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Introduction to String Theory and D–Branes - School of Natural ...

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Therefore we have<br />

from which we can derive<br />

<strong>and</strong> so substituting in<strong>to</strong> S, we recover the Nambu–Go<strong>to</strong> action, So.<br />

Let us note some <strong>of</strong> the symmetries <strong>of</strong> the action:<br />

• Spacetime Lorentz/Poincaré:<br />

hab − 1<br />

2 γabγ cd hcd = 0 , (14)<br />

γ ab hab = 2(−h) 1/2 (−γ) −1/2 , (15)<br />

X µ → X ′µ = Λ µ νX ν + A µ ,<br />

where Λ is an SO(1, D − 1) Lorentz matrix <strong>and</strong> A µ is an arbitrary constant D–vec<strong>to</strong>r. Just as before<br />

this is a trivial global symmetry <strong>of</strong> S (<strong>and</strong> also So), following from the fact that we wrote them in<br />

covariant form.<br />

• Worldsheet Reparametrisations:<br />

δX µ = ζ a ∂aX µ<br />

δγ ab = ζ c ∂cγ ab − ∂cζ a γ cb − ∂cζ b γ ac , (16)<br />

for two parameters ζ a (τ, σ). This is a non–trivial local or “gauge” symmetry <strong>of</strong> S. This is a large extra<br />

symmetry on the world–sheet <strong>of</strong> which we will make great use.<br />

• Weyl invariance:<br />

γab → γ ′ ab = e2ω γab , (17)<br />

specified by a function ω(τ, σ). This ability <strong>to</strong> do local rescalings <strong>of</strong> the metric results from the fact<br />

that we did not have <strong>to</strong> choose an overall scale when we chose γ ab <strong>to</strong> rewrite So in terms <strong>of</strong> S. This<br />

can be seen especially if we rewrite the relation (15) as (−h) −1/2 hab = (−γ) −1/2 γab.<br />

We note here for future use that there are just as many parameters needed <strong>to</strong> specify the local symmetries<br />

(three) as there are independent components <strong>of</strong> the world-sheet metric. This is very useful, as we shall see.<br />

2.2 <strong>String</strong> Equations <strong>of</strong> Motion<br />

We can get equations <strong>of</strong> motion for the string by varying our action (11) with respect <strong>to</strong> the X µ :<br />

1<br />

δS =<br />

2πα ′<br />

<br />

d 2 <br />

σ ∂a (−γ) 1/2 γ ab <br />

∂bXµ δX µ<br />

− 1<br />

2πα ′<br />

<br />

dτ (−γ) 1/2 ∂σXµδX µ<br />

<br />

<br />

σ=π<br />

, (18)<br />

σ=0<br />

which results in the equations <strong>of</strong> motion:<br />

<br />

(−γ) 1/2 γ ab ∂bX µ<br />

≡ (−γ) 1/2 ∇ 2 X µ = 0 , (19)<br />

with either:<br />

or:<br />

∂a<br />

X ′µ (τ, 0) = 0<br />

X ′µ <br />

(τ, π) = 0<br />

X ′µ (τ, 0) = X ′µ (τ, π)<br />

X µ (τ, 0) = X µ <br />

(τ, π)<br />

γab(τ, 0) = γab(τ, π)<br />

Open <strong>String</strong><br />

(Neumann b.c.’s)<br />

Closed <strong>String</strong><br />

(periodic b.c.’s)<br />

We shall study the equation <strong>of</strong> motion (19) <strong>and</strong> the accompanying boundary conditions a lot later. We are<br />

going <strong>to</strong> look at the st<strong>and</strong>ard Neumann boundary conditions mostly, <strong>and</strong> then consider the case <strong>of</strong> Dirichlet<br />

conditions later, when we uncover D–branes, using T–duality. Notice that we have taken the liberty <strong>of</strong><br />

introducing closed strings by imposing periodicity.<br />

8<br />

(20)<br />

(21)

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