December 05, 2025 | 12:00pm - 1:00pm
Add to calendar
12/05/2025 12:00
12/05/2025 13:00
Princeton University Gravity Group Lunch Seminar
use-title
Topic: Searching for New Signals in the Microwave Sky
Speakers: Colin Hill, Columbia University
More: https://www.ias.edu/sns/events/princeton-university-gravity-group-lunch-seminar-33
Measurements of the small-scale CMB temperature and polarization
fields have recently undergone transformative improvements with Data
Release 6 (DR6) of the Atacama Cosmology Telescope (ACT) and will soon
improve further with the Simons Observatory (SO), which will open new
windows into physics beyond the standard models (BSM) of particle
physics and cosmology. I will very briefly highlight key findings from
our ACT DR6 CMB power spectrum analysis, particularly pertaining to
beyond-LCDM models motivated by the "Hubble tension." I will then
discuss signals of BSM physics in CMB secondary anisotropies, as could
be imprinted by the conversion of CMB photons into massive dark
photons (DPs) or axion-like particles. I will show the first results
of searches for these signals in CMB data, enabled by our
state-of-the-art needlet internal linear combination (NILC) code,
yielding leading bounds on DP-photon and axion-photon couplings over
two decades in DP/axion mass. I will then present a new NILC-based
B-mode inference method, which yields unbiased constraints on the
tensor-to-scalar ratio at SO sensitivity and beyond, even for the most
complex foreground simulations currently available. Finally, if time
permits, I will present robust evidence of a new (standard-model)
secondary anisotropy in the microwave sky, arising from the kinematic
SZ effect.
Jadwin 102 (Joe Henry Room)
a7a99c3d46944b65a08073518d638c23