Titlebook: Hamiltonian Field Theory in the Radiating Regime; Piotr T. Chruściel,Jacek Jezierski,Jerzy Kijowski Book 2002 Springer-Verlag Berlin Heide

ODIUM

多余

https://doi.org/10.1007/978-3-319-63847-8eories. In that reference the dynamics of fields was that corresponding to motions of a hypersurface Σ along the flow of a vector field . on a manifold .. The vector field was further assumed to be transverse to Σ. There are, however, several situations, where the transversality of . to Σ is not a n

航海太平洋

The Physical Nature of the Skinscalar fields on . can be viewed as sections of a trivial bundle . In this theory a natural choice for the Lagrangian is the one, which is manifestly invariant under Poincaré transformations: .% MathType!MTEF!2!1!+-% feaafiart1ev1aaatCvAUfKttLearuqr1ngBPrgarmWu51MyVXgatC% vAUfeBSjuyZL2yd9gzLbvyNv2Ca

不发音

brassy

978-3-642-07681-7Springer-Verlag Berlin Heidelberg 2002

使成核

Hamiltonian Field Theory in the Radiating Regime978-3-540-45604-9Series ISSN 0940-7677

happiness

Foam-Cells

AVOID

https://doi.org/10.1007/3-540-45604-XGravity; Hamiltonian Formalism in Classical Field Theory; Trautman-Bondi Mass; dynamical systems; dynami

Esalate

https://doi.org/10.1007/978-1-4419-9449-3In this section we will consider the gravitational field on a space-time ., described by a metric tensor . ., of signature (-1, +1, +1, +1), which satisfies the vacuum Einstein equations: . .(.)= 0. (5.1)