Contents lists available atScienceDirect
Physics
Letters
B
www.elsevier.com/locate/physletb
Measurement
of
the
branching
fractions
of
D
+
s
→
η
X and
D
+
s
→
η
ρ
+
in
e
+
e
−
→
D
+
s
D
−
s
BESIII
Collaboration
M. Ablikim
a,
M.N. Achasov
i,
6,
X.C. Ai
a,
O. Albayrak
e,
M. Albrecht
d,
D.J. Ambrose
av,
A. Amoroso
az,
bb,
F.F. An
a,
Q. An
aw,
1,
J.Z. Bai
a,
R. Baldini Ferroli
t,
Y. Ban
ag,
D.W. Bennett
s,
J.V. Bennett
e,
M. Bertani
t,
D. Bettoni
v,
J.M. Bian
au,
F. Bianchi
az,
bb,
E. Boger
y,
4,
I. Boyko
y,
R.A. Briere
e,
H. Cai
bd,
X. Cai
a,
1,
O. Cakir
ap,
2,
A. Calcaterra
t,
G.F. Cao
a,
S.A. Cetin
aq,
J.F. Chang
a,
1,
G. Chelkov
y,
4,
5,
G. Chen
a,
H.S. Chen
a,
H.Y. Chen
b,
J.C. Chen
a,
M.L. Chen
a,
1,
S.J. Chen
ae,
X. Chen
a,
1,
X.R. Chen
ab,
Y.B. Chen
a,
1,
H.P. Cheng
q,
X.K. Chu
ag,
G. Cibinetto
v,
H.L. Dai
a,
1,
J.P. Dai
aj,
A. Dbeyssi
n,
D. Dedovich
y,
Z.Y. Deng
a,
A. Denig
x,
I. Denysenko
y,
M. Destefanis
az,
bb,
F. De Mori
az,
bb,
Y. Ding
ac,
C. Dong
af,
J. Dong
a,
1,
L.Y. Dong
a,
M.Y. Dong
a,
1,
S.X. Du
bf,
P.F. Duan
a,
E.E. Eren
aq,
J.Z. Fan
ao,
J. Fang
a,
1,
S.S. Fang
a,
X. Fang
aw,
1,
Y. Fang
a,
L. Fava
ba,
bb,
F. Feldbauer
x,
G. Felici
t,
C.Q. Feng
aw,
1,
E. Fioravanti
v,
M. Fritsch
n,
x,
C.D. Fu
a,
Q. Gao
a,
X.Y. Gao
b,
Y. Gao
ao,
Z. Gao
aw,
1,
I. Garzia
v,
C. Geng
aw,
1,
K. Goetzen
j,
W.X. Gong
a,
1,
W. Gradl
x,
M. Greco
az,
bb,
M.H. Gu
a,
1,
Y.T. Gu
l,
Y.H. Guan
a,
A.Q. Guo
a,
L.B. Guo
ad,
Y. Guo
a,
Y.P. Guo
x,
Z. Haddadi
aa,
A. Hafner
x,
S. Han
bd,
Y.L. Han
a,
X.Q. Hao
o,
F.A. Harris
at,
K.L. He
a,
Z.Y. He
af,
T. Held
d,
Y.K. Heng
a,
1,
Z.L. Hou
a,
C. Hu
ad,
H.M. Hu
a,
J.F. Hu
az,
bb,
T. Hu
a,
1,
Y. Hu
a,
G.M. Huang
f,
G.S. Huang
aw,
1,
H.P. Huang
bd,
J.S. Huang
o,
X.T. Huang
ai,
Y. Huang
ae,
T. Hussain
ay,
Q. Ji
a,
Q.P. Ji
af,
X.B. Ji
a,
X.L. Ji
a,
1,
L.L. Jiang
a,
L.W. Jiang
bd,
X.S. Jiang
a,
1,
X.Y. Jiang
af,
J.B. Jiao
ai,
Z. Jiao
q,
D.P. Jin
a,
1,
S. Jin
a,
T. Johansson
bc,
A. Julin
au,
N. Kalantar-Nayestanaki
aa,
X.L. Kang
a,
X.S. Kang
af,
M. Kavatsyuk
aa,
B.C. Ke
e,
P. Kiese
x,
R. Kliemt
n,
B. Kloss
x,
O.B. Kolcu
aq,
9,
B. Kopf
d,
M. Kornicer
at,
W. Kühn
z,
A. Kupsc
bc,
J.S. Lange
z,
M. Lara
s,
P. Larin
n,
C. Leng
bb,
C. Li
bc,
C.H. Li
a,
Cheng Li
aw,
1,
D.M. Li
bf,
F. Li
a,
1,
G. Li
a,
H.B. Li
a,
J.C. Li
a,
Jin Li
ah,
K. Li
m,
K. Li
ai,
Lei Li
c,
P.R. Li
as,
T. Li
ai,
W.D. Li
a,
W.G. Li
a,
X.L. Li
ai,
X.M. Li
l,
X.N. Li
a,
1,
X.Q. Li
af,
Z.B. Li
an,
H. Liang
aw,
1,
Y.F. Liang
al,
Y.T. Liang
z,
G.R. Liao
k,
D.X. Lin
n,
B.J. Liu
a,
C.X. Liu
a,
F.H. Liu
ak,
Fang Liu
a,
Feng Liu
f,
H.B. Liu
l,
H.H. Liu
p,
H.H. Liu
a,
H.M. Liu
a,
J. Liu
a,
J.B. Liu
aw,
1,
J.P. Liu
bd,
J.Y. Liu
a,
K. Liu
ao,
K.Y. Liu
ac,
L.D. Liu
ag,
P.L. Liu
a,
∗
,
1,
Q. Liu
as,
S.B. Liu
aw,
1,
X. Liu
ab,
X.X. Liu
as,
Y.B. Liu
af,
Z.A. Liu
a,
1,
Zhiqiang Liu
a,
Zhiqing Liu
x,
H. Loehner
aa,
X.C. Lou
a,
1,
8,
H.J. Lu
q,
J.G. Lu
a,
1,
R.Q. Lu
r,
Y. Lu
a,
Y.P. Lu
a,
1,
C.L. Luo
ad,
M.X. Luo
be,
T. Luo
at,
X.L. Luo
a,
1,
M. Lv
a,
X.R. Lyu
as,
F.C. Ma
ac,
H.L. Ma
a,
L.L. Ma
ai,
Q.M. Ma
a,
T. Ma
a,
X.N. Ma
af,
X.Y. Ma
a,
1,
F.E. Maas
n,
M. Maggiora
az,
bb,
Y.J. Mao
ag,
Z.P. Mao
a,
S. Marcello
az,
bb,
J.G. Messchendorp
aa,
J. Min
a,
1,
T.J. Min
a,
R.E. Mitchell
s,
X.H. Mo
a,
1,
Y.J. Mo
f,
C. Morales Morales
n,
K. Moriya
s,
N.Yu. Muchnoi
i,
6,
H. Muramatsu
au,
Y. Nefedov
y,
F. Nerling
n,
I.B. Nikolaev
i,
6,
Z. Ning
a,
1,
S. Nisar
h,
S.L. Niu
a,
1,
X.Y. Niu
a,
S.L. Olsen
ah,
Q. Ouyang
a,
1,
S. Pacetti
u,
P. Patteri
t,
M. Pelizaeus
d,
H.P. Peng
aw,
1,
K. Peters
j,
J. Pettersson
