For each nucleon Why an optical model ? A 1 nucleons A 2 nucleons N=A1+A2 equations to solve.... N body problem one body problem a particle with a mass.

Slides:



Advertisements
Similar presentations
Compound Nucleus Reactions
Advertisements

Radiopharmaceutical Production
NE Introduction to Nuclear Science Spring 2012
Reaction dynamics of light nuclei around the Coulomb barrier Alessia Di Pietro INFN-Laboratori Nazionali del Sud ARIS 2014Alessia Di Pietro,INFN-LNS.
Single Neutron Stripping Reactions for Structural Study of 23 O Ravinder Kumar Department of Physics Kurukshetra University, Kurukshetra Kurukshetra -
Microscopic time-dependent analysis of neutrons transfers at low-energy nuclear reactions with spherical and deformed nuclei V.V. Samarin.
Like the alchemist’s dream
Mean field description of the nucleus-nucleus optical potential Institute for Nuclear Science & Technique Vietnam Atomic Energy Commission (VAEC) Dao Tien.
RFSS: Lecture 9 Nuclear Reactions
Direct Reactions. Optical model Represent the target nucleus by a potential -- Attenuation length.
P460 - barriers1 Bound States and Tunneling V 0 0 State A will be bound with infinite lifetime. State B is bound but can decay to B->B’+X (unbound) with.
Probing nuclear potential with reactions Krzysztof Rusek Heavy Ion Laboratory, University of Warsaw, The Andrzej Soltan Institute for.
Lesson 10 Nuclear Reactions.

Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Nuclear Reactions Categorization of Nuclear Reactions According to: bombarding.
25 9. Direct reactions - for example direct capture: Direct transition from initial state |a+A> to final state B +  geometrical.
Lecture 10 Energy production. Summary We have now established three important equations: Hydrostatic equilibrium: Mass conservation: Equation of state:
Nucleon Optical Potential in Brueckner Theory Wasi Haider Department of Physics, AMU, Aligarh, India. E Mail:
Nuclear reactions 1) Introduction 2) Nuclear reaction yield
The Theory of Partial Fusion A theory of partial fusion is used to calculate the competition between escape (breakup) and absorption (compound-nucleus.
Computational Lab in Physics: Final Project Monte Carlo Nuclear Collisions: Glauber Model.
Nuclear Fundamentals Part I Unleashing the Power of the Atom.
1 This lecture: What can we learn from scattering experiments? Summary from last time: - planetary model of the atom - isotopes and mass spectroscopy -
Α - capture reactions using the 4π γ-summing technique Α. Lagoyannis Institute of Nuclear Physics, N.C.S.R. “Demokritos”
Cross Sections One of the most important quantities we measure in nuclear physics is the cross section. Cross sections always have units of area and in.
If the Coordinates system is. R r b (impact parameter.
Mean-Field Description of Heavy Neutron-Rich Nuclei P. D. Stevenson University of Surrey NUSTAR Neutron-Rich Minischool Surrey, 2005.
Lawrence Livermore National Laboratory SciDAC Reaction Theory LLNL-PRES Lawrence Livermore National Laboratory, P. O. Box 808, Livermore, CA
Extended optical model analyses of elastic scattering and fusion cross sections for 6, 7 Li Pb systems at near-Coulomb-barrier energies by using.
Nuclear Models Nuclear force is not yet fully understood.
Potential Approach to Scattering of Exotic Nuclei Goncharov S.A.
Single nucleon transfer between p- shell nuclei around 10 MeV/u - for nuclear astrophysics Livius Trache Cyclotron Institute, Texas A&M University ATLAS.
Lecture 11 Energy transport. Review: Nuclear energy If each reaction releases an energy  the amount of energy released per unit mass is just The sum.
1 Nuclear Reactions – 1/2 DTP 2010, ECT*, Trento 12 th April -11 th June 2010 Jeff Tostevin, Department of Physics Faculty of Engineering and Physical.
Neutron enrichment of the neck-originated intermediate mass fragments in predictions of the QMD model I. Skwira-Chalot, T. Cap, K. Siwek-Wilczyńska, J.
Application of correlated basis to a description of continuum states 19 th International IUPAP Conference on Few- Body Problems in Physics University of.
Some aspects of reaction mechanism study in collisions induced by Radioactive Beams Alessia Di Pietro.
The nuclear mean field and its symmetries W. Udo Schröder, 2011 Mean Field 1.
Nucleon DIffusion in Heavy-Ion Collisions
Mesut Karakoç May 31st, 2012 TAMU-Commerce & Akdeniz U. - Turkey Collaborators: Carlos Bertulani (TAMU-Commerce) Adriana Banu (James Madison U.) Livius.
Nucleon-Nucleon collisions. Nucleon-nucleon interaction at low energy Interaction between two nucleons: basic for all of nuclear physics Traditional goal.
Three-body force effect on the properties of asymmetric nuclear matter Wei Zuo Institute of Modern Physics, Lanzhou, China.
School of Cosmic-ray Astrophysics, Erice, July 4, 2004 Thomas K. Gaisser Role of particle interactions in high-energy astrophysics Uncorrelated fluxes.
Slide 1 of Woonyoung So International Workshop on e-Science for Physics 2008 Extended Optical Model Analyses for the 9 Be+ 144 Sm System.
Monday, Sept. 18, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #5 Monday, Sept. 18, 2006 Dr. Jae Yu 1.Nuclear Phenomenology 2.Properties of Nuclei.
PKU-CUSTIPEN 2015 Dirac Brueckner Hartree Fock and beyond Herbert Müther Institute of Theoretical Physics.
PROPERTIES OF HIGH-ENERGY ISOSCALAR MONOPOLE EXCITATIONS IN MEDIUM-HEAVY MASS SPHERICAL NUCLEI M. L. Gorelik 1), S. Shlomo 2), B. A. Tulupov 3), M. H.
Important role of three-body repulsive force effect in nuclear reactions Takenori FURUMOTO (Osaka City Univ. ) 19th International IUPAP Conference on Few-Body.
Crystal Ball Collaboration Meeting, Basel, October 2006 Claire Tarbert, Univeristy of Edinburgh Coherent  0 Photoproduction on Nuclei Claire Tarbert,
A. Dokhane, PHYS487, KSU, 2008 Chapter1- Neutron Reactions 1 NEWS Lecture1: Chapter 0 is already on my Website.
Study of repulsive nature of optical potential for high energy 12 C+ 12 C elastic scattering (Effect of the tensor and three-body interactions) Gaolong.
Dynamical Model of Surrogate Reaction Y. Aritomo, S. Chiba, and K. Nishio Japan Atomic Energy Agency, Tokai, Japan 1. Introduction Surrogate reactions.
Oct. 16 th, 2015, Yonsei. RAON 2 Far from Stability Line 3.
Improvements of microscopic transport models stimulated by spallation data for incident energies from 113 to MeV Umm Al-Qura University and King.
Study of microscopic complex potentials for nuclear scattering reaction Takenori Furumoto (Ichinoseki National College of Technology) YIPQS International.
Absorption of Nuclear Radiation & Radiation Effects on Matter: Atomic and Nuclear Physics Dr. David Roelant.
V. Nuclear Reactions Topics to be covered include:
Two-body force in three-body system: a case of (d,p) reactions
The Strong Force: NN Interaction
Phenomenological Optical Potentials
3. The optical model Prof. Dr. A.J. (Arjan) Koning1,2
Scattering Cross Sections (light projectile off heavy target)
PHL424: Semi-classical reaction theory
Intermediate-mass-fragment Production in Spallation Reactions
PHL424: Rutherford scattering discovery of nucleus
Chapter 4 Mechanisms and Models of Nuclear Reactions
PHL424: Semi-classical reaction theory
Elastic alpha scattering experiments
V.V. Sargsyan, G.G. Adamian, N.V.Antonenko
sinv in ABLA Particle-decay width in Weisskopf-Ewing approach:
Presentation transcript:

