Radiative meson transitions in the quark model Olga Lakhina University of Pittsburgh Research Advisor Eric Swanson.

Slides:



Advertisements
Similar presentations
1 The and -Z Exchange Corrections to Parity Violating Elastic Scattering 周海清 / 东南大学物理系 based on PRL99,262001(2007) in collaboration with C.W.Kao, S.N.Yang.
Advertisements

Kernfysica: quarks, nucleonen en kernen
HL-2 April 2004Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-2) Quarkonium Charmonium spectrum quark-antiquark potential chromomagnetic.
Branching Ratios of B c Meson Decaying to Vector and Axial-Vector Mesons Rohit Dhir Department of Physics, Yonsei University, Seoul, Korea. Dated:21-Sept-2012.
The Electromagnetic Structure of Hadrons Elastic scattering of spinless electrons by (pointlike) nuclei (Rutherford scattering) A A ZZ  1/q 2.
A Primer on Atomic Theory Calculations (for X-ray Astrophysicists) F. Robicheaux Auburn University Mitch Pindzola and Stuart Loch I.Physical Effects II.Atomic.
1  /e + e - arXiv: [nucl.th]. 2 3 Sometime ago it was noted that: “The ratio of the production rates (  /  +  - ) and (  o,  /  +  -
Particle Interactions
The semiclassical Rabi problem. We have a two level atom,with We look for the solution of the Schrödinger equation as: The atom has a hamiltonian: The.
Finite Size Effects on Dilepton Properties in Relativistic Heavy Ion Collisions Trent Strong, Texas A&M University Advisors: Dr. Ralf Rapp, Dr. Hendrik.
04/06/2015PHY 712 Spring Lecture 281 PHY 712 Electrodynamics 9-9:50 AM MWF Olin 103 Plan for Lecture 28: Continue reading Chap. 14 – Radiation.
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
Lecture 5: Electron Scattering, continued... 18/9/2003 1
Electromagnetic Radiation The speed of electromagnetic radiation (speed of light) is constant at x 10 m/s – We’ll express it as 3x10 m/s – The symbol.
Poincare sub-algebra and gauge invariance in nucleon structure Xiang-Song Chen Huazhong University of Science & Technology 陈相松 华中科技大学 武汉 10 July
Physics 452 Quantum mechanics II Winter 2011 Karine Chesnel.
Steffen A. RHIC #1 Steffen A. Bass Duke University & RIKEN-BNL Research Center The Protons Puzzle at RHIC - the demise of pQCD? Recombination.
Su Houng Lee with Kie Sang Jeong 1. Few words on Nuclear Symmetry Energy 2. A QCD sum rule method 3. Preliminary results Nuclear Symmetry Energy from QCD.
Lagrangian of QED: 8 9 fine-structure constant =
Graphic from poster by Sarah Lamb, UConn Honors Program event Frontiers in Undergraduate Research, April 2009 Collimator subtends
Coulomb corrections to R-correlation in the polarized neutron decay Alexey Pak University of Alberta, 2005 Lake Louise Winter Institute 2005, February.
Maksimenko N.V., Vakulina E.V., Deryuzkova О.М. Kuchin S.М. GSU, GOMEL The Amplitude of the Сompton Scattering of the Low-Energy Photons at Quark-Antiquark.
Extraction of SM parameters Onia and QCD Onia Scales and QCD Effective Field Theories Extraction of alpha_s and m_Q Other examples Open challenges in theory.
Four-potential of a field Section 16. For a given field, the action is the sum of two terms S = S m + S mf – Free-particle term – Particle-field interaction.
Physics 452 Quantum mechanics II Winter 2012 Karine Chesnel.
Size and Structure Mikhail Bashkanov University of Edinburgh UK Nuclear Physics Summer School III.
6 of the gluon fields are independent linear combinations of the simple gluon fields we enumerated G  1 = (rg + gr)/  2 G  4 = (bg + gb)/  2 G  6.
April 23, 2008 Workshop on “High energy photon collisions at the LHC 1 Cem Güçlü İstanbul Technical University Physics Department Physics of Ultra-Peripheral.
Electromagnetic Waves
12004, TorinoAram Kotzinian Neutrino Scattering Neutrino interactions Neutrino-electron scattering Neutrino-nucleon quasi-elastic scattering Neutrino-nucleon.
Threshold Resummation for Top- Quark Pair Production at ILC J.P. Ma ITP, CAS, Beijing 2005 年直线对撞机国际研讨会, Tsinghua Univ.
Neutrino cross sections in few hundred MeV energy region Jan T. Sobczyk Institute of Theoretical Physics, University of Wrocław (in collaboration with.
AAAS Symposia Nuclear Matter at the Highest Energies and Densities James Nagle Columbia University James Nagle Lepton and Dilepton Production: Current.
Towards a final criteria of separating momentum and angular momentum Outline: I.The matter of convenience II.The matter of reasonableness III.The matter.
Physics of Ultra-Peripheral Nuclear Collisions Melek YILMAZ ŞENGÜL Kadir Has University & İstanbul Technical University M.Cem GÜÇLÜ İstanbul Technical.
Heavy hadron phenomenology on light front Zheng-Tao Wei Nankai University 年两岸粒子物理与宇宙学 研讨会,重庆, 5.7—5.12 。
For long wavelength, compared to the size of the atom The term containing A 2 in the dipole approximation does not involve atomic operators, consequently.
Heavy Quark Energy Loss due to Three-body Scattering in a Quark- Gluon Plasma Wei Liu Texas A&M University  Introduction  Heavy quark scattering in QGP.
I=1 heavy-light tetraquarks and the Υ(mS) → Υ(nS)ππ puzzle Francisco Fernández Instituto de Física Fundamental y Matemáticas University of Salamanca.
Neutrino-Nucleus Reactions at Medium and Low Energies [contents] 1. Neutrino and weak interaction 2. Cross section for ν-A and e-A reactions 3. EMC effect.
Bethe-Salper equation and its applications Guo-Li Wang Department of Physics, Harbin Institute of Technology, China.
Modern Physics Chapters Wave-Particle Duality of Light Young’s Double Slit Experiment (diffraction) proves that light has wave properties So does.
Exclusive charmonium production in hard exclusive processes. V.V. Braguta Institute for High Energy Physics Protvino, Russia.
Static Polarizability of Mesons in the Quark Model N.V. Maksimenko, S.M. Kuchin.
More on the Standard Model Particles from quarks Particle interactions Particle decays More conservation laws Quark confinement Spin.
Xiangdong Ji University of Maryland — RIKEN workshop on polarized gluon distributions, Dec. 3, 2005 — Gluons in the proton.
Atomic Physics Quantum Physics 2002 Recommended Reading: Harris Chapter 7.
Beijing, QNP091 Matthias F.M. Lutz (GSI) and Madeleine Soyeur (Saclay) Irfu/SPhN CEA/ Saclay Irfu/SPhN CEA/ Saclay Dynamics of strong and radiative decays.
Electromagnetic Spectrum Chemistry 6(B). Lesson Objectives Explore the electromagnetic spectrum Understand the mathematical relationships between energy,
QCHS 2010 Lei Zhang1 Lei Zhang (on behalf of BESIII Collaboration) Physics School of Nanjing University Recent.
Higher Charmonium 1) Spectrum 2) Strong decays (main topic) 3) L’oops Ted Barnes Physics Div. ORNL Dept. of Physics, U.Tenn. GHP2004 Fermilab, Oct.
Radiative Decays involving Scalar Mesons Masayasu Harada (Nagoya Univ.) based Japan-US Workshop on “Electromagnetic Meson Production and Chiral Dynamics”
Nuclear recoil in the Lamb shift of hydrogen-like atoms
Study of Charmonium States in Vacuum and High Density Medium
The Electromagnetic Spectrum Part 1
Polarization in charmless B VV decays
dark matter Properties stable non-relativistic non-baryonic
QCD (Quantum ChromoDynamics)
Diatomic molecules
Charm2010 4TH International Workshop on Charm Physics
Perturbation Theory Lecture 5.
王国利(Guo-Li Wang) 哈尔滨工业大学
Electromagnetic Radiation
Which kind of electromagnetic radiation has the least amount of energy? RADIO WAVES.
Heavy-to-light transitions on the light cone
Interpretation of the observed hybrid candidates by the QGC Model
Fundamental Forces of Nature
Pion transition form factor in the light front quark model
Perturbation Theory Lecture 5.
The E.M.S. S1 Physics Energy.
Presentation transcript:

Radiative meson transitions in the quark model Olga Lakhina University of Pittsburgh Research Advisor Eric Swanson

Typically used approximations  Impulse approximation

quark antiquark + quark antiquark Typically used approximations  Impulse approximation

Typically used approximations  Impulse approximation  Using SHO meson wave functions

Typically used approximations  Impulse approximation  Using SHO meson wave functions Gaussian Coulomb+linear rr

Typically used approximations  Impulse approximation  Using SHO meson wave functions  Dipole (long wave-length) approximation

Typically used approximations  Impulse approximation  Using SHO meson wave functions  Dipole (long wave-length) approximation The momentum of the photon: (no recoil) In reality

Typically used approximations  Impulse approximation  Using SHO meson wave functions  Dipole (long wave-length) approximation  Non-relativistic approximation

Typically used approximations  Impulse approximation  Using SHO meson wave functions  Dipole (long wave-length) approximation  Non-relativistic approximation Not true (especially for the light quarks)

Typically used approximations  Impulse approximation  Using SHO meson wave functions  Dipole (long wave-length) approximation  Non-relativistic approximation  Applied to only light or heavy quark sector

Perform the detailed study of meson radiative transitions Motivation Use realistic wave functions Relativistic corrections / effects Higher order diagrams (beyond the impulse approximation) Bound state formalism

Our method Hamiltonian : Electromagnetic interaction:

Non-relativistic approximation Hamiltonian: Electromagnetic interaction:

Results for cc mesons

Results for light mesons

Higher order diagrams Nonrelativistic approximation of Hamiltonian: model: + other terms

Higher order diagrams

VMD model diagram We have to sum over the intermediate states

This diagram does not contribute if we don’t sum over the intermediate states Second order diagram

+ = 0 These diagrams cancel for cc mesons

Second order diagram

Effects of higher order diagrams (GeV -1/2 )

Cornell model + neglected - order

END

r V(r) Potential energy of quark interaction in a meson Coulomb dependence Linear dependence

where Decay rate:

Vector meson dominance model Quark model