Nuclear Physics (10 th lecture)

Size: px
Start display at page:

Download "Nuclear Physics (10 th lecture)"

Transcription

1 ~Theta Nuclear Physics ( th lecture) Content Nuclear Collective Model: Rainwater approx. (reinder) Consequences of nuclear deforation o Rotational states High spin states and back bending o Vibrational states Monopole, dipole and quadrupole vibrations, Giant resonances, experiental observations The nuclear collective odel (contd.) Rainwater approxiation (reinder) Marriage of the liquid drop odel and the shell odel. Concept: nucleus = core + valence nucleon(s) deforable shell odel liquid drop Consequence #: Soe nuclei are defored also in ground state. Consequence #: Nuclear quadrupole oent: Here S is the rigidity of the core, and Q N is the quadrupole oent of the valence nucleon Consequence #: Nilsson-schee of shell-odel levels Better description of (defored) ground-state properties Q ZR U 4 5 r S Q N Further consequences of the core & potential deforation 4) No ore isotropy rotational excitation is possible 5) Deforability vibrational excitation is possible Rotation Classical physics also a sphere can rotate Quantu physics only defored objects can rotate Rotator: I oent of inertia Total angular oentu : J I j valence nucleon J I j Ij (not a rotation!) core rotation Ij, since I is perpendicular to the syetry axis, and j is precessing around it. This eans that: I J j JJ j j For the rotational excitations we have: J J j j In the ground state I =, which gives J = j t a rotational excitation I is increasing, so we get J=j+, j+, J j ~Q (kev) 5,, 5,, 5,, 5,,,5 4,5 J 6,5 8,5 5/ 9/ / 7/,8,7,6,5,4,,,5,5 4,5 5,5 6,5 7,5 8,5 5/ 9/ J / 7/ Sees that slightly J J j j 4 increases (?)

2 For the rotational excitations we have: J J j j For even-even nuclei because of parity conservation only J=j+, j+4, can occur, and of course j= (kev),, 8, 6, 4,,,,, 4, 6, 8,, J This way can be easured! It can also be calculated using the nuclear shape r(r) (deduced fro the quadrupole oent)! z theor r r d r MR y 5 Big surprise:??? eas theor Why does it change (increases) as J gets larger??? x Q? J 5 6 xplanation (age Bohr): Nuclei are superfluid because of the pairing (like Cooper-pairs in superconductors) Rotation: not like a rigid body, but ore like a surface wave Rigid body: v rω rot v ω Superfluid: no friction inside rot v the core stays still, only the surface rotates Fro rot v follows: v grad (velocity potential) Fluid is incopressible: div v Fro all these the velocity potential: Fro B B v grad the velocity field can be deterined. age Bohr 9-9 Nobel-prize 975 yz 7 M d r The rotational energy: M r v d r Fro these two I can be calculated Result: The angular oentu: I r r v wave rigid rigid age Bohr, Ben Mottelson: wave final observed rigid good description, taking into account even the pair-correlation! Nobel-prize 975:. Bohr, Mottelson, Rainwater for the discovery of the connection between collective otion and particle otion in atoic nuclei and the developent of the theory of the structure of the atoic nucleus based on this connection. 8

3 High spin states and back bending Producing high spin states: fusion of heavy ions I rp Since p is big, large angular oentu states can be fored x I ap bands xaple: MeV 6 O + Po 8 U 4 5 Nuclear excitation energy: rot II This is only the rotational energy! The nucleus ay store energy in other fors (e.g. deforation, internal excitation etc.)! 6 Lu 9 Yrast = ost rotating What is the reason? The picture is even ore coplicated Superfluid solid transition g s What is the cause for the transition? Coriolis-force breaks up a nucleon-pair Rotational alignent

4 Vibration It is convenient to give the instantaneous coordinate R(t) of a point on the nuclear surface at (, ) in ters of the spherical haronics λ R(t) R λμ ( t) Yλμ ( θ,φ) λ μ λ Due to reflection syetry λμ λ, = vibration: onopole (GMR observed for >4) (breathing ode of a copressible fluid) 8 MeV = vibration: dipole R(t) R t Y ( θ,φ) R t Y t Y t Y μ μ μ -μ, -, - = vibration: quadrupole R(t) R t Y, 5 t Y R t cos θ R 4 π because = for (using appropriate coord. sys.) (for ellipsoidal shape, R is a function of only ) The shape of the surface can be described by Y, = ±, ±,. In the case of an ellipsoid R = R(θ) hence =. / R t Y R t cos θ π because μ t for μ (, -t t and Y, - Y) J π = +, +, 4 +. Giant dipole resonance (observed for >6) 77 Giant quadrupole resonance (observed for >6) 6 MeV 4 μ μ μ R Y Y / Y Y Y, -, - Quantization of quadrupole vibration is called a quadrupole phonon, J π = +. This ode is doinant. For ost even-even nuclei, a low lying state with J π = + exists and near closed shells second haronic states can be seen MeV = vibration: quadrupole For a haronic oscillation: H v r B d dt / 5 C N N ω; ω B Orthogonal transforation to get a diagonal for: a a a a,,,,, a, μ C μ, Y,, a, Y Coonly new variables are introduced: a, cos, a, The three ain axis (k =,,) of the 5 ellipsoid are then: R k R R cos k 4 sin 5 These two variables can be considered as polar coordinates, thus every shape can be represented by a point in a D surface The case of the two-phonon state There are -vibrations, -vibrations one phonon, two phonon, etc For every single-phonon state J = J = + Because of J J J J we would expect J = +, +, +, +, 4 + J 6 4

