4.4 Article

Stepped partially acoustic dark matter, large scale structure, and the Hubble tension

相关参考文献

注意:仅列出部分参考文献,下载原文获取全部文献信息。
Article Astronomy & Astrophysics

Thermal friction as a solution to the Hubble and large-scale structure tensions

Kim Berghaus et al.

Summary: Thermal friction can solve the Hubble and the large-scale structure tensions by converting scalar field energy into dark radiation. The addition of extra radiation to the Universe can also mitigate the LSS tension. However, the CMB data is incompatible with linear density perturbations of the dark radiation when injected at redshifts close to matter-radiation equality.

PHYSICAL REVIEW D (2023)

Article Physics, Multidisciplinary

Did the Universe experience a pressure non-crushing type cosmological singularity in the recent past?

S. D. Odintsov et al.

Summary: Recent literature suggests that the H-0 tension could be resolved if there was an abrupt physics transition that altered the Cepheid parameters in the recent past of the Universe (approximately 70-150 million years ago). This study explores the possibility that this transition was caused by the smooth passage of the Universe through a pressure finite-time cosmological singularity. The authors discuss how this scenario can be realized using F(R) gravity, without the need for a scalar field or specific matter fluids, and highlight the potential effects of the pressure singularity on the gravitational constant and trajectories of bound objects in the Universe.
Article Astronomy & Astrophysics

Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing

Martin White et al.

Summary: Using luminous red galaxies selected from imaging surveys for targeting by the Dark Energy Spectroscopic Instrument (DESI) in combination with CMB lensing maps from the Planck collaboration, researchers probed the amplitude of large-scale structure over 0.4 <= z <= 1. Their findings suggest a slower growth of structure at low redshift than model predictions, with only modest significance.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2022)

Review Physics, Multidisciplinary

Cosmological constraints on dark matter interactions with ordinary matter

Manuel A. Buen-Abad et al.

Summary: This article investigates the effects of dark matter interactions with electrons or protons on the cosmic microwave background and the matter power spectrum, and utilizes diverse data to study these interactions. The study finds that these interactions result in momentum and heat exchange between ordinary and dark matter, and provides constraints on dark matter models. These constraints are crucial for understanding the interactions between dark matter and ordinary matter.

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS (2022)

Article Physics, Particles & Fields

Mirror twin Higgs cosmology: constraints and a possible resolution to the H0 and S8 tensions

Saurabh Bansal et al.

JOURNAL OF HIGH ENERGY PHYSICS (2022)

Article Astronomy & Astrophysics

A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s-1 Mpc-1 Uncertainty from the Hubble Space Telescope and the SH0ES Team

Adam G. Riess et al.

Summary: This study reports observations of Cepheid variables in the host galaxies of 42 Type Ia supernovae (SNe Ia) using the Hubble Space Telescope (HST) to calibrate the Hubble constant (H (0)). The observations were collected over four decades and significantly improved the precision of the direct determination of H (0). The study presented multiple verifications of Cepheid photometry and explored different analysis variants to assess the sensitivity of H (0) determination. The baseline result for H (0) was found to be 73.04 +/- 1.04 km s(-1) Mpc(-1).

ASTROPHYSICAL JOURNAL LETTERS (2022)

Review Physics, Multidisciplinary

The H0 Olympics: A fair ranking of proposed models

Nils Schoeneberg et al.

Summary: This article systematically compares seventeen different models proposed to resolve the H0 tension and quantifies their relative success. The goal is to identify which proposed solutions and underlying mechanisms are most likely to explain the observed discrepancy.

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS (2022)

Article Astronomy & Astrophysics

A Step in understanding the Hubble tension

Daniel Aloni et al.

Summary: As cosmological data have improved, tensions have arisen, particularly regarding the difference between the locally measured Hubble constant H0 and the value inferred from the cosmic microwave background. Interacting radiation has been suggested as a solution, but conventional models are precluded by high polarization CMB data. It is possible that related models that distinguish between high- and low-multipole interactions may provide a solution.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Hot new early dark energy

Florian Niedermann et al.

