Some ideas and questions about the reaction of fission
|
|
- Horace Cox
- 5 years ago
- Views:
Transcription
1 1 Some ideas and questions about the reaction of fission G. Mouze, S. Hachem and C. Ythier University of Nice, France R.A Ricci Laboratori Nazionali di Legnaro, Università di Padova, Padova,Italy SIF XCVII Congresso Nazionale, L Aquila, Settembre 2011
2 2
3 3 Indeed the mass spectrum of Signarbieux can be translated into a Gaussian curve centered on the discrete mass-value 104 If DA,the f.w.h.m., measures the uncertainty in the mass A of the fragment, the uncertainty in t is D t = h/(c 2 DA) = second The reaction time is shorter than the lifetime of the W +- and Z 0 bosons, and s
4 4 The isotopic mass distribution reported by Signarbieux at Z= 50 can be translated into a Gaussian curve, centered on N = 83.3, which reveals an uncertainty DN in the neutron number equal ~ 2.54 u.
5 5
6 n = N MAX - N 6 These Gaussian curves can be viewed as distributions of N around its most probable value N n = 0, N MAx = Cm 142 Ba Zr or as distributions of n around its mean value n n = 0, N MAX = Cm 148 Ba Zr they are reminiscent of that of prompt neutrons:
7 7 The law giving the probability P(n) of emitting n neutrons per fission as a function of (n n) was established by James Terrell (PR 108 (1957) 783) From the value 1.08 of the s- parameter one gets DN = 1.08 X 2.35 = neutrons. Terrell s law is a consequence of DE.Dt = h
8 8
9 9 Dt is close to Dt ( 235 U + n), equal to s Is Dt constant for all fissioning systems? Is the main step of fission the same for all them, e.g. the transfer of a number of nucleons, say 68, from a 208 Pb core to a cluster of mass A cl? For Flynn et al [Phys. Rev.C 5(1972)1725], A L (product) is a linear function of A F. If A F is written as A cl, the law, after correction for neutron emission, becomes A L (fragment) = A cl + 68 Mouze and Ythier NCA 103 A (1990)617.
10 Pu + n 208 Pb + 32 Mg MeV: 32 Mg is a new kind of cluster*. It differs from 14 C, 20 O, 23 F, 22,24-26 Ne, 28,30 Mg, 32,34 Si clusters emitted in cluster-radioactivity ** The clusterization energy Q cl can be converted into vibrational energy and induce fission System Q cl (MeV) A cl 235 U + n Ne 239 Pu + n Mg 252 Cf sf S 258 Fm sf Ar 265 Hs + n ~ Fe 286 (112) sf ~ Zn If Q cl is greater than B C, cluster-fission becomes possible (EPL 58(2002)362) *Ythier and Mouze J. Nucl. Materials 166 (1989)74. ** Poenaru et al PRL 107 (2011)
11 11 Fragments of mass 82 and 126 do not emit prompt neutrons. The neutron yield increases linearly above these values (J. Terrell.Phys.Rev.127(1962)880) For Mouze and Ythier (2008 Bormio Meeting) this situation means that nucleon shells are closed at A = 82 and 126. The 208 Pb core can be destructed and changed into a hard A H = 126 core and 82 nucleons. Part of them are transferred to the cluster, and form a hard A L = 82 core. The remaining 82 ( 82 A cl ) nucleons are shared between these cores.
12 U + n 208 Pb + 28 Ne (A cl = 28) 208 Pb + 28 Ne A = 126 nucleon core + 82 nucleons There are two regions of appreciable yield: A L, from A = 82 to A cl + 82; A H, from A = 126 to A cl Width = A cl u [ JMPE 17,2008]
13 13 The nucleon phase model explains the width of asymmetric mass distributions. Data from Flynn and Glendenin (1970)(without correction) for 235 U + n D A L = 28 u D A H = 28 u Asymmetric fission is strongly confined: up to 256 Fm no fragment pair has a fission energy greater than its own Coulomb barrier
14 14 Symmetric fission results from the closure of a shell made of 126 nucleons in the light fragment (Mouze and Ythier,2008 Bormio Meeting) For 286 (112)(s.f.) the width of the region of appreciable yield is equal to (A cl -44) u, i.e = 34 u
15 15 The nucleon phase model explains the symmetric fission of superheavy nuclei (M.G. Itkis, et.al., Lipari Conf.2001) Symmetric fission Bormio, A cl = 78 Cluster-fission Europhys.Lett. 58(2002) A cl = A cl = 88 This fission is barrier-free (G. Mouze,2005 Bormio Meeting)
16 16 Discussion The magic mass numbers 82 and 126 result from a spin-orbit coupling similar to that of the neutron phase of ordinary matter, as if the Coulomb potential of the protons had disappeared... Moreover, uncertainty in Z exists, but no proton is emitted. Could new physics be hidden in back of this nucleon phase model? Anyway this model consistently explains a great number of experimental facts
17 17 Conclusion Recently Mouze et al. found in Terrell s law on prompt-neutron an answer to Gönnenwein s comment to my 2009 EPN-paper: Dt (fission) = 0.17 ys. And Terrell s law, which allows the chain reaction is simply the way in which Nature warrants the uncertainty in N of any fission fragment.
