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Non-supersymmetric type I strings with zero vacuum energy

1999/04/30 by C. Angelantonj, Carlo Angelantonj, Ignatios Antoniadis +3 · 83 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Brane #Cosmological constant #Cosmology and Gravitation Theories #Degeneracy (biology) #Fermi Gamma-ray Space Telescope #Heterotic string theory #Massless particle #Noncommutative and Quantum Gravity Theories #Particle physics #Physics #Quantum mechanics #String (physics) #Supersymmetry #Supersymmetry breaking #Theoretical physics #Type (biology) #Vacuum energy #Zero (linguistics) #Zero-point energy #hep-th

paper · pdf · doi:10.1016/s0550-3213(99)00344-2

published in Nuclear Physics B 555(1-2), 116-134 (Elsevier BV) · 22 pages, TeX, harvmac. Minor corrections. Final version to appear on Nucl.Phys.B

arxiv created 1999/07/02 · openalex publication_date 1999/08/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We study open descendants of non-supersymmetric type IIB asymmetric (freely acting) orbifolds with zero cosmological constant. A generic feature of these models is that supersymmetry remains unbroken on the brane at all mass levels, while it is broken in the bulk in a way that preserves Fermi-Bose degeneracy in both the massless and massive (closed string) spectrum. This property remains valid in the heterotic dual of the type II model but only for the massless excitations. A possible application of these constructions concerns scenarios of low-energy supersymmetry breaking with large dimensions.

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