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A new approach to the analysis of the phase space of f(R)-gravity

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arxiv 1505.06015 v2 pith:IMBT42XO submitted 2015-05-22 gr-qc astro-ph.COhep-thmath-phmath.MP

classification gr-qcastro-ph.COhep-thmath-phmath.MP
keywords analysisapproachdynamicalfixedgravitymodelsphasepoints
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We propose a new dynamical system formalism for the analysis of f(R) cosmologies. The new approach eliminates the need for cumbersome inversions to close the dynamical system and allows the analysis of the phase space of f(R)-gravity models which cannot be investigated using the standard technique. Differently form previously proposed similar techniques, the new method is constructed in such a way to associate to the fixed points scale factors, which contain four integration constants (i.e. solutions of fourth order differential equations). In this way a new light is shed on the physical meaning of the fixed points. We apply this technique to some f(R) Lagrangians relevant for inflationary and dark energy models.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. On phase-space singular surfaces in $f(R)$ gravity

    gr-qc 2026-06 unverdicted novelty 6.0 of 10

    Hamiltonian analysis reveals degenerate constraints on singular surfaces in f(R) gravity, leading to empty spectra on certain backgrounds and regularity conditions for dynamical crossings in Starobinsky model.

  2. Exploring the dynamics of coincident f(Q) gravity in the presence of DBI-essence scalar field

    gr-qc 2025-07 reject novelty 4.0 of 10

    The authors claim that power-law and exponential f(Q) gravity with a DBI-essence scalar field can reproduce matter, radiation, and late-time accelerating epochs, but the exponential model's critical points are not sho...

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