The Lorentz group. Generate the group SO(3,1) To construct representa;ons a more convenient (non- Hermi;an) basis is. i j ijk k. j ijk k.

Size: px
Start display at page:

Download "The Lorentz group. Generate the group SO(3,1) To construct representa;ons a more convenient (non- Hermi;an) basis is. i j ijk k. j ijk k."

Transcription

1 Fermons S 1 2

2 The Lorentz group Rotatons J Boosts K [ J, J ] ε J [ J, K ] ε K [ K, K ] ε J j jk k j jk k j jk k } Generate the group SO(3,1) ( M ( x x ) J M K M ) 1 ρσ ρ σ x σ ρ x 2 ε jk jk 0 To construct representa;ons a more convenent (non- Herm;an) bass s 1 N ( ) 2 J + K [ N, N ] ε N [ N, N ] ε N j jk k [ N, N ] 0 j jk k j } SU (2) SU (2) representaton ( n, m)

3 The Lorentz group Rotatons J Boosts K [ J, J ] ε J [ J, K ] ε K [ K, K ] ε J j jk k j jk k j jk k } Generate the group SO(3,1) ( M ( x x ) J M K M ) 1 ρσ ρ σ x σ ρ x 2 ε jk jk 0 To construct representa;ons a more convenent (non- Herm;an) bass s 1 N ( ) 2 J + K [ N, N ] ε N [ N, N ] ε N j jk k [ N, N ] 0 j jk k j SU (2) L SU (2) R J N + N ( n, m) J n + m Representa;ons (0,0) scalar J0 ( 1 2,0), (0, 1 2 ) LH and RH "spnors" J 1 2 ( 1, 1 ) vector J1, etc 2 2

4 Weyl spnors (,0) (0, ) L R 2- component spnors of SU(2) Rota;ons and Boosts L( R) SL( R) L( R) S L( R) e α 2.σ S L( R) e ν 2.σ : Rotatons : Boosts σ , σ 0 2 0, σ

5 Weyl spnors (,0) (0, ) L R Rota;ons and Boosts Drac spnor Can combne S L( R) L( R) L( R) 2- component spnors of SU(2), L R to form a 4- component Drac spnor S L( R) e α.σ 2 : Rotatons S L( R) e ν.σ 2 : Boosts L R where γ 0 Lorentz transforma;ons ω 0 0 I I 0 e, ωσ ω σ γ, γ ω 0 σ, γ σ o, γ γ 0 γ 1 γ 2 γ 3 I I ωσ µν µν µν 2 µ ν j boosts, ω rotatons, j 1,2,3 Weyl bass

6 Weyl spnors (,0) (0, ) L R Rota;ons and Boosts L( R) L( R) L( R) Drac spnor Can combne S 2- component spnors of SU(2), L R to form a 4- component Drac spnor S L( R) e α.σ 2 : Rotatons S L( R) e ν.σ 2 : Boosts L R where γ 0 Lorentz transforma;ons γ µ (Drac gamma matrces new 4- vector ) { } 0 I I 0 e, ωσ ω σ γ, γ ω 0 σ, γ σ o, γ γ 0 γ 1 γ 2 γ 3 I I µ ν µ ν ν µ µν γ, γ γ γ + γ γ 2g Clfford Algebra ωσ µν µν µν 2 µ ν

7 Weyl spnors (,0) (0, ) L R Rota;ons and Boosts L( R) L( R) L( R) Drac spnor Can combne S 2- component spnors of SU(2), L R to form a 4- component Drac spnor S L( R) e α.σ 2 : Rotatons S L( R) e ν.σ 2 : Boosts L R where γ 0 Lorentz transforma;ons { } 0 I I 0 γ, γ γ γ + γ γ 2g µ ν µ ν ν µ µν e, ωσ ω σ γ, γ ω 0 σ, γ σ o, γ γ 0 γ 1 γ 2 γ 3 I I γ µ (Drac gamma matrces new 4- vector ) ωσ µν µν µν 2 µ ν Note : L( R) 1 2 (1 γ 5 )

8 The Drac equa;on Fermons descrbed by 4- cpt Drac spnors L R γ 0 L R + R L Lorentz nvarant S L( R) e α 2.σ S L( R) e ν 2.σ : Rotatons : Boosts

9 The Drac equa;on Fermons descrbed by 4- cpt Drac spnors L R γ 0 L R + R L Lorentz nvarant New 4- vector γ µ

10 The Drac equa;on Fermons descrbed by 4- cpt Drac spnors L R γ 0 L R + R L Lorentz nvarant New 4- vector γ µ Lorentz nvarant Lagrangan L - γ µ µ m g µν Dag(1, 1, 1, 1) ( g µν Srednck!)

11 The Drac equa;on Fermons descrbed by 4- cpt Drac spnors L R γ 0 L R + R L Lorentz nvarant New 4- vector γ µ Lorentz nvarant Lagrangan L - γ µ µ m g µν Dag(1, 1, 1, 1) ( g µν Srednck!) From Euler Lagrange equa;on obtan the Drac equa;on ( γ µ µ m) 0 δs 0 L φ µ L ( µ φ) 0 Euler Lagrange equa;on

12 The Drac equa;on Fermons descrbed by 4- cpt Drac spnors γ 0 L R + R L Lorentz nvarant New 4- vector γ µ The Lagrangan L - γ µ µ m ( g µν Dag(1, 1, 1, 1) ) From Euler Lagrange equa;on obtan the Drac equa;on ( γ µ µ m) ( m) 0 p µ (m,0,0,0), ( γ 0 1) components projected out

13 The Drac equa;on Fermons descrbed by 4- cpt Drac spnors γ 0 L R + R L Lorentz nvarant New 4- vector γ µ The Lagrangan L - γ µ µ m ( g µν Dag(1, 1, 1, 1) ) From Euler Lagrange equa;on obtan the Drac equa;on ( γ µ µ m) ( m) 0 p µ (m,0,0,0), ( γ 0 1) ( γ µ µ + m) ( γ µ µ m) 0 ( 2 + m 2 ) components projected out Momentum components off shell Projected out

14 The Drac equa;on Fermons descrbed by 4- cpt Drac spnors γ 0 L R + R L New 4- vector γ µ Lorentz nvarant The Lagrangan L - γ µ µ m γ µ µ γ 0 (γ 0 0 γ ) I 0 0 I I 0 0 I 0 σ 0 0 σ 0 0 I I 0 0 σ σ 0 σ µ L µ L + R σ µ µ R σ µ ( 1,σ ), σ µ ( 1, σ )