bc,
J.L. Ping
ad,
R.G. Ping
a,
R. Poling
au,
V. Prasad
a,
Y.N. Pu
r,
M. Qi
ae,
S. Qian
a,
1,
C.F. Qiao
as,
L.Q. Qin
ai,
N. Qin
bd,
X.S. Qin
a,
Y. Qin
ag,
Z.H. Qin
a,
1,
J.F. Qiu
a,
K.H. Rashid
ay,
C.F. Redmer
x,
H.L. Ren
r,
M. Ripka
x,
G. Rong
a,
Ch. Rosner
n,
X.D. Ruan
l,
http://dx.doi.org/10.1016/j.physletb.2015.09.059
0370-2693/©2015TheAuthors.PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense(http://creativecommons.org/licenses/by/4.0/).Fundedby SCOAP3.
V. Santoro
v,
A. Sarantsev
y,
7,
M. Savrié
w,
K. Schoenning
bc,
S. Schumann
x,
W. Shan
ag,
M. Shao
aw,
1,
C.P. Shen
b,
P.X. Shen
af,
X.Y. Shen
a,
H.Y. Sheng
a,
W.M. Song
a,
X.Y. Song
a,
S. Sosio
az,
bb,
S. Spataro
az,
bb,
G.X. Sun
a,
J.F. Sun
o,
S.S. Sun
a,
Y.J. Sun
aw,
1,
Y.Z. Sun
a,
Z.J. Sun
a,
1,
Z.T. Sun
s,
C.J. Tang
al,
X. Tang
a,
I. Tapan
ar,
E.H. Thorndike
av,
M. Tiemens
aa,
M. Ullrich
z,
I. Uman
aq,
G.S. Varner
at,
B. Wang
af,
B.L. Wang
as,
D. Wang
ag,
D.Y. Wang
ag,
K. Wang
a,
1,
L.L. Wang
a,
L.S. Wang
a,
M. Wang
ai,
P. Wang
a,
P.L. Wang
a,
S.G. Wang
ag,
W. Wang
a,
1,
X.F. Wang
ao,
Y.D. Wang
n,
Y.F. Wang
a,
1,
Y.Q. Wang
x,
Z. Wang
a,
1,
Z.G. Wang
a,
1,
Z.H. Wang
aw,
1,
Z.Y. Wang
a,
T. Weber
x,
D.H. Wei
k,
J.B. Wei
ag,
P. Weidenkaff
x,
S.P. Wen
a,
U. Wiedner
d,
M. Wolke
bc,
L.H. Wu
a,
Z. Wu
a,
1,
L.G. Xia
ao,
Y. Xia
r,
D. Xiao
a,
Z.J. Xiao
ad,
Y.G. Xie
a,
1,
Q.L. Xiu
a,
1,
G.F. Xu
a,
L. Xu
a,
Q.J. Xu
m,
Q.N. Xu
as,
X.P. Xu
am,
L. Yan
aw,
1,
W.B. Yan
aw,
1,
W.C. Yan
aw,
1,
Y.H. Yan
r,
H.J. Yang
aj,
H.X. Yang
a,
L. Yang
bd,
Y. Yang
f,
Y.X. Yang
k,
H. Ye
a,
M. Ye
a,
1,
M.H. Ye
g,
J.H. Yin
a,
B.X. Yu
a,
1,
C.X. Yu
af,
H.W. Yu
ag,
J.S. Yu
ab,
C.Z. Yuan
a,
W.L. Yuan
ae,
Y. Yuan
a,
A. Yuncu
aq,
3,
A.A. Zafar
ay,
A. Zallo
t,
Y. Zeng
r,
B.X. Zhang
a,
B.Y. Zhang
a,
1,
C. Zhang
ae,
C.C. Zhang
a,
D.H. Zhang
a,
H.H. Zhang
an,
H.Y. Zhang
a,
1,
J.J. Zhang
a,
J.L. Zhang
a,
J.Q. Zhang
a,
J.W. Zhang
a,
1,
J.Y. Zhang
a,
J.Z. Zhang
a,
K. Zhang
a,
L. Zhang
a,
S.H. Zhang
a,
X.Y. Zhang
ai,
Y. Zhang
a,
Y.N. Zhang
as,
Y.H. Zhang
a,
1,
Y.T. Zhang
aw,
1,
Yu Zhang
as,
Z.H. Zhang
f,
Z.P. Zhang
aw,
Z.Y. Zhang
bd,
G. Zhao
a,
J.W. Zhao
a,
1,
J.Y. Zhao
a,
J.Z. Zhao
a,
1,
Lei Zhao
aw,
1,
Ling Zhao
a,
M.G. Zhao
af,
Q. Zhao
a,
Q.W. Zhao
a,
S.J. Zhao
bf,
T.C. Zhao
a,
Y.B. Zhao
a,
1,
Z.G. Zhao
aw,
1,
A. Zhemchugov
y,
4,
B. Zheng
ax,
J.P. Zheng
a,
1,
W.J. Zheng
ai,
Y.H. Zheng
as,
B. Zhong
ad,
L. Zhou
a,
1,
Li Zhou
af,
X. Zhou
bd,
X.K. Zhou
aw,
1,
X.R. Zhou
aw,
1,
X.Y. Zhou
a,
K. Zhu
a,
K.J. Zhu
a,
1,
S. Zhu
a,
X.L. Zhu
ao,
Y.C. Zhu
aw,
1,
Y.S. Zhu
a,
Z.A. Zhu
a,
J. Zhuang
a,
1,
L. Zotti
az,
bb,
B.S. Zou
a,
J.H. Zou
aaInstituteofHighEnergyPhysics,Beijing100049,People’sRepublicofChina bBeihangUniversity,Beijing100191,People’sRepublicofChina
cBeijingInstituteofPetrochemicalTechnology,Beijing102617,People’sRepublicofChina dBochumRuhr-University,D-44780Bochum,Germany
eCarnegieMellonUniversity,Pittsburgh,PA 15213,USA
fCentralChinaNormalUniversity,Wuhan430079,People’sRepublicofChina
gChinaCenterofAdvancedScienceandTechnology,Beijing100190,People’sRepublicofChina
hCOMSATSInstituteofInformationTechnology,Lahore,DefenceRoad,OffRaiwindRoad,54000Lahore,Pakistan iG.I.BudkerInstituteofNuclearPhysicsSBRAS(BINP),Novosibirsk630090,Russia
jGSIHelmholtzcentreforHeavyIonResearchGmbH,D-64291Darmstadt,Germany kGuangxiNormalUniversity,Guilin541004,People’sRepublicofChina
lGuangXiUniversity,Nanning530004,People’sRepublicofChina
mHangzhouNormalUniversity,Hangzhou310036,People’sRepublicofChina nHelmholtzInstituteMainz,Johann-Joachim-Becher-Weg45,D-55099Mainz,Germany oHenanNormalUniversity,Xinxiang453007,People’sRepublicofChina
