scieee Open visual document viewer

Measuring K0SK± interactions using Pb–Pb collisions at √sNN=2.76 TeV

ALICE Collaboration; González Ferreiro, Elena

Abstract

We present the first ever measurements of femtoscopic correlations between the K0Sand K±particles. The analysis was performed on the data from Pb–Pb collisions at √sNN=2.76TeV measured by the ALICE experiment. The observed femtoscopic correlations are consistent with final-state interactions proceeding via the a0(980)resonance. The extracted kaon source radius and correlation strength parameters for K0SK−are found to be equal within the experimental uncertainties to those for K0SK+. Comparing the results of the present study with those from published identical-kaon femtoscopic studies by ALICE, mass and coupling parameters for the a0resonance are tested. Our results are also compatible with the interpretation of the a0having a tetraquark structure instead of that of a diquark.

Full text

Physics Le e s B 774 (2017) 64–77 Con en s lis s a ailable a ScienceDi ec Physics Le e s B www.else ie .com/loca e/physle b Measu ing K0 SK±in e ac ions using Pb–Pb collisions a √sNN =2.76 TeV .ALICE Collabo a ion a i c l e i n o a b s a c A icle his o y: Recei ed 22 May 2017 Recei ed in e ised o m 24 Augus 2017 Accep ed 4 Sep embe 2017 A ailable online 8 Sep embe 2017 Edi o : L. Rolandi We p esen he fi s e e measu emen s o em oscopic co ela ions be ween he K0 Sand K±pa icles. The analysis was pe o med on he da a om Pb–Pb collisions a √sNN =2.76 TeV measu ed by he ALICE expe imen . The obse ed em oscopic co ela ions a e consis en wi h final-s a e in e ac ions p oceeding ia he a0(980) esonance. The ex ac ed kaon sou ce adius and co ela ion s eng h pa ame e s o K0 SK−a e ound o be equal wi hin he expe imen al unce ain ies o hose o K0 SK+. Compa ing he esul s o he p esen s udy wi h hose om published iden ical-kaon em oscopic s udies by ALICE, mass and coupling pa ame e s o he a0 esonance a e es ed. Ou esul s a e also compa ible wi h he in e p e a ion o he a0ha ing a e aqua k s uc u e ins ead o ha o a diqua k. ©2017 The Au ho . Published by Else ie B.V. This is an open access a icle unde he CC BY license (h p://c ea i ecommons.o g/licenses/by/4.0/). Funded by SCOAP3. 1. In oduc ion Iden ical boson em oscopy, especially o iden ical cha ged pi- ons, has been used ex ensi ely o e he yea s o s udy expe i- men ally he space– ime geome y o he collision egion in high- ene gy pa icle and hea y-ion collisions [1]. Iden ical-kaon em- oscopy s udies ha e also been ca ied ou , ecen examples o which a e he ones wi h Au–Au collisions a √sNN =200 GeV by he STAR Collabo a ion [2] (K0 SK0 S) and wi h pp a √s=7TeV and Pb–Pb collisions a √sNN =2.76 TeV by he ALICE Collabo a- ion [3–5] (K0 SK0 Sand K±K±). The pai -wise in e ac ions be ween he iden ical kaons ha o m he basis o em oscopy a e o K±K±quan um s a is ics and he Coulomb in e ac ion, and o K0 SK0 Squan um s a is ics and he final-s a e in e ac ion h ough he 0(980)/a0(980) h eshold esonances. One can also conside he case o non-iden ical kaon pai s, e.g. K0 SK±pai s. Besides he non- esonan channels which may be p esen , e.g. non- esonan elas ic sca e ing o ee-s eaming o he kaons om hei eeze-ou posi ions o he de ec o , he o he only pai -wise in e ac ion allowed o a K0 SK±pai a eeze ou om he collision sys em is a final-s a e in e ac ion (FSI) h ough he a0(980) esonance. The o he pai -wise in e ac ions p esen o iden ical-kaon pai s a e no p esen o K0 SK±pai s because: a) he e is no quan um s a is ics enhancemen since he kaons a e no iden ical, b) he e is no Coulomb e ec since one o he kaons is uncha ged, and c) he e is no s ong FSI h ough he 0 eso- E-mail add ess: [email p o ec ed]. nance since he kaon pai is in an I=1 isospin s a e, as is he a0, whe eas he 0is an I=0s a e. Ano he ea u e o he K0 SK±FSI h ough he a0 esonance is, due o he a0ha ing s angeness S=0 and he K0 Sbeing a linea combina ion o he K0and K0, K0 S=1 √2K0+K0,(1) only he K0K+pai om K0 SK+and he K0K−pai om K0 SK−ha e S=0 and hus can o m he a0 esonance. This allows he pos- sibili y o s udy he K0and K0sou ces sepa a ely since hey a e indi idually selec ed by s udying K0 SK−and K0 SK+pai s, espec- i ely. An addi ional consequence o his ea u e is ha only 50% o ei he he K0 SK−o K0 SK+de ec ed pai s will pass h ough he a0 esonance. This is aken in o accoun in he exp ession o he model used o fi he co ela ion unc ions. On he o he hand, he na u al equi emen ha he sou ce sizes ex ac ed om he K0 SK± em oscopy ag ee wi h hose ob- ained o he K0 SK0 Sand K±K±sys ems allows one o s udy he p ope ies o he a0 esonance i sel . This is in e es ing in i s own igh since many s udies discuss he possibili y ha he a0, lis ed by he Pa icle Da a G oup as a diqua k ligh unfla o ed meson s a e [6], could be a ou -qua k s a e, i.e. a e aqua k, o a “K–K molecule” [7–12]. Fo example, he p oduc ion c oss sec ion o he a0 esonance in a eac ion channel such as K0K−→a− 0should de- pend on whe he he a− 0is composed o duo dssuqua ks, he o me equi ing he annihila ion o he ss pai and he la e be- ing a di ec ans e o he qua ks in he kaons o he a− 0. The h p://dx.doi.o g/10.1016/j.physle b.2017.09.009 0370-2693/©2017 The Au ho . Published by Else ie B.V. This is an open access a icle unde he CC BY license (h p://c ea i ecommons.o g/licenses/by/4.0/). Funded by SCOAP3. ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 65 esul s om K0 SK− em oscopy migh be sensi i e o hese wo di - e en scena ios. In his Le e , esul s om he fi s s udy o K0 SK± em oscopy a e p esen ed. This has been done o Pb–Pb collisions a √sNN = 2.76 TeV measu ed by he ALICE expe imen a he LHC [13]. The physics goals o he p esen K0 SK± em oscopy s udy a e he ol- lowing: 1) show o wha ex en he FSI h ough he a0 esonance desc ibes he co ela ion unc ions, 2) s udy he K0and K0sou ces o see i he e a e di e ences in he sou ce pa ame e s, and 3) es published a0mass and coupling pa ame e s by compa isons wi h published iden ical kaon esul s [5]. 2. Desc ip ion o expe imen and da a selec ion The ALICE expe imen and i s pe o mance in he LHC Run 1 (2009–2013) a e desc ibed in Re . [13] and Re . [14,15], espec- i ely. Abou 22 ×106Pb–Pb collision e en s wi h 0–10% cen ali y class aken in 2011 we e used in his analysis ( he a e age cen- ali y in his ange is 4.9% due o a sligh igge inefficiency in he 8–10% ange). E en s we e classified acco ding o hei cen- ali y using he measu ed ampli udes in he V0 de ec o s, which consis o wo a ays o scin illa o s loca ed along he beamline and co e ing he ull azimu h [16]. Cha ged pa icles we e econ- s uc ed and iden ified wi h he cen al ba el de ec o s loca ed wi hin a solenoid magne wi h a field s eng h o B =0.5T. Cha ged pa icle acking was pe o med using he Time P ojec ion Chambe (TPC) [17] and he Inne T acking Sys em (ITS) [13]. The ITS allowed o high spa ial esolu ion in de e mining he p ima y (collision) e ex. T acks we e econs uc ed and hei momen a we e ob ained wi h he TPC. A momen um esolu ion o less han 10 MeV/cwas ypically ob ained o he cha ged acks o in e - es in his analysis. The p ima y e ex was ob ained om he ITS, he posi ion o he p ima y e ex being cons ained along he beam di ec ion ( he “z-posi ion”) o be wi hin ±10 cm o he cen- e o he ALICE de ec o . In addi ion o he s anda d ack quali y selec ions, he ack selec ions based on he quali y o ack e- cons uc ion fi and he numbe o de ec ed acking poin s in he TPC we e used o ensu e ha only well- econs uc ed acks we e aken in he analysis [14,15]. Pa icle iden ifica ion (PID) o econs uc ed acks was ca - ied ou using bo h he TPC and he Time-o -Fligh (TOF) de ec- o in he pseudo apidi y ange |η| <0.8[14,15]. Fo each PID me hod, a alue was assigned o each ack deno ing he numbe o s anda d de ia ions be ween he measu ed ack in o ma ion and calcula ed alues (Nσ) [5,14,15]. Fo TPC PID, a pa ame ized Be he–Bloch o mula was used o calcula e he specific ene gy loss dE/dxin he de ec o expec ed o a pa icle wi h a gi en mass and momen um. Fo PID wi h TOF, he pa icle mass was used o calcula e he expec ed ime-o -fligh as a unc ion o ack leng h and momen um. This p ocedu e was epea ed o ou “pa icle species hypo heses”—elec on, pion, kaon and p o on—, and, o each hypo hesis, a di e en Nσ alue was ob ained pe de ec o . 2.1. Kaon selec ion The me hods used o selec and iden i y indi idual K0 Sand K± pa icles a e he same as hose used o he ALICE Pb–Pb K0 SK0 Sand K±K±analyses [5]. These a e now desc ibed below. 2.1.1. K0 Sselec ion The K0 Spa icles we e econs uc ed om he decay K0 S→ π+π−, wi h he daugh e π+and π− acks de ec ed in he TPC and TOF de ec o s. Pions wi h pT>0.15 GeV/cwe e accep ed (since o lowe pT ack finding efficiency d ops apidly) and he dis ance o closes app oach o he p ima y e ex (DCA) o he econs uc ed K0 Swas equi ed o be less han 0.3 cm in all di- ec ions. The equi ed Nσ alues o he pions we e NσTPC <3 and NσTOF <3 o p >0.8 GeV/c. An in a ian mass dis ibu- ion o he π+π−pai s was p oduced and he K0 Swas defined o be esul ing om a pai ha ell in o he in a ian mass ange 0.480 <mπ+π−<0.515 GeV/c2. 2.1.2. K±selec ion Cha ged kaon acks we e also de ec ed using he TPC and TOF de ec o s, and we e accep ed i hey we e wi hin he ange 0.14 <pT<1.5GeV/c. In o de o educe he numbe o secon- da ies ( o ins ance he cha ged pa icles p oduced in he de ec o ma e ial, pa icles om weak decays, e c.) he p ima y cha ged kaon acks we e selec ed based on he DCA, such ha he DCA ans e se o he beam di ec ion was less han 2.4 cm and he DCA along he beam di ec ion was less han 3.2 cm. I he TOF signal we e no a ailable, he equi ed Nσ alues o he cha ged kaons we e NσTPC <2 o pT<0.5 GeV/c, and he ack was e- jec ed o pT>0.5 GeV/c. I he TOF signal we e also a ailable and pT>0.5GeV/c: NσTPC <3 and NσTOF <2(0.5 <pT<0.8 GeV/c), NσTOF <1.5(0.8 <pT<1.0GeV/c), NσTOF <1(1.0 <pT< 1.5GeV/c). K0 SK±expe imen al pai pu i y was es ima ed om a Mon e Ca lo (MC) s udy based on HIJING [18] simula ions using GEANT3 [19] o model pa icle anspo h ough he ALICE de ec o s. The pu i y was de e mined om he ac ion o he econs uc ed MC simula ed pai s ha we e iden ified as ac ual K0 SK±pai s inpu om HIJING. The pai pu i y was es ima ed o be 88% o all kine- ma ic egions s udied in his analysis. 3. Analysis me hods 3.1. Expe imen al co ela ion unc ions This analysis s udies he momen um co ela ions o K0 SK±pai s using he wo-pa icle co ela ion unc ion, defined as C(k∗)=A(k∗)/B(k∗)(2) whe e A(k∗)is he measu ed dis ibu ion o pai s om he same e en , B(k∗)is he e e ence dis ibu ion o pai s om mixed e en s, and k∗is he magni ude o he momen um o each o he pa icles in he pai es ame (PRF), k∗=(s−m2 K0−m2 K±)2−4m2 K0m2 K± 4s(3) whe e, s=m2 K0+m2 K±+2EK0EK±−2 pK0· pK±(4) and mK0(EK0) and mK±(EK±) a e he es masses ( o al ene gies) o he K0 Sand K±, espec i ely. The denomina o B(k∗)was o med by mixing K0 Sand K±pa - icles om each e en wi h pa icles om en o he e en s. The e exes o he mixed e en s we e cons ained o be wi hin 2 cm o each o he in he z-di ec ion. A cen ali y cons ain on he mixed e en s was ound no o be necessa y o he na ow cen- ali y ange, i.e. 0–10%, used in his analysis. Co ela ion unc ions we e ob ained