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Gravity and Strings

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2.2 Noether’s theorems 27<br />

The variation of the coordinates is zero by hypothesis. Then the variation of the field<br />

commutes with the derivatives. On integrating by parts to obtain an overall factor of δϕ,we<br />

find<br />

<br />

δS =<br />

<br />

d d x<br />

<br />

δS<br />

∂L<br />

δϕ + ∂µ<br />

δϕ ∂∂µϕ<br />

− ∂ν<br />

where we have defined the first variation of the action δS/δϕ,<br />

δS ∂L<br />

≡<br />

δϕ ∂ϕ<br />

− ∂µ<br />

∂L<br />

∂∂µϕ<br />

<br />

∂L<br />

δϕ +<br />

∂∂µ∂νϕ<br />

∂L<br />

∂∂µ∂νϕ ∂νδϕ<br />

<br />

+··· , (2.3)<br />

+ ∂µ∂ν<br />

∂L<br />

+ ···. (2.4)<br />

∂∂µ∂νϕ<br />

We now use Stokes’ theorem Eq. (1.141) to reexpress the integral of the total derivative<br />

as an integral over the boundary ∂:<br />

<br />

δS = d<br />

<br />

d x δS<br />

<br />

δϕ + (−1)d−1 d<br />

δϕ ∂<br />

d−1 <br />

∂L ∂L<br />

µ − ∂ν δϕ<br />

∂∂µϕ ∂∂µ∂νϕ<br />

+ ∂L<br />

∂∂µ∂νϕ ∂νδϕ<br />

<br />

+ ··· . (2.5)<br />

In theories without higher derivatives L(ϕ, ∂ϕ) it is enough to impose that the field variations<br />

vanish over the boundary δϕ| ∂ = 0, to see that the boundary term vanishes. Then,<br />

requiring that the action is stationary, δS = 0, under those variations we obtain the usual<br />

Euler–Lagrange equations<br />

<br />

δS ∂L ∂L<br />

= − ∂µ<br />

δϕ ∂ϕ ∂∂ µ <br />

= 0. (2.6)<br />

ϕ<br />

If the Lagrangian contains higher derivatives of the field, it is necessary either to impose<br />

boundary conditions for derivatives of the variation of the field or to introduce (if possible)<br />

into the action boundary terms that do not change the equations of motion but eliminate the<br />

∂δϕ term in the total derivative. In any of these cases we obtain the equations of motion<br />

<br />

δS ∂L ∂L<br />

= − ∂µ<br />

δϕ ∂ϕ ∂∂ µ <br />

+ ∂<br />

ϕ<br />

ν ∂ µ<br />

<br />

∂L<br />

∂∂ν∂ µ <br />

− ···=0. (2.7)<br />

ϕ<br />

As we can see, the equations of motion are of degree higher than two in derivatives of<br />

the field. Thus, to solve them completely it is also necessary to give boundary conditions<br />

for the field, <strong>and</strong> for its first <strong>and</strong> higher derivatives.<br />

If we add a total derivative term ∂µk µ (ϕ) to the Lagrangian, it is clear that the equations<br />

of motion will not be modified as long as the boundary conditions for δϕ <strong>and</strong> its derivatives<br />

make k µ (ϕ) = 0 on the boundary.<br />

2.2 Noether’s theorems<br />

Let us now consider the infinitesimal transformations of the coordinates <strong>and</strong> fields<br />

˜δx µ <strong>and</strong> ˜δϕ:<br />

˜δx µ = x ′ µ − x µ ,<br />

˜δϕ(x) ≡ ϕ ′ (x ′ ) − ϕ(x), (2.8)

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