activity
20242026
collaborators

8 papers

astro-ph.CO2026

High-redshift physics from the acoustic scale

Zachary J. Weiner

We present a simplified and general description of the high-redshift information in acoustic scale measurements from the cosmic microwave background and large-scale structure. The…

astro-ph.CO2025

Dark forces suppress structure growth

Marco Costa, Cyril Creque-Sarbinowski, Olivier Simon +1

No experimental test precludes the possibility that the dark matter experiences forces beyond general relativity -- in fact, a variety of cosmic microwave background observations s…

hep-ph2025

Searching for coupled, hyperlight scalars across cosmic history

Masha Baryakhtar, Olivier Simon, Zachary J. Weiner

Cosmological scalar fields coupled to the Standard Model drive temporal variations in the fundamental constants that grow with redshift, positioning the early Universe as a powerfu…

hep-ph2025

Experimental targets for dark photon dark matter

David Cyncynates, Zachary J. Weiner

Ultralight dark photon dark matter features distinctive cosmological and astrophysical signatures and is also supported by a burgeoning direct-detection program searching for its k…

hep-ph2025

Detectable and defect-free dark photon dark matter

David Cyncynates, Zachary J. Weiner

Ultralight dark photons are compelling dark matter candidates, but their allowed kinetic mixing with the Standard Model photon is severely constrained by requiring that the dark ph…

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…