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A new kind of cyclic universe

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

Combining intervals of ekpyrotic (ultra-slow) contraction with a (non-singular) classical bounce naturally leads to a novel cyclic theory of the universe in which the Hubble parameter, energy density and temperature oscillate periodically, but the scale factor grows by an exponential factor from one cycle to the next. The resulting cosmology not only resolves the homogeneity, isotropy, flatness and monopole problems and generates a nearly scale invariant spectrum of density perturbations, but it also addresses a number of age-old cosmological issues that big bang inflationary cosmology does not. There may also be wider-ranging implications for fundamental physics, black holes and quantum measurement.

years

2024 2

representative citing papers

Assessing observational constraints on dark energy

astro-ph.CO · 2024-05-07 · conditional · novelty 6.0

Quintessence models satisfying NEC everywhere predict the w0 > -1 and w0+wa < -1 sector favored by data, due to an approximate degeneracy in the w(z) = w0 + wa z/(1+z) parameterization.

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Showing 2 of 2 citing papers.

  • Assessing observational constraints on dark energy astro-ph.CO · 2024-05-07 · conditional · none · ref 27 · internal anchor

    Quintessence models satisfying NEC everywhere predict the w0 > -1 and w0+wa < -1 sector favored by data, due to an approximate degeneracy in the w(z) = w0 + wa z/(1+z) parameterization.

  • Dynamical system analysis in descending dark energy model gr-qc · 2024-02-02 · unverdicted · none · ref 25 · internal anchor

    Dynamical system analysis of Q-SC-CDM model finds stable attractor solution under alternative parameter choice.