activity
20242026
collaborators

7 papers

astro-ph.CO2026

Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics

Cynthia Trendafilova, Srinivasan Raghunathan, Benjamin Wallisch +33

Neutrinos and other light relics leave characteristic imprints in the cosmic microwave background anisotropies, making their observation a sensitive probe of the particle content a…

astro-ph.CO2026

Dark winds on the horizon: Prospects for detecting neutrino and hot dark matter wakes in large-scale structure

Caio B. de S. Nascimento, Marilena Loverde

We explore the cosmological signatures of neutrino and Hot Dark Matter (HDM) wakes, which refers to the preferential accumulation of neutrinos (or, more broadly, HDM particles) dow…

astro-ph.CO2025

Where does non-Universality in Assembly Bias come from?

Charuhas Shiveshwarkar, Marilena Loverde, Christopher M. Hirata +1

Constraints on local primordial non-Gaussianity (LPnG) obtained from galaxy power spectra are limited by the perfect degeneracy between the LPnG parameter and the bias…

astro-ph.CO2025

Cosmological perturbation theory for large scale structure in phase space

Caio Nascimento, Marilena Loverde

We develop a framework for Large Scale Structure (LSS) perturbation theory, that solves the Vlasov-Poisson system of equations for the distribution function in full phase space. Th…

astro-ph.CO2025

The Spectroscopic Stage-5 Experiment

Robert Besuner, Arjun Dey, Alex Drlica-Wagner +106

The existence, properties, and dynamics of the dark sectors of our universe pose fundamental challenges to our current model of physics, and large-scale astronomical surveys may be…

astro-ph.CO2025

Abundance and properties of dark radiation from the cosmic microwave background

Murali M. Saravanan, Thejs Brinckmann, Marilena Loverde +1

We study the cosmological signatures of new light relics that are collisionless like standard neutrinos or are strongly interacting. We provide a simple and succinct rephrasing of…