Nano-Hz gravitational wave signature from axion dark matter

Kitajima N, Soda J, Urakawa Y (2020)
arXiv:2010.10990.

Preprint | Englisch
 
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Autor*in
Kitajima, Naoya; Soda, Jiro; Urakawa, YukoUniBi
Abstract / Bemerkung
We calculate the accurate spectrum of the stochastic gravitational wave background from U(1) gauge fields produced by axion dark matter. The explosive production of gauge fields soon invalidates the applicability of the linear analysis and one needs nonlinear schemes. We make use of numerical lattice simulations to properly follow the nonlinear dynamics such as backreaction and rescattering which gives important contributions to the emission of gravitational waves. It turns out that the axion with the decay constant f∼1016f \sim 10^{16}f∼1016 GeV which gives the correct dark matter abundance predicts the circularly polarized gravitational wave signature detectable by SKA. We also show that the resulting gravitational wave spectrum has a potential to explain NANOGrav 12.5 year data.
Erscheinungsjahr
2020
Zeitschriftentitel
arXiv:2010.10990
Page URI
https://pub.uni-bielefeld.de/record/2949953

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Kitajima N, Soda J, Urakawa Y. Nano-Hz gravitational wave signature from axion dark matter. arXiv:2010.10990. 2020.
Kitajima, N., Soda, J., & Urakawa, Y. (2020). Nano-Hz gravitational wave signature from axion dark matter. arXiv:2010.10990
Kitajima, N., Soda, J., and Urakawa, Y. (2020). Nano-Hz gravitational wave signature from axion dark matter. arXiv:2010.10990.
Kitajima, N., Soda, J., & Urakawa, Y., 2020. Nano-Hz gravitational wave signature from axion dark matter. arXiv:2010.10990.
N. Kitajima, J. Soda, and Y. Urakawa, “Nano-Hz gravitational wave signature from axion dark matter”, arXiv:2010.10990, 2020.
Kitajima, N., Soda, J., Urakawa, Y.: Nano-Hz gravitational wave signature from axion dark matter. arXiv:2010.10990. (2020).
Kitajima, Naoya, Soda, Jiro, and Urakawa, Yuko. “Nano-Hz gravitational wave signature from axion dark matter”. arXiv:2010.10990 (2020).

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