Self-dual nonsupersymmetric Type II String Compactifications
Journal Article
·
· Journal of High Energy Physics
It has recently been proposed that certain nonsupersymmetric type II orbifolds have vanishing perturbative contributions to the cosmological constant. We show that techniques of Sen and Vafa allow one to construct dual type II descriptions of these models (some of which have no weakly coupled heterotic dual). The dual type II models are given by the same orbifolds with the string coupling S and a T{sup 2} volume T exchanged. This allows us to argue that in various strongly coupled limits of the original type II models, there are weakly coupled duals which exhibit the same perturbative cancellations as the original models.
- Research Organization:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Organization:
- USDOE Director. Office of Science. Office of High Energy Physics. Contracts DE-AC03-76SF00098 and DE-AC03-76SF00515, OJI Award; National Science Foundation Grant PHY-94-97194; A.P. Sloan Foundation (US)
- DOE Contract Number:
- AC03-76SF00098
- OSTI ID:
- 836359
- Report Number(s):
- LBNL-42139; R&D Project: PTHOPS; TRN: US0500541
- Journal Information:
- Journal of High Energy Physics, Journal Issue: 11; Other Information: Submitted to Journal of High Energy Physics: No.11; Journal Publication Date: 02/12/1999; PBD: 17 Aug 1998
- Country of Publication:
- United States
- Language:
- English
Similar Records
GUT precursors and entwined SUSY: The phenomenology of stable nonsupersymmetric strings
Vacuum energy cancellation in a nonsupersymmetric string
A chiral {ital N}=1 type I vacuum in four dimensions and its heterotic dual
Journal Article
·
Fri Jun 01 00:00:00 EDT 2018
· Physical Review. D.
·
OSTI ID:836359
Vacuum energy cancellation in a nonsupersymmetric string
Journal Article
·
Sat May 01 00:00:00 EDT 1999
· Physical Review, D
·
OSTI ID:836359
A chiral {ital N}=1 type I vacuum in four dimensions and its heterotic dual
Journal Article
·
Mon Sep 01 00:00:00 EDT 1997
· Physical Review, D
·
OSTI ID:836359