Yang-Mills Yang-Mills Yang-Mills 50 operator formalism operator formalism 1 I The Dawning of Gauge T

Size: px
Start display at page:

Download "Yang-Mills Yang-Mills Yang-Mills 50 operator formalism operator formalism 1 I The Dawning of Gauge T"

Transcription

1 Yang-Mills Yang-Mills Yang-Mills 50 operator formalism operator formalism 1 I The Dawning of Gauge Theory O Raifeartaigh [1] I, II, III O Raifeartaigh I Weyl O Raifeartaigh Weyl Pauli Pauli Handbuch Yang Yang-Mills Weyl I 1918 Einstein Maxwell Weyl 1

2 1: I 1918 Weyl Gravitation and Electricity Scale transformation of metric: g µν (x) λ(x)g µν (x) 1921 Kaluza 5 g 5µ = 2αA µ 1926 Klein g 5µ /g 55 = A µ Schrödinger µ µ ie A µ 26 London ψ exp[ ie A]ψ 1929 Weyl Electron and Gravitation Zeit f. Physik { e ieλ(x) ψ(x) µ D µ = µ iea µ F µν = µ A ν ν A µ Klein SU(2) gauge theory in Conf. Report (Kazimierz, Poland) 49 -Schwinger-Feynman-Dyson QED 50 Gupta-Bleuler 1953 Pais isospin Pauli SU(2) gauge theory in two Letters to Pais 1954 Yang-Mills Phys. Rev. 96 (1954) Shaw SU(2) gauge theory in Ph.D. Thesis 56 Phys. Rev. 101 (1956) 1597 g µν (x) λ(x)g µν (x) φ µ (x) φ µ (x) + µ ln λ(x) φ µ Bohm-Aharanov Einstein Weyl 1925 Schrödinger London Schrödinger 1922 Weyl exp[(e/γ) φ µ dx µ ] γ Weyl γ = /i 2

3 Bohr-Sommerfeld e 2πni = µ µ ie A µ 1922 London Schrödinger Schrödinger Weyl exp[i(e/ ) A µ dx µ ] Weyl 1929 Zeit f. Physik U(1) ψ(x) e ieλ(x) ψ(x) D µ = µ ie A µ F µν 2 Weyl Pauli Weyl 1933 Fermi 1935 Klein Kaluza 5 5 SU(2) Yang-Mills Klein SU(2) SU(2)doublet 1938 Poland Kazimierz Proceedings 2 QED Pais 1953 Leiden Pauli Pais SU(2) Yang-Mills doublet doublet 1954 Yang-Mills Yang-Mills Pais Pauli Yang Pauli Handbuch Mills Yang Mills Yang-Mills Princeton Yang Yang-Mills? Pauli Oppenheimer Pauli Yang 3

4 O Raifeartaigh [1] Yang-Mills Shaw 2 II II Yang-Mills : II 1960 Gauge Invariance in Superconductivity 60 J.J. Sakurai Massive Yang-Mills for ρ 61 S. Glashow Massive Yang-Mills for W, Z 61 Goldstone 63 Feynman ghost Higgs 66 -Lautrup 67 Kibble 67 DeWitt ghost 67 Faddeev-Popov 1967 Weinberg-Salam Theory of Electron 69 Adler, Bell-Jackiw 1971 t Hooft Yang-Mills T.K CP 1973 Gross-Wilczek Asymptotic Freedom Politzer 73 Nakanishi N-L Higgs 1974 Ken Wilson Lattice Gauge Theory 1974 t Hooft-Polyakov monopole 75 Nielsen-Olsen vortex 75 Bogomol nyi-prasad-sommerfield (BPS) 1975 Becchi-Rouet-Stora, Tyutin BRS 78 Kugo-Ojima 79 Fujikawa path-int measure anomaly Q B phys = Nambu-Jona-Lasinio 1960 Phys.Rev. Quasi-Particles and Gauge Invariance in the Theory of Superconductivity [2] U(1) massless massive 4

