activity
19952026
most citedCosmology and Brane Worlds: A Review

345 citations · 2.7k across the 66 of their papers we have counts for

collaborators

67 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…

hep-th2025

A no-go theorem in bumblebee vector-tensor cosmology

Carsten van de Bruck, Mohammad Ali Gorji, Nils A. Nilsson +2

Bumblebee models, a class of vector-tensor theories in which a vector field acquires a nonzero vacuum expectation value that spontaneously breaks spacetime symmetries, are ubiquito…

astro-ph.CO2024★ 4 cited

Model-Independent Test of Prerecombination New Physics: Measuring the Sound Horizon with Gravitational Wave Standard Sirens and the Baryon Acoustic Oscillation Angular Scale

William Giarè, Jonathan Betts, Carsten van de Bruck +1

In a broad class of cosmological models where spacetime is described by a pseudo-Riemannian manifold, photons propagate along null geodesics, and their number is conserved, upcomin…

gr-qc2024

Bouncing cosmologies in the presence of a Dirac-Born-Infeld field

Mariam Campbell, Richard Daniel, Peter K. S. Dunsby +1

We perform a detailed dynamical system analysis for the behaviour of a Dirac-Born-Infeld (DBI) field in a spatially closed Friedmann-Lemaître-Robertson-Walker (FLRW) cosmology. The…

astro-ph.CO2024★ 3 cited

Scalar field dark matter with time-varying equation of state

Gaspard Poulot, Elsa M. Teixeira, Carsten van de Bruck +1

We propose a new model of scalar field dark matter interacting with dark energy. Adopting a fluid description of the dark matter field in the regime of rapid oscillations, we find…

astro-ph.CO2024★ 45 cited

Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state

William Giarè, Yuejia Zhai, Supriya Pan +3

We present a comprehensive reassessment of the state of Interacting Dark Energy (IDE) cosmology, namely models featuring a non-gravitational interaction between Dark Matter (DM) an…

hep-th2024★ 4 cited

Gravitational waves in a cyclic Universe: resilience through cycles and vacuum state

Mariaveronica De Angelis, Adam Smith, William Giarè +1

We present a generalised calculation for the spectrum of primordial tensor perturbations in a cyclic Universe, making no assumptions about the vacuum state of the theory and accoun…

astro-ph.CO2023★ 15 cited

Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions

William Giarè, Adrià Gómez-Valent, Eleonora Di Valentino +1

We study scatter-like interactions between neutrinos and dark matter in light of different combinations of temperature, polarization and lensing data released by three independent…

astro-ph.CO2023★ 16 cited

Forecasts on interacting dark energy with standard sirens

Elsa M. Teixeira, Richard Daniel, Noemi Frusciante +1

We present the predictions with standard sirens at Gravitational Waves detectors, such as the Laser Interferometer Space Antenna (LISA) and the Einstein Telescope (ET), for interac…

astro-ph.CO2023★ 18 cited

Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach

William Giarè, Mariaveronica De Angelis, Carsten van de Bruck +1

We introduce a numerical method specifically designed for investigating generic multifield models of inflation where a number of scalar fields are minimally coupled to gravit…

astro-ph.CO2023★ 4 cited

Machine Learning and Structure Formation in Modified Gravity

Jonathan C. Betts, Carsten van de Bruck, Christian Arnold +1

In General Relativity approximations based on the spherical collapse model such as Press--Schechter theory and its extensions are able to predict the number of objects of a certain…

astro-ph.CO2023★ 17 cited

Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments

Philippe Brax, Carsten van de Bruck, Eleonora Di Valentino +2

We explore an extension of the standard CDM model by including an interaction between neutrinos and dark matter, and making use of the ground based telescope data of the Cosmic…

hep-th2023★ 9 cited

Adiabatic and isocurvature perturbations in extended theories with kinetic couplings

Mariaveronica De Angelis, Carsten van de Bruck

The scalar field sector in low--energy effective field theories motivated by string theory often contains several scalar fields, some of which possess non--standard kinetic terms.…

astro-ph.CO2023★ 11 cited

New insights on -DM Interactions

Philippe Brax, Carsten van de Bruck, Eleonora Di Valentino +2

We revisit the possibility of using cosmological observations to constrain models that involve interactions between neutrinos and dark matter. We show that small-scale measurements…

astro-ph.CO2023★ 76 cited

A Consistent View of Interacting Dark Energy from Multiple CMB Probes

Yuejia Zhai, William Giarè, Carsten van de Bruck +3

We analyze a cosmological model featuring an interaction between dark energy and dark matter in light of the measurements of the Cosmic Microwave Background released by three indep…

hep-th2022★ 7 cited

Constraints on Late Time Violations of the Equivalence Principle in the Dark Sector

Cameron C. Thomas, Carsten van de Bruck

If dark energy is dynamical due to the evolution of a scalar field, then in general it is expected that the scalar is coupled to matter. While couplings to the standard model parti…

hep-th2022★ 22 cited

Scalar field dark matter and dark energy: a hybrid model for the dark sector

Carsten van de Bruck, Gaspard Poulot, Elsa M. Teixeira

Diverse cosmological and astrophysical observations strongly hint at the presence of dark matter and dark energy in the Universe. One of the main goals of Cosmology is to explain t…

hep-ph2021★ 2 cited

Co-interacting dark matter and conformally coupled light scalars

Philippe Brax, Carsten van de Bruck, Sebastian Trojanowski

The increasing observational pressure on the standard cosmological model motivates analyses going beyond the paradigm of the collision-less cold dark matter (DM). Since the only cl…

astro-ph.CO2016★ 81 cited

Testing coupled dark energy models with their cosmological background evolution

Carsten van de Bruck, Jurgen Mifsud, Jack Morrice

We consider a cosmology in which dark matter and a quintessence scalar field responsible for the acceleration of the Universe are allowed to interact. Allowing for both conformal a…

astro-ph.CO2016★ 10 cited

Non-Gaussianity in multi-sound-speed disformally coupled inflation

Carsten van de Bruck, Tomi Koivisto, Chris Longden

Most, if not all, scalar-tensor theories are equivalent to General Relativity with a disformally coupled matter sector. In extra-dimensional theories such a coupling can be underst…

gr-qc2016★ 16 cited

Reheating and preheating in the simplest extension of Starobinsky inflation

C. van de Bruck, P. Dunsby, L. E. Paduraru

The epochs of reheating and preheating are studied in a simple extension of the Starobinsky inflationary model, which consists of an --correction to the Einstein--Hilbert acti…

gr-qc2016★ 17 cited

Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings

Carsten van de Bruck, Clare Burrage, Jack Morrice

The simplest way to modify gravity is to extend the gravitational sector to include an additional scalar degree of freedom. The most general metric that can be built in such a theo…

astro-ph.CO2016★ 21 cited

Running of the Running and Entropy Perturbations During Inflation

Carsten van de Bruck, Chris Longden

In single field slow-roll inflation, one expects that the spectral index is first order in slow-roll parameters. Similarly, its running and the runni…