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Cosmology at at Crossroads: Tension with the Hubble Constant

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

3 Pith papers citing it
abstract

We are at an interesting juncture in cosmology. With new methods and technology, the accuracy in measurement of the Hubble constant has vastly improved, but a recent tension has arisen that is either signaling new physics or as-yet unrecognized uncertainties.

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astro-ph.CO 3

years

2026 2 2019 1

verdicts

UNVERDICTED 3

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representative citing papers

Mapping the Universe as a Bianchi I cosmology with Gaia data

astro-ph.CO · 2026-05-28 · unverdicted · novelty 5.0

Gaia quasar proper motions show a significant quadrupole signal matching an axisymmetric Bianchi I anisotropy model, but the amplitude does not increase with redshift as the model requires and the inferred local shear exceeds expectations.

Cosmological searches for the neutrino mass scale and mass ordering

astro-ph.CO · 2019-07-18 · unverdicted · novelty 4.0

Thesis summarizing an upper limit of 0.12 eV on the neutrino mass sum, bias calibration via CMB lensing cross-correlations, and tighter limits plus stronger normal-ordering preference in non-phantom dynamical dark energy models.

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Showing 3 of 3 citing papers after filters.

  • Mapping the Universe as a Bianchi I cosmology with Gaia data astro-ph.CO · 2026-05-28 · unverdicted · none · ref 68 · internal anchor

    Gaia quasar proper motions show a significant quadrupole signal matching an axisymmetric Bianchi I anisotropy model, but the amplitude does not increase with redshift as the model requires and the inferred local shear exceeds expectations.

  • Cosmological searches for the neutrino mass scale and mass ordering astro-ph.CO · 2019-07-18 · unverdicted · none · ref 30 · internal anchor

    Thesis summarizing an upper limit of 0.12 eV on the neutrino mass sum, bias calibration via CMB lensing cross-correlations, and tighter limits plus stronger normal-ordering preference in non-phantom dynamical dark energy models.

  • Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension astro-ph.CO · 2026-05-25 · unverdicted · none · ref 24 · internal anchor

    An extended model with decaying dark matter around equality and w0 dark energy yields H0 ≈ 70 km/s/Mpc from Planck+ACT+DESI data, reducing Hubble tension to ~2.2σ while producing Bayesian evidence comparable to ΛCDM.