Nuclear models: Shell model

Size: px
Start display at page:

Download "Nuclear models: Shell model"

Transcription

1 Lectue 3 Nuclea models: Shell model WS0/3: Intoduction to Nuclea and Paticle Physics,, Pat I

2 Nuclea models Nuclea models Models with stong inteaction between the nucleons Liquid dop model α-paticle model Shell model Models of non-inteacting nucleons Femi gas model Optical model Nucleons inteact with the neaest neighbos and pactically don t move: mean fee path λ << R A nuclea adius Nucleons move feely inside the nucleus: mean fee path λ ~ R A nuclea adius

3 III. Shell model 3

4 Shell model Magic numbes: Nuclides with cetain poton and/o neuton numbes ae found to be exceptionally stable. These so-called magic numbes ae The doubly magic nuclei:, 8, 0, 8, 50, 8, 6 Nuclei with magic poton o neuton numbe have an unusually lage numbe of stable o long lived nuclides. A nucleus with a magic neuton (poton) numbe equies a lot of enegy to sepaate a neuton (poton) fom it. A nucleus with one moe neuton (poton) than a magic numbe is vey easy to sepaate. The fist exitation level is vey high: a lot of enegy is needed to excite such nuclei The doubly magic nuclei have a spheical fom Nucleons ae aanged into complete shells within the atomic nucleus 4

5 Excitation enegy fo magicm nuclei 5

6 Nuclea potential The enegy spectum is defined by the nuclea potential solution of Schödinge equation fo a ealistic potential The nuclea foce is vey shot-anged => the fom of the potential follows the density distibution of the nucleons within the nucleus: fo vey light nuclei (A < 7), the nucleon distibution has Gaussian fom (coesponding to a hamonic oscillato potential) fo heavie nuclei it can be paameteised by a Femi distibution. The latte coesponds to the Woods-Saxon potential e.g. 3) appoximation by the ) Woods-Saxon potential: U U( ) = ectangula potential well with infinite baie enegy : a=0 a>0 + 0 R a e ) a 0: appoximation by the ectangula potential well : U( ) = U 0, 0, < R R U() 0 U( ) = 0,, < R R R 6

7 Schödinge equation Schödinge equation: Single-paticle Hamiltonian opeato: = + sin θ ĤΨ = EΨ H ˆ = h + U( ) M Eigenstates: Ψ() - wave function Eigenvalues: E - enegy U() is a nuclea potential spheically symmetic θ sin θ ϕ ( sinθ ) + () () Conside U() - ectangula potential well with infinite baie enegy U( ) = 0,, < R R Angula pat: ˆ λ = sin θ θ h ˆ λ = L ˆ sin θ ϕ ( sinθ ) + L opeato fo the obital angula momentum = Lˆ h ( θ, ϕ) = h l( l + ) Υ ( θ, ϕ) ˆ Υlm L lm (3) Eigenstates: Y lm spheical hamonics 7

8 Radial pat The wave function of the paticles in the nuclea potential can be decomposed into two pats: a adial one Ψ (), which only depends on the adius, and an angula pat Y lm (θ,ϕ) which only depends on the oientation (this decomposition is possible fo all spheically symmetic potentials): Fom (4) and () => h M Ψ ( θ, ϕ) = Ψ ( ) Υ ( θ, ϕ), lm + => eq. fo the adial pat: ˆ L M Ψ h l( l + ) M + h M ( ) Υ ( θ, ϕ) = E Ψ ( ) Υ ( θ, ϕ) Ψ lm ( ) = E Ψ ( ) lm (4) (5) Substitute in (5): Ψ ( ) = R( ) h M d R( d ) + h l( l + ) R( M ) = E R( ) (6) 8

9 Constaints on E Eq. fo the adial pat: h d R( ) h l( l + ) + E ( ) = 0 (7) R M d M Fom (7) ) Enegy eigenvalues fo obital angula momentum l: E: l=0 s l= p states l= d l=3 f ) Fo each l: -l < m < l => (l+) pojections m of angula momentum. The enegy is independent of the m quantum numbe, which can be any intege value between ± l. Since nucleons also have two possible spin diections, this means that the l levels ae (l+) times degeneate if a spin-obit inteaction is neglected. 3) The paity of the wave function is fixed by the spheical wave function Y ml and ˆ l P Ψ, θ, ϕ = P Ψ ( ) Υ θ, ϕ = ( ) Ψ ( ) Υ θ, ϕ eads ( ) l : ( ) ( ) ( ) lm lm s,d,.. - even states; p,f, - odd states 9

10 Main quantum numbe n Eq. fo the adial pat: h M d R( ) h l( l + ) + E ( ) = 0 R d M Solution of diffeential eq: R( ) ( ) + λ( ) R( ) = 0 Spheical Bessel functions j l (x): Ψ A R The wave function: (7) ( θ, ϕ) = j l ( k) Υ ( θ, ϕ), lm A ) = j ( k ) ME k = h ( l U() Bounday condition fo the suface, i.e. at =R: Ψ(R,θ,ϕ) =0 0 R estictions on k in Bessel functions: j l ( kr) = 0 main quantum numbe n coesponds to nodes of the Bessel function : X nl ME h kr = Xnl k R = Xnl R = X nl (8) 0

11 Shell model with ectangula potential well Thus, accoding to Eq. (8) : Xnl h Enl = E nl = Const X nl (9) MR Nodes of Bessel function Enegy states ae quantized stuctue of enegy states E nl l = 0 n = n = n = 3 l = n = n = l = n = l = 3 n = l = 4 n = s states X X X = 3.4 = 6.8 = 9.4 p states X X X = 4.49 = 7.7 d states f X 3 = 5.76 states 4 = 6.99 g states X = 8. j j j j j state s p d s f p g E E E E E E E nl s p d s f p E g = C X nl = C 9.86 = C 0. = C 33. = C 39.5 = C 48.8 = C 59.7 = C 64 degeneacy (l+),l=0 (l+),l= states with E Fist 3 magic numbes ae epoduced, highe not!, 8, 0, 8, 50, 8, 6 Note: this esult coesponds to fo U() = ectangula potential well with infinite baie enegy E nl

12 Shell model with Woods-Saxon potential Woods-Saxon potential: U( ) = + U 0 R a e The fist thee magic numbes (, 8 and 0) can then be undestood as nucleon numbes fo full shells. Thus, this simple model does not wok fo the highe magic numbes. Fo them it is necessay to include spin-obit coupling effects which futhe split the nl shells.