pHenanUniversityofScienceandTechnology,Luoyang471003,People’sRepublicofChina qHuangshanCollege,Huangshan245000,People’sRepublicofChina
rHunanUniversity,Changsha410082,People’sRepublicofChina sIndianaUniversity,Bloomington,IN 47405,USA
tINFNLaboratoriNazionalidiFrascati,I-00044,Frascati,Italy uINFNandUniversityofPerugia,I-06100,Perugia,Italy vINFNSezionediFerrara,I-44122,Ferrara,Italy wUniversityofFerrara,I-44122,Ferrara,Italy
xJohannesGutenbergUniversityofMainz,Johann-Joachim-Becher-Weg45,D-55099Mainz,Germany yJointInstituteforNuclearResearch,141980Dubna,Moscowregion,Russia
zJustusLiebigUniversityGiessen,II.PhysikalischesInstitut,Heinrich-Buff-Ring16,D-35392Giessen,Germany aaKVI-CART,UniversityofGroningen,NL-9747AAGroningen,TheNetherlands
abLanzhouUniversity,Lanzhou730000,People’sRepublicofChina acLiaoningUniversity,Shenyang110036,People’sRepublicofChina adNanjingNormalUniversity,Nanjing210023,People’sRepublicofChina aeNanjingUniversity,Nanjing210093,People’sRepublicofChina afNankaiUniversity,Tianjin300071,People’sRepublicofChina agPekingUniversity,Beijing100871,People’sRepublicofChina ahSeoulNationalUniversity,Seoul,151-747, RepublicofKorea aiShandongUniversity,Jinan250100,People’sRepublicofChina
ajShanghaiJiaoTongUniversity,Shanghai200240,People’sRepublicofChina akShanxiUniversity,Taiyuan030006,People’sRepublicofChina
alSichuanUniversity,Chengdu610064,People’sRepublicofChina amSoochowUniversity,Suzhou215006,People’sRepublicofChina anSunYat-SenUniversity,Guangzhou510275,People’sRepublicofChina aoTsinghuaUniversity,Beijing100084,People’sRepublicofChina apIstanbulAydinUniversity,34295Sefakoy,Istanbul,Turkey aqDogusUniversity,34722Istanbul,Turkey
arUludagUniversity,16059Bursa,Turkey
asUniversityofChineseAcademyofSciences,Beijing100049,People’sRepublicofChina atUniversityofHawaii,Honolulu,HI 96822,USA
auUniversityofMinnesota,Minneapolis,MN 55455,USA avUniversityofRochester,Rochester,NY 14627,USA
awUniversityofScienceandTechnologyofChina,Hefei230026,People’sRepublicofChina axUniversityofSouthChina,Hengyang421001,People’sRepublicofChina
ayUniversityofthePunjab,Lahore54590,Pakistan azUniversityofTurin,I-10125,Turin,Italy
baUniversityofEasternPiedmont,I-15121,Alessandria,Italy bbINFN,I-10125,Turin,Italy
bcUppsalaUniversity,Box516,SE-75120Uppsala,Sweden bdWuhanUniversity,Wuhan430072,People’sRepublicofChina beZhejiangUniversity,Hangzhou310027,People’sRepublicofChina bfZhengzhouUniversity,Zhengzhou450001,People’sRepublicofChina
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Articlehistory:
Received30June2015
Receivedinrevisedform22September 2015
Accepted23September2015 Availableonline30September2015 Editor:L.Rolandi
Keywords:
BESIII
Ds
Branchingfractions
We study D+s decays to final states involving the
η
with a 482 pb−1 data sample collected at√
s=4.009 GeV with the BESIII detector at the BEPCIIcollider. We measure the branching fractions
B(D+s →
η
X)= (8.8±1.8±0.5)% andB(D+s →η
ρ
+)= (5.8±1.4±0.4)% wherethefirstuncertainty isstatisticalandthesecondissystematic.Inaddition,weestimateanupperlimitonthenon-resonant branchingratio B(D+s →η
π
+π
0)<5.1% atthe90% confidencelevel.Ourresults areconsistentwithCLEO’s recentmeasurements and helptoresolvethe disagreementbetweenthetheoretical prediction andCLEO’spreviousmeasurementofB(D+s →
η
ρ
+).©2015TheAuthors.PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense (http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.
