activity
20042024
most citedCompatibility of the chameleon-field model with fifth-force experiments, cosmology, and PVLAS and CAST results

147 citations · 424 across the 12 of their papers we have counts for

collaborators

13 papers

hep-th2024★ 5 cited

Inflation in non-local hybrid metric-Palatini gravity

Flavio Bombacigno, Mariaveronica De Angelis, Carsten van de Bruck +1

Within the framework of hybrid metric-Palatini gravity, we incorporate non-localities introduced via the inverse of the d'Alembert operators acting on the scalar curvature. We anal…

hep-th2024

CMB Implications of Multi-field Axio-dilaton Cosmology

Adam Smith, Maria Mylova, Philippe Brax +3

Axio-dilaton models are among the simplest scalar-tensor theories that contain the two-derivative interactions that naturally compete at low energies with the two-derivative inter-…

gr-qc2021★ 8 cited

Inflation and Scale-invariant -Gravity

Carsten van de Bruck, Richard Daniel

In scale-invariant models of fundamental physics, mass scales are generated by spontaneous symmetry breaking. In this work, we study inflation in scale-invariant gravity, in…

gr-qc2020★ 17 cited

Dark D-Brane Cosmology: from background evolution to cosmological perturbations

Carsten van de Bruck, Elsa M. Teixeira

We study the cosmological predictions of the dark D-brane model, in which dark matter resides on a D-brane moving in a higher-dimensional space. By construction, dark matter intera…

hep-ph2020★ 13 cited

Dark matter relic density from conformally or disformally coupled light scalars

Sebastian Trojanowski, Philippe Brax, Carsten van de Bruck

Thermal freeze-out is a prominent example of dark matter (DM) production mechanism in the early Universe that can yield the correct relic density of stable weakly interacting massi…

hep-th2019★ 39 cited

Dark Energy, the Swampland and the Equivalence Principle

Carsten van de Bruck, Cameron C. Thomas

It has recently been argued that string theory does not admit de Sitter vacua. This would imply that the current accelerated expansion of the universe is not driven by a cosmologic…