New- vs. chaotic- inflations
Abstract
We show that ''spiralized' models of new-inflation can be experimentally identified mostly by their positive spectral running in direct contrast with most chaotic-inflation models which have negative runnings typically in the range of O(10{sup −4}–10{sup −3})
- Authors:
-
- Departament de Física Teòrica and IFIC, Universitat de València-CSIC, E-46100, Burjassot (Spain)
- Publication Date:
- OSTI Identifier:
- 22524983
- Resource Type:
- Journal Article
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Additional Journal Information:
- Journal Volume: 2016; Journal Issue: 02; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 1475-7516
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; CHAOS THEORY; COSMOLOGICAL INFLATION; ENERGY SPECTRA; INFLATIONARY UNIVERSE; INFLATONS
Citation Formats
Barenboim, Gabriela, and Park, Wan-Il. New- vs. chaotic- inflations. United States: N. p., 2016.
Web. doi:10.1088/1475-7516/2016/02/061.
Barenboim, Gabriela, & Park, Wan-Il. New- vs. chaotic- inflations. United States. https://doi.org/10.1088/1475-7516/2016/02/061
Barenboim, Gabriela, and Park, Wan-Il. 2016.
"New- vs. chaotic- inflations". United States. https://doi.org/10.1088/1475-7516/2016/02/061.
@article{osti_22524983,
title = {New- vs. chaotic- inflations},
author = {Barenboim, Gabriela and Park, Wan-Il},
abstractNote = {We show that ''spiralized' models of new-inflation can be experimentally identified mostly by their positive spectral running in direct contrast with most chaotic-inflation models which have negative runnings typically in the range of O(10{sup −4}–10{sup −3})},
doi = {10.1088/1475-7516/2016/02/061},
url = {https://www.osti.gov/biblio/22524983},
journal = {Journal of Cosmology and Astroparticle Physics},
issn = {1475-7516},
number = 02,
volume = 2016,
place = {United States},
year = {Mon Feb 01 00:00:00 EST 2016},
month = {Mon Feb 01 00:00:00 EST 2016}
}
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