04.06.2013 Views

Gravity and Strings

Gravity and Strings

Gravity and Strings

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

30 Noether’s theorems<br />

First, observe that, in general, in the local case, the transformations contain derivatives of<br />

the local parameters. We eliminate these derivatives of the transformation parameters by<br />

integration by parts in Eq. (2.16). We obtain an identity of the form4 <br />

d d <br />

x ∂µj µ<br />

N2 (σ ) + σ I <br />

δS<br />

DI , (2.23)<br />

δϕ<br />

<br />

where DI are operators containing derivatives acting on the equations of motion. This identity<br />

is true for arbitrary parameters. We can choose parameters such that j µ<br />

N2 (σ ) vanishes on<br />

the boundary. Then, we obtain the off-shell identities that do not involve the transformation<br />

parameters<br />

δS<br />

DI = 0, (2.24)<br />

δϕ<br />

that relate the equations of motion, so not all of them are independent. These identities are<br />

called gauge or Bianchi identities. Since they are identically true for arbitrary values of the<br />

parameters, we obtain the off-shell “conservation law” 5<br />

∂µj µ<br />

N2 (σ ) = 0. (2.25)<br />

Since this is an identity that holds independently of the equations of motion, it follows<br />

that the current density j µ<br />

N2 (σ ) can always be written as the divergence of a two-index<br />

antisymmetric tensor, usually called the superpotential, that is,<br />

j µ<br />

N2<br />

νµ<br />

(σ ) = ∂νj (σ ), jνµ (σ ) =−jµν(σ<br />

). (2.26)<br />

N2<br />

This identity for the vector densities is written in terms of the vectors j µ<br />

N2 = √ |g| j µ<br />

N2 :<br />

j µ<br />

N2 (σ ) =∇ν j νµ<br />

N2 (σ ),<br />

νµ<br />

µν<br />

jN2 (σ ) =−j N2 (σ ). (2.27)<br />

Observe that the difference between j µ<br />

N1 <strong>and</strong> jµ<br />

N2 is always a term proportional to the<br />

equations of motion, i.e. it vanishes on-shell. Thus, these two currents are identical on-<br />

shell. In general we are free to add any term that vanishes on-shell to the current j µ<br />

N1 since<br />

it is conserved only on-shell. We have just seen that there is a specific on-shell vanishing<br />

term that relates j µ µ µ<br />

N1 to j N2 . j N2 cannot be modified in this way because its defining property<br />

is that it is conserved off-shell. However, we could add to both currents terms of the form<br />

∂ν νµ , where µν = [µν] , which would change the superpotential. If νµ is of the form<br />

∂ρU ρνµ , with U ρνµ = U [ρν]µ , then ∂ν νµ = 0 <strong>and</strong> the change in the superpotential will not<br />

change the Noether current.<br />

It is easy to see that Noether currents are sensitive to the addition of total derivatives<br />

to the Lagrangian even if these do not modify the equations of motion: on adding to the<br />

action (2.1)<br />

<br />

S = d<br />

<br />

d x ∂µL µ , (2.28)<br />

4 This expression is just symbolic. We need a more explicit form of the infinitesimal transformations in order<br />

to obtain more explicit expressions. We will find several examples in the following chapters.<br />

5 Strong conservation law in the language of [110].<br />

N2<br />

N2

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!