18 18
19 19
Colinear ternary fission and nucleon phase model G. Mouze, S. Hachem and C. Ythier
1 Colinear ternary fission and nucleon phase model G. Mouze, S. Hachem and C. Ythier Faculté des Sciences, Université de Nice, 06108 Nice cedex 2, France mouze@unice.fr bstract: The colinear ternary fission
More informationOn the true nature of transfer reactions. leading to the complete fusion of projectile and target. G. Mouze and C. Ythier
1 On the true nature of transfer reactions leading to the complete fusion of projectile and target G. Mouze and C. Ythier Université de Nice, Faculté des Sciences, 06 108 Nice cedex 2, France. mouze@unice.fr
More informationStability of heavy elements against alpha and cluster radioactivity
CHAPTER III Stability of heavy elements against alpha and cluster radioactivity The stability of heavy and super heavy elements via alpha and cluster decay for the isotopes in the heavy region is discussed
More informationNew Trends in the Nuclear Shell Structure O. Sorlin GANIL Caen
New Trends in the Nuclear Shell Structure O. Sorlin GANIL Caen I. General introduction to the atomic nucleus Charge density, shell gaps, shell occupancies, Nuclear forces, empirical monopoles, additivity,
More informationBody-centred-cubic (BCC) lattice model of nuclear structure
Body-centred-cubic (BCC) lattice model of nuclear structure Gamal A. Nasser Faculty of science, Mansoura University, Egypt. E-mail: chem.gamal@hotmail.com. Abstract: This model is development of solid
More informationFirst results from the AGATA Demonstrator. Francesco Recchia Università di Padova
First results from the AGATA Demonstrator Francesco Recchia Università di Padova XCVII Congresso Nazionale SIF L'Aquila, 26-30 Settembre, 2011 Challenges in Nuclear Structure Shell structure in nuclei
More informationChapter VIII: Nuclear fission
Chapter VIII: Nuclear fission 1 Summary 1. General remarks 2. Spontaneous and induced fissions 3. Nucleus deformation 4. Mass distribution of fragments 5. Number of emitted electrons 6. Radioactive decay
More informationExotic Nuclei II. Neutron-rich nuclides. Michael Thoennessen FRIB/NSCL Michigan State University
Exotic Nuclei II Neutron-rich nuclides Michael Thoennessen FRIB/NSCL Michigan State University Most neutron-rich nuclides N/Z = 1 n X not a nuclide but a nucleon N/Z = 3 8 He 11 Li: N/Z = 2.67 N/Z = 3
More informationPHYSICS CET-2014 MODEL QUESTIONS AND ANSWERS NUCLEAR PHYSICS
PHYSICS CET-2014 MODEL QUESTIONS AND ANSWERS NUCLEAR PHYSICS IMPORTANT FORMULE TO BE REMEMBERED IMPORTANT FORMULE TO BE REMEMBERED 1. Identify the correct statement with regards to nuclear density a) It
More informationPHY492: Nuclear & Particle Physics. Lecture 6 Models of the Nucleus Liquid Drop, Fermi Gas, Shell
PHY492: Nuclear & Particle Physics Lecture 6 Models of the Nucleus Liquid Drop, Fermi Gas, Shell Liquid drop model Five terms (+ means weaker binding) in a prediction of the B.E. r ~A 1/3, Binding is short
More informationChem 481 Lecture Material 1/23/09
Chem 481 Lecture Material 1/23/09 Nature of Radioactive Decay Radiochemistry Nomenclature nuclide - This refers to a nucleus with a specific number of protons and neutrons. The composition of a nuclide
More informationLecture 1. Introduction to Nuclear Science
Lecture 1 Introduction to Nuclear Science Composition of atoms Atoms are composed of electrons and nuclei. The electrons are held in the atom by a Coulomb attraction between the positively charged nucleus
More informationTheoretical basics and modern status of radioactivity studies
Leonid Grigorenko Flerov Laboratory of Nuclear Reactions Joint Institute for Nuclear Research Dubna, Russia Theoretical basics and modern status of radioactivity studies Lecture 2: Radioactivity Coefficients
More informationCHEM 312 Lecture 7: Fission
CHEM 312 Lecture 7: Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics The Probability of Fission Fission Product Distributions
More informationNuclear Physics Questions. 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of?
