Published August 1, 2017
| Version v1
Journal article
Slow-roll inflation and the BB-mode correlation spectrum of the Cosmic Microwave Background
Creators
- 1. School of Physics, University of Hyderabad P.O. Central University, Hyderabad 500046, India. (India)
Description
The BB-mode correlation angular spectrum of cosmic microwave background is studied for several inflation models. A comparative study of the resulting angular power spectrum with the recent joint analysis data of the BICEP2/Keck Array and Planck shows constraint to several slow-roll inflation models of cosmology. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/883/1/012007Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 883
- Journal Issue
- 1
- Journal Page Range
- [12 p.]
- ISSN
- 1742-6596
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49065301
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CORRELATIONS; COSMOLOGY; INFLATIONARY UNIVERSE; LIMITING VALUES; RELICT RADIATION; SPECTRA
- Descriptors DEC
- COSMOLOGICAL MODELS; ELECTROMAGNETIC RADIATION; MATHEMATICAL MODELS; MICROWAVE RADIATION; RADIATIONS