Published March 1990 | Version v1
Journal article

Topology of microwave background fluctuations - Theory

  • 1. Centrum Astronomiczne, Warsaw (Poland)
  • 2. Institute for Advanced Study, Princeton, NJ (USA)
  • 3. Princeton Univ., NJ (USA)

Description

Topological measures are used to characterize the microwave background temperature fluctuations produced by 'standard' scenarios (Gaussian) and by cosmic strings (non-Gaussian). Three topological quantities: total area of the excursion regions, total length, and total curvature (genus) of the isotemperature contours, are studied for simulated Gaussian microwave background anisotropy maps and then compared with those of the non-Gaussian anisotropy pattern produced by cosmic strings. In general, the temperature gradient field shows the non-Gaussian behavior of the string map more distinctively than the temperature field for all topology measures. The total contour length and the genus are found to be more sensitive to the existence of a stringy pattern than the usual temperature histogram. Situations when instrumental noise is superposed on the map, are considered to find the critical signal-to-noise ratio for which strings can be detected. 59 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
352
Series
Astrophys. J.
Journal Page Range
1-14
ISSN
0004-637X
CODEN
ASJOA