sepa a ely o wo di e en magne ic field o ien a- ions in he expe imen and hen ei he a e aged o fi sepa a ely, depending on he fi ing me hod used (see below). Co ela ion unc ions we e measu ed o h ee o e lapping/non- exclusi e pai ans e se momen um (kT=|pT,1+pT,2|/2) bins: all kT, kT<0.675 and kT>0.675 GeV/c. The mean kT alues o hese h ee bins we e 0.675, 0.425 and 0.970 GeV/c, espec i ely. 66 ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 Fig. 1. Examples o aw K0 SK+co ela ion unc ions o he h ee kTbins wi h linea fi s o he baseline a la ge k∗. S a is ical unce ain ies a e shown. Fig. 1 shows sample aw K0 SK+co ela ion unc ions o hese h ee bins o one o he magne ic field o ien a ions. One can see he main ea u e o he em oscopic co ela ion unc ion: he supp es- sion due o he s ong final-s a e in e ac ions o small k∗. In he highe k∗ egion, he e ec s o he a0appea o no be p esen and hus could be used as a e e ence, i.e. “baseline”, o he a0-based model fi ed o C(k∗)in o de o ex ac he sou ce pa ame e s. Also shown in he figu e a e linea fi s o he baseline o la ge k∗. The e ec s on C(k∗)by he a0 esonance a e mos ly seen in he k∗<0.2 GeV/c egion, whe e he wid h o he a0 egion eflec s he size o he kaon sou ce (see equa ions below). Co ela ion unc ions we e co ec ed o momen um esolu ion e ec s using HIJING calcula ions. HIJING was used o c ea e wo co ela ion unc ions: one in e ms o he gene a o -le el k∗and one in e ms o he simula ed de ec o -le el k∗. Because HIJING does no inco po a e final-s a e in e ac ions, weigh s we e calcu- la ed using a 9 h-o de polynomial fi in k∗ o an expe imen al co ela ion unc ion and we e used when filling he same-e en dis ibu ions. These weigh s we e calcula ed using k∗. Then, he a io o he “ideal” co ela ion unc ion o he “measu ed” one ( o each k∗bin) was mul iplied o he da a co ela ion unc ions be- o e he fi p ocedu e. This co ec ion mos ly a ec ed he lowes k∗bins, inc easing he ex ac ed sou ce pa ame e s by se e al pe - cen . 3.2. Final-s a e in e ac ion model The K0 SK±co ela ion unc ions we e fi wi h unc ions ha include a pa ame e iza ion which inco po a es s ong FSI. I was assumed ha he FSI a ises in he K0 SK±channels due o he nea - h eshold esonance, a0(980). This pa ame e iza ion was in- oduced by R. Lednicky and is based on he model by R. Lednicky and V.L. Lyuboshi z [20,21] (see also Re . [2] o mo e de ails on his pa ame e iza ion). Using an equal emission ime app oxima ion in he PRF [20], he elas ic K0 SK± ansi ion is w i en as a s a iona y solu ion − k∗( ∗)o he sca e ing p oblem in he PRF. The quan i y  ∗ ep- esen s he emission sepa a ion o he pai in he PRF, and he − k∗ subsc ip e e s o a e e sal o ime om he emission p ocess. A la ge dis ances his has he asymp o ic o m o a supe posi ion o a plane wa e and an ou going sphe ical wa e, − k∗( ∗)=e−i k∗· ∗+ (k∗)eik∗ ∗ ∗,(5) whe e (k∗)is he s-wa e K0K−o K0K+sca e ing ampli ude whose con ibu ion is he s-wa e iso ec o a0 esonance (see Eq. (11) in Re . [2]), Table 1 The a0masses and coupling pa ame e s, all in GeV ( aken om Re . [2]). Re e ence ma0γa0K¯ Kγa0πη Ma in [7] 0.974 0.333 0.222 An onelli [8] 0.985 0.4038 0.3711 Achaso 1 [9] 0.992 0.5555 0.4401 Achaso 2 [9] 1.003 0.8365 0.4580 (k∗)=γa0→KK m2 a0−s−i(γa0→KKk∗+γa0→πηkπη).(6) In Eq. (6), ma0is he mass o he a0 esonance, and γa0→KK and γa0→πη a e he couplings o he a0 esonance o he K0K−(o K0K+) and πη channels, espec i ely. Also, s =4(m2 K0+k∗2)and kπη deno es he momen um in he second decay channel (πη) (see Table 1). The co ela ion unc ion due o he FSI is hen calcula ed by in eg a ing − k∗( ∗)in he Koonin–P a equa ion [22,23] C( k∗)=d3 ∗S( ∗)− k∗( ∗) 2 ,(7) whe e S( ∗)is a one-dimensional Gaussian sou ce unc ion o he PRF ela i e dis ance  ∗wi h a Gaussian wid h Ro he o m S( ∗)∼e− ∗ 2/(4R2).(8) Equa ion (7) can be in eg a ed analy ically o K0 SK±co ela ions wi h FSI o he one-dimensional case, wi h he esul C(k∗)=1+λα1 2 (k∗) R 2 +2R (k∗) √πRF1(2k∗R) −I (k∗) RF2(2k∗R),(9) whe e F1(z)≡√πe−z2e fi(z) 2z;F2(z)≡1−e−z2 z.(10) In he abo e equa ions αis he ac ion o K0 SK±pai s ha come om he K0K−o K0K+sys em, se o 0.5 assuming symme y in K0and K0p oduc ion [2], Ris he adius pa ame e om he sphe ical Gaussian sou ce dis ibu ion gi en in Eq. (8), and λis he co ela ion s eng h. The co ela ion s eng h is uni y in he ideal case o pu e a0- esonan FSI, pe ec PID, a pe ec Gaussian kaon sou ce and he absence o long-li ed esonances which decay in o kaons. No e ha he o m o he FSI e m in Eq. (9) di e s om ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 67 he o m o he FSI e m o K0 SK0 Sco ela ions (Eq. (9) o Re . [2]) by a ac o o 1/2due o he non-iden ical pa icles in K0 SK±co - ela ions and hus he absence o he equi emen o symme ize he wa e unc ion gi en in Eq. (5). As seen in Eq. (6), he K0K−o K0K+s-wa e sca e ing am- pli ude depends on he a0mass and decay couplings. In he p esen wo k, we ha e aken he alues used in Re . [2] which ha e been ex ac ed om he analysis o he a0→πη spec a o se e al expe imen s [7–10], shown in Table 1. The ex ac ed a0mass and decay couplings ha e a ange o alues o he a - ious e e ences. Excep o he Ma in e e ence [7], which ex- ac s he a0 alues om he eac ion 4.2 GeV/cinciden mo- men um K−+p →+(1385)π−ηusing a wo-channel B ei – Wigne o mula, he o he e e ences ex ac he a0 alues om he adia i e φ-decay da a, i.e. φ→π0ηγ , om he KLOE col- labo a ion [24]. These la e h ee e e ences apply a model ha assumes, a e aking in o accoun he φ→π0ρ0→π0ηγ back- g ound p ocess, ha he φdecays o he π0ηγ final s a e h ough he in e media e p ocesses φ→K+K−γ→a0γo φ→K+K−→ a0γ, i.e. he “cha ged kaon loop model” [9]. The main di e ence be ween hese analyses is ha he An onelli e e ence [8] as- sumes a fixed a0mass in he fi o his model o he π0ηda a, whe eas he Achaso 1 and Achaso 2 analyses [9] allow he a0 mass o be a ee pa ame e in he wo di e en fi s made o he da a. I is assumed in he p esen analysis ha hese decay couplings will also be alid o K0K−and K0K+sca e ing due o isospin in a iance. Co ela ion unc ions we e fi ed wi h all ou o hese cases o see he e ec on he ex ac ed sou ce pa ame- e s. 3.3. Fi ing me hods In o de o es ima e he sys ema ic e o s in he fi ing me hod used o ex ac Rand λusing Eq. (9), wo di e en me hods, judged o be equally alid, ha e been used o handle he e ec s o he baseline: 1) a sepa a e linea fi o he “baseline egion,” ol- lowed by fi ing Eq. (9) o he co ela ion unc ion di ided by he linea fi o ex ac he sou ce pa ame e s, and 2) a combined fi o Eq. (9) and a quad a ic unc ion desc ibing he baseline whe e he sou ce pa ame e s and he pa ame e s o he quad a ic unc ion a e fi ed simul aneously. The sou ce pa ame e s a e ex ac ed o each case om bo h me hods and a e aged, he symme ic sys em- a ic e o o each case due o he fi ing me hod being one-hal o he di e ence be ween he wo me hods. Bo h fi ing me hods will now be desc ibed in mo e de ail. 3.3.1. Linea baseline me hod In he “linea baseline me hod,” o he all kT, kT<0.675 and kT>0.675 GeV/cbins he a0 egions we e aken o be k∗<0.3, k∗<0.2 and k∗<0.4GeV/c, espec i ely. In he highe k∗ egion i was assumed ha e ec s o he a0we e no p esen and hus can be used as a e e ence, i.e. “baseline”, o he a0-based model fi ed o C(k∗), which was a e aged o e he wo magne ic field o ien a ions used in he expe imen , o ex ac he sou ce pa am- e e s. Fo he h ee kTbins, linea fi s we e made in he k∗ anges 0.3–0.45, 0.2–0.45 and 0.4–0.6GeV/c, espec i ely, and he co - ela ion unc ions we e di ided by hese fi s o emo e baseline e ec s ex ending in o he low-k∗ egion. These anges we e aken o define he baselines since he measu ed co ela ion unc ions we e ound o be linea he e. Fo la ge alues o k∗ he co ela- ion unc ions became non-linea . The baseline was s udied using HIJING MC calcula ions which ake in o accoun he de ec o cha - ac e is ics as desc ibed ea lie . The C(k∗)dis ibu ions ob ained om HIJING do no show supp essions a low k∗as seen in Fig. 1 bu a he show linea dis ibu ions o e he en i e anges in k∗ shown in he figu e. HIJING also shows he baseline becoming non- linea o la ge alues o k∗, as seen in he measu emen s. The MC gene a o code AMPT [25] was also used o s udy he baseline. AMPT is simila o HIJING bu also includes final-s a e esca e - ing e ec s. AMPT calcula ions also showed linea baselines in he k∗ anges used in he p esen analysis, becoming non-linea o la ge k∗. Bo h HIJING and AMPT quali a i ely show he same di- ec ion o changes in he slopes o he baseline s. kTas seen in he da a, bu AMPT mo e accu a ely desc ibed he slope alues hem- sel es, sugges ing ha final-s a e esca e ing plays a ole in he kTdependence o he baseline slope. The sys ema ic unce ain ies on he ex ac ed sou ce pa ame e s due o he assump ion o lin- ea i y in hese k∗ egions we e es ima ed om HIJING o be less han 1%. Fig. 2 shows examples o K0 SK+and K0 SK−co ela ion unc- ions di ided by linea fi s o he baseline wi h Eq. (9) using he Achaso 2 pa ame e s. One can see he main ea u e o he em- oscopic co ela ion unc ion: he supp ession due o he s ong final-s a e in e ac ions o small k∗. As seen, he a0FSI pa ame e - iza ion gi es an excellen ep esen a ion o he “signal egion” o he da a, i.e. he supp ession o he co ela ion unc ions in he k∗ ange 0 o abou 0.15 GeV/c. 3.3.2. Quad a ic baseline me hod In he “quad a ic baseline me hod,” Rand λa e ex ac ed as- suming a quad a ic baseline unc ion by fi ing he p oduc o a quad a ic unc ion and he Lednicky equa ion, Eq. (9), o he aw co ela ion unc ions o each o he wo magne ic field o ien a- ions used in he expe imen , such as shown in Fig. 1, i.e., C i aw(k∗)=a(1−bk∗+ck∗2)C(k∗)(11) whe e C(k∗)is gi en by Eq. (9), and a, band ca e fi pa ame- e s. Eq. (11) is fi o he same k∗ anges as shown in Fig. 1, i.e. 0–0.45 GeV/c o all kTand kT<0.675 GeV/c, and 0–0.6GeV/c o kT>0.675 GeV/c. The fi s o he expe imen al co ela ion unc- ions a e ound o be o simila good quali y as seen o he linea baseline me hod fi s shown in Fig. 2. 3.4. Sys ema ic unce ain ies Sys ema ic unce ain ies on he ex ac ed sou ce pa ame e s we e es ima ed by a ying he anges o kinema ic and PID cu alues on he da a by ±10% and ±20%, as well as om MC simu- la ions. The main sys ema ic unce ain ies on he ex ac ed alues o Rand λdue o a ious sou ces, no including he baseline fi - ing me hod, a e: a) k∗fi ing ange: 2%, b) single-pa icle and pai cu s (e.g. DCA cu s, PID cu s, pai sepa a ion cu s): 2%–4% o R and 3%–8% o λ, and c) pai pu i y: 1% on λ. Combining he indi- idual sys ema ic unce ain ies in quad a u e, he o al sys ema ic unce ain ies on he ex ac ed sou ce pa ame e s, no including he baseline fi ing me hod con ibu ion, a e in he anges 3%–5% o Rand 4%–8% o λ. As men ioned ea lie , o he wo fi ing me hods, he sou ce pa ame e s a e ex ac ed o each case om bo h me hods and a - e aged, he symme ic sys ema ic e o o each case due o he fi ing me hod being one-hal o he di e ence be ween he wo me hods. The baseline fi ing me hod sys ema ic e o hus ob- ained is added in quad a u e wi h he sys ema ic e o s gi en abo e. I is ound ha he size o he baseline fi ing me hod sys- ema ic e o s a e abou 50% la ge o Rand o simila magni ude o λas hose quo ed abo e o he non-fi ing-me hod sys ema ic e o s. 68 ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 Fig. 2. Examples o K0 SK+and K0 SK−co ela ion unc ions di ided by linea fi s o he baseline wi h he Lednicky pa ame e iza ion using he Achaso 2 [9] pa ame e s. S a is ical (lines) and he linea sum o s a is ical and sys ema ic unce ain ies (boxes) a e shown. 