Saltatory Relaxation of the Cosmological Constant

We modify and extend an earlier proposal by Brown and Teitelboim to relax the effective cosmological term by nucleation of branes coupled to a three-index gauge potential. Microscopic considerations from string/M theory suggest two major innovations in the framework. First, the dependence of brane p...

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Hauptverfasser: Feng, J, March-Russell, J, Sethi, S, Wilczek, F
Format: Journal article
Sprache:English
Veröffentlicht: 2000
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author Feng, J
March-Russell, J
Sethi, S
Wilczek, F
author_facet Feng, J
March-Russell, J
Sethi, S
Wilczek, F
author_sort Feng, J
collection OXFORD
description We modify and extend an earlier proposal by Brown and Teitelboim to relax the effective cosmological term by nucleation of branes coupled to a three-index gauge potential. Microscopic considerations from string/M theory suggest two major innovations in the framework. First, the dependence of brane properties on the compactification of extra dimensions may generate a very small quantized unit for jumps in the effective cosmological term. Second, internal degrees of freedom for multiply coincident branes may enhance tunneling rates by exponentially large density of states factors. These new features essentially alter the relaxation dynamics. By requiring stability on the scale of the lifetime of the universe, rather than absolute stability, we derive a non-trivial relation between the supersymmetry breaking scale and the value of the cosmological term. It is plausibly, though not certainly, satisfied in Nature.
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spelling oxford-uuid:4c54efb5-a7f8-480a-be3f-88691147c9472022-03-26T15:48:54ZSaltatory Relaxation of the Cosmological ConstantJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:4c54efb5-a7f8-480a-be3f-88691147c947EnglishSymplectic Elements at Oxford2000Feng, JMarch-Russell, JSethi, SWilczek, FWe modify and extend an earlier proposal by Brown and Teitelboim to relax the effective cosmological term by nucleation of branes coupled to a three-index gauge potential. Microscopic considerations from string/M theory suggest two major innovations in the framework. First, the dependence of brane properties on the compactification of extra dimensions may generate a very small quantized unit for jumps in the effective cosmological term. Second, internal degrees of freedom for multiply coincident branes may enhance tunneling rates by exponentially large density of states factors. These new features essentially alter the relaxation dynamics. By requiring stability on the scale of the lifetime of the universe, rather than absolute stability, we derive a non-trivial relation between the supersymmetry breaking scale and the value of the cosmological term. It is plausibly, though not certainly, satisfied in Nature.
spellingShingle Feng, J
March-Russell, J
Sethi, S
Wilczek, F
Saltatory Relaxation of the Cosmological Constant
title Saltatory Relaxation of the Cosmological Constant
title_full Saltatory Relaxation of the Cosmological Constant
title_fullStr Saltatory Relaxation of the Cosmological Constant
title_full_unstemmed Saltatory Relaxation of the Cosmological Constant
title_short Saltatory Relaxation of the Cosmological Constant
title_sort saltatory relaxation of the cosmological constant
work_keys_str_mv AT fengj saltatoryrelaxationofthecosmologicalconstant
AT marchrussellj saltatoryrelaxationofthecosmologicalconstant
AT sethis saltatoryrelaxationofthecosmologicalconstant
AT wilczekf saltatoryrelaxationofthecosmologicalconstant