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Gravity and Strings

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416 String theory<br />

Table 14.1. A brane scan taking into account only scalar supermultiplets. N is<br />

given by the quotient between the numbers given <strong>and</strong> M.<br />

p =−1 p = 0 p = 1 p = 2 p = 3 p = 4 p = 5<br />

d M d (d − 1) (d − 2) (d − 3) (d − 4) (d − 5) (d − 6)<br />

2 1 8 4<br />

3 2 12 8 4<br />

4 4 16 12 8 4<br />

5 8 16 8<br />

6 8 16 8<br />

7 16 16<br />

8 16 32 16<br />

9 16 32 16<br />

10 16 32 16<br />

11 32 32<br />

<strong>and</strong> it can be solved in the cases represented in Table 14.1 [13]. There are five series of<br />

solutions. Four of them (with NM = 32, 16, 8, <strong>and</strong> 4) are associated with the four division<br />

algebras O, Q, C, <strong>and</strong> R, respectively. These series correspond to objects related by double<br />

dimensional reduction,aswewill see.<br />

There is another way to underst<strong>and</strong> this result: if there is linearly realized worldvolume<br />

supersymmetry, the worldvolume fields must fit in (p + 1)-dimensional scalar supermultiplets.<br />

Each solution in the table corresponds to a scalar multiplet. There is agreement with<br />

the fact that scalar multiplets exist only in up to six dimensions.<br />

For us, it is interesting that spacetime supersymmetric string actions could in principle<br />

be constructed in d = 3, 4, 6, <strong>and</strong> 10, provided that the action has κ-symmetry. Green <strong>and</strong><br />

Schwarz showed in [472] that the ten-dimensional action previously constructed by them in<br />

[471] has κ-symmetry. The Green–Schwarz (GS) action is not just a straightforward generalization<br />

of the superparticle action Eq. (14.28), because the kinetic term would not be<br />

κ-symmetric by itself. The key to κ-symmetry is the addition of a (super-)Wess–Zumino<br />

(WZ) term: the integral of a 2-form 2 such that 3 = d2 is (target) Poincaré- <strong>and</strong> supersymmetry<br />

invariant [528]: 10<br />

2 =−idX µ δ a µ ∧ ( ¯θ 1 Ɣaθ 1 − ¯θ 2 Ɣadθ 2 ) + ( ¯θ 1 Ɣadθ 1 ) ∧ ( ¯θ 2 Ɣ a dθ 2 ). (14.33)<br />

The GS action is then given by<br />

S=− T<br />

<br />

d<br />

2 <br />

2ξ √ |γ |γ ij (∂i X µ δa µ − i ¯θ I γ a∂iθ I )(∂ j X νδb ν − i ¯θ J γ b∂ jθ J <br />

)ηab + T 2.<br />

<br />

(14.34)<br />

10 According to Table 14.1, this is an N = 2 theory, with two minimal (Majorana–Weyl spinors with 16 real<br />

components) ten-dimensional spinors, θ 1 <strong>and</strong> θ 2 , with equal or opposite chiralities: type-IIB <strong>and</strong> type-IIA<br />

strings, respectively. These theories can also be described with the RNS theory, but only after quantization.

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