scieee Open visual document viewer

Inelastic electron-nucleus scattering and scaling at high inelasticity

Barbaro, M. B.; Caballero Carretero, Juan Antonio; Donnelly, T. W.; Maieron, C.

Abstract

Highly inelastic electron scattering is analyzed within the context of the unified relativistic approach previously considered in the case of quasielastic kinematics. Inelastic relativistic Fermi gas modeling that includes the complete inelastic spectrum—resonant, nonresonant, and deep inelastic scattering—is elaborated and compared with experimental data. A phenomenological extension of the model based on direct fits to data is also introduced. Within both models, cross sections and response functions are evaluated and binding energy effects are analyzed. Finally, an investigation of the second-kind scaling behavior is also presented.

Full text

Inelas ic elec on-nucleus sca e ing and scaling a high inelas ici y M. B. Ba ba o,1J. A. Caballe o,2T. W. Donnelly,3and C. Maie on2,4 1Dipa imen o di Fisica Teo ica, Uni e si à di To ino and INFN, Sezione di To ino, Via P. Giu ia 1, 10125 To ino, I aly 2Depa amen o de Física A ómica, Molecula y Nuclea , Uni e sidad de Se illa, Apa ado Pos al 1065, E-41080 Se illa, Spain 3Cen e o Theo e ical Physics, Labo a o y o Nuclea Science and Depa men o Physics, Massachuse s Ins i u e o Technology, Camb idge, Massachuse s 02139, USA 4INFN, Sezione di Ca ania, Via S. So ia 64, 95123 Ca ania, I aly (Recei ed 24 No embe 2003; published 24 Ma ch 2004) Highly inelas ic elec on sca e ing is analyzed wi hin he con ex o he uni ied ela i is ic app oach p e i- ously conside ed in he case o quasielas ic kinema ics. Inelas ic ela i is ic Fe mi gas modeling ha includes he comple e inelas ic spec um— esonan , non esonan , and deep inelas ic sca e ing—is elabo a ed and com- pa ed wi h expe imen al da a. A phenomenological ex ension o he model based on di ec i s o da a is also in oduced. Wi hin bo h models, c oss sec ions and esponse unc ions a e e alua ed and binding ene gy e ec s a e analyzed. Finally, an in es iga ion o he second-kind scaling beha io is also p esen ed. DOI: 10.1103/PhysRe C.69.035502 PACS numbe (s): 25.30.Fj, 24.10.J , 13.60.Hb I. INTRODUCTION In his wo k we conside highly inelas ic elec on sca e - ing and compa e i s analysis wi h he case o quasielas ic (QE)elec on sca e ing. The la e is domina ed by he p o- cess whe e he exchanged i ual pho on in e ac s wi h a nucleon in he nuclea g ound s a e and ejec s ha nucleon, he eby o ming a nuclea pa icle-hole exci a ion. Co ec- ions o his dominan p ocess in ol e going beyond he im- pulse app oxima ion o accoun o wo-body cu en s, inal- s a e in e ac ions, and nuclea co ela ions. Al hough hese con ibu ions a e known no o be en i ely negligible [1–7] his simple p ocess accoun s o he basic ea u e seen in he icini y o elas ic sca e ing om a nucleon a es , namely, he QE peak. Models such as hose discussed below ake in o accoun he ac ha he nucleons in he nucleus a e mo ing and a e bound and he eby p oduce a b oad peak in he in- elas ic spec um. In he p esen wo k ou goal is o ex end he analysis, s ill main aining he same basic ea u es o he ela i is ic modeling used o he QE egion, and now ocus on wha we call highly inelas ic sca e ing, o o b e i y, simply he inelas ic egion. This includes e e y hing ha goes beyond he QE p ocess: ha is, whe eas he QE p ocess assumes elas ic sca e ing om he nucleons, he inelas ic p ocess will assume inelas ic e-Nsca e ing. Fo ela i ely low inal-s a e in a ian masses one lies in he egion o eso- nance exci a ion and wo cases o his so ha e been ex- plo ed in ecen wo k [8,9]. In he p esen s udy hese ideas a e gene alized o include he comple e inelas ic spec um, bo h esonan and non esonan , including deep inelas ic sca - e ing (DIS), wi hin he con ex o he uni ied ela i is ic app oach used in ou p e ious wo k. Thus, in he p esen wo k ou goal is o begin by explo - ing ex ensions o he ela i is ic Fe mi gas (RFG)model [6,10,11] o an inelas ic e sion o his app oach. While his bea s some connec ion wi h adi ional con olu ion models o he high-ene gy esponse o nuclei (see, o example, Re s. [12–15]) i is no he same in ha , albei wi hin a model, i co ec ly inco po a es a speci ic ela i is ic nuclea spec al unc ion in o he p oblem, whe eas some o he ap- p oaches make addi ional assump ions and use only he in e- g al o he spec al unc ion, namely, he nuclea momen um dis ibu ion o make non ela i is ic app oxima ions when dealing wi h he spec al unc ion. This dis inc ion can be seen qui e clea ly in s udies o i s - and second-kind scaling [11,16–20]and will no be elabo a ed he e. Once he inelas ic RFG modeling is in hand, i becomes clea ha i migh be use ul o explo e a