1. Introduction
Hadronic weak decays of charmedmesons provide important
informationon flavormixing, CP violation,andstrong-interaction effects [1]. There are several proposed QCD-derived theoretical
approaches to handle heavy meson decays [2–6]. However, in
contrast to B mesons, theoretical treatment of charmed mesons suffers from large uncertainties since the c quark mass is too lightforgoodconvergenceoftheheavy quark expansionbutstill much too massive for chiral perturbative theory to be applica-ble. Currently, theoretical results for the partial decay widths of ground-state charmed mesons agree fairly well with experimen-tal results. However, there exists a contradiction concerning the branching fraction
B(
D+s→
η
ρ
+)
. CLEO reported(
12.
5±
2.
2)
%[7],while ageneralizedfactorizationmethod[8]predictsa factor offour less,
(
3.
0±
0.
5)
%. Summing the large experimental value ofB(
D+s→
η
ρ
+)
with other exclusive rates involvingη
givesB(
D+s→
η
X)
= (
18.
6±
2.
3)
% [9], while the measured inclusive decayrateB(
D+s→
η
X)
ismuchlower,(
11.
7±
1.
8)
%[10],whereX denotes all possible combinations of states. Therefore, further
experimental studyofthe
η
decaymodesis ofgreatimportance forresolvingthisconflict.*
Correspondingauthor.E-mailaddress:liupl@ihep.ac.cn(P.L. Liu).
1 Also at State Key Laboratory of Particle Detection and Electronics, Beijing 100049,Hefei230026,People’sRepublicofChina.
2 AlsoatAnkaraUniversity,06100Tandogan,Ankara,Turkey. 3 AlsoatBogaziciUniversity,34342Istanbul,Turkey.
4 AlsoattheMoscowInstituteofPhysicsandTechnology,Moscow141700,Russia. 5 Alsoatthe FunctionalElectronicsLaboratory,Tomsk StateUniversity,Tomsk, 634050,Russia.
6 AlsoattheNovosibirskStateUniversity,Novosibirsk,630090,Russia. 7 AlsoattheNRC“KurchatovInstitute”,PNPI,188300,Gatchina,Russia. 8 AlsoatUniversityofTexasatDallas,Richardson,TX 75083,USA. 9 CurrentlyatIstanbulArelUniversity,34295Istanbul,Turkey.
Recently, CLEO reportedan updated measurementof
B(
D+s→
η
π
+π
0)
= (
5.
6±
0.
5±
0.
6)
% [11]; this includes the resonantprocess
η
ρ
+.This is much smaller than the previous result [7]. In thispaper, we report the measurements of the inclusiverateB(
D+s→
η
X)
andtheexclusiverateB(
D+s→
η
ρ
+)
attheBESIII experiment.2. Datasampleanddetector
The analysis is carried out using a sample of 482 pb−1 [12] e+e−collisiondatacollectedwiththeBESIIIdetectoratthecenter ofmassenergy
√
s=
4.
009 GeV.TheBESIIIdetector,asdescribedindetailinRef.[13],hasa geo-metricalacceptanceof93%ofthesolidangle.Asmall-cell helium-basedmaindriftchamber(MDC)immersedina1 Tmagneticfield measures the momentum of charged particles with a resolution of0.5%at1 GeV
/
c.Theelectromagneticcalorimeter(EMC)detects photons with a resolution of 2.5% (5%) at an energy of 1 GeV in the barrel (end cap) region. A time-of-flight system(TOF) as-sistsinparticleidentification(PID)withatimeresolutionof80 ps (110 ps)inthebarrel(endcap)region.OurPIDmethodscombine the TOF information with the specific energy loss (dE/
dx) mea-surements of charged particles in the MDC to forma likelihoodL(
h)(
h=
π
,
K)
foreachhadron(h)hypothesis.A geant4-based [14] Monte Carlo (MC) simulation software, whichincludesthegeometricdescriptionoftheBESIIIdetectorand thedetectorresponse,isusedtooptimizetheeventselection cri-teria, determinethedetectionefficiencyandestimatebackground contributions.Thesimulationincludesthebeamenergyspreadand initial-state radiation (ISR), implemented with kkmc [15].
