Published August 15, 2011
| Version v1
Journal article
Production of a composite Higgs boson
Creators
- 1. Department of Physics and Astronomy, Northwestern University, Evanston, Illinois 60208 (United States)
- 2. High Energy Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
- 3. Institut de Theorie des Phenomenes Physiques, EPFL, CH-1015 Lausanne (Switzerland)
Description
We present a model-independent prescription for computing the gluon fusion production rate of a composite Higgs boson, which arises as a pseudo-Nambu-Goldstone boson, using effective Lagrangians. The calculation incorporates three different effects due to the composite nature of the Higgs, some of which were neglected previously. We apply the prescription to models with and without the collective breaking mechanism. In sharp contrast with the case of a fundamental Higgs scalar, the rate only depends on the decay constant f and is not sensitive to masses of new particles. After including electroweak constraints, there is a substantial reduction in the rate, in the range of 10%-30% or greater.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.84.045019;
- arXiv
- arXiv:1010.2753v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 84
- Journal Issue
- 4
- Journal Page Range
- p. 045019-045019.13
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43083255
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- GLUONS; GOLDSTONE BOSONS; HIGGS BOSONS; HIGGS MODEL; LAGRANGIAN FUNCTION; LIMITING VALUES; MASS; PARTICLE DECAY; PARTICLE PRODUCTION; REDUCTION; WEINBERG-SALAM GAUGE MODEL
- Descriptors DEC
- BOSONS; CHEMICAL REACTIONS; DECAY; ELEMENTARY PARTICLES; FIELD THEORIES; FUNCTIONS; MATHEMATICAL MODELS; PARTICLE MODELS; POSTULATED PARTICLES; QUANTUM FIELD THEORY; UNIFIED GAUGE MODELS; UNIFIED-FIELD THEORIES
Optional Information
- Notes
- (c) 2011 American Institute of Physics