Questioning the tension via the look-back time
arXiv:2302.13671 · doi:10.1016/j.dark.2023.101201
Abstract
The Hubble tension is investigated taking into account the cosmological look-back time. Specifically, considering a single equation, widely used in standard cosmology, it is possible to recover both values of the Hubble constant reported by the SH0ES and Planck collaborations: the former is obtained through cosmological ladder methods (e.g. Cepheids, Supernovae Type IA) and the latter through measurements of the Cosmic Microwave Background. Also, other values obtained in the literature are achieved with the same approach. We conclude that the Hubble tension can be removed if the look-back time is correctly referred to the redshift where the measurement is performed.
8 pages, 1 figure, accepted for publication in Physics of the Dark Universe
References in corpus (28)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Beyond the Cosmological Standard Model
- The trouble with
- Extended Gravity Cosmography
- Hydrostatic equilibrium and stellar structure in f(R)-gravity
- 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
- Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated - correlation
- The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
- A combined analysis of the late time direct measurements and the impact on the Dark Energy sector
- A measurement of the Hubble constant from Type II supernovae
- Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations
- Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
- Dark sector interaction and the supernova absolute magnitude tension
- Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
- The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
- Tests and problems of the standard model in Cosmology
- The local and distant Universe: stellar ages and
- Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
- Addressing the cosmological tension by the Heisenberg uncertainty
- Early and late time cosmology: the gravity perspective
- Cosmology and the massive photon frequency shift in the Standard-Model Extension
- The Heisenberg limit at cosmological scales
- Effects of a Pre-inflationary de Sitter Bounce on the Primordial Gravitational Waves in Gravity Theories
- Investigating dark energy by electromagnetic frequency shifts
- Cosmic voids and the kinetic analysis
Cited by in corpus (5)
- Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
- Is Dark Energy Dynamical in the DESI Era? A Critical Review
- A critical discussion on the tension
- Investigating the cosmic distance duality relation with gamma-ray bursts
- A Unified Interpretation of Supernova, GRB, and QSO Time Dilation Signals in a Generalized Cosmological Time Framework