phenom- enological ex ension o his model, namely, wha we call he ex ended ela i is ic Fe mi gas (ERFG). In his app oach we ake he esul o doing he co ec in eg al o e he nuclea spec al unc ion (i.e., no he ull in eg al, which is he mo- men um dis ibu ion, as alluded o abo e)di ec ly om i s made p e iously o he da a [21]. We shall see ha his has a signi ican impac on he nuclea esponses a high inelas ic- i y.An issue which will also become clea la e is ha he s o y is no ye comple e: in addi ion o he modeling done in he p esen wo k, whe e he ocus is placed on inco po a ing inelas ic e ec s a high ene gies, he e a e s ill o he con i- bu ions ha mus be added. Speci ically, in ecen wo k [22] on 2p-2hmeson-exchange cu en e ec s i is seen ha a signi ican incohe en con ibu ion mus be added o hose explo ed he e. Gi en ha he wo k on 2p-2he ec s is, as ye , incomple e—co ela ion con ibu ions a e p esen ly be- ing included—i is p ema u e o make oo much o compa i- sons wi h expe imen al da a, and, as we ema k la e in he app op ia e places, he inal unde s anding o how all o he a ious eac ion mechanisms en e , while becoming clea e is no ye achie ed. The pape is o ganized as ollows: in Sec. II we ecall he gene al o malism o inelas ic elec on-nucleus sca e ing; in Sec. III we de i e he exp essions o he inelas ic had- onic enso in h ee di e en models: he pu e RFG model [Sec. III A], he RFG including he e ec s o binding ene gy [Sec. III B]and he ERFG [Sec. III C]; in Sec. IV we p esen nume ical esul s o c oss sec ions [Sec. IV A], esponse unc ions [Sec. IV B], and scaling unc ions [Sec. IV C]and inally, in Sec. V we d aw ou conclusions. PHYSICAL REVIEW C 69, 035502 (2004) 0556-2813/2004/69(3)/035502(16)/$22.50 ©2004 The Ame ican Physical Socie y69 035502-1 II. INELASTIC ELECTRON-NUCLEUS SCATTERING: GENERAL FORMALISM Wi h he goal ou lined abo e in mind, we s a by ew i - ing he gene al exp essions ha apply in bo h elas ic and inelas ic egimes. The gene al o malism desc ibing inclu- si e elec on-nucleus sca e ing p ocesses is widely a ailable [23–25]; he e we simply ocus on hose aspec s ha a e o special ele ance o he discussion ha ollows. We ollow he con en ions and me ic o Re . [26]and use capi al le - e s o e e o ou - ec o s. The inciden and sca e ed elec- on ou -momen a a e deno ed by Ki ␮ =共␧i,ki兲and K ␮ =共␧ ,k 兲. The had onic a iables, PA ␮ =共MA,0兲and PB ␮ =共EB,pB兲 ep esen he ou momen a o he a ge and e- sidual nucleus, espec i ely. The ou -momen um ans e is gi en by Q ␮ =共 ␻ ,q兲(we assume he Bo n app oxima ion, i.e., only one i ual pho on exchanged in he p ocess). Following s anda d p ocedu es he di e en ial c oss sec- ion may be w i en d ␴ d⍀ d␧ =2 ␣ 2 Q4 ␧ ␧i ␩ ␮ ␯ W ␮ ␯ ,共1兲 whe e ␣ is he ine s uc u e cons an , ␩ ␮ ␯ is he lep onic enso ha can be e alua ed di ec ly using ace echniques 关27兴, and W ␮ ␯ is he had onic enso con aining all o he nuclea s uc u e and dynamics in o ma ion. Assuming ha he inal s a e can be desc ibed in e ms o a ecoiling nuclea s a e 兩 ␺ B典plus a 共highly兲inelas ic s a e 兩⌽X典, i s gene al ex- p ession is gi en by W ␮ ␯ =兺 A兺 B兺 X具 ␺ B,⌽X兩J ˆ ␮ 共q兲兩 ␺ A典*具 ␺ B,⌽X兩J ˆ ␯ 共q兲兩 ␺ A典 ⫻ ␳ 共EB兲dEB ␳ 共EX兲dEX ␦ 共␧i−␧ +EA−EB−EX兲, 共2兲 whe e 兺 ¯ A共兺B兺X兲indica es he app op ia e a e age 共sum兲 o e ini ial 共 inal兲s a es. He e J ˆ ␮ 共q兲is he Fou ie ans o m o he nuclea cu en ope a o e alua ed, 兩 ␺ A典and 兩 ␺ B,⌽X典 ep esen he ini ial and inal s a es, espec i ely, and he dis ibu ion unc ions ␳ 共EB兲and ␳ 共EX兲a e in oduced o ac- coun o he ene gy-momen um dispe sion ela ion o he inal nuclea 共B兲and had onic 共X兲sys ems. In his wo k we assume ha he inelas ici y o he p ocess is o ally ac- coun ed o by he inal s a e ⌽X; hence o he ene gy dis- ibu ion unc ion o he esidual nuclea sys em we use ␳ 共EB兲= ␦ 共EB−E ¯ B兲, whe e E ¯ B=冑pB 2+共MB *兲2. No e ha W ␮ ␯ in Eq. 共2兲is mean o be e alua ed a pB+pX=q=ki−k . The nuclea enso can equi alen ly be exp essed as an in eg al in he 共E,p兲plane, wi h −p=pB he h ee-momen um o he ecoiling daugh e nucleus and E⬅冑p2+共MB *兲2 −冑p2+共MB 0兲2 he exci a ion ene gy o he esidual nucleus (see Re . [19]). The domain o in eg a ion is he kinema i- cally allowed egion max关E共0兲,0兴艋E艋E共 ␲ 兲,共3兲 whe e E共 ␪ 兲=MA 0+ ␻ −冑共MB 0兲2+p2−冑WX 2+q2+p2+2pq cos ␪ 共4兲 wi h ␪ he angle be ween pand q, and whe e WXis he in a ian mass o he inal s a e. In he MB 0→⬁limi he abo e exp ession becomes E⬁共 ␪ 兲=mN+ ␻ ˜ −冑WX 2+q2+p2+2pq cos ␪ ,共5兲 whe e mNis he nucleon mass, ␻ ˜ ⬅ ␻ −ESand ES=MB 0+mN −MA 0is he sepa a ion ene gy. The uppe cu e E共 ␲ 兲c osses he paxis a p−=−yXand p+=YX, whe e yX=1 2W2关共MA 0+ ␻ 兲冑共W−MB 0兲2−WX 2 ⫻冑共W+MB 0兲2−WX 2−2q⌳X兴共6兲 and YX=1 2W2关共MA 0+ ␻ 兲冑共W−MB 0兲2−WX 2 ⫻冑共W+MB 0兲2−WX 2+2q⌳X兴,共7兲 and whe e W=冑共MA 0+ ␻ 兲2−q2and ⌳X=1 2关W2+共MB 0兲2−WX 2兴. 