Abstract

It has recently been appreciated that the conifold modulus plays an important role in string-phenomenological set-ups involving warped throats, both by imposing constraints on model building and for obtaining a 10-dimensional picture of SUSY-breaking. In this note, we point out that the stability of the conifold modulus furthermore prevents large super-Planckian axion monodromy field ranges caused by brane-flux decay processes down warped throats. Our findings imply a significant challenge for concrete string theory embeddings of the inflationary flux-unwinding scenario.

Highlights

  • KK modes cannot really be decoupled from the 4d effective field theory (EFT) their couplings might be rather harmless and they could just behave as spectators [14]

  • We find that a large number of monodromies, and a large field displacement, cannot be achieved without destabilising the geometry along the direction parametrised by the conifold modulus

  • In this note we have argued that axion monodromies related to brane-flux transitions down warped throats come with exponentially suppressed field ranges as given by equation (4.13)

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Summary

The conifold and brane-flux moduli

We introduce the basic ingredients required for our later analysis of instabilities of warped throats associated to conifold singularities. As many of the ingredients are well known, we will be rather concise and refer to the appropriate literature for further details

The conifold modulus
SUSY breaking and the conifold instability
The brane-flux transition modulus
Uplifting 5-brane runaway
Axion monodromies and field range bounds
General considerations
Anti-brane annihilation
Brane creation from fluxes
Discussion
A Mass ratio of the conifold and brane-flux moduli
Full Text
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