Summary: New Early Dark Energy (NEDE) can explain the consistency between the cosmic microwave background and the higher value of the Hubble constant inferred from supernova observations. It is a better alternative to the old EDE model as it naturally explains the decay of the extra energy component through a vacuum first-order phase transition triggered by a subdominant scalar field at zero temperature. With hot NEDE, a new mechanism to trigger the phase transition is introduced, relying on thermal corrections that subside with cooling in a dark gauge sector. The phenomenology of hot NEDE is explored, and the supercooled regime is identified as the favored scenario. Different microscopic embeddings of hot NEDE, including the (non-)Abelian dark matter model, are proposed, which can potentially resolve the LSS tension through interactions with the dark radiation fluid. The coincidence problem present in EDE models is addressed by relating NEDE to the mass generation of neutrinos via the inverse seesaw mechanism. Finally, a more complete dark sector model is proposed, embedding the NEDE field in a larger symmetry group and discussing the central role of the hot NEDE field in spontaneously breaking lepton number symmetry.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

Catherine Heymans et al.

Summary: This study combines weak gravitational lensing observations from KiDS-1000, redshift-space galaxy clustering observations from BOSS, and galaxy-galaxy lensing observations from overlapping surveys to constrain the structure growth parameter S-8, resulting in a discrepancy with the Planck observations by 8.3% relative to Planck. The systematic uncertainties identified through various analyses are incorporated into the cosmological analysis, revealing a tension in the matter fluctuation amplitude parameter, sigma(8).

ASTRONOMY & ASTROPHYSICS (2021)

Article Astronomy & Astrophysics

A new measurement of the Hubble constant using Type la supernovae calibrated with surface brightness fluctuations

Nandita Khetan et al.

Summary: A new calibration method for the peak absolute magnitude of SNe Ia based on the SBF method was proposed, with a sample of 96 SNe Ia calibrated and the value of the Hubble constant estimated. Results showed that SNe Ia distance moduli calibrated with SBF are on average larger by 0.07 mag than those calibrated with Cepheids, indicating possible differences among SNe in different types of galaxies.

ASTRONOMY & ASTROPHYSICS (2021)

Article Astronomy & Astrophysics

On the Hubble Constant Tension in the SNe Ia Pantheon Sample

M. G. Dainotti et al.

Summary: By analyzing the tension between Type Ia supernovae and Planck measurements regarding the Hubble constant, it was found that the Hubble constant evolves with redshift, showing a slowly decreasing trend. This trend may be attributed to astrophysical selection effects or modified gravity.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Updated constraints on massive neutrino self-interactions from cosmology in light of the H0 tension

Shouvik Roy Choudhury et al.

Summary: The study has updated constraints on flavour universal neutrino self-interactions mediated by a heavy scalar and confirmed the presence of a region with strong self-interactions in parameter space. However, the latest data, particularly high-l polarisation data from the Planck 2018 release, does not support this solution.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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)

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)

Article Astronomy & Astrophysics

Linear cosmological constraints on two-body decaying dark matter scenarios and the S8 tension

Guillermo F. Abellan et al.

Summary: The S-8 tension refers to the discrepancy between the cosmic microwave background (CMB) and weak gravitational lensing determination of matter fluctuations amplitude. A model involving dark matter decay has been proposed to ease this tension, with potential implications for anomalous electron recoil excess reported by the Xenon1T Collaboration. Current CMB data alone may not distinguish between standard cold dark matter and decaying dark matter, but future CMB observations can detect the signature of decaying dark matter.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

The Hubble tension in light of the Full-Shape analysis of Large-Scale Structure data

Guido D'Amico et al.

Summary: The disagreement between direct late-time measurements of the Hubble constant and early-universe measurements may be explained by new physics, but currently two models for early universe physics do not significantly alleviate the tension in cosmological parameters.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

Article Astronomy & Astrophysics

Self-interacting neutrinos, the Hubble parameter tension, and the cosmic microwave background

Thejs Brinckmann et al.

