collaborators

5 papers

hep-ph2026

Probing Confining Dark Sectors with Cosmological Perturbations

Daven Wei Ren Ho, Ameen Ismail, Yuhsin Tsai

Dark matter may emerge as a composite state of a dark sector which confines in a strongly first-order phase transition (PT). To avoid structure formation constraints on warm dark m…

astro-ph.CO2026

Observable CMB B-modes from Cosmological Phase Transitions

Kylar Greene, Aurora Ireland, Gordan Krnjaic +1

A B-mode polarization signal in the cosmic microwave background (CMB) is widely regarded as smoking gun evidence for gravitational waves produced during inflation. Here, we demonst…

hep-ph2026

Cosmological and Astrophysical Constraints on Late First-Order Phase Transitions

Kylar Greene, Daven Wei Ren Ho, Soubhik Kumar +1

First-order cosmological phase transitions (PT) can take place in a dark sector at relatively late times between the big-bang nucleosynthesis and recombination epochs. Because bubb…

astro-ph.CO2026

A Universal CMB -Mode Spectrum from Early Causal Tensor Sources

Kylar Greene, Aurora Ireland, Gordan Krnjaic +1

Many early universe scenarios predict post-inflationary tensor perturbations from causality-limited, sub-horizon sources. While the microphysical details may differ, as long as the…

astro-ph.CO2026

First constraints on causal sources of primordial gravitational waves from BICEP/Keck, SPTpol, SPT-3G, Planck and WMAP -mode data

Jessica A. Zebrowski, Aurora Ireland, Christian L. Reichardt +4

Non-inflationary sources of gravitational waves in the early Universe generically predict causality-limited tensor power spectra at low frequencies. We report the first-ever constr…