4. Resul s and discussion Fig. 3 shows sample esul s o he Rand λpa ame e s ex- ac ed in he p esen analysis om K0 SK± em oscopy using he Achaso 1 pa ame e s. The le column compa es K0 SK+and K0 SK− esul s om he quad a ic baseline fi me hod, and he igh col- umn compa es esul s a e aged o e K0 SK+and K0 SK− o he quad a ic baseline fi s and he linea baseline fi s. As i is usually he case in em oscopic analyses, he fi ed Rand λpa ame e s a e co ela ed. The fi ing (s a is ical) unce ain ies a e aken o be he ex eme alues o he 1σfi con ou s in R s. λ. S a is- ical unce ain ies a e plo ed o all esul s. I is seen in he figu e ha he Rand λ alues o K0 SK−ha e a sligh endency o be la ge han hose o K0 SK+. Such a di e ence could esul om he K−–nucleon sca e ing c oss sec ion being la ge han ha o K+–nucleon (see Fig. 51.9 o Re . [6]), possibly esul ing in mo e final-s a e esca e ing o he K−. Since he di e ence is no sig- nifican once sys ema ic unce ain ies a e aken in o accoun , K0 SK+ and K0 SK−a e a e aged o e in he final esul s. The di e ence in he ex ac ed pa ame e s be ween he wo baseline fi ing me h- ods is also seen o be small, and is accoun ed o as a sys ema ic e o , as desc ibed ea lie . The esul s o he Rand λpa ame e s ex ac ed in he p esen analysis om K0 SK± em oscopy, a e aged o e he wo baseline fi me hods and a e aged o e K0 SK+and K0 SK−, a e p esen ed in Table 2 and in Figs. 4 and 5. Fi esul s a e shown o all ou pa- ame e se s gi en in Table 1. Figs. 4 and 5 also show compa isons wi h iden ical kaon esul s o he same collision sys em and en- e gy om ALICE om Re . [5]. S a is ical and o al unce ain ies a e shown o all esul s. As shown in Fig. 4, bo h Achaso pa ame e se s, wi h he la ge a0masses and decay couplings, appea o gi e R alues ha ag ee bes wi h hose ob ained om iden ical-kaon em oscopy. The An- onelli pa ame e se appea s o gi e sligh ly lowe alues. Com- pa ing he measu ed R alues be ween K0 SK0 Sand K±K±in Fig. 4 hey a e seen o ag ee wi h each o he wi hin he unce ain ies. In ac , he only eason o he em oscopic K0 SK± adii o be di e en om he K0 SK0 Sand K±K±ones would be i he K0 Sand K±sou ces we e displaced wi h espec o each o he . This is no expec ed be- cause he collision dynamics is go e ned by s ong in e ac ions o which he isospin symme y applies. The esul s o he co ela ion s eng h pa ame e s λa e shown in Fig. 5. The λpa ame e s om K0 SK±and K±K±a e co ec ed o expe imen al pu i y [5]. The K0 SK0 Spai s ha e a high pu i y o >90%, so he co esponding co ec ion was neglec ed [5] (see he ea lie discussion on pu i y). S a is ical and o al unce ain ies a e shown o all esul s. The K0 SK±λ alues, wi h he excep ion o he Ma in pa ame- e s, appea o be in ag eemen wi h he λ alues o he iden ical kaons. All o he λ alues a e seen o be measu ed o be abou 0.6, i.e. less han he ideal alue o uni y, which can be due o he con ibu ion o kaons om K∗decay (∼50 MeV, whe e  is he decay wid h) and om o he long-li ed esonances (such as he D-meson) dis o ing he spa ial kaon sou ce dis ibu ion away om he ideal Gaussian which is assumed in he fi unc ion [26]. One would expec ha he K0 SK±λ alues ag ee wi h hose om he iden ical kaons i he FSI o he K0 SK±wen solely h ough he a0 esonan channel since his analysis should see he same sou ce dis ibu ion. In o de o ob ain a mo e quan i a i e compa ison o he p esen esul s o Rand λwi h he iden ical kaon esul s, he χ2/nd is calcula ed o Rand λ o each pa ame e se , χ2 ω/nd =1 nd 3  i=1 [ωi(K0 SK±)−ωi(KK)]2 σ2 i (12) ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 69 Fig. 3. Sample esul s o he Rand λpa ame e s ex ac ed in he p esen analysis om K0 SK± em oscopy using he Achaso 1 pa ame e s. The le column compa es K0 SK+ and K0 SK− esul s om he quad a ic baseline fi me hod, and he igh column compa es esul s a e aged o e K0 SK+and K0 SK− o he quad a ic baseline fi s and he linea baseline fi s. S a is ical unce ain ies a e plo ed o all esul s. Table 2 Fi esul s o Rand λex ac ed in he p esen analysis om K0 SK± em oscopy a e aged o e K0 SK+and K0 SK−. S a is ical and sys ema ic e o s a e also shown. Pa ame e s R( m) o λAll kTkT<0.675 GeV/ck T>0.675 GeV/c Achaso 2 R5.17 ±0.16 ±0.41 6.71 ±0.40 ±0.42 4.75 ±0.18 ±0.36 λ0.587 ±0.034 ±0.051 0.651 ±0.073 ±0.076 0.600 ±0.040 ±0.034 Achaso 1 R4.92 ±0.15 ±0.39 6.30 ±0.40 ±0.43 4.49 ±0.18 ±0.30 λ0.650 ±0.038 ±0.056 0.723 ±0.087 ±0.091 0.649 ±0.048 ±0.038 An onelli R4.66 ±0.17 ±0.46 5.74 ±0.36 ±0.26 4.07 ±0.18 ±0.29 λ0.624 ±0.044 ±0.058 0.703 ±0.085 ±0.077 0.613 ±0.052 ±0.037 Ma in R3.29 ±0.12 ±0.35 4.46 ±0.25 ±0.20 2.90 ±0.11 ±0.41 λ0.305 ±0.020 ±0.033 0.376 ±0.041 ±0.037 0.296 ±0.021 ±0.030 whe e ωis ei he Ro λ, i uns o e he h ee kT alues, he num- be o deg ees o eedom aken is nd =3 and σiis he sum o he s a is ical and sys ema ic unce ain ies on he i h K0 SK±ex ac ed pa ame e (No e ha he all kTbin indeed con ains he kaon pai s ha make up he kT<0.675 GeV/cand kT>0.675 GeV/cbins, bu in addi ion i con ains an equal numbe o new pai combina- ions be ween he kaons in he kT<0.675 GeV/cand kT>0.675 GeV/cbins. So o he pu poses o his simple compa ison, we ap- p oxima e he all kTbin as being independen .) The linea sum o he s a is ical and sys ema ic unce ain ies is used o σi o be consis en wi h he linea sum o he s a is