5 Meissner Goldstone Higgs! Goldstone (61 ) Higgs (64,66 ) 1960 J.J.Sakurai Yang-Mills ρ ρ ( hidden local symmetry [3]) 1961 Glashow SU(2) U(1) Yang-Mills 61 Goldstone massless Higgs 67 Kibble massive Kibble SU(2) Weinberg-Salam Higgs Kibble Weinberg Weinberg Kibble? (Weinberg Glashow?) Weinberg-Salam ( ) Glashow-Illiopoulos-Miani 1970 ( Glashow- Weinberg-Salam ) charm 2-doublets FCNC GIM 71 t Hooft Yang-Mills Weinberg-Salam Weinberg-Salam 1973 (1972?) Weinberg- Salam CP? - t Hooft Lee-Zinn-Justin Yang-Mills R ξ Fujikawa-Lee-Sanda R ξ R ξ 5

6 Bethe-Salpeter Gross-Wilczek, Politzer Asymptotic Freedom t Hooft-Polyakov monopole Nielsen-Olsen vortex BPS 1974 t Hooft Lee-Zinn-Justin t Hooft-Veltman 1975 BRS BRS BRS-formalism operator formalism BRS BRS Yang-Mills Lagrangian S Faddeev-Popov (FP) ghost FP anti-ghost FP ghost t Hooft 1963 Feynman 1-loop ghost 67 DeWitt Faddeev Popov Veltman Faddeev-Popov t Hooft Veltman S S Hamiltonian Feynman QED Gupta-Bleuler formalism 6

7 1950 Feynman QED Lautrup ( ) Yang-Mills 1978 Kugo-Ojima [4] ( 77 ) Q B phys = 0 Q B (BRS exact states) BRS Q B phys = 0 Kugo-Ojima [4, 5] 1974 K.Wilson QCD Wilson quark confinement Atiyah-Singer 3 III 3 3: III 1984 Green-Schwarz Anomaly cancellation in d = 10 SYM with SO(32), E 8 E Seiberg-Witten exact sol. for N = 2 SYM Seiberg N = 1 Seiberg s ele.-mag. duality Polchinski D-brane S, T, U duality M-theory 1997 Maldacena AdS/CFT 1984 Green-Schwarz d = 10 super Yang-Mills (SYM) SO(32) E 8 E 8 7

8 Seiberg-Witten N = 2 SYM Seiberg N = 1 SYM Seiberg duality Polchinski D-brane S-, T-, U-duality M-QCD 1997 Maldacena AdS/CFT supergravity superstring 1995 YKIS Seiberg Polchinski Seiberg Seiberg duality Power of Holomorphy Gauge symmetry is not a symmetry 4 Weyl Seiberg global dual powerful Symmetry Global Local Spt. Unbroken Spt. Broken Wigner phase Multiplet structure in the Spectrum Symmetry Relations between Amplitudes Nambu-Goldstone phase Nambu-Goldstone bosons Low energy theorems global symmetry Wigner phase Wigner-Eckert Nambu-Goldstone phase 8

9 Nambu-Goldstone boson Nambu-Goldstone boson local symmetry Symmetry Spt. Unbroken Spt. Broken Local Massless vector Massless vector Coulomb Colored states Wigner Confinement Color singlets Massless vector Higgs No charge operators (if g: Massive gauge bosons ) symmetry gauge x- independent global (color symmetry) Massless vector (gauge boson) Coulomb Confinement Coulomb U(1) Coulomb colored states Global Wigner Massless vector Confinement color singlets color Higgs Massless vector color charges g Higgs massive gauge boson Confinement Higgs 1970 Fradkin-Shenker [6] Confinement Higgs phase boundary color symmetry Confinement Higgs Massless vector Higgs 9

10 5? Is Spontaneously Broken Gauge Symmetry Meaningful? { Weak Coupling g 1 cutoff scale Λ µ massive gauge bosons M gv gauge boson massive bosons Pauli : ψσ µν ψf µν (1) ψ A µ massive on-shell coupling constant A µ massless F µν = µ A ν ν A µ 4 p µ 0 on-shell coupling massless p µ = 0 on-shell massless gauge boson gauge massive p µ = 0 on-shell on-shell 0 p 0 = M( ) 0 Pauli on-shell coupling weak coupling M gv cutoff Λ Pauli 5 1/Λ on-shell coupling coupling Weak Coupling g 1 cutoff scale Λ µ spontaneously broken gauge symmetry electro-weak gauge theory 70 cutoff sacle Λ cutoff GUT scale SU(3) SU(2) U(1) 4 10

