Coordinatore Prof. Filippo Frontera
Proton indu ed Deuteron Breakup
rea tion studies at COSY
Dottorando Tutore
Susanna Bertelli Dr. Paolo Lenisa
The present thesis isdedi ated to the study of the pd Breakup
re-a tion. The study is part of a proje t, realized at the COSY storage
ring, nalized to map pd breakup spin observables in a kinemati al
region where measurements are limited altough strongly ne essary to
ximportant onstraintsforinvestigatingthe roleof thethree-nu leon
for es viathe Chiral Perturbation Theory.
Intherstpartofthework,Idevelopedananalysis haintodetermine
whether adete tionsystem basedonSili onTra king Teles ope,
origi-nally on eivedtoidentifypd elasti events,was apabletoidentifythe
produ ts of the pd Breakup rea tion. This feasibility study has been
su essfullyappliedtoanexistingdatasampletakenattheCOSYring
inFebrauary2008,withaverti allypolarizedprotonbeamof49.3MeV
kineti energy impingingonaDeuterium luster target. In afollowing
phase, the identied pd Breakup events have been employed to tune
an algorithm to measure the analysing power in pd Breakup rea tion
using the neutron asymmetries. This observable represents one of the
probes to onstrain Chiral Perturbation Theory. The analysis of the
available data sample has allowed to outline the experimental
ondi-tionsrequiredforanexhaustiveinvestigationofthe spinobservablesin
pd breakup rea tion. On the other side, the low statisti sand the not
optimalworking onditions of the dete tion system made not possible
to nalize the result on the existing data sample. At present the
de-veloped analysis is being exploited on a new sample of data a quired
during 2011 beam-time.
In parallel, I arried out a study of a new apparatus devoted to the
pd Breakup investigation. In parti ular double spin asymmetries in
pd Breakup oer a ri h laboratory where to test Chiral Perturbation
Theory. For a essing these observables, an experiment where both
re-quired. Inadditionadete tionsystemprovidingalargeazimuthaland
longitudinalphase-spa e overage would be needed.
Forthis reason,I implemented the analysis software, developed inthe
rst stage of my work, for the hara terization and the optimization
of this dedi ated dete tion system on the basis of Monte Carlo
gen-erated data. The results of the analysis served as a guidan e for the
dete tordesign andhavebeen in ludedinaproposal[1℄submitted and
Questo lavoro di tesi è dedi ato allo studio della reazione di
fram-mentazione del Deutone indotta da un fas io di protoni, pd Breakup.
Questo studio ostituis e parte di un progetto di ri er a, realizzato
presso l'anello di a umulazione COSY, nalizzato alla misura delle
osservabili di polarizzazione della reazione di pd Breakup, in una
re-gione inemati a in uile misureesistenti sono limitatesebbene
indis-pensabili per ssare vin oliutiliper investigareil ruolo delle forze he
agis ono tra tre nu leoni 3NF attraverso la Chiral Perturbation
The-ory.
Nella prima parte del lavoro, ho sviluppato una atena di analisi per
stabilire se un sistema di rivelazione basato su sensori di sili io,
on- epiti originariamente per identi are gli eventi del anale pd
elas-ti o, fosse in grado di identi are an he i prodotti della reazione di
pd breakup.
Questo studio di fattibilità è stato appli ato on su esso ad un
am-pione di dati a quisiti presso l'a eleratore COSY nel Febbraio 2008,
in ui sono state indotte ollisioni tra un fas io di protoni
polariz-zato ad un'energia ineti a di 49.3 MeV e un bersaglio di Deuterio.
Nella fase su essiva, gli eventi di pd Breakup identi ati sono stati
utilizzatipermettereapuntounalgoritmoperdeterminarel'analysing
powerdellareazionedipd Breakup usandoleasimmetriedelneutrone.
Questa osservabile rappresenta un test hiave per vin olare la Chiral
Perturbation Theory. L'analisi del ampione di dati a disposizione ha
onsentito di delineare le ondizioni sperimentali ideali per studiare
in maniera esaustiva le osservabili di polarizzazione della reazione pd
Breakup. Tuttavia a ausa della statisti a limitata e delle ondizioni
di lavoro non ottimali del sistema di rivelazione, non è stato possibile
nalizzare un risultato per il ampione di dati esistente. Al momento
ampione didati a quisiti duranteuna presa dati nel 2011.
Inparallelo,hosviluppatol'analisidiunnuovoapparatoespli itamente
dedi atoallostudiodel analepd Breakup. Ledoublespinasymmetries
nel analedipd Breakup ostituis onounri olaboratoriodovetestare
laChiralPerturbationTheory. Pera edereaquesteosservabili,è
ne -essariorealizzareunesperimentoin uiilfas iodiprotonieilbersaglio
di Deuterio siano entrambi polarizzati e il sistema di rivelazione sia
aratterizzato da una estesa opertura longitudinale e azimutale dello
spazio delle fasi.
A questo s opo, ho implementato il software di analisi sviluppato per
laprimapartedellavoroditesi,alnedi aratterizzareeottimizzareil
sistemadirivelazionededi atoutilizzandodatiMonteCarlo. Irisultati
di questa analisi sono serviti ome guida per il design del sistema di
rivelazioneesono stati in lusiinun proposal[1℄ he èstato sottomesso
Abstra t iii
Riassunto v
Introdu tion 3
1 Physi s Motivation 7
1.1 Conventional approa hes to the Nu lear For e problem 8
1.2 The ChiralPerturbation Theory . . . 10
2 Experimental Setup 15 2.1 The COSY fa ility . . . 15
2.1.1 Ele tron Cooler . . . 17
2.2 PAX beam polarimeter . . . 17
2.2.1 Deuterium luster target . . . 17
2.2.2 SILICON TRACKINGTELESCOPES . . . 19
2.2.3 Front-end ele troni s . . . 20
2.2.4 Geometryand Trigger . . . 21
3 Deuteron Breakup events analysis 25 3.1 pd Breakup vs pd elasti . . . 26
3.1.1 Kinemati s of
pd → ppn
. . . 273.2 Simulationsand Data . . . 28
3.2.1 RUN SELECTION . . . 29
3.3 Tra k Re onstru tion . . . 30
3.3.2 Tra k "1" re onstru tion . . . 34
3.3.3 Tra k "2" re onstru tion . . . 34
3.3.4 Thirdlayer Calibration . . . 35
3.3.5 Tra k "3" re onstru tion . . . 36
3.4 DeuteronBreakup samples . . . 38
3.5 E ien yof Breakup identi ation . . . 40
3.6 Phase Spa eCoverage . . . 42
3.7 Method development for the analysing power
A
y
in pd→
ppn . . . 493.7.1 Considerations . . . 53
4 Future plans: Dedi ated setup for pd Breakup studies 55 4.1 PAX ExperimentalSetup. . . 55
4.1.1 The COSY beam . . . 56
4.1.2 Polarized Internal Target . . . 57
4.2 PAX Multipurpose Dete tionSystem . . . 59
4.3 pd Breakup event generation . . . 61
4.4 pd Breakup events identi ation . . . 61
4.4.1 Stopped protons: tra k "1" . . . 63
4.4.2 Stopped protons: tra k "2" and "3" . . . 63
4.5 pd Breakup re onstru tion e ien y . . . 65
4.6 Phase spa e overage . . . 67
4.6.1 Considerations . . . 70
Con lusions 71
Appendix A 73
Appendix B 79
Oneof themain issuesin nu learphysi sisdeterminingthe nature
ofthe intera tionsbetweenthe nu leonswhi his ru ialfor
investigat-ing the properties of nu lei. In general observables at the energy
rele-vant to nu lear physi s are well des ribed by a nu leon-nu leon (NN)
potential. Altough mu h has been learned about the NN intera tion,
itis ofinteresttond out whether these for es an alsobeinvolved in
systems where more than two nu leons intera t.
