Chapter 11 the Force Between Nucleons
Total Page:16
File Type:pdf, Size:1020Kb

Load more
Recommended publications
-
Meson-Exchange Forces and Medium Polarization in Finite Nuclei
—11005 MESON-EXCHANGE FORCES AND MEDIUM POLARIZATION IN FINITE NUCLEI a) 15 10 x/ r\ o 10 O W. Hengeveld MESON-EXCHANGE FORCES AND MEDIUM POLARIZATION IN FINITE NUCLEI Free University Press is an imprint of: VU BoekhandeUUHgeverij b.v. De Boelalaan 1105 1061 HV Amsterdam The Netherlands ISBN 90-8250-140-3 CIP © W. HengevekJ, Amsterdam, 1966. All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, mechanical, photocopying, recording, or otherwise, without the prior written permission of the author. VRIJE UNIVERSITEIT TE AMSTERDAM MESON-EXCHANGE FORCES AND MEDIUM POLARIZATION IN FINITE NUCLEI ACADEMISCH PROEFSCHRIFT ter verkrijging van de graad van doctor in de wiskunde en natuurwetenschappen aan de Vrije Universiteit te Amsterdam, op gezag van de rector magnificus dr. P.J.D. Drenth, hoogleraar in de faculteit der sociale wetenschappen, in het openbaar te verdedigen op donderdag 1 mei 1986 te 15.30 uur in het hoofdgebouw der universiteit. De Boelelaan 1105 door WILLEM HENGEVELD geboren te Woubrugge # Free University Press Amsterdam 1986 Promotor : prof. dr. E. Boeker Copromotor: dr. K. Allaart Referent : dr. W.H. Dickhoff DANKBETUIGING Zonder de volgende personen zou dit proefschrift niet geschreven of gedrukt zijn: Klaas Allaart worstelde de verschillende onleesbare eerste versies door. Zijn bijdrage aan de presentatie was, in alle opzichten, onmisbaar. Wim Dickhoff gaf niet alleen de grote lijn maar ook de details alle aandacht. Zijn onwrikbare geloof in de mogelijkheden van een formele benadering van kernstructuur, heeft de inhoud van dit proefschrift voor een groot deel bepaald. -
Probing Pulse Structure at the Spallation Neutron Source Via Polarimetry Measurements
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Masters Theses Graduate School 5-2017 Probing Pulse Structure at the Spallation Neutron Source via Polarimetry Measurements Connor Miller Gautam University of Tennessee, Knoxville, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_gradthes Part of the Nuclear Commons Recommended Citation Gautam, Connor Miller, "Probing Pulse Structure at the Spallation Neutron Source via Polarimetry Measurements. " Master's Thesis, University of Tennessee, 2017. https://trace.tennessee.edu/utk_gradthes/4741 This Thesis is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Masters Theses by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a thesis written by Connor Miller Gautam entitled "Probing Pulse Structure at the Spallation Neutron Source via Polarimetry Measurements." I have examined the final electronic copy of this thesis for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Master of Science, with a major in Physics. Geoffrey Greene, Major Professor We have read this thesis and recommend its acceptance: Marianne Breinig, Nadia Fomin Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Probing Pulse Structure at the Spallation Neutron Source via Polarimetry Measurements A Thesis Presented for the Master of Science Degree The University of Tennessee, Knoxville Connor Miller Gautam May 2017 c by Connor Miller Gautam, 2017 All Rights Reserved. -
Quantum Statistics: Is There an Effective Fermion Repulsion Or Boson Attraction? W
Quantum statistics: Is there an effective fermion repulsion or boson attraction? W. J. Mullin and G. Blaylock Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003 ͑Received 13 February 2003; accepted 16 May 2003͒ Physicists often claim that there is an effective repulsion between fermions, implied by the Pauli principle, and a corresponding effective attraction between bosons. We examine the origins and validity of such exchange force ideas and the areas where they are highly misleading. We propose that explanations of quantum statistics should avoid the idea of an effective force completely, and replace it with more appropriate physical insights, some of which are suggested here. © 2003 American Association of Physics Teachers. ͓DOI: 10.1119/1.1590658͔ ͒ϭ ͒ Ϫ␣ Ϫ ϩ ͒2 I. INTRODUCTION ͑x1 ,x2 ,t C͕f ͑x1 ,x2 exp͓ ͑x1 vt a Ϫ͑x ϩvtϪa͒2͔Ϫ f ͑x ,x ͒ The Pauli principle states that no two fermions can have 2 2 1 ϫ Ϫ␣ Ϫ ϩ ͒2Ϫ ϩ Ϫ ͒2 the same quantum numbers. The origin of this law is the exp͓ ͑x2 vt a ͑x1 vt a ͔͖, required antisymmetry of the multi-fermion wavefunction. ͑1͒ Most physicists have heard or read a shorthand way of ex- pressing the Pauli principle, which says something analogous where x1 and x2 are the particle coordinates, f (x1 ,x2) ϭ ͓ Ϫ ប͔ to fermions being ‘‘antisocial’’ and bosons ‘‘gregarious.’’ Of- exp imv(x1 x2)/ , C is a time-dependent factor, and the ten this intuitive approach involves the statement that there is packet width parameters ␣ and  are unequal. -
Consistent Treatment of Pion Exchange Force and Meson Versus Quark Dynamics in the N Ucleon-Nucleon Interaction
Aust. J. Phys., 1993, 46, 737-50 Consistent Treatment of Pion Exchange Force and Meson versus Quark Dynamics in the N ucleon-Nucleon Interaction G. Q. Liu A and A. W. Thomas B Department of Physics and Mathematical Physics, University of Adelaide, Adelaide, S.A. 5005, Australia. A E-mail: [email protected]. BE-mail: [email protected]. Abstract To distinguish explicit quark effects from meson exchange in the NN interaction, it is necessary to splice the long-range meson exchange forces and short-distance dynamics due to quarks. However, in most quark model studies the short-range part of the pion exchange is usually treated differently, which makes it difficult to get a uniform picture of the short-range dynamics. We make a comparison between meson exchange and quark-gluon dynamics using the same pion exchange potential based on a quark-pion coupling model. The roles of vector meson exchange and gluon exchange in the NN interaction are compared by calculating NN phase parameters. It is shown that, with this consistent one-pion exchange force, the vector meson exchange gives a better fit to the data. This suggests that non-perturbative mechanisms responsible for meson exchange may need more careful handling to supplement the usual one-gluon exchange mechanism in describing the NN interaction. 1. Introduction The extent to which the constituent quark model can be used to describe the NN interaction is still under debate. This is manifested by the various quark-based models that provide different pictures for the short-range NN force (for recent reviews see MyhreI' and Wroldsen 1988; Shimizu 1989). -
Nuclear Models: Shell Model
LectureLecture 33 NuclearNuclear models:models: ShellShell modelmodel WS2012/13 : ‚Introduction to Nuclear and Particle Physics ‘, Part I 1 NuclearNuclear modelsmodels Nuclear models Models with strong interaction between Models of non-interacting the nucleons nucleons Liquid drop model Fermi gas model ααα-particle model Optical model Shell model … … Nucleons interact with the nearest Nucleons move freely inside the nucleus: neighbors and practically don‘t move: mean free path λ ~ R A nuclear radius mean free path λ << R A nuclear radius 2 III.III. ShellShell modelmodel 3 ShellShell modelmodel Magic numbers: Nuclides with certain proton and/or neutron numbers are found to be exceptionally stable. These so-called magic numbers are 2, 8, 20, 28, 50, 82, 126 — The doubly magic nuclei: — Nuclei with magic proton or neutron number have an unusually large number of stable or long lived nuclides . — A nucleus with a magic neutron (proton) number requires a lot of energy to separate a neutron (proton) from it. — A nucleus with one more neutron (proton) than a magic number is very easy to separate. — The first exitation level is very high : a lot of energy is needed to excite such nuclei — The doubly magic nuclei have a spherical form Nucleons are arranged into complete shells within the atomic nucleus 4 ExcitationExcitation energyenergy forfor magicm nuclei 5 NuclearNuclear potentialpotential The energy spectrum is defined by the nuclear potential solution of Schrödinger equation for a realistic potential The nuclear force is very short-ranged => the form of the potential follows the density distribution of the nucleons within the nucleus: for very light nuclei (A < 7), the nucleon distribution has Gaussian form (corresponding to a harmonic oscillator potential ) for heavier nuclei it can be parameterised by a Fermi distribution. -
Phys 487 Discussion 4 – Symmetrization and the Exchange
Phys 487 Discussion 4 – Symmetrization and the Exchange Force It is considered a postulate (another axiom!) of quantum mechanics that the wavefunction for n identical particles must be either symmetric (S,+) or antisymmetric (A,–) under the exchange of any two particles: ! ! ! ! (r ,r ) (r ,r ) if particle 1 and particle 2 are indistinguishable. ψ 2 1 = ±ψ 1 2 Problem 1 : Fermi, Bose, and Pauli There is one more part to the postulate, which we mentioned at the ver end of last semester. ! ! ! ! • 2-Fermion wavefunctions are Antisymmetric under exchange → ψ (r ,r ) = –ψ (r ,r ) . !2 !1 !1 !2 • 2-Boson wavefunctions are Symmetric under exchange (r ,r ) (r ,r ) . → ψ 2 1 = +ψ 1 2 where • a Fermion is a particle with half-integer spin (e.g. electrons, protons, neutrons) • a Boson is a particle with integer spin (e.g. photons, many nuclei) (a) What if we have a system composed of one of each, e.g. a spin-1 deuterium nucleus (boson) and a spin-½ electron (fermion)? What is the symmetry of that under exchange? (Hint: No calculations required, and you will laugh when you realize the answer.) (b) Show that it is impossible for two fermions to occupy exactly the same state: show that you cannot build a ! ! wavefunction (r ,r ) with the necessary symmetry properties when particle 1 and particle 2 have the exact ψ 1 2 same individual wavefunctions. FYI: This result is the Pauli Exclusion Principle. It is an immediate consequence of the anti-symmetrization requirement on the wavefunctions of indistinguishable fermions, and is essential for understanding the periodic table – i.e. -
5.1 Two-Particle Systems
5.1 Two-Particle Systems We encountered a two-particle system in dealing with the addition of angular momentum. Let's treat such systems in a more formal way. The w.f. for a two-particle system must depend on the spatial coordinates of both particles as @Ψ well as t: Ψ(r1; r2; t), satisfying i~ @t = HΨ, ~2 2 ~2 2 where H = + V (r1; r2; t), −2m1r1 − 2m2r2 and d3r d3r Ψ(r ; r ; t) 2 = 1. 1 2 j 1 2 j R Iff V is independent of time, then we can separate the time and spatial variables, obtaining Ψ(r1; r2; t) = (r1; r2) exp( iEt=~), − where E is the total energy of the system. Let us now make a very fundamental assumption: that each particle occupies a one-particle e.s. [Note that this is often a poor approximation for the true many-body w.f.] The joint e.f. can then be written as the product of two one-particle e.f.'s: (r1; r2) = a(r1) b(r2). Suppose furthermore that the two particles are indistinguishable. Then, the above w.f. is not really adequate since you can't actually tell whether it's particle 1 in state a or particle 2. This indeterminacy is correctly reflected if we replace the above w.f. by (r ; r ) = a(r ) (r ) (r ) a(r ). 1 2 1 b 2 b 1 2 The `plus-or-minus' sign reflects that there are two distinct ways to accomplish this. Thus we are naturally led to consider two kinds of identical particles, which we have come to call `bosons' (+) and `fermions' ( ). -
Interaction of Neutrons with Matter
Interaction of Neutrons With Matter § Neutrons interactions depends on energies: from > 100 MeV to < 1 eV § Neutrons are uncharged particles: Þ No interaction with atomic electrons of material Þ interaction with the nuclei of these atoms § The nuclear force, leading to these interactions, is very short ranged Þ neutrons have to pass close to a nucleus to be able to interact ≈ 10-13 cm (nucleus radius) § Because of small size of the nucleus in relation to the atom, neutrons have low probability of interaction Þ long travelling distances in matter See Krane, Segre’, … While bound neutrons in stable nuclei are stable, FREE neutrons are unstable; they undergo beta decay with a lifetime of just under 15 minutes n ® p + e- +n tn = 885.7 ± 0.8 s ≈ 14.76 min Long life times Þ before decaying possibility to interact Þ n physics … x Free neutrons are produced in nuclear fission and fusion x Dedicated neutron sources like research reactors and spallation sources produce free neutrons for the use in irradiation neutron scattering exp. 33 N.B. Vita media del protone: tp > 1.6*10 anni età dell’universo: (13.72 ± 0,12) × 109 anni. beta decay can only occur with bound protons The neutron lifetime puzzle From 2016 Istitut Laue-Langevin (ILL, Grenoble) Annual Report A. Serebrov et al., Phys. Lett. B 605 (2005) 72 A.T. Yue et al., Phys. Rev. Lett. 111 (2013) 222501 Z. Berezhiani and L. Bento, Phys. Rev. Lett. 96 (2006) 081801 G.L. Greene and P. Geltenbort, Sci. Am. 314 (2016) 36 A discrepancy of more than 8 seconds !!!! https://www.scientificamerican.com/article/neutro -
Pauli's Principle in Probe Microscopy
Chapter 1 Pauli's Principle in Probe Microscopy SP Jarvisy, AM Sweetmany, L Kantorovichz, E McGlynn], and P Moriartyy It appears to be one of the few places in physics where there is a rule which can be stated very simply, but for which no one has found a simple and easy explanation. The explanation is deep down in relativistic quantum mechanics. This probably means that we do not have a complete understanding of the fundamental principle involved.RP Feynman, The Feynman Lectures on Physics, Vol III, Chapter 4 (1964) Abstract Exceptionally clear images of intramolecular structure can be attained in dynamic force microscopy through the combination of a passivated tip apex and operation in what has become known as the \Pauli exclusion regime" of the tip-sample interaction. We discuss, from an experimentalist's perspective, a number of aspects of the exclusion principle which underpin this ability to achieve submolecular resolution. Our particular focus is on the origins, history, and interpretation of Pauli's principle in the context of interatomic and intermolecular interactions. Keywords: dynamic force microscopy;non-contact atomic force microscopy; NC-AFM; Pauli exclusion principle; submolecular resolution; intramolecular; single molecule imaging From Imaging and Manipulation of Adsorbates using Dynamic Force Microscopy, Vol V of Advances in Atom and Single Molecule Machines, Springer-Verlag; http://www.springer.com/ series/10425. To be published late 2014. ySchool of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UK z Department of Physics, Kings College London, The Strand, London WC2R 2LS, UK ] School of Physical Sciences, Dublin City University, Glasnevin, Dublin 9, Ireland arXiv:1408.1026v1 [cond-mat.mes-hall] 5 Aug 2014 1 2 SP Jarvis, AM Sweetman, L Kantorovich, E McGlynn, and P Moriarty 1.1 Intramolecular resolution via Pauli exclusion In 2009 the results of a pioneering dynamic force microscopy (DFM1) experiment by Leo Gross and co-workers at IBM Z¨urich were published[1] and revolutionised the field of scanning probe microscopy. -
14. Structure of Nuclei Particle and Nuclear Physics
14. Structure of Nuclei Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 14. Structure of Nuclei 1 In this section... Magic Numbers The Nuclear Shell Model Excited States Dr. Tina Potter 14. Structure of Nuclei 2 Magic Numbers Magic Numbers = 2; 8; 20; 28; 50; 82; 126... Nuclei with a magic number of Z and/or N are particularly stable, e.g. Binding energy per nucleon is large for magic numbers Doubly magic nuclei are especially stable. Dr. Tina Potter 14. Structure of Nuclei 3 Magic Numbers Other notable behaviour includes Greater abundance of isotopes and isotones for magic numbers e.g. Z = 20 has6 stable isotopes (average=2) Z = 50 has 10 stable isotopes (average=4) Odd A nuclei have small quadrupole moments when magic First excited states