15 Can construct LH spnors out of RH an;spnors and vce- versa L σ 2 R * ( 1 2,0) R σ 2 L * (0, 1 2 ) Proof : L eσ!" 2.ν L?!" R e σ 2.ν R!" σ 2 * R σ 2 e σ *!" 2.ν" * R σ 2 e σ eσ!" * 2.ν" σ 2 σ 2 * 2 R.ν" * σ 2 R usng σ 2 σ * σ 2 σ

16 Majorana fermons Maj L R σ 2 L * only 2 ndependent components Majorana mass m( L R + R L ) M L t σ 2 L M! L L

17 Party x µ x x x x 0 0 (, ) (, ) J J K K N N N N N J + K 0 I L R γ 0 R L I 0.e. L σ µ L R σ µ R L Knetc L σ µ µ L + R σ µ µ R preserves party: 0 0, σ µ (1,σ ), σ µ (1, σ ) (neutrnos volate party).e. L σ µ µ L R σ µ µ R

18 Charge conjuga;on L Knetc L σ µ µ L + R σ µ µ R nvarant under L σ 2 R *, R σ 2 L * (σ 2 σ µ σ 2 σ 2 µt ) EM and QCD nterac;ons preserve charge conjuga;on: L EM Q( L σ µ A µ L + R σ µ A µ ) R provded QA µ QA µ Weak nterac;ons do not preserve charge conjuga;on:

19 Rela;on to Srednck nota;on ( g µν Dag( 1,1,1,1 ) [ N, N ] ε N [ N, N ] ε N j jk k [ N, N ] 0 j jk k j Hermtan conjugaton N N (2,1) a ε 12 ε 21 1 (c. f.g µν ) R L L T σ 2 L a ε ab b

20 Rela;on to Srednck nota;on ( g µν Dag( 1,1,1,1 ) [ N, N ] ε N [ N, N ] ε N j jk k [ N, N ] 0 j jk k j Hermtan conjugaton N N Conven;on: RH (do^ed) felds always (2,1) a, (1,2) [ ] a!a Dot denotes SU(2) R ndex L a R σ 2 L *!a ε!a!b!b

21 Rela;on to Srednck nota;on ( g µν Dag( 1,1,1,1 ) Lα a, Rα!a a χ a χ Invarants : * R χ L ( σ 2 L ) χ L T L σ 2 χ L ε ab b χ a L χ R ε!a!b!a χ b! L σ µ µ L + R σ µ µ R ξ a σ µ a!c µ ξ!c + χ!a σ µ!ac µ χ c ( ) χ σ µ µ χ + ξ σ µ µ ξ + µ ξσ µ ξ L R χ c ξ!c

22 Fermon Lagrangan Drac fermon: Drac equa;on Majorana fermon:

23 Free par;cle solu;on to the Drac equa;on

24 Drac- Paul bass µ γ β, βα ( ) 0 σ I 0 α β σ 0 0 I γ 0 I 0 0 σ γ 0 I σ 0 γ 5 0 I I γ γ γ γ Weyl bass α σ 0 0 σ β 0 I I 0 γ 0 0 I I 0, γ 0 σ σ o, γ γ 0 γ 1 γ 2 γ 3 5 I 0 0 I { } µ ν µ ν ν µ µν γ, γ γ γ + γ γ 2g ( g µν Dag(1, 1, 1, 1) )

25 Free par;cle solu;on Drac Paul bass - c.f. Chapter 38 Srednck for Weyl bass solu;on ( γ µ µ m) 0 e p. x u( p) ( γ µ p µ m)u( p) ( p m)u( p) 0 µ γ ( β, βα ).e. ( α.p + βm)u Eu 0 σ I 0 α β σ 0 0 I mi σ. p ua ua E σ. p mi ub ub σ. p u ( E m) u B σ. p u ( E + m) u A A B

26 σ. p u ( E m) u B σ. p u ( E + m) u A A B If p 0, E + m ( E + m) u 0 u 0 B B For the 2 E>0 solu;ons, we may take ( s) ( s u ) A χ, χ 1 0 χ 0 1 (1) (2) u σ. p χ E + m ( s) ( s) B Pos;ve energy 4- spnor solu;ons of Drac s equa;on ( s) χ, 0, 1, 2 χ > E + m ( s) u N σ. p E s ( s)

27 For the 2 E<0 solu;ons, we may take u u σ. p σ. p χ χ E m E + m ( s) ( s ) B χ, ( s) ( s) ( s) A σ. p u ( E m) u B σ. p u ( E + m) u A A B Nega;ve energy 4- spnor solu;ons of Drac s equa;on u (s+2) N ' σ.p E + m χ (s) χ (s), E < 0, s 1,2 Orthonormal states ( r) ( s) u u 0, r s Non- rela;vs;c correspondance (1) ( mc / ) t 0 (2) ( mc / ) t 1 (3) ( mc / ) t 0 (4) ( mc / ) t 0 e!, e!, e +!, e +!

28 Spn for state at rest p (1) ( mc / ) t 0 (2) ( mc / ) t 1 (3) ( mc / ) t 0 (4) ( mc / ) t 0 e!, e!, e +!, e +! Snce we have a (two- fold) degeneracy there must be some operator whch commutes wth the energy operator and whose egenvalues label the two states σ Σ 3 0 σ 3 (1,2) (1,2) Egenvalues ± 1 Σ ± σ Σ 0 0 σ ( ) 2 3 2! Σ! I,! Σ has egenvalues ±! ! Σ s spn operator S correspondng to S

29 Spn for state NOT at rest p [ H] [ α P βm]! Σ no longer a commutng observable! Σ,! Σ,. + 0 Helcty!! 1 σ. p 0 Σ. p ",! p 2 0 σ.! p p p 0 σ I 0 α β σ 0 0 I s Egenvalues 1 +! 2 p s 1! 2 p (More generally, n arbtrary frame, spn gven by boos;ng result at rest - s µ (0, s) s ' µ Λ µ s ν ν )

30

Advanced Quantum Mechanics

Advanced Quantum Mechanics Advanced Quantum Mechancs Rajdeep Sensarma! sensarma@theory.tfr.res.n ecture #9 QM of Relatvstc Partcles Recap of ast Class Scalar Felds and orentz nvarant actons Complex Scalar Feld and Charge conjugaton

