☆ 3.8 Article

On the Evolution of the Hubble Constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: A Feasibility Study for GRB-Cosmology in 2030

GALAXIES (2022)

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A dark energy model from generalized Proca theory

Chao-Qiang Geng et al.

Summary: In this study, a specific dark energy model up to cubic order in terms of vector field self-interactions in the generalized Proca theory was considered. The cosmological parameters were examined using CMB and CMB+HST data sets, revealing a Hubble constant that could alleviate the tension. The reduced chi(2) values in the model when fitting with CMB and CMB+HST were close to unity, indicating that the model is a good candidate to describe the cosmological evolutions of the universe.

PHYSICS OF THE DARK UNIVERSE (2021)

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Article Astronomy & Astrophysics

Geometry versus growth Internal consistency of the flat ?CDM model with KiDS-1000

Jaime Ruiz-Zapatero et al.

Summary: Researchers conducted a multi-probe self-consistency test of the flat ΛCDM model, finding strong consistency in the constraints on geometry and growth parameters, but tensions persist in aspects such as matter density fluctuation amplitude and the Hubble constant. Including a subset of CMB information in the probe combination enhances differences rather than alleviates them, signaling potential discrepancies between low and high multipoles in the Planck data.

ASTRONOMY & ASTROPHYSICS (2021)

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Article Astronomy & Astrophysics

Measurements of the Hubble Constant: Tensions in Perspective*

Wendy L. Freedman

Summary: Recent advancements in measuring the distances to nearby galaxies have led to improved calibrations of the tip of the red giant branch (TRGB) method, resulting in consistent values for the Hubble constant. The TRGB results show no statistically significant difference with values determined from the cosmic microwave background, and are also in agreement with other calibration methods such as SHoES and Spitzer plus Hubble Space Telescope (HST) Key Project Cepheid calibrations. The simplicity and small systematic uncertainties of the TRGB method make it a promising tool for exploring cosmological models without the need for additional physics beyond the standard (?CDM) cosmological model.

ASTROPHYSICAL JOURNAL (2021)

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Article Astronomy & Astrophysics

Toward Precision Cosmology with Improved PNLF Distances Using VLT-MUSEI. Methodology and Tests

Martin M. Roth et al.

Summary: This study explores the potential of the DELF technique using archival MUSE data, demonstrating its superiority in high surface brightness regions of galaxies and validating its effectiveness through data analysis of early-type and late-type spiral galaxies. The technique is capable of producing precise [O iii] photometry out to distances of 40 Mpc under excellent observing conditions, while also discriminating between different emission-line objects. These capabilities make MUSE a valuable tool for measuring PNLF distances beyond traditional methods and constraining the local value of the Hubble constant.

ASTROPHYSICAL JOURNAL (2021)

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Article Astronomy & Astrophysics

Influence of the Bounds of the Hyperparameters on the Reconstruction of the Hubble Constant with the Gaussian Process

Wen Sun et al.

Summary: The Gaussian process (GP) method is widely used in reconstructing the Hubble constant, with the hyperparameters inside GP influencing the results. Constraints on the lower and upper bounds of GP's hyperparameters are essential for reliable extrapolation of the Hubble constant from GP.

ASTROPHYSICAL JOURNAL (2021)

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Article Astronomy & Astrophysics

Cosmological Evolution of the Formation Rate of Short Gamma-Ray Bursts with and without Extended Emission

M. G. Dainotti et al.

Summary: This study determines the true formation rate (FR) of short gamma-ray bursts (SGRBs) and its relation to the cosmic star formation rate (SFR) through observations. The results suggest that SGRBs may have been more luminous in the past, with an FR delayed relative to the SFR as expected in the merger scenario.

ASTROPHYSICAL JOURNAL LETTERS (2021)

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Article Astronomy & Astrophysics

On the Existence of the Plateau Emission in High-energy Gamma-Ray Burst Light Curves Observed by Fermi-LAT

M. G. Dainotti et al.

Summary: The study reveals the existence of plateau-like features in some gamma-ray bursts observed by the Fermi Gamma-ray Space Telescope, showing different astrophysical environments and density characteristics. By comparing the end times of gamma-ray and X-ray plateaus, some interesting results are revealed. Additionally, a relation among the end time of the plateau, its corresponding luminosity, and the peak prompt luminosity for 222 GRBs observed by Swift is found.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2021)

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Article Astronomy & Astrophysics

Does Hubble tension signal a breakdown in FLRW cosmology?

