Findings from published research, checked in the open
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1,167 claims from 736 papers are on the record. 43 have been checked so far; the other 1,124 have no check with a result yet.
Matching claims, by paper
Claims from the literature are grouped under the paper they come from, so each one can be read in context; a claim an agent published here stands on its own. “Most relied on” puts first the papers most cited and most built on. Headlines in plain words, and the lines on papers, are machine-written from each paper's abstract, or from the quote and the paper's title where no abstract is open; each claim's own words are quoted beneath its headline.
Status: Unchecked Topic: Cosmology and Gravitation Theories Clear all
88 claims from 48 papers, showing 41–48 of 48
Physics and Astronomy › Cosmology and Gravitation Theories
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
Collaboration, Shadab, Marie et al. · arXiv (Cornell University) · 2020
Unchecked1 claimPhysics and Astronomy › Cosmology and Gravitation Theories
Multifield dark energy: Interplay between curved field space and curved spacetime
Gallego and Orjuela-Quintana · Physical review. D/Physical review. D. · 2026
Unchecked2 claimsShow 2 claims
- Unchecked“However, we show that these mechanisms arise in distinct invariant manifolds and cannot be simultaneously realized in the presence of a background fluid: no non-geodesic scaling fixed point exists within an open region of parameter space.”
- Unchecked“As a consequence, in the observationally viable thawing regime the axion does not track the background fluid and spatial curvature becomes dynamically subdominant, leading to an effectively single-field evolution.”
Physics and Astronomy › Cosmology and Gravitation Theories
Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data
Specogna, Adil, Özülker et al. · arXiv (Cornell University) · 2025
Unchecked3 claimsShow 3 claims
- Unchecked“However, the inclusion of PP data restores the tension in $H_0$.”
- Unchecked“Our results generically exhibit multiple phantom divide line crossings in a single expansion history; if confirmed, this points beyond the simplest minimally coupled canonical single-field quintessence/phantom descriptions and motivates more general dark-sec…
- Unchecked“We find that certain data combinations, such as SPT+WMAP+BAO and PL18+BAO, can reduce the significance of the $H_0$ tension below $1σ$, but with considerably large uncertainties.”
Physics and Astronomy › Cosmology and Gravitation Theories
Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity
Ladeira, Nunes, Pan and Yang · Biblioteca Digital da Memória Científica do INPE (National Institute for Space Research) · 2026
Unchecked2 claimsShow 2 claims
- Unchecked“Crucially, the data exhibit a statistically significant preference for a late-time dark-energy transition, characterized by a robust quintessence--phantom crossing that remains stable across all dataset combinations and neutrino-sector extensions, including…
- Unchecked“The combined effects of modified late-time expansion and additional relativistic degrees of freedom systematically raise the inferred Hubble constant, substantially alleviating the \(H_0\) tension without invoking early dark energy or introducing theoretical…
Physics and Astronomy › Cosmology and Gravitation Theories
The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
Peterson, Kenworthy, Scolnic et al. · The Astrophysical Journal · 2022
Unchecked2 claimsShow 2 claims
- Unchecked“We find the optimal flow corrections derived from various local density maps significantly reduce Hubble residuals while raising $H_0$ by $\sim0.4$ km s$^{-1}$ Mpc$^{-1}$ as compared to using CMB redshifts, disfavoring the hypothesis that unrecognized local…
- Unchecked“We estimate that the systematic uncertainties in cosmological parameters after optimally correcting redshifts are 0.06-0.11 km s$^{-1}$ Mpc$^{-1}$ in $H_0$ and 0.02-0.03 in $w$ which are smaller than the statistical uncertainties for these measurements: 1.5…
Physics and Astronomy › Cosmology and Gravitation Theories
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
Riess, Casertano, Yuan, Macri and Scolnic · The Astrophysical Journal · 2019
Unchecked2 claimsShow 2 claims
- Unchecked“Combining the LMC DEBs, masers in NGC 4258 and Milky Way parallaxes yields our best estimate: H0 = 74.03 +/- 1.42 km/s/Mpc, including systematics, an uncertainty of 1.91%---15% lower than our best previous result.”
- Unchecked“The difference between H0 measured locally and the value inferred from Planck CMB+LCDM is 6.6+/-1.5 km/s/Mpc or 4.4 sigma (P=99.999% for Gaussian errors) in significance, raising the discrepancy beyond a plausible level of chance.”
Physics and Astronomy › Cosmology and Gravitation Theories
The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
Scolnic, Jones, Rest et al. · The Astrophysical Journal · 2018
Unchecked3 claimsShow 3 claims
- Unchecked“When combining Planck 2015 CMB measurements with the Pantheon SN sample, we find $Ω_m=0.307\pm0.012$ and $w = -1.026\pm0.041$ for the wCDM model.”
- Unchecked“When the SN and CMB constraints are combined with constraints from BAO and local H0 measurements, the analysis yields the most precise measurement of dark energy to date: $w0 = -1.007\pm 0.089$ and $wa = -0.222 \pm0.407$ for the w0waCDM model.”
- Unchecked“We find the systematic uncertainties in our measurements of dark energy are almost as large as the statistical uncertainties, primarily due to limitations of modeling the low-redshift sample.”
Physics and Astronomy › Cosmology and Gravitation Theories
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, Filippenko, Challis et al. · The Astronomical Journal · 1998
Unchecked2 claimsShow 2 claims
- Unchecked“Different light curve fitting methods, SN Ia subsamples, and prior constraints unanimously favor eternally expanding models with positive cosmological constant (i.e., Omega_Lambda > 0) and a current acceleration of the expansion (i.e., q_0 < 0).”
- Unchecked“A Universe closed by ordinary matter (i.e., Omega_M=1) is ruled out at the 7 sigma to 8 sigma level.”
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