Download presentation
Presentation is loading. Please wait.
1
Study of New Hadron Spectroscopy at BESIII
Liu Fang (IHEP) for BESIII Collaboration The 9th National Workshop for Heavy Flavors and CP Violation Hangzhou, Zhejiang, China
2
OUTLINE Latest results on new hadron spectroscopy Introduction
pp mass threshold enhancement in J/ and ’ radiative decays Confirmation of X(1835) and observation of two new structures Observation X(1870) in J/(+-) Summary
3
Satellite view of BEPCII /BESIII
LINAC South 2004: start BEPCII construction 2008: test run of BEPCII 2009-now: BECPII/BESIII data taking BESIII detector
4
BEPCII storage rings Beam energy: 1.0-2.3 GeV Design Luminosity:
1×1033 cm-2s-1 Optimum energy: 1.89 GeV Energy spread: 5.16 ×10-4 No. of bunches: 93 Bunch length: 1.5 cm Total current: 0.91 A Circumference: 237m
5
BES Detector
6
Data samples So far BESIII has collected : BESIII will also collect:
2009: 225 Million J/(4 BESII) 2009: 106 Million ’ (4 CLEOC) : 2.9 fb1 (3770) (3.5 CLEO-c 0.818fb1) - May 2011: MeV (one month) for Ds and XYZ spectroscopy BESIII will also collect: more J/, ’, (3770) data at higher energies (for XYZ searches, R scan and Ds physics)
8
Light hadron QCD allows different type of hadrons:
9
Observation of pp mass threshold enhancement
@BESIII @BESIII @BESIII
10
Observation of mass threshold enhancement @ BESII
3-body phase space BESII X(1860) theoretical speculation: bound state (baryonium) FSI effect …… 0.1 0.2 0.3 acceptance Mpp-2mp (GeV) M= MeV/c2 G < 30 MeV/c2 (90% CL) PRL 91 (2003) 10 10
11
Several non-observations
PRD 73 (2006) EPJ C53 (2008) 15 No significant signal of X(1860) near threshold found (only 2 significance) PRL 99 (2007) Mpp (GeV) 11 11
12
Observation of pp mass threshold enhancement at BESIII
0.1 0.2 0.3 M= MeV/c2 G < 38 MeV/c2 (90% CL) M= MeV/c2 G < 30 MeV/c2 (90% CL) PRL 91 (2003) Chinese Physics C 34, 421 (2010)
13
PWA on the pp mass threshold structure in
BESIII X(pp) Preliminary results ηc Evident narrow ppbar mass threshold enhancement Partial Wave Analysis (PWA): Concentrate on dealing with the mass threshold structure, especially to determine the JPC (M(pp)<2.3GeV) . Convariant tensor amplitudes (S. Dulat and B. S. Zou, Eur.Phys.J A 26:125, 2005). Include the Juich-FSI effect (A. Sirbirtsen et al. Phys.Rev.D 71:054010, 2005). 13
14
PWA results and projections in
Preliminary results
15
Measurement for X(1860) >6.8σ better than other Jpc assignments.
PWA results are carefully checked from different aspects: Contribution of additional resonances Solution with different combinations Different background levels and fitting mass ranges Different BW formula … … All uncertainties are considered as systematic errors Different FSI models Model dependent uncertainty Spin-parity, mass, width and B.R. of X(1860): Preliminary results >6.8σ better than other Jpc assignments.
16
PWA on the pp mass threshold structure in
Preliminary results BESIII χcJ Obviously different line shape of ppbar mass spectrum near threshold from that in J/ψ decays ηc PWA results: PWA Projection: Significance of X(pp) is larger than 6.9σ. The production ratio R: It is suppressed compared with “12% rule”. first measurement
17
Confirmation of X(1835) in and observation of two new structures
at BESIII
18
X(1835) at BESII PRL 95,262001(2005) LQCD predicts the 0-+ glueball mass is ~2.3GeV. A 0-+ glueball may have similar property as c (mainly decay into ). J/+- was studied with 58M Need to confirm X(1835) with BESIII ~225M J/ data !!! 18 18
19
Mass spectrum of X(1835) X(1835) and c are evident.
BES III BES III Combination for to +- and X(1835) and c are evident. Two additional structures are observed at M~2.1GeV and 2.3GeV There maybe some f1(1510). X(2370) X(2120)
20
Fitting for the combined mass spectrum
Fitting with four resonances (acceptance weighted BW gauss) Three background components: Contribution from non-h’ events estimated by h’ mass sideband Contribution from with re-weighting method Contribution from “PS background” Red line: estimated contribution of ①+ ② Black line: total background Stat. sig. is conservatively estimated: fit range, background shape, contribution of extra resonances BES III
21
X(1835) , X(2120), X(2370) at BESIII BESIII fit results:
Resonance M( MeV/c2) ( MeV/c2) Stat.Sig. X(1835) 1836.5± 190.1± >20σ X(2120) 2122.4± 83± 7.2σ X(2370) 2376.3± 83± 6.4σ For the X(1835): BESIII X(1835) consistent with 0+ PWA is needed to understand these structures. 21
22
Summary of X(1835), X(2120) & X(2370) in J/(’+-)
X(1835) resonance is confirmed at BESIII, but the width is significantly larger than that measured at BESII with one resonance in the fit. Two new resonances, X(2120) and X(2370), are observed with significances larger than 7.2 and 6.4 respectively. PWA is needed not only to determine the spin-parities of above three resonances, but also to make more precise measurements on masses, widths and BRs by considering possible interferences among them.
23
Observation X(1870) in J/X, Xa0(980)(+-)
X(1835) observed at BESII and then confirmed at BESIII in J/→γπ+π-η´ theoretical interpretations: pseudoscalar glueball, / excited states .. study of its production in hadronic decays to our surprise, we observed a new structure around 1.87 GeV
24
X(1870) in J/X, Xa0(980) a0(980) In addition to the well-known ’, f1(1285) and (1405), an unknown structure (denoted as X(1870)) around 1.87GeV/c2 is observed. The f1(1285), (1405) and X(1870) primarily decay via a0(980)± mode. M(+) M() With a0(980): Veto a0(980): M(+) non-a0(980) M(a0(980))
25
Fitting results of X(1870) Fitting with three resonances (acceptance weighted BW Gauss) Background component described by Polynomial function X(1870): 7.2 f1(1285) (1405) Contribution from non- and/or non-a0(980) BG events Contribution from J/b1(1235)a0(980) Contribution from “PS” process of J/a0(980) M(a0(980)) BR(J/X, X )
26
Summary of X(1870) in J/(+-)
BESIII arxiv : Accepted by PRL.
27
Summary and Prospects Huge data samples collected for charmonium decays at BESIII. A lot of results have been obtained, The spin-parity of the pp mass threshold enhancement in J/γ pp was first determined as 0-+ Confirmation of X(1835) in J/ + and observation of two new structures X(2120) and X(2370) in J/ decays Observation of new structure X(1870) in J/ We expect more exciting results in the coming years from BESIII.
28
many thanks for your attention !
Similar presentations
© 2024 SlidePlayer.com. Inc.
All rights reserved.