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How to Create a Flat Ten or Eleven Dimensional Space-time in the Interior of an Asymptotically Flat Four Dimensional String Theory
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By taking large mass and charge limit of a black hole in string theory we can create arbitrarily large regions where the space-time is approximately flat, but the moduli fields take values different from their asymptotic values. In this paper we describe a special case of this where black hole solutions in a four dimensional string theory, in the large mass and charge limit, can have an arbitrarily large region outside the horizon where a local observer will experience type IIA string theory in flat ten dimensional space-time. The curvature and other field strengths remain small everywhere between the asymptotic four dimensional observer and the ten dimensional region. By going to a different region of space, we can also get a large region where a local observer experiences M-theory in flat eleven dimensional space-time. By taking another solution in the same theory, one can create an arbitrarily large region where a local observer will experience type IIB string theory in flat ten dimensional space-time.
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Cited by 4 Pith papers
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The Fate of Black Hole-Induced Moduli Excursions in the Presence of Scalar Potentials
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A classical solution construction is proposed that places any chosen moduli-space point B inside an arbitrarily large, nearly flat region of an asymptotically flat string compactification that approaches any other poi...
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Adiabatic Deformations of Black Hole Moduli: II. The Magnetic GHS Family
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