Deep Inelastic Scattering of Polarized Electrons by Polarized 3He and The
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Measurements of Elastic Electron-Proton Scattering at Large Momentum Transfer*
SLAC-PUB-4395 Rev. January 1993 m Measurements of Elastic Electron-Proton Scattering at Large Momentum Transfer* A. F. SILL,(~) R. G. ARNOLD,P. E. BOSTED,~. C. CHANG,@) J. GoMEz,(~)A. T. KATRAMATOU,C. J. MARTOFF, G. G. PETRATOS,(~)A. A. RAHBAR,S. E. ROCK,AND Z. M. SZALATA Department of Physics The American University, Washington DC 20016 D.J. SHERDEN Stanford Linear Accelerator Center , Stanford University, Stanford, California 94309 J. M. LAMBERT Department of Physics Georgetown University, Washington DC 20057 and R. M. LOMBARD-NELSEN De’partemente de Physique Nucle’aire CEN Saclay, Gif-sur- Yvette, 91191 Cedex, France Submitted to Physical Review D *Work supported by US Department of Energy contract DE-AC03-76SF00515 (SLAC), and National Science Foundation Grants PHY83-40337 and PHY85-10549 (American University). R. M. Lombard-Nelsen was supported by C. N. R. S. (French National Center for Scientific Research). Javier Gomez was partially supported by CONICIT, Venezuela. (‘)Present address: Department of Physics and Astronomy, University of Rochester, NY 14627. (*)Permanent address: Department of Physics and Astronomy, University of Maryland, College Park, MD 20742. (C)Present address: Continuous Electron Beam Accelerator Facility, Newport News, VA 23606. (d)Present address: Temple University, Philadelphia, PA 19122. (c)Present address: Stanford Linear Accelerator Center, Stanford CA 94309. ABSTRACT Measurements of the forward-angle differential cross section for elastic electron-proton scattering were made in the range of momentum transfer from Q2 = 2.9 to 31.3 (GeV/c)2 using an electron beam at the Stanford Linear Accel- erator Center. The data span six orders of magnitude in cross section. -
Part B. Radiation Sources Radiation Safety
Part B. Radiation sources Radiation Safety 1. Interaction of electrons-e with the matter −31 me = 9.11×10 kg ; E = m ec2 = 0.511 MeV; qe = -e 2. Interaction of photons-γ with the matter mγ = 0 kg ; E γ = 0 eV; q γ = 0 3. Interaction of neutrons-n with the matter −27 mn = 1.68 × 10 kg ; En = 939.57 MeV; qn = 0 4. Interaction of protons-p with the matter −27 mp = 1.67 × 10 kg ; Ep = 938.27 MeV; qp = +e Note: for any nucleus A: mass number – nucleons number A = Z + N Z: atomic number – proton (charge) number N: neutron number 1 / 35 1. Interaction of electrons with the matter Radiation Safety The physical processes: 1. Ionization losses inelastic collisions with orbital electrons 2. Bremsstrahlung losses inelastic collisions with atomic nuclei 3. Rutherford scattering elastic collisions with atomic nuclei Positrons at nearly rest energy: annihilation emission of two 511 keV photons 2 / 35 1. Interaction of electrons with1.E+02 the matter Radiation Safety ) 1.E+03 -1 Graphite – Z = 6 .g 2 1.E+01 ) Lead – Z = 82 -1 .g 2 1.E+02 1.E+00 1.E+01 1.E-01 1.E+00 collision 1.E-02 radiative collision 1.E-01 stopping pow er (MeV.cm total radiative 1.E-03 stopping pow er (MeV.cm total 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 1.E-02 energy (MeV) 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 Electrons – stopping power 1.E+02 energy (MeV) S 1 dE ) === -1 Copper – Z = 29 ρρρ ρρρ dl .g 2 1.E+01 S 1 dE 1 dE === +++ ρρρ ρρρ dl coll ρρρ dl rad 1 dE 1.E+00 : mass stopping power (MeV.cm 2 g. -
Neutron Scattering
