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Cited by 291

The DOI matches its Crossref record; 39 of the 39 references it cites were found in a registry or an index.

Improved calculation of the primordial gravitational wave spectrum in the standard model

Open access
Watanabe, Yuki, Komatsu, Eiichiro·2006·Physical Review D

Abstract

We show that the energy density spectrum of the primordial gravitational waves has characteristic features due to the successive changes in the relativistic degrees of freedom during the radiation era. These changes make the evolution of radiation energy density deviate from the conventional adiabatic evolution, ${\ensuremath{\rho}}_{r}\ensuremath{\propto}{a}^{\ensuremath{-}4}$, and thus cause the expansion rate of the universe to change suddenly at each transition which, in turn, modifies the spectrum of primordial gravitational waves. We take into account all the particles in the standard model of elementary particles. In addition, free-streaming of neutrinos damps the amplitude of gravitational waves, leaving characteristic features in the energy density spectrum. Our calculations are solely based on the standard model of cosmology and particle physics, and therefore these features must exist. Our calculations significantly improve the previous ones which ignored these effects and predicted a smooth, featureless spectrum.

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Metadata

Authors
Watanabe, Y., & Komatsu, E.
Venue
Physical Review D
Published
2006-06-12
Volume
73
Issue
12
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W1992950749
Cited by
291
References
39
FWCI
5.98
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Improved calculation of the primordial gravitational wave spectrum in the standard model. https://app.cochat.ai/papers/10.1103/physrevd.73.123515
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Watanabe, Y., & Komatsu, E. (2006). Improved calculation of the primordial gravitational wave spectrum in the standard model. Physical Review D. https://doi.org/10.1103/physrevd.73.123515

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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