Nuclear Physics Questions 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of? 2. What is the definition of the atomic number? What is its symbol?
More informationIntroduction to Nuclear Science
Introduction to Nuclear Science PIXIE-PAN Summer Science Program University of Notre Dame 2006 Tony Hyder, Professor of Physics Topics we will discuss Ground-state properties of the nucleus Radioactivity
More informationarxiv: v1 [nucl-th] 24 Oct 2007
February 2, 28 :28 WSPC/INSTRUCTION FILE kazi27d International Journal of Modern Physics E c World Scientific Publishing Company arxiv:71.4411v1 [nucl-th] 24 Oct 27 Cluster radioactivity of isotopes in
More informationExperimental Evidence for Magic Numbers
Experimental Evidence for Magic Numbers Ying CHEN ( L) SupervisorµProf. Jie MENG (Š#) School of Physics, Peking University June 7, 211 CHEN Ying () Experimental Evidence for Magic Numbers June 7, 211 1
More informationCHAPTER I. Introduction. There are 117 elements (Z=1-118) known at present, of which 94 occur naturally on
CHAPTER I Introduction There are 117 elements (Z=1-118) known at present, of which 94 occur naturally on the earth. Eighty elements have stable isotopes, namely all elements with atomic numbers 1 to 82,
More informationc E If photon Mass particle 8-1
Nuclear Force, Structure and Models Readings: Nuclear and Radiochemistry: Chapter 10 (Nuclear Models) Modern Nuclear Chemistry: Chapter 5 (Nuclear Forces) and Chapter 6 (Nuclear Structure) Characterization
More informationLesson 1. Introduction to Nuclear Science
Lesson 1 Introduction to Nuclear Science Introduction to Nuclear Chemistry What is nuclear chemistry? What is the relation of nuclear chemistry to other parts of chemistry? Nuclear chemistry vs nuclear
More informationPart II Particle and Nuclear Physics Examples Sheet 4
Part II Particle and Nuclear Physics Examples Sheet 4 T. Potter Lent/Easter Terms 018 Basic Nuclear Properties 8. (B) The Semi-Empirical mass formula (SEMF) for nuclear masses may be written in the form
More informationEffect of parent and daughter deformation on half-life time in exotic decay
PRAMANA cfl Indian Academy of Sciences Vol. 59, No. 4 journal of October 2002 physics pp. 679 684 Effect of parent and daughter deformation on half-life time in exotic decay K P SANTHOSH 1 and ANTONY JOSEPH
More informationThe Nuclear Many-Body problem. Lecture 3
The Nuclear Many-Body problem Lecture 3 Emergent phenomena at the drip lines. How do properties of nuclei change as we move towards the nuclear driplines? Many-body open quantum systems. Unification of
More informationNuclear Physics. PHY232 Remco Zegers Room W109 cyclotron building.
Nuclear Physics PHY232 Remco Zegers zegers@nscl.msu.edu Room W109 cyclotron building http://www.nscl.msu.edu/~zegers/phy232.html Periodic table of elements We saw that the periodic table of elements can
More informationNuclear Fission Fission discovered by Otto Hahn and Fritz Strassman, Lisa Meitner in 1938
Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics The Probability of Fission Fission Product Distributions Total Kinetic
More informationPre-scission shapes of fissioning nuclei
Pre-scission shapes of fissioning nuclei Micha l Warda Uniwersytet Marii Curie-Sk lodowskiej Lublin, Poland SSNET Workshop Gif-sur-Yvette, 6-11.11.216 Collaboration: J.L. Egido, UAM, Madrid W. Nazarewicz,
More informationNuclear Physics (13 th lecture)
uclear Physics ( th lecture) Cross sections of special neutron-induced reactions UCLR FISSIO Mechanism and characteristics of nuclear fission. o The fission process o Mass distribution of the fragments
More informationIntroduction to Nuclear Science
Introduction to Nuclear Science PAN Summer Science Program University of Notre Dame June, 2014 Tony Hyder Professor of Physics Topics we will discuss Ground-state properties of the nucleus size, shape,
More information8 Nuclei. introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1
8 Nuclei introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1 8.1 - The nucleus The atomic nucleus consists of protons and neutrons. Protons and neutrons are called nucleons. A nucleus is characterized
More informationNuclear Binding Energy
Nuclear Energy Nuclei contain Z number of protons and (A - Z) number of neutrons, with A the number of nucleons (mass number) Isotopes have a common Z and different A The masses of the nucleons and the
More informationHOMEWORK 22-1 (pp )
CHAPTER 22 HOMEWORK 22-1 (pp. 701 702) Define. 1. nucleons 2. nuclide 3. mass defect 4. nuclear binding energy Solve. Use masses of 1.0087 amu for the neutron, 1.00728 amu for the proton, and 5.486 x 10
More informationNucleus. Electron Cloud
Atomic Structure I. Picture of an Atom Nucleus Electron Cloud II. Subatomic particles Particle Symbol Charge Relative Mass (amu) protons p + +1 1.0073 neutrons n 0 1.0087 electrons e - -1 0.00054858 Compare
More informationNJCTL.org 2015 AP Physics 2 Nuclear Physics
AP Physics 2 Questions 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of? 2. What is the definition of the atomic number? What is its symbol?
More informationTesting the shell closure at N=82 via multinucleon transfer reactions at energies around the Coulomb barrier
Testing the shell closure at N=82 via multinucleon transfer reactions at energies around the Coulomb barrier E. Vardaci 1, E. M. Kozulin 2, D. Quero 1, A. Di Nitto 3, A. Karpov 2, L. Calabretta 4, M. Ashaduzzaman
More informationCoefficients and terms of the liquid drop model and mass formula
Coefficients and terms of the liquid drop model and mass formula G. Royer, Christian Gautier To cite this version: G. Royer, Christian Gautier. Coefficients and terms of the liquid drop model and mass
More informationFundamental Forces. Range Carrier Observed? Strength. Gravity Infinite Graviton No. Weak 10-6 Nuclear W+ W- Z Yes (1983)
Fundamental Forces Force Relative Strength Range Carrier Observed? Gravity 10-39 Infinite Graviton No Weak 10-6 Nuclear W+ W- Z Yes (1983) Electromagnetic 10-2 Infinite Photon Yes (1923) Strong 1 Nuclear
More informationRFSS: Lecture 8 Nuclear Force, Structure and Models Part 1 Readings: Nuclear Force Nuclear and Radiochemistry:
RFSS: Lecture 8 Nuclear Force, Structure and Models Part 1 Readings: Nuclear and Radiochemistry: Chapter 10 (Nuclear Models) Modern Nuclear Chemistry: Chapter 5 (Nuclear Forces) and Chapter 6 (Nuclear
More informationLecture 4: Nuclear Energy Generation
Lecture 4: Nuclear Energy Generation Literature: Prialnik chapter 4.1 & 4.2!" 1 a) Some properties of atomic nuclei Let: Z = atomic number = # of protons in nucleus A = atomic mass number = # of nucleons
More informationChemistry 1000 Lecture 3: Nuclear stability. Marc R. Roussel
Chemistry 1000 Lecture 3: Nuclear stability Marc R. Roussel Radioactive decay series Source: Wikimedia commons, http://commons.wikimedia.org/wiki/file: Decay_Chain_Thorium.svg Forces between nucleons Electrostatic
More information1) Radioactive Decay, Nucleosynthesis, and Basic Geochronology
1) Radioactive Decay, Nucleosynthesis, and Basic Geochronology Reading (all from White s Notes) Lecture 1: Introduction And Physics Of The Nucleus: Skim Lecture 1: Radioactive Decay- Read all Lecture 3:
More informationSOURCES of RADIOACTIVITY
Section 9: SOURCES of RADIOACTIVITY This section briefly describes various sources of radioactive nuclei, both naturally occurring and those produced artificially (man-made) in, for example, reactors or
More informationTwo-particle transfer and pairing correlations (for both T-0 and T=1): interplay of reaction mechanism and structure properties
Two-particle transfer and pairing correlations (for both T-0 and T=1): interplay of reaction mechanism and structure properties Andrea Vitturi and Jose Antonio Lay (Padova, Catania, Sevilla) ECT*, September
More informationQuantum mechanics of many-fermion systems
Quantum mechanics of many-fermion systems Kouichi Hagino Tohoku University, Sendai, Japan 1. Identical particles: Fermions and Bosons 2. Simple examples: systems with two identical particles 3. Pauli principle
More informationcapture touching point M.G. Itkis, Perspectives in Nuclear fission Tokai, Japan, March
Nuclear Reaction Mechanism Induced by Heavy Ions MG M.G. Itkis Joint Institute for Nuclear Research, Dubna 5 th ASCR International Workshop Perspectives in Nuclear fission Tokai, Japan, 14 16 16March 212
More informationRADIOACTIVITY. An atom consists of protons, neutrons and electrons.
