Will the upcoming experiment PICO measure kSZ temperature anisotropy?

Click For Summary
SUMMARY

PICO will measure polarization anisotropies with high fidelity, specifically focusing on E-mode anisotropies and the low-multipole B modes critical for cosmology. The PICO science paper indicates that full-sky Compton-y maps will be produced, primarily limited to l=1000, yet the satellite's angular resolution allows for kSZ temperature anisotropy measurements at l=3000. Key requirements for accurate B-mode measurements include multiple frequency bands and stringent control of systematic errors, as high multipoles are dominated by noise from lensing residuals.

PREREQUISITES
  • Understanding of polarization anisotropies in cosmology
  • Familiarity with Compton-y maps and their significance
  • Knowledge of E-mode and B-mode polarization signals
  • Awareness of systematic errors in astronomical measurements
NEXT STEPS
  • Research the methodology for measuring E-mode and B-mode polarization signals
  • Explore the impact of lensing on polarization measurements in cosmology
  • Study the design and capabilities of satellite instruments for cosmic microwave background observations
  • Investigate techniques for controlling systematic errors in astrophysical data analysis
USEFUL FOR

Astronomers, cosmologists, and researchers involved in cosmic microwave background studies, particularly those focusing on polarization measurements and systematic error management.

SherLOCKed
Messages
13
Reaction score
1
I know for sure PICO will be measuring polarization anisotropies with high fidelity. In addition, the PICO science paper shows that it will make full-sky Compton-y maps but the plots are mostly limited to l=1000. Will PICO be able to measure kSZ temperature anisotropy at l=3000?
 
Space news on Phys.org
Based upon the described angular resolution of the satellite, absolutely. For E-mode anisotropies. Indeed, if you look at Fig 2.1, you see they've plotted the E-mode anisotropies up to around 4000. But those aren't the primary focus, as the low-multipole B modes are the most critical for new cosmology. What's important for measuring those are:
1) Lots of frequency bands (this requires a satellite)
2) Good control of systematic errors for polarization

The high multipoles are swamped by noise for the B-mode polarization signal, as the B-mode polarization signal is much smaller than the E-mode signal. One of the limiting factors here is that for B-mode polarization, lensing of large scale structure mixes E and B modes, which creates a noise-like signal (this is the "lensing residual"). The instrument noise will still be below this threshold, but we just don't get useful information out of the B-mode spectrum above a hundred or so.
 
  • Informative
Likes   Reactions: SherLOCKed

Similar threads

  • · Replies 2 ·
Replies
2
Views
1K
  • · Replies 8 ·
Replies
8
Views
3K
  • · Replies 6 ·
Replies
6
Views
3K
Replies
8
Views
4K
  • · Replies 6 ·
Replies
6
Views
8K
  • · Replies 8 ·
Replies
8
Views
4K
  • · Replies 13 ·
Replies
13
Views
6K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 1 ·
Replies
1
Views
3K