More information

Lecture 6/7 (February 10/12, 2014) DIRAC EQUATION. The non-relativistic Schrödinger equation was obtained by noting that the Hamiltonian 2

Lecture 6/7 (February 10/12, 2014) DIRAC EQUATION. The non-relativistic Schrödinger equation was obtained by noting that the Hamiltonian 2 P470 Lecture 6/7 (February 10/1, 014) DIRAC EQUATION The non-relatvstc Schrödnger equaton was obtaned by notng that the Hamltonan H = P (1) m can be transformed nto an operator form wth the substtutons

More information

Lorentz Group. Ling Fong Li. 1 Lorentz group Generators Simple representations... 3

Lorentz Group. Ling Fong Li. 1 Lorentz group Generators Simple representations... 3 Lorentz Group Lng Fong L ontents Lorentz group. Generators............................................. Smple representatons..................................... 3 Lorentz group In the dervaton of Drac

More information

The Lorentz and Poincaré groups. By Joel Oredsson

The Lorentz and Poincaré groups. By Joel Oredsson The Lorentz and Poincaré groups By Joel Oredsson The Principle of Special Rela=vity: The laws of nature should be covariant with respect to the transforma=ons between iner=al reference frames. x µ x' µ

More information

Note 2. Ling fong Li. 1 Klein Gordon Equation Probablity interpretation Solutions to Klein-Gordon Equation... 2

Note 2. Ling fong Li. 1 Klein Gordon Equation Probablity interpretation Solutions to Klein-Gordon Equation... 2 Note 2 Lng fong L Contents Ken Gordon Equaton. Probabty nterpretaton......................................2 Soutons to Ken-Gordon Equaton............................... 2 2 Drac Equaton 3 2. Probabty nterpretaton.....................................

More information

Representation theory and quantum mechanics tutorial Representation theory and quantum conservation laws

Representation theory and quantum mechanics tutorial Representation theory and quantum conservation laws Representaton theory and quantum mechancs tutoral Representaton theory and quantum conservaton laws Justn Campbell August 1, 2017 1 Generaltes on representaton theory 1.1 Let G GL m (R) be a real algebrac

More information

Quantum Mechanics I - Session 4

Quantum Mechanics I - Session 4 Quantum Mechancs I - Sesson 4 Aprl 3, 05 Contents Operators Change of Bass 4 3 Egenvectors and Egenvalues 5 3. Denton....................................... 5 3. Rotaton n D....................................

More information

C/CS/Phy191 Problem Set 3 Solutions Out: Oct 1, 2008., where ( 00. ), so the overall state of the system is ) ( ( ( ( 00 ± 11 ), Φ ± = 1

C/CS/Phy191 Problem Set 3 Solutions Out: Oct 1, 2008., where ( 00. ), so the overall state of the system is ) ( ( ( ( 00 ± 11 ), Φ ± = 1 C/CS/Phy9 Problem Set 3 Solutons Out: Oct, 8 Suppose you have two qubts n some arbtrary entangled state ψ You apply the teleportaton protocol to each of the qubts separately What s the resultng state obtaned

More information

Homework & Solution. Contributors. Prof. Lee, Hyun Min. Particle Physics Winter School. Park, Ye

Homework & Solution. Contributors. Prof. Lee, Hyun Min. Particle Physics Winter School. Park, Ye Homework & Soluton Prof. Lee, Hyun Mn Contrbutors Park, Ye J(yej.park@yonse.ac.kr) Lee, Sung Mook(smlngsm0919@gmal.com) Cheong, Dhong Yeon(dhongyeoncheong@gmal.com) Ban, Ka Young(ban94gy@yonse.ac.kr) Ro,

More information

763622S ADVANCED QUANTUM MECHANICS Solution Set 1 Spring c n a n. c n 2 = 1.

763622S ADVANCED QUANTUM MECHANICS Solution Set 1 Spring c n a n. c n 2 = 1. 7636S ADVANCED QUANTUM MECHANICS Soluton Set 1 Sprng 013 1 Warm-up Show that the egenvalues of a Hermtan operator  are real and that the egenkets correspondng to dfferent egenvalues are orthogonal (b)

More information

Scattering of two identical particles in the center-of. of-mass frame. (b)

Scattering of two identical particles in the center-of. of-mass frame. (b) Lecture # November 5 Scatterng of two dentcal partcle Relatvtc Quantum Mechanc: The Klen-Gordon equaton Interpretaton of the Klen-Gordon equaton The Drac equaton Drac repreentaton for the matrce α and

More information

Canonical transformations

Canonical transformations Canoncal transformatons November 23, 2014 Recall that we have defned a symplectc transformaton to be any lnear transformaton M A B leavng the symplectc form nvarant, Ω AB M A CM B DΩ CD Coordnate transformatons,

More information

Lagrangian Field Theory

Lagrangian Field Theory Lagrangan Feld Theory Adam Lott PHY 391 Aprl 6, 017 1 Introducton Ths paper s a summary of Chapter of Mandl and Shaw s Quantum Feld Theory [1]. The frst thng to do s to fx the notaton. For the most part,

More information

NMT EE 589 & UNM ME 482/582 ROBOT ENGINEERING. Dr. Stephen Bruder NMT EE 589 & UNM ME 482/582

NMT EE 589 & UNM ME 482/582 ROBOT ENGINEERING. Dr. Stephen Bruder NMT EE 589 & UNM ME 482/582 NMT EE 589 & UNM ME 48/58 ROBOT ENGINEERING Dr. Stephen Bruder NMT EE 589 & UNM ME 48/58 7. Robot Dynamcs 7.5 The Equatons of Moton Gven that we wsh to fnd the path q(t (n jont space) whch mnmzes the energy

More information

Homework Notes Week 7

Homework Notes Week 7 Homework Notes Week 7 Math 4 Sprng 4 #4 (a Complete the proof n example 5 that s an nner product (the Frobenus nner product on M n n (F In the example propertes (a and (d have already been verfed so we

More information

Mechanics Physics 151

Mechanics Physics 151 Mechancs Physcs 5 Lecture 7 Specal Relatvty (Chapter 7) What We Dd Last Tme Worked on relatvstc knematcs Essental tool for epermental physcs Basc technques are easy: Defne all 4 vectors Calculate c-o-m

More information

PHYS 215C: Quantum Mechanics (Spring 2017) Problem Set 3 Solutions

PHYS 215C: Quantum Mechanics (Spring 2017) Problem Set 3 Solutions PHYS 5C: Quantum Mechancs Sprng 07 Problem Set 3 Solutons Prof. Matthew Fsher Solutons prepared by: Chatanya Murthy and James Sully June 4, 07 Please let me know f you encounter any typos n the solutons.

More information

arxiv: v2 [quant-ph] 29 Jun 2018

arxiv: v2 [quant-ph] 29 Jun 2018 Herarchy of Spn Operators, Quantum Gates, Entanglement, Tensor Product and Egenvalues Wll-Hans Steeb and Yorck Hardy arxv:59.7955v [quant-ph] 9 Jun 8 Internatonal School for Scentfc Computng, Unversty

More information

Chapter 1 LORENTZ/POINCARE INVARIANCE. 1.1 The Lorentz Algebra

Chapter 1 LORENTZ/POINCARE INVARIANCE. 1.1 The Lorentz Algebra Chapter 1 LORENTZ/POINCARE INVARIANCE 1.1 The Lorentz Algebra The requirement of relativistic invariance on any fundamental physical system amounts to invariance under Lorentz Transformations. These transformations

More information

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama Lorentz-covariant spectrum of single-particle states and their field theory Physics 30A, Spring 007, Hitoshi Murayama 1 Poincaré Symmetry In order to understand the number of degrees of freedom we need

More information

Quantum Mechanics I Problem set No.1

Quantum Mechanics I Problem set No.1 Quantum Mechancs I Problem set No.1 Septembe0, 2017 1 The Least Acton Prncple The acton reads S = d t L(q, q) (1) accordng to the least (extremal) acton prncple, the varaton of acton s zero 0 = δs = t

More information

Quantum Mechanics for Scientists and Engineers. David Miller

Quantum Mechanics for Scientists and Engineers. David Miller Quantum Mechancs for Scentsts and Engneers Davd Mller Types of lnear operators Types of lnear operators Blnear expanson of operators Blnear expanson of lnear operators We know that we can expand functons

More information

Lecture 9/10 (February 19/24, 2014) DIRAC EQUATION(III) i 2. ( x) σ = = Equation 66 is similar to the rotation of two-component Pauli spinor ( ) ( )

Lecture 9/10 (February 19/24, 2014) DIRAC EQUATION(III) i 2. ( x) σ = = Equation 66 is similar to the rotation of two-component Pauli spinor ( ) ( ) P47 For a Lorentz boost along the x-axis, Lecture 9/ (February 9/4, 4) DIRAC EQUATION(III) i ψ ωσ ψ ω exp α ψ ( x) ( x ) exp ( x) (65) where tanh ω β, cosh ω γ, sinh ω βγ β imilarly, for a rotation around

More information

The Lorentz and Poincaré Groups in Relativistic Field Theory

The Lorentz and Poincaré Groups in Relativistic Field Theory The and s in Relativistic Field Theory Term Project Nicolás Fernández González University of California Santa Cruz June 2015 1 / 14 the Our first encounter with the group is in special relativity it composed

More information

Unification Paradigm

Unification Paradigm Unfcaton Paradgm GUT 34 10 m D=10 Unfcaton of strong, weak and electromagnetc nteractons wthn Grand Unfed Theores s the new step n unfcaton of all forces of Nature Creaton of a unfed theory of everythng

More information

HW #6, due Oct Toy Dirac Model, Wick s theorem, LSZ reduction formula. Consider the following quantum mechanics Lagrangian,

HW #6, due Oct Toy Dirac Model, Wick s theorem, LSZ reduction formula. Consider the following quantum mechanics Lagrangian, HW #6, due Oct 5. Toy Drac Model, Wck s theorem, LSZ reducton formula. Consder the followng quantum mechancs Lagrangan, L ψ(σ 3 t m)ψ, () where σ 3 s a Paul matrx, and ψ s defned by ψ ψ σ 3. ψ s a twocomponent

More information

Note on the Electron EDM

Note on the Electron EDM Note on the Electron EDM W R Johnson October 25, 2002 Abstract Ths s a note on the setup of an electron EDM calculaton and Schff s Theorem 1 Basc Relatons The well-known relatvstc nteracton of the electron

More information

A particle in a state of uniform motion remain in that state of motion unless acted upon by external force.

A particle in a state of uniform motion remain in that state of motion unless acted upon by external force. The fundamental prncples of classcal mechancs were lad down by Galleo and Newton n the 16th and 17th centures. In 1686, Newton wrote the Prncpa where he gave us three laws of moton, one law of gravty,

More information

Yukawa Potential and the Propagator Term

Yukawa Potential and the Propagator Term PHY304 Partcle Physcs 4 Dr C N Booth Yukawa Potental an the Propagator Term Conser the electrostatc potental about a charge pont partcle Ths s gven by φ = 0, e whch has the soluton φ = Ths escrbes the

More information

Disclaimer. [disclaimer]

Disclaimer. [disclaimer] Disclaimer This is a problem set (as turned in) for the module physics755. This problem set is not reviewed by a tutor. This is just what I have turned in. All problem sets for this module can be found

More information

This model contains two bonds per unit cell (one along the x-direction and the other along y). So we can rewrite the Hamiltonian as:

This model contains two bonds per unit cell (one along the x-direction and the other along y). So we can rewrite the Hamiltonian as: 1 Problem set #1 1.1. A one-band model on a square lattce Fg. 1 Consder a square lattce wth only nearest-neghbor hoppngs (as shown n the fgure above): H t, j a a j (1.1) where,j stands for nearest neghbors

More information

The Dirac Field. Physics , Quantum Field Theory. October Michael Dine Department of Physics University of California, Santa Cruz

The Dirac Field. Physics , Quantum Field Theory. October Michael Dine Department of Physics University of California, Santa Cruz Michael Dine Department of Physics University of California, Santa Cruz October 2013 Lorentz Transformation Properties of the Dirac Field First, rotations. In ordinary quantum mechanics, ψ σ i ψ (1) is

More information

MSci EXAMINATION. Date: XX th May, Time: 14:30-17:00

MSci EXAMINATION. Date: XX th May, Time: 14:30-17:00 MSci EXAMINATION PHY-415 (MSci 4242 Relativistic Waves and Quantum Fields Time Allowed: 2 hours 30 minutes Date: XX th May, 2010 Time: 14:30-17:00 Instructions: Answer THREE QUESTIONS only. Each question