共8兲 The a iable yXis he gene aliza ion o he usual y-scaling a iable o he inelas ic p ocess whe e a esonance Xis p o- duced. In he limi MB 0→⬁i eads yX,⬁=冑共 ␻ ˜ +mN兲2−WX 2−q.共9兲 No e ha he allowed egion dec eases wi h WXand col- lapses o a poin when −yX=YX, which implies W=MB 0+WX o , in he MB 0→⬁limi , 共yX,⬁兲min=−q, co esponding o 共WX兲max= ␻ ˜ +mN. Summa izing, o ixed ou -momen um ans e , he esonan mass is limi ed o he ange mN+m ␲ 艋WX艋mN+ ␻ −ES.共10兲 III. THE RELATIVISTIC FERMI GAS MODEL In his sec ion we p oceed by e alua ing he had onic nuclea enso assuming he impulse app oxima ion and by wo king wi hin he amewo k o he RFG model. In his case, he i ual pho on is abso bed by an on-shell nucleon desc ibed by a Di ac spino u共h,sh兲, wi h ene gy E ¯ h =冑h2+mN 2. In eg a ing o e he momen a in he Fe mi sea, he ollowing exp ession o he inelas ic had onic enso e- sul s: BARBARO, CABALLERO, DONNELLY, AND MAIERON PHYSICAL REVIEW C 69, 035502 (2004) 035502-2 W ␮ ␯ 共q, ␻ 兲=3N 4 ␲ pF 3 冕 FdhmN E ¯ h 冕 dEX ␦ 共 ␻ +E ¯ h−EX兲 ⫻1 2兺 sh兺 Xi ␳ 共EXi兲关⌽ ¯ XiJ ˆ ␮ u共h,sh兲兴*关⌽ ¯ XiJ ˆ ␯ u共h,sh兲兴, 共11兲 whe e Nis he numbe o nucleons 共p o ons o neu ons兲and 兰Fdh⬅兰dh ␪ 共pF−h兲,pFbeing he Fe mi momen um. The symbol 兰dEXs ands o he in eg al o e he ene gy o he inelas ic inal s a e, while 兺Xiindica es in gene al he sum/ in eg al o e all he in e nal quan um numbe s o all possible inelas ic inal s a es ⌽Xi, ha ing o al ene gy EXand o al momen um pX, ixed by momen um conse a ion o be pX =h+q. The had onic enso in Eq. (11) o inelas ic p ocesses can be also w i en in he o m Winel ␮ ␯ 共q, ␻ 兲=3N 4 ␲ pF 3 冕 dEX 冕 FdhmN E ¯ h winel ␮ ␯ 共H,Q,EX兲 ⫻ ␦ 共 ␻ +E ¯ h−EX兲,共12兲 whe e H ␮ =共E ¯ h,h兲and we ha e in oduced he inelas ic single-nucleon enso winel ␮ ␯ 共H,Q,EX兲=1 2兺 sh兺 Xi ␳ 共EXi兲关⌽ ¯ XiJ ˆ ␮ u共h,sh兲兴* ⫻关⌽ ¯ XiJ ˆ ␯ u共h,sh兲兴.共13兲 No e ha he abo e single-nucleon enso has dimensions o E−1. As will be shown la e , his is in con as wi h ou pas wo k on QE and N→⌬sca e ing whe e he single-nucleon enso s we e de ined o be dimensionless. Nex we choose o exp ess he inelas ic had onic enso in Eq. (12)in e ms o he in a ian mass WX, Winel ␮ ␯ 共q, ␻ 兲=3N 4 ␲ pF 3 冕 dWX 冕 FdhmNWX E ¯ hEX winel ␮ ␯ 共H,Q,EX兲 ⫻ ␦ 共 ␻ +E ¯ h−EX兲共14兲 wi h EX=冑pX 2+WX 2. The ene gy in eg al can be pe o med by exploi ing he ␦ unc ion, yielding Winel ␮ ␯ 共q, ␻ 兲=3N 4 ␲ pF 3 冕 FdhmN E ¯ h winel ␮ ␯ 共H,Q, ␻ +E ¯ h兲.共15兲 In he case o DIS on a single nucleon, he inelas ic enso simply educes o he single-nucleon enso winel ␮ ␯ . Be o e en e ing in o a de ailed analysis o he inelas ic nuclea enso , i is in e es ing o no ice how he usual ex- p essions o he QE and N→⌬had onic enso s a e eco - e ed om he gene al esul gi en in Eq. (11). Fi s , in he case o QE sca e ing, he nuclea inal s a e is simply a pa icle-hole exci a ion, hence, in he RFG model, ⌽Xde- sc ibes an on-shell nucleon, namely, ⌽X=冑mN/E ¯ pu共p,sp兲. The ene gy dis ibu ion unc ion is simply ␳ 共EX兲= ␦ 共EX −E ¯ p兲and he sum o e he inal s a es educes o a sum o e spin p ojec ions, 兺Xi=兺sp. The QE had onic enso hen eads WQE ␮ ␯ 共q, ␻ 兲=3N 4 ␲ pF 3 冕 FdhmN 2 E ¯ hE ¯ p wQE ␮ ␯ 共H,Q兲 ␦ 共 ␻ +E ¯ h−E ¯ p兲, 共16兲 whe e wQE ␮ ␯ is he usual dimensionless QE single-nucleon en- so wQE ␮ ␯ =1 2兺 sh兺 sp 关u ¯ 共p,sp兲J ˆ ␮ u共h,sh兲兴*关u ¯ 共p,sp兲J ˆ ␯ u共h,sh兲兴. 共17兲 In he case o he ansi ion N→⌬, he inal s a e ⌽X, wi hin he con ex o he RFG model, is an on-shell ⌬, namely, ⌽X=冑m⌬/E ¯ ⌬u⌬共p,s⌬兲, wi h on-shell ene gy E ¯ ⌬=冑p2+m⌬ 2. The ene gy dis ibu ion unc ion in his case is ␳ 共EX兲 = ␦ 共EX−E ¯ ⌬兲and 兺Xi=兺s⌬. The N→⌬had onic enso ha esul s is W⌬ ␮ ␯ 共q, ␻ 兲=3N 4 ␲ pF 3 冕 FdhmN 2 E ¯ hE ¯ ⌬ w⌬ ␮ ␯ 共H,Q兲 ␦ 共 ␻ +E ¯ h−E ¯ ⌬兲 共18兲 wi h w⌬ ␮ ␯ he dimensionless nucleon-⌬ enso w⌬ ␮ ␯ =m⌬ 2mN兺 sh兺 s⌬ 关u ¯ ⌬共p,sp兲J ˆ ␮ u共h,sh兲兴*关u ¯ ⌬共p,sp兲J ˆ ␯ u共h,sh兲兴. 共19兲 As expec ed, hese exp essions o he dimensionless single- nucleon enso s coincide wi h he ones in oduced in Re . 关8,28兴. Likewise o he Rope esonance he exp essions ob- ained in Re . 关9兴a e eco e ed. A. The RFG inelas ic nuclea enso and esponse unc ions In his sec ion we e alua e he inelas ic nuclea enso in he RFG amewo k. Fo con enience, as usual we i s de- ine he dimensionless a iables ␬ ␮ =共␭, ␬ 兲= 冉 ␻ 2mN,q 2mN 冊 , ␶ = ␬ 2−␭2, ␩ F=pF mN, ⑀ F=冑1+ ␩ F 2, 共20兲 ␩ ␮ =共 ⑀ ¯ , ␩ 兲= 冉 E ¯ h mN,h mN 冊 , ␮ X=WX mN, ⑀ X=冑 ␮ X 2+共 ␩ +2 ␬ 兲2, in e ms o which he had onic enso in Eq. (14) eads INELASTIC ELECTRON-NUCLEUS SCATTERING AND…PHYSICAL REVIEW C 69, 035502 (2004) 035502-3 Winel ␮ ␯ 共 ␬ ,␭兲=3N 4 ␲ ␩ F 3 冕 d ␮ X 冕 d ␩ ␮ X ⑀ ¯ ⑀ Xwinel ␮ ␯ 共 ␩ , ␮ X; ␬ ,␭兲 ⫻ ␦ 共2␭+ ⑀ ¯ − ⑀ X兲 ␪ 共 ␩ F− ␩ 兲.共21兲 Be o e p esen ing he explici esul s o he RFG e- sponse unc ions, le us discuss an impo an ing edien o he calcula ion, he single-nucleon inelas ic had onic enso winel ␮ ␯ . Fo unpola ized sca e ing, he la e can be pa am- e ized in e ms o wo s uc u e unc ions, w1and w2, ac- co ding o winel ␮ ␯ =−w1 冉 g ␮ ␯ + ␬ ␮ ␬ ␯ ␶ 冊 +w2共 ␩ ␮ + ␬ ␮ ␳ 兲共 ␩ ␯ + ␬ ␯ ␳ 兲. 