The EMC Effect Gerald A. Miller, Univ. of Washington INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERNCOURIER VOLUME 53 NUMBER 4 MAY 2013 Deep in the nucleus: a puzzle revisited HEAVY IONS ASTROWATCH The key to finding out if a collision is head on p31 Planck reveals an almost perfect universe p12 IT’S A HIGGS BOSON The new particle is identified p21 Higinbotham, Miller, Hen CERN Courier 53N4(’13)24 WWW. What is the EMC effect? What does it mean? 1 What are the consequences? EMC Effect -Outline • Basic issues -what is the EMC effect, why important? • Simple ideas • What is Drell-Yan pair production, why relevant? • Why nucleon structure must be modified for nucleons in nuclei • Simple models and examples of tests • Two-nucleon effects are important • Necessities for future progress 2 Fundamental questions of Nuclear Physics • Is the nucleus made only of nucleons and mesons? • How does the nucleus emerge from QCD, a theory of quarks and gluons? • Why is the nucleon-meson picture of nuclei so accurate? • Is the gluonic content of the nucleus the same as for nucleons in free space? • Is there a non-perturbative sea in the nucleon? No one asked such questions before the EMC effect 3 was discovered Primer- Deep Inelastic Scattering- large ⌫, Q2 e Electron loses energy and is scattered by some angle: two variables: ⌫, Q2 Large ⌫, Q2 scattering on elementary quark. Four-momentum conservation ! Q dynamics depend on x = x P+ Q2 2M ⌫ x ratio of quark p+ to proton momentum P + (P ± ⌘ P 0 ± P 3 ) Nucleon from PDG P 1 0.9 NNPDF2.3 (NNLO) 0. xf(x,µ 2=10 GeV2) 0.8 The EMC effect involves deep inelastic scattering from nuclei EMC= European Muon Collaboration 0.7 0. g/10 0. 0.6 0. uv 0.5 0. 0.4 0.3 0. dv 0.2 u 0.1 0 -3 10 0. s 0. d 0. c 10-2 4x 10-1 1 0 1 Figure 19.4: The bands are x times the u (where f = uv , dv , u, d, s ≃ s̄, c = c̄, b = b̄, g) The EMC EFFECT Fig. 2: The image shows the ratio of deep-inelastic cross sections of Ca to D from NMC (solid circles) and SLAC (open circles). The downward slope from 0.3 < x < 0.7 and subsequent rise from xB > 0.7 is a universal characteristic of EMC data and has became known as the EMC effect. The reduction of the ratio at lower values of xB, where valence quarks should no longer be playing a significant role, is known as the shadowing region. Fig. 1: Image of the EMC data as it appeared in the November 1982 issue of the CERN Courier. This image nearly derailed the highly cited refereed publication (Aubert et al., 1983), as the editor argued that the data had already been published. Valence quark momentum is reduced Nucleon structure is modified: valence quark momentum depleted. How do quarks work in a nucleus? BUT EFFECTS ARE SMALL ~15% 5 The EMC EFFECT Fig. 2: The image shows the ratio of deep-inelastic cross sections of Ca to D from NMC (solid circles) and SLAC (open circles). The downward slope from 0.3 < x < 0.7 and subsequent rise from xB > 0.7 is a universal characteristic of EMC data and has became known as the EMC effect. The reduction of the ratio at lower values of xB, where valence quarks should no longer be playing a significant role, is known as the shadowing region. Fig. 1: Image of the EMC data as it appeared in the November 1982 issue of the CERN Courier. This image nearly derailed the highly cited refereed publication (Aubert et al., 1983), as the editor argued that the data had already been published. Valence quark momentum is reduced Nucleon structure is modified: valence quark momentum depleted. How do quarks