Poincaré recurrences of Schwarzschild black holes
نویسندگان
چکیده
منابع مشابه
Geometrodynamics of Schwarzschild black holes.
The curvature coordinates T, R of a Schwarzschild spacetime are turned into canonical coordinates T (r),R(r) on the phase space of spherically symmetric black holes. The entire dynamical content of the Hamiltonian theory is reduced to the constraints requiring that the momenta PT (r), PR(r) vanish. What remains is a conjugate pair of canonical variables m and p whose values are the same on ever...
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We start by pointing out that certain Riemann surfaces appear rather naturally in the context of wave equations in the black hole background. For a given black hole there are two closely related surfaces. One is the Riemann surface of complexified “tortoise” coordinate. The other Riemann surface appears when the radial wave equation is interpreted as the Fuchsian differential equation. We study...
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ژورنال
عنوان ژورنال: Classical and Quantum Gravity
سال: 2007
ISSN: 0264-9381,1361-6382
DOI: 10.1088/0264-9381/24/16/009