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- W3099014905 abstract "For arbitrary static spacetimes, it is shown that an equilibrium between a Killing horizon and matter is only possible for some discrete values of the parameter w = p1/ρ, where ρ is the density and p1 is the pressure in the direction normal to the horizon. In the generic situation of a simple (non-extremal) horizon and the slowest possible density decrease near the horizon, this corresponds to w = −1/3, the value known for a gas of disordered cosmic strings. An admixture of 'vacuum matter', characterized by w = −1 and nonzero density at the horizon, is also admitted. This extends the results obtained previously for static, spherically symmetric spacetimes. A new feature as compared to spherical symmetry is that higher order horizons can exist in the absence of vacuum matter if the horizon is a surface of zero curvature, which can occur, e.g., in cylindrically symmetric spacetimes." @default.
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- W3099014905 date "2009-07-30" @default.
- W3099014905 modified "2023-09-29" @default.
- W3099014905 title "General static black holes in matter" @default.
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