work in a nucleus? BUT EFFECTS ARE SMALL ~15% 5 Simple models of reduction of valence quark momentum • quarks in nuclei move through a larger confinement volume (uncertainty principle) • bound nucleons are larger than free ones • nucleons in nuclei move in 6, 9 or 3A quark bags • nuclear binding, Fermi motion, pionic effects 6 Simple models of reduction of valence quark momentum • quarks in nuclei move through a larger confinement volume (uncertainty principle) • bound nucleons are larger than free ones • nucleons in nuclei move in 6, 9 or 3A quark bags • nuclear binding, Fermi motion, pionic effects EMC – “Everyone’s Model is Cool (1985)’’ 6 One thing I learned since ‘85 One thing I learned since ‘85 • One model is not cool• unmodified nucleon -free structure function Deep Inelastic scattering from nucleinucleons only free structure function • Hugenholz van Hove theorem nuclear stability implies (in rest frame) P+=P- =MA Smith Miller ‘02 Binding causes no EMC effect Pb • P+ =A(MN - 8 MeV) • average nucleon k+ k+=MN-8 MeV, Not much spread F2A/A~F2N no EMC effect Smith & Miller Phys.Rev. C65 (2002) 015211, Phys.Rev. C66 (2002) 049903 SLAC-E139 Phys.Rev. C65 (2002) 055206 Nucleons and pions PA+ = PN+ + Pπ+ =MA Pπ+ /MA =.04, explain EMC try Drell-Yan, Bickerstaff, Birse, Miller 84 proton(x1) nucleus(x2) x1 x2 Phys.Rev.D33:3228,1986 Phys.Rev.Lett.53:2532,1984. Nucleons and pions PA+ = PN+ + Pπ+ =MA Pπ+ /MA =.04, explain EMC Drell-Yan, E772 PRL 69,1726 (92) π fails No one’s model is cool Nucleons and pions PA+ = PN+ + Pπ+ =MA Pπ+ /MA =.04, explain EMC Drell-Yan, E772 PRL 69,1726 (92) π fails No one’s model is cool Bertsch, Frankfurt, Strikman “crisis in nuclear theory” conventional physics does not work Nucleons, pions, shadowing, universal nucleon modification • A model containing all of these aspects does account for DIS and DY-Kulagin Petti • No underlying dynamics-can’t predict other phenomena 11 Single nucleon modification by nuclei p ⇡ n • Does it make sense? It is inevitable. Pion cloud modified by nucleus, W cloud too • Neutron in nucleus is modified, lifetime changed from 15 minutes to forever • Binding changes energy denominator, suppresses peν component • Change energy denominator change wave fun • Also Strong fields polarize nucleons- analog of Stark effect Inevitability of medium modifications-(e,e’p) ⇤ MA (⌫, ~q ) (Ef , p~ + ~q ) p Form factor modified because p2 6= M 2 Problem: conventional nuclear wave function involves on-mass shell nucleons (Es , p~) Nucleus A-1 13 Single nucleon in a nucleus 1968 SLAC-MIT nucleon not a point: ! quarks don’t interact 1947 Shell Model R R 1982 EMC or 14 ? ? Nucl.Phys. B250 (1985) 143- 1985 PLC Suppression Frankfurt Strikman 1995 BLC Frank Jennings Miller Phys.Rev. C54 (1996) 920- +✏ ? ? ? ? Nucleon has large blob-like configuration BLC and small point like configuration PLC! BLC is affected by nucleus PLC, not affected . Result PLC suppressed/BLC enhanced 15 Nucleon in medium- 5 models 1. QMC- quarks in nucleons (MIT bag) exchange mesons with nuclear Nuclear matter medium, quark mass 2. Use NJL instead of bag Cloét External fields 3. CQSM- quarks in nucleons (soliton) exchange infinite pairs of pions, vector mesons with nuclear medium, mq 4. Suppression of point-likeconfigurations, 5. Enhancement of blob-like configurations polarization Spin experiments-NJL in medium • g , g 1p in nuclei 1n Bentz, Cloet, Thomas ! • other way to enhance EMC? ratio of g1 medium to free Kuhn talk Spin Chiral Quark Soliton Model – Diakonov, Petrov, Polykov, quarks couple to vacuum instantons Negele et al hep-lat/9810053 • Vacuum dominated by topological charge density instantons • quarks with spontaneously generated masses interact with pions ! ! • Nucleon is soliton in pion field • M=420 MeV • good nucleon properties, DIS and magnetic moments Chiral Quark Soliton Model of NucleusSmith, Miller 2 π exchange – attraction ω (vector meson) exchange repulsion Phys.Rev. C72 (2005) 022203 Phys.Rev. C70 (2004) 065205 Phys.Rev.Lett. 91 (2003) 212301, Phys.Rev.Lett. 98 (2007) 099902 Double self consistency profile function and kf Results Smith & Miller ’03,04,05 g1 ratio EMC ratio full Nuclear Drell Yan valence only sea is not much modified About same as DIS, not larger contrasts QMC Kuhn talk Models Predict Form-Factor Medium Modifications Another medium effect: form factors • Changes in the internal structure of bound nucleons result also in bound nucleon form factors. • Observable effects predicted: CQS QMC ρ = 0.5 ρ0 ρ = 1.0 ρ0 ρ = 1.5 ρ0 Chiral Quark Soliton (CQS), Quark Meson Coupling (QMC), Skyrme, Nambu-Jona-Lasinio (NJL), GPD Models. • Model predictions: ‣ are density and Q2 dependent, ‣ show similar behavior, ‣ consistent with experimental CQS: J.R. Smith and G.A. Miller, Phys. Rev. C 70, 065205 (2004) QMC: D.H. Lu et al., Phys. Lett. B 417, 217 (1998) data (within large uncertainties). NJL: I.C. Cloet, W. Bentz, and A.W. Thomas (to be published) 7 S Strauch slide 21 S. Strauch ratio of GE /GM • 2H and 1H polarization-transfer data are similar ≈ 10% Effect • 4He data are significantly different than 2H, 1H data low pm data 2H: B. Hu et al., PRC 73, 064004 (2006). 4He: S. Dieterich et al., PLB 500, 47 (2001); S. S., et al., PRL 91, 052301 (2003); M. Paolone, et al., PRL 105, 0722001 (2010); S. Malace et al., PRL 106, 052501 (2011) 1 22 Enhancement of Blob-like Configurations- Frank,Jennings, Miller PRC 54, 920 free place in medium: normal size components attracted energy goes down PLC does not interact- color screening-FS BLC is enhanced quarks lose momentum in medium 1995 Frank, Jennings, Miller Enhancement of Blob-Like Configurations FS-PLC has NO int. with medium energy denominator increased EMC ratio Frank,Jennings Miller ‘95 evaluated as QCD Stark, not modified energy denominator More data [3-69] S. Bueltmann et al., Jefferson Lab Experiment E12-06-113 [4-1] J. Seely et al., Phys. Rev. Lett. 103, (2009) 202301 [3-70] G.G. Petratos et al., Jefferson Lab Experiment E12-10-103 [4-2] N. Fomin, et al., Rev. Lett. 108, 092502 (2012) Another outstanding question is whether the [3-71] nuclearP.A. medium alters of Phys. bound Souder et al.,the Thestructure SoLID Experiment, Jefferson Lab Experiment E12 (a) (b) (c) nucleons and, if so, how? The neutron lifetime in nuclei is certainly different. The first evidence [4-3] J.J. Aubert et al., Phys. Lett. 123B (1983) 275 [3-72] Accardi et al.,deep-inelastic Phys. Rev. D 84, 014008 (2011) for nucleon structure modification was the EMC effectA. [4-3], in which scattering [4-4] L.B. Weinstein et al., Phys. Rev. Lett. 106, 052301 (2011 from nuclear quarks is significantly different [3-73] than from a “free” nucleon G.D.quarks Cates,inside C.W. de Jager, S. Riodan(see and B. Wojtsekhowski, Phys. Rev L Figure 4.1a). The per-nucleon DIS cross section ratio of nucleus to Baillie deuterium [4-5]A N. et al.,decreases Phys. Rev. Lett. 108, 142001 (2012) (2011) 252003 approximately linearly for 0.3 < xB < 0.7. The slope of this ratio in this region increases with A [4-6] al., A.V. Klimenko Phys. Rev. C I.C. 73, 035212 Eur. Phys. J. et STal., 140, 53 (2007); Clöet et(2006) al., Fewbut does not scale simply with average nuclear[3-74] densityC.D. (see Roberts Figure et 4.2). Despite a world-wide Systems 46, 1 (2009) Bueltmann al.,GeV “The Structure of the Free Neutron a effort in experiment and theory, the origins of the EMC effect [4-7] remainS.unclear. Theet 12 LabMiller, Experiment E12-06-113. experimental program will measure the EMC effect in aI.C. wide range nuclei to help unravel the (2012) [3-75] Clöet andofG.A. PRC 86, 015208 mystery [4-24, 4-25]. Hen et al., Nucleon Structure Functions, [3-76] M. Guidal,[4-8] M. V.O. Polyakov, A.“In V. Medium Radyushkin, and M. Vanderhaeghen Ph Jefferson Lab Expt E12-11-107. 72,4.2) 054013 Recent phenomenological comparisons [4-4] (see Figure show(2005) that the strength of the EMC effect in different nuclei is linearly related to the short P.Maris range correlations factor, A62, /Sargsian, d055204 ). [4-9] W.scale Melnitchouk, and M.I. Strikman, Z. Phy [3-77] and P.Tandy, Phys. Rev.𝑎2C(M. (2000) This linear relation indicates, but does not prove, that the EMC effect is caused by local [4-10] L. ElA.V. Fassi,Radyushkin, et al., Phys. Lett. B712, 326 (2012) and modifications of nucleon structure occurring[3-78] when V.A. two Nesterenko would-be nucleons make a closePhys. Lett. B115, 410(1982) [4-11] Frankfurt, G.A. Miller encounter and briefly comprise a system of density enough toPhys.Rev.D beL.comparable to that of and M.Strikman, Phys. Rev. C [3-79] high C-W. Hwang, 64(2001)n034001 neutron stars. This relationship will be tested and refined at 12[4-12] GeV by seriesetofal.,EMC andof Color Transparency in Exclusi K. aHafidi “Study [4-1] J. Seely et al., Phys. Rev. Lett. 103, (2009) 202301 SRC experiments covering a wide range of nuclei [4-19, 4-20, 4-24,Electroproduction 4-25]. The deuteron off Nuclei”, Jefferson Lab Experiment N. (per-nucleon) Fomin, et al., Rev. Lett. 108, 092502 (2012) experiment mentioned [4-18]cross will increase our understanding of Phys. the system Figure 4.1: The electronabove scattering section[4-2] ratios of two-nucleon various nuclei to that we use as a baseline for both the EMC and SRC measurements. 12 [4-13] E.M. Aitala et al. [E791 Collaboration], Phys. Rev. Lett. al.,<Phys. 123B (1983) deuterium. (a) Ratios for 0.2 < xB < 0.9 [4-1]; (b) [4-3] RatiosJ.J. forAubert C foret0.3 xB < Lett. 2 [4-1, 4-2]; (c) 275 [4-14] L. Frankfurt, G.A. Miller and M. Strikman, Phys. Lett. B Ratios for 0.8 < xB < 1.8 [4-2]. [4-4] L.B. Weinstein et al., Phys. Rev. Lett. 106, 052301 (2011) [4-15] B. Clasie, et al., Phys. Rev. Lett. 99, 242502 (2007) Nucleons acquire high-momentum via short-range interactions, influence of [4-5] N. Baillie et rather al., Phys.than Rev.by Lett.the 108, 142001 (2012) 4a.2 Nucleon properties in nuclei relative NN wave function at short distances. the nuclear mean-field. Thus, for momenta above Fermi sea, the of the momentum [4-6]theA.V. Klimenko et al.,shape Phys. Rev. C 73, 035212 (2006) distribution should be universal. This is shown by[4-7] the plateaus (regions of constant cross section 60 S. Bueltmann et al., “The Structure of the Free Neutron at Large x-Bjorke ratio) observed at xB > 1.5 (see Figure 4.1c). The values of the ratio at these plateaus, a2(A/d), Lab Experiment E12-06-113. are closely related to the probability of finding a[4-8] nucleon belonging to a short-range correlated O. Hen et al., “In Medium Nucleon Structure Functions, SRC, and