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Interpretation ofDsJ(2632)+,Ds1(2700)±,DsJ*(2860)+, andDsJ(3040)+

2009/08/26 by Bing Chen, Deng-Xia Wang, Ailin Zhang
Medicine · Physics and Astronomy · #Medical Imaging Techniques and Applications #Quantum Chromodynamics and Particle Interactions #Radioactive Decay and Measurement Techniques #hep-ex #hep-ph

paper · pdf · doi:10.1103/physrevd.80.071502

published as Phys.Rev.D80:071502,2009 · 4 pages, 2 tables, no figures, RevTex

arxiv created 2009/08/26 · openalex publication_date 2009/10/23 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Ds mesons are investigated in a semiclassic flux tube model where the spin-orbit interaction is taken into account. Spectrum of D-wave Ds is predicted. The predicted spectrum is much lower than most previous predictions. Analysis of some Ds candidates is made. DsJ(2632)+ may be a 1^\ensuremath- jP=(3)/(2)^\ensuremath- or 1 3D1) orbitally excited Ds meson if it really exists. Ds1(2700)^\ifmmode±\else\textpm\fi is very possibly the first radially excited 1^\ensuremath- (jP=(1)/(2)^\ensuremath- or 2 3S1) Ds meson [the first radial excitation of Ds^\ensuremath⋆\ifmmode±\else\textpm\fi(2112)0]. DsJ^\ensuremath⋆(2860)+ should be a 3^\ensuremath- (jP=(5)/(2)^\ensuremath- or 1 3D3) orbitally excited Ds meson, and DsJ(3040)+ is the first radially excited 1+ (jP=(1)/(2)+) Ds meson. Our conclusions are consistent with the latest BABAR experiment.

Citations