Comparison of quasi-elastic cross sections using spectral functions with (e,e') data from 0.5 GeV to 1.5 GeV Hiroki Nakamura (Waseda U). Makoto Sakuda.

Slides:



Advertisements
Similar presentations
Weak Coherent Kaon Production L. Alvarez-Ruso 1, J. Nieves 1, I. Ruiz Simo 2, M. Valverde 3, M. Vicente Vacas 1 1.IFIC, Universidad de Valencia 2.Universidad.
Advertisements

BigBite K.Egiyan Probabilities of SRC in Nuclei Measured with A(e,e / ) Reactions K. Egiyan (Yerevan Physics Institute, Yerevan, Armenia and Jefferson.
1 Eta production Resonances, meson couplings Humberto Garcilazo, IPN Mexico Dan-Olof Riska, Helsinki … exotic hadronic matter?
Spectroscopy at the Particle Threshold H. Lenske 1.
Neutrino-induced meson production model for neutrino oscillation experiments Satoshi Nakamura Nuclear Theory Group.
JLab_Phys_Semin_Dec05 K. Egiyan Today’s Nucleonic Picture of Nuclei Kim Egiyan Yerevan Physics Institute, Armenia and Jefferson Lab, USA.
Neutrino Interactions with Nucleons and Nuclei Tina Leitner, Ulrich Mosel LAUNCH09 TexPoint fonts used in EMF. Read the TexPoint manual before you delete.
Degree of polarization of  produced in quasielastic charge current neutrino-nucleus scattering Krzysztof M. Graczyk Jaroslaw Nowak Institute of Theoretical.
N*(2007) observed at LNS Sendai H. Shimizu Laboratory of Nuclear Science Tohoku University Sendai NSTAR2007, Sep.5-8, 2007, Bonn 1670.
F.Sanchez (UAB/IFAE)ISS Meeting, Detector Parallel Meeting. Jan 2006 Low Energy Neutrino Interactions & Near Detectors F.Sánchez Universitat Autònoma de.
Howard Budd, Univ. of Rochester1 Vector and Axial Form Factors Applied to Neutrino Quasi-Elastic Scattering Howard Budd University of Rochester (in collaboration.
Arie Bodek, Univ. of Rochester1 Vector and Axial Form Factors Applied to Neutrino Quasi-Elastic Scattering Howard Budd University of Rochester
The method of extracting excitation energy for the ISiS data is described in T.Lefort et al, Phys. Rev. C, 64, (2001). Figure (mader-BUU) : Projectile.
African Summer School 2012 Connecting the SRC & EMC Effects by.
Nucleon Optical Potential in Brueckner Theory Wasi Haider Department of Physics, AMU, Aligarh, India. E Mail:
Lecture 10: Inelastic Scattering from the Proton 7/10/2003
A. Blondel, M.Campanelli, M.Fechner Energy measurement in quasi-elastics Unfolding detector and physics effects Alain Blondel Mario Campanelli Maximilien.
DPG Tagung, Breathing mode in an improved transport model T. Gaitanos, A.B. Larionov, H. Lenske, U. Mosel Introduction Improved relativistic transport.
UK Hadron Physics D. G. Ireland 10 October 2014 NuPECC Meeting, Edinburgh.
Study of hadron properties in cold nuclear matter with HADES Pavel Tlustý, Nuclear Physics Institute, Řež, Czech Republic for the HADES Collaboration ,
ニュートリノ原子核反応 佐藤 透 ( 阪大 理 ) JPARC Dec Our previous works on neutrino reaction single pion production(Delta region) nuclear coherent pion production.
12 February 2003 M.Sakuda Neutrino - Nucleus Interactions Low Energy Neutrino-Nucleus Interactions Makoto Sakuda (KEK) in collaboration with C.Walter,
1 Formation spectra of  -mesic nuclei by (  +,p) reaction at J-PARC and chiral symmetry for baryons Hideko Nagahiro (RCNP) Collaborators : Daisuke Jido.
1 Nuclear Physics and Electron Scattering. 2 Four forces in nature –Gravity –Electromagnetic –Weak –Strong  Responsible for binding protons and neutrons.
Extending the Bertini Cascade Model to Kaons Dennis H. Wright (SLAC) Monte Carlo April 2005.
Lecture 16: Beta Decay Spectrum 29/10/2003 (and related processes...) Goals: understand the shape of the energy spectrum total decay rate sheds.
F. Sammarruca, University of Idaho Supported in part by the US Department of Energy. From Neutron Skins to Neutron Stars to Nuclear.
Neutral pion photoproduction and neutron radii Dan Watts, Claire Tarbert University of Edinburgh Crystal Ball and A2 collaboration at MAMI Eurotag Meeting.
RCNP.08 Breakup of halo nuclei with Coulomb-corrected eikonal method Y. Suzuki (Niigata) 1.Motivation for breakup reactions 2.Eikonal and adiabatic approximations.
Isospin mixing and parity- violating electron scattering O. Moreno, P. Sarriguren, E. Moya de Guerra and J. M. Udías (IEM-CSIC Madrid and UCM Madrid) T.