ical and sys ema ic un- ce ain ies plo ed on he poin s in Figs. 4 and 5. The quan i y ωi(KK)is de e mined by fi ing a quad a ic o he iden ical kaon esul s and e alua ing he fi a he a e age kT alues o he K0 SK± measu emen s. Table 3 summa izes he esul s o each pa ame e se and he ex ac ed p- alues. As seen, he Achaso 2, Achaso 1 and An onelli pa ame e se s a e consis en wi h he iden ical kaon esul s o bo h Rand λ. The Ma in pa ame e se is seen o ha e anishingly small p- alues o bo h Rand λand is hus in clea Table 3 Compa isons o Rand λ om K0 SK±wi h iden ical kaon esul s. Pa ame e s χ2 R/nd Rp- alue χ2 λ/nd λp- alue λ(K0 SK±) λ(KK) Achaso 2 0.456 0.713 0.248 0.863 1.04 ±0.17 Achaso 1 0.583 0.626 0.712 0.545 1.14 ±0.20 An onelli 1.297 0.273 0.302 0.824 1.09 ±0.20 Ma in 14.0 0.000 22.2 0.000 0.55 ±0.10 disag eemen wi h he iden ical kaon esul s, as can easily be seen by examining Figs. 4 and 5. In o de o quan i a i ely es ima e he size o he non- esonan channel p esen , he a io λ(K0 SK±) λ(KK)has been calcula ed o each pa ame e s se , whe e he a e age is o e he h ee kT alues and he unce ain y is calcula ed om he a e age o he s a is i- cal+sys ema ic unce ain ies on he K0 SK±pa ame e s. These alues a e shown in he las column o Table 3. Dis ega ding he Ma in alue, he smalles alue his a io can ake wi hin he unce ain- 70 ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 Fig. 4. Sou ce adius pa ame e , R, ex ac ed in he p esen analysis om K0 SK± em oscopy a e aged o e K0 SK+and K0 SK−and he wo baseline fi me hods ( ed symbols), along wi h compa isons wi h iden ical kaon esul s om ALICE [5] (blue symbols). S a is ical (lines) and he linea sum o s a is ical and sys ema ic unce ain ies (boxes) a e shown. (Fo in e p e a ion o he colo s in his figu e, he eade is e e ed o he web e sion o his a icle.) Fig. 5. Co ela ion s eng h pa ame e , λ, ex ac ed in he p esen analysis om K0 SK± em oscopy a e aged o e K0 SK+and K0 SK−and he wo baseline fi me hods ( ed symbols), along wi h compa isons wi h iden ical kaon esul s om ALICE [5] (blue symbols). S a is ical (lines) and he linea sum o s a is ical and sys ema ic unce ain ies (boxes) a e shown. (Fo in e p e a ion o he colo s in his figu e, he eade is e e ed o he web e sion o his a icle.) ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 71 ies is 0.87 ( om he Achaso 2 pa ame e s) which would hus allow a mos a 13% non- esonan con ibu ion. The esul s o his s udy p esen ed abo e clea ly show ha he measu ed K0 SK±ha e dominan ly unde gone a FSI h ough he a0 esonance. This is ema kable conside ing ha we measu e in Pb– Pb collisions he a e age sepa a ion be ween he wo kaons a eeze ou o be ∼5 m, and due o he sho - anged na u e o he s ong in e ac ion o ∼1 m his would seem o no encou - age a FSI bu a he encou age ee-s eaming o he kaons o he de ec o esul ing in a “fla ” co ela ion unc ion. A dominan FSI is wha migh be expec ed i he a0would be a ou -qua k, i.e. e aqua k, s a e o a “K–K molecule.” The e appea s o be no cal- cula ions in he li e a u e o he e aqua k s. diqua k p oduc ion c oss sec ions o he in e ac ion KK →a0, bu quali a i e a gu- men s compa ible wi h he a0being a ou –qua k s a e can be made based on he p esen measu emen s. The main a gumen in a o o his is ha he eac ion channel K0K−→a− 0(K0K+→a+ 0) is s ongly a o ed i he a− 0(a+ 0) is composed o dssu(dssu) qua ks such ha a di ec ans e o he qua ks in he kaons o he a− 0(a+ 0) has aken place, since his is an “OZI supe allowed” eac- ion [12]. The “OZI ule” can be s a ed as “an inhibi ion associa ed wi h he c ea ion o annihila ion o qua k lines” [12]. Thus, adi- qua k a0final s a e is less a o ed acco ding o he OZI ule since i would equi e he annihila ion o he s ange qua ks in he kaon in e ac ion. This would allow o he possibili y o a significan non- esonan o ee-s eaming channel o he kaon in e ac ion ha would esul in a λ alue below he iden ical-kaon alue by dilu ing he a0signal. As men ioned abo e, he collision geome y i sel also supp esses he annihila ion o he s ange qua ks due o he la ge sepa a ion be ween he kaons a eeze ou . No e ha his assumes ha he C(k∗)dis ibu ion o a non- esonan channel would be mos ly “fla ” o “mono onic” in shape and no showing a s ong esonan -like signal as seen o he a0in Fig. 1 and Fig. 2. This assump ion is clea ly ue in he ee-s eaming case, which is assumed in Eq. (9) in se ing α=0.5due o he non- esonan kaon combina ions. A simila a gumen , namely ha he success o he “cha ged kaon loop model” in desc ibing he adia i e φ-decay da a a o s he a0as a e aqua k s a e, is gi en in Re . [9]. 5. Summa y In summa y, em oscopic co ela ions wi h K0 SK±pai s ha e been s udied o he fi s ime. This new em oscopic me hod was applied o da a om cen al Pb–Pb collisions a √sNN =2.76 TeV by he LHC ALICE expe imen . Co ela ions in he K0 SK±pai s a e p oduced by final-s a e in e ac ions which p oceed h ough he a0(980) esonance. The a0 esonan FSI is seen o gi e an excel- len ep esen a ion o he shape o he signal egion in he p esen s udy. The di e ences be ween K0K+and K0K− o he ex ac ed R and λ alues a e ound o be insignifican wi hin he unce ain ies o he p esen s udy. The h ee la ge a0mass and decay pa ame e se s a e a o ed by he compa ison wi h he iden ical kaon esul s. The p esen esul s a e also compa ible wi h he in e p e a ion o he a0 esonance as a e aqua k s a e. This wo k should p o ide a cons ain on models ha a e used o p edic kaon–kaon in e - ac ions [27,28]. I will be in e es ing o apply K0 SK± em oscopy o o he collision ene gies, e.g. he highe LHC ene gies now a ail- able, and bomba ding species, e.g. p o on–p o on collisions, since he di e en sou ce sizes encoun e ed in hese cases will p obe he in e ac ion o he K0 Swi h he K±in di e en sensi i i y anges (i.e. see he Rdependence in Eq. (9)). Acknowledgemen s The ALICE Collabo a ion would like o hank all i s enginee s and echnicians o hei in aluable con ibu ions o he cons uc- ion o he expe imen and he CERN accele a o eams o he ou s anding pe o mance o he LHC complex. The ALICE Collab- o a ion g a e ully acknowledges he esou ces and suppo p o- ided by all G id cen e s and he Wo ldwide LHC Compu ing G id (WLCG) collabo a ion. The ALICE Collabo a ion acknowledges he ollowing unding agencies o hei suppo in building and un- ning he ALICE de ec o : A. I. Alikhanyan Na ional Science Labo a- o y (Ye e an Physics Ins i u e) Founda ion (ANSL), S a e Commi - ee o Science and Wo ld Fede a ion o Scien is s (WFS), A menia; Aus ian Academy o Sciences and Na ionals i ung ü Fo schung, Technologie und En wicklung, Aus ia; Minis y o Communica- ions and High Technologies, Na ional Nuclea Resea ch Cen e , Aze baijan; Conselho Nacional de Desen ol imen o Cien ífico e Tecnológico (CNPq), Uni e sidade Fede al do Rio G ande do Sul (UFRGS), Financiado a de Es udos e P oje os (Finep) and Fun- dação de Ampa o à Pesquisa do Es ado de São Paulo (FAPESP), B azil; Minis y o Science & Technology o China (MSTC), Na- ional Na u al Science Founda ion o China (NSFC) and Minis y o Educa ion o China (MOEC), China; Minis y o Science, Edu- ca ion and Spo s and C oa ian Science Founda ion, C oa ia; Min- is y o Educa ion, You h and Spo s o he Czech Republic, Czech Republic; The Danish Council o Independen Resea ch Na u- al Sciences, he Ca lsbe g Founda ion and Danish Na ional Re- sea ch Founda ion (DNRF), Denma k; Helsinki Ins i u e o Physics (HIP), Finland; Commissa ia à l’Ene gie A omique (CEA) and Ins i- u Na ional de Physique Nucléai e e de Physique des Pa icules (IN2P3) and Cen e Na ional de la Reche che Scien ifique (CNRS), F ance; Bundesminis e ium ü Bildung, Wissenscha , Fo schung und Technologie (BMBF) and GSI Helmhol zzen um ü Schwe i- onen o schung GmbH, Ge many; Gene al Sec e a ia o Resea ch and Technology, Minis y o Educa ion, Resea ch and Religions, G eece; Na ional Resea ch, De elopmen and Inno a ion Office, Hunga y; Depa men o A omic Ene gy Go e nmen o India (DAE) and Council o Scien ific and Indus ial Resea ch (CSIR), New Delhi, India; Indonesian Ins i u e o Science, Indonesia; Cen o Fe mi – Museo S o ico della Fisica e Cen o S udi e Rice che En ico Fe mi and Is i u o Nazionale di Fisica Nuclea e (INFN), I aly; Ins i u e o Inno a i e Science and Technology, Nagasaki Ins i u e o Applied Science (IIST), Japan Socie y o he P omo ion o Science (JSPS) KAKENHI and Japanese Minis y o Educa ion, Cul u e, Spo s, Sci- ence and Technology (MEXT), Japan; Consejo Nacional de Ciencia y Tecnología (CONACYT), h ough Fondo de Coope ación In e na- cional en Ciencia y Tecnología (FONCICYT) and Di ección Gene al de Asun os del Pe sonal Academico (DGAPA), Mexico; Nede landse O ganisa ie oo We enschappelijk Onde zoek (NWO), Ne he lands; The Resea ch Council o No way, No way; Commission on Science and Technology o Sus ainable De elopmen in he Sou h (COM- SATS), Pakis an; Pon ificia Uni e sidad Ca ólica del Pe ú, Pe u; Min- is y o Science and Highe Educa ion and Na ional Science Cen- e, Poland; Ko ea Ins i u e o Science and Technology In o ma- ion and Na ional Resea ch Founda ion o Ko ea (NRF), Republic o Ko ea; Minis y o Educa ion and Scien ific Resea ch, Ins i u e o A omic Physics and Romanian Na ional Agency o Science, Tech- nology and Inno a ion, Romania; Join Ins i u e o Nuclea Re- sea ch (JINR), Minis y o Educa ion and Science o he Russian Fede a ion and Na ional Resea ch Cen e Ku cha o Ins i u e, Rus- sia; Minis y o Educa ion, Science, Resea ch and Spo o he Slo ak Republic, Slo akia; Na ional Resea ch Founda ion o Sou h A ica, Sou h A ica; Cen o de Aplicaciones Tecnológicas y Desa - ollo Nuclea (CEADEN), Cubaene gía, Cuba, Minis e io de Ciencia e Inno acion and Cen o de In es igaciones Ene gé icas, Medioambi- en ales y Tecnológicas (CIEMAT), Spain; Swedish Resea ch Council (VR) and Knu & Alice Wallenbe g Founda ion (KAW), Sweden; Eu- opean O ganiza ion o Nuclea Resea ch, Swi ze land; Na ional Science and Technology De elopmen Agency (NSDTA), Su ana ee 72 ALICE Collabo a ion / Physics Le e s B 774 (2017) 64–77 Uni e si y o Technology (SUT) and Office o he Highe Educa- ion Commission unde NRU p ojec o Thailand, Thailand; Tu kish A omic Ene gy Agency (TAEK), Tu key; Na ional Academy o Sci- ences o Uk aine, Uk aine; Science and Technology Facili ies Coun- cil (STFC), Uni ed Kingdom; Na ional Science Founda ion o he Uni ed S a es o Ame ica (NSF) and Uni ed S a es Depa men o Ene gy, Office o Nuclea Physics (DOE NP), Uni ed S a es o Ame - ica. Re e ences [1] M.A. Lisa, S. P a , R. Sol z, U. Wiedemann, Fem oscopy in ela i is ic hea y ion collisions, Ann. Re . Nucl. Pa . Sci. 55 (2005) 357–402, a Xi :nucl-ex/0505014. [2] STAR Collabo a ion, B.I. Abele , e al., Neu al kaon in e e ome y in Au + Au collisions a √sNN =200 GeV, Phys. Re . C 74 (2006) 054902, a Xi :nucl- ex/0608012. [3] ALICE Collabo a ion, B. Abele , e al., K0 s–K0 sco ela ions in pp collisions a √s=7TeV om he LHC ALICE expe imen , Phys. Le . B 717 (2012) 151–161, a Xi :1206.2056 [hep-ex]. [4] ALICE Collabo a ion, B. Abele , e al., Cha ged kaon em oscopic co ela- ions in pp collisions a √s=7TeV, Phys. Re . D 87 (5) (2013) 052016, a Xi :1212.5958 [hep-ex]. [5] ALICE Collabo a ion, J. Adam, e al., One-dimensional pion, kaon, and