5 But consider the quantu nubers: M J = J = M J = 4 J = J = Note: Only non-negative and M values are shown. The table is syetric for M < Only J = +, +, 4 + occurs! xaple: vibrational states in 4 Cd Nuber of phonons N = ω N = N = ω single-phonon state two-phonon states ω ground state 7 8 vibrations: octupole, hexadecupole etc. xperiental evidences for giant resonances Mainly (inelastic) scattering experients Giant dipole resonance (p,p ), (e,e ), (,p) etc. (, ), (d,d ) etc. Octupole (λ = ) odes with J π = can be observed in any nuclei. The collective Hailtonian (for = ) Rotation Vibrational (the ain axis rotate) potential energy kk H B C k the total kinetic energy The energy: coll vibr rot coll n I I 9 Giant Quadrupole (GQR) and Giant Monopole (GMR) resonances Many different vibrational odes have been established also experientally. GQR GMR Morsch, Sükösd et al. Phys Rev. C (98)

Nuclear vibrations and rotations

Nuclear vibrations and rotations Nuclear vibrations and rotations Introduction to Nuclear Science Simon Fraser University Spring 2011 NUCS 342 February 2, 2011 NUCS 342 (Lecture 9) February 2, 2011 1 / 29 Outline 1 Significance of collective

More information

Nuclear models: Collective Nuclear Models (part 2)

Nuclear models: Collective Nuclear Models (part 2) Lecture 4 Nuclear models: Collective Nuclear Models (part 2) WS2012/13: Introduction to Nuclear and Particle Physics,, Part I 1 Reminder : cf. Lecture 3 Collective excitations of nuclei The single-particle

More information

which is the moment of inertia mm -- the center of mass is given by: m11 r m2r 2

which is the moment of inertia mm -- the center of mass is given by: m11 r m2r 2 Chapter 6: The Rigid Rotator * Energy Levels of the Rigid Rotator - this is the odel for icrowave/rotational spectroscopy - a rotating diatoic is odeled as a rigid rotator -- we have two atos with asses

More information

B. PHENOMENOLOGICAL NUCLEAR MODELS

B. PHENOMENOLOGICAL NUCLEAR MODELS B. PHENOMENOLOGICAL NUCLEAR MODELS B.0. Basic concepts of nuclear physics B.0. Binding energy B.03. Liquid drop model B.04. Spherical operators B.05. Bohr-Mottelson model B.06. Intrinsic system of coordinates

More information

p(p,e + ν)d reaction determines the lifetime of the sun

p(p,e + ν)d reaction determines the lifetime of the sun 2013.12.25 Contents Basic properties of nuclear systems Different aspects in different time scales Symmetry breaking in finite time scale Rapidly rotating nuclei Superdeformation and new type of symmetry

More information

Some (more) High(ish)-Spin Nuclear Structure. Lecture 2 Low-energy Collective Modes and Electromagnetic Decays in Nuclei

Some (more) High(ish)-Spin Nuclear Structure. Lecture 2 Low-energy Collective Modes and Electromagnetic Decays in Nuclei Some (more) High(ish)-Spin Nuclear Structure Lecture 2 Low-energy Collective Modes and Electromagnetic Decays in Nuclei Paddy Regan Department of Physics Univesity of Surrey Guildford, UK p.regan@surrey.ac.uk

More information

Some consequences of a Universal Tension arising from Dark Energy for structures from Atomic Nuclei to Galaxy Clusters

Some consequences of a Universal Tension arising from Dark Energy for structures from Atomic Nuclei to Galaxy Clusters unning Head: Universal Tension fro DE Article Type: Original esearch Soe consequences of a Universal Tension arising fro Dark Energy for structures fro Atoic Nuclei to Galaxy Clusters C Sivara Indian Institute

More information

Lecture 8 Symmetries, conserved quantities, and the labeling of states Angular Momentum

Lecture 8 Symmetries, conserved quantities, and the labeling of states Angular Momentum Lecture 8 Syetries, conserved quantities, and the labeling of states Angular Moentu Today s Progra: 1. Syetries and conserved quantities labeling of states. hrenfest Theore the greatest theore of all ties

More information

Lecture #8-3 Oscillations, Simple Harmonic Motion

Lecture #8-3 Oscillations, Simple Harmonic Motion Lecture #8-3 Oscillations Siple Haronic Motion So far we have considered two basic types of otion: translation and rotation. But these are not the only two types of otion we can observe in every day life.

More information

arxiv: v1 [nucl-th] 8 Sep 2011

arxiv: v1 [nucl-th] 8 Sep 2011 Tidal Waves a non-adiabatic microscopic description of the yrast states in near-spherical nuclei S. Frauendorf, Y. Gu, and J. Sun Department of Physics, University of Notre Dame, Notre Dame, IN 6556, USA

More information

13 Harmonic oscillator revisited: Dirac s approach and introduction to Second Quantization

13 Harmonic oscillator revisited: Dirac s approach and introduction to Second Quantization 3 Haronic oscillator revisited: Dirac s approach and introduction to Second Quantization. Dirac cae up with a ore elegant way to solve the haronic oscillator proble. We will now study this approach. The

More information

PHL424: Nuclear surface vibration. Indian Institute of Technology Ropar

PHL424: Nuclear surface vibration. Indian Institute of Technology Ropar PL44: Nuclear surface vibration Systeatics xcitation energy (kev) Ground state Configuration. Spin/parity π ; x kev 4 / nergy ratio: irrors systeatics xcitation energy (kev) 4 Ground state Configuration.

More information

Nuclear Structure (II) Collective models

Nuclear Structure (II) Collective models Nuclear Structure (II) Collective models P. Van Isacker, GANIL, France NSDD Workshop, Trieste, March 2014 TALENT school TALENT (Training in Advanced Low-Energy Nuclear Theory, see http://www.nucleartalent.org).

More information

14. Structure of Nuclei

14. Structure of Nuclei 14. Structure of Nuclei Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 14. Structure of Nuclei 1 In this section... Magic Numbers The Nuclear Shell Model Excited States Dr. Tina Potter 14.

More information

Nuclear Spectroscopy I

Nuclear Spectroscopy I Nuclear Spectroscopy I Augusto O. Macchiavelli Nuclear Science Division Lawrence Berkeley National Laboratory Many thanks to Rod Clark, I.Y. Lee, and Dirk Weisshaar Work supported under contract number

More information

Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation August Introduction to Nuclear Physics - 2

Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation August Introduction to Nuclear Physics - 2 2358-20 Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation 6-17 August 2012 Introduction to Nuclear Physics - 2 P. Van Isacker GANIL, Grand Accelerateur National d'ions Lourds

More information

The 2010 US National Nuclear Physics Summer School and the TRIUMF Summer Institute, NNPSS-TSI June 21 July 02, 2010, Vancouver, BC, Canada

The 2010 US National Nuclear Physics Summer School and the TRIUMF Summer Institute, NNPSS-TSI June 21 July 02, 2010, Vancouver, BC, Canada TU DARMSTADT The 2010 US National Nuclear Physics Summer School and the TRIUMF Summer Institute, NNPSS-TSI June 21 July 02, 2010, Vancouver, BC, Canada Achim Richter ECT* Trento/Italy and TU Darmstadt/Germany

More information

Physics 2210 Fall smartphysics 20 Conservation of Angular Momentum 21 Simple Harmonic Motion 11/23/2015

Physics 2210 Fall smartphysics 20 Conservation of Angular Momentum 21 Simple Harmonic Motion 11/23/2015 Physics 2210 Fall 2015 sartphysics 20 Conservation of Angular Moentu 21 Siple Haronic Motion 11/23/2015 Exa 4: sartphysics units 14-20 Midter Exa 2: Day: Fri Dec. 04, 2015 Tie: regular class tie Section

More information

Collective model. Large quadrupole moments nucleus as a collective

Collective model. Large quadrupole moments nucleus as a collective Collective model Large quadrupole moments nucleus as a collective body (Liquid drop model). Interactions between outer nucleons and closed shells cause permanent deformation. Single-particle state calculated

More information

Department of Physics Preliminary Exam January 3 6, 2006

Department of Physics Preliminary Exam January 3 6, 2006 Departent of Physics Preliinary Exa January 3 6, 2006 Day 1: Classical Mechanics Tuesday, January 3, 2006 9:00 a.. 12:00 p.. Instructions: 1. Write the answer to each question on a separate sheet of paper.

More information

Scattering and bound states

Scattering and bound states Chapter Scattering and bound states In this chapter we give a review of quantu-echanical scattering theory. We focus on the relation between the scattering aplitude of a potential and its bound states

More information

Physics 221B: Solution to HW # 6. 1) Born-Oppenheimer for Coupled Harmonic Oscillators

Physics 221B: Solution to HW # 6. 1) Born-Oppenheimer for Coupled Harmonic Oscillators Physics B: Solution to HW # 6 ) Born-Oppenheier for Coupled Haronic Oscillators This proble is eant to convince you of the validity of the Born-Oppenheier BO) Approxiation through a toy odel of coupled

More information

Theoretical Nuclear Physics

Theoretical 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 information

Methodology of Projection of Wave Functions of. Light Nuclei on Cluster Channels on

Methodology of Projection of Wave Functions of. Light Nuclei on Cluster Channels on Advanced Studies in Theoretical Physics Vol. 0 06 no. 89-97 HIKARI td www.-hikari.co http://dx.doi.org/0.988/astp.06.65 Methodology of Proection of Wave Functions of ight Nuclei on Cluster Channels on

More information

Physics 139B Solutions to Homework Set 3 Fall 2009

Physics 139B Solutions to Homework Set 3 Fall 2009 Physics 139B Solutions to Hoework Set 3 Fall 009 1. Consider a particle of ass attached to a rigid assless rod of fixed length R whose other end is fixed at the origin. The rod is free to rotate about

More information

THE RIGID ROTOR. mrmr= + m K = I. r 2 2. I = m 1. m + m K = Diatomic molecule. m 1 r 1. r 2 m 2. I moment of inertia. (center of mass) COM K.E.

THE RIGID ROTOR. mrmr= + m K = I. r 2 2. I = m 1. m + m K = Diatomic molecule. m 1 r 1. r 2 m 2. I moment of inertia. (center of mass) COM K.E. 5.6 Fall 4 Lecture #7-9 page Diatoic olecule THE RIGID ROTOR r r r r rr= (center of ass) COM r K.E. K = r r K = I ( = r r ) I oent of inertia I = r r = µ r µ = (reduced ass) K = µ r = µv z Prob l e reduced

More information

Krane Enge Cohen Willaims NUCLEAR PROPERTIES 1 Binding energy and stability Semi-empirical mass formula Ch 4

Krane Enge Cohen Willaims NUCLEAR PROPERTIES 1 Binding energy and stability Semi-empirical mass formula Ch 4 Lecture 3 Krane Enge Cohen Willaims NUCLER PROPERTIES 1 Binding energy and stability Semi-empirical mass formula 3.3 4.6 7. Ch 4 Nuclear Spin 3.4 1.5 1.6 8.6 3 Magnetic dipole moment 3.5 1.7 1.6 8.7 4

More information

MOMENT OF INERTIA AND SUPERFLUIDITY

MOMENT OF INERTIA AND SUPERFLUIDITY 1 Chaire Européenne du College de France (004/005) Sandro Stringari Lecture 6 1 Mar 05 MOMENT OF INERTIA AND SUPERFLUIDITY Previous lecture: BEC in low diensions - Theores on long range order. Algebraic

More information

1 Introduction. 2 The hadronic many body problem

1 Introduction. 2 The hadronic many body problem Models Lecture 18 1 Introduction In the next series of lectures we discuss various models, in particluar models that are used to describe strong interaction problems. We introduce this by discussing the

More information

Gamma-ray spectroscopy I

Gamma-ray spectroscopy I Gamma-ray spectroscopy I Andreas Görgen DAPNIA/SPhN, CEA Saclay F-91191 Gif-sur-Yvette France agoergen@cea.fr Lectures presented at the IoP Nuclear Physics Summer School September 4 17, 2005 Chester, UK

More information

Lecture Frontier of complexity more is different Think of a spin - a multitude gives all sorts of magnetism due to interactions

Lecture Frontier of complexity more is different Think of a spin - a multitude gives all sorts of magnetism due to interactions Lecture 1 Motivation for course The title of this course is condensed atter physics which includes solids and liquids (and occasionally gases). There are also interediate fors of atter, e.g., glasses,

More information

(a) As a reminder, the classical definition of angular momentum is: l = r p

(a) As a reminder, the classical definition of angular momentum is: l = r p PHYSICS T8: Standard Model Midter Exa Solution Key (216) 1. [2 points] Short Answer ( points each) (a) As a reinder, the classical definition of angular oentu is: l r p Based on this, what are the units

More information

ROTATIONAL MOTION FROM TRANSLATIONAL MOTION

ROTATIONAL MOTION FROM TRANSLATIONAL MOTION ROTATIONAL MOTION FROM TRANSLATIONAL MOTION Velocity Acceleration 1-D otion 3-D otion Linear oentu TO We have shown that, the translational otion of a acroscopic object is equivalent to the translational

More information

Nuclear structure theory

Nuclear structure theory Nuclear structure theory Thomas Papenbrock and Lecture 2: Traditional shell model National Nuclear Physics Summer School 2008 George Washington University Shell structure in nuclei Mass differences: Liquid

More information

Shape Coexistence and Band Termination in Doubly Magic Nucleus 40 Ca

Shape Coexistence and Band Termination in Doubly Magic Nucleus 40 Ca Commun. Theor. Phys. (Beijing, China) 43 (2005) pp. 509 514 c International Academic Publishers Vol. 43, No. 3, March 15, 2005 Shape Coexistence and Band Termination in Doubly Magic Nucleus 40 Ca DONG

More information

RFSS: 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 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 information

PHYSICS 110A : CLASSICAL MECHANICS MIDTERM EXAM #2

PHYSICS 110A : CLASSICAL MECHANICS MIDTERM EXAM #2 PHYSICS 110A : CLASSICAL MECHANICS MIDTERM EXAM #2 [1] Two blocks connected by a spring of spring constant k are free to slide frictionlessly along a horizontal surface, as shown in Fig. 1. The unstretched

More information

Feshbach Resonances in Ultracold Gases

Feshbach Resonances in Ultracold Gases Feshbach Resonances in Ultracold Gases Sara L. Capbell MIT Departent of Physics Dated: May 5, 9) First described by Heran Feshbach in a 958 paper, Feshbach resonances describe resonant scattering between

More information

1 (40) Gravitational Systems Two heavy spherical (radius 0.05R) objects are located at fixed positions along

1 (40) Gravitational Systems Two heavy spherical (radius 0.05R) objects are located at fixed positions along (40) Gravitational Systes Two heavy spherical (radius 0.05) objects are located at fixed positions along 2M 2M 0 an axis in space. The first ass is centered at r = 0 and has a ass of 2M. The second ass

More information

Design and Experimental Research of Atomizer Based on Micro Abrasive Ultrasonic Polishing Bang-fu WANG, Yin ZHEN, Juan SONG and A-chun ZHU

Design and Experimental Research of Atomizer Based on Micro Abrasive Ultrasonic Polishing Bang-fu WANG, Yin ZHEN, Juan SONG and A-chun ZHU 217 3rd International Conference on Applied Mechanics and Mechanical Autoation (AMMA 217) ISBN: 978-1-6595-479- Design and Experiental Research of Atoizer Based on Micro Abrasive Ultrasonic Polishing Bang-fu

More information

Lecture 4: Nuclear Energy Generation

Lecture 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 information

Yields of Possible Ternary Fission Channels of 260 No in Collinear Configuration

Yields of Possible Ternary Fission Channels of 260 No in Collinear Configuration Arab Journal of Nuclear Science and Applications, (), (319-33) 017 Yields of Possible Ternary Fission Channels of 60 No in Configuration M. M. Botros and A. S. Hashe Departent of Physics, Faculty of Science,

More information

Nuclear Shell Model. 1d 3/2 2s 1/2 1d 5/2. 1p 1/2 1p 3/2. 1s 1/2. configuration 1 configuration 2