13 Spin-obit inteaction Intoduce the spin-obit inteaction V ls a coupling of the spin and the obital angula momentum: Hˆ = h + U( ) + Vˆ ls M U( ) Vˆ + + ls Ψ (, θ, ϕ) = E Ψ(, θ, ϕ) h M + U( ) Ψ (, θ, ϕ) = ( E Vls ) Ψ(, θ, ϕ) h M whee Vˆ ls Ψ(, θ, ϕ) = V Eigenstates spin-obit inteaction: Vˆ ls = ls Ψ(, θ, ϕ) eigenvalues C ls ( l,s ) - scala poduct of l and s total angula momentum: j = l + s j j = ( l + s)( l + s) = l + s + ls l s = ( j l s ) 3

14 Spin-obit inteaction Eigenvalues: C ls ( j l s ) Ψ(, θ, ϕ) = V ls Ψ(, θ, ϕ) h Vls = Cls + [ j( j + ) l( l + ) s( s ) ] Conside: j = l + : V ls = C ls h ( l + )( l + ) l l 3 = C ls h l j h 3 h = l : Vls = Cls ( l )( l + ) l l = Cls ( l + ) This leads to an enegy splitting E ls which linealy inceases with the angula momentum as l + Els = V ls It is found expeimentally that V ls is negative, which means that the state with j =l+ / is always enegetically below the j = l / level. 4

15 Spin-obit inteaction The total angula momentum quantum numbe j = l±/ of the nucleon is denoted by an exta index j: nl j Single paticle enegy levels: j (j+) e.g., the f state splits into a f 7/ and a f 5/ state f f 5/ f 7/ The nlj level is (j + ) times degeneate Spin-obit inteaction leads to a sizeable splitting of the enegy states which ae indeed compaable with the gaps between the nl shells themselves. Magic numbes appea when the gaps between successive enegy shells ae paticulaly lage:, 8, 0, 8, 50, 8, 6 (0) () (6) (4) (8) (4) () (6) () (4) () 5

16 Collective Nuclea Models 6

17 Collective excitations of nuclei The single-paticle shell model can not popely descibe the excited states of nuclei: the excitation specta of even-even nuclei show chaacteistic band stuctues which can be intepeted as vibations and otations of the nuclea suface low enegy excitations have a collective oigin! The liquid dop model is used fo the desciption of collective excitations of nuclei: the inteio stuctue, i.e., the existence of individual nucleons, is neglected in favo of the pictue of a homogeneous fluid-like nuclea matte. The moving nuclea suface may be descibed quite geneally by an expansion in spheical hamonics with time-dependent shape paametes as coefficients: whee R(θ,φ,t) denotes the nuclea adius in the diection (θ,φ) at time t, and R 0 is the adius of the spheical nucleus, which is ealized when all α λµ =0. The time-dependent amplitudes α λµ (t) descibe the vibations of the nucleus with diffeent multipolaity aound the gound state and thus seve as collective coodinates (tenso). 7 λµ ()

18 Collective excitations of nuclei vibations otations 8

19 Collective coodinates Popeties of the coefficients α λµ λµ : - Complex conjugation: the nuclea adius must be eal, i.e., R(θ,φ,t)=R*(θ,φ,t). () Applying () to () and using the popety of the spheical hamonics (3) () one finds that the α λµ have to fulfill the condition: λµ (4) - The dynamical collective coodinates α λµ (tensos!) define the distotion - vibations - of the nuclea suface elative to the goundstate. - The geneal expansion of the nuclea suface in () allows fo abitay distotions: λ=0,,,. 9

20 Types of Multipole Defomations Goundstate The monopole mode, λ = 0. α Y 00 = 00 R( ϑ, φ,t ) = R 0(+ α00y00 ) = R 0(+ ) 4π 4π The spheical hamonic Y 00 is constant, so that a nonvanishing value of α 00 coesponds to a change of the adius of the sphee. Monopole mode λ=0 The associated excitation is the so-called beathing mode of the nucleus. Because of the lage amount of enegy needed fo the compession of nuclea matte, this mode is fa too high in enegy to be impotant fo the low-enegy specta discussed hee. The defomation paamete α 00 can be used to cancel the oveall density change pesent as a side effect in the othe multipole defomations. The dipole mode, λ =. Y 0 cosθ Dipole defomations, λ = to lowest ode, eally do not coespond to a defomation of the nucleus but athe to a shift of the cente of mass, i.e. a tanslation of the nucleus, and should be disegaded fo nuclea excitations since tanslational shifts ae spuious. 0

21 Types of Multipole Defomations The quadupole mode, λ = The quadupole defomations - the most impotant collective low enegy excitations of the nucleus. The octupole mode, λ = 3 The octupole defomations ae the pincipal asymmetic modes of the nucleus associated with negative-paity bands. The hexadecupole mode, λ = 4 The hexadecupole defomations: this is the highest angula momentum that has been of any impotance in nuclea theoy. While thee is no evidence fo pue hexadecupole excitations in the specta, it seems to play an impotant ole as an admixtue to quadupole excitations and fo the goundstate shape of heavy nuclei.

22 Types of Multipole Defomations

23 Quadupole defomations The quadupole defomations ae the most impotant vibational degees of feedom of the nucleus. Fo the case of pue quadupole defomation (λ = ) the nuclea suface is given by (5) Conside the diffeent components of the quadupole defomation tenso α µ The paametes α µ ae not independent - cf. (4): Fom (4): (6) => α 0 is eal (since α 0 = α 0 ) ; and we ae left with five independent eal degees of feedom: α 0 and the eal and imaginay pats of α and α 0 To investigate the actual fom of the nucleus, it is best to expess this in catesian coodinates by ewiting the spheical hamonics in tems of the catesian components of the unit vecto in the diection (θ,φ) : (6) (7) µ 3

24 Fom spheical to catesian coodinates Spheical coodinates (,θ,φ) Catesian coodinates (x,y,z)=>(ζ,ξ,η) The invention of Catesian coodinates in the 7th centuy by René Descates (Latinized name: Catesius) 4

25 Catesian coodinates Catesian coodinates fulfil subsidiay conditions (8) (9) Substitute (9) in (5): (0) whee the catesian components of the defomation ae elated to the spheical ones by () 5

26 Catesian coodinates In () six independent catesian components appea (all eal), compaed to the five degees of feedom contained in the spheical components. Howeve, the function R(θ,φ) fulfills () Subs. (0) into () and accounting that we obtain: 5 independent catesian components As the catesian defomations ae diectly elated to the steching (o contaction) of the nucleus in the appopiate diection, we can ead off that: α 0 descibes a stetching of the z axis with espect to the у and x axes, α, α descibes the elative length of the x axis compaed to the у axis (eal pat), as well as an oblique defomation in the x-y plane, α, α indicate an oblique defomation of the z axis. () 6

Nuclear and Particle Physics - Lecture 20 The shell model

Nuclear and Particle Physics - Lecture 20 The shell model 1 Intoduction Nuclea and Paticle Physics - Lectue 0 The shell model It is appaent that the semi-empiical mass fomula does a good job of descibing tends but not the non-smooth behaviou of the binding enegy.