RADIOACTIVITY An atom consists of protons, neutrons and electrons. - Protons and neutrons are inside the nucleus - Electrons revolve around the nucleus in specific orbits ATOMIC NUMBER: - Total number
More informationTheoretical Nuclear Physics
Theoretical Nuclear Physics (SH2011, Second cycle, 6.0cr) Comments and corrections are welcome! Chong Qi, chongq@kth.se The course contains 12 sections 1-4 Introduction Basic Quantum Mechanics concepts
More informationLecture 3 Radioactivity
Objectives In this lecture you will learn the following We shall begin with a general discussion on the nucleus. Learn about some characteristics of nucleons. Understand some concepts on stability of a
More informationQuantum Theory of Many-Particle Systems, Phys. 540
Quantum Theory of Many-Particle Systems, Phys. 540 IPM? Atoms? Nuclei: more now Other questions about last class? Assignment for next week Wednesday ---> Comments? Nuclear shell structure Ground-state
More informationFusion Barrier of Super-heavy Elements in a Generalized Liquid Drop Model
Commun. Theor. Phys. (Beijing, China) 42 (2004) pp. 594 598 c International Academic Publishers Vol. 42, No. 4, October 15, 2004 Fusion Barrier of Super-heavy Elements in a Generalized Liquid Drop Model
More informationRFSS: Lecture 2 Nuclear Properties
RFSS: Lecture 2 Nuclear Properties Readings: Modern Nuclear Chemistry: Chapter 2 Nuclear Properties Nuclear and Radiochemistry: Chapter 1 Introduction, Chapter 2 Atomic Nuclei Nuclear properties Masses
More informationAtomic Quantum number summary. From last time. Na Optical spectrum. Another possibility: Stimulated emission. How do atomic transitions occur?
From last time Hydrogen atom Multi-electron atoms This week s honors lecture: Prof. Brad Christian, Positron Emission Tomography Course evaluations next week Tues. Prof Montaruli Thurs. Prof. Rzchowski
More informationChapter 10 - Nuclear Physics
The release of atomic energy has not created a new problem. It has merely made more urgent the necessity of solving an existing one. -Albert Einstein David J. Starling Penn State Hazleton PHYS 214 Ernest
More informationRole of multipolarity Six deformation parameter on exotic decay half-lives of Berkelium nucleus
IOSR Journal of Applied Physics (IOSR-JAP) e-issn: 2278-4861, PP 84-91 www.iosrjournals.org Role of multipolarity Six deformation parameter on exotic decay half-lives of Berkelium nucleus G. M. Carmel
More informationSpin Cut-off Parameter of Nuclear Level Density and Effective Moment of Inertia
Commun. Theor. Phys. (Beijing, China) 43 (005) pp. 709 718 c International Academic Publishers Vol. 43, No. 4, April 15, 005 Spin Cut-off Parameter of Nuclear Level Density and Effective Moment of Inertia
More informationChapter 13 Nuclear physics
OCR (A) specifications: 5.4.11i,j,k,l Chapter 13 Nuclear physics Worksheet Worked examples Practical: Simulation (applet) websites nuclear physics End-of-chapter test Marking scheme: Worksheet Marking
More informationLesson 5 The Shell Model
Lesson 5 The Shell Model Why models? Nuclear force not known! What do we know about the nuclear force? (chapter 5) It is an exchange force, mediated by the virtual exchange of gluons or mesons. Electromagnetic
More informationFusion probability and survivability in estimates of heaviest nuclei production R.N. Sagaidak Flerov Laboratory of Nuclear Reactions, JINR, Dubna, RF
Fusion probability and survivability in estimates of heaviest nuclei production R.N. Sagaidak Flerov Laboratory of Nuclear Reactions, JINR, Dubna, RF 1. Fusion probability and survivability as main values
More informationAlpha decay, ssion, and nuclear reactions
Alpha decay, ssion, and nuclear reactions March 11, 2002 1 Energy release in alpha-decay ² Consider a nucleus which is stable against decay by proton or neutron emission { the least bound nucleon still
