Radiativeϒ(1S)decays

Radiativeϒ(1S)decays

R. Fulton,M. Hempstead,T. Jensen,D. R. Johnson,H. Kagan,R. Kass,F. Morrow,J. Whitmore,W. -Y. Chen,J. Dominick,R. L. McIlwain,D. H. Miller,C. R. Ng,E. I. Shibata,W. -M. Yao,K. Sparks,E. H. Thorndike,M. S. Alam,N. Katayama,I. J. Kim,W. C. Li,X. C. Lou,C. R. Sun,D. Bortoletto,M. Goldberg,N. Horwitz,P. Lubrano,M. D. Mestayer,G. C. Moneti,V. Sharma,I. P. J. Shipsey,T. Skwarnicki,S. E. Csorna,T. Letson,I. C. Brock,T. Ferguson,Helmut Vogel,J. Alexander,Marina Artuso,C. Bebek,J. Byrd,K. Berkelman,E. Blucher,D. G. Cassel,E. Cheu,D. M. Coffman,T. Copie,G. Crawford,J. W. DeWire,P. S. Drell,R. Ehrlich,R. S. Galik,B. Gittelman,S. W. Gray,A. M. Halling,D. L. Hartill,B. K. Heltsley,J. Kandaswamy,Robert Kowalewski,D. L. Kreinick,Y. Kubota,J. D. Lewis,N. B. Mistry,James Mueller,R. Namjoshi,S. Nandi,E. Nordberg,C. O'Grady,D. Peterson,M. Pisharody,D. Riley,M. Sapper,A. Silverman,Sheldon Stone,H. Worden,M. Worris,A. J. Sadoff,P. Avery,D. Besson,L. Garren,J. Yelton,Themistocles Bowcock,K. Kinoshita,F. M. Pipkin,M. Procario,Richard Wilson,J. Wolinski,D. Xiao,P. Baringer,P. Haas,Ha Lam,A. Jawahery,C. H. Park,D. Perticone,Ronald Poling;R. Fulton;M. Hempstead;T. Jensen;D. R. Johnson;H. Kagan;R. Kass;F. Morrow;J. Whitmore;W. -Y. Chen;J. Dominick;R. L. McIlwain;D. H. Miller;C. R. Ng;E. I. Shibata;W. -M. Yao;K. Sparks;E. H. Thorndike;M. S. Alam;N. Katayama;I. J. Kim;W. C. Li;X. C. Lou;C. R. Sun;D. Bortoletto;M. Goldberg;N. Horwitz;P. Lubrano;M. D. Mestayer;G. C. Moneti;V. Sharma;I. P. J. Shipsey;T. Skwarnicki;S. E. Csorna;T. Letson;I. C. Brock;T. Ferguson;Helmut Vogel;J. Alexander;Marina Artuso;C. Bebek;J. Byrd;K. Berkelman;E. Blucher;D. G. Cassel;E. Cheu;D. M. Coffman;T. Copie;G. Crawford;J. W. DeWire;P. S. Drell;R. Ehrlich;R. S. Galik;B. Gittelman;S. W. Gray;A. M. Halling;D. L. Hartill;B. K. Heltsley;J. Kandaswamy;Robert Kowalewski;D. L. Kreinick;Y. Kubota;J. D. Lewis;N. B. Mistry;James Mueller;R. Namjoshi;S. Nandi;E. Nordberg;C. O'Grady;D. Peterson;M. Pisharody;D. Riley;M. Sapper;A. Silverman;Sheldon Stone;H. Worden;M. Worris;A. J. Sadoff;P. Avery;D. Besson;L. Garren;J. Yelton;Themistocles Bowcock;K. Kinoshita;F. M. Pipkin;M. Procario;Richard Wilson;J. Wolinski;D. Xiao;P. Baringer;P. Haas;Ha Lam;A. Jawahery;C. H. Park;D. Perticone;Ronald Poling;
physical review d 1990 Vol. 41 pp. 1401-1409
147
poling1990physicalradiativeϒ(1s)decays

Abstract

We report on a study of exclusive radiative decays of the ϒ(1S) resonance. We have considered decays into final states of the form ϒ→γn(h+h−), with (h+h−) denoting a charged-hadron pair (either π+π−, K+K−, or pp¯), and n denoting the number of such pairs in the event. We measure branching ratios for n=2, 3, and 4, and search for structure in the recoiling hadronic system. For the n=1 case, we present upper limits. No evidence is observed for two-body radiative decays of the ϒ(1S) meson in any of the above channels.

Citation

ID: 268713
Ref Key: poling1990physicalradiativeϒ(1s)decays
Use this key to autocite in SciMatic or Thesis Manager

References

Blockchain Verification

Account:
NFT Contract Address:
0x95644003c57E6F55A65596E3D9Eac6813e3566dA
Article ID:
268713
Unique Identifier:
10.1103/physrevd.41.1401
Network:
Scimatic Chain (ID: 481)
Loading...
Blockchain Readiness Checklist
Authors
Abstract
Journal Name
Year
Title
5/5
Creates 1,000,000 NFT tokens for this article
Token Features:
  • ERC-1155 Standard NFT
  • 1 Million Supply per Article
  • Transferable via MetaMask
  • Permanent Blockchain Record
Blockchain QR Code
Scan with Saymatik Web3.0 Wallet

Saymatik Web3.0 Wallet