More information

Lecture 7: Angular Momentum, Hydrogen Atom

Lecture 7: Angular Momentum, Hydrogen Atom Lectue 7: Angula Momentum, Hydogen Atom Vecto Quantization of Angula Momentum and Nomalization of 3D Rigid Roto wavefunctions Conside l, so L 2 2 2. Thus, we have L 2. Thee ae thee possibilities fo L z

More information

3D-Central Force Problems I

3D-Central Force Problems I 5.73 Lectue #1 1-1 Roadmap 1. define adial momentum 3D-Cental Foce Poblems I Read: C-TDL, pages 643-660 fo next lectue. All -Body, 3-D poblems can be educed to * a -D angula pat that is exactly and univesally

More information

Physical Chemistry II (Chapter 4 1) Rigid Rotor Models and Angular Momentum Eigenstates

Physical Chemistry II (Chapter 4 1) Rigid Rotor Models and Angular Momentum Eigenstates Physical Chemisty II (Chapte 4 ) Rigid Roto Models and Angula Momentum Eigenstates Tae Kyu Kim Depatment of Chemisty Rm. 30 (tkkim@pusan.ac.k) http://cafe.nave.com/moneo76 SUMMAR CHAPTER 3 A simple QM

More information

Physics 505 Homework No. 9 Solutions S9-1

Physics 505 Homework No. 9 Solutions S9-1 Physics 505 Homewok No 9 s S9-1 1 As pomised, hee is the tick fo summing the matix elements fo the Stak effect fo the gound state of the hydogen atom Recall, we need to calculate the coection to the gound

More information

Anyone who can contemplate quantum mechanics without getting dizzy hasn t understood it. --Niels Bohr. Lecture 17, p 1

Anyone who can contemplate quantum mechanics without getting dizzy hasn t understood it. --Niels Bohr. Lecture 17, p 1 Anyone who can contemplate quantum mechanics without getting dizzy hasn t undestood it. --Niels Boh Lectue 17, p 1 Special (Optional) Lectue Quantum Infomation One of the most moden applications of QM

More information

= e2. = 2e2. = 3e2. V = Ze2. where Z is the atomic numnber. Thus, we take as the Hamiltonian for a hydrogenic. H = p2 r. (19.4)

= e2. = 2e2. = 3e2. V = Ze2. where Z is the atomic numnber. Thus, we take as the Hamiltonian for a hydrogenic. H = p2 r. (19.4) Chapte 9 Hydogen Atom I What is H int? That depends on the physical system and the accuacy with which it is descibed. A natual stating point is the fom H int = p + V, (9.) µ which descibes a two-paticle

More information

11) A thin, uniform rod of mass M is supported by two vertical strings, as shown below.

11) A thin, uniform rod of mass M is supported by two vertical strings, as shown below. Fall 2007 Qualifie Pat II 12 minute questions 11) A thin, unifom od of mass M is suppoted by two vetical stings, as shown below. Find the tension in the emaining sting immediately afte one of the stings

More information

1 Spherical multipole moments

1 Spherical multipole moments Jackson notes 9 Spheical multipole moments Suppose we have a chage distibution ρ (x) wheeallofthechageiscontained within a spheical egion of adius R, as shown in the diagam. Then thee is no chage in the

More information

ON THE TWO-BODY PROBLEM IN QUANTUM MECHANICS

ON THE TWO-BODY PROBLEM IN QUANTUM MECHANICS ON THE TWO-BODY PROBLEM IN QUANTUM MECHANICS L. MICU Hoia Hulubei National Institute fo Physics and Nuclea Engineeing, P.O. Box MG-6, RO-0775 Buchaest-Maguele, Romania, E-mail: lmicu@theoy.nipne.o (Received

More information

20th Century Atomic Theory - Hydrogen Atom

20th Century Atomic Theory - Hydrogen Atom 0th Centuy Atomic Theoy - Hydogen Atom Ruthefod s scatteing expeiments (Section.5, pp. 53-55) in 1910 led to a nuclea model of the atom whee all the positive chage and most of the mass wee concentated

More information

5.111 Lecture Summary #6 Monday, September 15, 2014

5.111 Lecture Summary #6 Monday, September 15, 2014 5.111 Lectue Summay #6 Monday, Septembe 15, 014 Readings fo today: Section 1.9 Atomic Obitals. Section 1.10 Electon Spin, Section 1.11 The Electonic Stuctue of Hydogen. (Same sections in 4 th ed.) Read

More information

3.23 Electrical, Optical, and Magnetic Properties of Materials

3.23 Electrical, Optical, and Magnetic Properties of Materials MIT OpenCouseWae http://ocw.mit.edu 3.23 Electical, Optical, and Magnetic Popeties of Mateials Fall 27 Fo infomation about citing these mateials o ou Tems of Use, visit: http://ocw.mit.edu/tems. 3.23 Fall

More information

Calculation of Quark-antiquark Potential Coefficient and Charge Radius of Light Mesons

Calculation of Quark-antiquark Potential Coefficient and Charge Radius of Light Mesons Applied Physics Reseach ISSN: 96-9639 Vol., No., May E-ISSN: 96-9647 Calculation of Quak-antiquak Potential Coefficient and Chage Radius of Light Mesons M.R. Shojaei (Coesponding autho ) Depatment of Physics

More information

APPENDIX. For the 2 lectures of Claude Cohen-Tannoudji on Atom-Atom Interactions in Ultracold Quantum Gases