the EM pair in nucleus A relative to deuterium. Jefferson Lab Expt E12-11-107. W.understand Melnitchouk, the M. Sargsian, M.I. Strikman, Experiments at 12 GeV will study the deuteron to[4-9] better simplestand nuclear systemZ. Phys. A359, 99 (199 El Fassi, et above al., Phys. B712,greater 326 (2012) [4-18]. Other experiments will extend the SRC [4-10] studiesL.described toLett. a much range 3 3 of xB, momentum transfers, and nuclei (including H and He) toG.A. study two three nucleon [4-11] L. Frankfurt, Miller andand M.Strikman, Phys. Rev. C 78, 015208 (2008 correlations (including their isospin character), with higher nucleon momenta [4-19, 4-20]. The [4-12] K.plotted Hafidi et al.,the“Study Color Transparency in Figure 4.2: (left) The strength of the EMC effect (the EMC slope) versus averageofnuclear density [426Exclusive Vector Meson 2 (right)from The strength effect plotted versus the probe SRCElectroproduction scale factors [4-4]. off TheNuclei”, drawing in the upper highest Q1]. data the xofB the > 1EMC measurements will the distribution of superfast quarks in Jefferson Lab Experiment E12-06-106. left shows deep inelastic electron scattering from a quark in a nucleon. The drawing in the lower right shows nuclei, greatly extending our understanding of nucleons at short [4-13] E.M. Aitaladistances. et al. [E791 Collaboration], Phys. Rev. Lett. 86, 4773 (2001) More data [3-69] S. Bueltmann et al., Jefferson Lab Experiment E12-06-113 [4-1] J. Seely et al., Phys. Rev. Lett. 103, (2009) 202301 [3-70] G.G. Petratos et al., Jefferson Lab Experiment E12-10-103 [4-2] N. Fomin, et al., Rev. Lett. 108, 092502 (2012) Another outstanding question is whether the [3-71] nuclearP.A. medium alters of Phys. bound Souder et al.,the Thestructure SoLID Experiment, Jefferson Lab Experiment E12 (a) (b) (c) nucleons and, if so, how? The neutron lifetime in nuclei is certainly different. The first evidence [4-3] J.J. Aubert et al., Phys. Lett. 123B (1983) 275 [3-72] Accardi et al.,deep-inelastic Phys. Rev. D 84, 014008 (2011) for nucleon structure modification was the EMC effectA. [4-3], in which scattering [4-4] L.B. Weinstein et al., Phys. Rev. Lett. 106, 052301 (2011 from nuclear quarks is significantly different [3-73] than from a “free” nucleon G.D.quarks Cates,inside C.W. de Jager, S. Riodan(see and B. Wojtsekhowski, Phys. Rev L Figure 4.1a). The per-nucleon DIS cross section ratio of nucleus to Baillie deuterium [4-5]A N. et al.,decreases Phys. Rev. Lett. 108, 142001 (2012) (2011) 252003 approximately linearly for 0.3 < xB < 0.7. The slope of this ratio in this region increases with A [4-6] al., A.V. Klimenko Phys. Rev. C I.C. 73, 035212 Eur. Phys. J. et STal., 140, 53 (2007); Clöet et(2006) al., Fewbut does not scale simply with average nuclear[3-74] densityC.D. (see Roberts Figure et 4.2). Despite a world-wide Systems 46, 1 (2009) Bueltmann al.,GeV “The Structure of the Free Neutron a effort in experiment and theory, the origins of the EMC effect [4-7] remainS.unclear. Theet 12 LabMiller, Experiment E12-06-113. experimental program will measure the EMC effect in aI.C. wide range nuclei to help unravel the (2012) [3-75] Clöet andofG.A. PRC 86, 015208 mystery [4-24, 4-25]. Hen et al., Nucleon Structure Functions, [3-76] M. Guidal,[4-8] M. V.O. Polyakov, A.“In V. Medium Radyushkin, and M. Vanderhaeghen Ph Jefferson Lab Expt E12-11-107. 