Precision Measurement of R L and R T of Quasi-Elastic Electron Scattering In the Momentum Transfer Range 0.55GeV/c≤|q|≤1.0GeV/c* Yan Xinhu Department of.
N* Production in α-p and p-p Scattering (Study of the Breathing Mode of the Nucleon) Investigation of the Scalar Structure of baryons (related to strong.
M. Matsuo, PRC73(’06) Matter Calc. Two-particle density.
Preliminary Results from the MINER A Experiment Deborah Harris Fermilab on behalf of the MINERvA Collaboration.
Dott. Antonio Botrugno Ph.D. course UNIVERSITY OF LECCE (ITALY) DEPARTMENT OF PHYSICS.
Few Body-18Santos, Brazil August 25, Meson Exchange Currents in Pion Double Charge Exchange Reaction Roman Ya. Kezerashvili NY City College of Technology.
1 Physics Requirements on Reconstruction and Simulation Software Jorge G. Morfín - Fermilab.
Neutrino-Nucleus QE Scattering GTG Los Alamos Nat. Lab.
Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology.
Three-body force effect on the properties of asymmetric nuclear matter Wei Zuo Institute of Modern Physics, Lanzhou, China.
Model independent extraction of neutron structure functions from deuterium data. Svyatoslav Tkachenko University of South Carolina.
Neutrino cross sections in few hundred MeV energy region Jan T. Sobczyk Institute of Theoretical Physics, University of Wrocław (in collaboration with.
Issues in the Quasi-free Delta Production Region Ryoichi Seki (CSUN/Caltech) in collaboration with Hiroki Nakamura (Waseda) RCCN International Workshop;
Effects Of Distortion On Trojan Horse Applications Rosario Gianluca Pizzone INFN – Laboratori Nazionali del Sud Catania.
PKU-CUSTIPEN 2015 Dirac Brueckner Hartree Fock and beyond Herbert Müther Institute of Theoretical Physics.
Reaction cross sections of carbon isotopes incident on proton and 12 C International Nuclear Physics Conference, Tokyo, Japan June 3-8, 2007 W. Horiuchi.
PROPERTIES OF HIGH-ENERGY ISOSCALAR MONOPOLE EXCITATIONS IN MEDIUM-HEAVY MASS SPHERICAL NUCLEI M. L. Gorelik 1), S. Shlomo 2), B. A. Tulupov 3), M. H.
Important role of three-body repulsive force effect in nuclear reactions Takenori FURUMOTO (Osaka City Univ. ) 19th International IUPAP Conference on Few-Body.
Simultaneous photo-production measurement of the  and  mesons on the nucleons at the range 680 – 1500 MeV N.Rudnev, V.Nedorezov, A.Turinge for the GRAAL.
THE K + -NUCLEUS MICROSCOPIC OPTICAL POTENTIAL AND CALCULATIONS OF THE CORRESPONDING DIFFERENTIAL ELASTIC AND TOTAL REACTION CROSS SECTIONS V.K.LUKYANOV,
Comparison of GENIE with Garino Data Xin Qian BNL In collaboration with Steve Dytman 1.
1  - mesic nuclei and baryon chiral symmetry in medium Hideko Nagahiro (Nara Women’s Univ.) collaborators: Daisuke Jido (Tech. Univ. Muenchen) Satoru.
Search for direct evidence of tensor interaction in nuclei = high momentum component in nuclei = TERASHIMA Satoru 寺嶋 知 Depart. of Nuclear Science and Technology,
HADRON 2009, FloridaAnar Rustamov, GSI Darmstadt, Germany 1 Inclusive meson production at 3.5 GeV pp collisions with the HADES spectrometer Anar Rustamov.
Comparison of GENIE with Garino Data Xin Qian BNL In collaboration with Steve Dytman 1.
Path forward: theory vs experiment needs, QE discussion input Comments/Observations: R. Tayloe, Nuint'09.
Possible Ambiguities of Neutrino-Nucleus Scattering in Quasi-elastic Region K. S. Kim School of Liberal Arts and Science, Korea Aerospace University, Korea.
Axial-vector mass MA and K2K Q2 distribution
Jun Kameda (ICRR) RCCN International workshop at Kashiwa (Dec.10,2004)
Possible Ambiguities of Neutrino-Nucleus
Kaons Propagation Through Nuclei
Quasielastic Scattering at MiniBooNE Energies
Carlotta Giusti University and INFN Pavia
Satoshi Adachi Research Center for Nuclear Physics (RCNP),
PHL424: γ-decay γ-decay is an electromagnetic process where the nucleus decreases in excitation energy, but does not change proton or neutron numbers This.
presented by Werner Boeglin Florida International University Miami
Deeply Bound Mesonic States -Case of Kaon-
On a Search for -Mesic Nuclei at MAMI-C
Di-nucleon correlations and soft dipole excitations in exotic nuclei
for the A1 collaboration
Presentation transcript:

Comparison of quasi-elastic cross sections using spectral functions with (e,e') data from 0.5 GeV to 1.5 GeV Hiroki Nakamura (Waseda U). Makoto Sakuda (Okayama U.) Ryoichi Seki (CSUN,Caltech)

Introduction Goal is to calculate -A (mainly quasi-elastic) cross sections with appropriate Nuclear Effects and Form Factors. Nuclear Effects and Form Factors are verified with comparing C,O(e,e’) data. Spectral function vs. Fermi Gas model (NuInt04 hep-ph/ ) The latest form factors are compared with dipole form factor. Pauli blocking and Final State Interaction.

Vertex Correction Final State Interaction Initial State Nuclear Effect on QE -A -A reaction ~ -N with Nuclear Effect 3 Stages of Nuclear Effect ` Quasi-elastic  Fermi gas, spectral function Pauli blocking, optical potential

Quasielastic -A and e-A Comparison Nuclear Effect between -A and e-A –Initial State of Nucleons: Same Fermi gas, Spectral function –Final State Interaction: Same Pauli Blocking, Optical potential,… Information obtained from e-A –Vector Form Factors –Initial State of Nucleons –FSI

Differential Cross Section A(e,e’) cross section p : initial nucleon momentum, q : momentum transfer,  : energy transfer

Form Factors The latest form factors are used. Brash et al., PRC65,051001(2002). Bosted PRC51,409(1995) Axial form factor: dipole

Fermi Gas Model Non-interacting and uniform Fermi Gas Model (Moniz) Initial State : Fermi Gas Final State Interaction: Pauli Blocking Fermi Gas Pauli Blocking

Spectral Function More realistic model than FG Initial State: realistic spectral function (Benhar et al.) (single particle + correlation with local density approx.) P (MeV/c) E (MeV) P h ( p;! )= 1 E p P ( p;! ) Probability of removing a nucleon of momentum p with excitation energy E.