APPENDIX. For the 2 lectures of Claude Cohen-Tannoudji on Atom-Atom Interactions in Ultracold Quantum Gases APPENDIX Fo the lectues of Claude Cohen-Tannoudji on Atom-Atom Inteactions in Ultacold Quantum Gases Pupose of this Appendix Demonstate the othonomalization elation(ϕ ϕ = δ k k δ δ )k - The wave function

More information

The Schrödinger Equation in Three Dimensions

The Schrödinger Equation in Three Dimensions The Schödinge Equation in Thee Dimensions Paticle in a Rigid Thee-Dimensional Box (Catesian Coodinates) To illustate the solution of the time-independent Schödinge equation (TISE) in thee dimensions, we

More information

arxiv: v1 [physics.gen-ph] 18 Aug 2018

arxiv: v1 [physics.gen-ph] 18 Aug 2018 Path integal and Sommefeld quantization axiv:1809.04416v1 [physics.gen-ph] 18 Aug 018 Mikoto Matsuda 1, and Takehisa Fujita, 1 Japan Health and Medical technological college, Tokyo, Japan College of Science

More information

Introduction to Nuclear Forces

Introduction to Nuclear Forces Intoduction to Nuclea Foces One of the main poblems of nuclea physics is to find out the natue of nuclea foces. Nuclea foces diffe fom all othe known types of foces. They cannot be of electical oigin since

More information

Quantum theory of angular momentum

Quantum theory of angular momentum Quantum theoy of angula momentum Igo Mazets igo.mazets+e141@tuwien.ac.at (Atominstitut TU Wien, Stadionallee 2, 1020 Wien Time: Fiday, 13:00 14:30 Place: Feihaus, Sem.R. DA gün 06B (exception date 18 Nov.:

More information

c n ψ n (r)e ient/ h (2) where E n = 1 mc 2 α 2 Z 2 ψ(r) = c n ψ n (r) = c n = ψn(r)ψ(r)d 3 x e 2r/a0 1 πa e 3r/a0 r 2 dr c 1 2 = 2 9 /3 6 = 0.

c n ψ n (r)e ient/ h (2) where E n = 1 mc 2 α 2 Z 2 ψ(r) = c n ψ n (r) = c n = ψn(r)ψ(r)d 3 x e 2r/a0 1 πa e 3r/a0 r 2 dr c 1 2 = 2 9 /3 6 = 0. Poblem {a} Fo t : Ψ(, t ψ(e iet/ h ( whee E mc α (α /7 ψ( e /a πa Hee we have used the gound state wavefunction fo Z. Fo t, Ψ(, t can be witten as a supeposition of Z hydogenic wavefunctions ψ n (: Ψ(,

More information

Scattering in Three Dimensions

Scattering in Three Dimensions Scatteing in Thee Dimensions Scatteing expeiments ae an impotant souce of infomation about quantum systems, anging in enegy fom vey low enegy chemical eactions to the highest possible enegies at the LHC.

More information

Many Electron Atoms. Electrons can be put into approximate orbitals and the properties of the many electron systems can be catalogued

Many Electron Atoms. Electrons can be put into approximate orbitals and the properties of the many electron systems can be catalogued Many Electon Atoms The many body poblem cannot be solved analytically. We content ouselves with developing appoximate methods that can yield quite accuate esults (but usually equie a compute). The electons

More information

Chapter 6: Rotational and Rovibrational Spectra. A) General discussion of two- body problem with central potential

Chapter 6: Rotational and Rovibrational Spectra. A) General discussion of two- body problem with central potential Fall 4 Chapte 6: Rotational and Rovibational Specta... 75 Diffeent Appoximations... 8 Spectum fo Hamonic Oscillato + Rigid Rotato... 8 Polyatomic Molecules... 84 Hamonic Oscillato + Rigid Roto Model to

More information

Doublet structure of Alkali spectra:

Doublet structure of Alkali spectra: Doublet stuctue of : Caeful examination of the specta of alkali metals shows that each membe of some of the seies ae closed doublets. Fo example, sodium yellow line, coesponding to 3p 3s tansition, is

More information

SIO 229 Gravity and Geomagnetism. Lecture 6. J 2 for Earth. J 2 in the solar system. A first look at the geoid.

SIO 229 Gravity and Geomagnetism. Lecture 6. J 2 for Earth. J 2 in the solar system. A first look at the geoid. SIO 229 Gavity and Geomagnetism Lectue 6. J 2 fo Eath. J 2 in the sola system. A fist look at the geoid. The Thee Big Themes of the Gavity Lectues 1.) An ellipsoidal otating Eath Refeence body (mass +

More information

Energy Levels Of Hydrogen Atom Using Ladder Operators. Ava Khamseh Supervisor: Dr. Brian Pendleton The University of Edinburgh August 2011

Energy Levels Of Hydrogen Atom Using Ladder Operators. Ava Khamseh Supervisor: Dr. Brian Pendleton The University of Edinburgh August 2011 Enegy Levels Of Hydogen Atom Using Ladde Opeatos Ava Khamseh Supeviso: D. Bian Pendleton The Univesity of Edinbugh August 11 1 Abstact The aim of this pape is to fist use the Schödinge wavefunction methods

More information

PHYSICS 4E FINAL EXAM SPRING QUARTER 2010 PROF. HIRSCH JUNE 11 Formulas and constants: hc =12,400 ev A ; k B. = hf " #, # $ work function.

PHYSICS 4E FINAL EXAM SPRING QUARTER 2010 PROF. HIRSCH JUNE 11 Formulas and constants: hc =12,400 ev A ; k B. = hf  #, # $ work function. PHYSICS 4E FINAL EXAM SPRING QUARTER 1 Fomulas and constants: hc =1,4 ev A ; k B =1/11,6 ev/k ; ke =14.4eVA ; m e c =.511"1 6 ev ; m p /m e =1836 Relativistic enegy - momentum elation E = m c 4 + p c ;

More information

Quantum Mechanics II

Quantum Mechanics II Quantum Mechanics II Pof. Bois Altshule Apil 25, 2 Lectue 25 We have been dicussing the analytic popeties of the S-matix element. Remembe the adial wave function was u kl () = R kl () e ik iπl/2 S l (k)e

More information

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx.