72,4.2) 054013 Recent phenomenological comparisons [4-4] (see Figure show(2005) that the strength of the EMC effect in different nuclei is linearly related to the short P.Maris range correlations factor, A62, /Sargsian, d055204 ). [4-9] W.scale Melnitchouk, and M.I. Strikman, Z. Phy [3-77] and P.Tandy, Phys. Rev.𝑎2C(M. (2000) This linear relation indicates, but does not prove, that the EMC effect is caused by local [4-10] L. ElA.V. Fassi,Radyushkin, et al., Phys. Lett. B712, 326 (2012) and modifications of nucleon structure occurring[3-78] when V.A. two Nesterenko would-be nucleons make a closePhys. Lett. B115, 410(1982) [4-11] Frankfurt, G.A. Miller encounter and briefly comprise a system of density enough toPhys.Rev.D beL.comparable to that of and M.Strikman, Phys. Rev. C [3-79] high C-W. Hwang, 64(2001)n034001 neutron stars. This relationship will be tested and refined at 12[4-12] GeV by seriesetofal.,EMC andof Color Transparency in Exclusi K. aHafidi “Study [4-1] J. Seely et al., Phys. Rev. Lett. 103, (2009) 202301 SRC experiments covering a wide range of nuclei [4-19, 4-20, 4-24,Electroproduction 4-25]. The deuteron off Nuclei”, Jefferson Lab Experiment N. (per-nucleon) Fomin, et al., Rev. Lett. 108, 092502 (2012) experiment mentioned [4-18]cross will increase our understanding of Phys. the system Figure 4.1: The electronabove scattering section[4-2] ratios of two-nucleon various nuclei to that we use as a baseline for both the EMC and SRC measurements. 12 [4-13] E.M. Aitala et al. [E791 Collaboration], Phys. Rev. Lett. al.,<Phys. 123B (1983) deuterium. (a) Ratios for 0.2 < xB < 0.9 [4-1]; (b) [4-3] RatiosJ.J. forAubert C foret0.3 xB < Lett. 2 [4-1, 4-2]; (c) 275 [4-14] L. Frankfurt, G.A. Miller and M. Strikman, Phys. Lett. B Ratios for 0.8 < xB < 1.8 [4-2]. [4-4] L.B. Weinstein et al., Phys. Rev. Lett. 106, 052301 (2011) [4-15] B. Clasie, et al., Phys. Rev. Lett. 99, 242502 (2007) Nucleons acquire high-momentum via short-range interactions, influence of [4-5] N. Baillie et rather al., Phys.than Rev.by Lett.the 108, 142001 (2012) 4a.2 Nucleon properties in nuclei relative NN wave function at short distances. the nuclear mean-field. Thus, for momenta above Fermi sea, the of the momentum [4-6]theA.V. Klimenko et al.,shape Phys. Rev. C 73, 035212 (2006) distribution should be universal. This is shown by[4-7] the plateaus (regions of constant cross section 60 S. Bueltmann et al., “The Structure of the Free Neutron at Large x-Bjorke ratio) observed at xB > 1.5 (see Figure 4.1c). The values of the ratio at these plateaus, a2(A/d), Lab Experiment E12-06-113. are closely related to the probability of finding a[4-8] nucleon belonging to a short-range correlated O. Hen et al., “In Medium Nucleon Structure Functions, SRC, and the EM pair in nucleus A relative to deuterium. Jefferson Lab Expt E12-11-107. Coincidence? W.understand Melnitchouk, the M. Sargsian, M.I. Strikman, Experiments at 12 GeV will study the deuteron to[4-9] better simplestand nuclear systemZ. Phys. A359, 99 (199 El Fassi, et above al., Phys. B712,greater 326 (2012) [4-18]. Other experiments will extend the SRC [4-10] studiesL.described toLett. a much range 3 3 of xB, momentum transfers, and nuclei (including H and He) toG.A. study two three nucleon [4-11] L. Frankfurt, Miller andand M.Strikman, Phys. Rev. C 78, 015208 (2008 correlations (including their isospin character), with higher nucleon momenta [4-19, 4-20]. The [4-12] K.plotted Hafidi et al.,the“Study Color Transparency in Figure 4.2: (left) The strength of the EMC effect (the EMC slope) versus averageofnuclear density [426Exclusive Vector Meson 2 (right)from The strength effect plotted versus