HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen1 Nuclear Physics: quarks, nucleons and nuclei (QNK) Prof. dr. G. van der Steenhoven and Prof. dr.

Slides:



Advertisements
Similar presentations
Introduction to nuclear and particle physics
Advertisements

Günther Rosner EUROHORC/NuPECC, Paris, 29/11/04 1 Hadron Structure & Spectroscopy Experimental frontiers: High precision High intensity Theoretical symbiosis:
Introduction Glasgow’s NPE research Group uses high precision electromagnetic probes to study the subatomic structure of matter. Alongside this we are.
HL-1 May 2, 2006Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-1) Particle Production Particle production in e + e - collisions Detection.
Kernfysica: quarks, nucleonen en kernen
HL-3 May 2006Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-3) Structure of nuclei NN potential exchange force Terra incognita in nuclear.
HL-5 May 2005Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-5) Collective excitations of nuclei photo-excitation of GDR particle-hole excitations.
Kernfysica: quarks, nucleonen en kernen
HL-2 April 2004Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-2) Quarkonium Charmonium spectrum quark-antiquark potential chromomagnetic.
Properties and Decays of Heavy Flavor S-Wave Hadrons Rohit Dhir Department of Physics, Yonsei University, Seoul Dated:11 th June, 2012.
Lecture 3 – neutrino oscillations and hadrons
"Now I am become Death, the destroyer of worlds." Robert Oppenheimer after the first test of the atomic bomb.
A nucleus can be specified By an atomic number and a Mass number.
Early Universe Chapter 38. Reminders Complete last Mallard-based reading quiz before class on Thursday (Ch 39). I will be sending out last weekly reflection.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE  5-Feb pm Physics LRA Dr M Burleigh Intro lecture  9-Feb-04.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 3-Feb pm Physics LRA Dr Matt Burleigh Intro lecture 7-Feb-05.
1 The elusive neutrino Piet Mulders Vrije Universiteit Amsterdam Fysica 2002 Groningen.
Schlüsselexperimente der Elementarteilchenphysik:.
Particle Physics Introductory notes, January 23, 2006 Division of Experimental High Energy Physics (
Opportunities for low energy nuclear physics with rare isotope beam 현창호 대구대학교 과학교육학부 2008 년 11 월 14 일 APCTP.
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
Revelations of the neutrino:
Christina Markert Physics Workshop UT Austin November Christina Markert The ‘Little Bang in the Laboratory’ – Accelorator Physics. Big Bang Quarks.
New States of Matter and RHIC Outstanding questions about strongly interacting matter: How does matter behave at very high temperature and/or density?
Frontiers of Nuclear Physics A Personal Outlook Huan Zhong Huang Department of Physics and Astronomy University of California, Los Angeles Department of.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
My Chapter 30 Lecture.
Nuclear Physics at Richmond The Frontier One of the major frontiers in nuclear physics is understanding why quarks and gluons act the way they do to create.
Petten 29/10/99 ANTARES an underwater neutrino observatory Contents: – Introduction – Neutrino Astronomy and Physics the cosmic ray spectrum sources of.
1 FK7003 Elementary Particle Physics David Milstead A4:1021 tel: /
School of Arts & Sciences Dean’s Coffee Presentation SUNY Institute of Technology, February 4, 2005 High Energy Physics: An Overview of Objectives, Challenges.
The Discoveries of Particle & Nuclear Physics Models and Experimental Facts.
Subatomic Physics Chapter Properties of the Nucleus The nucleus is the small, dense core of an atom. Atoms that have the same atomic number but.
Elementary Particles: Physical Principles Benjamin Schumacher Physics April 2002.
Quarks, Leptons and the Big Bang particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
First Results of Curtis A. Meyer GlueX Spokesperson.
Jeopardy Jeopardy PHY101 Chapter 12 Review Study of Special Relativity Cheryl Dellai.
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
High Energy Nuclear Physics and the Nature of Matter Outstanding questions about strongly interacting matter: How does matter behave at very high temperature.
Student Seminar Subatomic Physics Herbert Löhner, Olaf Scholten, Johan Messchendorp 1st block, semester 1, 2008/2009 Wednesday 15:15-17:00 This course.
Lecture 12: The neutron 14/10/ Particle Data Group entry: slightly heavier than the proton by 1.29 MeV (otherwise very similar) electrically.
The FAIR* Project *Facility for Antiproton and Ion Research Outline:  FAIR layout  Research programs Peter Senger, GSI USTC Hefei Nov. 21, 2006 and CCNU.
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
Jets as a probe of the Quark Gluon Plasma Jets as a probe of the Quark Gluon Plasma Christine Nattrass Yale University Goldhaber Lecture 2008 Christine.
Introduction to CERN Activities
PHY418 Particle Astrophysics
Lecture 2: The First Second Baryogenisis: origin of neutrons and protons Hot Big Bang Expanding and cooling “Pair Soup” free particle + anti-particle pairs.
Phys 102 – Lecture 28 Life, the universe, and everything 1.
Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.
CEBAF - Continuous Electron Beam Accelerator Facility.
Goals of future p-pbar experiment Elmaddin Guliyev Student Seminar, KVI, Groningen University 6 November 2008.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #1.
Introduction to Particle Physics (for non physics students) 3. FORCES.
Structure of Matter. Nucleons and quarks 1950’s: nucleons are not elementary : quark model and QCD (Nobel prize 2004) : Higgs particle discovered?
Phy107 Fall From Last Time… Particles are quanta of a quantum field –Often called excitations of the associated field –Particles can appear and.
10/29/2007Julia VelkovskaPHY 340a Lecture 4: Last time we talked about deep- inelastic scattering and the evidence of quarks Next time we will talk about.
EIC NAS review Charge-2 What are the capabilities of other facilities, existing and planned, domestic and abroad, to address the science opportunities.
Elementary Particle Physics
Welcome Stuart Henderson May 22, 2017.
CERN Students Summer School 2006
Nuclear Physics -- Today and Tomorrow From the infinitely strong –
CERN Students Summer School 2008
EIC NAS review Charge-2 What are the capabilities of other facilities, existing and planned, domestic and abroad, to address the science opportunities.
Kernfysica: quarks, nucleonen en kernen
ELEMENTARY PARTICLES.
Early Universe.
Quarks, Colors, and Confinement
PHYS 3446 – Lecture #23 Standard Model Wednesday, Apr 25, 2012
Modern Studies of the Atom
u c s b d n Hadron & Nuclear Physics Particle Physics Quarks Leptons
Presentation transcript:

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen1 Nuclear Physics: quarks, nucleons and nuclei (QNK) Prof. dr. G. van der Steenhoven and Prof. dr. H. Löhner 5 th ( and last!) edition, Rijksuniversiteit Groningen, May 2 - June23, ‘06

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen2 Some excitement to begin with…. 2003: the claimed discovery of : Pentaquarks Known particles built up from quarks: –Mesons (or - pairs): –Baryons (or - configurations): Theoretical prediction (“QCD”) – configurations exist  – but they were never found….

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen3

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen4 The experimental work 5 GeV electron accelerator - JLab at Newport News: The reaction  + p   + (1540) in Hall B: Hall B

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen5 HERMES SAPHIRLEPS The experimental evidence Results of three more experiments: In all cases: surprisingly narrow peak near 1535 MeV/c 2 ??

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen6 Why would this be a pentaquark? What is observed:  + p → (K + + n) + X Positive kaon (K + ) and neutron (n) originate from: [There is no s-quark that can annihilate the anti s-quark.] But many questions remain: –What is the dynamic structure of the  + ? –What are the quantum numbers of the  + ? –Is there evidence for other pentaquark particles ?

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen7 u u d d u d d u u u u d d d u d u a) Five quarks in a s - state configuration. b) Five quarks in a K + -n molecular configuration. c) Five quarks in a strong diquark correlation state. d) Collective excitation of a multiquark configuration. Pentaquark models…..... u d d

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen8 The bottom line… Pentaquarks: example of exciting ongoing frontline research topic in QNK Physics…(to be continued !) What else today: –What is the scope of Modern Nuclear/Particle Physics? –Purpose, organization and terms of the lectures –The real beginning: some basic Particle Physics

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen9 Study of resonances by hyperon production hyperon polarization models for resonance structure

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen10 Some Places to Explore Non-Pertubative QCD charmonium spectroscopy ( states) gluonic excitations: hybrids: “ordinary” quark states containing excited glue glueballs: gluonic states without valence quark contribution  -ray spectroscopy of hypernuclei

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen11 Stranges s Neutron Number Extension of the Nuclear Chart We do not yet understand the interaction of normal matter with hyperon matter !

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen12 Neutrino Astronomy Consider distant sources of radiation: –Supernovae,  Quasars, GRBs, AGNs, …. Effect of interstellar medium: –High-energy EM radiation is (partly) absorbed –Protons are bended – can be traced back to the source  p

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen13 Active Galaxy (e.g. M87) Black hole with 10 8 x mass of sun  10 4 ly extra-galactic Microquasar (SS433 etc.) Black hole with  mass of sun  1 ly galactic Possible neutrino point sources Supernova remnant (Crab nebula)

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen14 p p  KM3NET: basic concept Underwater Cherenkov detector of ~ 1 km 3

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen15 present experiment: “Antares” Neutrino Telescope Strings with phototubes in the water of the Mediterranean Sea Sequence of light signals indicates the track and the energy of particles

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen16 Many subfields Not all covered in present lectures! Many front lines! Nuclear structure Super heavy nuclei Rare isotopes Nucl. astrophysics nucleons atomicnuclei The scope of Nuclear Physics NN-interaction Few-body physics Entanglement Strangeness QCD New qg-systems The origin of mass and spin of hadrons Parity violation Neutrino masses Fundamental constants Beyond Standard Model Astroparticle Physics heavy ions quarks & gluons neutrinos Quark Gluon Plasma Phases of matter

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen17 The scope of this lecture series Physics of elementary constituents: quarks, gluons Physics of elementary interactions: QCD Composite quark-gluon systems: pions, protons Protons, neutrons & other hadrons: NN-interactions Atomic nuclei: structure, reactions What we hope to achieve: Understanding of modern subatomic physics literature

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen18 Selection of topics The discovery of quarks The discovery of gluons Structure of nucleons Relativistic quantum mechanics Quantum chromodynamics (QCD) The N-N interaction, the deuteron Nuclear reactions, spectroscopy Models of the atomic nucleus

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen19 Educational methods used Regular lectures: use the opportunity! Student presentations on, e.g.: –Neutrino mass and oscillations –Nuclear  -decay –The quark-gluon plasma –CP violation –The nuclear shell model –Weak neutral currents Oral exam end June or early July 2006: –Discuss recent nuclear physics article from Physical Review Letters (4 pages)

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen20 Literature and notes Recommended text books: –Povh, Rith, Scholz and Zetsche (Springer) 1995: “Particles and Nuclei” –Burcham and Jobes (Prentice Hall) 1995: “Nuclear and Particle Physics” Additional useful sources Heyde (IoP) 1994: “Basic ideas and concepts in nuclear physics” Zuber (IoP) 2004: “Neutrino Physics” Lecture notes on the web: – under Lectures –

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen21 How to study? Lectures: –Emphasis on physical concepts –No long derivations → home work For each subject: –Introduction in the lectures –In-depth understanding → self study –Application: student presentations Exam: –Discussion of recent paper

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen22 Who is who? Gerard van der Steenhoven: –Quark-gluon physics at DESY/Hamburg –ANTARES Groupleader at NIKHEF –Chair Committee for Astroparticle Physics NL –Professor of Exp. Nuclear Physics RUG Herbert Löhner: –Meson-nucleon physics at KVI/Bonn/GSI –PANDA (GSI / D) Groupleader at KVI –Professor of Exp. Nuclear Physics RUG –dir. opleiding natuurkunde/techn. natuurkunde

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen23 What else today The beauty of QNK! Practical issues… Introduction “Basic Particle Physics” ‘Particles and Nuclei’ particle production in e+e- ollisions hadron resonances

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen24 Why quarks, nucleons and nuclei? Basis of modern nuclear physics Current themes in nuclear physics: 1.QCD-basis of nuclear physics? 2.Does the Quark-Gluon Plasma exist? 

