Gravitational particle production and the Hubble tension
arXiv:2402.16791 · doi:10.3390/universe10090338
Abstract
The effect of gravitational particle production of scalar particles on the total effective cosmic energy density (in the era after photon decoupling till the present) is considered. The effect is significant for heavy particles. It is found that gravitational particle production results in an effective increase in the directly measured value of the Hubble constant while it does not affect the value of the Hubble constant in the calculation of the number density of baryons at present time that is used to calculate recombination redshift. This may explain why the Hubble constant determined by local measurements and non-local measurements (such as CMB) are different. This suggests that gravitational particle production may have a non-negligible impact on the tension.
arXiv commentPresentation is improved, some points are discussed in more detail, new references are added
References in corpus (28)
- 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
- In the Realm of the Hubble tension a Review of Solutions
- Small Scale Cosmological Perturbations: An Analytic Approach
- The Olympics: A fair ranking of proposed models
- On the Hubble constant tension in the SNe Ia Pantheon sample
- Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra
- Elucidating CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
- 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
- On the gravitational production of superheavy dark matter
- Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
- A rapid transition of at as a solution of the Hubble and growth tensions
- Gravitational production of vector dark matter
- Cosmological Particle Production: A Review
- Field theoretic interpretations of interacting dark energy scenarios and recent observations
- Gravitational Fermion Production in Inflationary Cosmology
- gravity in the Jordan Frame as a Paradigm for the Hubble Tension
- Metric gravity with dynamical dark energy as a scenario for the Hubble tension
- Slow-rolling scalar dynamics and as solution for the Hubble tension
- Superheavy Particles in Friedmann Cosmology and the Dark Matter Problem
- A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
- Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample
- Modified gravity in the presence of matter creation: scenario for the late Universe
- Searching for Heavy Dark Matter near the Planck Mass with XENON1T
- Particle creation in the early Universe: achievements and problems
- Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
- Is it possible to obtain cosmic accelerated expansion through energy transfer between different energy densities?
- A mechanism for formation of Bose-Einstein condensation in cosmology
- Interaction rates in cosmology: heavy particle production and scattering
Cited by in corpus (6)
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Modified gravity in the presence of matter creation: scenario for the late Universe
- Effects of a local physics change on the SH0ES determination of
- One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
- Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced Tension with Reconstructed Scalar-Tensor Gravity
- Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension