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- W2988780927 abstract "We study spherically symmetric solutions with a scalar field in the shift-symmetric subclass of the Horndeski theory. Constructing an effective energy-momentum tensor of the scalar field based on the two-fluid model, we decompose the scalar field into two components: dark matter and dark energy.We find the dark-matter fluid is pressure-less, and its distribution of energy density obeys the inverse-square law. We show the scalar field dark matter can explain the galaxy rotation curve and discuss the time evolution of the dark matter in the cosmic background." @default.
- W2988780927 created "2019-11-22" @default.
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- W2988780927 date "2020-01-23" @default.
- W2988780927 modified "2023-10-17" @default.
- W2988780927 title "Dark matter candidate induced by Horndeski theory: Dark matter halo and cosmological evolution" @default.
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- W2988780927 doi "https://doi.org/10.1103/physrevd.101.024046" @default.
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