Nuclear Shell Model. 1d 3/2 2s 1/2 1d 5/2. 1p 1/2 1p 3/2. 1s 1/2. configuration 1 configuration 2 Nuclear Shell Model 1d 3/2 2s 1/2 1d 5/2 1d 3/2 2s 1/2 1d 5/2 1p 1/2 1p 3/2 1p 1/2 1p 3/2 1s 1/2 1s 1/2 configuration 1 configuration 2 Nuclear Shell Model MeV 5.02 3/2-2 + 1p 1/2 1p 3/2 4.44 5/2-1s 1/2

More information

Physics 106a, Caltech 4 December, Lecture 18: Examples on Rigid Body Dynamics. Rotating rectangle. Heavy symmetric top

Physics 106a, Caltech 4 December, Lecture 18: Examples on Rigid Body Dynamics. Rotating rectangle. Heavy symmetric top Physics 106a, Caltech 4 December, 2018 Lecture 18: Examples on Rigid Body Dynamics I go through a number of examples illustrating the methods of solving rigid body dynamics. In most cases, the problem

More information

Reassessing the Vibrational Nuclear Structure of 112 Cd

Reassessing the Vibrational Nuclear Structure of 112 Cd Reassessing the Vibrational Nuclear Structure of 112 Cd February 212 1 Vibrational Nuclear Structure Nuclear Vibrations in the Collective Model Vibrational Structure of the 112 Cd Sources of Inconsistency

More information

= T. Oscillations and Waves. Example of an Oscillating System IB 12 IB 12

= T. Oscillations and Waves. Example of an Oscillating System IB 12 IB 12 Oscillation: the vibration of an object Oscillations and Waves Eaple of an Oscillating Syste A ass oscillates on a horizontal spring without friction as shown below. At each position, analyze its displaceent,

More information

FIGURE 1. Excitation energy versus angular-momentum plot of the yrast structure of 32 S calculated with the Skyrme III interaction. Density distributi

FIGURE 1. Excitation energy versus angular-momentum plot of the yrast structure of 32 S calculated with the Skyrme III interaction. Density distributi KUNS1529 Exotic Shapes in 32 S suggested by the Symmetry-Unrestricted Cranked Hartree-Fock Calculations 1 Masayuki Yamagami and Kenichi Matsuyanagi Department of Physics, Graduate School of Science, Kyoto

More information

Phys463.nb. Many electrons in 1D at T = 0. For a large system (L ), ΕF =? (6.7) The solutions of this equation are plane waves (6.

Phys463.nb. Many electrons in 1D at T = 0. For a large system (L ), ΕF =? (6.7) The solutions of this equation are plane waves (6. â â x Ψn Hx Ε Ψn Hx 35 (6.7) he solutions of this equation are plane waves Ψn Hx A exphä n x (6.8) he eigen-energy Εn is n (6.9) Εn For a D syste with length and periodic boundary conditions, Ψn Hx Ψn

More information

Lecture 4: Nuclear Structure 2 Independent vs collective models Collective Model Rotation Vibration Coupled excitations Nilsson model

Lecture 4: Nuclear Structure 2 Independent vs collective models Collective Model Rotation Vibration Coupled excitations Nilsson model Lecture 4: Nuclear Structure 2 Independent vs collective models Collective Model Rotation Vibration Coupled excitations Nilsson model Lecture 4: Ohio University PHYS7501, Fall 2017, Z. Meisel (meisel@ohio.edu)

More information

On the summations involving Wigner rotation matrix elements

On the summations involving Wigner rotation matrix elements Journal of Matheatical Cheistry 24 (1998 123 132 123 On the suations involving Wigner rotation atrix eleents Shan-Tao Lai a, Pancracio Palting b, Ying-Nan Chiu b and Harris J. Silverstone c a Vitreous

More information

P (t) = P (t = 0) + F t Conclusion: If we wait long enough, the velocity of an electron will diverge, which is obviously impossible and wrong.

P (t) = P (t = 0) + F t Conclusion: If we wait long enough, the velocity of an electron will diverge, which is obviously impossible and wrong. 4 Phys520.nb 2 Drude theory ~ Chapter in textbook 2.. The relaxation tie approxiation Here we treat electrons as a free ideal gas (classical) 2... Totally ignore interactions/scatterings Under a static

More information

Lecture contents. Magnetic properties Diamagnetism Band paramagnetism Atomic paramagnetism. NNSE508 / NENG452 Lecture #14

Lecture contents. Magnetic properties Diamagnetism Band paramagnetism Atomic paramagnetism. NNSE508 / NENG452 Lecture #14 1 Lecture contents agnetic properties Diaagnetis and paraagnetis Atoic paraagnetis NNSE58 / NENG45 Lecture #14 agnetic units H /r V s 1 Wb T 1 T Wb T 1H A A Fro Treolet de Lacheisserie, 5 NNSE58 / NENG45

More information

Dispersion. February 12, 2014

Dispersion. February 12, 2014 Dispersion February 1, 014 In aterials, the dielectric constant and pereability are actually frequency dependent. This does not affect our results for single frequency odes, but when we have a superposition

More information

The semi-empirical mass formula, based on the liquid drop model, compared to the data

The semi-empirical mass formula, based on the liquid drop model, compared to the data Nucleonic Shells The semi-empirical mass formula, based on the liquid drop model, compared to the data E shell = E total E LD (Z=82, N=126) (Z=28, N=50) Nature 449, 411 (2007) Magic numbers at Z or N=

More information

In the session you will be divided into groups and perform four separate experiments:

In the session you will be divided into groups and perform four separate experiments: Mechanics Lab (Civil Engineers) Nae (please print): Tutor (please print): Lab group: Date of lab: Experients In the session you will be divided into groups and perfor four separate experients: (1) air-track