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx. 9. LAGRANGIAN OF THE ELECTROMAGNETIC FIELD In the pevious section the Lagangian and Hamiltonian of an ensemble of point paticles was developed. This appoach is based on a qt. This discete fomulation can

More information

Homework # 3 Solution Key

Homework # 3 Solution Key PHYSICS 631: Geneal Relativity Homewok # 3 Solution Key 1. You e on you hono not to do this one by hand. I ealize you can use a compute o simply look it up. Please don t. In a flat space, the metic in

More information

3.012 Fund of Mat Sci: Bonding Lecture 5/6. Comic strip removed for copyright reasons.

3.012 Fund of Mat Sci: Bonding Lecture 5/6. Comic strip removed for copyright reasons. 3.12 Fund of Mat Sci: Bonding Lectue 5/6 THE HYDROGEN ATOM Comic stip emoved fo copyight easons. Last Time Metal sufaces and STM Diac notation Opeatos, commutatos, some postulates Homewok fo Mon Oct 3

More information

Lecture 4 Povh Krane Enge Williams

Lecture 4 Povh Krane Enge Williams Lectue 4 Povh Kane Enge Williams the Deuteon 6. Ch. 4 Ch. Ch 3 d-wave admixtue 4..6 3.5 tenso foce 4..6 3.5 missing S state 4.4.5 3.4 isospin.3 6.7 3.4 Poblems on Lectue 4 What is the minimum photon enegy

More information

PROBLEM SET #1 SOLUTIONS by Robert A. DiStasio Jr.

PROBLEM SET #1 SOLUTIONS by Robert A. DiStasio Jr. POBLM S # SOLUIONS by obet A. DiStasio J. Q. he Bon-Oppenheime appoximation is the standad way of appoximating the gound state of a molecula system. Wite down the conditions that detemine the tonic and

More information

Lecture 8 - Gauss s Law

Lecture 8 - Gauss s Law Lectue 8 - Gauss s Law A Puzzle... Example Calculate the potential enegy, pe ion, fo an infinite 1D ionic cystal with sepaation a; that is, a ow of equally spaced chages of magnitude e and altenating sign.

More information

Preliminary Exam: Quantum Physics 1/14/2011, 9:00-3:00

Preliminary Exam: Quantum Physics 1/14/2011, 9:00-3:00 Peliminay Exam: Quantum Physics /4/ 9:-: Answe a total of SIX questions of which at least TWO ae fom section A and at least THREE ae fom section B Fo you answes you can use eithe the blue books o individual

More information

Rigid Body Dynamics 2. CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2018

Rigid Body Dynamics 2. CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2018 Rigid Body Dynamics 2 CSE169: Compute Animation nstucto: Steve Rotenbeg UCSD, Winte 2018 Coss Poduct & Hat Opeato Deivative of a Rotating Vecto Let s say that vecto is otating aound the oigin, maintaining

More information

Three-dimensional systems with spherical symmetry

Three-dimensional systems with spherical symmetry Thee-dimensiona systems with spheica symmety Thee-dimensiona systems with spheica symmety 006 Quantum Mechanics Pof. Y. F. Chen Thee-dimensiona systems with spheica symmety We conside a patice moving in

More information

A Relativistic Electron in a Coulomb Potential

A Relativistic Electron in a Coulomb Potential A Relativistic Electon in a Coulomb Potential Alfed Whitehead Physics 518, Fall 009 The Poblem Solve the Diac Equation fo an electon in a Coulomb potential. Identify the conseved quantum numbes. Specify

More information

Tutorial Exercises: Central Forces

Tutorial Exercises: Central Forces Tutoial Execises: Cental Foces. Tuning Points fo the Keple potential (a) Wite down the two fist integals fo cental motion in the Keple potential V () = µm/ using J fo the angula momentum and E fo the total

More information

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1 Please ead this fist... AST S: The oigin and evolution of the Univese Intoduction to Mathematical Handout This is an unusually long hand-out and one which uses in places mathematics that you may not be

More information

EFFECTS OF FRINGING FIELDS ON SINGLE PARTICLE DYNAMICS. M. Bassetti and C. Biscari INFN-LNF, CP 13, Frascati (RM), Italy

EFFECTS OF FRINGING FIELDS ON SINGLE PARTICLE DYNAMICS. M. Bassetti and C. Biscari INFN-LNF, CP 13, Frascati (RM), Italy Fascati Physics Seies Vol. X (998), pp. 47-54 4 th Advanced ICFA Beam Dynamics Wokshop, Fascati, Oct. -5, 997 EFFECTS OF FRININ FIELDS ON SINLE PARTICLE DYNAMICS M. Bassetti and C. Biscai INFN-LNF, CP

More information

Physics 235 Chapter 5. Chapter 5 Gravitation

Physics 235 Chapter 5. Chapter 5 Gravitation Chapte 5 Gavitation In this Chapte we will eview the popeties of the gavitational foce. The gavitational foce has been discussed in geat detail in you intoductoy physics couses, and we will pimaily focus

More information

Rydberg-Rydberg Interactions

Rydberg-Rydberg Interactions Rydbeg-Rydbeg Inteactions F. Robicheaux Aubun Univesity Rydbeg gas goes to plasma Dipole blockade Coheent pocesses in fozen Rydbeg gases (expts) Theoetical investigation of an excitation hopping though

More information

15 Solving the Laplace equation by Fourier method

15 Solving the Laplace equation by Fourier method 5 Solving the Laplace equation by Fouie method I aleady intoduced two o thee dimensional heat equation, when I deived it, ecall that it taes the fom u t = α 2 u + F, (5.) whee u: [0, ) D R, D R is the

More information

Classical Mechanics Homework set 7, due Nov 8th: Solutions

Classical Mechanics Homework set 7, due Nov 8th: Solutions Classical Mechanics Homewok set 7, due Nov 8th: Solutions 1. Do deivation 8.. It has been asked what effect does a total deivative as a function of q i, t have on the Hamiltonian. Thus, lets us begin with

More information

Chapter 13 Gravitation

Chapter 13 Gravitation Chapte 13 Gavitation In this chapte we will exploe the following topics: -Newton s law of gavitation, which descibes the attactive foce between two point masses and its application to extended objects

More information

ASTR415: Problem Set #6

ASTR415: Problem Set #6 ASTR45: Poblem Set #6 Cuan D. Muhlbege Univesity of Mayland (Dated: May 7, 27) Using existing implementations of the leapfog and Runge-Kutta methods fo solving coupled odinay diffeential equations, seveal

More information

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3.