C. Krishnan et al.

Summary: The study focuses on reanalyzing the Hubble tension with a recent age of the Universe constraint, finding that low redshift data and well-motivated priors only permit a dark energy sector close to the cosmological constant, ruling out late Universe modifications within FLRW. Future data, especially strongly lensed quasar data, could provide further confirmation of this resolution.

CLASSICAL AND QUANTUM GRAVITY (2021)

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Review Astronomy & Astrophysics

In the realm of the Hubble tension-a review of solutions *

Eleonora Di Valentino et al.

Summary: There are significant discrepancies in predictions of the Hubble constant, leading to various proposed solutions including new physics theories or modifications to existing cosmological models. Some solutions successfully reduce tension and improve agreement with data, while many others fail to do so, highlighting the need for further research and evidence.

CLASSICAL AND QUANTUM GRAVITY (2021)

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Article Physics, Particles & Fields

Is non-particle dark matter equation of state parameter evolving with time?

Souvik Ghose et al.

EUROPEAN PHYSICAL JOURNAL C (2021)

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Article Physics, Particles & Fields

Constraining the anisotropy of the Universe with the X-ray and UV fluxes of quasars

Dong Zhao et al.

Summary: In this study, the anisotropy in the Finslerian cosmological model was tested using X-ray and UV fluxes of quasars. The dipole anisotropy was found to be weak, and the Hubble constant H0 showed a slight decrease in the central value but remained consistent within statistical uncertainties with other results.

EUROPEAN PHYSICAL JOURNAL C (2021)

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Article Physics, Multidisciplinary

Cosmological Models with Big Rip and Pseudo Rip Scenarios in Extended Theory of Gravity

Pratik P. Ray et al.

Summary: In this paper, we explore the big rip and pseudo rip cosmological models in an extended theory of gravity. Both models violate strong energy conditions to facilitate late-time cosmic acceleration. The choice of coupling parameter significantly impacts the evolution of the universe.

FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS (2021)

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Article Astronomy & Astrophysics

Nonminimal coupling inflation with constant slow roll

Mehdi Shokri et al.

Summary: In this paper, a single-field inflationary model modified by a nonminimal coupling term is studied in the context of constant-roll inflation, using a first-order formalism. The approach considers two functions of the scalar field and can be applied to various cosmological situations, analyzing power-law and exponential couplings separately. The inflationary parameters of the models are compared with CMB observations to achieve a physically motivated model.

INTERNATIONAL JOURNAL OF MODERN PHYSICS D (2021)

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Article Astronomy & Astrophysics

Dark energy as a critical phenomenon: a hint from Hubble tension

Abdolali Banihashemi et al.

Summary: A new critically emergent dark energy model (CEDE) is proposed, which is consistent with both Planck's CMB data and Riess et al.'s local Hubble constant measurements. The model suggests that dark energy emerges at a transition redshift, providing a possible explanation for the Hubble constant tension.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Article Astronomy & Astrophysics

Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology

Mauricio Reyes et al.

Summary: This work presents an improvement on Gaussian reconstruction of the Hubble parameter data and explores new constraints in the Horndeski theory of gravity. The research finds that the prior used to calibrate the Pantheon supernovae data significantly affects the reconstructions, with the best fit reconstruction calibrated using the Ho value from The Carnegie-Chicago Hubble Program.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Article Astronomy & Astrophysics

Can the Hubble tension be resolved by bulk viscosity?

Ben David Normann et al.

Summary: The cosmic bulk viscosity estimated in previous works may provide a way to reconcile the H-0 values inferred from observations of the early universe with those inferred from the local (late) universe.

MODERN PHYSICS LETTERS A (2021)

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Article Astronomy & Astrophysics

Constraining cosmological parameters from strong lensing with DECIGO and B-DECIGO sources

Shaoqi Hou et al.

Summary: Gravitational lensing can be used to constrain cosmology models through statistical lensing and time delay methods, with potential improvements in measurements tightening constraints on parameters. Estimated events from future interferometers could significantly impact the knowledge of cosmological parameters.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Article Physics, Particles & Fields

A gravitino distance conjecture

Alberto Castellano et al.

