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  An upper bound from helioseismology on the stochastic background of gravitational waves [Erratum (2014, ApJ, 784, 88)]

Siegel, D. M., & Roth, M. (2015). An upper bound from helioseismology on the stochastic background of gravitational waves [Erratum (2014, ApJ, 784, 88)]. Astrophysical Journal, 810(1): 84. doi:10.1088/0004-637X/810/1/84.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-9F26-6 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-9F27-4
Genre: Journal Article

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 Creators:
Siegel, Daniel M.1, Author
Roth, Markus, Author
Affiliations:
1AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24008              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, Solar and Stellar Astrophysics, astro-ph.SR
 Abstract: The universe is expected to be permeated by a stochastic background of gravitational radiation of astrophysical and cosmological origin. This background is capable of exciting oscillations in solar-like stars. Here we show that solar-like oscillators can be employed as giant hydrodynamical detectors for such a background in the muHz to mHz frequency range, which has remained essentially unexplored until today. We demonstrate this approach by using high-precision radial velocity data for the Sun to constrain the normalized energy density of the stochastic gravitational-wave background around 0.11 mHz. These results open up the possibility for asteroseismic missions like CoRoT and Kepler to probe fundamental physics.

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 Dates: 20152015
 Publication Status: Published in print
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 Identifiers: DOI: 10.1088/0004-637X/810/1/84
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Title: Astrophysical Journal
Source Genre: Journal
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Publ. Info: Chicago, IL : University of Chicago Press for the American Astronomical Society
Pages: - Volume / Issue: 810 (1) Sequence Number: 84 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: /journals/resource/954922828215_2