Neutron Scattering Basic properties of neutron and electron neutron electron −27 −31 mass mkn =×1.675 10 g mke =×9.109 10 g charge 0 e spin s = ½ s = ½ −e= −e= magnetic dipole moment µnn= gs with gn = 3.826 µee= gs with ge = 2.0 2mn 2me =22k 2π =22k Ek== E = 2m λ 2m energy n e 81.81 150.26 Em[]eV = 2 Ee[]V = 2 λ ⎣⎡Å⎦⎤ λ ⎣⎦⎡⎤Å interaction with matter: Coulomb interaction — 9 strong-force interaction 9 — magnetic dipole-dipole 9 9 interaction Several salient features are apparent from this table: – electrons are charged and experience strong, long-range Coulomb interactions in a solid. They therefore typically only penetrate a few atomic layers into the solid. Electron scattering is therefore a surface-sensitive probe. Neutrons are uncharged and do not experience Coulomb interaction. The strong-force interaction is naturally strong but very short-range, and the magnetic interaction is long-range but weak. Neutrons therefore penetrate deeply into most materials, so that neutron scattering is a bulk probe. – Electrons with wavelengths comparable to interatomic distances (λ ~2Å ) have energies of several tens of electron volts, comparable to energies of plasmons and interband transitions in solids. Electron scattering is therefore well suited as a probe of these high-energy excitations. Neutrons with λ ~2Å have energies of several tens of meV , comparable to the thermal energies kTB at room temperature. These so-called “thermal neutrons” are excellent probes of low-energy excitations such as lattice vibrations and spin waves with energies in the meV range. -
Compton Sources of Electromagnetic Radiation∗
August 25, 2010 13:33 WSPC/INSTRUCTION FILE RAST˙Compton Reviews of Accelerator Science and Technology Vol. 1 (2008) 1–16 c World Scientific Publishing Company COMPTON SOURCES OF ELECTROMAGNETIC RADIATION∗ GEOFFREY KRAFFT Center for Advanced Studies of Accelerators, Jefferson Laboratory, 12050 Jefferson Ave. Newport News, Virginia 23606, United States of America kraff[email protected] GERD PRIEBE Division Leader High Field Laboratory, Max-Born-Institute, Max-Born-Straße 2 A Berlin, 12489, Germany [email protected] When a relativistic electron beam interacts with a high-field laser beam, the beam electrons can radiate intense and highly collimated electromagnetic radiation through Compton scattering. Through relativistic upshifting and the relativistic Doppler effect, highly energetic polarized photons are radiated along the electron beam motion when the electrons interact with the laser light. For example, X-ray radiation can be obtained when optical lasers are scattered from electrons of tens of MeV beam energy. Because of the desirable properties of the radiation produced, many groups around the world have been designing, building, and utilizing Compton sources for a wide variety of purposes. In this review paper, we discuss the generation and properties of the scattered radiation, the types of Compton source devices that have been constructed to present, and the future prospects of radiation sources of this general type. Due to the possibilities to produce hard electromagnetic radiation in a device small compared to the alternative storage ring sources, it is foreseen that large numbers of such sources may be constructed in the future. Keywords: Compton backscattering, Inverse Compton source, Thomson scattering, X-rays, Spectral brilliance 1. -
Some Polarized Target Experiments for Elementary Particle Physics
SOME POLARIZED TARGET EXPERIMENTS FOR ELEMENTARY PARTICLE PHYSICS R.H. DALITZ Department of Theoretical Physics, Oxford INTRODUCTION At the present stage in elementary particle physics, there are three major areas of phenomena where the use of polarized targets may lead to especially illuminating information. a. High energy scattering, in the energy range where the dominant contributions to the processes observed may arise from Reggion ex change. The features of particular interest in these situjtions will be discussed at this meeting by Dr R.J.N. Phillips 1 • b. Tests of time-reversal (T) invariance for electrom~gnetic pro cesses, following the suggestion by Bernstein et al 2) that the CF-violation observed in the weak decay of kaons arises from the existence of an electromagnetic interaction which strongly viola tes T-invariance. Evidence for this hypothetical T-violating elec tromagnetic interaction can be sought most directly in the study of electromagnetic processes from a polarized proton target, for example in the study of the electro-excitation process e + N-+ e + N* , as discussed by Christ and Lee 3J. The experi~ents proposed will be discussed at this meeting by Dr M. Jacob 4J. c. Hadron spectroscopy. Very many resonant states have been obser ved for masonic and baryonic states. These hadronic states are be lieved to correspond to the patterns appropriate to unitary multi plets of states, and these unitary multiplets appear to be grouped in supermultiplet patterns. In our attempt to classify and under stand all these hadronic states, our first need is for the deter mination of the spin and parity for each state. -
