Special Issue on Modified Gravity Approaches to the Tensions of CDM: Goals and Highlights
arXiv:2404.13981 · doi:10.3390/universe10040184
Abstract
The Special Issue on "Modified Gravity Approaches to the Tensions of CDM"} in the Universe journal tackles significant challenges faced by the CDM model, including discrepancies in the Hubble constant, growth rate of structures, and cosmological anisotropies. These issues suggest foundational cracks in the model, raising questions about the validity of General Relativity, dark energy, and cosmological principles at large scales. This collection brings together leading researchers to delve into Modified Gravity theories as potential solutions. Covering approaches from Scalar-Tensor theories to gravity and beyond, each contribution presents innovative research aimed at addressing the limitations of the CDM model. This Special Issue not only highlights the theoretical and empirical strengths of Modified Gravity models but also opens avenues for future investigations, emphasizing the synergy between theoretical advancements and observational evidence to deepen our cosmological understanding.
6 pages no figures Published in Universe in the Special Issue "Modified Gravity Approaches to the Tensions of CDM" ( https://www.mdpi.com/journal/universe/special_issues/Gravit )
References in corpus (40)
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- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
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- Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
- Horndeski theory and beyond: a review
- Cosmology Intertwined II: The Hubble Constant Tension
- Teleparallel Gravity: From Theory to Cosmology
- Cosmology Intertwined III: and
- On the Hubble constant tension in the SNe Ia Pantheon sample
- Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
- The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth
- A Test of the Cosmological Principle with Quasars
- Is the Observable Universe Consistent with the Cosmological Principle?
- Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
- Time drift of cosmological redshifts as a test of the Copernican principle
- DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
- Early modified gravity in light of the tension and LSS data
- A rapid transition of at as a solution of the Hubble and growth tensions
- KiDS-1000 Cosmology: constraints beyond flat CDM
- Implications for the Hubble tension from the ages of the oldest astrophysical objects
- Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model
- Analyzing the tension in gravity models
- Can late-time extensions solve the and tensions?
- Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
- Testing the Cosmological Principle with CatWISE Quasars: A Bayesian Analysis of the Number-Count Dipole
- CDM Tensions: Localising Missing Physics through Consistency Checks
- Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
- Proca in the sky
- Dipole Cosmology: The Copernican Paradigm Beyond FLRW
- An exploration of an early gravity transition in light of cosmological tensions
- Probing Early Modification of Gravity with Planck, ACT and SPT
- Dynamical systems analysis of gravity
- Alleviating tension in scalar-tensor and bi-scalar-tensor theories
- Testing the isotropy of cosmic acceleration with Pantheon+ and SH0ES: A cosmographic analysis
- Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
- Addressing Cosmological Tensions by Non-Local Gravity
- Tension on the Light of Supermassive Black Hole Shadows Data
- DE models with combined from BAO and CMB dataset and friends
- The Effective Fluid approach for Modified Gravity and its applications