In a three-nu leonsystem it isimportantto investigate howthe
inter-a tion between two nu leons is inuen ed by the presen e of a third
nu leon. This extra ee t is related to a for e whi h is beyond the
two-nu leon intera tion and is known asthree-nu leon for e (3NF).
At present, few-nu leon systems an be studied using
phenomenolog-i al models that, despite some remarkable su esses in des ribing
ex-perimentaldata, leave some open problems, amongwhi h is the loose
onne tion toQCD.
The drawba ks of phenomenologi al models are over ome by
employ-ing the modern theory of nu lear for e Chiral Perturbation Theory
(ChPT). ChPT is an ee tive eld theory (EFT), that allows a
sys-temati approa htostudyinglow-energyhadrondynami sadheringto
the symmetries of QCD.
To provide a better understanding of 3NFs ee ts, dierential ross
se tions and polarization observables have been measured in
nu leon-deuterons attering. Inathree-nu leon(3N) ontinuumthe
experimen-tal data and the theoreti al predi tions reveal both very good
agree-mentand signi antdisagreement.
An alternativeto Nds attering, spin observables in
pd→ppn
deuteron breakup rea tions, due to the ri her kinemati s, oer a fertilelabora-tory wherestudying the 3NFs.
three-nu leonintera tionsandinparti ulartheirspindependen e,amajority
of possible observables need to be measured with high a ura y, sin e
3NFs ee ts are in general very smallin the three-nu leon system. In
parti ular the energy range between 30 and 50 MeV is an ideal range
wherethe3NF ee tsare expe tedtoappear andbesigni antandat
thesametimeitisasuitablerangetotestthepredi tivepowerof hiral
EFT. In this range previous measurements are s ar e and limited and
itwould bevery interesting to have at disposala omplete database.
Thereaser h ofthis thesishas been performedintheframeworkofthe
PAX Collaboration that aims at the produ tion of the rst polarized
antiprotonbeam. In parti ular, inthe past three years, the PAX
Col-laboration has performed a series of tests onprotons at COSY aimed
at investigating spin-ltering and spin-ip as possible me hanisms to
polarizeastoredbeamofprotons. Inthis environmentadedi ated
po-larimeter to measure the stored beam polarization has been installed
inthe COSYring. Thepolarimeterhasbeen implementedbymeansof
a ouple of Sili on-Tra king Teles opes that serve to dete t deuterons
omingfrom pd elasti s attering.
Therst partofmyworkhasbeen devotedtoafeasibilitystudyofthe
useofthe samepolarimetertoidentifydeuteronbreakupevents, whi h
onstituted part of the ba kground with respe t tothe elasti
s atter-ing. To this purpose, I analyzed the data taken during a dedi ated
beamtimein2008 andI developed a hain of sele tion riteriato arry
out the pd Breakup events identi ation. After a lean identi ation
of the deuteron breakupevents,I investigated the possibilityto a ess
the neutron analyzing power by the two outgoing protonsdete ted in
the polarimeter.
This analysis pro edure of pd breakupevents forms partof the
feasib-bility studies for an a epted experiment proposal submitted by the
PAX ollaboration [1℄ to be performed at COSY. The obje tive of
the planned experiment is to provide a means of testing the
predi -tive power of hiral EFT, in luding the ee ts of three-nu leon for es
in few-nu leon systems. Most of the spin orrelation parameters and
the ve tor and tensor analysingpowers inpd breakup rea tions at
30-50 MeV proton beam energy will be measured with large phase spa e
overage.
To this aima dedi ated dete tion system is being developed that will
atthenewlyinstalledPAXsetupatCOSY.Thisdete tordevelopment
wastheobje tofthese ondpartofmythesis. Inparti ularIanalyzed
MonteCarlo dataforthe hara terization and theoptimizationof this
dete tion system. The results of the simulation analysis were adopted
in the proposal[1℄.
The thesis is organized as follows: Chapter 1 reports the motivations
supporting the ne essity of additional measurements in the three
nu- leon se tor; in Chapter 2 the experimental setup used to realize the
feasibility study for pd-breakup is presented; Chapter 3 is devoted to
the pro edure of breakupidenti ationand analysis;in Chapter 4 the
results of Monte Carlo studies for the future dedi ated dete tor are
Physi s Motivation
One of the main issues in Nu lear Physi s is the role of the for es
a tingbetween nu lear onstituentsandfew-nu leonsystemsrepresent
the ideal laboratories where these for es an be investigated. In
par-ti ular it is important to study the dynami s related to the presen e
of a third nu leon, whi his ru ial tounderstand the ontributions of
three-nu leon for es (3NFs).
Evenifthe theoryof3NFswasdevelopedinthe30'softhelast entury
[2℄, still many problems remain open. Presently, the spin stru ture of
the three-nu leon ontinuum exhibits disparate results when
ompar-ing experimentaldata totheoreti al predi tions based on two-nu leon
potentials either with or without the in lusion of three-nu leon
inter-a tions. A detailedreview of the urrent status of the resear h on the
role ofthe three-nu leon for es an be foundin [3℄. The ri h
kinemati- alregioninproton-deuteronbreakuprea tions atlowtointermediate
energy oers agoodtesting groundfor the hiral ee tive eld theory
(EFT), the modern theory of nu lear for es in the low-energyregime.
In parti ular, in the energy range between 30 and 50 MeV, that is of
interest for the experiments presented in this thesis, very s ar e
po-larized experimentaldata exist. This is an ideal range where the
pre-di tive powerof hiral EFT in three-nu leon ontinuum an be tested
by measuring analysingpowers and doublespin observables with high
pre isionover large areas of the phase-spa e.
The hapter is organized as follow: se tion 1 introdu es a survey of
the main approa hes developed tostudy the ontributionofthe
three-nu leon for es (3NFs) in nu lear systems, se tion 2 provides a review
1.1 Conventional approa hes to the Nu lear For e
problem
Sin e the typi al energy s ale in Nu lear Physi s is in the order
of nu lear binding energies, the N-body problem an be des ribed by
thenon-relativisti S hrödingerequation. Inarstapproximation,
ob-servables in this energy range are well des ribed by a nu leon-nu leon
(NN)potential. The onventionalwaytodes ribethenu learfor eis
Figure1.1: The entralnu leon-nu leon(NN)potentialisdisplayed. Thelongestrange
ontribution orresponds to the 1-
π
ex hange, the intermediate range attra tion isde-s ribedby2-
π
ex hangesandothershorterrange ontributions. Atshorterdistan es,theNNintera tionisstronglyrepulsive. ThisgureistakenfromRef. [4 ℄.
based onthe meson-ex hangepi ture as proposed by Yukawa[5 ℄. This
approa henri hed by mesoneld theory and dispersion relations
(em-ployed to onstru tthetwo-pionex hange ontribution)broughttothe
development of high pre isionsemi-phenomenologi al nu leon-nu leon
(NN) potentialmodels like AV18[6℄, CDBonn[7 , 8, 9℄, Nijmegen I and
II[10℄. These models des ribe the long-range tail of the nu lear for e
due to ele tromagneti intera tion and the one-pion ex hange
poten-tialandparametrizethemedium-andshort-range ontributions. These
potentials an reprodu e alargesampleofproton-proton and
neutron-protons atteringdataoberservablesup tothepion produ tion
thresh-old with a
χ
2
/datum
∼
1 and provide an a urate representation of most deuteron properties. In Nd s attering dierential ross se tion,a dis repan y with data is observed as the energy in reases (for the
analysing power this dis repan y is known as
A
y
-puzzle[11℄).The dieren e between al ulations in luding solely 2NFs and data is
usually interpreted as an indi ation of the existen e of three-nu leon
for es (3NFs). 3NFs are many-body intera tions that have to be
in- ludedbeyondpairfor estodes ribenu leiandnu learrea tions
prop-erly. Systemati studies of the dynami s of systems involving threeor
four nu leons allow pre ise tests of the role and the stru ture of the
3NFs.
The Urbana-Argonne group[12℄ showed that three-nu leon for es have
tobein ludedtodes ribethenu learbindingenergieswhi hareknown
to beunderestimated by two-nu leon potentials.
TheextensionofYukawatheoryto3NFisduetoFujitaandMiyazawa[13℄,
who implemented the meson ex hange idea by sandwi hing the
pion-nu leon s attering amplitude between nu leon lines, thus originating
the 3NF oflongest range.
The des ribed approa his frequentlyused innu learstru ture and
re-a tion al ulations but reveals some de ien ies like the absen e of a
way toassignatheoreti alerror,the di ultytoimplementgaugeand
hiral symmetries, the in onsisten y between three-nu leon for es and
the nu leon-nu leon intera tion models and avery loose onne tionto
Quantum ChromoDynami s (QCD).
These de ien ies an be over ome in hiral Ee tive Field Theory
(EFT), an approa h to study the low-energy hadron onsistent with
the QCD. ChiralEFT is linked to QCDvia itssymmetries and allows
to treat the low-energy properties of hadroni systems in a ontrolled
way. Whenthismethodisappliedtoasystemofthreenu leons,graphs
in luding3NFsappearnaturallyina ompleteagreementwiththe
hi-ralNN intera tions, asdes ribed inthe next se tion.
Theexperimentaldataand thetheoreti al predi tionsforrea tions
in- luding three nu leons at low and intermediate energies are today at
varian e. Insomepartsofthephasespa eforsomeobservables, the
in- lusionofthe3NFinthemodelsleadtoagoodagreementbetweendata
and theory,while inother partsthe agreement isworsened[14 , 15, 16℄.
This ambiguity requiresa omplete and high pre ision database.
The Deuteron breakup oers, with respe t to the elasti hannel, a
ri her kinemati sto study observables in the threenu leon ontinuum
demonstratethe possibile eviden eof the 3NFs.
1.2 The Chiral Perturbation Theory
ChiralPerturbationTheory(ChPT) istheee tivetheoryof
Quan-tum ChromoDynami s (QCD) formulatedby Weinberg[17℄ and
devel-opedintoasystemati toolforstudyingthe propertiesof hadroni
sys-temsatlowenergies inamodel-independentframework. Itisbasedon
thespontaneouslybroken hiralsymmetryofQCD,providingamethod
to improve the results by onsidering higher orders in a perturbative
expansion. Weinberg attemptedageneralizationofthis methodtothe
few-nu leonse tor,fa inganon-perturbativeproblemsin e one hasto
deal with the strong nu leon-nu leon intera tion.
Inthe frameworkofChPTtwokindofintera tionsemerge: long-range
pionex hangesand onta tintera tions,withtheasso iatedlow-energy
onstants(LEC).Dueto hiralsymmetry,apower ounting anbeused
toestimatethe ontributionofindividualgraphstotheNNintera tion.
Weinbergproposed toapply hiralperturbation theorytothe ee tive
potential,dened as the sum of allthe ontributions of irredu ible
di-agrams, instead of applying it to the s attering amplitude, obtained
by solving the orrisponding dynami al equation. In this way, only a
nitenumberofdiagrams ontributesatagiven orderandthe
nonper-turbativity of nu lear systems is taken intoa ount.
In this framework, one an onsider the most general ee tive
La-grangian
L
EF F
forpionsandnu leons onsistentwiththesymmetriesof QCD. Nu lear for es an be determinedfromL
EF F
perturbatively via anexpansioninpowers ofQ/Λ
,whereQreferstoatypi almomentum ofthenu leonsorthepionmassandΛ
isthe hiralsymmetry-breaking s ale of≈
1GeV.The importan e of a parti ular ontribution to the nu lear potential
is xed by the power
ν
of the expansion parameter Q/Λ
, providing the a ura y at orderν
. In this sense, the theory an be al ulated atany a ura y and has a predi tive power. The nu lear for e an beespressed by:
V =
X
ν
V
ν
= V
0
+ V
1
+ V
2
+ ....
(1.1)expan-Chiralpower ountingexplainsthedominan eofthe 2NF ontribution
that starts at
ν
=0.•
ν
=0: atthisleadingorder(LO),the2NFisprovidedtwo nu leon-nu leon onta tintera tionswithoutderivates,representedinFig.1.2by the four-nu leon-leg graph with a small-dot vertex, and by
one pion ex hange, se ond diagram in the rst row of Fig.1.2.
The oupling ostantslinkedtoNN onta tinterationatthis and
higherorders anbederived fromthelow-energynu leon-nu leon
data.
Figure 1.2: The Hierar hy of nu lear for es in ChPT is shown. Solid lines are
nu leons and dashed lines are pions. Solid dots, lled/open squares and ir les
depi tverti esfrom
L
EF F
. Figuretakenfrom ref.[4℄.•
ν
=1: Theparity onservation pre ludes any ontributions atthis order.•
ν
=2: The rst orre tions at next-to-leading order (NLO) arise from two-pion ex hange, without new parameters and onta t•
ν
=3: atnext-to-next-to-leadingorder(N
2
L0),two-pionex hange
ontributionstogetherwithoneinsertionofthesubleading
ππ
NN verti es has to be onsidered. The related low-energy onstantsc
1,3,4
are determined byπ
N s attering. At this level the rstontribution to the 3NF from diagrams appears[18℄. Two-pion
ex hangepartinvolvesnonewparameters,whereasthe twoother
topologies depend on one unknown onstant ea h, whi h an be
xed from three-or more-nu leonobservables.
•
ν
=4: at next-to-next-to-next-to-leading order (N
3
LO), further
orre tions to the 2NF has to be in luded, onsidering the
sub-leadingtwo-pionex hange,theleadingthree-pionex hangeterms
and the onne ted onta t terms; at this order the four-nu leon
for e(4NF) originates.
In the framework of EFT it is natural to dene a qualitative
expla-nation of the observed hierar hy of two-, three-, more-nu leon for es:
V
2N
≫
V
3N
≫
V
4N
.Byfar, the 2NF has been worked out and appliedto
N
3
LOinthe NN
system, while the results for three- ormore-nu leonsystems are
avail-able up to
N
2
LO[19℄.
TheLowEnergy Constants(LECs) DandE entering theexpression of
3NF are determinedby tting the
3
H and
4
Hebinding energy[20 ℄ and
either the nd s attering lenght[21℄ or the properties of the nu lei[22℄.
On eD and E are xed, the resultingnu learHamiltonian an be
em-ployed todes ribethe dynami sof few-nu leon systems. This method
has the advantage, withrespe t tothe otherapproa hes, of estimating
un ertainties of the obtained predi tions.
3N s attering observables and in parti ular the breakup rea tion is
a fertile testing ground for the hiral for es. The deuteron breakup
rea tion has been re ently measured at the intermediate energy of
E
N
=65MeV(E
N
referstokineti energyofthein identnu leonbeam) andsomedata, on erning ross se tions,inkinemati al ongurationsasthenal stateintera tion, symmetri spa estar andquasi-free
s at-tering 1
are available in the range below20 MeV.
Nosystemati data existinthe energyrange between 30and 50MeV.