The Basic Interactions Between Photons and Charged Particles With
Outline Chapter 6 The Basic Interactions between • Photon interactions Photons and Charged Particles – Photoelectric effect – Compton scattering with Matter – Pair productions Radiation Dosimetry I – Coherent scattering • Charged particle interactions – Stopping power and range Text: H.E Johns and J.R. Cunningham, The – Bremsstrahlung interaction th physics of radiology, 4 ed. – Bragg peak http://www.utoledo.edu/med/depts/radther Photon interactions Photoelectric effect • Collision between a photon and an • With energy deposition atom results in ejection of a bound – Photoelectric effect electron – Compton scattering • The photon disappears and is replaced by an electron ejected from the atom • No energy deposition in classical Thomson treatment with kinetic energy KE = hν − Eb – Pair production (above the threshold of 1.02 MeV) • Highest probability if the photon – Photo-nuclear interactions for higher energies energy is just above the binding energy (above 10 MeV) of the electron (absorption edge) • Additional energy may be deposited • Without energy deposition locally by Auger electrons and/or – Coherent scattering Photoelectric mass attenuation coefficients fluorescence photons of lead and soft tissue as a function of photon energy. K and L-absorption edges are shown for lead Thomson scattering Photoelectric effect (classical treatment) • Electron tends to be ejected • Elastic scattering of photon (EM wave) on free electron o at 90 for low energy • Electron is accelerated by EM wave and radiates a wave photons, and approaching • No -
A Peek Into Spin Physics
A Peek into Spin Physics Dustin Keller University of Virginia Colloquium at Kent State Physics Outline ● What is Spin Physics ● How Do we Use It ● An Example Physics ● Instrumentation What is Spin Physics The Physics of exploiting spin - Spin in nuclear reactions - Nucleon helicity structure - 3D Structure of nucleons - Fundamental symmetries - Spin probes in beyond SM - Polarized Beams and Targets,... What is Spin Physics What is Spin Physics ● The Physics of exploiting spin : By using Polarized Observables Spin: The intrinsic form of angular momentum carried by elementary particles, composite particles, and atomic nuclei. The Spin quantum number is one of two types of angular momentum in quantum mechanics, the other being orbital angular momentum. What is Spin Physics What Quantum Numbers? What is Spin Physics What Quantum Numbers? Internal or intrinsic quantum properties of particles, which can be used to uniquely characterize What is Spin Physics What Quantum Numbers? Internal or intrinsic quantum properties of particles, which can be used to uniquely characterize These numbers describe values of conserved quantities in the dynamics of a quantum system What is Spin Physics But a particle is not a sphere and spin is solely a quantum-mechanical phenomena What is Spin Physics Stern-Gerlach: If spin had continuous values like the classical picture we would see it What is Spin Physics Stern-Gerlach: Instead we see spin has only two values in the field with opposite directions: or spin-up and spin-down What is Spin Physics W. Pauli (1925) -
Particles and Deep Inelastic Scattering