for each nucleon Why an optical model ? A 1 nucleons A 2 nucleons N=A1+A2 equations to solve.... N body problem one body problem a particle with a mass  is in a potential well V(r) which replaces all the interactions between the different nucleons.  :reduced mass of the system all the interactions between the nucleons are replaced by an average and central interaction V(r) between the projectile and the target Optical model References: P. E. Hodgson, The nucleon optical potential, Clarendon Press, 1994 G. R. Satchler, Direct nuclear reactions, Oxford University Press, New York, 1983

Optical potential V(r) = U(r) + i W(r) The optical model used to describe the interaction between two nuclei is inspired by the optical phenomena. represents the elastic scattering reflexion of the incident wave imaginary real partimaginary part absorption of the incident wave simulates the loss of flux due to no elastic collisions to take into account the others reactions which can occured V(r) = U(r) + iW(r) + V so (r) + V c (r) spin-orbite Coulomb

Phenomenogical optical potential 6 He(p,p) 6 He 150 MeV  cm (deg) d  /d  (mb/sr) U(r) = U v f(r) W(r) = W s g(r) + W v f(r) Woods- Saxon R: potential radius a: potential diffusness elastic scattering data: parametrization of U v, W s, W v, a v, a Ws, a Wv, R, V so p-nucleus, n-nucleus interaction: parametrization CH89 from Varner et al. nucleus-nucleus interaction: not general parametrization a projectile on a reduced number of target or limitation in energy. parameters adjusted case by case nuclei in their ground sates !!!!

Microscopic optical potential OpOp OtOt Projectile Target r pt rtrt rprp r pp pp Folding effective nucleon-nucleon force densities  : microscopic or macroscopic densities

Link with ABLA Now: a real potential is used to describe the transmission probability of particles The decay width  for evaporation: another possibility to calculate  capture : optical potentials Kildir et al., PRC 51, 1873 (1995) Aleksandra (nuclei not in their groundstates) E = E imf + E partner + Q +  - B