A Search for Narrow States in Radiative Upsilicon Decays

A Search for Narrow States in Radiative Upsilicon Decays PDF Author: Stephen T. Lowe
Publisher:
ISBN:
Category :
Languages : en
Pages :

Get Book Here

Book Description

A Search for Narrow States in Radiative Upsilicon Decays

A Search for Narrow States in Radiative Upsilicon Decays PDF Author: Stephen T. Lowe
Publisher:
ISBN:
Category :
Languages : en
Pages :

Get Book Here

Book Description


A Search for Narrow States in Radiative Upsilon Decays

A Search for Narrow States in Radiative Upsilon Decays PDF Author: Stephen T. Lowe
Publisher:
ISBN:
Category : Mesons
Languages : en
Pages : 266

Get Book Here

Book Description


A Search for Narrow States in Radiative Upsilon Decays

A Search for Narrow States in Radiative Upsilon Decays PDF Author:
Publisher:
ISBN:
Category :
Languages : en
Pages :

Get Book Here

Book Description
A search for new states produced in radiative UPSILON(1S) decays is accomplished by observing the inclusive photon energy spectrum. A narrow resonance in the energy spectrum indicates the existence of a new state X produced by the process UPSILON .-->. .gamma. X. The analysis is based on approximately 0.44 x 106 UPSILON(1S) events produced at the DORIS II ee− storage ring. These data were collected with the Crystal Ball detector between April 1983 and May 1986. This analysis finds no evidence for a new state, so upper limits on the branching ratio BR(UPSILON .-->. .gamma. X) are derived, assuming the state X decays primarily to high-multiplicity hadronic final states. In particular, if the state X were a minimal Higgs particle, its primary decay mode would be to the heaviest fermion-antifermion pair energetically available. For the radiative UPSILON(1S) decays studied here, the heavy fermions would be c anti c or s anti s quark states, over most of the relevant Higgs' mass range. The resulting upper limit for BR(UPSILON(1S) .-->. .gamma. X) is highly energy dependent but for X mass between 1.5 GeV and 8.0 GeV, the 90% confidence level upper limit is better than 8.0 x 10−4. For a Higgs' mass near 5.0 GeV, the upper limit is about 2.0 x 10−4 which is approximately equal to the lowest order calculation for the Wilczek mechanism. The Wilczek calculation with QCD radiative corrections predict branching ratios below the limits set here for all Higgs' masses.

Search for narrow states coupling to _t63 pairs in radiative _t63 decays

Search for narrow states coupling to _t63 pairs in radiative _t63 decays PDF Author:
Publisher:
ISBN:
Category :
Languages : de
Pages :

Get Book Here

Book Description


Evidence for a narrow massive state in the radiative decays of the upsilon

Evidence for a narrow massive state in the radiative decays of the upsilon PDF Author:
Publisher:
ISBN:
Category :
Languages : de
Pages :

Get Book Here

Book Description


Search for Narrow States Coupling to [tau] Pairs in Radiative [upsilon] Decays

Search for Narrow States Coupling to [tau] Pairs in Radiative [upsilon] Decays PDF Author: Argus Corporation
Publisher:
ISBN:
Category :
Languages : en
Pages : 7

Get Book Here

Book Description


Evidence for a Narrow Massive State in the Radiative Decays of the Upsilon

Evidence for a Narrow Massive State in the Radiative Decays of the Upsilon PDF Author: Chrystal Ball Collaboration
Publisher:
ISBN:
Category :
Languages : en
Pages : 13

Get Book Here

Book Description


Upper Limits on Inclusive Branching Fractions to Narrow States in Radiative J/psi Decays

Upper Limits on Inclusive Branching Fractions to Narrow States in Radiative J/psi Decays PDF Author: Gregory P. Dubois
Publisher:
ISBN:
Category :
Languages : en
Pages : 248

Get Book Here

Book Description


Search for Narrow States Coupling to Τ Pairs in Radiative Υ Decays

Search for Narrow States Coupling to Τ Pairs in Radiative Υ Decays PDF Author:
Publisher:
ISBN:
Category :
Languages : en
Pages :

Get Book Here

Book Description


Energy Research Abstracts

Energy Research Abstracts PDF Author:
Publisher:
ISBN:
Category : Power resources
Languages : en
Pages : 1180

Get Book Here

Book Description