Heidi Schellman Northwestern Particles and Deep Inelastic Scattering Heidi Schellman Northwestern University HUGS - JLab - June 2010 June 2010 HUGS 1 Heidi Schellman Northwestern k’ k q P P’ A generic scatter of a lepton off of some target. kµ and k0µ are the 4-momenta of the lepton and P µ and P 0µ indicate the target and the final state of the target, which may consist of many particles. qµ = kµ − k0µ is the 4-momentum transfer to the target. June 2010 HUGS 2 Heidi Schellman Northwestern Lorentz invariants k’ k q P P’ 2 2 02 2 2 2 02 2 2 2 The 5 invariant masses k = m` , k = m`0, P = M , P ≡ W , q ≡ −Q are invariants. In addition you can define 3 Mandelstam variables: s = (k + P )2, t = (k − k0)2 and u = (P − k0)2. 2 2 2 2 s + t + u = m` + M + m`0 + W . There are also handy variables ν = (p · q)=M , x = Q2=2Mµ and y = (p · q)=(p · k). June 2010 HUGS 3 Heidi Schellman Northwestern In the lab frame k’ k θ q M P’ The beam k is going in the z direction. Confine the scatter to the x − z plane. µ k = (Ek; 0; 0; k) P µ = (M; 0; 0; 0) 0µ 0 0 0 k = (Ek; k sin θ; 0; k cos θ) qµ = kµ − k0µ June 2010 HUGS 4 Heidi Schellman Northwestern In the lab frame k’ k θ q M P’ 2 2 2 s = ECM = 2EkM + M − m ! 2EkM 2 0 0 2 02 0 t = −Q = −2EkEk + 2kk cos θ + mk + mk ! −2kk (1 − cos θ) 0 ν = (p · q)=M = Ek − Ek energy transfer to target 0 y = (p · q)=(p · k) = (Ek − Ek)=Ek the inelasticity P 02 = W 2 = 2Mν + M 2 − Q2 invariant mass of P 0µ June 2010 HUGS 5 Heidi Schellman Northwestern In the CM frame k’ k q P P’ The beam k is going in the z direction. -
Polarized Target for the Measurement of the Gluon Contribution to the Nucleon Spin in the COMPASS Experiment
Polarized target for the measurement of the gluon contribution to the nucleon spin in the COMPASS experiment Nagoya University Thesis for the degree Doctor of Philosophy in Physics by Naoki TAKABAYASHI 1 2002 1 Supported by Research Fellowships of the Japan Society for the Promotion of Science for Young Scientists. CONTENTS 1. Introduction : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : 1 2. Spin structure of the nucleon : : : : : : : : : : : : : : : : : : : : : 5 2.1 Deep inelastic scattering . 5 2.2 Cross section and structure functions in unpolarized DIS . 7 2.3 Cross section and structure functions in polarized DIS . 9 2.4 Structure functions and spin puzzle in Parton Model picture . 13 2.4.1 Parton distribution . 14 2.4.2 Spin puzzle in Parton Model picture . 16 2.5 Structure functions and spin puzzle in QCD evolved Parton Model . 18 2.5.1 Unpolarized structure functions . 18 2.5.2 Factorization schemes . 20 2.5.3 DGLAP equation and Scaling violation . 22 2.5.4 Spin-dependent structure functions and polarized DGLAP equation . 23 2.6 Interpretation of small ∆Σ. Is gluon contribution large? . 24 2.6.1 Sum rules . 25 2.6.2 Axial anomaly . 26 3. COMPASS experiment : : : : : : : : : : : : : : : : : : : : : : : : : 30 3.1 Open charm lepto-production via photon-gluon fusion . 30 3.2 Expectations . 35 3.2.1 Luminosity . 35 3.2.2 Reconstruction of the open charm events . 35 3.2.3 Statistical accuracy . 37 3.3 Comparison with the other experiments on ∆g . 40 3.3.1 High pT hadron pairs . 40 3.3.2 pp¯ collision . 41 3.3.3 Comparison of the expected precisions and the kine- matic ranges . -
Hadron Spin Dynamics∗
SLAC-PUB-9107 January 2002 Hadron Spin Dynamics¤ Stanley J. Brodsky Stanford Linear Accelerator Center, Stanford University Stanford, California 94309 e-mail: [email protected] Abstract Spin effects in exclusive and inclusive reactions provide an essential new dimension for testing QCD and unraveling hadron structure. Remarkable new experiments from SLAC, HERMES (DESY), and Jefferson Lab present many challenges to theory, including measurements at HERMES and SMC of the sin- gle spin asymmetries in ep ! e0¼X where the proton is polarized normal to the scattering plane. This type of single spin asymmetry may be due to the effects of rescattering of the outgoing quark on the spectators of the target proton, an effect usually neglected in conventional QCD analyses. Many aspects of spin, such as single-spin asymmetries and baryon magnetic moments are sensitive to the dynamics of hadrons at the amplitude level, rather than probability dis- tributions. I will illustrate the novel features of spin dynamics for relativistic systems by examining the explicit form of the light-front wavefunctions for the two-particle Fock state of the electron in QED, thus connecting the Schwinger