11 massless gauge boson on-shell coupling (i.e., at p µ = 0) p µ = 0 non-zero coupling massless Weinberg[7], Kugo-Uehara[8]) p µ = 0 non-zero coupling spin j 1 massless teosorial rank j 1 spin j 1 massless couple spin 1 massless vector boson A µ scalar Q couple spin 3/2 massless vector-spinor fermion ψ µα spinor Q α couple spin 2 massless tensor boson h µν vector Q ν couple Coleman-Mandula- Haag- Lopuszanski-Sohnius S- vector P µ spin 2 massless tensor boson h µν spinor supersymmetry spin 3/2 massless vector-spinor fermion ψ µα 8 Rarita-Schwinger 6? Higgs Is Confined Gauge Symmetry Meaningful? SU(3) color N c = 3 1) Drell ratio R 2) π 0 2γ 3) Baryon qqq 3 Seiberg duality N c + Ñc = N f N c Ñc SU(N c ) with N f flavors SU(Ñc) with N f flavors duality SU(3) 3? 11

12 duality coupling coupling weak-strong duality gauge coupling N f = 3 massless quarks SU(3) gauge coupling gauge coupling 1 Λ QCD Seiberg duality asymptotically free infrared fixed point infrared fixed point conformal QCD N c = 3 MeV( 1GeV) SU(3) 1GeV SU(3) QCD 1GeV SU(3) QCD ( ) (B)(2) ( ) 12

13 A :? BRS Kugo-Ojima BRS Lautrup formalism QED M QED -Lautrup 1977 Quark Confinement QED QED free confinement Yang-Mills Faddeev-Popov ghost confinement QED Formalism Yang-Mills Yang-Mills consistent Faddeev-Popov ghost loop S Ward QED 2 Ward- FP ghost- ghost Faddeev-Popov ghost FP ghost ghost i Lagrangian 3 Ward- 13

14 4 Ward- Ward- Ward- bilinear Zinn-Justin Bonn Lecture Note[9] Ward- BRS Noether free part [1] L. O Raifeartaigh, The Dawning of Gauge Theory, Princeton Series in Physics, (Princeton Univ. Press, Princeton, 1997) [2] Y. Nambu, Quasi-Particles and Gauge Invariance in the Theory of Superconductivity, Phys. Rev. 117 (1960) 648. [3] M. Bando, T. Kugo, S. Uehara, K. Yamawaki and T. Yanagida, Is ρ Meson a Dynamical Gauge Boson of Hidden Local Symmetry?, Phys. Rev. Lett. 54 (1985) [4] T. Kugo and I. Ojima, Manifestly Covariant Canonical Formulation of Yang-Mills Field Theories: Physical State Subsidiary Conditions and Physical S Matrix Unitarity, Phys. Lett. B 73 (1978) 459. [5] T. Kugo and I. Ojima, Local Covariant Operator Formalism of Nonabelian Gauge Theories and Quark Confinement Problem, Prog. Theor. Phys. Suppl. 66 (1979) 1. [6] E. H. Fradkin and S. H. Shenker, Phase Diagrams of Lattice Gauge Theories with Higgs Fields, Phys. Rev. D 19 (1979) [7] S. Weinberg, Phys. Lett. 9 (1964) 357; Phys. Rev. 135 (1964), B1049. [8] T. Kugo and S. Uehara, Massless Particle with Spin j 1 Implies the S-Matrix Symmetry Prog. Theor. Phys. 66 (1981) [9] J. Zinn-Justin, Renormalization of Gauge Theories, SACLAY-D.PH-T Lectures given at Int. Summer Inst. for Theoretical Physics, Jul 29 - Aug 9, 1974, Bonn, West Germany 14

