Published May 2016
| Version v1
Journal article
Slow-roll inflation and BB-mode angular power spectrum of CMB
Creators
- 1. University of Hyderabad, School of Physics, Hyderabad (India)
Description
The BB-mode correlation angular power spectrum of CMB is obtained by considering the primordial gravitational waves in the squeezed vacuum state for various inflationary models and results are compared with the joint analysis of the BICEP2/Keck Array and Planck 353 GHz data. The present results may constrain several models of inflation. (orig.)
Availability note (English)
Available from: http://dx.doi.org/10.1140/epjc/s10052-016-4029-5Additional details
Identifiers
Publishing Information
- Journal Title
- European Physical Journal. C, Particles and Fields (Online)
- Journal Volume
- 76
- Journal Issue
- 5
- Journal Page Range
- p. 1-9
- ISSN
- 1434-6052
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 47087757
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANGULAR DISTRIBUTION; CHAOS THEORY; CORRELATIONS; EXPANSION; FIELD EQUATIONS; GRAVITATIONAL WAVES; HUBBLE EFFECT; INFLATIONARY UNIVERSE; INFLATONS; METRICS; MULTIPOLARITY; POLARIZATION; POTENTIALS; RELICT RADIATION; SCALAR FIELDS; SPECTRA; UNIVERSE; VACUUM STATES
- Descriptors DEC
- COSMOLOGICAL MODELS; DISTRIBUTION; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; EQUATIONS; MATHEMATICAL MODELS; MATHEMATICS; MICROWAVE RADIATION; POSTULATED PARTICLES; RADIATIONS