Dark energy-like stars from nonminimally coupled scalar field

DOI10.1088/0264-9381/30/14/145006zbMath1273.83148arXiv1212.3781OpenAlexW3102256678MaRDI QIDQ2843849

Anja Marunović, Dubravko Horvat

Publication date: 26 August 2013

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1212.3781

zbMATH Keywords

negative pressurenonminimally coupled scalar fielddark energy starminimal extension of the Einstein-Hilbert actionordinary boson star

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Related Items (2)

Merger of dark matter axion clumps and resonant photon emission ⋮ Dynamical boson stars

Uses Software

• COLSYS

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