Published October 29, 1990
| Version v1
Journal article
Characteristic microwave-background distortions from collapsing spherical domain walls
Creators
- 1. NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL (USA)
- 2. Astronomy and Astrophysics Center, University of Chicago, Chicago, IL (USA)
Description
We analyze the magnitude and angular pattern of distortions of the microwave background by collapsing spherical domain walls. We find a characteristic pattern of red-shift distortions of red or blue spikes surrounded by blue disks. The width and height of a spike is related to the diameter and magnitude of the disk. A measurement of the relations between these quantities thus can serve as an unambiguous indicator for a collapsing spherical domain wall. From the red-shift distortion in the blue disks we find an upper bound on the surface energy density of the walls σ approx-lt 8 MeV3
Additional details
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 65
- Journal Issue
- 18
- Series
- Phys. Rev. Lett.
- Journal Page Range
- 2229-2232
- ISSN
- 0031-9007
- CODEN
- PRLTA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22040480
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BLACK HOLES; COSMIC RADIATION; MICROWAVE RADIATION; PHASE TRANSFORMATIONS; PHOTONS; UNIVERSE
- Descriptors DEC
- BOSONS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; IONIZING RADIATIONS; MASSLESS PARTICLES; RADIATIONS