More information

Srednicki Chapter 34

Srednicki Chapter 34 Srednck Chapter 3 QFT Problems & Solutons A. George January 0, 203 Srednck 3.. Verfy that equaton 3.6 follows from equaton 3.. We take Λ = + δω: U + δω ψu + δω = + δωψ[ + δω] x Next we use equaton 3.3,

More information

Foldy-Wouthuysen Transformation with Dirac Matrices in Chiral Representation. V.P.Neznamov RFNC-VNIIEF, , Sarov, Nizhniy Novgorod region

Foldy-Wouthuysen Transformation with Dirac Matrices in Chiral Representation. V.P.Neznamov RFNC-VNIIEF, , Sarov, Nizhniy Novgorod region Foldy-Wouthuysen Transormaton wth Drac Matrces n Chral Representaton V.P.Neznamov RFNC-VNIIEF, 679, Sarov, Nzhny Novgorod regon Abstract The paper oers an expresson o the general Foldy-Wouthuysen transormaton

More information

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 6: Lectures 11, 12

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 6: Lectures 11, 12 As usual, these notes are intended for use by class participants only, and are not for circulation Week 6: Lectures, The Dirac equation and algebra March 5, 0 The Lagrange density for the Dirac equation

More information

A Short Note on D=3 N=1 Supergravity

A Short Note on D=3 N=1 Supergravity A Short Note on D=3 N=1 Supergravity Sunny Guha December 13, 015 1 Why 3-dimensional gravity? Three-dimensional field theories have a number of unique features, the massless states do not carry helicity,

More information

11 Spinor solutions and CPT

11 Spinor solutions and CPT 11 Spinor solutions and CPT 184 In the previous chapter, we cataloged the irreducible representations of the Lorentz group O(1, 3. We found that in addition to the obvious tensor representations, φ, A

More information

Solution 1 for USTC class Physics of Quantum Information

Solution 1 for USTC class Physics of Quantum Information Soluton 1 for 017 018 USTC class Physcs of Quantum Informaton Shua Zhao, Xn-Yu Xu and Ka Chen Natonal Laboratory for Physcal Scences at Mcroscale and Department of Modern Physcs, Unversty of Scence and

More information

8.4 COMPLEX VECTOR SPACES AND INNER PRODUCTS

8.4 COMPLEX VECTOR SPACES AND INNER PRODUCTS SECTION 8.4 COMPLEX VECTOR SPACES AND INNER PRODUCTS 493 8.4 COMPLEX VECTOR SPACES AND INNER PRODUCTS All the vector spaces you have studed thus far n the text are real vector spaces because the scalars

More information

This chapter illustrates the idea that all properties of the homogeneous electron gas (HEG) can be calculated from electron density.

This chapter illustrates the idea that all properties of the homogeneous electron gas (HEG) can be calculated from electron density. 1 Unform Electron Gas Ths chapter llustrates the dea that all propertes of the homogeneous electron gas (HEG) can be calculated from electron densty. Intutve Representaton of Densty Electron densty n s

More information

ψ = i c i u i c i a i b i u i = i b 0 0 b 0 0

ψ = i c i u i c i a i b i u i = i b 0 0 b 0 0 Quantum Mechancs, Advanced Course FMFN/FYSN7 Solutons Sheet Soluton. Lets denote the two operators by  and ˆB, the set of egenstates by { u }, and the egenvalues as  u = a u and ˆB u = b u. Snce the

More information

7. Products and matrix elements

7. Products and matrix elements 7. Products and matrx elements 1 7. Products and matrx elements Based on the propertes of group representatons, a number of useful results can be derved. Consder a vector space V wth an nner product ψ

More information

Solution 1 for USTC class Physics of Quantum Information

Solution 1 for USTC class Physics of Quantum Information Soluton 1 for 018 019 USTC class Physcs of Quantum Informaton Shua Zhao, Xn-Yu Xu and Ka Chen Natonal Laboratory for Physcal Scences at Mcroscale and Department of Modern Physcs, Unversty of Scence and

More information

Spinor Formulation of Relativistic Quantum Mechanics

Spinor Formulation of Relativistic Quantum Mechanics Chapter Spinor Formulation of Relativistic Quantum Mechanics. The Lorentz Transformation of the Dirac Bispinor We will provide in the following a new formulation of the Dirac equation in the chiral representation

More information

SL n (F ) Equals its Own Derived Group

SL n (F ) Equals its Own Derived Group Internatonal Journal of Algebra, Vol. 2, 2008, no. 12, 585-594 SL n (F ) Equals ts Own Derved Group Jorge Macel BMCC-The Cty Unversty of New York, CUNY 199 Chambers street, New York, NY 10007, USA macel@cms.nyu.edu

More information

The Dirac Equation. Elementary Particle Physics Strong Interaction Fenomenology. Diego Bettoni Academic year

The Dirac Equation. Elementary Particle Physics Strong Interaction Fenomenology. Diego Bettoni Academic year The Drac Equaton Eleentary artcle hyscs Strong Interacton Fenoenology Dego Betton Acadec year - D Betton Fenoenologa Interazon Fort elatvstc equaton to descrbe the electron (ncludng ts sn) Conservaton

More information

THEOREMS OF QUANTUM MECHANICS

THEOREMS OF QUANTUM MECHANICS THEOREMS OF QUANTUM MECHANICS In order to develop methods to treat many-electron systems (atoms & molecules), many of the theorems of quantum mechancs are useful. Useful Notaton The matrx element A mn

More information

5.76 Lecture #5 2/07/94 Page 1 of 10 pages. Lecture #5: Atoms: 1e and Alkali. centrifugal term ( +1)

5.76 Lecture #5 2/07/94 Page 1 of 10 pages. Lecture #5: Atoms: 1e and Alkali. centrifugal term ( +1) 5.76 Lecture #5 /07/94 Page 1 of 10 pages 1e Atoms: H, H + e, L +, etc. coupled and uncoupled bass sets Lecture #5: Atoms: 1e and Alkal centrfugal term (+1) r radal Schrödnger Equaton spn-orbt l s r 3

More information

Change. Flamenco Chuck Keyser. Updates 11/26/2017, 11/28/2017, 11/29/2017, 12/05/2017. Most Recent Update 12/22/2017

Change. Flamenco Chuck Keyser. Updates 11/26/2017, 11/28/2017, 11/29/2017, 12/05/2017. Most Recent Update 12/22/2017 Change Flamenco Chuck Keyser Updates /6/7, /8/7, /9/7, /5/7 Most Recent Update //7 The Relatvstc Unt Crcle (ncludng proof of Fermat s Theorem) Relatvty Page (n progress, much more to be sad, and revsons

