Dynamical dark energy can amplify the expansion rate of the Universe
arXiv:2305.16586 · doi:10.1103/PhysRevD.107.103529
Abstract
By adding a matter-coupled dark energy field to Einstein's General Relativity (GR), this paper proves that the dynamical dark energy field can change the frequency of photons from distant galaxies as well as from background radiation of remote Universe. Therefore, when the observed frequency-shift of the photons is entirely attributed to the temporal variation of the cosmic scale factor, the calculated expansion rate of the Universe will be slightly greater than its actual value. The predicted values of the temperature of the cosmic blackbody radiation in the past (future) of the Universe are slightly larger (gradually smaller and smaller) than those in the standard cosmology. Since the blackbody radiation becomes the present cosmic microwave background (CMB) and its present-day temperature is directly estimated according to the Planck's law of blackbody radiation, the measured value of the CMB temperature is independent of whether to consider the scalar field or not.
arXiv comment15 pages,4 figures
References in corpus (46)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Cosmological Imprint of an Energy Component with General Equation of State
- Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- The galileon as a local modification of gravity
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Beyond the Cosmological Standard Model
- Tensions between the Early and the Late Universe
- Quintessence and the Rest of the World
- Early Dark Energy Can Resolve The Hubble Tension
- Tests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale
- A Cyclic Model of the Universe
- Planck evidence for a closed Universe and a possible crisis for cosmology
- Measurements of the Hubble Constant: Tensions in Perspective
- Are f(R) dark energy models cosmologically viable ?
- The Relation between Physical and Gravitational Geometry
- Calibration of the Tip of the Red Giant Branch (TRGB)
- TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
- Environmental Dependence of Masses and Coupling Constants
- The conformal frame freedom in theories of gravitation
- Dynamical Lambda Models of Structure Formation
- The Dilaton and Modified Gravity
- A Unified Description of Screened Modified Gravity
- Late universe decaying dark matter can relieve the H_0 tension
- The microwave background temperature at the redshift of 2.33771
- An 8\% Determination of the Hubble Constant from localized Fast Radio Bursts
- Disformal couplings and the dark sector of the universe
- A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light -ray attenuation
- Molecular Hydrogen in the Damped Ly alpha Absorber of Q1331+170
- Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
- The cosmic microwave background radiation temperature at z = 3.025 toward QSO 0347--3819
- Measurement of the evolution from the Sunyaev-Zel'dovich effect
- Constraints on the CMB Temperature Evolution using Multi-Band Measurements of the Sunyaev Zel'dovich Effect with the South Pole Telescope
- Microwave Background Temperature at a Redshift of 6.34 from H2O Absorption
- Quantum Stability of Chameleon Field Theories
- A Bayesian interpretation of inconsistency measures in cosmology
- Dark Energy coupling with electromagnetism as seen from future low-medium redshift probes
- Peculiar velocities in the local Universe: comparison of different models and the implications for and dark matter
- Cosmology and the massive photon frequency shift in the Standard-Model Extension
- Note on Tsallis holographic dark energy in Brans-Dicke cosmology
- Estimation of the CMB temperature from atomic C\,{\sc i} and molecular CO lines in the interstellar medium of early galaxies
- Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
- Quasi-geodesics in relativistic gravity
- Obtaining a scalar fifth force via a broken-symmetry couple between the scalar field and matter
- Could trapped quintessence account for the laser-detuning-dependent acceleration of cold atoms in varying-frequency time-of-flight experiments?
- The Higgs Field and the Jordan Brans Dicke Cosmology