activity
20242026
collaborators

5 papers

astro-ph.CO2026

Simultaneous inference of isotropic and anisotropic polarization rotation angles for next-generation cosmic microwave background experiments

Yue Zhang, Chang Feng, Sen Li +1

The ultrahigh-sensitivity polarization imaging of the cosmic microwave background (CMB) is a treasure trove for new physics. Searching for a predicted polarization angle rotation k…

astro-ph.CO2025

Inference of -mode polarization in the presence of non-Gaussian foregrounds

Sen Li, Chang Feng, Filipe B. Abdalla

The inflationary -mode signals encode invaluable information about the origin of our Universe and searching for potential signatures of primordial gravitational waves (PGWs) is…

astro-ph.CO2025

Improved constraints on ultralight axions using latest observations of the early and late Universe

Qianshuo Liu, Chang Feng, Filipe B. Abdalla

Ultralight axions (ULAs) are hypothetical particles which can behave like dark matter (DM) or dark energy (DE) depending on masses generated at the symmetry-breaking scale. It rema…

astro-ph.CO2025

Investigating cross-correlations between cosmic microwave background lensing and 21 cm intensity mapping

Alessandro Marins, Chang Feng, Filipe B. Abdalla

The neutral hydrogen (HI) signal is a crucial probe for astrophysics and cosmology, but it is quite challenging to measure from raw data because of bright foreground contaminants a…

astro-ph.CO2024

Detecting ultralight axions from multifrequency observations of neutral hydrogen intensity mapping

Qianshuo Liu, Chang Feng, Filipe B. Abdalla

We investigate the effects of ultralight axions (ULAs) on the differential brightness temperature fluctuations of neutral hydrogen at the post-reionization stage. Unique structure…