# Gauge Symmetries and Lagrangian

Random notes for Section 14.1 of Halzen & Martin.

## Conserved Quantities

Conserved quantities are conserved locally in space, not just globally.

In classical mechanics

1. Lagrangian is $$L = T-V.$$
2. Lagrange’s equation

$$\frac{d}{dt}\left( \frac{\partial L}{\partial \dot q_i} \right) - \frac{\partial L}{\partial q_i} = 0,$$

where $q_i$ are the generalized coordinates and $\dot q_i \equiv \frac{d q_i}{dt}$.

To generalize to quantum fields, we generalize the generalized coordinates to fields, so that descretized coordinates $q_i$ becomes fields $\phi(x,t)$.

1. Lagrangian density is $$\mathcal L (\phi,\partial \phi/\partial x_\mu, x_\mu).$$
2. Lagrangian is $$L = \int \mathcal L d^3 x.$$
3. The equation of dynamics is Euler-Lagrangian equation $$\frac{\partial }{\partial x_\mu} \left( \frac{ \partial \mathcal L }{ \partial ( \phi_{,\mu} ) } \right) - \frac{\partial \mathcal L}{\partial \phi} = 0,$$ where we denoted $\partial \phi/\partial x_\mu$ as $\phi_{,\mu}$.

By convention, Lagrangian density is usually called Lagrangian in QFT.

1. Klein-Gordon equation $(\Box^2 + m^2)\phi = 0$: Lagrangian is $\mathcal L = \frac{1}{2} \partial_\mu \phi \partial^\mu \phi - \frac{1}{2} m^2 \phi^2$.
2. Dirac equation: Lagrangian is $\mathcal L = i \bar \psi \gamma_\mu \partial^\mu \psi - m \bar \psi \psi$.
3. Maxwell equation $\partial_\mu F^{\mu\nu} = j^\nu$ ($F^{\mu\nu} = \partial^\mu A^\nu - \partial^\nu A^\mu$): Lagrangian is $\mathcal L = - \frac{1}{4} F_{\mu\nu} F^{\mu\nu} - j^\mu A_\mu$.
4. Massive photons $(\Box^2 + m^2)A^\mu= j^\mu$: Lagrangian is $\mathcal L = - \frac{1}{4} F_{\mu\nu} F^{\mu\nu} - j^\mu A_\mu + \frac{1}{2}m^2 A_\mu A^\mu$.

One should connect Feynmann rules with Lagrangians.