Summary: The study conjectures that in a consistent supergravity theory, the limit as the gravitino mass approaches zero is at an infinite distance. This conjecture may be motivated by the Weak Gravity Conjecture and implies the AdS Distance Conjecture. By examining classical 4D type IIA orientifold vacua, one can determine parameter values related to the scale decoupling exponent in AdS vacua.

JOURNAL OF HIGH ENERGY PHYSICS (2021)

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Article Astronomy & Astrophysics

The Hubble Tension, the M Crisis of Late Time H(z) Deformation Models and the Reconstruction of Quintessence Lagrangians

Anastasios Theodoropoulos et al.

Summary: This study provides a detailed analysis of recent cosmological data, including CMB, BAO, and SnIa, to constrain dark energy parameterizations. The results show inconsistencies with locally determined values and reveal late phantom behavior in the dark energy equation-of-state parameter.

UNIVERSE (2021)

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Article Astronomy & Astrophysics

Testing AdS early dark energy with Planck, SPTpol, and LSS data

Jun-Qian Jiang et al.

Summary: This study tests the AdS-EDE model with CMB and large-scale structure data, finding the best fit values that may resolve the Hubble tension issue.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Late-time acceleration due to a generic modification of gravity and the Hubble tension

Shahnawaz A. Adil et al.

Summary: A scenario of modified gravity is considered, where late-time acceleration is achieved through interaction between dark matter and baryonic components. This leads to distinctive late-time cosmic features and significant reduction in the Hubble tension under chosen scale factor parametrizations.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Spatial curvature in f (R) gravity

Christine R. Farrugia et al.

Summary: In this study, the researcher constrained four f(R) gravity models using cosmological data and sampling techniques, finding differences in results when treating Omega(k,0) as a free parameter compared to a flat scenario. Including the Hubble constant in the analysis favored a slightly open universe at just over 1 sigma, highlighting the important implications of the Hubble tension for spatial curvature assumptions.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Small-scale clumping at recombination and the Hubble tension

Michael Rashkovetskyi et al.

Summary: Recent data improvements have led to tensions between low-and high-redshift observables, particularly in determinations of the Hubble constant H-0 and the (rescaled) clustering amplitude S-8. Study shows that small-scale baryon inhomogeneities can affect recombination and potentially alleviate tensions between H-0 and S-8. However, current data suggest that clumping parameters altering the CMB sound horizon may not be favored by Planck 2018 data.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Accounting for Selection Bias and Redshift Evolution in GRB Radio Afterglow Data

Maria Dainotti et al.

Summary: This study addresses inherent bias in Gamma-ray Burst (GRB) data and corrects for important variables related to GRB emission, revealing strong evolution with redshift in most variables. The analysis emphasizes the necessity of correcting observational data for evolutionary effects to use them as discriminators among theoretical models and as reliable cosmological tools.

GALAXIES (2021)

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Article Astronomy & Astrophysics

Unbiased likelihood-free inference of the Hubble constant from light standard sirens

Francesca Gerardi et al.

Summary: The study demonstrates that using likelihood-free inference (LFI) in multimessenger observations of binary neutron star mergers can result in unbiased estimation of H-0 in the presence of selection effects, with precision matching that of traditional Bayesian methods.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Probing elastic interactions in the dark sector and the role of S8

Jose Beltran Jimenez et al.

Summary: Observational constraints were placed on two models featuring an elastic interaction between dark energy and dark matter. The findings suggest that the Hubble tension can be alleviated due to additional radiation, and the sigma 8 tension present in the ?-cold-dark-matter model can be eased by weaker galaxy clustering in these interacting models. Furthermore, while CMB + BAO + SnIa data provide upper bounds on the coupling strength, low-redshift data strongly support nonvanishing values of the interaction parameters.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Dark sector to restore cosmological concordance

Itamar J. Allali et al.

Summary: The study introduces a new phenomenological model to address tensions between early and late universe observations by incorporating decaying dark energy and an ultralight axion. Analysis shows that this dark sector model fits a combination of cosmic microwave background, baryon acoustic oscillations, and Large Scale Structure data slightly better than the ACDM model.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Late-time Universe, H0-tension, and unparticles

Maryam Aghaei Abchouyeh et al.

