Protons Neutrons Nuclear structure at finite temperature probed by the Giant Dipole Resonance G. Benzoni, O. Wieland, A. Bracco, N. Blasi, F. Camera, F.

Slides:



Advertisements
Similar presentations
? Nuclear Reactions Categorization of Nuclear Reactions
Advertisements

Exotic Shapes and High Spin physics with Intense Stable Beams.
Future prospects and needs for nuclear structure studies with high intensity stable beams.
Gamma-ray strength functions Also called in the literature: radiative strength functions photon strength functions Presentation OCL group meeting Ann-Cecilie.
Γ spectroscopy of neutron-rich 95,96 Rb nuclei by the incomplete fusion reaction of 94 Kr on 7 Li Simone Bottoni University of Milan Mini Workshop 1°-
Oslo-07-TD Landscapes and fluctuations of two-dimensional rotational  - spectra – coupling between rotational and thermal motion Rare earth nuclei p resolved.
The Collective Model and the Fermi Gas Model
The Collective Model Aard Keimpema.
Section 2Nuclear Changes Nuclear Forces 〉 What holds the nuclei of atoms together? 〉 The stability of a nucleus depends on the nuclear forces that hold.
Monday, Feb. 14, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #8 Monday, Feb. 14, 2005 Dr. Jae Yu 1.Nuclear Models Shell Model Predictions Collective.
Nuclear Fission and Fusion. Nuclear Fission Nuclear Fission: The splitting of a massive nucleus into two smaller nuclei.
Nuclear Chemistry Bravo – 15,000 kilotons. CA Standards.
Nuclear Fission and Fusion
Congresso del Dipartimento di Fisica Highlights in Physics –14 October 2005, Dipartimento di Fisica, Università di Milano Study of exotic nuclei.
Nuclear Fission The splitting of a nucleus into two smaller fragments.
Doctoral Defense of Barak Hadina 18 th January 2008 In-Beam Study of Extremely Neutron Deficient Nuclei Using the Recoil Decay Tagging Technique Opponent:
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Nuclear Reactions Categorization of Nuclear Reactions According to: bombarding.
NUCLEAR STRUCTURE PHENOMENOLOGICAL MODELS
Radiation Objectives Understand the concepts of ½ life and ½ thickness in radiation Differentiate between fusion and fission Describe the processes involved.
Objectives To learn the types of radioactive decay
NUCLEAR CHEMISTRY QUIZ.
Nuclear structure investigations in the future. J. Jolie, Universität zu Köln.
NUCLEAR MODELS.
Nuclear Reactions Atomic structure: Atomic structure: –Proton (+), Neutron (0), Electron (-) –Protons and Neutrons are found in the nucleus, where the.
Nuclear Fission vs. Fusion What is what????. Fission…what is it? Nuclear reaction OR radioactive decay Nucleus of an atom splits into smaller parts, neutrons.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Reactions Sample.
Collective Model. Nuclei Z N Character j Q obs. Q sp. Qobs/Qsp 17 O 8 9 doubly magic+1n 5/ K doubly magic -1p 3/
The Giant Dipole Resonance, new measurements F. Camera University of Milano and INFN sect. of Milano HECTOR Collaboration Giant Dipole Resonance in very.
Aim: Why do fission and fusion reactions release so much energy? Essential Questions : Compare and contrast nuclear fission with fusion. Distinguish between.
Nuclear Structure studies using fast radioactive beams J. Gerl SNP2008 July Ohio University, Athens Ohio USA –The RISING experiment –Relativistic.
Nuclear Models Nuclear force is not yet fully understood.
Pygmy Dipole Resonance in 64Fe
Radiation. Atomic Anatomy Atoms –electrons (e-) –protons (p+) –neutrons (n)
Nuclear Physics PHY Outline  history  structure of the nucleus nuclear binding force liquid drop model shell model – magic numbers 
Alpha Decay A Helium- 4 nucleus (two protons and two neutrons). Is produced by nuclear fission Massive nucleus breaks apart into two less-massive nuclei.
10-1 Fission General Overview of Fission The Probability of Fission §The Liquid Drop Model §Shell Corrections §Spontaneous Fission §Spontaneously Fissioning.
 Test on Friday – Make sure you are studying!!  If you got below an 85 on your test, you can come to my Knight Time… Talk to me if you are interested.
W. Nazarewicz. Limit of stability for heavy nuclei Meitner & Frisch (1939): Nucleus is like liquid drop For Z>100: repulsive Coulomb force stronger than.
Living By Chemistry SECOND EDITION Unit 1: ALCHEMY Matter, Atomic Structure, and Bonding.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Shell model Notes: 1. The shell model is most useful when applied to closed-shell.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Extreme independent particle model!!! Does the core really remain inert?
Some (more) High(ish)-Spin Nuclear Structure Paddy Regan Department of Physics Univesity of Surrey Guildford, UK Lecture 2 Low-energy.
Nuclear Chemistry By: Sean Krayca. Unstable Nucleus An unstable nucleus releases energy by Radioactive decay.
Nuclear Reactions. Going Nuclear A nuclear reaction is a reaction in which there are changes to the nuclei of the atoms involved. This differs from previous.
Nuclear Chemistry. Nuclear Chemistry looks at the number of protons and neutrons in an atom Radioactive Decay = Spontaneous disintegration of a nucleus.
Nuclear Reactions Fission and Fusion. FISSION The splitting of an atomic nucleus into 2 smaller particles. Animation.
Nuclear Chemistry. Radioactivity The process by which materials give off such rays radioactivity; the rays and particles emitted by a radioactive source.
PSC 4010 Nuclear Technology: A matter of Energy. PSC 4010: Chapter 4 Goals: _ SWBAT classify examples of changes in matter (physical, chemical, nuclear)
NUCLEAR CHANGES What is Radioactivity?. What happens when an element undergoes radioactive decay? During radioactive decay an unstable nuclei of an isotope.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1.
STAAR Ladder to Success Rung 7. – Alpha particles are helium nuclei with low penetrating power; they can be shielded by paper or cloth. – Beta particles.
Adam Maj IFJ PAN Krakow Search for Pigmy Dipole Resonance in 68 Ni RISING experiment in GSI EWON Meeting Prague, May, 2007.
Monday, Oct. 2, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #8 Monday, Oct. 2, 2006 Dr. Jae Yu 1.Nuclear Models Shell Model Collective Model.
Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion.
Status of Photon Evaporation Alessandro Brunengo INFN Genova Alessandro Brunengo Geant4 Workshop at Noordwijk, The Netherlands September 1999.
 Nuclear Chemistry. Nuclear Vs. Chemical Reactions  Nuclear reactions involve a change in an atom’s nucleus, usually producing a different element.
Congresso del Dipartimento di Fisica Highlights in Physics –14 October 2005, Dipartimento di Fisica, Università di Milano Contribution to nuclear.
CLICK HERE TO BEGIN! Directions: Click the term that correctly matches the definition in each question.
HIRG 重离子反应组 Heavy Ion Reaction Group GDR as a Probe of Alpha Cluster in Light Nuclei Wan-Bing He ( 何万兵 ) SINAP-CUSTIPEN Collaborators : Yu-Gang.
Entry distributions for fragments produced in deep-inelastic collisions with stable and radioactive beams For the PARIS collaboration W. Królas, M. Kmiecik,
Heat Transfer and Nuclear Reactions
Nuclear Stability and Nuclear Decay Reactions
Giant Dipole Resonance decay of hot rotating 88Mo
Nuclear Reactions --Part 2
Feeding of low-energy structures with different deformations by the GDR decay: the nuBall array coupled to PARIS M. Kmiecik, A. Maj, B. Fornal, P. Bednarczyk.
Nuclear Physics, JU, Second Semester,
Evolution of the GDR properties vs E*
Nuclear Chemistry The energy of life.
Unit 4 – Nuclear Reactions
Chemistry Unit Two, Day Four.
Presentation transcript:

