Journal
PHYSICAL REVIEW D
Volume 98, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.98.064010
Keywords
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Funding
- National Natural Science Foundation of China (NNSFC) [11375153, 11675145]
- JSPS KAKENHI [JP17H02890, JP17H06359]
- World Premier International Research Center Initiative (WPI), MEXT, Japan
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We numerically study the gravitational collapse of a massless scalar field with spherical symmetry in Einstein-aether theory, and show that apparent, spin-0, and dynamical universal horizons (dUHs) can be all formed. The spacetime and the tether field are well-behaved and regular, including regions nearby these horizons (but away from the center of spherical symmetry). The spacetime outside the apparent and spin-0 horizons settles down to a static configuration, and some of such resulting static black holes were already found numerically in the literature. On the other hand, the proper distance of the outermost dUH from the apparent (or spin-0) horizon keeps increasing on tether-orthogonal time slices. This indicates that the outermost dUH is evolving into the causal boundary, even for excitations with large speeds of propagation.
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