More informationProduction of new neutron rich heavy and superheavy nuclei
Production of new neutron rich heavy and superheavy nuclei Fusion reactions Elements 119 and 120 are on the way. What s the next? Radioactive ion beams? Multinucleon transfer reactions Shell effects in
More information13 Synthesis of heavier elements. introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1
13 Synthesis of heavier elements introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1 The triple α Reaction When hydrogen fusion ends, the core of a star collapses and the temperature can reach
More informationAtomic Structure. Atomic weight = m protons + m neutrons Atomic number (Z) = # of protons Isotope corresponds to # of neutrons
Atomic Structure Neutrons: neutral Protons: positive charge (1.6x10 19 C, 1.67x10 27 kg) Electrons: negative charge (1.6x10 19 C, 9.11x10 31 kg) Atomic weight = m protons + m neutrons Atomic number (Z)
More informationBasic Nuclear Theory. Lecture 1 The Atom and Nuclear Stability
Basic Nuclear Theory Lecture 1 The Atom and Nuclear Stability Introduction Nuclear power is made possible by energy emitted from either nuclear fission or nuclear fusion. Current nuclear power plants utilize
More informationPHL424: Nuclear fusion
PHL424: Nuclear fusion Hot Fusion 5 10 15 5 10 8 projectiles on target compound nuclei 1 atom Hot fusion (1961 1974) successful up to element 106 (Seaborgium) Coulomb barrier V C between projectile and
More informationSubbarrier cold fusion reactions leading to superheavy elements( )
IL NUOVO CIMENTO VOL. 110 A, N. 9-10 Settembre-Ottobre 1997 Subbarrier cold fusion reactions leading to superheavy elements( ) A. G. POPEKO Flerov Laboratory of Nuclear Reactions, JINR - 141980 Dubna,
More informationSubatomic Particles. proton. neutron. electron. positron. particle. 1 H or 1 p. 4 α or 4 He. 0 e or 0 β
Nuclear Chemistry Subatomic Particles proton neutron 1n 0 1 H or 1 p 1 1 positron electron 0 e or 0 β +1 +1 0 e or 0 β 1 1 particle 4 α or 4 He 2 2 Nuclear Reactions A balanced nuclear equation has the
More informationLaser Spectroscopy on Bunched Radioactive Ion Beams
Laser Spectroscopy on Bunched Radioactive Ion Beams Jon Billowes University of Manchester Balkan School on Nuclear Physics, Bodrum 2004 Lecture 1. 1.1 Nuclear moments 1.2 Hyperfine interaction in free
More informationInstead, the probability to find an electron is given by a 3D standing wave.
Lecture 24-1 The Hydrogen Atom According to the Uncertainty Principle, we cannot know both the position and momentum of any particle precisely at the same time. The electron in a hydrogen atom cannot orbit
More informationFission fragment mass distributions via prompt γ -ray spectroscopy
PRAMANA c Indian Academy of Sciences Vol. 85, No. 3 journal of September 2015 physics pp. 379 384 Fission fragment mass distributions via prompt γ -ray spectroscopy L S DANU, D C BISWAS, B K NAYAK and
More informationAn introduction to Nuclear Physics
An introduction to Nuclear Physics Jorge Pereira pereira@nscl.msu.edu National Superconducting Cyclotron Laboratory Joint Institute for Nuclear Astrophysics The Origin of Everything Layout The Nucleus.
More informationNuclear Reactions A Z. Radioactivity, Spontaneous Decay: Nuclear Reaction, Induced Process: x + X Y + y + Q Q > 0. Exothermic Endothermic
Radioactivity, Spontaneous Decay: Nuclear Reactions A Z 4 P D+ He + Q A 4 Z 2 Q > 0 Nuclear Reaction, Induced Process: x + X Y + y + Q Q = ( m + m m m ) c 2 x X Y y Q > 0 Q < 0 Exothermic Endothermic 2
More informationLecture 4. Magic Numbers
Lecture 4 In last lecture we discussed how one can solve the Schroedinger equation to determine the allowed energies of a particle trapped in a spherically symmetric potential. We will apply these methods
More information5 questions, 3 points each, 15 points total possible. 26 Fe Cu Ni Co Pd Ag Ru 101.
