activity
20142026
most citedCosmology Intertwined II: The Hubble Constant Tension

540 citations · 2.3k across the 37 of their papers we have counts for

collaborators
Showing 2026Show all

11 papers · 1 filter

gr-qc2026

Charge-regular formulation and radiative amplitudes of Kerr-Newman perturbations

Hayato Motohashi

We establish a charge-regular formulation of separated Kerr--Newman perturbations and an explicit map from master solutions to physical radiative fields. We derive regular angular…

astro-ph.CO2026

or : DESI constraints on relative baryon-CDM perturbations

Ananda F. Smith, Mikhail M. Ivanov, Roger de Belsunce +3

We carry out a search for the relative baryon-cold dark matter (CDM) density and velocity modes in the DESI full-shape (FS) data, and investigate whether DESI's preference for evol…

astro-ph.CO2026

One-point matter PDFs beyond TopHat filters

Anton Chudaykin, Alexander M. Kayssi, Sergey Sibiryakov

We study the one-point probability distribution function (PDF) for matter densities averaged with an arbitrary spherically symmetric window function. The PDF is analytically modele…

astro-ph.CO2026

Inflation, Open Universes, and Dark Energy

Anton Chudaykin, Mikhail M. Ivanov, Renata Kallosh +3

We study the impact of spatial curvature () and dynamical dark energy (parametrized by and ) on the spectral index using a combination of cosmic microwave bac…

astro-ph.CO2026

Inflationary interpretation of the gravitational-wave signal in the European Pulsar Timing Array DR2 with constraints

Philippe Turgeon, Chiara Caprini, Anton Chudaykin +5

The second data release of the European Pulsar Timing Array (EPTA) collaboration provides evidence for the presence of a gravitational-wave (GW) background. In this work, we explor…

astro-ph.CO2026

Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum

Euclid Collaboration, D. Linde, A. Moradinezhad Dizgah +281

Primordial non-Gaussianity (PNG) is a powerful probe of the origin of cosmic structure. Stage-IV surveys like \Euclid will measure galaxy - and -point clustering at high sign…

astro-ph.CO2026

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior

Gen Ye, Anton Chudaykin, Camille Bonvin +1

We present a non-parametric, model-independent reconstruction of the cosmological background and perturbation dynamics in non-minimally coupled theories of gravity. Within the Effe…

astro-ph.CO2026

Euclid preparation. Galaxy power spectrum and bispectrum modelling

Euclid Collaboration, K. Pardede, A. Eggemeier +306

Higher-order correlation functions of the large-scale galaxy distribution offer access to information beyond that contained in standard 2-point statistics such as the power spectru…

astro-ph.CO2026

Euclid preparation. Galaxy 2-point correlation function modelling in redshift space

Euclid Collaboration, M. Kärcher, M. -A. Breton +309

The Euclid satellite will measure spectroscopic redshifts for tens of millions of emission-line galaxies. In the context of Stage-IV surveys, the 3-dimensional clustering of galaxi…

astro-ph.CO2026

Euclid preparation. Galaxy power spectrum modelling in redshift space

Euclid Collaboration, B. Camacho Quevedo, M. Crocce +292

Accurate modelling of redshift-space distortions (RSD) is essential for maximizing the cosmological information extracted from large galaxy redshift surveys. In preparation for the…

astro-ph.CO2026

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy

Mikhail M. Ivanov, James M. Sullivan, Roger de Belsunce +4

We present cosmological parameter measurements from the full combination of DESI DR1 galaxy clustering data, described with large-scale structure effective field theory. By incorpo…