Anti-de Sitter neutron stars in the theory of gravity with nonminimal derivative coupling
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Publication:5878825
DOI10.1088/1475-7516/2023/01/005OpenAlexW4313990835MaRDI QIDQ5878825
P. E. Kashargin, Sergey V. Sushkov
Publication date: 23 February 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2205.08949
Cites Work
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- Extended gravity description for the GW190814 supermassive neutron star
- Stellar structure models in modified theories of gravity: lessons and challenges
- Structure of neutron stars in \(R\)-squared gravity
- The physics and astrophysics of neutron stars. With a foreword by Valeria Ferrari, Jerome Margueron and Jose A. Pons
- Neutron stars in scalar-tensor gravity with quartic order scalar potential
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Exact black hole solutions in shift symmetric scalar-tensor theories
- Compact objects in Horndeski gravity
- SOME ASPECTS OF GENERALIZED MODIFIED GRAVITY MODELS
- Scalar wormholes with nonminimal derivative coupling
- Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
- Stability of a Schwarzschild Singularity
- A no-hair theorem for stars in Horndeski theories
- Neutron star solutions with curvature induced scalarization in the extended Gauss-Bonnet scalar-tensor theories
- Instability of compact stars with a nonminimal scalar-derivative coupling
- Neutron stars in f(R,T) gravity with conserved energy-momentum tensor: Hydrostatic equilibrium and asteroseismology
- Dark energy and modified gravity in degenerate higher-order scalar–tensor (DHOST) theories: A review
- General Relativistic Polytropic Fluid Spheres.
- Neutron stars inf(R) gravity and scalar-tensor theories
- The confrontation between general relativity and experiment
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