This energy range is extremely suitable to nd relevant ontributions
1
Inthenalstateintera tionFSI,twonu leonsleavetheintera tionregionwithequal
due to 3NF and at the same time the energies are lowenough tooer
pre ise theoreti al predi tions based on hiral EFT. Data in this
en-ergy range will provide an independent sour e for a determination of
the LECs D andEand thuswillallowa onsisten y he k ofthe
theo-reti al approa h. Moreover, pre ise data in this range willbe relevant
to explore ee ts of the new stru tures whi h appear in the 3NF at
N
3
LOwithoutanyadditionalunknownparameters. Thisisthe energy
range wherethe planned pd breakupdouble-polarized experiment will
take pla e at the COSY-fa ility, see the beam proposal submitted to
the COSY Program Advisory Program[1℄. To map out 3N, pre ision
measurements of some relevant observables as well as a large phase
spa e overage are required; these onditions are fullled using both
polarized beam and target and a large azimuthal overage dete tion
system. Appendix A is devoted to the des ription of the analysis tool
Sampling method, that provides a dire t omparison between
experi-ment and theory and willbe appliedfor the future measurements. In
parti ular the spin observables that an be a essed in a double
po-larized pd breakup experiment are reported. In Chapter 4 the future
Experimental Setup
Theexperimentaldataanalyzed inthis thesishave been taken ina
xed-target experiment performed at the COoler SYn hrotron COSY
of the Fors hungszentrum Juli h (FZJ). In these experiments a
verti- ally polarized proton beam of 49 MeV kineti energy s atters on an
unpolarizeddeuteriumtarget. Inthe s atteringpro essbothpd elasti
and pd breakup events an take pla e. Thesetworea tions are
identi-edbytheSili onTra kingTeles ope(STT)dete tionsystem,whi his
alsopartofthe beampolarimeter. Inthis hapterate hni aloverview
of the various omponents of the experimentalsetup is presented.
2.1 The COSY fa ility
TheCOolerSYn hroton(COSY)attheInstitutforNu learPhysi s
(IKP)of the Resear h Centre of Jueli h (FZJ)is ana elarator whi h
providesprotonanddeuteronbeams(
∆
p/p=10
−4
-
10
−3
)inthe
momen-tumrangefrom300MeV/ (550MeV/ inthedeuterons ase)upto3.7
GeV/ . The phase spa e ooling of the stored beam isprovided toan
ele tron ooler(up toa momentumof600 MeV/ )and ompleted bya
sto hasti ooling that overs the momentum range above 1.5GeV/ .
Unpolarized and polarized beams originate from external or internal
experiments. Polarizedbeams are produ ed by a polarizedion sour e
whi h provides a ve tor polarized proton beam and deuteron beams
with all possible ombinations of ve tor and tensor polarization. The
Figure2.1: TheCOSY-fa ilitywiththeinje tionandextra tionline;themaininternal
andexternalesperimentsareindi ated.
for a transversely polarized proton beam is
10
10
parti les (
3 · 10
10
for
deuterons) with
70%
of polarization (70%
ve tor and50%
tensor po-larization for deuterons). An overview of the COSY-ring is shown in2.1.1 Ele tron Cooler
TheCOSY ele tron ooler has been optimizedforele tron energies
up to 100 keV, enabling phase spa e ooling up to 183.6 MeV proton
energy. Its basi appli ation is redu ing the large emittan e and the
large momentum spread due to the inje tion stripping pro ess before
the ion beam is a elerated to the requested energy[23 ℄. The ele tron
beam is extra ted from a thermioni athode and ele trostati ally
a - elerated up to the velo ity ion beam. The ele tron beam is driven
by the longitudinal magneti eld provided by toroids and solenoids
through the region of intera tion with the ionbeam and, after energy
re overing by ele trostati de elaration, it enters the olle tor. Two
solenoids with reversed longitudinal eld up- and downstream of the
ooler devi e hinder oupling between horizontal and verti al phase
spa e plane and distortionof the ionspin dire tionin the COSY ring.
Steerer magnets balan e the orbit distortion indu ed by the toroids
and enable the mat h between the ion beam and the ele tron beamin
positionandinangle. Whentheoptimumsettingisfound, theele tron
beam anbetiltedby steering oils onthe driftsolenoidand itslightly
redu ed its ooling for e.
2.2 PAX beam polarimeter
Thebeampolarizationismeasuredusingthe Sili onTra kingT
ele-s opes(STTs)dete tionsystem,pla edattheANKEintera tionpoint,
see Fig.2.1. As des ribed in detail in se tion 3, the beam polarization
an be determined exploiting the left-right asymmetry of the sele ted
deuteronsfromproton-deuteronelasti s attering,wherethedeuterium
is delivered fromthe ANKE Deuterium lustertarget[24℄.
2.2.1 Deuterium luster target
ADeuterium luster targetispla edatthe internaltargetposition
of the ANKE experiment. It provides a target density of
10
13
-
10
15
atoms/
cm
2
and a target beam of 10 mm diameter, entailing a small
beam target overlap. Clusters of
10
3
-
10
4
atoms are delireved from a
Figure 2.2: As hemati view of theDeuteriumClusterTargetis shown. The luster
sour epla edabovetheCOSYbeamprovidesawell-denedtargetbeamofhydrogenor
deuterium lusters. The olle torse tionkeepstheva uumbelow
10
−7
mbar.
range of 15-20 bar, the gas is for ed into the va uum of the skimmer
hamber using the Laval-nozzle of 20
µm
opening diameter. On e insidetheskimmer hamber,the gasexpandsadiabati allyand it oolsdown. Inoversaturated gas onditions,the ondensationof atomsinto
lusterstakespla e. Thereareabout
10
3
atoms losetothetriplepoint
per luster. The skimmer provides the separation of the luster beam
from the residual gas whi h is the main omponent of the total gas
load into the skimmer hamber. The target se tion alled olle tor,
see Fig.2.2hosts adierentialpumpingsystem(three ryo-pumpsplus
one turbomole olar pump) whi h limits the gas load into the target
hamber, keeping the va uum below
10
−7
mbar.
Figure2.3: ThetwoSili onTra kingTeles opespla ed olsetothebeam-targetoverlap
regioninthetarget hamberisshown. Thepolarizedprotonbeam(redline)enters the
hamberandhitsthedeuterium lustertarget(yellowline),inje tedfromthetop.
2.2.2 SILICON TRACKING TELESCOPES
Thedete tionsystem onsistsoftwogroupsofsili onstripdete tors
arranged in a teles opelayout aroundthe beam targetoverlap region.
A Sili onTra kingTeles opeis madeby three double-sidedmi rostrip
dete torsofdierentthi kness;therstlayer anbeof65
µm
or300µm
thi kness, the se ond layer of 300µm
thi kness and the third layer is a5100 µ
m sensor tomaximize the number of stopped parti les. This system is able to fullllthe followingtasks:•
Identi ationofstoppedparti lesbythe∆
E/Emethod,providing inparti ular the protonidenti ationinthe kineti energy range2.5 − 40
MeV with a resolution of 150 keV.•
Parti le tra king over a large energy range, from2.5
MeV up to minimum ionizingparti les(MIP); vertex resolution of 1 mm.•
Self-triggering apabilitiesrealizedbyafastamplierwitha peak-ingtimeof75
nsbymeansofwhi haparti lepassageisregistred fast and provide a trigger; in this way the system behaves like astand-alone dete tor.
Theparti leidenti ation, ru ialforthe polarizationmeasurement,is
realizedusingthe
∆
E/Emethodanalysingthe orrelationbetweenthe energy lossin dierent layers, as des ribed in se tion3.The dete tors used for the rst two layers of the STTs are the BaBar
IVdete torsandhavebeenoriginallydesignedbythe ompanyMi ron
Ltd[25℄fortheBaBarexperiment[26,27,28,29,30℄attheSLAC
PEP-II B fa tory. The size of their a tive area is 51mm
×
62mm and the strip pit his of 400µ
m.The p-doped side has 1023 strips, whereas the n-doped side has 631
strips. In order to in rease the ee tive strip pit h up to 400
µ
m, the strips are arranged intogroups that are onne ted tosegments onthe kapton at able used to onne t the dete tor and the front-end
ele troni s (see Fig.2.4for the onne tion s heme).