共22兲 Fo on-shell nucleons, he s uc u e unc ions w1and w2de- pend on wo a iables, he ou -momen um ans e Q2and he in a ian mass WXo he inal s a e eached by he nucleon, o , equi alen ly, he single-nucleon Bjo ken a i- able x=兩Q2兩 2H·Q=兩Q2兩 WX 2−mN 2−Q2= ␶ ␩ · ␬ .共23兲 In ou o malism i is con enien o in oduce he inelas- ici y pa ame e [8,29] ␳ ⬅1+ 1 4 ␶ 共 ␮ X 2−1兲,共24兲 he alue uni y co esponding o elas ic sca e ing. No e ha ␳ is simply linked o he Bjo ken scaling a iable o he on-shell nucleon mo ing inside he a ge nucleus by he ela ion ␳ =1/x, hus in he ollowing we will use ␳ as a gu- men o he s uc u e unc ions w1,w2. In p esen ing ou esul s we will also use he “labo a o y” Bjo ken a iable xL=兩Q2兩 2mN ␻ = ␶ ␭,共25兲 co esponding o a single nucleon a es in he labo a o y ame. Le us now e u n o he inelas ic nuclea enso o Eq. (21): a e pe o ming he pola angula in eg a ion by means o he ene gy-conse ing ␦ unc ion one ge s Winel ␮ ␯ 共 ␬ ,␭兲=3N ␶ 2 ␩ F 3 ␬ 冕 0 2 ␲ d⌽ 2 ␲ 冕 ␳ 1共 ␬ ,␭兲 ␳ 2共 ␬ ,␭兲d ␳ 冕 ⑀ 0共 ␳ 兲 ⑀ Fd ⑀ ¯ ⫻winel ␮ ␯ 共 ⑀ ¯ , ␪ 0, ␳ ; ␬ ,␭兲,共26兲 whe e cos ␪ 0=1 ␬ ␩ 共␭ ⑀ ¯ − ␶ ␳ 兲.共27兲 The condi ion 兩cos ␪ 0兩艋1 ixes he in eg a ion limi s o e ⑀ ¯ : ⑀ ¯ 艌 ⑀ 0共 ␳ 兲⬅ ␬ 冑1 ␶ + ␳ 2−␭ ␳ .共28兲 Mo eo e , by equi ing ha ⑀ 0共 ␳ 兲艋 ⑀ Fand ha he eso- nance mass is abo e he pion-p oduc ion h eshold (i.e., ␮ X 艌 ␮ h esh⬅1+ ␮ ␲ ) he ollowing egion is ob ained o he in eg a ion o e ␳ : 关 ␳ 1共 ␬ ,␭兲, ␳ 2共 ␬ ,␭兲兴 = 冋 max 再 ␭ ⑀ F− ␬ ␩ F ␶ , ␳ h esh 冎 ,␭ ⑀ F+ ␬ ␩ F ␶ 册 共29兲 wi h ␳ h esh =1+ ␮ ␲ 共 ␮ ␲ +2兲 4 ␶ .共30兲 No e ha he uppe in eg a ion limi ␳ 2共 ␬ ,␭兲always lies be- low he cu o co esponding o Eq. 共10兲. Indeed using Eqs. 共10兲and 共24兲and keeping in mind ha he 共nega i e兲sepa- a ion ene gy o he RFG is ES RFG=−TF⬅mN共1− ⑀ F兲, he maximum ␳ allowed by Eq. 共10兲 eads ␳ max RFG =1+ 1 4 ␶ 关共2␭+ ⑀ F兲2−1兴= ␳ 2共 ␬ ,␭兲+1 4 ␶ 共2 ␬ − ␩ F兲2, 共31兲 ␳ 2 he e o e esul ing in he mo e s ingen in eg a ion limi . Now by w i ing he single-nucleon inelas ic enso in e ms o s uc u e unc ions w1and w2as in Eq. (22)and choosing he zdi ec ion along q, he in eg a ion o e ⌽and ⑀ ¯ can be pe o med analy ically (see Appendix A)and he had onic inelas ic enso can be exp essed in he gene al o m Winel ␮ ␯ 共 ␬ ,␭兲=3N ␶ 2 ␩ F 3 ␬ ␰ F 冕 ␳ 1共 ␬ ,␭兲 ␳ 2共 ␬ ,␭兲d ␳ 共1− ␺ X 2兲 ␪ 共1− ␺ X 2兲 ⫻U ␮ ␯ 共 ␬ , ␶ , ␳ 兲,共32兲 whe e ␰ F= ⑀ F−1 is he Fe mi kine ic ene gy and he inelas ic scaling a iable ␺ X⬅sgn共␭− ␶ ␳ 兲冑 ⑀ 0共 ␳ 兲−1 ⑀ F−1 共33兲 has been de ined. Fo each alue o ␳ 共and hence ␮ X兲a “peak” can hus be iden i ied, co esponding o he egion −1艋 ␺ X艋1, cen e ed a ␺ X=0, ␭P= ␶ P ␳ =1 2 ␳ 共冑1+4 ␬ P 2 ␳ 2−1兲, ␬ P=冑 ␶ P共1+ ␶ P ␳ 2兲,共34兲 whose wid h ⌬␭ =1 2关冑共2 ␬ + ␩ F兲2+ ␮ X 2−冑共2 ␬ − ␩ F兲2+ ␮ X 2兴⯝ 2 ␬ ␩ F 冑4 ␬ 2+ ␮ X 2 共35兲 is a unc ion ha g ows wi h ␬ and dec eases wi h ␮ X. BARBARO, CABALLERO, DONNELLY, AND MAIERON PHYSICAL REVIEW C 69, 035502 (2004) 035502-4 The gene al exp ession o he enso U ␮ ␯ is de i ed in Appendix A. He e we only epo he longi udinal and ans- e se componen s UL=U00 = ␬ 2 ␶ 关共1+ ␶ ␳ 2兲w2共 ␶ , ␳ 兲−w1共 ␶ , ␳ 兲 +w2共 ␶ , ␳ 兲D共 ␬ , ␶ , ␳ 兲兴,共36兲 UT=U11 +U22 =2w1共 ␶ , ␳ 兲+w2共 ␶ , ␳ 兲D共 ␬ , ␶ , ␳ 兲,共37兲 which a e linked o he longi udinal and ans e se esponse unc ions by he ollowing ela ions: Rinel L,T共 ␬ , ␶ 兲=3N ␶ 2 ␩ F 3 ␬ ␰ F 冕 −1 ␺ X max共 ␬ ,␭兲d ␺ X冏 ⳵␳ ⳵ ␺ X冏共1− ␺ X 2兲 ⫻UL,T„ ␬ , ␶ , ␳ 共 ␺ X兲…,共38兲 wi h ␺ X max共 ␬ ,␭兲= min 冦 1, 冢 ␬ 冑1 ␶ + ␳ h esh 2−␭ ␳ h esh −1 ␰ F 冣 1/2 冧 共39兲 and ⳵␳ ⳵ ␺ X=−冑2 ␰ F ␬ 共1+ ␰ F ␺ X 2兲−␭ ␺ X冑2 ␰ F 冉 1+1 2 ␰ F ␺ X 2 冊 ␶ 冑1+1 2 ␰ F ␺ X 2 . 共40兲 In Eqs. 共36兲and 共37兲 he unc ion D共 ␬ , ␶ , ␳ 兲=1 ⑀ F− ⑀ 0共 ␳ 兲 冕 ⑀ 0共 ␳ 兲 ⑀ Fd ⑀ ¯ 冕 0 2 ␲ d⌽ 2 ␲ 共 ␩ ⫻ ␬ ˆ兲2 = ␶ ␬ 2 再 1 3关 ⑀ F 2+ ⑀ F ⑀ 0共 ␳ 兲+ ⑀ 0共 ␳ 兲2兴 +␭关 ⑀ F+ ⑀ 0共 ␳ 兲兴 +␭2 冎 −共1+ ␶ 兲+共 ␳ −1兲 ⫻ ␶ ␬ 2兵␭关 ⑀ F+ ⑀ 0共 ␳ 兲兴 − ␶ 共 ␳ +1兲其 = ␰ F共1− ␺ X 2兲 冋 1+ ␰ F ␺ X 2−␭ ␬␺ X冑 ␰ F共2+ ␰ F ␺ X 2兲 + ␶ 3 ␬ 2 ␰ F共1− ␺ X 2兲 册 共41兲 a ises om he Fe mi mo ion and goes o ze o as ␰ F→0; being p opo ional o ␰ F⬵ ␩ F 2/2Ⰶ1, his p o ides ela i ely mode a e co ec ions o he es o he con ibu ions in Eqs. 共36兲and 共37兲. The alue ␳ =1 co esponds o QE kinema ics: in his case he well-known exp essions o he QE esponses a e eco - e ed. The “ o al” obse ables a e hen ob ained by adding he usual RFG QE esponse o he inelas ic esul s: R o L,T=RQE L,T+Rinel L,T.共42兲 In he deep inelas ic egime i is cus oma y o deal wi h nuclea s uc u e unc ions W1,2 Aand/o F1,2 A. These can be exp essed in e ms o he longi udinal and ans e se e- sponse unc ions h ough he ollowing ela ions: W1 A=1 2RT,共43兲 W2 A= 冉 ␶ ␬ 2 冊 2RL+1 2 ␶ ␬ 2RT共44兲 and F1 A=mNW1 A,共45兲 F2 A=2mN␭W2 A.共46兲 B. E ec s o binding ene gy In he s udy o supe scaling o inclusi e QE elec on sca e ing om nuclei, an app op ia e scaling a iable ␺ ⬘ was in oduced by including a small ene gy shi o ha e he QE peak occu a he place whe e he scaling a iable is ze o. A de ailed s udy o he sensi i i y o he scaling unc ion o a ia ions o he Fe mi momen um and ene gy shi was p e- sen ed in Re s. [16,18,20]. He e we ex end his analysis o he inelas ic egion. In p inciple, he in oduc ion o an en- e gy shi ␻ shi in he o malism is s aigh o wa d and he calcula ion o he inelas ic esponses p oceeds as in he ␻ shi =0 case. Howe e , as will be made clea in he ollow- ing, some complica ions a ise. Fi s , due o he gene al o m assumed o he single-nucleon inelas ic had onic enso , a ce ain asymme y appea s be ween he ene gy shi e ec s in he longi udinal and ans e se esponses. These shi e - ec s a e la ge in he longi udinal esponse. No ice ha his asymme y al eady en e s a he le el o he QE nuclea e- sponses. Second, he e exis s an ambigui y in he de ini ion o he a iable which should be used as he Bjo ken x-scaling a iable co esponding o he mo ing nucleon. The e ec s o he inclusion o an ene gy shi on he in- elas ic nuclea had onic enso ha e been s udied in he li - e a u e, wi h pa icula emphasis on he s uc u e unc ion F2 and he Eu opean Muon Collabo a ion (EMC)e ec a la ge alues o x, in he con ex o so called “binding models” (see, o example, Re s. [30,31]and he gene al e iews [12,13]). The app oach we ollow he e is he sel -consis en gene ali- za ion o p e ious wo ks on he RFG. I is o mally simila o he binding model app oach, whe e in gene al he on-shell ene gy o he ini ial nucleon is modi ied by sub ac ing a cons an e m which e ec i ely accoun s o he nucleon sepa a ion ene gy and o he possibili y ha he esidual nuclea sys em is le in an (highly)exci ed s a e. Howe e , since he exis ing models ei he ocus only on EMC a ios and/o use mo e ealis ic, al hough gene ally non ela i is ic wa e unc ions, a p ecise quan i a i e compa ison wi h hose models is no possible. As we will discuss in he Resul s INELASTIC ELECTRON-NUCLEUS SCATTERING AND…PHYSICAL REVIEW C 69, 035502 (2004) 035502-5 sec ion, ou calcula ions s ill miss some ing edien s, coming om meson-exchange cu en s, and his makes a de ailed quan i a i e compa ison wi h expe imen al da a p ema u e; i is clea ha , when his compa ison will be made in he u- u e, a mo e in-dep h s udy o binding e ec s will also be needed. In he RFG he ene gy shi is usually in oduced by modi ying he a gumen o he ␦ unc ion appea ing in he gene al exp ession o he inelas ic had onic enso in Eq. (12), acco ding o ␻ +E ¯ h−EX→ ␻ ⬘+E ¯ h−EX, whe e ␻ ⬘= ␻ − ␻ shi . Then, in oducing he in a ian mass WX ⬘2⬅EX 2−pX 2 =共 ␻ ⬘+E ¯ h兲2−pX 2, we can w i e he inelas ic had onic enso in he o m Winel ␮ ␯ 共 ␬ ,␭兲=3N 4 ␲ ␩ F 3 冕 d ␮ X ⬘ 冕 d ␩ ␮ X ⬘ ⑀ ¯ ⑀ Xwinel ␮ ␯ 共 ␩ , ␮ X ⬘; ␬ ,␭兲 ⫻ ␦ 共2␭⬘+ ⑀ ¯ − ⑀ X兲 ␪ 共 ␩ F− ␩ 兲,共47兲 whe e ␮ X ⬘=WX ⬘/mNand ␭⬘= ␻ ⬘/共2mN兲. As in he unshi ed analysis, he ␦ unc ion can be used o pe o m he pola angula in eg a ion, leading o he esul Winel ␮ ␯ 共 ␬ ,␭兲=3N ␶ ⬘ 2 ␩ F 3 ␬ 冕 ␳ 1 ⬘共 ␬ ,␭⬘兲 ␳ 2 ⬘共 ␬ ,␭⬘兲d ␳ ⬘ 冕 0 2 ␲ ⫻d⌽ 2 ␲ 冕 ⑀ 0 ⬘共 ␳ ⬘兲 ⑀ Fd ⑀ ¯ winel ␮ ␯ 共 ⑀ ¯ , ␳ ⬘; ␬ ,␭兲,共48兲 whe e he a iable ␳ ⬘is de ined as ␳ ⬘⬅2H·Q⬘ 兩Q⬘2兩= 冋 1+ 1 4 ␶ ⬘共 ␮ X ⬘2−1兲 册 共49兲 and ␶ ⬘⬅ ␬ 2−␭⬘2. The inclusion o he ene gy shi modi ies he in eg a ion limi s o e ⑀ ¯ in he ollowing way: ⑀ ¯ 艌 ⑀ 0 ⬘共 ␳ ⬘兲⬅ ␬ 冑1 ␶ ⬘+ ␳ ⬘2−␭⬘ ␳ ⬘.共50兲 Co espondingly, he egion o he in eg a ion o e ␳ ⬘is gi en by 关 ␳ 1 ⬘共 ␬ ,␭⬘兲, ␳ 2 ⬘共 ␬ ,␭⬘兲兴 = 冋 max 再 ␭⬘ ⑀ F− ␬ ␩ F ␶ ⬘, 1+ ␮ ␲ 4 ␶ ⬘共2+ ␮ ␲ 兲 冎 ,␭⬘ ⑀ F+ ␬ ␩ F ␶ ⬘ 册 . 共51兲 The de ini ion o he inelas ic scaling a iable becomes now ␺ X ⬘2⬅ ⑀ 0 ⬘共 ␳ ⬘兲−1 ⑀ F−1 共52兲 and he inelas ic longi udinal and ans e se esponse unc- ions, calcula ed as Rinel L=Winel 00 and Rinel T=Winel 11 +Winel 22 , ha e he ollowing gene al o ms: Rinel L,T共 ␬ , ␶ 兲=3N ␶ ⬘ 2 ␩ F 3 ␬ ␰ F 冕 ␳ 1 ⬘共 ␬ ,␭⬘兲 ␳ 2 ⬘共 ␬ ,␭⬘兲d ␳ ⬘共1− ␺ X ⬘2兲UL,T共 ␬ , ␶ , ␳ ⬘兲. 共53兲 In o de o e alua e he longi udinal and ans e se nuclea unc ions UL,T共 ␬ , ␶ , ␳ ⬘兲one needs o assume a speci ic o m o he inelas ic single-nucleon enso winel ␮ ␯ 共 ⑀ ¯ , ␳ ⬘; ␬ ,␭兲.I is impo an o ema k ha he e exis s some ambigui y in he choice made he e: o ins ance, se e al al e na i es in ol ing di e en exp essions con aining he ou -momen a Q ␮ and/o Q⬘ ␮ a e possible, and hese can lead o di e en esul s. Fo example, in Re . 关30兴, he modi ied ou momen um ans e Q⬘ ␮ is used, al hough hen a p esc ip ion mus be used in o de o eco e he gauge in a iance o he nuclea had onic enso , which is los by making his choice. In Appendix B we p esen he speci ic exp essions o he inelas ic and QE esponses ob ained o a gi en selec ion o he single- nucleon enso s accoun ing o he ene gy shi . Apa om he speci ic o m o he enso w ␮ ␯ , he choice o he a gu- men s o he single-nucleon inelas ic s uc u e unc ions, w1,w2, also p esen s some ambigui ies. In ac , he a ailable pa ame iza ions o w1,w2 ha we employ in ou calcula- ions a e gi en o ee, on-shell, nucleons, while he inclu- sion o he ene gy shi e ec i ely in oduces some “o - shellness” o he ini ial nucleon, by al e ing he ene gy balance a he e ex whe e i couples o he exchanged i - ual pho on. In his case he bound-nucleon Bjo ken a iable is no uniquely de e mined by he inal-s a e in a ian mass and, since no heo e ically de i ed p esc ip ions exis , one has o make some assump ions. As shown in Appendix B, he inelas ici y pa ame e selec ed in his wo k, ␳ ˜ , co e- sponds o he one gi en as 共2mN ␻ ˜ 兲/兩Q2兩= ␳ ⬘共 ␶ ⬘/ ␶ 兲, whe e ␻ ˜ is he ene gy ans e ed o he nucleon in he sys em in which he nucleon is a es . This means ha in ou nume i- cal calcula ions, o a gi en se o alues o ␻ ,Q2, and ␳ ⬘we employ ee-nucleon s uc u e unc ions aken a ou - momen um Q2and Bjo ken a iable 1/ ␳ ˜ . C. Ex ended ela i is ic e mi gas As discussed in p e ious wo ks [8,16,18,20], o a ixed alue o he in a ian mass ␮ X, he RFG yields a scaling unc ion 共 ␺ X ⬘兲= L共 ␺ X ⬘兲= T共 ␺ X ⬘兲=3 4共1− ␺ X ⬘2兲 ␪ 共1− ␺ X ⬘2兲共54兲 which, as a unc ion o he app op ia e scaling a iable ␺ X ⬘,is he same o all alues o ␮ X.1 In Re . [18] he beha io o he longi udinal scaling unc- ion was s udied o he exis ing wo ld da a in he QE egion. This s udy showed ha o a good app oxima ion L共 ␺ ⬘兲su- pe scales, ha is, i does no show any signi ican depen- dence on he momen um ans e ␬ (scaling o he i s kind) and is app oxima ely he same o all nuclea species (scal- 1The unc ion in Eq. (54)di e s om he one used in p e ious wo k [20]by a mul iplica i e unc ion 2 ␰ F/ ␩ F 2关1+1 2 ␰ F共1+ ␺ X ⬘2兲兴.We ha e checked ha his is nume ically unimpo an o all o he kinema ical condi ions conside ed he e. BARBARO, CABALLERO, DONNELLY, AND MAIERON PHYSICAL REVIEW C 69, 035502 (2004) 035502-6 ing o he second kind). An exp ession o a phenomenologi- cal longi udinal scaling unc ion, uni 共 ␺ ⬘兲, was ob ained by i ing he da a [21]. Based on hese esul s, we now make he ollowing hypo hesis: we assume ha his uni 共 ␺ ⬘兲, de i ed om he da a, p o ides a good desc ip ion o 共 ␺ X ⬘兲= L共 ␺ X ⬘兲 = T共 ␺ X ⬘兲,(“scaling o he ze o h kind”)as i implici ly con- ains he ini ial-s a e physics, and hus we make, o any ␮ X, he ollowing subs i u ion: 3 4共1− ␺ X ⬘2兲 ␪ 共1− ␺ X ⬘2兲→ ERFG共 ␺ X ⬘兲= uni 共 ␺ X ⬘兲.共55兲 To be mo e speci ic, we calcula e he esponse unc ions as RQE L,T=N ␩ F 3 ␬ mN ␰ F model共 ␺ ⬘兲UQE L,T,共56兲 Rinel L,T共 ␬ , ␶ 兲=N ␩ F 3 ␬ ␰ F 冕 ␮ h esh 1+2␭− ⑀ Sd ␮ X ␮ X model共 ␺ X ⬘兲UL,T,共57兲 whe e ⑀ S=ES/mNis he dimensionless sepa a ion ene gy and model共 ␺ X ⬘兲= 再 3 4共1− ␺ X ⬘2兲 ␪ 共1− ␺ X ⬘2兲model = RFG uni 共 ␺ X ⬘兲model = ERFG. 共58兲 The unc ions RFG and ERFG a e shown in Fig. 1 as unc- ions o ␺ X ⬘, while he unc ions UQE L,Tand UL,Tin Eqs. 共56兲 and 共57兲a e gi en in Appendix B. IV. RESULTS In his sec ion we p esen ou esul s o c oss sec ions and esponse and s uc u e unc ions. In compu ing he in- elas ic had onic enso o Eq. (47), we employ phenomeno- logical i s o he single-nucleon inelas ic s uc u e unc ions. The la e a e measu ed in DIS expe imen s and a a ie y o pa ame iza ions o w1and w2can be ound in he li e a u e [15,32–36], including some a ia ions a ising om he di - e en assump ions made o how o ex ac he neu on s uc u e unc ions om deu e on da a. Unless s a ed o he - wise, in he ollowing we adop he Bodek e al. i o Re s. [15,32,33], which desc ibes bo h he deep inelas ic and eso- nance egions. Fo he QE con ibu ions, we employ he o m ac o pa ame iza ion o Re . [37]. The sensi i i y o he esul s o he di e en pa ame iza ion choices will be dis- cussed la e . Addi ionally, o he Fe mi momen um and he ene gy shi we will employ he alues ob ained in Re . [20], namely, kF=220 MeV/c, ␻ shi =20 MeV o ca bon, kF =236 MeV/c, ␻ shi =18 MeV o aluminum, kF =241 MeV/c, ␻ shi =23 MeV o i on, and kF=245 MeV/c, ␻ shi =25 MeV o gold. A. C oss sec ions In his sec ion we p esen ou esul s o he c oss sec ions in he RFG and ERFG models and compa e hem wi h he a ailable expe imen al da a [38–41]. FIG. 2. Inclusi e c oss sec ion o elec on sca e ing om ca - bon a Einc=500 MeV and ␪ e=60° s he ene gy ans e . The cal- cula ion includes an ene gy shi ␻ shi =20 MeV and he sepa a e QE and inelas ic con ibu ions o he c oss sec ion a e shown. Da a a e om Re . [41]. FIG. 3. As o Fig. 2, bu a Einc=2.020 GeV and sca e ing angle ␪ e=15° (a)and ␪ e=20° (b). Da a a e om Re . [39]. FIG. 1. Scaling unc ion model共 ␺ X ⬘兲o Eq. (58) o he RFG and ERFG models. INELASTIC ELECTRON-NUCLEUS SCATTERING AND…PHYSICAL REVIEW C 69, 035502 (2004) 035502-7 In Fig. 2 we show he inclusi e c oss sec ion o a 12C a ge a Ee=500 MeV and ␪ e=60°. We sepa a e he QE om he inelas ic con ibu ion. We no ice ha he shi ed RFG model (solid line)yields oughly he igh posi ion and heigh o he QE peak, bu ails o ep oduce he ails o he peak, gi ing in pa icula an unobse ed dip a ␻ ⯝200 MeV. On he o he hand he ERFG model (do ed line), while ep oducing he da a in he ails be e , signi i- can ly unde es ima es he c oss sec ion a he peak. This is ela ed o he ac ha , as shown in Fig. 1, he peak o he ERFG uni e sal unc ion ERFG is lowe han he co espond- ing RFG alue. Due o he la ge ex ension o ERFG o e ␺ X ⬘ he no maliza ion o he wo unc ions is he same, namely, 兰 RFGd ␺ X ⬘=兰 ERFGd ␺ X ⬘=1. One migh hen nai ely expec he in eg al in Eq. (57)which yields he inelas ic esponse unc- ions o be he same in he wo models. Howe e , a close inspec ion shows ha his is no he case because he in e- g a ion limi s and/o he weigh ing p o ided by UL,Ta e such ha he ERFG in eg al does no “sa u a e” as does he RFG one. Figu es 3–5 co espond o di e en kinema ical condi- ions, namely, Ee=2.020 and 3.595 GeV (SLAC)and Ee =4.045 GeV (JLab)and a ious sca e ing angles. Conce n- ing Figs. 3(a)and 3(b), a simila end pe sis s, wi h he FIG. 4. As o Fig. 2, bu a Ee=3.595 GeV and sca e ing angle ␪ e=16° (a), 20° (b), 25° (c), and 30° (d). Da a a e om Re . [39]. FIG. 5. As o Fig. 2, bu a Einc=4.045 GeV and sca e ing angle ␪ e=15° (a), 30° (b), 45° (c), and 74° (d). Da a a e om Re . [38]. BARBARO, CABALLERO, DONNELLY, AND MAIERON PHYSICAL REVIEW C 69, 035502 (2004) 035502-8 ERFG model signi ican ly unde es ima ing he da a in he egion o he QE peak, whe eas he RFG is close o he da a (pa icula ly o ␪ e=20°), al hough i lea es no oom o o he con ibu ions o be added. No e also ha o his sca - e ing angle he inelas ic channel s a s o be sizable. Examining Figs. 4 we ema k ha he QE peak, which is mo e clea ly sepa a ed om he inelas ic egion in Fig. 4(a), is again well ep oduced in he low- ␻ ail by he ERFG, while i s maximum ag ees be e wi h he RFG. On he o he hand he inelas ic c oss sec ion is in all cases unde es ima ed by he ERFG, while he RFG alone would oughly accoun o wha is obse ed. Simila commen s apply o Fig. 5(a), co esponding o highe ene gy and low sca e ing angle. Fo highe angles [Figs. 5(b)–5(d)] he da a lie oughly in be ween he p edic- ions o he ERFG (smalle )and RFG (la ge )models, he o me again ep oducing he low- ␻ beha io be e . As a gene al esul we obse e ha as he sca e ing angle in- c eases he ange o alidi y o he ERFG also inc eases. Finally, in Figs. 6 and 7 we conside sligh ly di e en kinema ical condi ions, co esponding o ixed alues o 兩Q2兩 in he ange 2–10 共GeV/c兲2, and a ious elec on ene gies (in he ange 8–25 GeV)and angles 共12° –22°兲. Theo e ical esul s o 56Fe a e shown as unc ions o he “labo a o y” Bjo ken a iable xL. The da a co esponding o a ixed Q2a e aken a di e en alues o Eeand ␪ e. Fo 兩Q2兩=2 and 10 共GeV/c兲2(Fig. 6) he a ious da a i easonably well on one plo , whe eas o 兩Q2兩=5 共GeV/c兲2(Fig. 7), o cla i y we ha e sepa a ed he da a in o h ee se s as indica ed in he igu e cap ion. We no ice ha a la ge xL共艌0.6兲 he da a a e close o he ERFG p edic ions, a low xL共0.1–0.3兲 hey a e close o he RFG calcula ion and o 0.3艋xL艋0.6 hey lie in be ween he wo models. This gene al end seems o be espec ed o all alues o Q2(a leas whe e da a a e a ail- able). We ha e also analyzed he e ec in oduced by di e en elec omagne ic o m ac o pa ame iza ions ([42–44]) and e i ied ha i can p oduce a ±3 % unce ain y a he QE peak, bu does no change he gene al ag eemen / disag eemen o he models wi h he da a. Mo eo e , i should be ema ked ha , a he ene gies conside ed in his sec ion, he con ibu ion om he esonance egion o he inelas ic pa o he c oss sec ion is qui e impo an and hus a compa ison wi h esul s ob ained by using pu ely DIS pa- ame iza ions [34,36]o he single-nucleon s uc u e unc- ions is no app op ia e. A he highes 兩Q2兩 alues conside ed he e [Figs. 6(b)and 7], he use o di e en pa ame iza ions [34,36]does no p oduce signi ican a ia ions in he esul s. An impo an commen , al eady an icipa ed in he in o- duc ion, is in o de . The RFG and ERFG models conside ed FIG. 6. Di e en ial c oss sec ion d ␴ /d ␻ d⍀e o elec on sca - e ing on i on, shown as a unc ion o xLa ixed 兩Q2兩. Panel (a): 兩Q2兩=2共GeV/c兲2, he expe imen al poin s, om igh o le , a e aken a 关Ee共GeV兲, ␪ e共deg兲兴=共8,11.8兲,共8,12.4兲,共8,13.6兲,共9.7, 11.8兲,共12,11.8兲,共15,11.8兲. Panel (b):兩Q2兩=10 共GeV/c兲2, he ex- pe imen al poin s, om igh o le , a e aken a 关Ee共GeV兲, ␪ e共deg兲兴⫽(15,16.0),(15,17.1),(17,15.0),(17,16.9),(21, 14.1),(24,14.1). Da a a e om Re . [40]. FIG. 7. As o Fig. 6, bu a 兩Q2兩=5共GeV/c兲2. The wo da a in