Protons Neutrons Nuclear structure at finite temperature probed by the Giant Dipole Resonance G. Benzoni, O. Wieland, A. Bracco, N. Blasi, F. Camera, F. Crespi, S. Leoni, B. Million Dipartimento di Fisica, Università di Milano INFN – Sezione di Milano The protons and the neutrons inside an atomic nucleus behave in a collective way The nucleus can vibrate and rotate as a liquid drop Gamma Rays probes such collective excitations Parameters governing the GDR: E GDR Nuclear Shape  GDR Lifetime and Damping of GDR  GDR How many protons and neutrons vibrates In deformed nuclei the vibrations along the three axes have different resonance frequencies. In spherical nuclei, vibrations along the three axes are identical and correspond to a single resonance frequency. The Giant Dipole Resonance (GDR) is a collective coherent vibration of ALL the protons against ALL the neutrons inside the nucleus Gamma rays energy measures directly the resonance frequency Hector Coupled to the RISING array at GSI The nuclear structure group of Milano has developed and built the HECTOR ARRAY to measure the  -decay of the GDR How GDR properties evolves with nuclear temperature ? Gamma_Lifetime 5* s 1* s "Search for Exotic Shapes of Hot Nuclei at Critical Angular Momenta“ Nucl.Phys.A687(2001)192 "Radiative Fusion from very symmetric reactions: The Giant Dipole Resonance in 179Au nucleus" PLB 560/ (2003)155 How GDR properties evolves with Rotation ? As angular momentum increases the nucleus becomes more and more deformed Nuclear deformation Nuclei can be heated using heavy ion fusion reaction, namely accelerating a projectile against a target. In certain conditions, the two nuclei fuse, and a hot thermalized system, which does not remember how it was formed, is created (compound nucleus) Hot thermalized nuclei cools down ‘evaporating’ particles and gammas which are measured by detectors. Experimental measurements has shown that: The dipole vibration is superimposed on the nucleus whatever is its state (ground state, single particle excitation, compound) The main damping width does not change whatever is its nuclear temperature or angular momentum The measured FWHM of the GDR increases due to the increasing deformation induced by a softening of the nucleus because of temperature At very high temperature compound intrinsic lifetime contributes significantly to the damping width At low temperature shell effects strongly affects GDR width  GDR E GDR "Probing Nuclear Shapes Close to the Fission Limit with GDR in 216Rn“ Physics Review C 70(2004)64317 "Evidence for the Jacobi shape transition in hot 46Ti“ Nucl.Phys.A731(2004)319 "Double Giant Dipole Resonance in Hot Nuclei“ Nucl.Phys.A731(2004)202 "Compound and Rotational Damping in Warm Deformed Rare-Earth Nuclei“ Physical Review Letters 93,2(2004) "Effect of E1 decay in the population of superdeformed structures" Phys.Lett.B 540(2002)199 "The gamma-decay of the GDR in highly excited Ce nuclei" JoP G 31(2005)S1973