A va uum-feedthrough for ea h segment is not appli able be ause of
the large number of the readout hannels, one per segment, so the
front-end ele troni s isused inva uum.
Thethi kLithiumdriftedSili ondete torsSi(Li)[31℄usedforthethird
layer has an a tive area of 64 mm
×
64 mm and a strip pit h of 666µ
m (96 strips per side). They have been developed in the dete tor laboratoryof the Institut fürKernphysik (IKP) ofFZJ. They allowtostopparti lesuptoanenergyofabout32MeVforprotonsand43MeV
for deuterons.
2.2.3 Front-end ele troni s
The signals oming from the sili on sensors are transported tothe
in-va uum front-end ele troni s by kapton at ables. The VA32TA2
hips are used. The hip provides a low trigger threshold of 100 keV;
two boards 90 mm
×
90 mm (one per dete tor side) with 5 hips are utilized. The front-end ele troni s onsists of 32 hannels logi allyseparated into an amplitude and a trigger part. In the preamplier
stage, a harge signal in the input pad of the hannel is amplied
and then split into the two bran hes. The pre-pro essed signals are
driven by addi tional kapton at ables to the va uum feedthrough
onne tors. The onne tors are pla edonthe ele troni s tofavour the
dismounting of the kapton at ables inorder tofulllthe modularity
request.
Figure2.4: The onne tions hemeofthep-dopedside(a)andn-dopedside(b)ofthe
BaBarIVdete tor.
trigger pattern threshold and alibration pulse amplitudes. The total
read-out hain ontributes toa total dead time of less than 50
µ
s.2.2.4 Geometry and Trigger
The displa ement of the STTs has been optimized to measure the
beam polarization in proton-deuteron elasti ollisions a ording to
Monte Carlosimulations.
The geometry of the setup has to meetthese requirements:
Figure2.5: Thein-va uumfront-endele troni boardisshown,withtheinput/output
onne torsandthefront-end hipsindi ated.
Figure2.6: Intheleftpi tureonesili on-dete torwiththefront-endele troni boards
andkaptonplat ables isshown;intherightpi ture thenalassemblyfor onedete tor
in ludingthe oolingplatefortheele troni boardisdisplayed. Figurestakenfrom[42 ℄.
•
the setup has to be arranged in an azimuthal symmetry (left-right) inφ
to use the double-ratio method for the asymmetry measurements,that serve to al ulatethe beam polarizationandanalysingpowers, see Chapter 3.
a eptan e toallow forthe setupalignment.
Figure 2.7: S hemati view of the zx plane of the dete tor (thebeam is along the z
dire tion). Targetpositionanddistan esbewteenlayersareindi ated.
The beam polarizationP isdeterminedusing theleft-rightasymmetry
ǫ
of the s attered deuterons. This asymmetry is proportional to the analysing powerA
y
of the pd elasti s attering through the relation:ǫ = P · A
y
.
(2.1)The STT is pla edin the region wherethe pd elasti Figure Of Merit
(FOM)dened by:
F oM =
dσ
dΩ(θ
cm
)
·
(A
y
(θ))
2
,
(2.2)exhibits the maximum value.
A ording to experimental data at
T
p
= 46.3
MeV, see Fig.2.8, it is taken in onsideration the FOM value atθ
p
cm
=110
o
(that in the
labo-ratory is
θ
p
lab
= 80
o
), sin e the rst peak orresponds to angles in the forward s attering region where itis not possibleto pla e the STT.To optimize the FOM the STT was pla ed 12 mmdownstream along
the beam dire tion. Therst layeris pla edat28mmfromthe enter
of the beam pipe to prote t the dete tor; the distan e between rst
and se ond layer is 20 mm. The distan e between se ond and third
layer is 13.5 mm. The trigger signal was produ ed when at least one
Figure 2.8: In the upper panels the pd elasti dierential roos se tion is
rep-resented in the enter of mass and laboratory system. In the lower panels the
Analysingpower
A
y
andtheFigureofMeritFoMofthepd elasti s atteringinthe enterofmasssystemaredisplayed.Figure 2.9: The omplete setup of aSili on Tra kingTeles ope is shown. The three
sili on mi rostrips sensors are indi ated as well as the kaptonat ables that link the
Deuteron Breakup events
analysis
The pd
→
ppn Deuteron Breakup hannel has been studied using Monte Carloand experimentaldata.The ultimategoalof the analysisis the sele tionofpd Breakup andin
parti ular theidenti ationofthe neutron. The identiedpd Breakup
events areusedtodevelop amethodfor al ulatingtheanalysing
pow-ers
A
y
of pd Breakup with respe t to the neutron.The presented data had been taken during the February 2008 beam
time, when an experiment to test the possibility of using unpolarized
ele trons to depolarize an initially polarized proton beam was
per-formed at the COSY-ring. A polarized proton beam was stored in
COSY and the ele trons of the ele tron- ooler have been employed as
free ele tron target. The depolarization of the beam , aused by the
intera tions with the ele trons, was monitored measuring the beam
polarizationby means of the proton-deuteron elasti s attering events
indu ed at the deuteron luster target [32℄.
In these experimental onditions, proton-deuteron ollisions an give
rise to Deuteron Breakup events. Sin e the experimentalsetup is able
to identify this rea tion, DeuteronBreakup hannel an be studiedas
a omplete independent Physi s ase.
In this hapter the data analysis pro edure to re onstru t Deuteron
Breakup events, insimulatedandexperimentaldata,and inparti ular
the sele tion riteriadeveloped to tag thisrea tion are des ribed. The
identied deuteron breakup events are employed in the method
with respe t tothe neutron.
3.1 pd Breakup vs pd elasti
When a proton beam of 49.3 MeV kineti energy impinges on a
deuteriumtarget, two hannels an be a essible: pd elasti s attering
pd → pd
and Deuteron Breakuppd → ppn
. In the experimental data these two hannels are present together and need to be separated.Whilethe phase spa eof the pd elasti hannel iswelldened, the pd
Breakup, being a three-body nal state rea tion, o upies a broader
phasespa ewhi hoverlapstotheelasti one. The basi ideatoisolate
the pd Breakup hannel is to ex lude the pd elasti hannel from the
phase-spa eandgetalltheinfomationsfromthetwooutgoingprotons.
This se ond requirement is ne essary sin e the neutron is invisible for
the used dete tion system and pd Breakup ould be identied when
the two outgoing protons stop inside the dete tor a eptan e. On e
the two protons are stopped, using the four momentum onservation,
the ompletekinemati anbedetermined. Thefour-momentumofthe
missingneutron isgiven by:
n
µ
= p
µ
Beam
+ d
µ
T arget
−
p
µ
1,T elescope
−
p
µ
2,T elescope
,
(3.1) in whi hp
µ
Beam
is the four-momentum of the in oming proton,d
µ
T arget
the four-momentum of the deuteron target (it is a xed target, so it
oin ides with the deuteron mass),
p
µ
1,T elescope
andp
µ
2,T elescope
thefour-momentum of two outgoingprotons dete ted and stopped in the
tele-s opes.
