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Geometric field theory and weak Euler-Lagrange equation for classical relativistic particle-field systems
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作者 Peifeng Fan Hong Qin +2 位作者 Jian Liu Nong Xiang Zhi Yu 《Frontiers of physics》 SCIE CSCD 2018年第4期209-220,共12页
A manifestly covariant, or geometric, field theory of relativistic classical particle-field systems is devel- oped. The connection between the space-time symmetry and energy-momentum conservation laws of the system is... A manifestly covariant, or geometric, field theory of relativistic classical particle-field systems is devel- oped. The connection between the space-time symmetry and energy-momentum conservation laws of the system is established geometrically without splitting the space and time coordinates; i.e., space- time is treated as one entity without choosing a coordinate system. To achieve this goal, we need to overcome two difficulties. The first difficulty arises from the fact that the particles and the field reside on different manifolds. As a result, the geometric Lagrangian density of the system is a function of the 4-potential of the electromagnetic fields and also a functional of the particles' world lines. The other difficulty associated with the geometric setting results from the mass-shell constraint. The standard Euler-Lagrange (EL) equation for a particle is generalized into the geometric EL equation when the mass-shell constraint is imposed. For the particle-field system, the geometric EL equation is further generalized into a weak geometric EL equation for particles. With the EL equation for the field and the geometric weak EL equation for particles, the symmetries and conservation laws can be established geometrically. A geometric expression for the particle energy-momentum tensor is derived for the first time, which recovers the non-geometric form in the literature for a chosen coordinate system. 展开更多
关键词 relativistic particle-field system different manifolds mass-shell constraint geometric weakEuler-Lagrange equation symmetry conservation laws
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