Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Strong dynamics at the muon collider: Working group report

Conference · · AIP Conf.Proc.
DOI:https://doi.org/10.1063/1.56234· OSTI ID:603071
New strong dynamics at the energy scale ~ 1 TeV is an attractive and elegant theoretical ansatz for the origin of electroweak symmetry breaking. We review here the theoretical models for strong dynamics, particularly, technicolor theories and their low energy signatures. We emphasize that the fantastic beam energy resolution (sigma_E/E ~10^{-4}) expected at the first muon collider (sqrt{s} = 100-500 GeV) allows the possibility of resolving some extraordinarily narrow technihadron resonances and, Higgs-like techniscalars produced in the s-channel. Investigating indirect probes for strong dynamics such as search for muon compositeness, we find that the muon colliders provide unparallel reaches. A big muon collider (sqrt{s} =3-4 TeV) would be a remarkable facility to study heavy technicolor particles such as the topcolor Z', to probe the dynamics underlying fermion masses and mixings and to fully explore the strongly interacting electroweak sector.
Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
DOE Contract Number:
AC02-07CH11359
OSTI ID:
603071
Report Number(s):
FERMILAB-CONF-98-072; arXiv:hep-ph/9803468; oai:inspirehep.net:454162
Conference Information:
Journal Name: AIP Conf.Proc. Journal Issue: 1 Journal Volume: 435
Country of Publication:
United States
Language:
English

Similar Records

Strong dynamics at the muon collider: Working group report
Journal Article · Sat Aug 01 00:00:00 EDT 1998 · AIP Conference Proceedings · OSTI ID:663623

Narrow Technihadron Production at the First Muon Collider
Journal Article · Mon Jun 01 00:00:00 EDT 1998 · Physical Review Letters · OSTI ID:636195

The Muon Collider
Journal Article · Wed Apr 30 00:00:00 EDT 2025 · No journal information · OSTI ID:2568602