the probe SRCElectroproduction scale factors [4-4]. off TheNuclei”, drawing in the upper highest Q1]. data the xofB the > 1EMC measurements will the distribution of superfast quarks in Jefferson Lab Experiment E12-06-106. left shows deep inelastic electron scattering from a quark in a nucleon. The drawing in the lower right shows nuclei, greatly extending our understanding of nucleons at short [4-13] E.M. Aitaladistances. et al. [E791 Collaboration], Phys. Rev. Lett. 86, 4773 (2001) Inclusive A(e,e ) measurements ! At high nucleon momentum, distributions are similar in shape for light and heavy nuclei: SCALING. nA (k ) = CA ⋅ nD (k ) high k Adapted from Ciofi degli Atti ! Short distance two-nucleon relative wave function same in all nuclei . ! One can get the probability of 2N-SRC in any nucleus, from the scaling factor. Piasetzky talk 27 Implications of data • Previous models need to be extended to a larger range of x • Detailed nuclear dependence must be explained (Dutta talk) • Challenge: is EMC effect best described as being on single nucleon or a correlated pair of nucleons? 28 Are nucleons in the SRC modified? • Need to start with a nuclear model of SRC and compute resulting EMC effect caused by modified structure function • Medium modification due to mean field (previously discussed models) alternate hypothesis 29 Phenomenology Hen et al Int. J. Mod. Phys.E22, (’13)1330017 • Ciofi degli Atti & Simula, PRC53,1689 (96)-nuclear model- Spectral function has two terms - low momentum, mean-field MF part 80%, high momentum short-ranged correlations SRC 20% • Strikman & Frankurt: relate nuclear DIS to nucleon structure function using spectral function PLB 183, 254 (87) • Modification of nucleon structure function is associated with MF or with SRC- two models 30 April 11, 2013 0:17 WSPC/INSTRUCTION FILE EMC˙reviewMar15b April 11, 2013 0:17 WSPC/INSTRUCTION FILE Universal modification to nucleon in SRC The EMC Effect and High Momentum Nucleons in Nuclei Universal modification to nucleon in MF 21 Which gives a better fit? 31 Int. J. Mod. Phys.E22, (’13)1330017 Fig. 9: The ratios of free to bound structure functions for various nuclei, extracted EMC˙reviewMar15b The EMC Effect and High Momentum Nucleons in Nuclei 23 13 0:17 WSPC/INSTRUCTION FILE M o the EMC effect is the unique association with short ranged correlations. Note 9 Be was not included in the model calculations since a 9 Be spectral function not available. Note also that this model does not separate valence and sea q distributions and therefore can’t make predictions about the Drell-Yan data. Further experiments are needed to determine whether the Mean-Field or (SRC) nucleonsModified Function MFquasi-elastic ele are modified byStructure the nuclear medium. For example, scattering would be sensitive to the former but not the latter. Modified Structure Functions Modified Structure Function O. Hen et al. ([1]* (x-[0])+[2]*(x -[0 ])^2)/((1./5 6)*(5./9 )*1.094*s qrt(x )*(26* 2* (1-x )^3+30*(9./8)* (1-x )^4)+(11./9)* 0.1857*(1-x)^ 7) ([1]* (x-[0])+[2]*(x- [0 ])^2)/((1./5 6)*(5./9 )*1.094*s qrt(x )*(26* 2* (1-x )^3+30*(9./8)*(1-x )^4)+(11./9)* 0.1857*(1-x)^ 7) N ∆FN 2 / F2 N ∆FN 2 / F2 0 EMC˙reviewMar15b 0.3 0.25 0.04 0.03 0.02 0.01 0.2 0 -0.01 0.15 -0.02 0.1 -0.03 0.05 0.3 0.3 0.35 0.4 0.45 0.5 0.55 0.6 0.65 0.35 0.7 x 0.4 0.45 0.5 0.55 0.6 0.65 0.7 x Fig. 10: Same as Fig. 8, assuming universal modification to Mean-Field nucl It is assumed that deuterium has no Mean-Field component, see text for deta ig. 8: The