he uppe panel, om igh o le , co espond o Ee=8 GeV and ␪ e=22° and o Ee=9.7 GeV and ␪ e=19.7°; he da a in he middle panel ha e ixed Ee=12 GeV and, om igh o le , ␪ e =12.8,13.3,14.2,15.8,20.6°; he da a in he lowe panel, om igh o le , a e aken a 共Ee=15 GeV, ␪ e=13.2°兲,共Ee=17 GeV, ␪ e =13.5°兲,共Ee=24.5 GeV ␪ e=11.1°兲. Da a a e om Re . [40]. INELASTIC ELECTRON-NUCLEUS SCATTERING AND…PHYSICAL REVIEW C 69, 035502 (2004) 035502-9 ␺ ⬘2=1 ␰ F 冉 ␬ 冑1 ␶ ⬘+1−␭⬘−1 冊 共B13兲 and he elec omagne ic s uc u e unc ions by w1,QE共 ␶ 兲= ␶ GM 2共 ␶ 兲, w2,QE共 ␶ 兲=GE 2共 ␶ 兲+ ␶ GM 2共 ␶ 兲 1+ ␶ wi h GE,M he p o on o neu on Sachs elec omagne ic o m ac o s. Finally, he “ o al” esponse unc ions a e e alua ed by adding he abo e QE esponses o he inelas ic ones, i.e., R o L,T=RQE L,T+Rinel L,T. [1]W. M. Albe ico, T. W. Donnelly, and A. Molina i, Nucl. Phys. A512, 541 (1990). [2]W. M. Albe ico, M. B. Ba ba o, A. De Pace, T. W. Donnelly, and A. Molina i, Nucl. Phys. A563, 605 (1993). [3]M. B. Ba ba o, A. De Pace, T. W. Donnelly, and A. Molina i, Nucl. Phys. A596, 553 (1996). [4]J. E. Ama o, M. B. Ba ba o, J. A. Caballe o, T. W. Donnelly, and A. Molina i, Nucl. Phys. A643, 349 (1998). [5]J. E. Ama o, M. B. Ba ba o, J. A. Caballe o, T. W. Donnelly, and A. Molina i, Nucl. Phys. A697, 388 (2002). [6]J. E. Ama o, M. B. Ba ba o, J. A. Caballe o, T. W. Donnelly, and A. Molina i, Phys. Rep. 368, 317 (2002). [7]J. E. Ama o, M. B. Ba ba o, J. A. Caballe o, T. W. Donnelly, and A. Molina i, Nucl. Phys. A723, 181 (2003). [8]J. E. Ama o, M. B. Ba ba o, J. A. Caballe o, T. W. Donnelly, and A. Molina i, Nucl. Phys. A657, 161 (1999). [9]L. Al a ez-Ruso, M. B. Ba ba o, T. W. Donnelly, and A. Mo- lina i, Nucl. Phys. A724, 157 (2003). [10]B. D. Se o and J. D. Walecka, Ad . Nucl. Phys. 16,1(1986). [11]W. M. Albe ico, A. Molina i, T. W. Donnelly, E. L. K onen- be g, and J. W. Van O den, Phys. Re . C 38, 1801 (1988). [12]R. P. Bicke s a and A. W. Thomas, J. Phys. G 15, 1523 (1989). [13]P. R. No on, Rep. P og. Phys. 66, 1253 (2003). [14]S. Simula, Few-Body Sys ., Suppl. 8, 423 (1995). [15]A. Bodek and J. L. Ri chie, Phys. Re . D 23, 1070 (1981);24, 1400 (1981). [16]T. W. Donnelly and I. Sick, Phys. Re . Le . 82, 3212 (1999). [17]M. B. Ba ba o, R. Cenni, A. De Pace, T. W. Donnelly, and A. Molina i, Nucl. Phys. A643, 137 (1998). [18]T. W. Donnelly and I. Sick, Phys. Re . C 60, 065502 (1999). [19]D. B. Day, J. S. McCa hy, T. W. Donnelly, and I. Sick, Annu. Re . Nucl. Pa . Sci. 40, 357 (1990). [20]C. Maie on, T. W. Donnelly, and I. Sick, Phys. Re . C 65, 025502 (2002). [21]J. Jou dan, Nucl. Phys. A603,117(1996). [22]A. De Pace, M. Na di, W. M. Albe ico, T. W. Donnelly, and A. Molina i, Nucl. Phys. A726, 303 (2003). [23]T. De Fo es and J. D. Walecka, Ad . Phys. 15,1(1966). [24]S. Bo i, C. Gius i, and F. D. Paca i, Phys. Rep. 226,1(1993). [25]T. W. Donnelly, in Nuclea /Nucleonic S uc u e and Inclusi e Elec on Sca e ing, P oceedings o he In e na ional School o Physics “En ico Fe mi,” Cou se CLIII, edi ed by A. Molina i and L. Ricca i (IOS, Ams e dam, 2003), p. 183. [26]J. D. Bjo ken and S. D. D ell, Rela i is ic Quan um Mechanics (McG aw-Hill, New Yo k, 1965). [27]T. W. Donnelly and A. S. Raskin, Ann. Phys. (N.Y.)169, 247 (1986). [28]T. W. Donnelly, M. J. Musol , W. M. Albe ico, M. B. Ba ba o, A. De Pace, and A. Molina i, Nucl. Phys. A541, 525 (1992). [29]L. Al a ez-Ruso, M. B. Ba ba o, T. W. Donnelly, and A. Mo- lina i, Phys. Le . B 497, 214 (2001). [30]O. Benha , V. R. Pandha ipande, and I. Sick, Phys. Le . B 410,79(1997). [31]C. Cio i Degli A i and S. Liu i, Phys. Le . B 225, 215 (1989). [32]A. Bodek e al., Phys. Re . D 20, 1471 (1979). [33]A. S ein e al., Phys. Re . D 12, 1884 (1975). [34]P. Amaud uz e al., New Muon Collabo a ion, Phys. Le . B 295, 159 (1992). [35]L. W. Whi low, S. Rock, A. Bodek, E. M. Rio dan, and S. Dasu, Phys. Le . B 250, 193 (1990). [36]A. D. Ma in, R. G. Robe s, W. J. S i ling, and R. S. Tho ne, Eu . Phys. J. C 4, 463 (1998); see also h p://du pdg.du .ac.uk/ hepda a/m s.h ml [37]G. Hohle , E. Pie a inen, I. Sabba S e anescu, F. Bo kowski, G. G. Simon, V. H. Wal he , and R. D. Wendling, Nucl. Phys. B114, 505 (1976). [38]J. A ing on e al., Phys. Re . Le . 82, 2056 (1999). [39]D. B. Day e al., Phys. Re . C 48, 1849 (1993). [40]R. G. A nold e al., Phys. Re . Le . 52, 727 (1984). [41]R. R. Whi ney, I. Sick, J. R. Ficenec, R. D. Kepha , and W. P. T owe , Phys. Re . C 9, 2230 (1974). [42]S. Gals e , H. Klein, J. Mo i z, K. H. Schmid , D. Wegene , and J. Bleckwenn, Nucl. Phys. B32, 221 (1971). [43]F. Iachello, A. D. Jackson, and A. Lande, Phys. Le . B 43, 191 (1973). [44]P. E. Bos ed, Phys. Re . C 51, 409 (1995). BARBARO, CABALLERO, DONNELLY, AND MAIERON PHYSICAL REVIEW C 69, 035502 (2004) 035502-16