Seiberg Witten 1994 N = 2 SU(2) Yang-Mills 1 1 3 2 5 2.1..................... 5 2.2.............. 8 2.3................................. 9 3 N = 2 Yang-Mills 11 3.1............................... 11 3.2

More information

2017 II 1 Schwinger Yang-Mills 5. Higgs 1

2017 II 1 Schwinger Yang-Mills 5. Higgs 1 2017 II 1 Schwinger 2 3 4. Yang-Mills 5. Higgs 1 1 Schwinger Schwinger φ 4 L J 1 2 µφ(x) µ φ(x) 1 2 m2 φ 2 (x) λφ 4 (x) + φ(x)j(x) (1.1) J(x) Schwinger source term) c J(x) x S φ d 4 xl J (1.2) φ(x) m 2

More information

1. 1.1....................... 1.2............................ 1.3.................... 1.4.................. 2. 2.1.................... 2.2..................... 2.3.................... 3. 3.1.....................

More information

YITP50.dvi

YITP50.dvi 1 70 80 90 50 2 3 3 84 first revolution 4 94 second revolution 5 6 2 1: 1 3 consistent 1-loop Feynman 1-loop Feynman loop loop loop Feynman 2 3 2: 1-loop Feynman loop 3 cycle 4 = 3: 4: 4 cycle loop Feynman

More information

q quark L left-handed lepton. λ Gell-Mann SU(3), a = 8 σ Pauli, i =, 2, 3 U() T a T i 2 Ỹ = 60 traceless tr Ỹ 2 = 2 notation. 2 off-diagonal matrices

q quark L left-handed lepton. λ Gell-Mann SU(3), a = 8 σ Pauli, i =, 2, 3 U() T a T i 2 Ỹ = 60 traceless tr Ỹ 2 = 2 notation. 2 off-diagonal matrices Grand Unification M.Dine, Supersymmetry And String Theory: Beyond the Standard Model 6 2009 2 24 by Standard Model Coupling constant θ-parameter 8 Charge quantization. hypercharge charge Gauge group. simple

More information

1. Introduction Palatini formalism vierbein e a µ spin connection ω ab µ Lgrav = e (R + Λ). 16πG R µνab µ ω νab ν ω µab ω µac ω νcb + ω νac ω µcb, e =

1. Introduction Palatini formalism vierbein e a µ spin connection ω ab µ Lgrav = e (R + Λ). 16πG R µνab µ ω νab ν ω µab ω µac ω νcb + ω νac ω µcb, e = Chiral Fermion in AdS(dS) Gravity Fermions in (Anti) de Sitter Gravity in Four Dimensions, N.I, Takeshi Fukuyama, arxiv:0904.1936. Prog. Theor. Phys. 122 (2009) 339-353. 1. Introduction Palatini formalism

More information

Einstein 1905 Lorentz Maxwell c E p E 2 (pc) 2 = m 2 c 4 (7.1) m E ( ) E p µ =(p 0,p 1,p 2,p 3 )=(p 0, p )= c, p (7.2) x µ =(x 0,x 1,x 2,x

Einstein 1905 Lorentz Maxwell c E p E 2 (pc) 2 = m 2 c 4 (7.1) m E ( ) E p µ =(p 0,p 1,p 2,p 3 )=(p 0, p )= c, p (7.2) x µ =(x 0,x 1,x 2,x 7 7.1 7.1.1 Einstein 1905 Lorentz Maxwell c E p E 2 (pc) 2 = m 2 c 4 (7.1) m E ( ) E p µ =(p 0,p 1,p 2,p 3 )=(p 0, p )= c, p (7.2) x µ =(x 0,x 1,x 2,x 3 )=(x 0, x )=(ct, x ) (7.3) E/c ct K = E mc 2 (7.4)

More information

main.dvi

main.dvi SGC - 48 208X Y Z Z 2006 1930 β Z 2006! 1 2 3 Z 1930 SGC -12, 2001 5 6 http://www.saiensu.co.jp/support.htm http://www.shinshu-u.ac.jp/ haru/ xy.z :-P 3 4 2006 3 ii 1 1 1.1... 1 1.2 1930... 1 1.3 1930...

