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The mass of dark scalar and phase space analysis of realistic models of static spherically symmetric objects

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arxiv 1512.03931 v1 pith:AAH6A7W2 submitted 2015-12-12 gr-qc

classification gr-qc
keywords darkformgravityintroducemassmodelsobjectsphase
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We consider singularities of static spherically symmetric objects in minimal dilatonic gravity. They are only partially studied and purely understood even in the simplest models of extended gravity. We introduce the proper form of the structure equations and derive a set of all singularities, which turn to form several types of sub-manifolds of the phase space. We also introduce for the first time the Lyapunov function for the corresponding system, its equation, and its basic properties. The dependence on the mass of the dark scalar is discussed.

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  1. White dwarfs in minimal dilatonic gravity

    gr-qc 2026-08 accept novelty 6.0 of 10

    White dwarfs in minimal dilatonic gravity are sub-Chandrasekhar for all scalar Compton lengths, with maximum mass dropping from 1.425 to 1.09 solar masses at λΦ = 500 km.

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