Allow-ing for a maximum ISR photon energy of 72 MeV, open charm
processes are simulated from D+sD−s threshold at 3.937 GeV to the center-of-mass energy 4.009 GeV. Cross sections have been takenfromRef.[16].Forbackgroundcontributionstudiesandthe validation oftheanalysisprocedure, aninclusiveMC sample cor-responding to an integrated luminosity of 10 fb−1 is analyzed.
In addition to the open charm modes, this sample includes ISR production, continuum light quark production and QED events.
The known decay modes are generated with evtgen [17] with
branching fractions setto the world average values [9], and the remainingunknowneventsaregeneratedwith lundcharm[18]. 3. Dataanalysis
3.1.Measurementof
B(
D+s→
η
X)
Fordatatakenat4.009 GeV,energyconservationprohibitsany additionalhadronsaccompanyingtheproductionofa D+sD−s pair. Followingatechnique firstintroducedby theMARK III Collabora-tion
[19]
, theinclusivedecayrateof D+s→
η
X ismeasured. Weselectsingletag(ST)eventsinwhichatleastone D+s orD−s can-didateisreconstructed,anddoubletag(DT)eventsinwhichboth
D+s and D−s are reconstructed.To illustrate themethod, we take theSTmode D−s
→
α
andthesignal mode D+s→
η
X for exam-ple.Theη
candidates inthesignal modeare reconstructedfrom thedecaymodeη
→
π
+π
−η
withtheη
subsequentlydecaying intoγ γ
.TheSTyieldsaregivenasyαST
=
ND+sD−s
B
(
D−
s
→
α
)
ε
αST,
(1)whereND+
sD−s is thenumberofproduced D
+
s D−s pairsand
ε
STα isthe detectionefficiency of reconstructing D−s
→
α
. Similarly, the DTyieldsaregivenasyαDT
=
ND+sD−s
B
(
D−
s
→
α
)
B
(
D+s→
η
X)
B
ηPDGε
DTα,
(2)where
B
PDGη istheproduct branchingfractionsB(
η
→
π
+π
−η
)
·
B(
η
→
γ γ
)
,ε
αDT is the detection efficiency of reconstructing D−s
→
α
and D+s→
η
X atthesame time.Withε
αST and
ε
αDTes-timatedfrom MC simulations, theratio of yαDT to yαST provides a measurementof
B(
D+s→
η
X)
,B
(
D+s→
η
X)
B
PDGη=
yαDT yαST·
ε
STαε
α DT.
(3)WhenmultipleSTmodesareused,thebranchingfractionis deter-minedas
B
(
D+s→
η
X)
B
PDGη=
αyαDT αyαST·
εDTα εα ST=
yDT αyαST
·
εαDT εα ST,
(4)whereyDT
=
α yαDTisthetotalnumberofDTevents.Inthisanalysis, theSTeventsare selectedby reconstructinga
D−s inninedifferentdecaymodes:K0
SK−,K+K−
π
−,K+K−π
−π
0,K0SK+
π
−π
−,π
+π
−π
−,π
−η
,π
−η
(
η
→
π
+π
−η
)
,π
−η
(
η
→
ρ
0γ
,
ρ
0→
π
+π
−)
, andπ
−π
0η
. The DT events are selected byfurther reconstructing an
η
among the remaining particles not used in the ST reconstruction. Throughout the paper, charged-conjugatemodesarealwaysimplied.Foreachchargedtrack(exceptforthoseusedforreconstructing
K0S decays),thepolarangleintheMDCmustsatisfy
|
cosθ
|
<
0.
93, andthe point of closest approach to the e+e− interaction point (IP)mustbewithin±
10 cm along thebeamdirectionandwithin 1 cmintheplane perpendiculartothebeamdirection.AchargedK
(
π
)
mesonisidentifiedbyrequiringthePIDlikelihoodtosatisfyL(
K)
>
L(
π
)
(L(
π
)
>
L(
K)
).Showersidentified as photon candidates must satisfy the fol-lowingrequirements.ThedepositedenergyintheEMCisrequired to be larger than 25 MeV in the barrel region (
|
cosθ|
<
0.
8) or largerthan50 MeVinthe endcapregion (0.
86<
|
cosθ
|
<
0.
92). Tosuppresselectronicnoise andenergydepositsunrelatedtothe event,theEMCtimedeviationfromtheeventstarttimeisrequiredTable 1
Requirementson E forSTD−s candidates.
ST modeα Data (GeV) MC (GeV)
K0 SK− (−0.027,0.021) (−0.025,0.021) K+K−π− (−0.032,0.023) (−0.031,0.024) K+K−π−π0 (−0.041,0.022) (−0.041,0.022) K0 SK+π−π− (−0.035,0.024) (−0.032,0.026) π+π−π− (−0.036,0.023) (−0.033,0.025) π−η (−0.038,0.037) (−0.041,0.032) π−ηπ π η (−0.035,0.027) (−0.034,0.028) π−ηργ (−0.035,0.022) (−0.035,0.021) π−π0η (−0.053,0.030) (−0.053,0.028)
tobe 0
≤
T≤
700 ns.Photoncandidatesmustbe separatedby at least 10 degrees from the extrapolated positions of any charged tracksintheEMC.The K0S candidatesareformedfrompairsofoppositelycharged tracks.Forthesetwotracks,thepolaranglesintheMDCmust sat-isfy
|
cosθ|
<
0.
93,andthepointofclosestapproachtotheIPmust be within±
20 cm alongthe beamdirection. No requirementson thedistanceofclosestapproachinthetransverseplaneoron par-ticleidentificationcriteriaareappliedtothetracks.Theirinvariant massisrequiredtosatisfy0.
487<
M(
π
+π
−)
<
0.
511 GeV/
c2.Thetwotracksareconstrainedtooriginatefromacommondecay ver-tex, which is required to be separated from the IP by a decay lengthofatleasttwicethevertexresolution.
