activity
20242026
collaborators

10 papers

astro-ph.CO2026

Evolving Dark Energy Is Vacuum Energy After All

Dong Ha Lee, Carsten van de Bruck, Eleonora Di Valentino +2

We investigate a physically motivated model of dynamical dark energy arising from the non-perturbative topological structure of the Quantum Chromodynamics (QCD) vacuum. The model i…

astro-ph.CO2026

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies

Yuejia Zhai, Carsten van de Bruck, Eleonora Di Valentino +2

Following our previous work constraining interacting dark energy (IDE) models, which showed their potential to alleviate the Hubble tension, in this work we investigate the non-lin…

astro-ph.CO2026

Shape of Dark Energy: Constraining Its Evolution with a General Parametrization

Dong Ha Lee, Weiqiang Yang, Eleonora Di Valentino +2

We consider a general dark energy (DE) model parametrized by its equation-of-state (EoS), featuring three free parameters: (the present-day value of the DE EoS), (quan…

hep-ph2026

Can QCD Axions Survive the Cosmological Constant Problem?

Carsten van de Bruck, C. P. Burgess, Adam Smith

Mechanisms that dynamically relax the vacuum energy offer a concrete way to approach the cosmological constant problem, but because relaxation is not confined to the vacuum energy…

gr-qc2026

Multi-Field Dilaton Screening Beyond the Thin-Shell Mechanism

Philippe Brax, Carsten van de Bruck, Anne-Christine Davis +1

We analyse screening in multi-field scalar-tensor theories, focusing on systems with a dilaton coupled to matter and an axion with a dilaton-dependent kinetic term, in the presence…

astro-ph.CO2025

The Serendipitous Axiodilaton: A Self-Consistent Recombination-Era Solution to the Hubble Tension

Adam Smith, Maria Mylova, Carsten van de Bruck +2

Axio-dilaton cosmology provides a minimal benchmark model for both Dark Matter (DM) and Dark Energy (DE) that is well motivated by fundamental physics. The axion and dilaton arise…