More information

Introduction SFT Tachyon condensation in SFT SFT ( ) at 1 / 38

Introduction SFT Tachyon condensation in SFT SFT ( ) at 1 / 38 ( ) 2011 5 14 at 1 / 38 Introduction? = String Field Theory = SFT 2 / 38 String Field : ϕ(x, t) x ϕ x / ( ) X ( σ) (string field): Φ[X(σ), t] X(σ) Φ (Φ X(σ) ) X(σ) & / 3 / 38 SFT with Lorentz & Gauge Invariance

More information

Einstein ( ) YITP

Einstein ( ) YITP Einstein ( ) 2013 8 21 YITP 0. massivegravity Massive spin 2 field theory Fierz-Pauli (FP ) Kinetic term L (2) EH = 1 2 [ λh µν λ h µν λ h λ h 2 µ h µλ ν h νλ + 2 µ h µλ λ h], (1) Mass term FP L mass =

More information

kougiroku7_26.dvi

kougiroku7_26.dvi 2005 : D-brane tachyon : ( ) 2005 8 7 8 :,,,,,,, 1 2 1.1 Introduction............................... 2 1.2......................... 6 1.3 Second Revolution (1994 )................... 11 2 Type II 26 2.1

More information

橡超弦理論はブラックホールの謎を解けるか?

橡超弦理論はブラックホールの謎を解けるか? 1999 3 (Can String Theory Solve the Puzzles of Black Holes?) 305-0801 1-1 makoto.natsuume@kek.jp D-brane 1 Schwarzschild 60 80 2 [1] 1 1 1 2 2 [2] 25 2.2 2 2.1 [7,8] Schwarzschild 2GM/c 2 Schwarzschild

More information

non-gaussianities de Sitter space non-gaussianities N. Arkani-Hamed, J. Maldacena [arxiv: v1[hep-th]] T. Noumi, M. Yamaguchi, D. Yokoyama [ar

non-gaussianities de Sitter space non-gaussianities N. Arkani-Hamed, J. Maldacena [arxiv: v1[hep-th]] T. Noumi, M. Yamaguchi, D. Yokoyama [ar 64 2018 8 6 8 11 @ 1 2018 8 7 ( ) 1.1 1 (19:00-22:15) 1.1.1 ( ) 1.1.2 ( ) MSSM MSSM 1.1.3 ( ) ON ANOMALOUS ELECTROWEAK BARYON-NUMBER NON-CONSERVATION IN THE EARLY UNIVERSE (review) ( ) 100 GeV GUT 1.1.4

More information

0406_total.pdf

0406_total.pdf 59 7 7.1 σ-ω σ-ω σ ω σ = σ(r), ω µ = δ µ,0 ω(r) (6-4) (iγ µ µ m U(r) γ 0 V (r))ψ(x) = 0 (7-1) U(r) = g σ σ(r), V (r) = g ω ω(r) σ(r) ω(r) (6-3) ( 2 + m 2 σ)σ(r) = g σ ψψ (7-2) ( 2 + m 2 ω)ω(r) = g ω ψγ

More information

cm λ λ = h/p p ( ) λ = cm E pc [ev] 2.2 quark lepton u d c s t b e 1 3e electric charge e color charge red blue green qq

cm λ λ = h/p p ( ) λ = cm E pc [ev] 2.2 quark lepton u d c s t b e 1 3e electric charge e color charge red blue green qq 2007 2007 7 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 1 2007 2 4 5 6 6 2 2.1 1: KEK Web page 1 1 1 10 16 cm λ λ = h/p p ( ) λ = 10 16 cm E pc [ev] 2.2 quark lepton 2 2.2.1 u d c s t b + 2 3 e 1 3e electric charge

More information

Kaluza-Klein(KK) SO(11) KK 1 2 1

Kaluza-Klein(KK) SO(11) KK 1 2 1 Maskawa Institute, Kyoto Sangyo University Naoki Yamatsu 2016 4 12 ( ) @ Kaluza-Klein(KK) SO(11) KK 1 2 1 1. 2. 3. 4. 2 1. 標準理論 物質場 ( フェルミオン ) スカラー ゲージ場 クォーク ヒッグス u d s b ν c レプトン ν t ν e μ τ e μ τ e h

