skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Bounds on the mass of W sub R and the W sub L - W sub R mixing angle. zeta. in general SU(2) sub L times SU(2) sub R times U(1) models

Journal Article · · Physical Review (Section) D: Particles and Fields; (USA)
;  [1]
  1. Department of Physics, University of Pennsylvania, Philadelphia, Pennsylvania 19104 (US)

We consider the phenomenological constraints on the mass {ital M}{sub {ital R}} and the {ital W}{sub {ital L}}-{ital W}{sub {ital R}} mixing angle {zeta} in a very general class of SU(2){sub {ital L}}{times}SU(2){sub {ital R}}{times}U(1) models. In particular, almost no model-dependent assumptions are made concerning left-right symmetry or the Higgs structure of the theory, which means that {ital U}{sup {ital R}}, the mixing matrix for right-handed quarks, is unrelated to the left-handed Cabibbo-Kobayashi-Maskawa matrix {ital U}{sup {ital L}}. We consider a number of possibilities for the neutrinos occurring in right-handed currents, including (a) heavy Majorana neutrinos, (b) heavy Dirac neutrinos, (c) intermediate-mass (10--100 MeV) neutrinos, and (d) light neutrinos (e.g., the Dirac partners of the ordinary left-handed neutrinos). For each case we utilize relevant constraints from the {ital K}{sub {ital L}}-{ital K}{sub {ital S}} mass difference, {ital B}{sub {ital d}}{bar B}{sub d} oscillations, the {ital b} semileptonic branching ratio and decay rate, neutrinoless double-beta decay, theoretical relations between mass and mixing, universality, nonleptonic kaon decays, muon decay, and astrophysical constraints from nucleosynthesis and SN 1987A. As is to be expected the limits on {ital M}{sub {ital R}} are considerably weaker than for the special case of manifest or pseudomanifest left-right symmetry ({ital M}{sub {ital R}}{gt}1.4 TeV). In fact, if extreme fine-tuning is allowed the {ital W}{sub {ital R}} could be as light as the ordinary {ital W}{sub {ital L}}. However, with reasonable restrictions on fine-tuning one obtains {ital M}{sub {ital R}}{gt}300 GeV for {ital g}{sub {ital R}}=g{sub L}, with more stringent limits holding for most of parameter space.

OSTI ID:
5554335
Journal Information:
Physical Review (Section) D: Particles and Fields; (USA), Vol. 40:5; ISSN 0556-2821
Country of Publication:
United States
Language:
English

Similar Records

K/sub L/. --> mu. e in SU(2)/sub L/ x U(1) and SU(2)/sub L/ x SU(2)/sub R/ x U(1) models with large neutrino masses
Journal Article · Tue Nov 01 00:00:00 EST 1988 · Phys. Rev. D; (United States) · OSTI ID:5554335

Low-mass right-handed gauge bosons, proton decay, and other observable predictions in SU(8){sub {ital L}}{times}SU(8){sub {ital R}} and SU(16)
Journal Article · Sat Jul 01 00:00:00 EDT 1995 · Physical Review, D · OSTI ID:5554335

Determination of g sub R / g sub L in left-right symmetric models at hadron colliders
Journal Article · Mon May 11 00:00:00 EDT 1992 · Physical Review Letters; (United States) · OSTI ID:5554335