The Euler–Lagrange Equations and Noether’s Theorem

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Lectures on Classical and Quantum Theory of Fields

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Abstract

The stationary action principle and the general form of the Euler–Lagrange equations. The notion of symmetry in classical field theory. Noether’s conserved currents.

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Notes

  1. 1.

    L is regarded as a function of q\(\dot{q}\) and t.

  2. 2.

    This assumption has been made in the derivation of the Euler–Lagrange equation (2.6).

  3. 3.

    It may happen that some of the relations (2.9) reduce to trivial identities like \(0=0\).

  4. 4.

    Nevertheless, up to formula (2.30) below, we do not make use of the assumption that the transformations are global. Only the derivation of Noether’s identity (2.31) from formula (2.30) depends on this assumption.

  5. 5.

    \(\partial \Omega \) is called surface in the space-time because its dimension, equal to 3, differs from the dimension of the space-time by 1.

  6. 6.

    One should not confuse a symmetry of a model with a symmetry of a concrete physical state. For example, a model which is invariant under rotations can predict the existence of physical states which are not invariant under rotations.

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Correspondence to Henryk Arodź .

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Arodź, H., Hadasz, L. (2017). The Euler–Lagrange Equations and Noether’s Theorem. In: Lectures on Classical and Quantum Theory of Fields. Graduate Texts in Physics. Springer, Cham. https://doi.org/10.1007/978-3-319-55619-2_2

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