Electron mass variation from dark sector interactions and compatibility with cosmological observations

Abstract

We investigate the model where electrons and dark matter interact with dark energy through the rolling of a scalar field which comes from extra dimensional theories such as the braneworld theory and Brans-Dicke theory. In this model, dark energy couples to dark matter and electrons, which leads to larger values of the mass energies of dark matter and electrons in the early universe. We also fit our model to the cosmological data. By analyzing the data from Planck, baryon acoustic oscillation (BAO), light curves (Pantheon), and type-Ia supernovae (SH0ES), it can be seen that the Hubble tension is relieved in our model and the coupling parameter prefers a non-zero value with a significance of over 2σ.

arXiv comment18 pages, 7 figures, version published in Phys. Rev. D

References in corpus (64)

• A Large Mass Hierarchy from a Small Extra Dimension
• Efficient Computation of CMB anisotropies in closed FRW models
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
• Brane-World Gravity
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• Planck 2018 results. VIII. Gravitational lensing
• The Universe as a Domain Wall
• The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
• One percent determination of the primordial deuterium abundance
• The $H_0$ Olympics: A fair ranking of proposed models
• Non-minimal dark sector physics and cosmological tensions
• Structure Formation with Generalized Dark Matter
• Calibration of the Tip of the Red Giant Branch (TRGB)
• Precision big bang nucleosynthesis with improved Helium-4 predictions
• Large-scale instability in interacting dark energy and dark matter fluids
• KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Precision measures of the primordial abundance of deuterium
• H0 Revisited
• Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
• Large Scale Cosmic Microwave Background Anisotropies and Dark Energy
• Coupled dark energy: Towards a general description of the dynamics
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• Testing the Interaction between Dark Energy and Dark Matter with Planck Data
• Constraints on dark matter interactions with standard model particles from CMB spectral distortions
• Testing the interaction between dark energy and dark matter via latest observations
• Early recombination as a solution to the $H_0$ tension
• Velocities as a probe of dark sector interactions
• A new tension in the cosmological model from primordial deuterium?
• Cosmological constraints on a decomposed Chaplygin gas
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Evidence for interacting dark energy from BOSS
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• New constraints on time-dependent variations of fundamental constants using Planck data
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• Inhomogeneous vacuum energy
• Direct detection of dark energy: the XENON1T excess and future prospects
• Scattering of Dark Matter and Dark Energy
• H0 tension or T0 tension?
• Cosmological Evolution of Brane World Moduli
• Probing elastic interactions in the dark sector and the role of $S_8$
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Is there really a Hubble tension?
• Testing interacting dark matter and dark energy model with cosmological data
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• CMB Anisotropies in the Presence of Extra Dimensions
• Axi-Higgs Cosmology
• On cosmological signatures of baryons-dark energy elastic couplings
• Brane World of Warp Geometry: An Introductory Review
• Field Theories and Fluids for an Interacting Dark Sector
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• FLRW accelerating universe with interactive dark energy
• Environment Dependent Electron Mass and the H${}_0$-Tension
• Addressing the High-$f$ Problem in Pseudo-Nambu-Goldstone Boson Dark Energy Models with Dark Matter - Dark Energy Interaction
• Brane World Cosmology, the CMB and the Radion
• Non linear equation of state and effective phantom divide in brane models

Cited by in corpus (10)

• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Solar chameleons: Novel channels
• Variation of the fine structure constant in the light of recent helium abundance measurement
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• On the Stability of Dark Energy Scalar Field Reconstruction from SNe Ia Data