mathcal{R})\) gravity
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Publication:1750576
DOI10.1016/J.PHYSLETB.2018.03.001zbMath1390.83301arXiv1802.09073OpenAlexW2788060873WikidataQ63380382 ScholiaQ63380382MaRDI QIDQ1750576
Publication date: 22 May 2018
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1802.09073
Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)
Related Items (3)
Stellar structure models in modified theories of gravity: lessons and challenges ⋮ Stellar structures in \(f(\mathcal{G})\) gravity admitting Noether symmetries ⋮ Static spherically symmetric solutions in a subclass of Horndeski theories of gravity
Cites Work
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- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- The dark matter problem from f(R) gravity viewpoint
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- Spherically symmetric solutions in f ( R ) gravity via the Noether symmetry approach
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- Analytical representations of unified equations of state of neutron-star matter
- Noether symmetry approach for Dirac–Born–Infeld cosmology
- Rotating stars in relativity
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