More information

T 1! p k. = T r! k., s k. ', x' ] = i!, s y. ', s y

T 1! p k. = T r! k., s k. ', x' ] = i!, s y. ', s y Time Reversal r k ' = r k = T r k T 1 p k ' = p k, s k ' = s k T cannot be represented by an unitary operator. Unitary opera$ons preserve algebraic rela$ons between operators, while T changes the sign

More information

Question 1: Axiomatic Newtonian mechanics

Question 1: Axiomatic Newtonian mechanics February 9, 017 Cornell University, Department of Physics PHYS 4444, Particle physics, HW # 1, due: //017, 11:40 AM Question 1: Axiomatic Newtonian mechanics In this question you are asked to develop Newtonian

More information

Spin one matter elds. November 2015

Spin one matter elds. November 2015 Spin one matter elds M. Napsuciale, S. Rodriguez, R.Ferro-Hernández, S. Gomez-Ávila Universidad de Guanajuato Mexican Workshop on Particles and Fields November 2015 M. Napsuciale, S. Rodriguez, R.Ferro-Hernández,

More information

Exercises Symmetries in Particle Physics

Exercises Symmetries in Particle Physics Exercises Symmetries in Particle Physics 1. A particle is moving in an external field. Which components of the momentum p and the angular momentum L are conserved? a) Field of an infinite homogeneous plane.

More information

QCD Lagrangian. ψ qi. δ ij. ψ i L QCD. m q. = ψ qi. G α µν = µ G α ν ν G α µ gf αβγ G β µ G γ. G α t α f αβγ. g = 4πα s. (!

QCD Lagrangian. ψ qi. δ ij. ψ i L QCD. m q. = ψ qi. G α µν = µ G α ν ν G α µ gf αβγ G β µ G γ. G α t α f αβγ. g = 4πα s. (! QCD Lagrangian L QCD = ψ qi iγ µ! δ ij µ + ig G α µ t $ "# α %& ψ qj m q ψ qi ψ qi 1 4 G µν q ( ( ) ) ij L QED = ψ e iγ µ!" µ + iea µ # $ ψ e m e ψ e ψ e 1 4 F F µν µν α G α µν G α µν = µ G α ν ν G α µ

More information

N.T.Phong Y.H.Ahn YongPhyong Yonsei Univ.

N.T.Phong Y.H.Ahn YongPhyong Yonsei Univ. Leptogeness n a seesaw model wth Frtzsch type lepton mass matrces N.T.Phong Y.H.hn 008. 0. 6 YongPhyong Yonse Unv. Introducton Present knowledge of Neutrno data (at 3 σ ) hep-ph/040517 Mxng ngles 0.3 Sn

More information

1 4-dimensional Weyl spinor

1 4-dimensional Weyl spinor 4-dimensional Weyl spinor Left moving ψ α, α =, Right moving ψ α, α =, They are related by the complex conjugation. The indices are raised or lowerd by the ϵ tensor as ψ α := ϵ αβ ψ β, α := ϵ α β β. (.)

More information

Ph 219a/CS 219a. Exercises Due: Wednesday 12 November 2008

Ph 219a/CS 219a. Exercises Due: Wednesday 12 November 2008 1 Ph 19a/CS 19a Exercses Due: Wednesday 1 November 008.1 Whch state dd Alce make? Consder a game n whch Alce prepares one of two possble states: ether ρ 1 wth a pror probablty p 1, or ρ wth a pror probablty

More information

Lecture 4 - Relativistic wave equations. Relativistic wave equations must satisfy several general postulates. These are;

Lecture 4 - Relativistic wave equations. Relativistic wave equations must satisfy several general postulates. These are; Lecture 4 - Relativistic wave equations Postulates Relativistic wave equations must satisfy several general postulates. These are;. The equation is developed for a field amplitude function, ψ 2. The normal

More information

= = = (a) Use the MATLAB command rref to solve the system. (b) Let A be the coefficient matrix and B be the right-hand side of the system.

= = = (a) Use the MATLAB command rref to solve the system. (b) Let A be the coefficient matrix and B be the right-hand side of the system. Chapter Matlab Exercses Chapter Matlab Exercses. Consder the lnear system of Example n Secton.. x x x y z y y z (a) Use the MATLAB command rref to solve the system. (b) Let A be the coeffcent matrx and

More information

Übungen zur Elektrodynamik (T3)

Übungen zur Elektrodynamik (T3) Arnold Sommerfeld Center Ludwig Maximilians Universität München Prof. Dr. Ivo Sachs SoSe 08 Übungen zur Elektrodynamik (T3) Lösungen zum Übungsblatt 7 Lorentz Force Calculate dx µ and ds explicitly in

More information

SPECIAL RELATIVITY AND ELECTROMAGNETISM

SPECIAL RELATIVITY AND ELECTROMAGNETISM SPECIAL RELATIVITY AND ELECTROMAGNETISM MATH 460, SECTION 500 The following problems (composed by Professor P.B. Yasskin) will lead you through the construction of the theory of electromagnetism in special

More information

EML 5223 Structural Dynamics HW 10. Gun Lee(UFID )

EML 5223 Structural Dynamics HW 10. Gun Lee(UFID ) E 5 Structural Dynamcs HW Gun ee(ufid895-47) Problem 9. ubular shaft of radus r ( ) r[ + ( )/ ], thcknesst, mass per unt volume ρ and shear modulus G. t r( ). Shaft s symmetrc wth respect to /. ass moment

More information

Instructor: Sudipta Mukherji, Institute of Physics, Bhubaneswar

Instructor: Sudipta Mukherji, Institute of Physics, Bhubaneswar Chapter 1 Lorentz and Poincare Instructor: Sudipta Mukherji, Institute of Physics, Bhubaneswar 1.1 Lorentz Transformation Consider two inertial frames S and S, where S moves with a velocity v with respect

More information

Mechanics Physics 151

Mechanics Physics 151 Mechancs Physcs 151 Lecture 3 Lagrange s Equatons (Goldsten Chapter 1) Hamlton s Prncple (Chapter 2) What We Dd Last Tme! Dscussed mult-partcle systems! Internal and external forces! Laws of acton and

More information

On Finite Rank Perturbation of Diagonalizable Operators

On Finite Rank Perturbation of Diagonalizable Operators Functonal Analyss, Approxmaton and Computaton 6 (1) (2014), 49 53 Publshed by Faculty of Scences and Mathematcs, Unversty of Nš, Serba Avalable at: http://wwwpmfnacrs/faac On Fnte Rank Perturbaton of Dagonalzable