p o on em oscopy in Pb–Pb collisions a √sNN =2.76 TeV, Phys. Re . C 92 (5) (2015) 054908, a Xi :1506.07884 [nucl-ex]. [6] Pa icle Da a G oup Collabo a ion, C. Pa ignani, e al., Re iew o pa icle physics, Chin. Phys. C 40 (10) (2016) 100001. [7] A. Ma in, E. Ozmu lu, E. Squi es, The ππ and K¯ Kampli udes, he S∗and he qua k s uc u e o 0++ esonances, Nucl. Phys. B 121 (1977) 514–530. [8] KLOE Collabo a ion, A. An onelli, Radia i e phi decays, eCon C020620 (2002) THAT06, a Xi :hep-ex/029069. [9] N.N. Achaso , A.V. Kisele , The new analysis o he KLOE da a on he phi → e a pi0 gamma decay, Phys. Re . D 68 (2003) 014006, a Xi :hep-ph/0212153. [10] N. Achaso , V. Gubin, Analysis o he na u e o he  ϕγπη and  ϕγπ0π0decays, Phys. Re . D 63 (2001) 094007. [11] E. San opin o, G. Gala a, Spec oscopy o e aqua k s a es, Phys. Re . C 75 (2007) 045206, a Xi :hep-ph/0605333. [12] R.L. Ja e, Mul i-qua k had ons. 1. The phenomenology o qqqqmesons, Phys. Re . D 15 (1977) 267. [13] ALICE Collabo a ion, K. Aamod , e al., The ALICE expe imen a he CERN LHC, JINST 3 (2008) S08002. [14] ALICE Collabo a ion, B.B. Abele , e al., Pe o mance o he ALICE expe imen a he CERN LHC, In . J. Mod. Phys. A 29 (2014) 1430044, a Xi :1402.4476 [nucl- ex]. [15] A. Akindino , e al., Pe o mance o he ALICE Time-O -Fligh de ec o a he LHC, Eu . Phys. J. Plus 128 (2013) 44. [16] ALICE Collabo a ion, B. Abele , e al., Cen ali y dependence o π, K, p p oduc- ion in Pb–Pb collisions a √sNN =2.76 TeV, Phys. Re . C 88 (2013) 044910, a Xi :1303.0737 [hep-ex]. [17] J. Alme, e al., The ALICE TPC, a la ge 3-dimensional acking de ice wi h as eadou o ul a-high mul iplici y e en s, Nucl. Ins um. Me h. A 622 (2010) 316–367, a Xi :1001.1950 [physics.ins-de ]. [18] X.-N. Wang, M. Gyulassy, HIJING: a Mon e Ca lo model o mul iple je p oduc- ion in pp, pA and AA collisions, Phys. Re . D 44 (1991) 3501–3516. [19] R. B un, F. B uyan , F. Ca mina i, S. Giani, M. Mai e, A. McPhe son, G. Pa ick, L. U ban, GEANT de ec o desc ip ion and simula ion ool, CERN-W5013 1 (1994) 1. [20] R. Lednicky, V. Lyuboshi s, Final s a e in e ac ion e ec on pai ing co ela ions be ween pa icles wi h small ela i e momen a, So . J. Nucl. Phys. 35 (1982) 770. [21] R. Lednicky, Co ela ion em oscopy, Nucl. Phys. A 774 (2006) 189–198, a Xi :nucl- h/0510020. [22] S. Koonin, P o on pic u es o high-ene gy nuclea collisions, Phys. Le . B 70 (1977) 43–47. [23] S. P a , T. Cso go, J. Zimanyi, De ailed p edic ions o wo pion co ela ions in ul a ela i is ic hea y ion collisions, Phys. Re . C 42 (1990) 2646–2652. [24] KLOE Collabo a ion, A. Aloisio, e al., S udy o he decay φ→ηπ0γwi h he KLOE de ec o , Phys. Le . B 536 (2002) 209–216, a Xi :hep-ex/0204012. [25] Z.-W. Lin, C.M. Ko, B.-A. Li, B. Zhang, S. Pal, A mul i-phase anspo model o ela i is ic hea y ion collisions, Phys. Re . C 72 (2005) 064901, a Xi :nucl- h/0411110. [26] T.J. Humanic, Ex ac ing he had oniza ion imescale in √s=7TeV p o on- p o on collisions om pion and kaon em oscopy, J. Phys. G 41 (2014) 075105, a Xi :1312.2303 [hep-ph]. [27] J.A. Olle , E. Ose , J.R. Pelaez, Meson meson in e ac ion in a nonpe u ba i e chi al app oach, Phys. Re . D 59 (1999) 074001, a Xi :hep-ph/9804209, Phys. Re . D 75 (2007) 099903, E a um. [28] N.T. Hong Xiem, S. Shinmu a, Pion–pion, pion–kaon, and kaon–kaon in e ac- ions in he one-meson-exchange model, PTEP 2014 (2) (2014), 023D04. ALICE Collabo a ion S. Acha ya139, D. Adamo á96, J. Adol sson34, M.M. Agga wal101, G. Aglie i Rinella35, M. Agnello31, N. Ag awal48, Z. Ahammed 139, N. Ahmad17, S.U. Ahn80, S. Aiola143, A. Akindino 65, S.N. Alam139, J.L.B. Alba114, D.S.D. Albuque que 125, D. Aleksand o 92, B. Alessand o59, R. Al a o Molina75, A. Alici54,12,27, A. Alkin3, J. Alme22, T. Al 71, L. Al enkampe 22, I. Al sybee 138, C. Al es Ga cia P ado 124, M. An7, C. And ei89, D. And eou35, H.A. And ews113, A. And onic109, V. Anguelo 106, C. Anson99, T. An iˇ ci´ c110, F. An ino i 57, P. An onioli 54, R. Anwa 127, L. Aphece che117, H. Appelshäuse 71, S. A celli27, R. A naldi59, O.W. A nold107,36, I.C. A sene21, M. A slandok106, B. Audu ie 117, A. Augus inus35, R. A e beck109, M.D. Azmi17, A. Badalà56, Y.W. Baek 79,61, S. Bagnasco59, R. Bailhache71, R. Bala 103, A. Baldisse i76, M. Ball45, R.C. Ba al68, A.M. Ba bano26, R. Ba be a28, F. Ba ile 53,33, L. Ba ioglio 26, G.G. Ba na öldi142, L.S. Ba nby113,95, V. Ba e 82, P. Ba alini7, K. Ba h35, J. Ba ke121,i, E. Ba sch71, M. Basile27, N. Bas id82, S. Basu139,141, B. Ba hen72, G. Ba igne117, A. Ba is a Camejo82, B. Ba yunya78, P.C. Ba zing21, I.G. Bea den93, H. Beck106, C. Bedda 64, N.K. Behe a61, I. Beliko 135, F. Bellini 27, H. Bello Ma inez2, R. Bellwied 127, L.G.E. Bel an123, V. Belyae 85, G. Bencedi 142, S. Beole26, A. Be cuci89, Y. Be dniko 98, D. Be enyi 142, R.A. Be ens130, D. Be zano35, L. Be e 35, A. Bhasin103, I.R. Bha 103, A.K. Bha i101, B. Bha acha jee44, J. Bhom121, L. Bianchi127, N. Bianchi51, C. Bianchin141, J. Bielˇ cík39, J. Bielˇ cíko á96, A. Bilandzic36,107, R. Biswas4, S. Biswas4, J.T. Blai 122, D. Blau92, C. Blume 71, G. Boca136, F. Bock 84,35,106, A. Bogdano 85, L. Boldizsá 142, M. Bomba a40, G. Bonomi137, M. Bono a35, J. Book71, H. Bo el76, A. Bo isso 19, M. Bo i129, E. Bo a26, C. Bou jau93, P. B aun-Munzinge 109, M. B egan 124, T.A. B oke 71, T.A. B owning108, M. B oz39, E.J. B ucken46, E. B una59, G.E. B uno 33, D. Budniko 111, H. Buesching71, S. Bu alino31, P. Buhle 116, P. Buncic 35, O. Busch133, Z. Bu helezi77, J.B. Bu 15, J.T. Bux on18, J. Cabala119, D. Ca a i 35,94, H. Caines143, A. Cali a64, E. Cal o Villa 114, P. Came ini25, A.A. Capon116,