Deep Inelastic Scattering in the Valence Regime

Total Page:16

File Type:pdf, Size:1020Kb

Deep Inelastic Scattering in the Valence Regime Deep Inelastic Scattering in the Valence Regime Thia Keppel ICNFP 2019 Thomas Jefferson National Accelerator Facility Kolympari, Crete, Greece Newport News, VA How to probe the nucleon structure? • Electron scattering experiments employ high momentum point-like leptons, + electromagnetic interactions, which are well understood, to probe hadronic structure (which isn’t). High energy electrons are a great tool for the job! short distance -> large momentum Deep Inelastic Electron Scattering Beginnings: e-p and e-d at SLAC J. Friedman, H.Kendall, R.Taylor Nobel Prize 1990 • Q2 = four-momentum transfer in electron scattering process • First SLAC experiment (‘69): – expected from proton form factor: 2 ds / dE'dW æ 1 ö -8 = ç ÷ µ Q ç 2 2 ÷ (ds / dW)Mott è (1+ Q / 0.71) ø • First data show big surprise: – very weak Q2-dependence – scattering off point-like objects? – quark structure of the proton! Structure Functions in Deep Inelastic Electron-Nucleon Scattering Probability of inelastic interaction: 푑2휎 훼2 휃 1 2 휃 = cos2 퐹 푥, 푄2 + 퐹 푥, 푄2 tan2 ′ 휃 2 1 푑Ω푑퐸 4퐸2 sin4 2 휈 푀 2 0 2 Unpolarized “Structure 2 2 Functions” F1(x,Q ) and F2(x,Q ): - Account for the sub-structure of the protons and neutrons - Give access to partonic structure of the nucleon, i.e. x : Bjorken “scaling” variable (= Q2/2Mn), momentum fraction of struck quark Fast forward…. 50 years of charged lepton Deep Inelastic Scattering at multiple laboratories including SLAC (to ~2000), CERN 80-90s EMC, NMC, BCDMS..), DESY (90s – 21st century H1, ZEUS,...), and more! H1 HERMES HERMES BCDMS 2 Q Evolution of the F2 Proton Structure Function Allows extraction of “Parton Distribution Functions” f(x,Q2) - think momentum distribution of quarks Some 50% things of momentumwe now know carriedreally bywell…. gluons …and some things we don’t. n p F2 /F2 • The neutron structure function is not well known at large x • Large x is the valence regime Some 50% things of momentumwe now know of nucleon structure carriedreally bywell…. gluons Deep Inelastic Scattering in the Valence Regime Thia Keppel ICNFP 2019 Thomas Jefferson National Accelerator Facility Kolympari, Crete, Greece Newport News, VA Why is the valence regime interesting? • Partonic structure in the valence region defines a hadron - Baryon number, charge, flavor content, total spin, … • “Valence regime” at large x, low Q2 evolves to low x, high Q2 - Intersection of nuclear and particle physics • Keen discriminator of nucleon structure models • New generation of experiments at JLab focused on high x 1 0 Neutron Structure Function sea quark dominance F n/F p 1 Parton model: 2 2 u quark dominance, d/u 0 n p F2 /F2 Neutron Structure Function sea quark dominance F n/F p 1 Parton model: 2 2 u quark dominance, d/u 0 n p F2 /F2 The deuteron is a nucleus! Neutron structure is typically derived from deuterium target data by subtracting proton data …..but….. Large uncertainty in unfolding nuclear effects (Fermi motion, off-shell effects, deuteron wave function, coherent scattering, final state interactions, nucleon structure modification (“EMC”-effect),……….. d p F2 /F2 The moon at nuclear density n Deuteron nuclear effects are an obstacle to extracting F2 n p No free neutrons, so F2 /F2 use the deuteron SAME data set Different deuteron nuclear effect analyses n p 0.2 < F2 /F2 < 0.8 ?!?! n p Predictions for F2 /F2 (neutron/proton) ratio at Large x • SU(6)-symmetric wave function of the proton in the quark model: 1 p 3uud uud 2uud 2duu 2duu 18 S 0 S1 S1 S1 S1 – SU(6) spin/flavor symmetry in u,d n p – In this model: d/u = 1/2, F2 /F2 = 2/3 for x -> 1 – But, N and D would be degenerate in mass…. • SU(6) symmetry is broken: N-D Mass Splitting – Mechanism produces mass splitting between S=1 and S=0 diquark spectator. – symmetric states are raised, antisymmetric states are lowered (~300 MeV). n p – S=1 suppressed => d/u = 0, F2 /F2 = 1/4, for x -> 1 n p • pQCD: helicity conservation (qp) => d/u =2/(9+1) = 1/5, F2 /F2 = 3/7 for x -> 1 There are • Dyson-Schwinger Eq.: Contains finite size S=0 and S=1 diquarks n p more! – d/u = 0.28, F2 /F2 = 0.49 for x -> 1 Multiple predictions for large x 1 1 1 p u (ud) u (ud) u (ud) 2 S 0 18 S 1 3 S 1 1 2 d (uu) d (uu) 3 S1 3 S1 n p A Longstanding Problem! Nucleon Model F2 /F2 d/u Numerous Review Articles: SU(6) 2/3 1/2 • N. Isgur, PRD 59 (1999) • S Brodsky et al NP B441 (1995) Valence Quark 1/4 0 • W. Melnitchouk and A. Thomas PL B377 (1996) DSE contact 0.41 0.18 • R.J. Holt and C. D. Roberts, Rev. interaction Mod. Phys. 82 (2010) DSE realistic 0.49 0.28 • I. Cloet et al, Few Body Syst. 46 interaction (2009) 1. pQCD 3/7 1/5 A measurement is needed… 12 n p F2 /F2 (and, hence, d/u) essentially unknown at large x: - Conflicting fundamental theory pictures n - F2 data inconclusive due to uncertainties in deuterium nuclear corrections - Translates directly to large uncertainties on d(x), g(x) parton distribution functions SU(6) symmetry pQCD DSE: 0+ & 1+ qq 0+ qq only 17 Present status: large uncertainties on PDFs at large x 18 Why is the valence regime interesting? • Partonic structure in the valence region defines a hadron - Baryon number, charge, flavor content, total spin, … • “Valence regime” at large x, low Q2 evolves to low x, high Q2 - Intersection of nuclear and particle physics • Keen discriminator of nucleon structure models • New generation of experiments at JLab focused on high x Jefferson Lab Overview • DOE Office of Science Laboratory with a single program focused on Nuclear Physics. o In operation since 1995 • Created to build and operate the Continuous Electron Beam Accelerator Facility (CEBAF), unique user facility for Nuclear Physics. • Mission is to gain a deeper understanding of the structure of Jefferson Lab by the numbers: matter: • 700 employees, 27 Joint faculty o Through advances in • 169 acre site fundamental research in nuclear physics • 1,630 Active Users • 630 PhDs granted to-date (212 in progress) o Through advances in accelerator • K-12 programs serve more than 12,000 and nuclear science and students and 950 teachers annually technology • Scientific users from 39 countries, 278 institutes (124 institutions in 34 states) 20 Jefferson Lab’s user community continues to grow 1800 1600 1400 1200 1000 US University Users International Users 800 Other Users Total Users 600 400 200 0 FY06 FY07 FY08 FY09 FY10 FY11 FY12 FY13 FY14 FY15 FY16 FY17 FY18 21 Diagram representational of below ground structure 22 RECENTLY COMPLETED UPGRADE AT JEFFERSON LAB (as of September 27, 2017) Secures a forefront scientific program for the next 10 or more years 23 TDIS to access nucleon valence structure ”BONuS” Experiment at Jefferson Lab – use fixed target Tagged DIS to create an effective free neutron target Measure DIS electron in coincidence with proton tag n p • “Hard” scattering inelastic event (high Q, W) p Deuteron Target • Proton remains intact • Low momentum proton = nucleons barely off shell Neutron target! The BONuS approach: use low mass radial TPC detector / target in magnetic field to TAG “spectator” proton at (very) low momenta (~65 MeV/c) and large angles (> 90o in lab) ….difficult but doable 2.0 1.4 ps = 0 2 2 A Q = 4 (GeV/c) 1.2 p = 0.1 I Bound / free neutron s W A p = 0.2 I P s 1.5 1.0 / x = 0.6 structure W P ) . S / F I . 0.8 S T F + S O (1%) A 0.6 I 1.0 W P ( p = 0.3 0.4 p = 0.4 p = 0.5 0.2 0.5 0 30 60 90 120 150 180 0 2 0406080 100 120 1.05 q (degrees) q [degr] pq x=0.3 1 0.4 0.95 0.5 x=0.6 n Final state Target fragmentation R 0.9 interactions 0.85 negligible O (5%) 0.8 0 100 200 300 400 |p| (MeV/c) The technique works! angle - momentum dependence W 2 = M 2 + 2Mn - Q2 78 MeV/c 93 MeV/c 110 MeV/c 135 MeV/c cospq cospq BONUS effective neutron target via TDIS achieved! Phys.Rev. C92 (2015) no.1, 015211 Phys.Rev. C91 (2015) no.5, 055206 Phys. Rev. C89 (2014) 045206 – editor’s suggestion Phys. Rev. Lett. 108 (2012) 199902 Nucl. Instrum. Meth. A592 (2008) 273-286 27 > 400 neutron data points! • Lower W, Q2 than desirable…. • Still powerful input for global PDF fits • Provides deuteron nuclear correction EMC effect in deuterium – correction for (nuclear) PDFs D n p n F2 /(F2 + F2 ) with F2 from BONUS S.I. Alekhin, S.A. Kulagin, R. Petti Phys. Rev. D 96, 054005 (2017) “The recent direct measurement of the deuteron nuclear correction by the BONuS experiment substantially reduces this uncertainty by constraining the normalization of the overall nuclear corrections.” 28 E12-06-113 “BONUS12”: Larger x and 2 higher Q CLAS12 Central High Impact Detector Hall B CLAS12 Spectrometer BONUS12 RTPC Adapter Down boards stream end plate Gas circulation slots Ground Foil Up stream Cathod field cage e Gas outlet Down Gas inlets Chamfe stream r field Downstream cage Rings Read Out GEM foil Read Out Connectors cylinders Up stream Pads end plate Up stream rings RTPC UNDER CONSTRUCTION Preparing for 2020 run! Self aligning puller assembly Removal of glued capton cylinder using puller mechanism Tagged Neutron Structure at an Electron Ion Collider The TDIS technique is better suited to colliders: no target material absorbing low-momentum nucleons, forward acceptance only! Need: • good momentum resolution (∆pT ~20 MeV, < Fermi momentum) • small intrinsic momentum spread in the ion beam for accurate reconstruction EIC being designed with this physics in mind e + D → e′ + p + X a la BONUS – neutron structure functions up to Q2 ~ 40 GeV2 JLEIC See Spectator Tagging Project at 32 https://www.jlab.org/theory/tag/ p d F2 & F2 Structure Functions in Hall C p JLab12 Hall C commissioning experiment aims to reduce uncertainties in F2 d and F2 structure functions at large x and high Q Goal @ 12 GeV: <2% total precision cross sections, (as achieved by E00-116 @ 6 GeV) E12-10-002: High Precision Measurement of the F2 Structure Function on p,D • 10.6 GeV beam • Targets: HMS SHMS LH2, LD2, Al Q2 • Fix energy and angle • Scan in momentum • Effective scan in x • Stringent check on spectrometer acceptance x 34 Preliminary Results: Structure Functions (and CJ fit) F d/F p p 2 2 F2 x x d F2 Still working on: • Some background subtractions • Systematic uncertainties • Looking towards F2d/F2p paper submission this Fall 35 Or, a nuclear physicists approach to the problem….
Recommended publications
  • B2.IV Nuclear and Particle Physics
    B2.IV Nuclear and Particle Physics A.J. Barr February 13, 2014 ii Contents 1 Introduction 1 2 Nuclear 3 2.1 Structure of matter and energy scales . 3 2.2 Binding Energy . 4 2.2.1 Semi-empirical mass formula . 4 2.3 Decays and reactions . 8 2.3.1 Alpha Decays . 10 2.3.2 Beta decays . 13 2.4 Nuclear Scattering . 18 2.4.1 Cross sections . 18 2.4.2 Resonances and the Breit-Wigner formula . 19 2.4.3 Nuclear scattering and form factors . 22 2.5 Key points . 24 Appendices 25 2.A Natural units . 25 2.B Tools . 26 2.B.1 Decays and the Fermi Golden Rule . 26 2.B.2 Density of states . 26 2.B.3 Fermi G.R. example . 27 2.B.4 Lifetimes and decays . 27 2.B.5 The flux factor . 28 2.B.6 Luminosity . 28 2.C Shell Model § ............................. 29 2.D Gamma decays § ............................ 29 3 Hadrons 33 3.1 Introduction . 33 3.1.1 Pions . 33 3.1.2 Baryon number conservation . 34 3.1.3 Delta baryons . 35 3.2 Linear Accelerators . 36 iii CONTENTS CONTENTS 3.3 Symmetries . 36 3.3.1 Baryons . 37 3.3.2 Mesons . 37 3.3.3 Quark flow diagrams . 38 3.3.4 Strangeness . 39 3.3.5 Pseudoscalar octet . 40 3.3.6 Baryon octet . 40 3.4 Colour . 41 3.5 Heavier quarks . 43 3.6 Charmonium . 45 3.7 Hadron decays . 47 Appendices 48 3.A Isospin § ................................ 49 3.B Discovery of the Omega § ......................
    [Show full text]
  • Particle Production at Small-X in Deep Inelastic Scattering Dajing Wu Iowa State University
    Iowa State University Capstones, Theses and Graduate Theses and Dissertations Dissertations 2014 Particle production at small-x in deep inelastic scattering Dajing Wu Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/etd Part of the Physics Commons Recommended Citation Wu, Dajing, "Particle production at small-x in deep inelastic scattering" (2014). Graduate Theses and Dissertations. 13846. https://lib.dr.iastate.edu/etd/13846 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Graduate Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. Particle production at small-x in deep inelastic scattering by Dajing Wu A dissertation submitted to the graduate faculty in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Major: Nuclear Physics Program of Study Committee: Kirill Tuchin, Major Professor James Vary Marzia Rosati Kerry Whisnant Alexander Roitershtein Iowa State University Ames, Iowa 2014 Copyright © Dajing Wu, 2014. All rights reserved. ii DEDICATION I would like to dedicate this thesis to my father, Xianggui Wu, and my mother, Wenfang Tang. Without their encouragement and support, I could not have completed such work. iii TABLE OF CONTENTS LIST OF FIGURES . vi ABSTRACT . x ACKNOWLEGEMENT . xi PART I Theoretical foundations for small-x physics1 CHAPTER 1. QCD as a theory for strong interactions . 2 1.1 QCD Lagrangian . .2 1.2 Perturbative QCD . .2 1.3 Light-cone perturbation theory .
    [Show full text]
  • Physics 301 1-Nov-2004 17-1 Reading Finish K&K Chapter 7 And
    Physics 301 1-Nov-2004 17-1 Reading Finish K&K chapter 7 and start on chapter 8. Also, I’m passing out several Physics Today articles. The first is by Graham P. Collins, August, 1995, vol. 48, no. 8, p. 17, “Gaseous Bose-Einstein Condensate Finally Observed.” This describes the research leading up the first observation of a BE condensate that’s not a superfluid or superconductor. The second is by Barbara Goss Levi, March, 1997, vol. 50, no. 3, p. 17, “Bose Condensates are Coherent Inside and Outside an Atom Trap,” describing the first “atom laser” which was based on a BE condensate. The third is also by Levi, October, 1998, vol. 51, no. 10, p. 17, “At Long Last, a Bose-Einstein Condensate is Formed in Hydrogen,” describing even more progress on BE condensates. In addition, there is a recent Science report on an atomic Fermi Gas, DeMarco, B., and Jin, D. S., September 10, 1999, vol. 285, p. 1703, “Onset of Fermi Degeneracy in a Trapped Atomic Gas.” Bose condensates and Fermi degeneracy are current hot topics in Condensed Matter Research. Searching the preprint server or “Googling” with appropriate keywords is bound to turn up many more articles. More on Fermi Gases So far, we’ve considered the zero temperature Fermi gas and done an approximate treatment of the low temperature heat capacity of Fermi gases. The zero temperature Fermi gas was straightforward. We simply said that all states, starting from the lowest energy state, are filled until we run out of particles. The energy at which this happens is called the Fermi energy and is the same as the chemical potential at 0 temperature, ǫF = µ(τ = 0).
    [Show full text]
  • Superfast Quarks, Short Range Correlations and QCD at High Density John Arrington Argonne National Laboratory
    Superfast Quarks, Short Range Correlations and QCD at High Density John Arrington Argonne National Laboratory A(e,e’) at PDFs at x>1 High Energy Superfast quarks PN12, The Physics of Nuclei with 12 GeV Electrons Workshop, Nov. 1, 2004 Superfast Quarks, Short Range Correlations and QCD at High Density John Arrington Argonne National Laboratory Nuclear structure SRCs Nuclear PDFs A(e,e’) at PDFs at x>1 EMC effect High Energy Superfast quarks QCD Phase Transition Cold, dense nuclear matter PN12, The Physics of Nuclei with 12 GeV Electrons Workshop, Nov. 1, 2004 Short Range Correlations (SRCs) Mean field contributions: k < kF Well understood High momentum tails: k > kF Calculable for few-body nuclei, nuclear matter. Dominated by two-nucleon short range correlations. Calculation of proton momentum distribution in 4He Wiringa, PRC 43 k > 250 MeV/c 1585 (1991) 15% of nucleons 60% of the K.E. k < 250 MeV/c 85% of nucleons 40% of the K.E. Isolate short range interaction (and SRCs) by probing at high Pm (x>1) V(r) N-N potential Poorly understood part of nuclear structure Significant fraction of nucleons have k > kF 0 Uncertainty in short-range interaction leads to uncertainty at large momenta (>400-600 MeV/c), even for the Deuteron r [fm] ~1 fm A(e,e’): Short range correlations 56Fe(e,e/ )X We want to be able to isolate and probe -1 10 /A 2 Fe two-nucleon and multi-nucleon SRCs F -2 F2 /A 10 x=1 x = 1 -3 10 -4 Dotted =mean field approx.
    [Show full text]
  • Phenomenological Review on Quark–Gluon Plasma: Concepts Vs
    Review Phenomenological Review on Quark–Gluon Plasma: Concepts vs. Observations Roman Pasechnik 1,* and Michal Šumbera 2 1 Department of Astronomy and Theoretical Physics, Lund University, SE-223 62 Lund, Sweden 2 Nuclear Physics Institute ASCR 250 68 Rez/Prague,ˇ Czech Republic; [email protected] * Correspondence: [email protected] Abstract: In this review, we present an up-to-date phenomenological summary of research developments in the physics of the Quark–Gluon Plasma (QGP). A short historical perspective and theoretical motivation for this rapidly developing field of contemporary particle physics is provided. In addition, we introduce and discuss the role of the quantum chromodynamics (QCD) ground state, non-perturbative and lattice QCD results on the QGP properties, as well as the transport models used to make a connection between theory and experiment. The experimental part presents the selected results on bulk observables, hard and penetrating probes obtained in the ultra-relativistic heavy-ion experiments carried out at the Brookhaven National Laboratory Relativistic Heavy Ion Collider (BNL RHIC) and CERN Super Proton Synchrotron (SPS) and Large Hadron Collider (LHC) accelerators. We also give a brief overview of new developments related to the ongoing searches of the QCD critical point and to the collectivity in small (p + p and p + A) systems. Keywords: extreme states of matter; heavy ion collisions; QCD critical point; quark–gluon plasma; saturation phenomena; QCD vacuum PACS: 25.75.-q, 12.38.Mh, 25.75.Nq, 21.65.Qr 1. Introduction Quark–gluon plasma (QGP) is a new state of nuclear matter existing at extremely high temperatures and densities when composite states called hadrons (protons, neutrons, pions, etc.) lose their identity and dissolve into a soup of their constituents—quarks and gluons.
    [Show full text]
  • Deep-Inelastic Scattering on the Tri-Nucleons
    Three-body dynamics in hadron structure & hadronic systems: A symposium in celebration of Iraj Afnan’s 70th birthday Jefferson Lab, July 24, 2009 Deep-inelastic scattering on the tri-nucleons Wally Melnitchouk Outline Motivation: neutron structure at large x d/u ratio, duality in the neutron Status of large-x quark distributions nuclear corrections new global analysis of inclusive DIS data (CTEQx) DIS from A=3 nuclei model-independent extraction of neutron F2 plans for helium-3/tritium experiments Quark distributions at large x Parton distributions functions (PDFs) provide basic information on structure of hadronic systems needed to understand backgrounds in searches for new physics beyond the Standard Model in high-energy colliders, neutrino oscillation experiments, ... DGLAP evolution feeds low x, high Q2 from high x, low Q 2 1 dq(x, t) αs(t) dy x x = Pqq q(y, t)+Pqg g(y, t) dt 2π x y y y ! " # $ # $ % 2 2 t = log Q /ΛQCD Ratio of d to u quark distributions at large x particularly sensitiveHigher to twistsquark dynamics in nucleon SU(6) spin-flavor symmetry (a) (b) (c) proton wave function ↑ 1 ↑ √2 ↓ p = d (uu)1 d (uu)1 −3 − 3 Higher twists √2 ↑ 1 ↓ 1 ↑ + u (ud)1 u (ud)1 + u (ud)0 τ = 2 6 τ >− 23 √2 (τ = 2) (a) (b) (c) diquark spin single quark interactingqq and qg corquarkrelationsspectator scattering diquark τ = 2 τ > 2 single quark qq and qg scattering correlations Ratio of d to u quark distributions at large x particularly sensitive to quark dynamics in nucleon SU(6) spin-flavor symmetry proton wave function ↑ 1 ↑ √2 ↓ p = d (uu)1 d (uu)1 −3 − 3 √2 ↑ 1 ↓ 1 ↑ + u (ud)1 u (ud)1 + u (ud)0 6 − 3 √2 u(x)=2d(x) for all x n F2 2 p = F2 3 scalar diquark dominance M∆ >MN =⇒ (qq)1 has larger energy than (qq)0 .
    [Show full text]
  • Density and Moisture Content Measurements by Nuclear Methods Interim Report
    NATIONAL COOPERATIVE HIGHWAY RESEARCH PROGRAM REPORT 14. DENSITY AND MOISTURE CONTENT MEASUREMENTS BY NUCLEAR METHODS INTERIM REPORT HIGHWAY RESEARCH BOARD NATIONAL ACADEMY OF SCIENCES - NATIONAL RESEARCH COUNCIL HIGHWAY RESEARCH BOARD 1965 Officers DONALD S. BERRY, Chairman J. B. McMORRAN, First Vice Chairman EDWARD G. WETZEL, Second Vice Chairman GRANT MICKLE, Executive Director W. N. CAREY, JR., Deputy Executive Director Executive Committee REX M. WHrrrON, Federal Highway Administrator, Bureau of Public Roads (ex officio) A. E. JOHNSON, Executive Secretary, American Association of State Highway Officials (ex officio) LOUIS JORDAN, Executive Secretary, Division of Engineering and Industrial Research, National Research Council (ex officio) C. D. CURTISS, Special Assistant to the Executive Vice President, American Road Builders' Association (ex officio, Past Chairman 1963) WILBUR S. SMITH, Wilbur Smith and Associates (ex officio, Past Chairman 1964) W. BAUMAN, Managing Director, National Slag Association DONALD S. BERRY, Chairman, Department of Civil Engineering, Northwestern University MASON A. BUTCHER, County Manager, Montgomery County, Md. J. DOUGLAS CARROLL, JR., Executive Director, Tn-State Transportation Committee, New York City HARMER E. DAVIS, Director, Institute of Transportation and Traffic Engineering, University of California DUKE W. DUNBAR, Attorney General of Colorado JOHN T. HOWARD, Head, Department of City and Regional Planning, Massachusetts Institute of Technology PYKE JOHNSON, Retired LOUIS C. LUNDSTROM, Director, General Motors Proving Grounds BURTON W. MARSH, Executive Director, Foundation for Traffic Safety, American Automobile Association OSCAR T. MARZKE, Vice President, Fundamental Research, U. S. Steel Corporation J. B. McMORRAN, Superintendent of Public Works, New York State Department of Public Works CLIFFORD F. RASSWEILER, Retired M. L. SHADBUTRN, State Highway Engineer, Georgia State Highway Department T.
    [Show full text]
  • Arxiv:1112.0335V1 [Astro-Ph.HE] 1 Dec 2011 Ini Nitnesuc Fnurnso L Aos It flavors
    Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy L.F. Roberts,1 G. Shen,2 V. Cirigliano,2 J.A. Pons,3 S. Reddy,2, 4 and S.E. Woosley1 1Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 USA 2Theoretical Division, Los Alamos National Laboratory, Los Alamos, NM 87544 3Departament de F´ısica Aplicada, Universitat d’Alacant, Ap. Correus 99, 03080 Alacant, Spain 4Institute for Nuclear Theory, University of Washington, Seattle, Washington 98195 We model neutrino emission from a newly born neutron star subsequent to a supernova explosion to study its sensitivity to the equation of state, neutrino opacities, and convective instabilities at high baryon density. We find the time period and spatial extent over which convection operates is sensitive to the behavior of the nuclear symmetry energy at and above nuclear density. When convection ends within the proto-neutron star, there is a break in the predicted neutrino emission that may be clearly observable. PACS numbers: 26.50.+x, 26.60.-c, 21.65.Mn, 95.85.Ry The hot and dense proto-neutron star (PNS) born sub- formation. It has long been recognized that the outer sequent to core-collapse in a type II supernova explo- PNS mantle is unstable to convection soon after the pas- sion is an intense source of neutrinos of all flavors. It sage of the supernova shock, due to negative entropy gra- emits the 3 − 5 × 1053 ergs of gravitational binding en- dients [10]. This early period of instability beneath the ergy gained during collapse as neutrino radiation on a neutrino spheres has been studied extensively in both one time scale of tens of seconds as it contracts, becomes and two dimensions, with the hope that it could increase increasingly neutron-rich and cools.
    [Show full text]
  • Nuclear Physics and Astrophysics SPA5302, 2019 Chris Clarkson, School of Physics & Astronomy [email protected]
    Nuclear Physics and Astrophysics SPA5302, 2019 Chris Clarkson, School of Physics & Astronomy [email protected] These notes are evolving, so please let me know of any typos, factual errors etc. They will be updated weekly on QM+ (and may include updates to early parts we have already covered). Note that material in purple ‘Digression’ boxes is not examinable. Updated 16:29, on 05/12/2019. Contents 1 Basic Nuclear Properties4 1.1 Length Scales, Units and Dimensions............................7 2 Nuclear Properties and Models8 2.1 Nuclear Radius and Distribution of Nucleons.......................8 2.1.1 Scattering Cross Section............................... 12 2.1.2 Matter Distribution................................. 18 2.2 Nuclear Binding Energy................................... 20 2.3 The Nuclear Force....................................... 24 2.4 The Liquid Drop Model and the Semi-Empirical Mass Formula............ 26 2.5 The Shell Model........................................ 33 2.5.1 Nuclei Configurations................................ 44 3 Radioactive Decay and Nuclear Instability 48 3.1 Radioactive Decay...................................... 49 CONTENTS CONTENTS 3.2 a Decay............................................. 56 3.2.1 Decay Mechanism and a calculation of t1/2(Q) .................. 58 3.3 b-Decay............................................. 62 3.3.1 The Valley of Stability................................ 64 3.3.2 Neutrinos, Leptons and Weak Force........................ 68 3.4 g-Decay...........................................
    [Show full text]
  • Chapter 10 Nuclear Properties
    Chapter 10 Nuclear Properties Note to students and other readers: This Chapter is intended to supplement Chapter 3 of Krane’s excellent book, ”Introductory Nuclear Physics”. Kindly read the relevant sections in Krane’s book first. This reading is supplementary to that, and the subsection ordering will mirror that of Krane’s, at least until further notice. A nucleus, discovered by Ernest Rutherford in 1911, is made up of nucleons, a collective name encompassing both neutrons (n) and protons (p). Name symbol mass (MeV/c2 charge lifetime magnetic moment neutron n 939.565378(21) 0 e 881.5(15) s -1.91304272(45) µN proton p 938.272046(21) 1 e stable 2.792847356(23) µN The neutron was theorized by Rutherford in 1920, and discovered by James Chadwick in 1932, while the proton was theorized by William Prout in 1815, and was discovered by Rutherford between 1917 and 1919m and named by him, in 1920. Neutrons and protons are subject to all the four forces in nature, (strong, electromagnetic, weak, and gravity), but the strong force that binds nucleons is an intermediate-range force that extends for a range of about the nucleon diameter (about 1 fm) and then dies off very quickly, in the form of a decaying exponential. The force that keeps the nucleons in a nucleus from collapsing, is a short-range repulsive force that begins to get very large and repulsive 1 for separations less than a nucleon radius, about 2 fm. See Fig. 10.1 (yet to be created). 1 2 CHAPTER 10. NUCLEAR PROPERTIES The total nucleon−nucleon force 10 5 (r) (arbitrary units) 0 nn,att −5 (r) + V −10 nn,rep V 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 r (fm) Figure 10.1: A sketch of the nucleon-nucleon potential.
    [Show full text]
  • Systematics of Nucleon Density Distributions and Neutron Skin of Nuclei
    Systematics of nucleon density distributions and neutron skin of nuclei W. M. Seif and Hesham Mansour Physics Department, Faculty of Science, Cairo University, Egypt Abstract Proton and neutron density profiles of 760 nuclei in the mass region of are analyzed using the Skyrme energy density for the parameter set SLy4. Simple formulae are obtained to fit the resulting radii and diffuseness data. These formulae are useful to estimate the values of the unmeasured radii, and especially in extrapolating charge radii values for nuclei which are far from the valley of stability or to perform analytic calculations for bound and/or scattering problems. The obtained neutron and proton root-mean-square radii and the neutron skin thicknesses are in agreement with the available experimental data and previous Hartree-Fock calculations. I. Introduction To get accurate information on the density distributions of finite nuclei is of high priority in nuclear physics. Basically, to describe perfectly finite nuclei we have to start with full information regarding the root-mean-square (rms) radii of their proton and neutron density distributions, their surface diffuseness, and their neutron skin thickness. Unlike the available experimental data on the charged proton distributions, the available data for the neutral neutron distributions and their rms radii inside nuclei, as well as the neutron skin thickness are not enough yet. Previous extensive studies are aimed to investigate the correlation between the differences in the proton and neutron radii in finite nuclear systems and the nuclear symmetry energy [1, 2, 3, and 4] and neutron skin thickness. Most works are restricted to spherical nuclei.
    [Show full text]
  • Formation of Hot Heavy Nuclei in Supernova Explosions
    Physics Letters B 584 (2004) 233–240 www.elsevier.com/locate/physletb Formation of hot heavy nuclei in supernova explosions A.S. Botvina a,b, I.N. Mishustin c,d,e a Cyclotron Institute, Texas A&M University, College Station, TX 77843, USA b Institute for Nuclear Research, 117312 Moscow, Russia c Institut für Theoretische Physik, Goethe Universität, D-60054 Frankfurt am Main, Germany d Niels Bohr Institute, DK-2100 Copenhagen, Denmark e Kurchatov Institute, RRC, 123182 Moscow, Russia Received 30 December 2003; accepted 23 January 2004 Editor: P.V. Landshoff Abstract We point out that during the supernova II type explosion the thermodynamical conditions of stellar matter between the protoneutron star and the shock front correspond to the nuclear liquid–gas coexistence region, which can be investigated in nuclear multifragmentation reactions. We have demonstrated, that neutron-rich hot heavy nuclei can be produced in this region. The production of these nuclei may influence dynamics of the explosion and contribute to the synthesis of heavy elements. 2004 Elsevier B.V. All rights reserved. PACS: 25.70.Pq; 26.50.+x; 26.30.+k; 21.65.+f In recent years significant progress has been made nucleons and lightest clusters (vaporisation). These by nuclear community in understanding properties of different intermediate states can be understood as a highly excited nuclear systems. Such systems are rou- manifestation of the liquid–gas type phase transition tinely produced now in nuclear reactions induced by in finite nuclear systems [1]. A very good description hadrons and heavy ions of various energies. Under cer- of such systems is obtained within the framework of tain conditions, which are well studied experimentally, statistical multifragmentation model (SMM) [2].
    [Show full text]