More information

Math. 460, Sec. 500 Fall, Special Relativity and Electromagnetism

Math. 460, Sec. 500 Fall, Special Relativity and Electromagnetism Math. 460, Sec. 500 Fall, 2011 Special Relativity and Electromagnetism The following problems (composed by Professor P. B. Yasskin) will lead you through the construction of the theory of electromagnetism

More information

Introduction to relativistic quantum mechanics

Introduction to relativistic quantum mechanics Introduction to relativistic quantum mechanics. Tensor notation In this book, we will most often use so-called natural units, which means that we have set c = and =. Furthermore, a general 4-vector will

More information

Lie Algebra Cohomology and the Borel-Weil-Bott Theorem. 1 Lie algebra cohomology and cohomology of G/T with coefficients in a line bundle

Lie Algebra Cohomology and the Borel-Weil-Bott Theorem. 1 Lie algebra cohomology and cohomology of G/T with coefficients in a line bundle Le Algebra Cohomology and the Borel-Wel-Bott Theorem Math G4344, Sprng 2012 We have seen that rreducble fnte dmensonal representatons of a complex smple Le algebra g or correspondng compact Le group are

More information

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK7003 08 SU() Isospin Isospin introduced based on the observa4on that: m p =

More information

The Feynman path integral

The Feynman path integral The Feynman path ntegral Aprl 3, 205 Hesenberg and Schrödnger pctures The Schrödnger wave functon places the tme dependence of a physcal system n the state, ψ, t, where the state s a vector n Hlbert space

More information

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK7003 33 SU() Isospin Isospin introduced based on the observa4on that: m p = 0.9383 GeV and

More information

Non-Abelian Berry phase and Chern numbers in higher spin-pairing condensates

Non-Abelian Berry phase and Chern numbers in higher spin-pairing condensates PHYSICAL REVIEW B 69, 2452 (2004) Non-Abelan Berry phase and Chern numbers n hgher spn-parng condensates Chyh-Hong Chern, Han-Dong Chen, 2 Congjun Wu, Jang-Png Hu, 3 and Shou-Cheng Zhang Department of

More information

Physics 513, Quantum Field Theory Homework 4 Due Tuesday, 30th September 2003

Physics 513, Quantum Field Theory Homework 4 Due Tuesday, 30th September 2003 PHYSICS 513: QUANTUM FIELD THEORY HOMEWORK 1 Physics 513, Quantum Fiel Theory Homework Due Tuesay, 30th September 003 Jacob Lewis Bourjaily 1. We have efine the coherent state by the relation { } 3 k η

More information

232A Lecture Notes Representation Theory of Lorentz Group

232A Lecture Notes Representation Theory of Lorentz Group 232A Lecture Notes Representation Theory of Lorentz Group 1 Symmetries in Physics Symmetries play crucial roles in physics. Noether s theorem relates symmetries of the system to conservation laws. In quantum

More information

Spin. Introduction. Michael Fowler 11/26/06

Spin. Introduction. Michael Fowler 11/26/06 Spn Mchael Fowler /6/6 Introducton The Stern Gerlach experment for the smplest possble atom, hydrogen n ts ground state, demonstrated unambguously that the component of the magnetc moment of the atom along

More information

Appendix A List of Symbols, Notation, and Useful Expressions

Appendix A List of Symbols, Notation, and Useful Expressions Appendx A Lst of Symbols, Notaton, and Useful Expressons In ths appendx the reader wll fnd a more detaled descrpton of the conventons and notaton used throughout ths book, together wth a bref descrpton

More information

Introduction to Modern Quantum Field Theory

Introduction to Modern Quantum Field Theory Department of Mathematics University of Texas at Arlington Arlington, TX USA Febuary, 2016 Recall Einstein s famous equation, E 2 = (Mc 2 ) 2 + (c p) 2, where c is the speed of light, M is the classical

More information

Notes on Analytical Dynamics

Notes on Analytical Dynamics Notes on Analytcal Dynamcs Jan Peters & Mchael Mstry October 7, 004 Newtonan Mechancs Basc Asssumptons and Newtons Laws Lonely pontmasses wth postve mass Newtons st: Constant velocty v n an nertal frame

More information

Towards a finite conformal QED

Towards a finite conformal QED Towards a fnte conformal QED A D Alhadar Saud Center for Theoretcal Physcs P O Box 3741 Jeddah 143 Saud Araba In 196 whle at UCLA workng wth C Fronsdal and M Flato I proposed a model for conformal QED

More information

9 Characteristic classes

9 Characteristic classes THEODORE VORONOV DIFFERENTIAL GEOMETRY. Sprng 2009 [under constructon] 9 Characterstc classes 9.1 The frst Chern class of a lne bundle Consder a complex vector bundle E B of rank p. We shall construct

More information

Fermi-Dirac statistics

Fermi-Dirac statistics UCC/Physcs/MK/EM/October 8, 205 Fer-Drac statstcs Fer-Drac dstrbuton Matter partcles that are eleentary ostly have a type of angular oentu called spn. hese partcles are known to have a agnetc oent whch

More information

Elementary Par,cles Rohlf Ch , p474 et seq.

Elementary Par,cles Rohlf Ch , p474 et seq. Elementary Par,cles Rohlf Ch. 17-18, p474 et seq. The Schroedinger equa,on is non- rela,vis,c. Rela,vis,c wave equa,on (Klein- Gordon eq.) Rela,vis,c equa,on connec,ng the energy and momentum of a free

More information

A how to guide to second quantization method.

A how to guide to second quantization method. Phys. 67 (Graduate Quantum Mechancs Sprng 2009 Prof. Pu K. Lam. Verson 3 (4/3/2009 A how to gude to second quantzaton method. -> Second quantzaton s a mathematcal notaton desgned to handle dentcal partcle

More information

Representations of Lorentz Group

Representations of Lorentz Group Representations of Lorentz Group based on S-33 We defined a unitary operator that implemented a Lorentz transformation on a scalar field: How do we find the smallest (irreducible) representations of the

More information

ECEN 5005 Crystals, Nanocrystals and Device Applications Class 19 Group Theory For Crystals

ECEN 5005 Crystals, Nanocrystals and Device Applications Class 19 Group Theory For Crystals ECEN 5005 Crystals, Nanocrystals and Devce Applcatons Class 9 Group Theory For Crystals Dee Dagram Radatve Transton Probablty Wgner-Ecart Theorem Selecton Rule Dee Dagram Expermentally determned energy

More information

E 2 = p 2 + m 2. [J i, J j ] = iɛ ijk J k

E 2 = p 2 + m 2. [J i, J j ] = iɛ ijk J k 3.1. KLEIN GORDON April 17, 2015 Lecture XXXI Relativsitic Quantum Mechanics 3.1 Klein Gordon Before we get to the Dirac equation, let s consider the most straightforward derivation of a relativistically

More information

GRAVITATION F10. Lecture Maxwell s Equations in Curved Space-Time 1.1. Recall that Maxwell equations in Lorentz covariant form are.

