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Populating the swampland: the case of U(1)⁴96 and E₈ x U(1)²48

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arxiv 0809.1525 v1 pith:VPDBRARA submitted 2008-09-09 hep-th

Populating the swampland: the case of U(1)⁴96 and E₈ x U(1)²48

classification hep-th
keywords theoriesgaugeknownquantumsingularitiessupergravityallowedfirst
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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For d=10 N=1 SUGRA coupled to d=10 N=1 SYM, anomaly cancellation places severe constraints on the allowed gauge groups. Besides the ones known to appear in string theory, only U(1)^496 and E_8 x U(1)^248 are allowed. There are no known theories of quantum gravity that reduce in some limit to these two last supergravity theories, and in this note I present some evidence that those quantum theories might not exist. The first observation is that, upon compactification, requring that the quantum theory possesses a moduli space with finite volume typically implies the existence of singularities where the 4d gauge group is enhanced, but for these two theories that gauge enhancement is problematic from the 10d point of view. I also point out that while these four supergravity theories present repulson-type singularities, the known mechanism that repairs those singularities for the first two - the non-Abelian enhancon - is not available for the last two theories. In short, these two supergravity theories might be too Abelian for their own good.

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