Combining pre- and post-recombination new physics to address cosmological tensions: Case study with varying electron mass and sign-switching cosmological constant
Year: 2024
Type: article
Abstract: It has recently been argued that the Hubble tension may call for a combination of both pre- and post-recombination new physics . Motivated by these considerations, we provide one of the first concrete case studies aimed at constructing such a viable combination. We consider models that have individually worked best on either end of recombination so far: a spatially uniform time-varying electron mass leading to earlier recombination (also adding non-zero spatial curvature), and a sign-switching cosmological constant inducing an AdS-to-dS transition within the Λ s CDM model. When confronted against Cosmic Microwave Background (CMB), Baryon Acoustic Oscillations , and Type Ia Supernovae data, we show that no combination of these ingredients can successfully solve the Hubble tension. We find that the matter density parameter Ω m plays a critical role, driving important physical scales in opposite directions: the AdS-to-dS transition requires a larger Ω m to maintain the CMB acoustic scale fixed, whereas the varying electron mass requires a smaller Ω m to maintain the redshift of matter-radiation equality fixed. Despite the overall failure, we use our results to draw general model-building lessons, highlighting the importance of assessing tension-solving directions in the parameter space of new physics parameters and how these correlate with shifts in other standard parameters, while underscoring the crucial role of Ω m in this sense.
Source: Physics of the Dark Universe
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Estimated APC paid: $3,240
Funders: Royal Society, European Cooperation in Science and Technology, Università degli Studi di Trento, Türkiye Bilimsel ve Teknolojik Araştırma Kurumu, Provincia Autonoma di Trento, Istituto Nazionale di Fisica Nucleare, Science and Technology Facilities Council, Japan Science and Technology Agency
OpenAlex ID: W4402905547
