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- W2782660219 endingPage "023" @default.
- W2782660219 startingPage "023" @default.
- W2782660219 abstract "We consider the inflationary universe with a spectator scalar field coupled to a U(1) gauge field and calculate curvature perturbation and gravitational waves (GWs). We find that the sourced GWs can be larger than the one from vacuum fluctuation and they are statistically anisotropic as well as linearly polarized. The GW power spectrum acquires higher multipole moments with respect to the angle θ between a wave number k and a background vector field as h∝ (1−cos2θ+cos4θ−cos6θ) irrespective of the model parameters." @default.
- W2782660219 created "2018-01-26" @default.
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- W2782660219 date "2018-07-12" @default.
- W2782660219 modified "2023-10-11" @default.
- W2782660219 title "Statistically anisotropic tensor modes from inflation" @default.
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- W2782660219 doi "https://doi.org/10.1088/1475-7516/2018/07/023" @default.
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