Hubble Hullabaloo and String Cosmology
arXiv:2005.01217
Abstract
The discrepancy in measurements of the Hubble constant indicates new physics in dark energy, dark matter, or both. Drawing inspiration from string theory, we explore possible solutions to overcome the problem. We investigate the interplay between the cosmological determination of and searches at the LHC Run3.
Based on a talk given at the Phenomenology 2020 Symposium, University of Pittsburgh, 4-6 May 2020
References in corpus (9)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
- Equation of state and QCD transition at finite temperature
- The effects of He I 10830 on helium abundance determinations
- Indications of a late-time interaction in the dark sector
- Swampland Conjectures and Late-Time Cosmology
- Constraining Fundamental Physics with Future CMB Experiments
- The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. III. NGC 4038/39 and NGC 5584
- Hot thermal universe endowed with massive dark vector fields and the Hubble tension