Topology of microwave background fluctuations - Theory
Creators
- 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
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21073602
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANISOTROPY; ASTROPHYSICS; DISTRIBUTION FUNCTIONS; MICROWAVE RADIATION; RELICT RADIATION; SIGNAL-TO-NOISE RATIO; STRING MODELS; TEMPERATURE GRADIENTS; TOPOLOGY
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; EXTENDED PARTICLE MODEL; MATHEMATICAL MODELS; MATHEMATICS; PARTICLE MODELS; RADIATIONS