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3. Appendix A Vecto Algeba As is natual, ou Aeospace Stuctues will be descibed in a Euclidean thee-dimensional space R 3. A.1 Vectos A vecto is used to epesent quantities that have both magnitude and diection.

More information

B. Spherical Wave Propagation

B. Spherical Wave Propagation 11/8/007 Spheical Wave Popagation notes 1/1 B. Spheical Wave Popagation Evey antenna launches a spheical wave, thus its powe density educes as a function of 1, whee is the distance fom the antenna. We

More information

Right-handed screw dislocation in an isotropic solid

Right-handed screw dislocation in an isotropic solid Dislocation Mechanics Elastic Popeties of Isolated Dislocations Ou study of dislocations to this point has focused on thei geomety and thei ole in accommodating plastic defomation though thei motion. We

More information

221B Lecture Notes Scattering Theory I

221B Lecture Notes Scattering Theory I Why Scatteing? B Lectue Notes Scatteing Theoy I Scatteing of paticles off taget has been one of the most impotant applications of quantum mechanics. It is pobably the most effective way to study the stuctue

More information

TheWaveandHelmholtzEquations

TheWaveandHelmholtzEquations TheWaveandHelmholtzEquations Ramani Duaiswami The Univesity of Mayland, College Pak Febuay 3, 2006 Abstact CMSC828D notes (adapted fom mateial witten with Nail Gumeov). Wok in pogess 1 Acoustic Waves 1.1

More information

Mechanics Physics 151

Mechanics Physics 151 Mechanics Physics 151 Lectue 5 Cental Foce Poblem (Chapte 3) What We Did Last Time Intoduced Hamilton s Pinciple Action integal is stationay fo the actual path Deived Lagange s Equations Used calculus

More information

1.2 Differential cross section

1.2 Differential cross section .2. DIFFERENTIAL CROSS SECTION Febuay 9, 205 Lectue VIII.2 Diffeential coss section We found that the solution to the Schodinge equation has the fom e ik x ψ 2π 3/2 fk, k + e ik x and that fk, k = 2 m

More information

AH Mechanics Checklist (Unit 2) AH Mechanics Checklist (Unit 2) Circular Motion

AH Mechanics Checklist (Unit 2) AH Mechanics Checklist (Unit 2) Circular Motion AH Mechanics Checklist (Unit ) AH Mechanics Checklist (Unit ) Cicula Motion No. kill Done 1 Know that cicula motion efes to motion in a cicle of constant adius Know that cicula motion is conveniently descibed

More information

Geometry of the homogeneous and isotropic spaces

Geometry of the homogeneous and isotropic spaces Geomety of the homogeneous and isotopic spaces H. Sonoda Septembe 2000; last evised Octobe 2009 Abstact We summaize the aspects of the geomety of the homogeneous and isotopic spaces which ae most elevant

More information

( n x ( ) Last Time Exam 3 results. Question. 3-D particle in box: summary. Modified Bohr model. 3-D Hydrogen atom. r n. = n 2 a o

( n x ( ) Last Time Exam 3 results. Question. 3-D particle in box: summary. Modified Bohr model. 3-D Hydrogen atom. r n. = n 2 a o Last Time Exam 3 esults Quantum tunneling 3-dimensional wave functions Deceasing paticle size Quantum dots paticle in box) This week s honos lectue: Pof. ad histian, Positon Emission Tomogaphy Tue. Dec.

More information

F(r) = r f (r) 4.8. Central forces The most interesting problems in classical mechanics are about central forces.

F(r) = r f (r) 4.8. Central forces The most interesting problems in classical mechanics are about central forces. 4.8. Cental foces The most inteesting poblems in classical mechanics ae about cental foces. Definition of a cental foce: (i) the diection of the foce F() is paallel o antipaallel to ; in othe wods, fo

More information

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!!

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!! Physics 161 Fall 011 Exta Cedit Investigating Black Holes - olutions The Following is Woth 50 Points!!! This exta cedit assignment will investigate vaious popeties of black holes that we didn t have time

More information

Orbital Angular Momentum Eigenfunctions

Orbital Angular Momentum Eigenfunctions Obital Angula Moentu Eigenfunctions Michael Fowle 1/11/08 Intoduction In the last lectue we established that the opeatos J Jz have a coon set of eigenkets j J j = j( j+ 1 ) j Jz j = j whee j ae integes

More information

The Poisson bracket and magnetic monopoles

The Poisson bracket and magnetic monopoles FYST420 Advanced electodynamics Olli Aleksante Koskivaaa Final poject ollikoskivaaa@gmail.com The Poisson backet and magnetic monopoles Abstact: In this wok magnetic monopoles ae studied using the Poisson

More information

d 2 x 0a d d =0. Relative to an arbitrary (accelerating frame) specified by x a = x a (x 0b ), the latter becomes: d 2 x a d 2 + a dx b dx c

d 2 x 0a d d =0. Relative to an arbitrary (accelerating frame) specified by x a = x a (x 0b ), the latter becomes: d 2 x a d 2 + a dx b dx c Chapte 6 Geneal Relativity 6.1 Towads the Einstein equations Thee ae seveal ways of motivating the Einstein equations. The most natual is pehaps though consideations involving the Equivalence Pinciple.

More information

Nuclear size corrections to the energy levels of single-electron atoms

Nuclear size corrections to the energy levels of single-electron atoms Nuclea size coections to the enegy levels of single-electon atoms Babak Nadii Nii a eseach Institute fo Astonomy and Astophysics of Maagha (IAAM IAN P. O. Box: 554-44. Abstact A study is made of nuclea

More information

AY 7A - Fall 2010 Section Worksheet 2 - Solutions Energy and Kepler s Law

AY 7A - Fall 2010 Section Worksheet 2 - Solutions Energy and Kepler s Law AY 7A - Fall 00 Section Woksheet - Solutions Enegy and Keple s Law. Escape Velocity (a) A planet is obiting aound a sta. What is the total obital enegy of the planet? (i.e. Total Enegy = Potential Enegy

More information

I. CONSTRUCTION OF THE GREEN S FUNCTION

I. CONSTRUCTION OF THE GREEN S FUNCTION I. CONSTRUCTION OF THE GREEN S FUNCTION The Helmohltz equation in 4 dimensions is 4 + k G 4 x, x = δ 4 x x. In this equation, G is the Geen s function and 4 efes to the dimensionality. In the vey end,

More information

Newton s Laws, Kepler s Laws, and Planetary Orbits

Newton s Laws, Kepler s Laws, and Planetary Orbits Newton s Laws, Keple s Laws, and Planetay Obits PROBLEM SET 4 DUE TUESDAY AT START OF LECTURE 28 Septembe 2017 ASTRONOMY 111 FALL 2017 1 Newton s & Keple s laws and planetay obits Unifom cicula motion

More information

? this lecture. ? next lecture. What we have learned so far. a Q E F = q E a. F = q v B a. a Q in motion B. db/dt E. de/dt B.

