lagrangian density उदाहरण वाक्य
उदाहरण वाक्य
- Let \ mathcal { L } _ \ mathrm { M } represent the Lagrangian density of matter and \ mathcal { L } _ \ mathrm { G } represent the Lagrangian density of the gravitational field.
- To use the Dyson series to calculate anything, one needs more than a gauge-invariant Lagrangian density; one also needs the quantization and gauge fixing prescriptions that enter into the Feynman rules of the theory.
- For example, in the case of Newtonian gravity, the Lagrangian density integrated over spacetime gives you an equation which, if solved, would yield \ Phi ( \ mathbf { x }, t ).
- Dirac s two preceding remarks suggest that we should start searching for a realistic regularization in the case of quantum electrodynamics ( QED ) in the four-dimensional Minkowski spacetime, starting with the original QED Lagrangian density.
- Instead of " fixing " the gauge to a particular " constraint surface " in configuration space, one can break the gauge freedom with an additional, non-gauge-invariant term added to the Lagrangian density.
- The fundamental Lagrangian density of one's theory is presumed to lie in the subspace " Pl " 0 of polynomials which are real-valued and invariant under any unbroken non-gauge symmetry groups.
- Noether's theorem begins with the assumption that a specific transformation of the coordinates and field variables does not change the action, which is defined as the integral of the Lagrangian density over the given region of spacetime.
- In Lagrangian field theory, the Lagrangian as a function of generalized coordinates is replaced by a Lagrangian density, a function of the fields in the system and their derivatives, and possibly the space and time coordinates themselves.
- Using a Taylor series expansion for the second integral around the mean free-surface elevation z = 0, and only retaining quadratic terms in \ Phi and \ zeta, the Lagrangian density L _ 0 for linear wave motion becomes
- To obtain the field equations the electromagnetic tensor in the Lagrangian density needs to be replaced by its definition in terms of the 4-potential " A ", and its this potential which enter the Euler-Lagrange equations.