Momentum Distribution Momentum distribution of a nucleon in nucleus. Spectral function has long tail due to correlation.

Pauli Blocking for Spectral function model PWIA (no Pauli blocking) Simple Pauli Blocking ( same as FG) Modified Pauli Blocking Sum rule for uniform Nuclear Matter  ~ 0.4  0

Experimental Data 16 O(e,e’) : E= MeV  =32 deg Anghinolfi et al., NPA602(’96), C(e,e’) : E=780 MeV  =50.4 deg Garino et al., PRC45(’92),780. E=500 MeV  =60 deg Whittney et al., PRC9(’74),2230.

QE  Resonance (e,e’): Fermi Gas vs. Spectral function Data: 16 O(e,e’) E=1080 MeV  =32 deg FG > SF at peak. SF agrees better with data. SF can explain ‘dip region’, because of ‘correlation’.

16 O(e,e’)  =32 deg E=700,880,1080,1200 MeV

12 C(e,e’) quasielastic E=500MeV  =60 deg E=780 MeV  =50.4 deg Red: spectral func Blue: Fermi Gas

16 O(   - ) QE E=800 MeV d  /dQ 2 E=800MeV – Blue:Fermi Gas – Red: Spectral Function+PWIA – Green: Spectral Function + Pauli Blocking Pauli Blocking has large effect at small Q d  /dQ 2 [ fm 2 /MeV 2 ] Q 2 [GeV 2 ] E = 800 MeV SF SF+PB FG

16 O(   - ) QE E=800 MeV d  /dE  E=800MeV – Blue:Fermi Gas – Red: Spectral Function +PWIA – Green: Spectral Function + Pauli Blocking Clear difference at peak (FG > SP). – FG has low-energy-transfer nucleons more than SF d  /dE lep [ fm 2 /MeV] E lep [MeV] E = 800 MeV SF SF+PB FG

16 O(   - ) QE E=2000 MeV d  /dE  d  /dQ d  /dE lep [ fm 2 /MeV] E lep [MeV] E = 2000 MeV SF SF+PB FG d  /dQ 2 [ fm 2 /MeV 2 ] Q 2 [GeV 2 ] E = 2000 MeV SF SF+PB FG

Form Factor: Dipole vs. Latest The latest form factor make smaller cross sections at QE peak than dipole. Difference: < 10% (e,e’) (  )

Pauli Blocking for Spectral function model PWIA (no Pauli blocking) Simple Pauli Blocking ( same as FG) Modified Pauli Blocking Sum rule for uniform NM  ~ 0.4  0

Comparison of Pauli Blocking Simple PB suppresses cross section at small Q 2, more strongly than Modified PB. O(  )

Final State Interaction Simple approach is tried here. Optical Potential Model Imaginary part of potential On-shell condition of recoiled nucleon is changed:  =0.16 fm -3 Nuclear Matter density  NN = 40 mb Typical value of NN cross section

16 O(e,e’)  =32 deg: QE with FSI E=700,1080 MeV Red: Spectral Function Green: Fermi Gas Blue: SF+FSI SP +FSI < SP only SP+FSI: broader width. Difference 10% at peak

Summary Systematic comparison of the model calculation with A(e,e’) data in the wide energy range with the latest form factors. (e,e’): SF agrees better with the experimental data than FG, in particular, at dip region. (,  ): More than 20 % difference between FG and SF shows at d  /dE  peak. Pauli blocking should be verified by forward e-A scattering data. Appropriate FSI is necessary.

N-  Form Factors Paschos et al. PRD69,014013(2004),