? this lecture. ? next lecture. What we have learned so far. a Q E F = q E a. F = q v B a. a Q in motion B. db/dt E. de/dt B. PHY 249 Lectue Notes Chapte 32: Page 1 of 12 What we have leaned so fa a a F q a a in motion F q v a a d/ Ae thee othe "static" chages that can make -field? this lectue d/? next lectue da dl Cuve Cuve

More information

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum 2. Electostatics D. Rakhesh Singh Kshetimayum 1 2.1 Intoduction In this chapte, we will study how to find the electostatic fields fo vaious cases? fo symmetic known chage distibution fo un-symmetic known

More information

Chem 453/544 Fall /08/03. Exam #1 Solutions

Chem 453/544 Fall /08/03. Exam #1 Solutions Chem 453/544 Fall 3 /8/3 Exam # Solutions. ( points) Use the genealized compessibility diagam povided on the last page to estimate ove what ange of pessues A at oom tempeatue confoms to the ideal gas law

More information

Differential Cross Section of Elastic and Inelastic p 15 N Scattering

Differential Cross Section of Elastic and Inelastic p 15 N Scattering NUCLEAR THEORY, Vol. 32 (2013) eds. A.I. Geogieva, N. Minkov, Heon Pess, Sofia Dfeential Coss Section of Elastic and Inelastic p 15 N Scatteing E. Ibaeva 1, N. Butebaev 1, M. Zhusupov 2 1 Institute of

More information

Structure of Hadrons. quarks d (down) s (strange) c (charm)

Structure of Hadrons. quarks d (down) s (strange) c (charm) quaks Flavo A t t 0 S B T Q(e) Mc 2 (GeV) u (up) 1 3 1 2-1 2 0 0 0 0 2 3 0.002-0.008 d (down) 1 3 1 2 1 2 0 0 0 0-1 3 0.005-0.015 s (stange) 1 3 0 0-1 0 0 0-1 3 0.1-0.3 c (cham) 1 3 0 0 0 1 0 0 2 3 1.0-1.6

More information

MAGNETIC FIELD AROUND TWO SEPARATED MAGNETIZING COILS

MAGNETIC FIELD AROUND TWO SEPARATED MAGNETIZING COILS The 8 th Intenational Confeence of the Slovenian Society fo Non-Destuctive Testing»pplication of Contempoay Non-Destuctive Testing in Engineeing«Septembe 1-3, 5, Potoož, Slovenia, pp. 17-1 MGNETIC FIELD

More information

KEPLER S LAWS OF PLANETARY MOTION

KEPLER S LAWS OF PLANETARY MOTION EPER S AWS OF PANETARY MOTION 1. Intoduction We ae now in a position to apply what we have leaned about the coss poduct and vecto valued functions to deive eple s aws of planetay motion. These laws wee

More information

working pages for Paul Richards class notes; do not copy or circulate without permission from PGR 2004/11/3 10:50

working pages for Paul Richards class notes; do not copy or circulate without permission from PGR 2004/11/3 10:50 woking pages fo Paul Richads class notes; do not copy o ciculate without pemission fom PGR 2004/11/3 10:50 CHAPTER7 Solid angle, 3D integals, Gauss s Theoem, and a Delta Function We define the solid angle,

More information

Physics 506 Winter 2006 Homework Assignment #9 Solutions

Physics 506 Winter 2006 Homework Assignment #9 Solutions Physics 506 Winte 2006 Homewok Assignment #9 Solutions Textbook poblems: Ch. 12: 12.2, 12.9, 12.13, 12.14 12.2 a) Show fom Hamilton s pinciple that Lagangians that diffe only by a total time deivative

More information

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925)

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925) 1 Lectue 1: The beginnings of quantum physics 1. The Sten-Gelach expeiment. Atomic clocks 3. Planck 1900, blackbody adiation, and E ω 4. Photoelectic effect 5. Electon diffaction though cystals, de Boglie

More information

A NEW VARIABLE STIFFNESS SPRING USING A PRESTRESSED MECHANISM

A NEW VARIABLE STIFFNESS SPRING USING A PRESTRESSED MECHANISM Poceedings of the ASME 2010 Intenational Design Engineeing Technical Confeences & Computes and Infomation in Engineeing Confeence IDETC/CIE 2010 August 15-18, 2010, Monteal, Quebec, Canada DETC2010-28496

More information

Chapter 5 Force and Motion

Chapter 5 Force and Motion Chapte 5 Foce and Motion In chaptes 2 and 4 we have studied kinematics i.e. descibed the motion of objects using paametes such as the position vecto, velocity and acceleation without any insights as to

More information

EQUATIONS OF MOTION LUCA GUIDO MOLINARI

EQUATIONS OF MOTION LUCA GUIDO MOLINARI EQUATIONS OF MOTION LUCA GUIDO MOLINARI 1. Equation of motion of destuction opeatos Conside a system of bosons o femions descibed by a Hamiltonian H = H 1 + H 2, whee H 1 and H 2 ae espectively the one

More information

The geometric construction of Ewald sphere and Bragg condition:

The geometric construction of Ewald sphere and Bragg condition: The geometic constuction of Ewald sphee and Bagg condition: The constuction of Ewald sphee must be done such that the Bagg condition is satisfied. This can be done as follows: i) Daw a wave vecto k in

More information

Nuclear reactions of heavy ions

Nuclear reactions of heavy ions Autho: Facultat de Física, Univesitat de Bacelona, Diagonal 645, 08028 Bacelona, Spain. Adviso: Xavie Vinyes Abstact: In this wok nuclea eactions of heavy ions ae studied, focusing on elastic scatteing.

