Published April 20, 2009
| Version v1
Journal article
Invisible Decays of Supersymmetric Higgs Bosons
- 1. Fac. de Cs. Fisico Matematicas, Benemerita Universidad Autonoma de Puebla, Apdo. Postal 1152, 72570 Puebla, Pue. (Mexico)
- 2. Fac. de Cs. de la Electronica, Benemerita Universidad Autonoma de Puebla, Apdo. Postal 157, 72570 Puebla, Pue. (Mexico)
Description
We study the detection of the complete spectrum of Higgs bosons of the minimal supersymmetric standard model, through their decays into chargino (χ-tildei±) and neutralinos (χ-tildeio), for several parametric scenarios. In the minimal supersymmetric model there are two charginos and four neutralinos, and the Higgs boson spectrum contains three neutral scalars, two CP-even (h0 and H0 with mH0>mh0) and one CP-odd (A0, with mA0 as a free parameter); as well as a charged pair (H±). An interesting signal comes from the decays of the Higgs bosons into invisible SUSY modes (h0, H0,A0→χ-tilde1oχ-tilde1o), which could be detected at present and future high energy machines.
Additional details
Identifiers
- DOI
- 10.1063/1.3131584;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1116
- Journal Issue
- 1
- Journal Page Range
- p. 402-406
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 13. Mexican school of particles and fields
- Dates
- 2-11 Oct 2008
- Place
- Hermosillo (Mexico); San Carlos (Mexico)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41045275
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CP INVARIANCE; HIGGS BOSONS; PARTICLE DECAY; PARTICLE IDENTIFICATION; SCALARS; STANDARD MODEL; SUPERSYMMETRY
- Descriptors DEC
- BOSONS; DECAY; ELEMENTARY PARTICLES; FIELD THEORIES; GRAND UNIFIED THEORY; INVARIANCE PRINCIPLES; MATHEMATICAL MODELS; PARTICLE MODELS; POSTULATED PARTICLES; QUANTUM FIELD THEORY; SYMMETRY; UNIFIED GAUGE MODELS
Optional Information
- Notes
- (c) 2009 American Institute of Physics