Physical Chemistry II Lab CHEM 4644 spring 2017 final exam KEY 5 questions, 3 points each, 15 points total possible h = 6.626 10-34 J s c = 3.00 10 8 m/s 1 GHz = 10 9 s -1. B= h 8π 2 I ν= 1 2 π k μ 6 P
More informationChapter 37. Nuclear Chemistry. Copyright (c) 2011 by Michael A. Janusa, PhD. All rights reserved.
Chapter 37 Nuclear Chemistry Copyright (c) 2 by Michael A. Janusa, PhD. All rights reserved. 37. Radioactivity Radioactive decay is the process in which a nucleus spontaneously disintegrates, giving off
More information[2] State in what form the energy is released in such a reaction.... [1]
(a) The following nuclear reaction occurs when a slow-moving neutron is absorbed by an isotope of uranium-35. 0n + 35 9 U 4 56 Ba + 9 36Kr + 3 0 n Explain how this reaction is able to produce energy....
More informationIntroductory Nuclear Physics. Glatzmaier and Krumholz 7 Prialnik 4 Pols 6 Clayton 4.1, 4.4
Introductory Nuclear Physics Glatzmaier and Krumholz 7 Prialnik 4 Pols 6 Clayton 4.1, 4.4 Each nucleus is a bound collection of N neutrons and Z protons. The mass number is A = N + Z, the atomic number
More informationarxiv:nucl-th/ v1 24 Nov 2004
LETTER TO THE EDITOR On stability of the neutron rich Oxygen isotopes arxiv:nucl-th/4119v1 24 Nov 24 K.A. Gridnev 1,2, D.K. Gridnev 1,2, V.G. Kartavenko 2,3, V.E. Mitroshin, V.N. Tarasov, D.V. Tarasov
More informationAtomic Structure & Interatomic Bonding
Atomic Structure & Interatomic Bonding Chapter Outline Review of Atomic Structure Atomic Bonding Atomic Structure Atoms are the smallest structural units of all solids, liquids & gases. Atom: The smallest
More informationCorrection to Relativistic Mean Field binding energy and N p N n scheme
arxiv:0808.1945v1 [nucl-th] 14 Aug 2008 Correction to Relativistic Mean Field binding energy and N p N n scheme Madhubrata Bhattacharya and G. Gangopadhyay Department of Physics, University of Calcutta
More informationStability of Cf isotopes against alpha and cluster radioactivity
Stability of 48-54 Cf isotopes against alpha and cluster radioactivity K. P. Santhosh* and R. K. Biju School of Pure and Applied Physics, Kannur University, Swami Anandatheertha Campus, Payyanur 670 37,
More informationThe Periodic Table. Periodic Properties. Can you explain this graph? Valence Electrons. Valence Electrons. Paramagnetism
Periodic Properties Atomic & Ionic Radius Energy Electron Affinity We want to understand the variations in these properties in terms of electron configurations. The Periodic Table Elements in a column
More informationStability of Fm isotopes against alpha and cluster radioactivity
PRAMANA c Indian Academy of Sciences Vol. 73, No. 6 journal of December 2009 physics pp. 1059 1072 Stability of 244 260 Fm isotopes against alpha and cluster radioactivity K P SANTHOSH 1,, R K BIJU and
More informationMicroscopic description of fission in the neutron-deficient Pb region
Microscopic description of fission in the neutron-deficient Pb region Micha l Warda Maria Curie-Sk lodowska University, Lublin, Poland INT Seattle, 1-1-213 Fr 87 At 85 Rn 86 Po 84 Bi 83 Pb 82 Tl 81 Pb
More informationThere are 82 protons in a lead nucleus. Why doesn t the lead nucleus burst apart?