anomalous magnetic moment to the spin and orbital momentum carried by its Fock state constituents and providing a transparent basis for understand- ing the structure of relativistic composite systems and their matrix elements in hadronic physics. I also present a survey of outstanding spin puzzles in QCD, particularly ANN in elastic pp scattering, the J=Ã ! ½¼ puzzle, and J=Ã polarization at the Tevatron. Concluding Theory Talk, presented at the 3rd Circum-Pan-Pacific Symposium On High Energy Spin Physics (SPIN 2001) Beijing, China 8–13 October 2001 ¤Work supported by the Department of Energy, contract DE–AC03–76SF00515. -
Solid Polarized Targets for Nuclear and Particle Physics Experiments
P1: NBL October 6, 1997 15:46 Annual Reviews AR043-03 Annu. Rev. Nucl. Part. Sci. 1997. 47:67–109 Copyright c 1997 by Annual Reviews Inc. All rights reserved ! SOLID POLARIZED TARGETS FOR NUCLEAR AND PARTICLE PHYSICS EXPERIMENTS D. G. Crabb Physics Department, University of Virginia, Charlottesville, Virginia 22901 W. Meyer Institut fur¨ Experimentalphysik I, Ruhr-Universitat¨ Bochum, Bochum, Germany KEY WORDS: dynamic polarization, nucleon spin structure, lepton scattering, cryogenics, asymmetry ABSTRACT The development, in the early 1960s, of the dynamic nuclear polarization process in solid diamagnetic materials, doped with paramagnetic radicals, led to the use of solid polarized targets in numerous nuclear and particle physics experiments. Since then steady progress has been made in all contributing subsystems so that proton polarizations near 100% and deuteron polarizations higher than 50% have been achieved in various materials. More radiation-resistant materials, such as ammonia, have made it possible to perform experiments with high beam intensi- ties and experiments that benefit from 4He cooling at 1K and high magnetic fields. The development of dilution refrigerators have allowed frozen spin operation so that experiments with large angular acceptance for the scattered particles have by University of Virginia Libraries on 05/18/07. For personal use only. become routine. Many experiments have taken advantage of these developments and many more are being planned, especially with electromagnetic probes. Annu. Rev. Nucl. Part. Sci. 1997.47:67-109. Downloaded from arjournals.annualreviews.org CONTENTS 1. INTRODUCTION . 68 2. POLARIZATION MECHANISMS . 71 2.1 Thermal Equilibrium Polarization . 72 2.2 Solid-State Effect . 72 2.3 Equal Spin Temperature Theory . -
DEUTERON POLARIZED TARGET for Nd EXPERIMENTS at THE
DEUTERON FROZEN SPIN POLARIZED TARGET FOR nd EXPERIMENTS AT THE VdG ACCELERATOR OF CHARLES UNIVERSITY N.S. Borisov1, N.A. Bazhanov1, A.A. Belyaev4, J. Brož2, J. Černý2, Z. Doležal2, A.N. Fedorov1, G.M. Gurevich3, M.P. Ivanov1, P. Kodyš2, P. Kubík2, E.S. Kuzmin1, A.B. Lazarev1, F. Lehar5,6 , O.O. Lukhanin4, V.N. Matafonov†1, A.B. Neganov1, I.L. Pisarev1, J. Švejda2, S.N. Shilov1, Yu.A. Usov1 and I.Wilhelm2 1Joint Institute for Nuclear Research, Dubna, Russia; 2Institute of Particle and Nuclear Physics, Faculty of Mathematics and Physics, Charles University in Prague; V Holešovičkách 2, CZ18000 Prague 8, Czech Republic; 3Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia; 4NSC KIPT, Kharkov, 5SPP DAPNIA CEA Saclay, F-91190 Gif sur Yvette, France 6IEAP CTU, Horska 3a/22 CZ 12800 Prague 2, Czech Republic Abstract. A frozen spin polarized deuteron target cooled by the 3He/4He dilution refrigerator is described. Fully deuterated 1,2-propanediol was used as a target material. Deuteron vector polarization about 40% was obtained for the target in the shape of a cylinder of 2 cm diameter and 6 cm length. The target is intended for a study of 3N interactions at the polarized neutron beam generated by the Van de Graaff accelerator at the Charles University in Prague. 1. Introduction The Charles University proton polarized target (PPT) [1] has been used previously to measure spin–dependent total cross section differences ∆σT and ∆σL in neutron-proton scattering at the 16.2 MeV polarized neutron beam of the VdG accelerator (Fig.1) [2, 3].