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen25 Why quarks, nucleons and nuclei? Current themes in nuclear physics (cnt’d): 3.What are the limits of nuclear stability? 4.New physics beyond the Standard Model at low E (neutrino mass!)  Interface nuclear and particle physics

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen26 Why quarks, nucleons and nuclei? Current themes in nuclear physics (cnt’d): 5.Relevance to astronomy: [Development of Astroparticle Physics in NL!] 6.Applications: Archeology: dating Lungs: 3 He tomographyProton therapy

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen27 Some practical issues Please ask questions: – Now…. or at any moment…… – ….or at the next lecture…… – – List of names + addresses Overview of lecturing dates Organization of student presentations

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen28 Kernfysica: Quarks Nucleonen en Kernen This lecture will be given in quarter 4 of the study-year 2005/2006. lecture period: lectures will be given by Prof. dr. Herbert Löhner (KVI Groningen) and Prof. dr. Gerard van der Steenhoven (NIKHEF Amsterdam) lecture hours: Tuesday 09: :00 in room Friday 09: :00 in room schedule of the lectures and student contributions (.ppt) find slides from Herbert Löhner here: ( ) lecture 1: Tuesday, May 2 lecture 2: Tuesday, May 16 lecture 3: Friday, May 19 lecture 4: Tuesday, May 23 lecture 5: Friday, May 25 schedule lecture 6: Tuesday, June 13 find slides from Gerard van der Steenhoven herefind slides from Gerard van der Steenhoven here ( ) Student contributions: (will be listed here once presented) Oral tentamen: schedule will be discussed in the course of the lecture. Every student will receive one week in advance a recent publication for the tentamen-discussion.

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen29 Tuesday 09:15-11:00 room Friday 9:15 –12:00 room HL Introduction, basic particle physics and hadron structure 5.5. General Holiday No lectures 9.5. GvdS Basic nuclear physics12.5. GvdS Electron scattering off nuclei, nucleons and quarks HL The structure of mesons and baryons19.5. HL The nucleon-nucleon interaction HL Nuclear reactions26.5. HL Collective nuclear excitations GvdS Relativistic Quantum Mechanics2.6. GvdS Applications of Dirac Theory 6.6. GvdS Quantum Chromodynamics I9.6. GvdS Quantum Chromodynamics II + astro-particle physics HL (spare time) + charmonium, hybrids and glueballs HL/GvdS 3 student presentations GvdS &HL; 2 student presentations GvdS &HL; 3 student presentations (extra day) 9:00 – 14:00 KVI: Oral Examination (ca. 30 min p.p.) Lecturers: GvdS = G. van der Steenhoven; HL = H. Löhner

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen30 Subjects for student presentations DateSubjectName Neutrino Mass and Oscillations (BJ 15.3) Nuclear  decay (Povh, 17.6 and BJ 5.2) Neutrino Scattering (BJ & ) The nuclear shell model (Heyde Ch. 9) Charmonium spectroscopy (handout) Neutron stars (Povh, p. 226 etc.) Collective model & Superdeform. (BJ 4.3) The quark-gluon plasma (Povh, Ch. 20) 9Weak neutral currents (BJ ) 10CP violation in kaon decay (BJ 11.13) 11Nuclear reactions (BJ 6.2 – 6.5) 12The spin of the proton (handout) 13Analysis of resonances (BJ 9.2)

HL- May 2, 2006Kernfysica: quarks, nucleonen en kernen31 Select a subject Discuss literature with one of the lecturers Study the subject Make link to the rest of the lecture Design a presentation (30 min.) Make use of Power Point or Foil-Tex (PDF) Pre-discussion with lecturer Make final presentation Give at least one rehearsal talk Transport presentation via CD or memory stick How to prepare a student lecture?