On e the protons from pd Breakup events are sele ted, the Missing Mass:
M
missing
=
q
(E
Beam
p
+ m
d
−
E
p1
−
E
p2
)
2
−
(−
→
p
p
Beam
− −
→
p
p1
− −
→
p
p2
)
2
(3.2)is used as a ontrol riteria to tag the rea tion and it should peak at
the Neutron mass
939.57
MeV/c
2
. In equation 3.2,E
p
Beam
and−
→
p
p
Beam
are the total energy and 3-momenta of the in oming proton,
m
d
the
deuteron mass,
1875.61
MeV/c
2
,
E
p1
,E
p2
are the total energies of the two outgoing protons,−
→
p
p1
and−
→
p
p2
are the 3-momenta of the two outgoingprotons.3.1.1 Kinemati s of
pd → ppn
Ingeneralinarea tion
A + B → 1 + 2 + 3
withtwo initialparti les and three parti lesin thenal state,3 × (2 + 3)
momenta omponents have to be dened. The momentum-energy onservation laws x fourrelations between momenta omponents of the parti les in the initial
and nal state; moreover if the enter of mass system is used, one an
dene three onditions forthe initialstate derived by:
−
→
p
c.m.
A
+ −
→
p
c.m.
B
= 0,
(3.3)and three onditions for the nal state:
−
→
p
c.m.
1
+ −
→
p
c.m.
2
+ −
→
p
c.m.
3
= 0.
(3.4)Therefore a three-nal state hannel an be des ribed by means of
3 × (2 + 3) − 4 − 3 − 3 = 5
independentvariables.In the ase of pd Breakup rea tion the ve independent variables
the ja obi momenta p and q, and the ex itation energy of the proton
pair
E
pp
dened as:E
pp
=
q
(E
p1
+ E
p2
)
2
−
(−
→
p
p1
+ −
→
p
p2
)
2
−
2m
p
,
(3.5) whereE
p1
,E
p2
,−
→
p
p1
and−
→
p
p2
are the total energies and the 3-momenta of the twooutgoingprotons andm
p
is the proton mass.Figure3.1: Ja obimomentaof
pd → ppn
inthe enter-of-masssystem. p=1/2(p1+p2)andq=-(p1+p2).
3.2 Simulations and Data
The data analysis is divided in two stages: one on erning Monte
Carlo simulationsand the other experimentaldata.
Inordertoestimatethe expe teddete tor performan es andin
parti -ular to study the re onstru tion e ien y for pd Breakup events and
thepd elasti ontamination,dierentsamplesofsimulatedpd Breakup
and pd elasti events have been analyzed, implementing the February
2008 dete tor onguration.
Thepd elasti s atteringisgeneratedbasedexperimentaldata[33℄. The
lowenergypd Breakupisgeneratedintheframeworkofthepure
phase-spa e GENBOD model with the proton beam kineti energy of 49.3
MeV. The GEANT pa kage [34℄ was used for the dete tor response.
The output of the simulations onsists of a list of events ontaining
hits informations like spatial oordinates, angles and deposited
ener-gies.
Simulated hannel Number of generated events pd
→
pd10
6
,T
p
=49 MeV pd→
ppn10
6
,Tp
=49 MeVTable 3.1: ThistabledisplaysMonteCarloinformations on erningthe hannel
simu-latedandthenumberofgeneratedeventsforea h hannel.
Con erning experimental data, the exe ution of the primary data
analysis, energy alibration orre tion, hits and tra king analysis is
ontrolledbytheRootsorter frameworksoftwaredevelopedatIKP[35℄.
The output is arranged in a list of events with omplete event
identi- ation data (i.e. time, beam polarization index, target polarization,
et .) and hits informations. Ea h hit ontains the information about
the energy loss of the parti le and its position in the dete tor. In the
next se tionthetra kre onstru tionandthepd Breakupidenti ation
te hniques (used either inMonte Carloor data) are des ribed.
3.2.1 RUN SELECTION
The data taking was performed with
10
8
stored protons. For this
analysis seven runs have been analyzed. During ea h run the proton
beam polarization was alternated between state UP (
↑
), DOWN (↓
) and unpolarized (0). The geometry is represented in Fig.3.2. Duringthe beam time the third layerin one teles opewasnot working.
Date RUN Start Stop Events
Feb 03,2008 260 16:49 17:00 1360305 Feb 03,2008 262 17:06 17:16 1364067 Feb 03,2008 264 17:16 17:26 1362196 Feb 03,2008 266 17:26 17:36 1350207 Feb 03,2008 267 17:36 17:58 1368407 Feb 03,2008 270 18:15 18:27 1352119 Feb 03,2008 272 18:36 18:50 1174226
Table3.2: Thistable ontainssomeinformationsontherunsofFebruary2008analysed
Figure3.2: Intheuppergure,thezxplaneofthedete torisshown. Theprotonbeam
isdire tedalongthepositivesideofthezaxis. Theprotonbeampolarization isdire ted
along y-axis. The indi ated angles show the geometri al a eptan e of the polar angle
whena s attered parti le impinges on the rst two layers. Inthe lower gure, the yx
plane,lookinginthebeamdire tion,isshown.
3.3 Tra k Re onstru tion
A tra k is dened as a straight line between two orrelated hits
in the rst two layers. Firstly ontiguous signals (within a radius of
1 mm) in the sili on strips are merged together into the so- alled
sili- on hits. Only events with at least two hits inthe rst layers and one
hit in the se ond layer of the dete tor are onsidered. Se ondly the
in azimuthal angle.
Ahitinthe thirdsili onlayerislinked tothere onstru ted tra k if its
distan e from the extrapolatedpointof the tra k is less than 1 m.
Ineventswheretwotra ksaretra ed,themethodofdistan eof losest
approa h is applied to re onstru t the intera tion vertex. Whereas in
eventsinwhi honlyonetra kistra ed,themethodofdistan eof
los-est approa hisappliedbetween the tra k andthebeamlinetolo alize
the vertex point; after that the se ond tra k is tra ed onne ting the
vertex pointto the oordinates of any untra ed hitin the rst layer.
Three tra k typologies are onsidered: tra k "1", if the parti le stops
into the rst layer, tra k "2" and "3", if the parti le stops into the
se ond orthe third layer respe tively, see Fig.3.3.
Figure3.3: S hemati viewofthezxdete torplaneinwhi htra k1,2 and3are
repre-sented.
InMonteCarlo,pd elasti andpd Breakup hannels anbeswit hed
onseparately, whereas indata they are present together; the rst part
of the analysis is dedi ated to the identi ation and separation of the
two rea tions.
The request to suppress the elasti hannel to negligible ontribution
is realized applying a o-planarity ut, shown in Fig.3.4. This ut,
in addition to the request of having no deuterons in the nal state,
2
Θ
+
1
Θ
60
80
100
120
140
160
180
200
|
2
Φ-1
Φ|
50
100
150
200
250
300
350
2
Θ
+
1
Θ
60
80
100
120
140
160
180
200
|
2
Φ-1
Φ|
50
100
150
200
250
300
350
2
Θ
+
1
Θ
60
80
100
120
140
160
180
200
|
2
Φ-1
Φ|
50
100
150
200
250
300
350
Figure 3.4: MonteCarlo: the o-planarity ut. Therelationbetweenthe polarangles
ofthe2-outgoingparti lesversustheirazimuthalangleisdisplayed.Theleftpanelshows
thephasespa eofthepdelasti hannelinsimulations,themiddlepanelshowsthephase
spa e of the pd elasti (red) and pd Breakup hannel (blue) together, the right panel
displaysthe phase spa e of pdBreakup inwhi h theellypse-like area of pdelasti has
beenex luded;inthiswaythemain on entrationofpdBreakupremains.
