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Cited by 309

The DOI matches its Crossref record; 46 of the 46 references it cites were found in a registry or an index.

Gravitational radiation from cosmological turbulence

Open access
Kosowsky, Arthur, Mack, Andrew, Kahniashvili, Tinatin·2002·Physical Review D

Abstract

An injection of energy into the early Universe on a given characteristic length scale will result in turbulent motions of the primordial plasma. We calculate the stochastic background of gravitational radiation arising from a period of cosmological turbulence, using a simple model of isotropic Kolmogoroff turbulence produced in a cosmological phase transition. We also derive the gravitational radiation generated by magnetic fields arising from a dynamo operating during the period of turbulence. The resulting gravitational radiation background has a maximum amplitude comparable to the radiation background from the collision of bubbles in a first-order phase transition, but at a lower frequency, while the radiation from the induced magnetic fields is always subdominant to that from the turbulence itself. We briefly discuss the detectability of such a signal.

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Metadata

Authors
Kosowsky, A., Mack, A., & Kahniashvili, T.
Venue
Physical Review D
Published
2002-07-24
Volume
66
Issue
2
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2154533575
Cited by
309
References
46
FWCI
2.54
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Gravitational radiation from cosmological turbulence. https://app.cochat.ai/papers/10.1103/physrevd.66.024030
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Kosowsky, A., Mack, A., & Kahniashvili, T. (2002). Gravitational radiation from cosmological turbulence. Physical Review D. https://doi.org/10.1103/physrevd.66.024030

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