More information

Antimagnetic Rotation in Cd isotopes

Antimagnetic Rotation in Cd isotopes Proceedings of the DAE Symp. on Nucl. Phys. 56 (2011) 3 Antimagnetic Rotation in Cd isotopes S.Chattopadhyay,* and S. Roy Saha Institute of Nuclear Physics, Kolkata - 700064, INDIA. * email: Sukalyan.chattopadhyay@saha.ac.in

More information

CHAPTER 15: Vibratory Motion

CHAPTER 15: Vibratory Motion CHAPTER 15: Vibratory Motion courtesy of Richard White courtesy of Richard White 2.) 1.) Two glaring observations can be ade fro the graphic on the previous slide: 1.) The PROJECTION of a point on a circle

More information

c E If photon Mass particle 8-1

c 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 information

The Hydrogen Atom. Nucleus charge +Ze mass m 1 coordinates x 1, y 1, z 1. Electron charge e mass m 2 coordinates x 2, y 2, z 2

The Hydrogen Atom. Nucleus charge +Ze mass m 1 coordinates x 1, y 1, z 1. Electron charge e mass m 2 coordinates x 2, y 2, z 2 The Hydrogen Ato The only ato that can be solved exactly. The results becoe the basis for understanding all other atos and olecules. Orbital Angular Moentu Spherical Haronics Nucleus charge +Ze ass coordinates

More information

Hee = ~ dxdy\jj+ (x) 'IJ+ (y) u (x- y) \jj (y) \jj (x), V, = ~ dx 'IJ+ (x) \jj (x) V (x), Hii = Z 2 ~ dx dy cp+ (x) cp+ (y) u (x- y) cp (y) cp (x),

Hee = ~ dxdy\jj+ (x) 'IJ+ (y) u (x- y) \jj (y) \jj (x), V, = ~ dx 'IJ+ (x) \jj (x) V (x), Hii = Z 2 ~ dx dy cp+ (x) cp+ (y) u (x- y) cp (y) cp (x), SOVIET PHYSICS JETP VOLUME 14, NUMBER 4 APRIL, 1962 SHIFT OF ATOMIC ENERGY LEVELS IN A PLASMA L. E. PARGAMANIK Khar'kov State University Subitted to JETP editor February 16, 1961; resubitted June 19, 1961

More information

Angular Momentum Properties

Angular Momentum Properties Cheistry 460 Fall 017 Dr. Jean M. Standard October 30, 017 Angular Moentu Properties Classical Definition of Angular Moentu In classical echanics, the angular oentu vector L is defined as L = r p, (1)

More information

Transverse wobbling. F. Dönau 1 and S. Frauendorf 2 1 XXX 2 Department of Physics, University of Notre Dame, South Bend, Indiana 46556

Transverse wobbling. F. Dönau 1 and S. Frauendorf 2 1 XXX 2 Department of Physics, University of Notre Dame, South Bend, Indiana 46556 Transverse wobbling F. Dönau and S. Frauendorf XXX Department of Physics, University of Notre Dame, South Bend, Indiana 46556 PACS numbers:..re, 3..Lv, 7.7.+q II. I. INTRODUCTION TRANSVERSE AND LONGITUDINAL

More information

12 Towards hydrodynamic equations J Nonlinear Dynamics II: Continuum Systems Lecture 12 Spring 2015

12 Towards hydrodynamic equations J Nonlinear Dynamics II: Continuum Systems Lecture 12 Spring 2015 18.354J Nonlinear Dynaics II: Continuu Systes Lecture 12 Spring 2015 12 Towards hydrodynaic equations The previous classes focussed on the continuu description of static (tie-independent) elastic systes.

More information

13. Basic Nuclear Properties

13. Basic Nuclear Properties 13. Basic Nuclear Properties Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 13. Basic Nuclear Properties 1 In this section... Motivation for study The strong nuclear force Stable nuclei Binding

More information

Rotations and vibrations of polyatomic molecules

Rotations and vibrations of polyatomic molecules Rotations and vibrations of polyatomic molecules When the potential energy surface V( R 1, R 2,..., R N ) is known we can compute the energy levels of the molecule. These levels can be an effect of: Rotation

More information

Lecture 12: Waves in periodic structures

Lecture 12: Waves in periodic structures Lecture : Waves in periodic structures Phonons: quantised lattice vibrations of a crystalline solid is: To approach the general topic of waves in periodic structures fro a specific standpoint: Lattice

More information

Classical systems in equilibrium

Classical systems in equilibrium 35 Classical systes in equilibriu Ideal gas Distinguishable particles Here we assue that every particle can be labeled by an index i... and distinguished fro any other particle by its label if not by any

More information

Stern-Gerlach Experiment

Stern-Gerlach Experiment Stern-Gerlach Experient HOE: The Physics of Bruce Harvey This is the experient that is said to prove that the electron has an intrinsic agnetic oent. Hydrogen like atos are projected in a bea through a

More information

Spinning Disk and Chladni Plates

Spinning Disk and Chladni Plates Spinning Disk and Chladni Plates Subitted By MD MARUFUR RAHMAN Msc Sustainable Energy Systes Beng(Hons) Mechanical Engineering Bsc Coputer Science and Engineering Table of Contents Spinning Disk... 3 1.0

More information

Evolution Of Shell Structure, Shapes & Collective Modes. Dario Vretenar

Evolution Of Shell Structure, Shapes & Collective Modes. Dario Vretenar Evolution Of Shell Structure, Shapes & Collective Modes Dario Vretenar vretenar@phy.hr 1. Evolution of shell structure with N and Z A. Modification of the effective single-nucleon potential Relativistic