Summary: This study presents a framework for evaluating the viability of late-time cosmology models by investigating unparticle cosmology, which proposes a scale invariant contribution by a dimensionless parameter delta. It is found that for most values of delta, the late-time Universe will be matter dominated, with negligible contribution of unparticles. While unparticle cosmology fails to address challenges to late-time Lambda CDM, it does provide a pointer to holographic dark energy.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4

Leander Thiele et al.

Summary: Small-scale inhomogeneities in baryon density around recombination have been suggested as a solution to discrepancies in Hubble constant determinations. Predictions from baryon clumping models were tested using data from the Atacama Cosmology Telescope, but no evidence of baryon clumping was found. The inferred Hubble constant remains significantly different from measurements by SHOES.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Cosmic variance of H0 in light of forthcoming high-redshift surveys

Giuseppe Fanizza et al.

Summary: The study introduces a fully relativistic framework to evaluate the impact of stochastic inhomogeneities on the determination of the Hubble constant, linking fluctuations of the luminosity distance-redshift relation to the intrinsic uncertainty associated with high-redshift surveys. Analytical results suggest that deep surveys will provide a more precise estimation of H-0 compared to local sources.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Generalized emergent dark energy model and the Hubble constant tension

Weiqiang Yang et al.

Summary: The study investigates a generalized emergent dark energy model and evaluates the preferred model under different parameter values. Results show evidence in favor of the GEDE model with Planck data and in combination with R19, while the Bayesian model comparison is inconclusive when including Ia supernovae or BAO data.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Implication of the Hubble tension for the primordial Universe in light of recent cosmological data

Gen Ye et al.

Summary: In resolving the Hubble tension, this paper explores how early dark energy and new physics before recombination can alter cosmological parameters to fit observational data from cosmic microwave background and baryon acoustic oscillations. Through analysis, it is found that a complete resolution of the Hubble tension may point towards a scale invariant spectrum.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Modeling and testing the equation of state for (Early) dark energy

Shin'ichi Nojiri et al.

Summary: This study examines the behavior of dark energy using a general equation of state to address the Hubble parameter tension problem. By analyzing the cosmological evolution and dominance of each term in the equation, interesting consequences such as future singularities are revealed. Fits of free parameters in two general models demonstrate their effectiveness compared to standard models, offering promising insights into understanding the overall cosmological evolution.

PHYSICS OF THE DARK UNIVERSE (2021)

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Article Astronomy & Astrophysics

Rapid transition of Geff at zt ≃ 0.01 as a possible solution of the Hubble and growth tensions

Valerio Marra et al.

Summary: The discrepancy in the value of the Hubble constant between low- and high-redshift observations may be explained by a rapid transition in the relative effective gravitational constant around z=0.01, which could account for the differences in the luminosity of Type Ia supernovae. This transition not only resolves the Hubble tension, but also helps ease the growth tension by reducing density perturbations without affecting the background expansion.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Can dark energy be dynamical?

Eoin O. Colgain et al.

Summary: The study demonstrates that parametric models of dynamical dark energy have a degree of arbitrariness, with errors in wa being sensitive to different redshift functions f(z). Additionally, classic DDE models such as the Chevallier-Polarski-Linder model are less sensitive to DDE, while wiggles uncovered in nonparametric reconstructions require a thorough analysis of correlations.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Do the observational data favor a local void?

Rong-Gen Cai et al.

Summary: The current tension on the Hubble constant cannot be explained solely by a local void, as suggested by previous studies.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Touch of neutrinos on the vacuum metamorphosis: Is the H0 solution back?

Eleonora Di Valentino et al.

Summary: This study explores tensions in the measurements of expansion rate and matter clustering in the universe by extending the neutrino sector and considering the curvature of the universe as a model parameter. The inclusion of massive neutrinos and extra relativistic species did not significantly affect the results, with the physically motivated VM model producing consistent values for H-0 and S-8.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Running Hubble tension and a H0 diagnostic

C. Krishnan et al.

Summary: Hubble tension refers to the mismatch between the locally determined Hubble constant H-0 and the value inferred from flat CDM cosmology. This tension arises from cosmological origins and predicts variations in H-0, potentially related to differences between the FLRW cosmology framework and the standard model. An introduced diagnostic can track these variations in H-0.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Trouble beyond H0 and the new cosmic triangles

Jose Luis Bernal et al.