ratio of the modification term, ∆F2N to the free nucleon structure Is the effect due to nucleons in SRC pairs or to nucleons unction, F2NEMC . moving in the mean field? Summary We next proceed by assuming that nucleons in high energy excited5.states (corelated nucleons) have a different structure function F!2N (x) than free ones F (x). We have recent data showing that the detailed A dependence of the 2Nreviewed hus we make the replacements effect provides important hints in understanding the origin of that effect. The (0) (1) (0+1) I1 (A)F2 → I1 (A)F2N + I1 (A)F!2N = I1 (1) (A)F2N + I1 (A)∆F2N , etc, (19) here N N 32 N 13 0:17 WSPC/INSTRUCTION FILE M o the EMC effect is the unique association with short ranged correlations. Note 9 Be was not included in the model calculations since a 9 Be spectral function not available. Note also that this model does not separate valence and sea q distributions and therefore can’t make predictions about the Drell-Yan data. Further experiments are needed to determine whether the Mean-Field or (SRC) nucleonsModified Function MFquasi-elastic ele are modified byStructure the nuclear medium. For example, scattering would be sensitive to the former but not the latter. Modified Structure Functions Modified Structure Function O. Hen et al. ([1]* (x-[0])+[2]*(x -[0 ])^2)/((1./5 6)*(5./9 )*1.094*s qrt(x )*(26* 2* (1-x )^3+30*(9./8)* (1-x )^4)+(11./9)* 0.1857*(1-x)^ 7) ([1]* (x-[0])+[2]*(x- [0 ])^2)/((1./5 6)*(5./9 )*1.094*s qrt(x )*(26* 2* (1-x )^3+30*(9./8)*(1-x )^4)+(11./9)* 0.1857*(1-x)^ 7) N ∆FN 2 / F2 N ∆FN 2 / F2 0 EMC˙reviewMar15b 0.3 0.25 0.04 0.03 0.02 0.01 0.2 0 -0.01 0.15 -0.02 0.1 -0.03 0.05 0.3 0.3 0.35 0.4 0.45 0.5 0.55 0.6 0.65 0.35 0.7 x 0.4 0.45 0.5 0.55 0.6 0.65 0.7 x Fig. 10: Same as Fig. 8, assuming universal modification to Mean-Field nucl It is assumed that deuterium has no Mean-Field component, see text for deta ig. 8: The ratio of the modification term, ∆F2N to the free nucleon structure Is the effect due to nucleons in SRC pairs or to nucleons unction, F2NEMC . moving in the mean field? Summary We next proceed by assuming that nucleons in high energy excited5.states (corelated nucleons) have a different structure function F!2N (x) than free ones F (x). We have recent data showing that the detailed A dependence of the 2Nreviewed hus we make the replacements effect provides important hints in understanding the origin of that effect. The I1 (A)F2 → here (0) I1 (A)F2N + (1) I1 (A)F!2N N YES = N (0+1) I1 (A)F2N (1) + I1 (A)∆F2N , etc, (19) 32 N Requirements & Goals • • • • Model the free distributions Good support Consistency with nuclear properties Describe deep inelastic and di-muon production data- valence plus sea • describe detailed A (N,Z) dependence • Predict new phenomena Ways to search for medium modification of nucleon structure • Quasi-elastic scattering, Coulomb sum rule form factors of bound nucleons • Quasi-elastic, recoil polarization- GE /GM • DIS on deuteron, detect spectator • A dependence • Parity violating DIS 34 Summary • nucleon structure is modified by nucleus • minimum model requirements- EMC, DY, nuclear saturation, A-dependence • predict new phenomena • needed –better evaluations of models • experimental tests –form factors in medium, ( eA ! e0 XN ) spectator tag, PVDIS nuclear gluon distribution?? • new experiments Jlab and others to find out how quarks work in a nucleus Where do we stand after 33 years? 36 Where do we stand after 33 years? 36
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