Bluetilted tensor spectrum and thermal history of the Universe
Abstract
We investigate constraints on the spectral index of primordial gravitational waves (GWs), paying particular attention to a bluetilted spectrum. Such constraints can be used to test a certain class of models of the early Universe. We investigate observational bounds from LIGO+Virgo, pulsar timing and big bang nucleosynthesis, taking into account the suppression of the amplitude at high frequencies due to reheating after inflation and also latetime entropy production. Constraints on the spectral index are presented by changing values of parameters such as reheating temperatures and the amount of entropy produced at late time. We also consider constraints under the general modeling approach which can approximately describe various scenarios of the early Universe. We show that the constraints on the blue spectral tilt strongly depend on the underlying assumption and, in some cases, a highly bluetilted spectrum can still be allowed.
 Authors:
 Department of Physics, Faculty of Science, Tokyo University of Science, 13, Kagurazaka, Shinjukuku, Tokyo, 1628601 Japan (Japan)
 Department of Physics, Saga University, Saga, 8408502 Japan (Japan)
 Department of Physics, Rikkyo University, 3341 NishiIkebukuro, Toshima, Tokyo, 1718501 Japan (Japan)
 Publication Date:
 OSTI Identifier:
 22382002
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2015; Journal Issue: 02; Other Information: Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; AMPLITUDES; APPROXIMATIONS; COSMOLOGICAL INFLATION; ENTROPY; GRAVITATIONAL WAVES; LIMITING VALUES; NUCLEOSYNTHESIS; PULSARS; SPECTRA; TENSORS; UNIVERSE
Citation Formats
Kuroyanagi, Sachiko, Takahashi, Tomo, and Yokoyama, Shuichiro, Email: skuro@rs.tus.ac.jp, Email: tomot@cc.sagau.ac.jp, Email: shuichiro@rikkyo.ac.jp. Bluetilted tensor spectrum and thermal history of the Universe. United States: N. p., 2015.
Web. doi:10.1088/14757516/2015/02/003.
Kuroyanagi, Sachiko, Takahashi, Tomo, & Yokoyama, Shuichiro, Email: skuro@rs.tus.ac.jp, Email: tomot@cc.sagau.ac.jp, Email: shuichiro@rikkyo.ac.jp. Bluetilted tensor spectrum and thermal history of the Universe. United States. doi:10.1088/14757516/2015/02/003.
Kuroyanagi, Sachiko, Takahashi, Tomo, and Yokoyama, Shuichiro, Email: skuro@rs.tus.ac.jp, Email: tomot@cc.sagau.ac.jp, Email: shuichiro@rikkyo.ac.jp. 2015.
"Bluetilted tensor spectrum and thermal history of the Universe". United States.
doi:10.1088/14757516/2015/02/003.
@article{osti_22382002,
title = {Bluetilted tensor spectrum and thermal history of the Universe},
author = {Kuroyanagi, Sachiko and Takahashi, Tomo and Yokoyama, Shuichiro, Email: skuro@rs.tus.ac.jp, Email: tomot@cc.sagau.ac.jp, Email: shuichiro@rikkyo.ac.jp},
abstractNote = {We investigate constraints on the spectral index of primordial gravitational waves (GWs), paying particular attention to a bluetilted spectrum. Such constraints can be used to test a certain class of models of the early Universe. We investigate observational bounds from LIGO+Virgo, pulsar timing and big bang nucleosynthesis, taking into account the suppression of the amplitude at high frequencies due to reheating after inflation and also latetime entropy production. Constraints on the spectral index are presented by changing values of parameters such as reheating temperatures and the amount of entropy produced at late time. We also consider constraints under the general modeling approach which can approximately describe various scenarios of the early Universe. We show that the constraints on the blue spectral tilt strongly depend on the underlying assumption and, in some cases, a highly bluetilted spectrum can still be allowed.},
doi = {10.1088/14757516/2015/02/003},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 02,
volume = 2015,
place = {United States},
year = 2015,
month = 2
}

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