Question 32.1 The Nucleus There are 82 protons in a lead nucleus. Why doesn t the lead nucleus burst apart? a) Coulomb repulsive force doesn t act inside the nucleus b) gravity overpowers the Coulomb repulsive
More informationFundamental Stellar Parameters. Radiative Transfer. Stellar Atmospheres. Equations of Stellar Structure
Fundamental Stellar Parameters Radiative Transfer Stellar Atmospheres Equations of Stellar Structure Nuclear Reactions in Stellar Interiors Binding Energy Coulomb Barrier Penetration Hydrogen Burning Reactions
More informationNuclear Chemistry. Decay Reactions The most common form of nuclear decay reactions are the following:
Nuclear Chemistry Nuclear reactions are transmutation of the one element into another. We can describe nuclear reactions in a similar manner as regular chemical reactions using ideas of stoichiometry,
More informationNuclear Physics 2. D. atomic energy levels. (1) D. scattered back along the original direction. (1)
Name: Date: Nuclear Physics 2. Which of the following gives the correct number of protons and number of neutrons in the nucleus of B? 5 Number of protons Number of neutrons A. 5 6 B. 5 C. 6 5 D. 5 2. The
More informationA New Explanation of Quark Causing Binding Energy between Nucleons in the Nuclide
A New Explanation of Quark Causing Binding Energy between Nucleons in the Nuclide by: Dr. Rasool Javahery Associated Professor, University of Tehran E-mail: rjavaheri@ut.ac.ir Abstract The nuclear binding
More informationChapter 44. Nuclear Structure
Chapter 44 Nuclear Structure Milestones in the Development of Nuclear Physics 1896: the birth of nuclear physics Becquerel discovered radioactivity in uranium compounds Rutherford showed the radiation
More informationPhysics 107: Ideas of Modern Physics
Physics 107: Ideas of Modern Physics Exam 3 Apr. 19, 2006 Name ID # Section # On the Scantron sheet, 1) Fill in your name 2) Fill in your student ID # (not your social security #) 3) Fill in your section
More informationPhysics 107: Ideas of Modern Physics
Physics 107: Ideas of Modern Physics Exam 3 Apr. 19, 2006 Name ID # Section # On the Scantron sheet, 1) Fill in your name 2) Fill in your student ID # (not your social security #) 3) Fill in your section
More informationBeyond mean-field study on collective vibrations and beta-decay
Advanced many-body and statistical methods in mesoscopic systems III September 4 th 8 th, 2017, Busteni, Romania Beyond mean-field study on collective vibrations and beta-decay Yifei Niu Collaborators:
More informationα-decay half-lives for Pb isotopes within Gamow-like model
α-decay half-lives for Pb isotopes within Gamow-like model Dashty T. Akrawy a,b* a Akre Coputer Institute, Ministry of Education, Akre, Kurdistan, Iraq. b Becquereal Institute For Radiation Research and
More informationExperiments with exotic nuclei I. Thursday. Preliminaries Nuclear existence Decay modes beyond the driplines Ground-state half-lives.
Experiments with exotic nuclei I Thursday Preliminaries Nuclear existence Decay modes beyond the driplines Ground-state half-lives Friday Motivation Nuclear structure at extreme N/Z ratios or high A? Changes
More informationSystematic study of heavy cluster emission from Ra isotopes
Systematic study of heavy cluster emission from 10-6 Ra isotopes K. P. Santhosh a, *, Sabina Sahadevan, B. Priyanka and M. S. Unnikrishnan School of Pure and Applied Physics, Kannur University, Payyanur
More informationNuclear Structure from Decay Spectroscopy
Nuclear Structure from Decay Spectroscopy Most nuclei decay. Provides complementary information to reaction studies. Studies can be done at the lowest count rates access furthest from stability. Alpha,
More informationThe Periodic Table of the Elements
The Periodic Table of the Elements All matter is composed of elements. All of the elements are composed of atoms. An atom is the smallest part of an element which still retains the properties of that element.
More information2007 Fall Nuc Med Physics Lectures
2007 Fall Nuc Med Physics Lectures Tuesdays, 9:30am, NN203 Date Title Lecturer 9/4/07 Introduction to Nuclear Physics RS 9/11/07 Decay of radioactivity RS 9/18/07 Interactions with matter RM 9/25/07 Radiation
More informationRadioactivity is the emission of high energy released when the of atoms change. Radioactivity can be or.
Chapter 19 1 RADIOACTIVITY Radioactivity is the emission of high energy released when the of atoms change. Radioactivity can be or. TYPES OF RADIATION OR EMITTED ENERGY IN NUCLEAR CHANGES Radiation is
More informationCorrelation between alpha-decay energies of superheavy nuclei
Correlation between alpha-decay energies of superheavy nuclei J. M. Dong, W. Zuo*, W. Schied, J. Z. Gu Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou,China Institute for Theoretical
More information