More information

From Gravitational Collapse to Black Holes

From Gravitational Collapse to Black Holes Fom Gavitational Collapse to Black Holes T. Nguyen PHY 391 Independent Study Tem Pape Pof. S.G. Rajeev Univesity of Rocheste Decembe 0, 018 1 Intoduction The pupose of this independent study is to familiaize

More information

The Precession of Mercury s Perihelion

The Precession of Mercury s Perihelion The Pecession of Mecuy s Peihelion Owen Biesel Januay 25, 2008 Contents 1 Intoduction 2 2 The Classical olution 2 3 Classical Calculation of the Peiod 4 4 The Relativistic olution 5 5 Remaks 9 1 1 Intoduction

More information

3.23 Electrical, Optical, and Magnetic Properties of Materials

3.23 Electrical, Optical, and Magnetic Properties of Materials MIT OpenCouseWae http://ocw.mit.edu 3.3 Electical, Optical, and Magnetic Popeties of Mateials Fall 7 Fo infomation about citing these mateials o ou Tems of Use, visit: http://ocw.mit.edu/tems. 3.3 Fall

More information

is the instantaneous position vector of any grid point or fluid

is the instantaneous position vector of any grid point or fluid Absolute inetial, elative inetial and non-inetial coodinates fo a moving but non-defoming contol volume Tao Xing, Pablo Caica, and Fed Sten bjective Deive and coelate the govening equations of motion in

More information

, and the curve BC is symmetrical. Find also the horizontal force in x-direction on one side of the body. h C

, and the curve BC is symmetrical. Find also the horizontal force in x-direction on one side of the body. h C Umeå Univesitet, Fysik 1 Vitaly Bychkov Pov i teknisk fysik, Fluid Dynamics (Stömningsläa), 2013-05-31, kl 9.00-15.00 jälpmedel: Students may use any book including the textbook Lectues on Fluid Dynamics.

More information

Section 26 The Laws of Rotational Motion

Section 26 The Laws of Rotational Motion Physics 24A Class Notes Section 26 The Laws of otational Motion What do objects do and why do they do it? They otate and we have established the quantities needed to descibe this motion. We now need to

More information

Is there a magnification paradox in gravitational lensing?

Is there a magnification paradox in gravitational lensing? Is thee a magnification paadox in gavitational ing? Olaf Wucknitz wucknitz@asto.uni-bonn.de Astophysics semina/colloquium, Potsdam, 6 Novembe 7 Is thee a magnification paadox in gavitational ing? gavitational

More information

Chapter 5 Force and Motion

Chapter 5 Force and Motion Chapte 5 Foce and Motion In Chaptes 2 and 4 we have studied kinematics, i.e., we descibed the motion of objects using paametes such as the position vecto, velocity, and acceleation without any insights

More information

Math 2263 Solutions for Spring 2003 Final Exam

Math 2263 Solutions for Spring 2003 Final Exam Math 6 Solutions fo Sping Final Exam ) A staightfowad appoach to finding the tangent plane to a suface at a point ( x, y, z ) would be to expess the cuve as an explicit function z = f ( x, y ), calculate

More information

where ω 0 is the angular frequency of rotation. Using this, we first examine the time-dependent multipole moments

where ω 0 is the angular frequency of rotation. Using this, we first examine the time-dependent multipole moments 9. A common textbook example of a adiating system (see Poblem 9.2) is a configuation of chages fixed elative to each othe but in otation. The chage density is obviously a function of time, but it is not

More information

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 10 Solutions. r s

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 10 Solutions. r s MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Depatment Physics 8.033 Decembe 5, 003 Poblem Set 10 Solutions Poblem 1 M s y x test paticle The figue above depicts the geomety of the poblem. The position

More information

Objectives. We will also get to know about the wavefunction and its use in developing the concept of the structure of atoms.

Objectives. We will also get to know about the wavefunction and its use in developing the concept of the structure of atoms. Modue "Atomic physics and atomic stuctue" Lectue 7 Quantum Mechanica teatment of One-eecton atoms Page 1 Objectives In this ectue, we wi appy the Schodinge Equation to the simpe system Hydogen and compae

More information

Problem Set 10 Solutions

Problem Set 10 Solutions Chemisty 6 D. Jean M. Standad Poblem Set 0 Solutions. Give the explicit fom of the Hamiltonian opeato (in atomic units) fo the lithium atom. You expession should not include any summations (expand them

More information

Physics 1502: Lecture 4 Today s Agenda

Physics 1502: Lecture 4 Today s Agenda 1 Physics 1502: Today s genda nnouncements: Lectues posted on: www.phys.uconn.edu/~cote/ HW assignments, solutions etc. Homewok #1: On Mastephysics today: due next Fiday Go to masteingphysics.com and egiste

More information

An Exact Solution of Navier Stokes Equation

An Exact Solution of Navier Stokes Equation An Exact Solution of Navie Stokes Equation A. Salih Depatment of Aeospace Engineeing Indian Institute of Space Science and Technology, Thiuvananthapuam, Keala, India. July 20 The pincipal difficulty in

More information

r cos, and y r sin with the origin of coordinate system located at

r cos, and y r sin with the origin of coordinate system located at Lectue 3-3 Kinematics of Rotation Duing ou peious lectues we hae consideed diffeent examples of motion in one and seeal dimensions. But in each case the moing object was consideed as a paticle-like object,

More information

Electromagnetism Physics 15b

Electromagnetism Physics 15b lectomagnetism Physics 15b Lectue #20 Dielectics lectic Dipoles Pucell 10.1 10.6 What We Did Last Time Plane wave solutions of Maxwell s equations = 0 sin(k ωt) B = B 0 sin(k ωt) ω = kc, 0 = B, 0 ˆk =

More information

Stress, Cauchy s equation and the Navier-Stokes equations

Stress, Cauchy s equation and the Navier-Stokes equations Chapte 3 Stess, Cauchy s equation and the Navie-Stokes equations 3. The concept of taction/stess Conside the volume of fluid shown in the left half of Fig. 3.. The volume of fluid is subjected to distibuted

More information

arxiv: v1 [physics.pop-ph] 3 Jun 2013

arxiv: v1 [physics.pop-ph] 3 Jun 2013 A note on the electostatic enegy of two point chages axiv:1306.0401v1 [physics.pop-ph] 3 Jun 013 A C Tot Instituto de Física Univesidade Fedeal do io de Janeio Caixa Postal 68.58; CEP 1941-97 io de Janeio,

More information