A compactified phase-space analysis of four dark matter/phantom scalar interactions shows one model avoids Big Rip singularities, one needs a small coupling to avoid them, and two have singular surfaces that make them unattractive.
A dynamical systems formulation for inhomogeneous LRS-II spacetimes
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
We present a dynamical system formulation for inhomogeneous LRS-II spacetimes using the covariant 1+1+2 decomposition approach. Our approach describes the LRS-II dynamics from the point of view of a comoving observer. Promoting the covariant radial derivatives of the covariant dynamical quantities to new dynamical variables and utilizing the commutation relation between the covariant temporal and radial derivatives, we were able to construct an autonomous system of first-order ordinary differential equations along with some purely algebraic constraints. Using our dynamical system formulation we found several interesting features in the LRS-II phase space with dust, one of them being that the homogeneous solutions constitute an invariant submanifold. For the particular case of LTB, we were also able to recover the previously known result that an expanding LTB tends to Milne in the absence of a cosmological constant, providing a potential validation of our formalism.
citation-role summary
citation-polarity summary
fields
gr-qc 1years
2024 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Revise the Dark Matter-Phantom Scalar Field Interaction
A compactified phase-space analysis of four dark matter/phantom scalar interactions shows one model avoids Big Rip singularities, one needs a small coupling to avoid them, and two have singular surfaces that make them unattractive.