Microwave Background Fluctuations Due to the Sunyaev-Zel'dovich Effect in Pancakes
Abstract
We calculate distortions in the microwave background radiation from the Sunyaev-Zel'dovich effect, produced by hot gas in large (~100 Mpc) pancakes. The large-scale distribution of the pancakes is taken to be that of a Voronoi foam. Fluctuations for this scenario are estimated to be on the order of {DELTA}T/T~10^-5^. Using computer simulations, we produce several 32^deg^ x 32^deg^ images with 0.25^deg^ resolution. These images show characteristic linear features produced when a pancake is viewed nearly edge-on. By calculating the two-point and the degenerate three-point correlation functions, we are able to statistically detect such non-Gaussian features even in the presence of a relatively large amount of Gaussian noise. The degenerate three-point correlation function is found to be particularly useful since it is insensitive to correlated Gaussian noise. We also smooth our data over a 7^deg^ FWHM Gaussian window to simulate the COBE observations. We find that under such low- resolution conditions, the features are highly suppressed.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- January 1994
- DOI:
- 10.1086/173578
- Bibcode:
- 1994ApJ...420..474S
- Keywords:
-
- Background Radiation;
- Computerized Simulation;
- Cosmic Rays;
- Cosmology;
- Microwaves;
- Variations;
- Cooling;
- Data Smoothing;
- Molecular Clouds;
- Random Noise;
- Sky Surveys (Astronomy);
- Astrophysics;
- COSMOLOGY: COSMIC MICROWAVE BACKGROUND;
- COSMOLOGY: THEORY