The
π
0 andη
candidates are reconstructed from photonpairs. Theinvariant massis requiredtosatisfy 0
.
115<
M(
γ γ
)
<
0
.
150 GeV/
c2 forπ
0, and0.
510<
M(
γ γ
)
<
0.
570 GeV/
c2 forη
.Toimprovethemassresolution,a mass-constrainedfittothe nom-inal mass of
π
0 orη
[9] is applied to the photon pairs. Forη
candidates, the invariant mass must satisfy 0
.
943<
M(
η
π π η)
<
0
.
973 GeV/
c2 and 0.
932<
M(
η
ργ
)
<
0.
980 GeV/
c2. For theη
ργ candidates, we additionally require 0.
570<
M(
π
+π
−)
<
0
.
970 GeV/
c2 to reduce contributions from combinatorialback-ground.
Wedefine theenergydifference,
E
≡
E−
E0,where E isthe total measured energy ofthe particles in the D−s candidate andE0 isthebeamenergy.The D−s candidatesarerejectediftheyfail
topass
E requirements correspondingto3timestheresolution,
as given in Table 1. To reduce systematic uncertainty, we apply differentrequirementson
E fordataandMCsamples.Ifthereis morethanone D−s candidateinaspecificSTmode,thecandidate withthesmallest
|
E|
iskeptforfurtheranalysis.ToidentifySTsignals, thebeam-constrainedmassMBCisused. ThisisthemassoftheD−s candidatecalculatedbysubstitutingthe
beam energy E0 forthe measured energy of the D−s candidate:
M2
BCc4
≡
E20−
p2c2,where p isthe measured momentum of the D−s candidate.True D−s→
α
single-tagspeakatthe nominal D−smassinMBC.
We fit the MBC distribution of each mode
α
to obtain yαST.Backgroundcontributionsforeachmodearewelldescribedbythe ARGUS function [20],asverified withMC simulations.The signal distributionsaremodeledbyaMC-derivedsignalshapeconvoluted withaGaussianfunctionwhoseparametersareleftfreeinthefit. The Gaussian function compensatesthe resolution difference be-tween data andMC simulation. Fig. 1shows thefits to the MBC
distributionsindata;thefittedSTyields arepresentedin
Table 2
alongwiththedetectionefficienciesestimatedbasedonMC simu-lations.
Toselecteventswherethe D+s decaysto
η
X ,we requirethat theDTeventscontainanη
candidateamongtheparticles recoil-ing against theST candidate. As mentioned above, theη
candi-dates are reconstructed in the decayη
→
π
+π
−η
, with theη
Fig. 1. FitstotheMBCdistributionsfortheSTDscandidates.Ineachplot,thepointswitherrorbarsaredata,thedashedcurveisthebackgroundcontributionandthesolid lineshowsthetotalfit.
Table 2
ThedetectionefficienciesandthedatayieldsoftheSTandDTevents.The efficien-ciesdonotincludetheintermediatebranchingfractionsfor π0→γ γ,η→γ γ, K0
S→π+π−,η→π+π−ηandη→ρ0γ.Alluncertaintiesarestatisticalonly.
ST modeα εα ST(%) yαST εDTα (%) yDT K0SK− 47.89±0.35 1088±40 13.75±0.14 K+K−π− 44.16±0.18 5355±118 12.46±0.14 K+K−π−π0 13.25±0.22 1972±145 4.32±0.08 K0 SK+π−π− 24.27±0.37 595±50 6.05±0.09 π+π−π− 60.26±0.90 1657±143 17.18±0.16 68±14 π−η 48.39±0.70 843±54 14.82±0.16 π−ηπ π η 29.48±0.52 461±41 7.91±0.11 π−ηργ 43.11±0.88 1424±147 11.96±0.13 π−π0η 26.02±0.32 2260±156 7.90±0.11
subsequently decaying into
γ γ
. All particles used in theη
re-constructionmustsatisfytherequirementsdetailedabove.Ifthere ismore thanoneη
candidate, theone withthesmallestM
≡
|
M(
η
π π η)
−
m(
η
)
|
iskept,wherem(
η
)
isthenominalη
mass[9]. Thedecaymodeη
→
ρ
0γ
isnotusedduetolargecontributionsfromcombinatorialbackground.
There are peakingbackground contributions in M
(
η
π π η)
pro-ducedbyeventsinwhichthereisawrongly-reconstructed D−s tag accompanied by arealη
in the restofthe event. To obtainthe DTyields,wethereforeperformatwo-dimensionalunbinnedfitto thevariables MBC(
α
)
and M(
η
π π η)
.For MBC(
α
)
,thefitfunctions arethesameasthoseusedintheextractionofyαST.ForM(
η
π π η)
, thesignal isdescribed bythe convolutionofa MC-derivedsignal shapeandaGaussianfunctionwithparametersleftfreeinthefit. BackgroundcontributionsinM(
η
π π η)
consistof(a) D+sD−s events inwhich D−s decays tothe desiredST modes,but the D+s decay does not involve anη
; (b) other (non-ST signal) decays of D−sandalso non-D+sD−s processes.Component (a) isdescribed with afirst-orderpolynomialfunction.Component(b) ismodeledwith the sum of two Gaussian functions plus a quadratic polynomial function.ThemeansofthetwoGaussiansarefixedtothe
η
nom-inalmass[9].Otherparametersandalltheamplitudesareleftfree in thefit. The ARGUS function of MBC(
α
)
helpsto constrain the descriptionofM(
η
π π η)
incomponent(b).Thistreatmenton back-groundcontributions has been verified in MC simulations. Thereis no obvious correlation between MBC
(
α
)
and M(
η
π π η)
, so the probability densityfunctions(PDFs)ofthesetwo variablesare di-rectly multiplied.We obtainthecombinedDTyield yDTfromthe unbinned fit shown in Fig. 2. Table 2 gives the total yields of DT in dataand thecorresponding DT efficiencies. Combining the yields and efficiencies, we obtainB(
D+s→
η
X)
= (
8.
