Cited by 2,490Cosmology and Gravitation TheoriesDark Matter and Cosmic PhenomenaGalaxies: Formation, Evolution, Phenomena

ACCELERATING UNIVERSES WITH SCALING DARK MATTER

Open access
CHEVALLIER, MICHEL, POLARSKI, DAVID·2001·International Journal of Modern Physics D

Abstract

Friedmann–Robertson–Walker universes with a presently large fraction of the energy density stored in an X-component with w X <-1/3, are considered. We find all the critical points of the system for constant equations of state in that range. We consider further several background quantities that can distinguish the models with different w X values. Using a simple toy model with a varying equation of state, we show that even a large variation of w X at small redshifts is very difficult to observe with d L (z) measurements up to z~1. Therefore, it will require accurate measurements in the range 1<z<2 and independent accurate knowledge of Ω m,0 (and/or Ω X,0 ) in order to resolve a variable w X from a constant w X .

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1142/s0218271801000822

Cites

Statistics

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • In this construction, a single scalar field drives both late-time acceleration and ekpyrotic smoothing at the background level, while the spin-torsion sector supplies the repulsive ρs ∝ a^-6 contribution that regulates the high-density regime, instead of introducing separate ingredients for each phase.

    “In this restricted sense the construction is a direct extension of familiar quintessence dynamics [31,32]: a single scalar field drives both late-time acceleration and ekpyrotic smoothing at the background level, while the spin-torsion sector supplies the repulsive ρ s ∝ a -6 contribution that regulates the high-density regime, instead of introducing separate ingredients for each phase.”

    From Dynamical systems analysis of an Einstein–Cartan ekpyrotic nonsingular bounce cosmology (2026) · cites this paper as [31]

    Split into 2 atoms — 0 confirmed, 1 partially supported, 0 disputed, 0 misattributed, 1 unverifiable. Expand the claim to see per-atom verdicts.

    Experimental — accuracy not yet measured

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Cites

No references could be resolved yet.

Research works printed but not linked: 5

  1. [4][4] V. Sahni and A.A. Starobinsky, IJMPD, to appear (2000); astro-ph/9904398. - · arXiv
  2. [10][10] J. Weller and A. Albrecht, astro-ph/0008314; I.Maor, R. Brustein and P.J. Steinhardt, astro-ph/0007297 - · arXiv
  3. [12][12] R.R. Caldwell, astro-ph/9908168. - · arXiv
  4. [13][13] E. di Pietro and J. Demaret, gr-qc/9908071, IJMPD, to appear - · arXiv
  5. [15][15] S. Hanany et al. , astro-ph/0005123; A. Balbi et al. , astro-ph/0005124 - · arXiv

Cited by

Sorted by citations

Authors
CHEVALLIER, M., & POLARSKI, D.
Affiliations
Université de Tours (FR)
Venue
International Journal of Modern Physics D
Published
2001-04
Volume
10
Issue
02
Pages
213-223
ISSN
  • 0218-2718 (ISSN-L)
  • 1793-6594
OpenAlex
W2117797710
Cited by
2,490
References
0
Citations by year
2026: 274 · 2025: 305 · 2024: 155 · 2023: 128 · 2022: 100 · 2021: 115 · 2020: 105 · 2019: 130 · 2018: 135 · 2017: 88 · 2016: 106 · 2015: 64 · 2014: 100 · 2013: 81 · 2012: 100
FWCI
1.82
Type
journal article
Language
en
Open access
Locations
  • International Journal of Modern Physics D (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Keywords
FRW universe, dark energy equation of state, critical points, cosmic acceleration, luminosity distance, cosmological constraints

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review