2022
DOI: 10.48550/arxiv.2203.04167
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Is the dark energy equation of state parameter singular?

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Cited by 5 publications
(7 citation statements)
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“…On the other hand, the BAO data from intermediate redshifts z ∼ 0.5, viz., galaxy BAO data, are consistent with the Planck-ΛCDM [220]. This picture can be explained with a DE density that decreases significantly with increasing redshift within the redshift range 0.5 z 2.3, possibly, transitioning to the values below zero (implying a pole in the DE EoS parameter [752]), which can give rise to a non-monotonic behavior of H(z). This also finds support from model-independent (non-parametric) reconstructions of DE that consider Ly-α together with other data sets.…”
Section: Cmb Dipole: Intrinsic Versus Kinematic?supporting
confidence: 75%
See 1 more Smart Citation
“…On the other hand, the BAO data from intermediate redshifts z ∼ 0.5, viz., galaxy BAO data, are consistent with the Planck-ΛCDM [220]. This picture can be explained with a DE density that decreases significantly with increasing redshift within the redshift range 0.5 z 2.3, possibly, transitioning to the values below zero (implying a pole in the DE EoS parameter [752]), which can give rise to a non-monotonic behavior of H(z). This also finds support from model-independent (non-parametric) reconstructions of DE that consider Ly-α together with other data sets.…”
Section: Cmb Dipole: Intrinsic Versus Kinematic?supporting
confidence: 75%
“…Here "sgn" is the signum function that reads sgn[x] = −1, 0, 1 for x < 0, x = 0 and x > 0, respectively. This expression indicates if there exists a sign change in the energy density of the gDE (accompanied by a pole in its EoS parameter [752]), it will happen at the redshift…”
Section: Graduated Dark Energy -Ads To Ds Transition In the Late Univ...mentioning
confidence: 99%
“…The occurrence of w-singularities in various other contexts has also been discussed in [103,[144][145][146][147]. Hence while type V singularities deal primarily with a more indirect cosmological parameter, it by no means diminishes its cosmological importance and it does appear in a variety of cosmological expansion scenarios.…”
Section: W Singularities (Type V)mentioning
confidence: 98%
“…[7] (see also Refs. [8][9][10][11]), which considers the minimal dynamical deviation from the null inertial mass density (corresponding to the minimal deviation from simple-graduated dark energy) of the form ∝ ρ λ < 0 (where λ is a ratio of two odd integers).…”
Section: Introductionmentioning
confidence: 99%
“…Due to the presence of the logarithmic function of the trace of EMT, similar generation of constant inertial mass density is also possible in f (R, T ) gravity of the form f (R, T ) = R + 2β ln T , proposed in[30], yet it has not been mentioned by the authors [see Eqs (11). and(12)].…”
mentioning
confidence: 99%