3.3.1 Parti le Identi ation
Theenergylossinformation arriedby hitsprovidesthesele tionof
the harged parti les by the
∆E
/E and Parti le IDenti ation (PID) methods. These twomethodsare developed ombiningthe energylossdete ted in the Sili on Tra king Teles ope and the energy lossof
par-ti les inmatter, asdes ribed by the Bethe-Blo k formula:
−
dE
dx
=
4πnz
2
m
e
v
2
·
(
e
2
4πǫ
0
)
2
·
ln
2m
e
v
2
I
,
(3.6)where v is the velo ity of the in oming parti le,
ǫ
0
the va uum per-mittivity,m
e
the ele tron mass, n the ele tron density, z the atomi number and I the average ionizationenergy.Showing
E
1
, the deposited energy in the rst layer, as fun tion ofE
2
thedepositedenergy inthese ondlayer,one ansee thatdierentpar-ti les populate dierent regions of the phase-spa e (
∆E/E
method). Theborderlineoftheseregionsisbroadsin etheparti lespassthroughmore orless dete tor materialdependingon the in ident angles.
Tosimplify proton/deuteron separation, the PID method an be
ap-plied; in this ase the energy loss are parametrized by the so- alled
parameter dened as follow:
Figure3.5: MonteCarlopdelasti andpdBreakuptogether.Intheleftpanelthe
∆
E/Eplotisshown. InMonteCarloaagtags parti lesas protons(bluepoints)or deuterons
(redpoints); protons and deuteronspopulatedierent lo iof the phasespa e. Looking
atthe deuterons(same isfor protons),theupperband orrespondsto parti lesstopped
inthe
2
nd
layera eptan eandthe lowerband orrespondsto deuteronshavingenough
energytopassthroughthe
2
nd
layer. Heredeuterons anmissthe
3
rd
layeror anenter
the
3
rd
layerandstopbe auseofitsthi kness. Inthisregiondeuteronslayonthestopped
protonsband. Ifthesedeuteronsenterthe
3
rd
layer,they anbeseparatedfromprotons,
otherwisethe separation betweenprotons and deuteronsis notappli able. Inthe rigth
panelthePID utisshown. Usinganenergyparametrizationitispossibleto onvertthe
leftplotintherightoneinwhi htheprotons-deuteronsseparationisrealizedapplyinga
horizontal ut.
Figure 3.6: Experimentaldata. Intheleft panelthe
∆
E/Eplotisshown, aagindi- atingprotonsordeuteronsisnolongeravailable. Thesele tionofprotonsanddeuterons
anbe arriedoutwithalinear ut(magentaline)whi hdividestheplaneinprotonsand
deuteronslo i. Thesame onsiderationsfortheoverlappingprotons-deuteronsregionsare
appliedhere. Intherigthpanel thePID utisshown, theseparationis realizedusinga
A ut around the horizontal band (see Fig.3.6) allows the separation
between protonsand deuterons.
Afterhavingseparatedthetwo hannels,thefurtherstepoftheanalysis
isaimedtoidentifythetra kswithtwoprotonsstoppedinthedete tor.
3.3.2 Tra k "1" re onstru tion
Whenaparti lestopsintherstlayerislabelledastra k"1". Tra k
"1" is sele ted by means of a geometri al ut in whi h the parti le is
supposedtohaveonehitintherstlayeranditstra k,originatingfrom
the target region, is proje ted in the forward dire tion to he k if it
inter epts these ondlayera eptan e. Sin etheparti leidenti ation
is not appli able in the rst layer, to eliminate the high ba kground
fromdeuteronsstoppedintherstlayer,a o-planarity ut isrequired.
Figure3.7: Sele tionofprotontra k"1". YZplaneofthese ondlayer. The yanpoints
referstothe nominalpositionofthe
2
nd
layer; the pinkpointsareproje tionsof tra ks
withonehitinthe
1
rst
layerthatmissthe
2
nd
layera eptan e. Ifaproje tionbelongs
tothe
2
nd
layera eptan eandno orrelatedhitisfoundthenitislabelledastra k"1".
3.3.3 Tra k "2" re onstru tion
Tra k "2" refers toparti les stopped in the se ond layer of the
IDen-ti ation(PID) methods. Parti les displayed inFig.3.6 are those that
pass the rst layer and give rise to a signal in the se ond layer.
Par-ti les with the highest energy loss in the rst layer have a low energy
loss in the se ond; as the energy of the parti le in reases, the energy
loss inthe se ond layer in reases and the deposited energy inthe rst
layerde reases,sin etheenergylossisproportionalto1/
v
2
. Theupper
Figure 3.8: Experimental data. In the left panel the
∆
E/E plot and in the rightpanelthePIDplotaredisplayedinboth aseswithoutthedeuteronslo i;herethemain
on entrationofpdBreakuphasbeenidentied. Protonsstoppedinthese ondlayerare
isolatedsele tingthebandboundedbythepinklines.
bands are populated by deuterons andprotons respe tively stopped in
the se ond layer and their initial kineti energy is determined by the
sum of the deposited energy in the rst two layers. The lower bands
are populated by protons and deuterons that pass through the se ond
layer a eptan e and an enter the third layer. Restri ting our
analy-sis to protons, the sele tion of a tra k "2" proton is arried out with
theserequirements: rsttwolayersred, theparti leshouldlayonthe
stopped protonsregions (see Fig.3.8)and no hits onthe third layer.
3.3.4 Third layer Calibration
Before dis ussing the re onstru tion of Tra k "3", it is here
pre-sented the alibration pro edure of the third layer. The thi kness of
the third layerrequired the use of apa itors to a omplish the
atten-uation of the input signal, therefore the deposited energies have to be
alibrated to get the orre t value. At this aim, the
∆
E/E plots (2
versus
3
rd
layer)inMonteCarloandexperimentaldatahavebeen
om-pared inorder tomakethem oin ide.
The resultsof this alibrationhas the ee t ofshifting the peak ofthe
MissingMassdistributiontothe orre tvalue, asreportedinFig.3.11.
Figure3.9: The
∆
E/Eplotdisplayingtheenergylossin2
nd
layerversusenergylossin
3
rd
layerisshownforMonteCarlo(leftpanel)andexperimentaldata(rightpanels). The middlepanelshowsexperimentaldatawithoutthe alibration, theright panelrepresentsexperimentaldataaftertheenergy alibration. The alibrationhasbeenrealizedmaking
theenergylossesshownintherstandse ondpanel oin ide.
3.3.5 Tra k "3" re onstru tion
A tra k labelled as "3" is originated by a parti le stopped in the
third layer and is sele ted using the plot representing
E
2
, the energy loss in the se ond layer, as a fun tion ofE
3
, the energy loss in the third layer. The upper band refers to deuterons entering the thirdlayer. Deuterons that rea h the third layer, due to its thi kness, are
here stopped. The lower band in the
∆
E/E plot refers to protons. Also in this ase a parametrization of the deposited energies an beused todisantangle protonsand deuteronsand toidentify the stopped
parti les:
c
3
= (E
1
+ E
2
+ E
3
)
1.7
−
E
3
1.7
(3.8)The sele tionof a"3" tra kprotonis madelookingfor3-hits tra ksin
the proper region of the phase spa e of protons stopped in the third
Figure 3.10: Experimentaldata. Inthe upperbox the
∆
E/Eplot(leftpanel)for2
nd
and
3
rd
layer anditsparametrization PIDplot (right panel)are shown, onsideringpd
elasti and pd Breakup. Applying the ut identied by the pink line, one an sele t
protons or deuterons. Inthe lower panel
∆
E/E plot and PID plotwithout pdelasti .Protons labelledas tra k "3"are isolated applyingthe ut indi ated by the pinklines,
whi hsele tstheprotonsstoppedinthe
3
rd
layer.
