TY - JOUR
T1 - Flux compactifications grow lumps
AU - Dahlen, Alex
AU - Zukowski, Claire
N1 - Publisher Copyright:
© 2014 American Physical Society.
PY - 2014/12/16
Y1 - 2014/12/16
N2 - The simplest flux compactifications are highly symmetric - a q-form flux is wrapped uniformly around an extra-dimensional q-sphere. In this paper, we investigate solutions that break the internal SO(q+1) symmetry down to SO(q)×Z2; we find a large number of such lumpy solutions, and show that often at least one of them has lower vacuum energy, larger entropy, and is more stable than the symmetric solution. We construct the phase diagram of lumpy solutions, and provide an interpretation in terms of an effective potential. Finally, we provide evidence that the perturbatively stable vacua have a nonperturbative instability to spontaneously sprout lumps. We give an estimate of the decay rate and argue that generically it is exponentially faster than all other known decays.
AB - The simplest flux compactifications are highly symmetric - a q-form flux is wrapped uniformly around an extra-dimensional q-sphere. In this paper, we investigate solutions that break the internal SO(q+1) symmetry down to SO(q)×Z2; we find a large number of such lumpy solutions, and show that often at least one of them has lower vacuum energy, larger entropy, and is more stable than the symmetric solution. We construct the phase diagram of lumpy solutions, and provide an interpretation in terms of an effective potential. Finally, we provide evidence that the perturbatively stable vacua have a nonperturbative instability to spontaneously sprout lumps. We give an estimate of the decay rate and argue that generically it is exponentially faster than all other known decays.
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U2 - 10.1103/PhysRevD.90.125013
DO - 10.1103/PhysRevD.90.125013
M3 - Article
AN - SCOPUS:84947118492
SN - 1550-7998
VL - 90
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 12
M1 - 125013
ER -