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  Gravitational waves from compact dark matter objects in the solar system

Horowitz, C. J., Papa, M. A., & Reddy, S. (in preparation). Gravitational waves from compact dark matter objects in the solar system.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0003-5509-4 Version Permalink: http://hdl.handle.net/21.11116/0000-0003-550A-3
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1902.08273.pdf (Preprint), 9MB
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1902.08273.pdf
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 Creators:
Horowitz , C. J., Author
Papa, M. A.1, 2, Author              
Reddy, S., Author
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              
2Searching for Continuous Gravitational Waves, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_2630691              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE, Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM,High Energy Physics - Phenomenology, hep-ph
 Abstract: Dark matter could be composed of compact dark objects (CDOs). We find that a close binary of CDOs orbiting {\it inside} solar system bodies can be a loud source of gravitational waves (GWs) for the LIGO and VIRGO detectors. An initial search of data from the first Advanced LIGO observing run (O1), sensitive to $h_0\approx 10^{-24}$, rules out close binaries orbiting near the center of the Sun with GW frequencies (twice the orbital frequency) between 50 and 550 Hz and CDO masses above approximately 10^{-9} M_sun.

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 Dates: 2019-02-21
 Publication Status: Not specified
 Pages: 5 pages, 3 figures
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 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1902.08273
URI: http://arxiv.org/abs/1902.08273
 Degree: -

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