Figure 3.11: Experimental data: run 260. The Missing Mass distribution is shown
3.4 Deuteron Breakup samples
The ombinationoftwostopped-protonstra ks(1,2or3)generates
veeventsampleslabelled2-1,2-2,3-1,3-2,3-3referringtothenumber
of hits in ea h tra k. These event samples are investigated separately
as they populate dierent lo i of the phase spa e. Every sample is
identied by meansof a ombinationof thesele tion riteriades ribed
above.
•
2-1 sample: This ategory is identied applying the param-eter ut and the tra k "1" geometri al ut. In addi tion theo-planarity ut is applied be ause of the high ba kground of
deuterons stopped inthe
1
rst
layer.
Figure3.12: 2-1sample. Upperpanels: MonteCarlo.Theleftpanelshowsthesele tion
toidentifytheprotonsstoppedinthe
2
nd
layer, themiddlepanelshows thegeometri al
ut on the proje tion of the tra k to identify protons stopped in the
1
rst
layer. The
right panel displaysthe MissingMass distributions: thered onerefers tore onstru ted
events(21seventsthatenterthegeometri ala eptan ebutnotne essarilystopped),the
green onerefers to generated stopped events (21s eventsthat are stoppeda ording to
simulations),theblueonereferstotheeventsstoppedusingthesele tion riteria. Lower
panels: DATA.Startingfromtheleftthesele tionstoidentifystoppedprotonsinthe
2
nd
and
1
rst
layerareshown. IntherightpaneltheMissingMassforre onstru ted(red)and
•
2-2 sample: This ategory is identied applying the parameter and the o-planarity ut.•
3-1 sample: This sample is identied applying the 3 parameter (eq.3.8)and thetra k"1" geometri al ut;the o-planarity utisappliedfor the reasonalready mentionedfor the 2-1sample.
E1+E2 (MeV)
0
5
10
15
20
25
30
35
c (MeV)
20
40
60
80
100
z (cm)
-4
-2
0
2
4
6
8
y (cm)
-6
-4
-2
0
2
4
6
MM31geant
Entries 4543
Mean 939.3
RMS 1.867
)
2
Neutron Mass (MeV/c
910
920
930
940
950
960
970
0
200
400
600
800
1000
1200
1400
1600
MM31geant
Entries 4543
Mean 939.3
RMS 1.867
MM31stop
Entries 5785
Mean 938.2
RMS 3.747
MM31stop
Entries 5785
Mean 938.2
RMS 3.747
MM31rec
Entries 20860
Mean
938.2
RMS
4.861
MM31rec
Entries 20860
Mean
938.2
RMS
4.861
Missing Mass 31
E1+E2 (MeV)
0
5
10
15
20
25
30
35
c (MeV)
20
40
60
80
100
z (cm)
-4
-2
0
2
4
6
8
y (cm)
-6
-4
-2
0
2
4
6
Entries 5785
Mean 939.9
RMS 5.136
)
2
Neutron Mass (MeV/c
910
920
930
940
950
960
970
0
100
200
300
400
500
600
700
Entries 5785
Mean 939.9
RMS 5.136
Missing Mass 31
Entries 22186
Mean
940.9
RMS
7.102
Entries 22186
Mean
940.9
RMS
7.102
0
200
400
600
800
1000
1200
1400
1600
Figure 3.13: 3-1sample: inthe upperpanels: MonteCarlo. Theleftpanel shows the
sele tion to identifythe protons stopped inthe
3
rd
layer. Inthe middlepanel, the ut
forprotonsstoppedintherstlayerisrepresented. TherightpaneldisplaystheMissing
Mass distributions: the red one refersto re onstru tedevents, the green one refers to
generated stoppedevents,the blue one refersto the eventsstoppedusing the sele tion
riteria. Lowerpanels: DATA.Sameplotsasmentionedabovebutdisplayedfor data.In
therightpaneltheMissingMassfor re onstru ted(red)andstopped(blue)31sevents.
•
3-2 sample: This sample is identied applying the 3 parameter (eq.3.8)and the parameter(eq.3.7) sele tion; the requestof the3.5 E ien y of Breakup identi ation
The Missing Mass of the dierent samples are shown for Monte
Carlo,seeFig.3.14anddata, seeFig.3.15. TheMissingMassisapplied
as a ontrol riteria to tag a breakup event. The number of events
identied for ea h run is displayed in Table 3.2.
Figure3.14: MonteCarlo.TheMissingMassdistributionisshownfortheBreakupevent
samplesinviduallyandtogether(bottomright).RED:theMissingMassforre onstru ted
events(eventsnotne essarystoppedinsidethedete tora eptan e),GREEN:theMissing
Mass for generated stoppedevents(events inwhi hgenerated andre on truted energy
oin ides), BLUE:the MissingMass forstoppedevents(eventsidentiedwithsele tion
Figure 3.15: Experimental data: The Missing Mass distribution is shown for the
Breakup event samples invidually and together (bottom right) for a single run. These
MONTE CARLO
Monte Carlo 21 22 31 32 ALL
Re onstru ted 26280 3765 30131 10122 74595
Truly Geant Stopped 3518 417 6823 2511 17141
Stopped 2361 419 4870 2612 14280
Table3.3: MonteCarlostatisti s:thistable ontainsthenumberofre onstru tedevents
(eventsthatenterthedete tora eptan ebutnitne essarilystopped),trulygeantstopped
events(eventsinwhi hgeneratedandre onstru tedenergies oin ide)andstoppedevents
(eventsthatfulllthesele tion riteria). The ountsarereportedforea hsampleandall
together. DATA RUN 21 22 31 32 ALL 260 4299 188 5785 10730 21002 262 4073 162 5843 10780 20858 264 4178 145 5795 10741 20859 266 4015 189 5771 10409 20384 267 3821 174 5701 10305 20001 270 3489 165 4948 9265 17867 272 3178 131 4841 9055 17205
Table 3.4: Numberof identieddeuteron breakup events for ea hsample and for all
samples onsideredtogetherinexperimentaldata. Thepresen eofthethirdlayerof5mm
in reasesthestoppingeen ybyafa tor3withrespe ttothestoppinge ien yofthe
rst two layers. The 3-3 sampleis not onsidered sin e one of the thirdlayerwas not
workingduringthewholebeamtime.
3.6 Phase Spa e Coverage
The identied Breakup samples populate dierent regions of the
phase spa e. The ja obi momenta of the identied samples are
dis-played in Fig.3.16, 3.17, 3.18, 3.20, 3.21, 3.22, 3.23 to show the phase
MeV/c
20
40
60
80
100 120 140 160 180
0
50
100
150
200
250
P sample 21
P sample 21
MeV/c
20
40
60
80
100 120 140 160 180
0
5
10
15
20
25
P sample 22
P sample 22
MeV/c
50
100
150
200
250
300
0
50
100
150
200
250
Q sample 21
Q sample 21
MeV/c
50
100
150
200
250
300
0
2
4
6
8
10
12
14
16
18
Q sample 22
Q sample 22
Figure3.16: Experimentaldata: Ja obimomentapandqfor 2-1and2-2samples. In
parti ular,qrepresentstheneutroninthe enterofmasssystem.
MeV/c
20
40
60
80
100 120 140 160 180
0
50
100
150
200
250
P sample 31
P sample 31
MeV/c
20
40
60
80
100 120 140 160 180
0
200
400
600
800
1000
1200
1400
1600
P sample 32
P sample 32
MeV/c
50
100
150
200
250
300
0
50
100
150
200
250
300
350
400
Q sample 31
Q sample 31
MeV/c
50
100
150
200
250
300
0
200
400
600
800
1000
1200
1400
1600
1800
2000
2200
2400
Q sample 32
Q sample 32
Figure3.17: Experimentaldata: Ja obimomentapandqfor 3-1and3-2samples. In