8±
1.
8)
% withEq.(4).3.2. Measurementof
B(
D+s→
η
ρ
+)
Inordertoimprovethestatisticalprecision,we determinethe branching fraction for D+s
→
η
ρ
+ using STs. As a standalone measurement, this doesnot benefit fromcancellationof system-atic uncertainties as inthe double-tag method.However, a simi-lar cancellationcan be achievedby measuring the signal relative to asimilar, alreadywell-measured finalstate. Thus, we measureB(
D+s→
η
ρ
+)
relativetoB(
D+s→
K+K−π
+)
,usingB
(
D+s→
η
ρ
+)
B
PDGρ+B
PDGηB
(
D+s→
K+K−π
+)
=
yηSTρ+ ySTK+K−π+·
ε
K+K−π+ STε
ηSTρ+,
(5) whereB
PDGρ+=
B(
ρ
+→
π
+π
0)B(
π
0→
γ γ
)
.Thedecay D+s
→
K+K−π
+ isreconstructedinthesame man-ner asreportedabove intheSTmode.OurMCsimulationofthis mode includes a full treatment of interfering resonances in the Dalitz plot [21]. The decay D+s→
η
ρ
+ is reconstructed via the decaysη
→
π
+π
−η
andρ
+→
π
+π
0,whereη
(
π
0)
→
γ γ
.Weapply thesamecriteriatofind
π
0 andη
candidatesaswereusedin the analysis of D+s
→
η
X . We do not requirePID criteria on the chargedtracks, but instead assume them all to be pions. In the reconstruction ofρ
+ andη
,theπ
+ are randomlyassigned. Theinvariant mass,M(
π
+π
0)
,oftheρ
+ candidateisrequiredtobe within
±
0.
170 GeV/
c2 of the nominalρ
+ mass, and thein-variant mass of the
η
candidate, M(
η
π π η)
, is requiredto lie in the interval(
0.
943,
0.
973)
GeV/
c2.Additionally requiring1.
955<
MBC
<
1.
985 GeV/
c2 to enrich signal events, the M(
π
+π
0)
dis-tribution of D+s
→
η
ρ
+ ininclusive MC simulationsand datainFig. 3 show good agreement. The small difference visible in the
M
(
η
π π η)
distributionwillbetakenintoaccountinthesystematic uncertainties.Fig. 2. Projections of the two-dimensional unbinned fit to DT events from data onto MBC(left) and M(ηπ+π−η)(right).
Fig. 3. ComparisonoftheM(π+π0)(left)andM(η
π π η)(right)distributionsinSTeventsofD+s →ηρ+indata(points)andinclusiveMC(solidline).Thearrowsshowthe signalregion.
Fig. 4. Projectionplotsofthetwo-dimensional unbinnedfitontoMBC(left)andcosθπ+ (right).Thesignaleventsareenrichedbyrequiring1.955<MBC<1.985 GeV/c2in therightplot.
If multiple
η
ρ
+ candidates are found in an event, only the one with the smallest|
E|
is kept. We require−
0.
035<
E<
0
.
023 GeV fordataand−
0.
037<
E<
0.
029 GeV forMC.Fitsto theMBCdistributionsareusedtoextractsignalyields.Toseparate thethree bodyprocess D+s→
η
π
+π
0 fromthe two bodydecay D+s→
η
ρ
+,thehelicityangleθ
π+ isusedtoextracttheρ
+ com-ponent,whereθ
π+ istheanglebetweenthemomentumoftheπ
+fromthe
ρ
+decayandthedirectionopposite tothe D+smomen-tuminthe
ρ
+restframe.ThesignalD+s→
η
ρ
+isdistributedas cos2θ
π+,whilethethreebodyprocessisflatincos
θ
π+.Weperformatwo-dimensional unbinnedmaximumlikelihood
fittothedistributionofMBCversuscos
θ
π+ todeterminetheyieldyηSTρ+.ThesignalmodelofMBC isthesameasthatintheanalysis of D+s
→
η
X . Forcosθ
π+,the signal shapesof D+s→
η
ρ
+ andD+s
→
η
π
+π
0 are determined based on MC simulations.Back-ground contributions in MBC are modeled withan ARGUS
func-tion, while background contributions in cos
θ
π+ are taken from the events in the MBC sidebands 1.
932<
MBC<
1.
950 GeV/
c2and1
.
988<
MBC<
1.
997 GeV/
c2.Thereisnoobviouscorrelationbetween MBC and cos
θ
π+, so the PDFsused for thesetwovari-ables are directlymultiplied. Fig. 4 showsthe projections of the two-dimensional fit results in data. In the rightplot, we further require1
.
955<
MBC<
1.
985 GeV/
c2 to enrichsignal events.The fitreturns yηSTρ+=
210±
50, and ySTηπ+π0= −
13±
56, which in-dicates that no significant non-resonant D+s→
η
π
+π
0 signal isobserved. Anupper limit of
B(
D+s→
η
π
+π
0)
atthe 90%confi-dencelevelisevaluatedto be5.1%,afteraprobability scan based on 2000 separate toy MC simulations, taking into account both
Fig. 5. MBCdistributions with the requirement of|cosθπ+| <0.5 (left) or|cosθπ+| >0.5 (right).
Table 3
Summaryofrelativesystematicuncertaintiesinpercent.Thetotaluncertaintyis takenasthesuminquadratureoftheindividualcontributions.