More information

Nucleon Pair Approximation to the nuclear Shell Model

Nucleon Pair Approximation to the nuclear Shell Model Nucleon Pair Approximation to the nuclear Shell Model Yiyuan Cheng Department of Physics and Astronomy, Shanghai Jiao Tong University, China RCNP, Osaka university, Japan Collaborators: Yu-Min Zhao, Akito

More information

Moment of inertia and torsional vibrations (Item No.: P )

Moment of inertia and torsional vibrations (Item No.: P ) Moent of inertia and torsional vibrations (Ite No.: P2133100) Curricular Relevance Area of Expertise: Physics Education Level: University Topic: Mechanics Subtopic: Static Equilibriu and Elasticity Experient:

More information

The interacting boson model

The interacting boson model The interacting boson model P. Van Isacker, GANIL, France Introduction to the IBM Practical applications of the IBM Overview of nuclear models Ab initio methods: Description of nuclei starting from the

More information

Question number 1 to 8 carries 2 marks each, 9 to 16 carries 4 marks each and 17 to 18 carries 6 marks each.

Question number 1 to 8 carries 2 marks each, 9 to 16 carries 4 marks each and 17 to 18 carries 6 marks each. IIT-JEE5-PH-1 FIITJEE Solutions to IITJEE 5 Mains Paper Tie: hours Physics Note: Question nuber 1 to 8 carries arks each, 9 to 16 carries 4 arks each and 17 to 18 carries 6 arks each. Q1. whistling train

More information

WYSE Academic Challenge Sectional Physics 2006 Solution Set

WYSE Academic Challenge Sectional Physics 2006 Solution Set WYSE Acadeic Challenge Sectional Physics 6 Solution Set. Correct answer: d. Using Newton s nd Law: r r F 6.N a.kg 6./s.. Correct answer: c. 6. sin θ 98. 3. Correct answer: b. o 37.8 98. N 6. N Using Newton

More information

which proves the motion is simple harmonic. Now A = a 2 + b 2 = =

which proves the motion is simple harmonic. Now A = a 2 + b 2 = = Worked out Exaples. The potential energy function for the force between two atos in a diatoic olecules can be expressed as follows: a U(x) = b x / x6 where a and b are positive constants and x is the distance

More information

Overview of Nuclear Structure and Excitations

Overview of Nuclear Structure and Excitations Overview of Nuclear Structure and Excitations MAJOR FEATURES OF OUR SUN -the 3rd lecture- SS Jyvaskyla August 06-12, 2014 T= ~10 7 K at the core = ~1 kev Yoshitaka Fujita Osaka University Layer Structure

More information

The Nuclear Many-Body Problem. Lecture 2

The Nuclear Many-Body Problem. Lecture 2 The Nuclear Many-Body Problem Lecture 2 How do we describe nuclei? Shell structure in nuclei and the phenomenological shell model approach to nuclear structure. Ab-initio approach to nuclear structure.

More information

Reading from Young & Freedman: For this topic, read the introduction to chapter 25 and sections 25.1 to 25.3 & 25.6.

Reading from Young & Freedman: For this topic, read the introduction to chapter 25 and sections 25.1 to 25.3 & 25.6. PHY10 Electricity Topic 6 (Lectures 9 & 10) Electric Current and Resistance n this topic, we will cover: 1) Current in a conductor ) Resistivity 3) Resistance 4) Oh s Law 5) The Drude Model of conduction

More information

5.2. Example: Landau levels and quantum Hall effect

5.2. Example: Landau levels and quantum Hall effect 68 Phs460.nb i ħ (-i ħ -q A') -q φ' ψ' = + V(r) ψ' (5.49) t i.e., using the new gauge, the Schrodinger equation takes eactl the sae for (i.e. the phsics law reains the sae). 5.. Eaple: Lau levels quantu

More information

Mechanics Physics 151

Mechanics Physics 151 Mechanics Physics 5 Lecture Oscillations (Chapter 6) What We Did Last Tie Analyzed the otion of a heavy top Reduced into -diensional proble of θ Qualitative behavior Precession + nutation Initial condition

More information

Giant Resonances in Argon Isotopes

Giant Resonances in Argon Isotopes Giant Resonances in Argon Isotopes A Thesis Presented for the Master of Science Degree The University of Tennessee, Knoxville William George Newton December 2002 Acknowledgments Firstly, I would like to

More information

All you need to know about QM for this course

All you need to know about QM for this course Introduction to Eleentary Particle Physics. Note 04 Page 1 of 9 All you need to know about QM for this course Ψ(q) State of particles is described by a coplex contiguous wave function Ψ(q) of soe coordinates

More information

Model-independent description of nuclear rotation in an effective theory

Model-independent description of nuclear rotation in an effective theory Model-independent description of nuclear rotation in an effective theory Thomas Papenbrock and University of Aizu-JUSTIPEN-EFES Symposium on "Cutting-Edge Physics of Unstable Nuclei Aizu, November 10-13,

More information

Symmetries and collective Nuclear excitations PRESENT AND FUTURE EXOTICS IN NUCLEAR PHYSICS In honor of Geirr Sletten at his 70 th birthday

Symmetries and collective Nuclear excitations PRESENT AND FUTURE EXOTICS IN NUCLEAR PHYSICS In honor of Geirr Sletten at his 70 th birthday Symmetries and collective Nuclear excitations PRESENT AND FUTURE EXOTICS IN NUCLEAR PYSICS In honor of Geirr Sletten at his 70 th birthday Stefan Frauendorf, Y. Gu, Daniel Almehed Department of Physics

More information

The calculation method of interaction between metal atoms under influence of the radiation

