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Feynman Path Integral Formulation

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48 1 Continuum <strong>Formulation</strong><br />

ultraviolet cutoff. This implies that the coupling α is asymptotically free, and therefore<br />

grows with distance. Since it is 1/α that appears in the action, one would still<br />

recover the Nambu-Goto string in the continuum limit, unless some new unexpected<br />

fixed points emerge to higher order.<br />

Finally it is possible to generalize the bosonic string action of Eq. (1.195) by<br />

including a background X that is not flat (Callan, Friedan, Martinec and Perry, 1985)<br />

I nlsm [g,X,b,φ] = 1<br />

4πα ′<br />

∫<br />

d 2 σ √ g[ √ gg ab g μν (X)∂ a X μ ∂ b X μ<br />

+ g −1/2 ε ab A μν (X)∂ a X μ ∂ b X μ − 1 2 α′ 2 Rφ(X)] ,<br />

(1.226)<br />

where the new fields include the graviton g μν (X), an antisymmetric tensor field<br />

A μν (X), and the dilaton φ(X). These models are usually referred to, for historical<br />

reasons, as non-linear sigma models for strings. Note, from the structure of the last<br />

term in Eq. (1.226) involving 2 R, that the dilaton field is related to the string coupling<br />

“constant”, with the n-loop amplitude involving a factor e −2(1−n)φ (at least for a<br />

slowly varying dilaton field).<br />

In general these theories will no longer be conformally invariant unless one imposes<br />

conditions on the “beta functions for each field”, such as R μν (X)+... = 0,<br />

where the ellipsis refers to contributions from the other two fields φ(X) and A μν (X).<br />

It can be shown that these string consistency equations can be derived from a d-<br />

dimensional action with a rather simple form<br />

I dil = − 1 ∫<br />

16πG<br />

d d X √ Ge φ { R + 4(∇φ) 2 − 1<br />

12 F2 μνσ + ... } , (1.227)<br />

with F μνσ the curl of A μν . After rescaling the d-dimensional metric<br />

G μν → e 4φ/(d−2) G μν one obtains the more familiar form<br />

I dil = − 1 ∫<br />

16πG<br />

d d X √ {<br />

G R − 4<br />

}<br />

d − 2 (∇φ)2 −<br />

12 1 e−8φ(d−2) Fμνσ 2 + ...<br />

(1.228)<br />

which shows the general feature of strings coupled to background gravity: they generally<br />

involve dilaton corrections to Einstein gravity.<br />

,<br />

1.11 Supersymmetric Strings<br />

From the preceding discussion it appears that there are three main problems with<br />

the bosonic string, the first one being that the ground state is a tachyon, a particle<br />

of mass m 2 < 0. The second problem is that the bosonic string is only consistently<br />

defined in d = 26 spacetime dimensions, and the third problem is that it does not<br />

contain fermions which are after all an essential component of ordinary matter.

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