1 | The situation is even more puzzling in the
Einstein-Yang-Mills theory where the right side of
Equation (1![]() ![]() ![]() ![]() ![]() ![]() |
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2 | However, Condition (6![]() ![]() |
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3 | Indeed, the situation is similar for black holes in equilibrium. While it is physically reasonable to restrict oneself to IHs, most results require only the WIH boundary conditions. The distinction can be important in certain applications, e.g., in finding boundary conditions on the quasi-equilibrium initial data at inner horizons. | |
4 | Note that we could replace ![]() ![]() ![]() |
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5 | This formula has a different sign from that given
in [85![]() |
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6 | Cook’s boundary condition on the conformal
factor ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
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7 | We are grateful to Alejandro Corichi for correspondence on the recent results in this area. |