The calculation method of interaction between metal atoms under influence of the radiation IOP Conference Series: Materials Science and Engineering PAPER OPEN ACCESS The calculation ethod of interaction between etal atos under influence of the radiation To cite this article: S N Yanin 015 IOP

More information

P235 Midterm Examination Prof. Cline

P235 Midterm Examination Prof. Cline P235 Mier Exaination Prof. Cline THIS IS A CLOSED BOOK EXAMINATION. Do all parts of all four questions. Show all steps to get full credit. 7:00-10.00p, 30 October 2009 1:(20pts) Consider a rocket fired

More information

Tutorial Exercises: Incorporating constraints

Tutorial Exercises: Incorporating constraints Tutorial Exercises: Incorporating constraints 1. A siple pendulu of length l ass is suspended fro a pivot of ass M that is free to slide on a frictionless wire frae in the shape of a parabola y = ax. The

More information

Department of mechanics, Faculty of engineering Hamadan branch, Islamic azad university, Hamadan, Iran. Abstract

Department of mechanics, Faculty of engineering Hamadan branch, Islamic azad university, Hamadan, Iran. Abstract 194 Ciência enatura, Santa Maria, v. 37 Part 1 015, p. 194 198 ISSN ipressa: 0100-8307 ISSN on-line: 179-460X Vibration Siulation of the cylindrical reservoir shell containing fluid vortex with the help

More information

PHY 171. Lecture 14. (February 16, 2012)

PHY 171. Lecture 14. (February 16, 2012) PHY 171 Lecture 14 (February 16, 212) In the last lecture, we looked at a quantitative connection between acroscopic and icroscopic quantities by deriving an expression for pressure based on the assuptions

More information

Time Evolution of Matter States

Time Evolution of Matter States Tie Evolution of Matter States W. M. Hetherington February 15, 1 The Tie-Evolution Operat The tie-evolution of a wavefunction is deterined by the effect of a tie evolution operat through the relation Ψ

More information

RFSS: Lecture 6 Gamma Decay

RFSS: Lecture 6 Gamma Decay RFSS: Lecture 6 Gamma Decay Readings: Modern Nuclear Chemistry, Chap. 9; Nuclear and Radiochemistry, Chapter 3 Energetics Decay Types Transition Probabilities Internal Conversion Angular Correlations Moessbauer

More information

High Spin States in Nuclei: Exotic Quantal Rotation III. Umesh Garg. University of Notre Dame. Supported in part by the National Science Foundation

High Spin States in Nuclei: Exotic Quantal Rotation III. Umesh Garg. University of Notre Dame. Supported in part by the National Science Foundation High Spin States in Nuclei: Exotic Quantal Rotation III Umesh Garg University of Notre Dame Supported in part by the National Science Foundation CNSSS17 August 23-29, 2017 u normal collective rotation

More information

NERS 311 Current Old notes notes Chapter Chapter 1: Introduction to the course 1 - Chapter 1.1: About the course 2 - Chapter 1.

NERS 311 Current Old notes notes Chapter Chapter 1: Introduction to the course 1 - Chapter 1.1: About the course 2 - Chapter 1. NERS311/Fall 2014 Revision: August 27, 2014 Index to the Lecture notes Alex Bielajew, 2927 Cooley, bielajew@umich.edu NERS 311 Current Old notes notes Chapter 1 1 1 Chapter 1: Introduction to the course

More information

Problem T1. Main sequence stars (11 points)

Problem T1. Main sequence stars (11 points) Proble T1. Main sequence stars 11 points Part. Lifetie of Sun points i..7 pts Since the Sun behaves as a perfectly black body it s total radiation power can be expressed fro the Stefan- Boltzann law as

More information

Four-vector, Dirac spinor representation and Lorentz Transformations

Four-vector, Dirac spinor representation and Lorentz Transformations Available online at www.pelagiaresearchlibrary.co Advances in Applied Science Research, 2012, 3 (2):749-756 Four-vector, Dirac spinor representation and Lorentz Transforations S. B. Khasare 1, J. N. Rateke

More information

PY241 Solutions Set 9 (Dated: November 7, 2002)

PY241 Solutions Set 9 (Dated: November 7, 2002) PY241 Solutions Set 9 (Dated: Noveber 7, 2002) 9-9 At what displaceent of an object undergoing siple haronic otion is the agnitude greatest for the... (a) velocity? The velocity is greatest at x = 0, the

More information

Introduction to Robotics (CS223A) (Winter 2006/2007) Homework #5 solutions

Introduction to Robotics (CS223A) (Winter 2006/2007) Homework #5 solutions Introduction to Robotics (CS3A) Handout (Winter 6/7) Hoework #5 solutions. (a) Derive a forula that transfors an inertia tensor given in soe frae {C} into a new frae {A}. The frae {A} can differ fro frae

More information

The interacting boson model

The interacting boson model The interacting boson model P. Van Isacker, GANIL, France Dynamical symmetries of the IBM Neutrons, protons and F-spin (IBM-2) T=0 and T=1 bosons: IBM-3 and IBM-4 The interacting boson model Nuclear collective

More information

Alpha decay. Introduction to Nuclear Science. Simon Fraser University Spring NUCS 342 February 21, 2011

Alpha decay. Introduction to Nuclear Science. Simon Fraser University Spring NUCS 342 February 21, 2011 Alpha decay Introduction to Nuclear Science Simon Fraser University Spring 2011 NUCS 342 February 21, 2011 NUCS 342 (Lecture 13) February 21, 2011 1 / 27 Outline 1 The Geiger-Nuttall law NUCS 342 (Lecture

More information