Summary: The study comprehensively explores cosmological constraints on nonstandard neutrino self-interactions, revealing no compelling evidence for new neutrino interactions or nonstandard values of N-eff. In some cases, additional modes with neutrino decoupling occurring at lower redshifts were found. The effectiveness of solving the H-0 tension is not as strong as allowing a variable N-eff comprised of free-streaming particles.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Early dark energy is not excluded by current large-scale structure data

Tristan L. Smith et al.

Summary: Recent studies have found that there are stringent constraints on the maximum abundance of early dark energy in the Universe, but this may be due to the choice of priors rather than actual disagreements between the data and the model. The EDE model still provides a potential resolution to the Hubble tension, and further research is needed to test its predictions with future datasets.

PHYSICAL REVIEW D (2021)

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)

Article Astronomy & Astrophysics

Cosmological constraints on late-Universe decaying dark matter as a solution to the H0 tension

Steven J. Clark et al.

Summary: Recent research suggests that late-Universe dark matter decays could help alleviate the tension between H-0 measurements in the local Universe and its value inferred from cosmic microwave background fluctuations. However, the low multipole amplitude of the cosmic microwave background anisotropy power spectrum severely constrains the feasibility of this solution to the H-0 tension.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with ?CDM

Adam G. Riess et al.

Summary: This study recalibrated the extragalactic distance ladder and refined the determination of the Hubble constant using Hubble Space Telescope and Gaia EDR3 data. The results, based on Milky Way Cepheids observations and estimates, are in good agreement with conclusions based on earlier Gaia data releases.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

The Parallax of omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant

John Soltis et al.

Summary: The study utilized data from the ESA Gaia mission to measure the trigonometric parallax of omega Cen, the most massive globular cluster in the Milky Way, resulting in a precise distance measurement. The calibrated luminosity of the red giant branch tip from the parallax data allowed for a precise estimation of the Hubble constant.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Physics, Particles & Fields

A CMB search for the neutrino mass mechanism and its relation to the Hubble tension

Miguel Escudero et al.

EUROPEAN PHYSICAL JOURNAL C (2020)

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)

Article Astronomy & Astrophysics

Interacting radiation after Planck and its implications for the Hubble tension

Nikita Blinov et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

Article Astronomy & Astrophysics

Cannibalism hinders growth: Cannibal Dark Matter and the S8 tension

Stefan Heimersheim et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

Article Astronomy & Astrophysics

Neutrino puzzle: Anomalies, interactions, and cosmological tensions

Christina D. Kreisch et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

The Megamaser Cosmology Project. XIII. Combined Hubble Constant Constraints

D. W. Pesce et al.

ASTROPHYSICAL JOURNAL LETTERS (2020)

Article Astronomy & Astrophysics

Using the Baryonic Tully-Fisher Relation to MeasureHo

James Schombert et al.

ASTRONOMICAL JOURNAL (2020)

Article Astronomy & Astrophysics

Thermal friction as a solution to the Hubble tension

Kim Berghaus et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

Oscillating scalar fields and the Hubble tension: A resolution with novel signatures

Tristan L. Smith et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

Hubble constant hunter's guide

L. Knox et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

Chiaki Hikage et al.

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN (2019)

Article Astronomy & Astrophysics

MontePython 3: Boosted MCMC sampler and other features

Thejs Brinckmann et al.

PHYSICS OF THE DARK UNIVERSE (2019)

Article Physics, Multidisciplinary

Early Dark Energy can Resolve the Hubble Tension

Vivian Poulin et al.

PHYSICAL REVIEW LETTERS (2019)

Article Astronomy & Astrophysics

Baryon acoustic oscillations from the cross-correlation of Lyα absorption and quasars in eBOSS DR14

Michael Blomqvist et al.

ASTRONOMY & ASTROPHYSICS (2019)

Editorial Material Astronomy & Astrophysics

Tensions between the early and late Universe

Licia Verde et al.

NATURE ASTRONOMY (2019)

Article Astronomy & Astrophysics

The BAO plus BBN take on the Hubble tension

Nils Schoeneberg et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2019)

Article Astronomy & Astrophysics

Baryon Acoustic Oscillations and the Hubble constant: past, present and future

Andrei Cuceu et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2019)

Article Astronomy & Astrophysics

Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman-α

Maria Archidiacono et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2019)

Article Astronomy & Astrophysics

Making dark matter out of light: Freeze-in from plasma effects

Cora Dvorkin et al.