Summary: The article discusses the discrepancy in the values of the Hubble constant H-0 in astronomy, known as the Hubble tension, and explores potential solutions to this issue by extending the standard cosmological model and measuring the age of the Universe. It also points out the need to consider the effects on other quantities when addressing problems beyond the H-0 value within existing cosmological models.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Cobaya: code for Bayesian analysis of hierarchical physical models

Jesus Torrado et al.

Summary: Cobaya is a general-purpose Bayesian analysis code designed for models with complex internal interdependencies. It efficiently exploits interdependencies between different stages of a model pipeline, automatically caches intermediate results, and optimally sorts parameters to minimize computational costs during sampling. The code allows exploration of posteriors using Monte Carlo samplers, functions for maximization and importance-reweighting of samples, and can be extended and parallelized with minimal overhead per posterior evaluation.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Article Astronomy & Astrophysics

w - M phantom transition at zt < 0.1 as a resolution of the Hubble tension

George Alestas et al.

Summary: The text introduces a new theoretical model, Late w-M Phantom Transition (LwMPT), which adjusts the transition of the dark energy equation of state parameter and absolute magnitude to better address tension in cosmological data. This model demonstrates a potential solution to the Hubble constant tension and growth tension by inducing abrupt features in the w-M relationship at low redshifts.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

Early dark energy in k-essence

S. X. Tian et al.

Summary: In an effort to solve the coincidence problem between the energy scale of EDE and matter-radiation equality, a new EDE scenario triggered by radiation-matter transition was proposed. Although k-essence seems unable to realize this new EDE scenario, an EDE model with a different scenario was achieved within the k-essence framework. The study suggests that more research is needed to fully address the coincidence problem in the originally proposed scenario.

PHYSICAL REVIEW D (2021)

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Article Astronomy & Astrophysics

A Luminous Quasar at Redshift 7.642

Feige Wang et al.

Summary: The discovery of the distant quasar J0313-1806 challenges theoretical models of supermassive black hole growth, with a mass similar to 670 million years after the big bang. The complex structure of this quasar suggests the presence of a massive supermassive black hole and a star-forming galaxy, providing insights into the formation and evolution of the earliest massive galaxies.

ASTROPHYSICAL JOURNAL LETTERS (2021)

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Article Astronomy & Astrophysics

Kinematic constraints on spatial curvature from supernovae Ia and cosmic chronometers

J. F. Jesus et al.

Summary: An independent method to estimate the spatial curvature Omega(k) without relying on dynamical models was proposed, using kinematic parametrizations of comoving distance, Hubble parameter, and deceleration parameter as functions of redshift. Analysis of SNe Ia data and H(z) data resulted in specific values for the spatial curvature.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Article Astronomy & Astrophysics

Updating constraints on f(T) teleparallel cosmology and the consistency with big bang nucleosynthesis

Micol Benetti et al.

Summary: Researchers conducted a detailed study on viable f(T) teleparallel cosmological models, including power law, exponential, and square-root exponential, analyzing their evolution at different scales. Through a combination of measurements, they obtained narrow constraints on the free parameters of these models, indicating a preference for extended gravity models in observations.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Article Astronomy & Astrophysics

A massive blow for ACDM - the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology

Elena Asencio et al.

Summary: The research analyzed the formation and properties of the galaxy cluster El Gordo, and determined the probability of finding a similar cluster in a ΛCDM cosmology through simulations of turnaround pairs. The study results indicate that the properties of El Gordo and the fast collision between two individually rare massive clusters are unexpected, potentially revealing new cosmological theories.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Article Astronomy & Astrophysics

Model-independently Calibrating the Luminosity Correlations of Gamma-Ray Bursts Using Deep Learning

Li Tang et al.

Summary: This paper investigates the redshift dependence of six luminosity correlations using a deep-learning method, finding that only the E-p - E-gamma relation shows no evidence for redshift dependence. Calibrating GRBs with this relation provides tight constraints on the flat ΛCDM model, with the best-fitting parameter Omega(M) = 0.307(-0.073)(+0.065).

ASTROPHYSICAL JOURNAL (2021)

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Article Astronomy & Astrophysics

Exploring the evidence for a large local void with supernovae Ia data

Vladimir V. Lukovic et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

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Article Astronomy & Astrophysics

Planck evidence for a closed Universe and a possible crisis for cosmology

Eleonora Di Valentino et al.

