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17 Apr 2007: IOP PUBLISHING CLASSICAL AND QUANTUM GRAVITY. Class. Quantum Grav. 24 (2007) 1841–1862 doi:10.1088/0264-9381/24/7/010. ... An early example of this technique in gravityis the slow motion of Majumdar–Papepetrou black holes [24].

25 Jan 2007: N M Mt 2ik2[σ3, M ] kA(x, t)M B(x, t)M. (4.3.13). ... iqt qxx 2rq2 = 0irt rxx 2r2q = 0. (4.3.24). The reduction r = σq̄, σ = 1, yields the celebrated NLS equation (1.2).

27 Nov 2007: Instead, one uses a space oftempered distributions). 24. Example 6.1.2 H = L2(Rn) (where n = 1, 2, 3 are important cases) is a space of complex-valued functions such ... Ĥ =. 3j=1 P̂. 2j. 2m+ V (X̂j) =. 2. 2m2 V (xj) (6.24).

27 Jul 2007: K bb Ka = 12ηKa. Thus K is automatically geodesic, and if it is pure then its trajectories are parameterizedby an affine parameter.

5 Dec 2007: Conditions in the outer flow, including the boundary conditions, can be chosen in a special way (Warn & Warn 1978, 56; (2.24) below) such that the changes induced in the outer ... 2.24) jl,n being the nth zero of the Bessel function J1.