Pseudo double-source plane lenses enable statistical strong lensing tomography that forecasts σ(w0) ~ 0.45 from the LSST 10-year photometric sample in flat w0waCDM cosmology.
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Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
Canonical reference. 91% of citing Pith papers cite this work as background.
abstract
In this paper we will list a few important goals that need to be addressed in the next decade, also taking into account the current discordances between the different cosmological probes, such as the disagreement in the value of the Hubble constant $H_0$, the $\sigma_8$--$S_8$ tension, and other less statistically significant anomalies. While these discordances can still be in part the result of systematic errors, their persistence after several years of accurate analysis strongly hints at cracks in the standard cosmological scenario and the necessity for new physics or generalisations beyond the standard model. In this paper, we focus on the $5.0\,\sigma$ tension between the {\it Planck} CMB estimate of the Hubble constant $H_0$ and the SH0ES collaboration measurements. After showing the $H_0$ evaluations made from different teams using different methods and geometric calibrations, we list a few interesting new physics models that could alleviate this tension and discuss how the next decade's experiments will be crucial. Moreover, we focus on the tension of the {\it Planck} CMB data with weak lensing measurements and redshift surveys, about the value of the matter energy density $\Omega_m$, and the amplitude or rate of the growth of structure ($\sigma_8,f\sigma_8$). We list a few interesting models proposed for alleviating this tension, and we discuss the importance of trying to fit a full array of data with a single model and not just one parameter at a time. Additionally, we present a wide range of other less discussed anomalies at a statistical significance level lower than the $H_0$--$S_8$ tensions which may also constitute hints towards new physics, and we discuss possible generic theoretical approaches that can collectively explain the non-standard nature of these signals.[Abridged]
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representative citing papers
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citing papers explorer
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Strong Lensing Tomography: Double and pseudo multi-source plane strong gravitational lensing to constrain dark energy
Pseudo double-source plane lenses enable statistical strong lensing tomography that forecasts σ(w0) ~ 0.45 from the LSST 10-year photometric sample in flat w0waCDM cosmology.
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Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions
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DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
DESI measures BAO scales in six redshift bins with 0.52% combined precision using 5.7 million objects, detecting the signal at up to 9.1 sigma and finding larger scales than Planck LCDM at z<0.8.
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$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity
Λ_s VCDM is a predictive model combining Λ_s CDM with VCDM gravity via an auxiliary scalar field and sigmoid-smoothed potentials to enable stable mirror AdS-to-dS transitions with possible transient acceleration.
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Skipping the rungs! Calibrating distance indicators through their clustering with galaxies
Cross-correlations of SN Ia in redshift and distance space with galaxies can constrain a constant magnitude offset ΔM at the ~0.05 level in optimistic survey forecasts, partially breaking the H0–ΔM degeneracy.
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Can Distance Duality Violation Save Late-time Solutions to the Hubble Tension?
For fixed sound-horizon and supernova calibrations, no late-time modification—even one violating cosmic distance duality—can resolve the Hubble tension, because the required ~8-10% CDDR violation is excluded by BAO, cosmic-chronometer, and CMB spectral constraints.
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HETDEX [OII] galaxies at $z \le 0.48$: Volume-limited samples and their power spectra
Volume-limited HETDEX [OII] samples at z≤0.48 have number densities 5–10 imes higher than typical ELG surveys and power spectra consistent with log(M0/h−1M⊙)≈11.9–12.3 and a weak luminosity slope a=0.37±0.10.
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Multipolar structure of the local expansion rate from incomplete sky data
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Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in 5 year data from the SPT-3G Main Survey
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Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM
Assuming τ=0.11±0.006 yields a 2σ positive neutrino mass detection (Σmν=0.10^{+0.04}_{-0.05} eV) and removes CMB-DESI tensions within ΛCDM.
-
Reduction of the Finsler gravity vacuum equation and dynamics for the cosmological Landsberg spacetimes
Finsler gravity vacuum equation reduces to vanishing Finsler Ricci curvature when some power F^n is regular with non-degenerate metric on light cones and Landsberg term vanishes, enabling solutions for homogeneous isotropic Landsberg spacetimes.
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Dark Matter with a Drag at Low Redshift
iDCDM adds two parameters to LambdaCDM so that dark matter decay produces late-time interacting radiation, yielding a distinctive low-redshift suppression of structure growth while leaving BBN and primary CMB unchanged.
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Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies
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Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension
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MG-NECOLA: A Field-Level Emulator for $f(R)$ Gravity and Massive Neutrino Cosmologies
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Observational Tests for Distinguishing Classes of Cosmological Models
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Constraining Neutrino Mass with the Void Weak Lensing Effect
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On the Physical Nature of the Scalar Mode Mass in the Jordan frame of a Metric $f(R)$ gravity
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Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology
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Linearized transverse diffeomorphism invariant spin-2 theories via gauge invariants
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Novel geometrical test of cosmological expansion from photometric data
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Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension
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Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference
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Validation of the Hybrid Bias Expansion model for the galaxy bispectrum
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Metastability in Emergent Dark Energy: A New Framework Confronting Cosmological Observations
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Rotating traversable wormholes and particle dynamics in $f(R,T)$ gravity
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Expected redshift drift for tilted observers
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Cosmological Dynamics of a Non-Canonical Generalised Brans-Dicke Theory
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Cosmological intercept tension
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A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension
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Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe?
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New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method
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Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
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Probing Dark Energy Microphysics with kSZ Tomography
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Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
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Cosmological Viability of Exponential Infrared $f(T)$ Gravity
Exponential IR f(T) gravity Model I alleviates Hubble tension but is disfavoured by combined Planck/ACT/SPT+DESI+Pantheon+ data; Model II is ruled out because background constraints force unphysical shifts in CMB parameters.
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Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
Axion EDE model fitted to Planck/ACT/SPT CMB, DESI BAO, and JWST UV luminosity function data yields H0 = 71.58 ± 1.05 km s^{-1} Mpc^{-1}, reduces H0 tension to 1.0 sigma, and improves Δχ^{2}_tot = -18.26 over Λ CDM.
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Observing Cosmic Reheating with the expanded Simons Observatory
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