Radius stabilization by constant boundary superpotentials in warped space
- 1. Department of Physics, Kobe University, Kobe 657-8501 (Japan)
- 2. Department of Physics, Tokyo Institute of Technology, Tokyo 152-8551 (Japan)
- 3. High Energy Physics Division, Department of Physical Sciences, University of Helsinki, and Helsinki Institute of Physics, P.O. Box 64, FIN-00014 Helsinki (Finland)
Description
A warped space model with a constant boundary superpotential has been an efficient model both to break supersymmetry and to stabilize the radius, when a hypermultiplet, a compensator, and a radion multiplet are taken into account. In such a model of radius stabilization, the radion and moduli masses, the gravitino mass, and the induced soft masses are studied. We find that a lighter physical mode composed of the radion and the moduli can have mass of the order of a TeV and that the gravitino mass can be of the order of 107 GeV. It is also shown that soft mass induced by the anomaly mediation can be of the order of 100 GeV and can be dominant compared to that mediated by bulk fields. Localized F-terms and D-terms are discussed as candidates for canceling the cosmological constant. We find that there is no flavor changing neutral current problem in a wide range of parameters
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.75.125014;
- arXiv
- arXiv:hep-th/0612071v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 75
- Journal Issue
- 12
- Journal Page Range
- p. 125014-125014.12
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38090849
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COSMOLOGICAL CONSTANT; GEV RANGE 100-1000; MASS; NEUTRAL CURRENTS; PEV RANGE; POTENTIALS; SPACE; STABILIZATION; SUPERSYMMETRY
- Descriptors DEC
- ALGEBRAIC CURRENTS; CURRENTS; ENERGY RANGE; GEV RANGE; SYMMETRY
Optional Information
- Notes
- (c) 2007 The American Physical Society