NATURE ASTRONOMY (2020)

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Article Astronomy & Astrophysics

Generalized covariant prescriptions for averaging cosmological observables

G. Fanizza et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

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Article Astronomy & Astrophysics

Tsallis holographic dark energy in fractal universe

S. Ghaffari et al.

MODERN PHYSICS LETTERS A (2020)

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Article Astronomy & Astrophysics

General cosmography model with spatial curvature

En-Kun Li et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

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Article Astronomy & Astrophysics

Planck 2018 results: VI. Cosmological parameters

N. Aghanim et al.

ASTRONOMY & ASTROPHYSICS (2020)

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Correction Physics, Multidisciplinary

Cosmological renormalization of model parameters in the second-order perturbation theory (vol 2017, 053E01, 2017)

Kenji Tomita

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS (2020)

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Article Physics, Multidisciplinary

Measuring H0 from low-z datasets

Xue Zhang et al.

SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY (2020)

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Article Astronomy & Astrophysics

Reaffirmation of cosmological oscillations in the scale factor from the Pantheon compilation of 1048 Type Ia supernovae

H. Ringermacher et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

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Article Astronomy & Astrophysics

H0LiCOW-XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3σ tension between early- and late-Universe probes

Kenneth C. Wong et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

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Article Astronomy & Astrophysics

Kinematic constraints beyond z≃0 using calibrated GRB correlations

Orlando Luongo et al.

ASTRONOMY & ASTROPHYSICS (2020)

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Article Astronomy & Astrophysics

Phase transition of cosmological model with statistical techniques

R. K. Mishra et al.

ASTROPHYSICS AND SPACE SCIENCE (2020)

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Article Physics, Particles & Fields

Constraints on Newton's constant from cosmological observations

Ke Wang et al.

EUROPEAN PHYSICAL JOURNAL C (2020)

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Article Astronomy & Astrophysics

Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection

Sandro M. R. Micheletti

INTERNATIONAL JOURNAL OF MODERN PHYSICS D (2020)

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Article Astronomy & Astrophysics

Reconciling H0 tension in a six parameter space?

Supriya Pan et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

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Article Astronomy & Astrophysics

Soundness of dark energy properties

Eleonora Di Valentino et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

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Article Astronomy & Astrophysics

Pantheon update on a model-independent analysis of cosmological supernova data

A. Kazim Camlibel et al.

CLASSICAL AND QUANTUM GRAVITY (2020)

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Article Physics, Particles & Fields

Observational constraints on Barrow holographic dark energy

Fotios K. Anagnostopoulos et al.

EUROPEAN PHYSICAL JOURNAL C (2020)

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Article Astronomy & Astrophysics

The logotropic dark fluid: Observational and thermodynamic constraints

Abdulla Al Mamon et al.

INTERNATIONAL JOURNAL OF MODERN PHYSICS D (2020)

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Article Astronomy & Astrophysics

Inflation wars: a new hope

Ryan E. Keeley et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

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Article Astronomy & Astrophysics

The KBC void and Hubble tension contradict ΛCDM on a Gpc scale - Milgromian dynamics as a possible solution

Moritz Haslbauer et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

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Article Astronomy & Astrophysics

Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample

Chao Gao et al.

RESEARCH IN ASTRONOMY AND ASTROPHYSICS (2020)

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Article Astronomy & Astrophysics

Current constraints on deviations from General Relativity using binning in redshift and scale

Cristhian Garcia-Quintero et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

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Article Astronomy & Astrophysics

H0 ex machina: Vacuum metamorphosis and beyond H0

Eleonora Di Valentino et al.

PHYSICS OF THE DARK UNIVERSE (2020)

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Article Astronomy & Astrophysics

Cosmography and flat ACDM tensions at high redshift

Tao Yang et al.

PHYSICAL REVIEW D (2020)

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Article Astronomy & Astrophysics

Is there an early Universe solution to Hubble tension?

C. Krishnan et al.

PHYSICAL REVIEW D (2020)

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Article Astronomy & Astrophysics

Gravitational-wave Constraints on the Cosmic Opacity at z ∼ 5: Forecast from Space Gravitational-wave Antenna DECIGO

Shuaibo Geng et al.

ASTROPHYSICAL JOURNAL (2020)

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