Contribution of long-wavelength gravitational waves to the cosmic microwave background anisotropy

Physical Review D

Volumn 46, Issue 10, 1992, Pages 4198-4205

  White, Martin ^a,b  

^a YALE UNIVERSITY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000386368     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.46.4198     Document Type: Article

References (44)

1. A general, gauge-invariant analysis of the cosmic microwave anisotropy
2. Preliminary results from the COBE differential microwave radiometers - Large angular scale isotropy of the cosmic microwave background
3. A map of the cosmic background radiation at 3 millimeters
4. GRAVITON CREATION IN THE EARLY UNIVERSE
5. Limits from the timing of pulsars on the cosmic gravitational wave background
6. Perturbations of a Cosmological Model and Angular Variations of the Microwave Background
7. Large-scale anisotropy of the microwave background and the amplitude of energy density fluctuations in the early universe
8. On the anisotropy of the cosmological background matter and radiation distribution. I - The radiation anisotropy in a spatially flat universe
9. The statistics of cosmic background radiation fluctuations