for magic nuclei higher than neighbours Large energy release in α, β decay when the daughter nucleus is magic Spontaneous neutron emitters have N = magic + 1 Nuclear radius shows only small change with Z, N at magic numbers. etc... etc... Dr. Tina Potter 14. Structure of Nuclei 4 Magic Numbers Analogy with atomic behaviour as electron shells fill. Atomic case - reminder Electrons move independently in central potential V (r) ∼ 1=r (Coulomb field of nucleus). Shells filled progressively according to Pauli exclusion principle. Chemical properties of an atom defined by valence (unpaired) electrons. Energy levels can be obtained (to first order) by solving Schr¨odinger equation for central potential. 1 E = n = principle quantum number n n2 Shell closure gives noble gas atoms. Are magic nuclei analogous to the noble gas atoms? Dr. -
1663-29-Othernuclearreaction.Pdf
it’s not fission or fusion. It’s not alpha, beta, or gamma dosimeter around his neck to track his exposure to radiation decay, nor any other nuclear reaction normally discussed in in the lab. And when he’s not in the lab, he can keep tabs on his an introductory physics textbook. Yet it is responsible for various experiments simultaneously from his office computer the existence of more than two thirds of the elements on the with not one or two but five widescreen monitors—displaying periodic table and is virtually ubiquitous anywhere nuclear graphs and computer codes without a single pixel of unused reactions are taking place—in nuclear reactors, nuclear bombs, space. Data printouts pinned to the wall on the left side of the stellar cores, and supernova explosions. office and techno-scribble densely covering the whiteboard It’s neutron capture, in which a neutron merges with an on the right side testify to a man on a mission: developing, or atomic nucleus. And at first blush, it may even sound deserving at least contributing to, a detailed understanding of complex of its relative obscurity, since neutrons are electrically neutral. atomic nuclei. For that, he’ll need to collect and tabulate a lot For example, add a neutron to carbon’s most common isotope, of cold, hard data. carbon-12, and you just get carbon-13. It’s slightly heavier than Mosby’s primary experimental apparatus for doing this carbon-12, but in terms of how it looks and behaves, the two is the Detector for Advanced Neutron Capture Experiments are essentially identical. -
Nuclear Physics: the ISOLDE Facility
Nuclear physics: the ISOLDE facility Lecture 1: Nuclear physics Magdalena Kowalska CERN, EP-Dept. [email protected] on behalf of the CERN ISOLDE team www.cern.ch/isolde Outline Aimed at both physics and non-physics students This lecture: Introduction to nuclear physics Key dates and terms Forces inside atomic nuclei Nuclear landscape Nuclear decay General properties of nuclei Nuclear models Open questions in nuclear physics Lecture 2: CERN-ISOLDE facility Elements of a Radioactive Ion Beam Facility Lecture 3: Physics of ISOLDE Examples of experimental setups and results 2 Small quiz 1 What is Hulk’s connection to the topic of these lectures? Replies should be sent to [email protected] Prize: part of ISOLDE facility 3 Nuclear scale Matter Crystal Atom Atomic nucleus Macroscopic Nucleon Quark Angstrom Nuclear physics: femtometer studies the properties of nuclei and the interactions inside and between them 4 and with a matching theoretical effort theoretical a matching with and facilities experimental dedicated many with better and better it know to getting are we but Today Becquerel, discovery of radioactivity Skłodowska-Curie and Curie, isolation of radium : the exact form of the nuclear interaction is still not known, known, not still is interaction of nuclearthe form exact the : Known nuclides Known Chadwick, neutron discovered History 5 Goeppert-Meyer, Jensen, Haxel, Suess, nuclear shell model first studies on short-lived nuclei Discovery of 1-proton decay Discovery of halo nuclei Discovery of 2-proton decay Calculations with