GRAVITATION F10. Lecture Maxwell s Equations in Curved Space-Time 1.1. Recall that Maxwell equations in Lorentz covariant form are. GRAVITATION F0 S. G. RAJEEV Lecture. Maxwell s Equations in Curved Space-Time.. Recall that Maxwell equations in Lorentz covariant form are. µ F µν = j ν, F µν = µ A ν ν A µ... They follow from the variational

More information

1 Matrix representations of canonical matrices

1 Matrix representations of canonical matrices 1 Matrx representatons of canoncal matrces 2-d rotaton around the orgn: ( ) cos θ sn θ R 0 = sn θ cos θ 3-d rotaton around the x-axs: R x = 1 0 0 0 cos θ sn θ 0 sn θ cos θ 3-d rotaton around the y-axs:

More information

CS 468 Lecture 16: Isometry Invariance and Spectral Techniques

CS 468 Lecture 16: Isometry Invariance and Spectral Techniques CS 468 Lecture 16: Isometry Invarance and Spectral Technques Justn Solomon Scrbe: Evan Gawlk Introducton. In geometry processng, t s often desrable to characterze the shape of an object n a manner that

More information

Errata to Invariant Theory with Applications January 28, 2017

Errata to Invariant Theory with Applications January 28, 2017 Invarant Theory wth Applcatons Jan Drasma and Don Gjswjt http: //www.wn.tue.nl/~jdrasma/teachng/nvtheory0910/lecturenotes12.pdf verson of 7 December 2009 Errata and addenda by Darj Grnberg The followng

More information

Neutrino Mass, Dark Matter, and Leptogenesis

Neutrino Mass, Dark Matter, and Leptogenesis UCRHEP-T44 November 006 arxv:hep-ph/0611181v1 13 Nov 006 Neutrno Mass, Dark Matter, and Leptogeness Ernest Ma Physcs and Astronomy Department, Unversty of Calforna, Rversde, Calforna 951 Abstract It s

More information

1 Vectors over the complex numbers

1 Vectors over the complex numbers Vectors for quantum mechancs 1 D. E. Soper 2 Unversty of Oregon 5 October 2011 I offer here some background for Chapter 1 of J. J. Sakura, Modern Quantum Mechancs. 1 Vectors over the complex numbers What

More information

Tensor Analysis. For orthogonal curvilinear coordinates, ˆ ˆ (98) Expanding the derivative, we have, ˆ. h q. . h q h q

Tensor Analysis. For orthogonal curvilinear coordinates, ˆ ˆ (98) Expanding the derivative, we have, ˆ. h q. . h q h q For orthogonal curvlnear coordnates, eˆ grad a a= ( aˆ ˆ e). h q (98) Expandng the dervatve, we have, eˆ aˆ ˆ e a= ˆ ˆ a h e + q q 1 aˆ ˆ ˆ a e = ee ˆˆ ˆ + e. h q h q Now expandng eˆ / q (some of the detals

More information

MEM633 Lectures 7&8. Chapter 4. Descriptions of MIMO Systems 4-1 Direct Realizations. (i) x u. y x

MEM633 Lectures 7&8. Chapter 4. Descriptions of MIMO Systems 4-1 Direct Realizations. (i) x u. y x MEM633 Lectures 7&8 Chapter 4 Descrptons of MIMO Systems 4- Drect ealzatons y() s s su() s y () s u () s ( s)( s) s y() s u (), s y() s u() s s s y() s u(), s y() s u() s ( s)( s) s () ( s ) y ( s) u (

More information

Attempts at relativistic QM

Attempts at relativistic QM Attempts at relativistic QM based on S-1 A proper description of particle physics should incorporate both quantum mechanics and special relativity. However historically combining quantum mechanics and

More information

24. Atomic Spectra, Term Symbols and Hund s Rules

24. Atomic Spectra, Term Symbols and Hund s Rules Page of 4. Atomc Spectra, Term Symbols and Hund s Rules Date: 5 October 00 Suggested Readng: Chapters 8-8 to 8- of the text. Introducton Electron confguratons, at least n the forms used n general chemstry

More information

5.03, Inorganic Chemistry Prof. Daniel G. Nocera Lecture 2 May 11: Ligand Field Theory

5.03, Inorganic Chemistry Prof. Daniel G. Nocera Lecture 2 May 11: Ligand Field Theory 5.03, Inorganc Chemstry Prof. Danel G. Nocera Lecture May : Lgand Feld Theory The lgand feld problem s defned by the followng Hamltonan, h p Η = wth E n = KE = where = m m x y z h m Ze r hydrogen atom

More information

Reevalua'on of Neutron Electric Dipole Moment with QCD Sum Rules

Reevalua'on of Neutron Electric Dipole Moment with QCD Sum Rules Reevalua'on of Neutron Electric Dipole Moment with QCD Sum Rules Natsumi Nagata Nagoya University Na1onal Taiwan University 5 November, 2012 J. Hisano, J. Y. Lee, N. Nagata, and Y. Shimizu, Phys. Rev.

More information

CONDITIONS FOR INVARIANT SUBMANIFOLD OF A MANIFOLD WITH THE (ϕ, ξ, η, G)-STRUCTURE. Jovanka Nikić

CONDITIONS FOR INVARIANT SUBMANIFOLD OF A MANIFOLD WITH THE (ϕ, ξ, η, G)-STRUCTURE. Jovanka Nikić 147 Kragujevac J. Math. 25 (2003) 147 154. CONDITIONS FOR INVARIANT SUBMANIFOLD OF A MANIFOLD WITH THE (ϕ, ξ, η, G)-STRUCTURE Jovanka Nkć Faculty of Techncal Scences, Unversty of Nov Sad, Trg Dosteja Obradovća

More information