Source B(D+s →ηX) B(D+s →ηρ+) MDC track reconstruction 2.0 PID 2.0 3.0 π0detection 2.4 ηdetection 2.7 3.5 E requirement 1.0 1.4 M(ηπ π η)requirement 2.0 M(ηπ π η)backgrounds 1.5 Peaking backgrounds in ST 0.3 MBCsignal shape 1.0 0.6 MBCfit range 1.7 0.5 cosθπ+backgrounds 2.9 Uncertainty of efficiency 1.6 0.5
Quoted branching fractions 1.7 3.8
Total 5.3 7.5
thestatisticalandsystematicuncertainties.Asshownin
Fig. 5
,we seeobvious D+s signalsinthe MBC distribution withthe require-ment of|
cosθ
π+|
>
0.
5, while it is not the casewhen requiring|
cosθ
π+|
<
0.
5. This indicates that the three body process is notsignificant.
We study the MBC distributions for events in
ρ
+ andη
sidebands. The
ρ
+ sideband region is chosen as M(
π
+π
0)
<
0
.
500 GeV/
c2, and theη
sidebands are 0.
915<
M(
η
π π η)
<
0
.
925 GeV/
c2 and0.
990<
M(
η
π π η)
<
1.
000 GeV/
c2. No D+ssig-nalisvisibleinthesidebandevents,furthersubstantiatingthatthe non-resonantprocesses D+s
→
η
π
+π
0 andD+s
→
ηπ
+π
−ρ
+arenegligible.Asimulationstudyshowsthatthepotentialbackground contributionfrom
η
→
ρ
0γ
isnegligible.Thedetectionefficiency
ε
STηρ+ isestimatedtobe(
9.
80±
0.
04)
%. Combinedwiththeresultsforthenormalizationmode K+K−π
+, asgiveninTable 2
, weobtain fromEq.(5)theratioofB(
D+s→
η
ρ
+)
relative toB(
D+s→
K+K−π
+)
as 1.
04±
0.
25. Taking the mostprecise measurement ofB(
D+s→
K+K−π
+)
= (
5.
55±
0
.
19)
% from CLEO [11] as input, we obtainB(
D+s→
η
ρ
+)
=
(
5.
8±
1.
4)
%.3.3. Systematicuncertainties
In the measurement of
B(
D+s→
η
X)
,many uncertainties on theST side mostly cancelinthe efficiencyratios inEq.(4). Sim-ilarly, for D+s→
η
ρ
+, the uncertainty in the tracking efficiency cancelsto anegligiblelevel bytakingtheratioto the normaliza-tionmode D+s→
K+K−π
+ inEq.(5).The followingitems, sum-marizedinTable 3
,aretakenintoaccountassourcesofsystematic uncertainty.a. MDCtrackreconstructionefficiency. Thetrackreconstruction ef-ficiencyisstudiedusingacontrolsample ofD+
→
K−π
+π
+inthedatasampletakenat
√
s=
3.
773 GeV.Thedifferencein the trackreconstruction efficiencies between dataand MC is found to be 1.0%per charged pionandkaon.Therefore, 2.0% istakenasthesystematicuncertaintyoftheMDCtrack recon-structionefficiencyforD+s→
η
X .b. PIDefficiency. We study the PID efficiencies using the same control sampleasinthetrackreconstructionefficiencystudy. ThedifferenceinPIDefficienciesbetweendataandMCis de-termined to be 1.0% per charged pion or kaon. Hence, 2.0% (3.0%) is takenasthe systematic uncertaintyof the PID effi-ciencyforD+s
→
η
X (D+s→
η
ρ
+).c.
π
0andη
detection. Theπ
0 reconstruction efficiency,includ-ing the photon detection efficiency, is studied using a con-trol sample of D0
→
K−π
+π
0 in the data sample taken at√
s
=
3.
773 GeV. After weighting the systematic uncertainty inthemomentumspectraofπ
0,2.8%istakenasthesystem-aticuncertaintyforthe
π
0efficiencyinD+s
→
η
ρ
+.Similarly,the systematicuncertainty forthe
η
efficiencyin D+s→
η
X(D+s
→
η
ρ
+) is determined to be 2.7% (3.5%) byassum-ingdata-MCdifferenceshavethesamemomentum-dependent valuesasfor
π
0 detection. Thesystematicuncertaintiesweresetconservativelyusingthecentralvalue ofthedata-MC dis-agreements plus 1.0(1.64) standarddeviations for
π
0 (η
),asappropriate fora 68% (95%)confidencelevel.Here we inflate the
η
uncertainty,becausetheuncertaintyoftheη
detection isestimatedreferringtoπ
0.d.
E requirement. Differences in detector resolutions between
dataandMCmayleadtoadifferenceintheefficienciesofthe
E requirements.In ourstandardanalysisprocedure,we
ap-plydifferent
E requirements ondataandMC,toreducethe systematicuncertainties. To be conservative,we examine the relative changesoftheefficiencies byusingthesame
E
re-quirementsforMCasfordata.Weassignthesechanges,1.0% forD+s
→
η
X and1.4%forD+s→
η
ρ
+,asthesystematic un-certaintiesontheE requirement.
e. M
(
η
π π η)
requirement. In the right plot in Fig. 3, the resolu-tionoftheη
peakinMCisnarrowerthandata.Wetakethe change in efficiency of 2.0%, after using a Gaussian function tocompensateforthisresolutiondifference,asthesystematic uncertaintyoftheM(
η
π π η)
requirementforD+s→
η
ρ
+.f. M
(
η
π π η)
background contributions. In the measurement ofB(
D+s→
η
X)
, a two-dimensional fit is performed to theMBC
(
ST)
and M(
η
π π η)
distributions. The uncertainty due tothe description of the M