PHYSICAL REVIEW D (2019)

Article Astronomy & Astrophysics

Addressing astrophysical and cosmological problems with secretly asymmetric dark matter

Christopher Dessert et al.

PHYSICAL REVIEW D (2019)

Article Astronomy & Astrophysics

Interacting dark sector and precision cosmology

Manuel A. Buen-Abad et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2018)

Article Astronomy & Astrophysics

Elucidating.CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy

G. E. Addison et al.

ASTROPHYSICAL JOURNAL (2018)

Article Astronomy & Astrophysics

CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics

Shahab Joudaki et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2017)

Article Astronomy & Astrophysics

Cosmological constraints on interacting light particles

Christopher Brust et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2017)

Article Astronomy & Astrophysics

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Shadab Alam et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2017)

Editorial Material Astronomy & Astrophysics

DARK UNIVERSE Crack in the cosmological paradigm

Eleonora Di Valentino

NATURE ASTRONOMY (2017)

Article Astronomy & Astrophysics

Dynamical dark energy in light of the latest observations

Gong-Bo Zhao et al.

NATURE ASTRONOMY (2017)

Article Astronomy & Astrophysics

Phases of new physics in the CMB

Daniel Baumann et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2016)

Article Astronomy & Astrophysics

Evidence for dark matter interactions in cosmological precision data?

Julien Lesgourgues et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2016)

Article Astronomy & Astrophysics

A fresh look at linear cosmological constraints on a decaying Dark Matter component

Vivian Poulin et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2016)

Article Astronomy & Astrophysics

Constraints on the coupling between dark energy and dark matter from CMB data

R. Murgia et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2016)

Article Astronomy & Astrophysics

The trouble with H0

Jose Luis Bernal et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2016)

Article Physics, Particles & Fields

Partially acoustic dark matter, interacting dark radiation, and large scale structure

Zackaria Chacko et al.

JOURNAL OF HIGH ENERGY PHYSICS (2016)

Article Astronomy & Astrophysics

Dark energy at early times, the Hubble parameter, and the string axiverse

Tanvi Karwal et al.

PHYSICAL REVIEW D (2016)

Article Astronomy & Astrophysics

Decaying dark matter and the tension in σ8

Kari Enqvist et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2015)

Article Astronomy & Astrophysics

The clustering of the SDSS DR7 main Galaxy sample - I. A 4 per cent distance measure at z=0.15

Ashley J. Ross et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2015)

Article Astronomy & Astrophysics

Tension between the power spectrum of density perturbations measured on large and small scales

Richard A. Battye et al.

PHYSICAL REVIEW D (2015)

Article Astronomy & Astrophysics

Cosmological implications of baryon acoustic oscillation measurements

Eric Aubourg et al.

PHYSICAL REVIEW D (2015)

Article Astronomy & Astrophysics

Constraining dark matter-baryon scattering with linear cosmology

Cora Dvorkin et al.

PHYSICAL REVIEW D (2014)

Article Astronomy & Astrophysics

Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure

G. E. Addison et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2013)

Article Astronomy & Astrophysics

The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes

Diego Blas et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2011)

Article Astronomy & Astrophysics

The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant

Florian Beutler et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)

Article Astronomy & Astrophysics

Turning off the lights: How dark is dark matter?

Samuel D. McDermott et al.

PHYSICAL REVIEW D (2011)

Article Astronomy & Astrophysics

Thermal relic abundances of particles with velocity-dependent interactions

James B. Dent et al.

PHYSICS LETTERS B (2010)

Article Astronomy & Astrophysics

A theory of dark matter

Nima Arkani-Hamed et al.

PHYSICAL REVIEW D (2009)

Review Physics, Multidisciplinary

The cosmological constant and dark energy

PJE Peebles et al.

REVIEWS OF MODERN PHYSICS (2003)