More information

SUSY DWs

SUSY DWs @ 2013 1 25 Supersymmetric Domain Walls Eric A. Bergshoeff, Axel Kleinschmidt, and Fabio Riccioni Phys. Rev. D86 (2012) 085043 (arxiv:1206.5697) ( ) Contents 1 2 SUSY Domain Walls Wess-Zumino Embedding

More information

D 2009 A * 1 ( ) *1 ( ) 0 1 1 6 2 32 2.1............................................. 32 2.2.................................. 41 2.3...................................... 47 3 65 3.1..............................................

More information

QCD 1 QCD GeV 2014 QCD 2015 QCD SU(3) QCD A µ g µν QCD 1

QCD 1 QCD GeV 2014 QCD 2015 QCD SU(3) QCD A µ g µν QCD 1 QCD 1 QCD GeV 2014 QCD 2015 QCD SU(3) QCD A µ g µν QCD 1 (vierbein) QCD QCD 1 1: QCD QCD Γ ρ µν A µ R σ µνρ F µν g µν A µ Lagrangian gr TrFµν F µν No. Yes. Yes. No. No! Yes! [1] Nash & Sen [2] Riemann

More information

[ ] = L [δ (D ) (x )] = L D [g ] = L D [E ] = L Table : ħh = m = D D, V (x ) = g δ (D ) (x ) E g D E (Table )D = Schrödinger (.3)D = (regularization)

[ ] = L [δ (D ) (x )] = L D [g ] = L D [E ] = L Table : ħh = m = D D, V (x ) = g δ (D ) (x ) E g D E (Table )D = Schrödinger (.3)D = (regularization) . D............................................... : E = κ ............................................ 3.................................................

More information

main.dvi

main.dvi Ver. 1.50 2001 ( ) 1 4 2 Effective Theory 5 2.1 Effective theory... 5 2.2 massless 2-flavor QCD... 5 2.3..................... 9 2.4 Standard model... 10 2.5... 11 2.6... 13 3 Supersymmetry 15 3.1 Supersymmetry...

More information

* 1 1 (i) (ii) Brückner-Hartree-Fock (iii) (HF, BCS, HFB) (iv) (TDHF,TDHFB) (RPA) (QRPA) (v) (vi) *

* 1 1 (i) (ii) Brückner-Hartree-Fock (iii) (HF, BCS, HFB) (iv) (TDHF,TDHFB) (RPA) (QRPA) (v) (vi) * * 1 1 (i) (ii) Brückner-Hartree-Fock (iii) (HF, BCS, HFB) (iv) (TDHF,TDHFB) (RPA) (QRPA) (v) (vi) *1 2004 1 1 ( ) ( ) 1.1 140 MeV 1.2 ( ) ( ) 1.3 2.6 10 8 s 7.6 10 17 s? Λ 2.5 10 10 s 6 10 24 s 1.4 ( m

More information

反D中間子と核子のエキゾチックな 束縛状態と散乱状態の解析

反D中間子と核子のエキゾチックな   束縛状態と散乱状態の解析 .... D 1 in collaboration with 1, 2, 1 RCNP 1, KEK 2 . Exotic hadron qqq q q Θ + Λ(1405) etc. uudd s? KN quasi-bound state? . D(B)-N bound state { { D D0 ( cu) B = D ( cd), B = + ( bu) B 0 ( bd) D(B)-N

More information

Confinement dual Meissener effect dual Meissener effect

Confinement dual Meissener effect dual Meissener effect BASED ON WORK WITH KENICHI KONISHI (UNIV. OF PISA) [0909.3781 TO APPEAR IN NPB] Confinement dual Meissener effect dual Meissener effect 1) Perturbed SU(N) Seiberg WiRen theory : 2) SU(N) with Flavors at

More information

2016 ǯ¥Î¡¼¥Ù¥ëʪÍý³Ø¾Þ²òÀ⥻¥ß¥Ê¡¼ Kosterlitz-Thouless ž°Ü¤È Haldane ͽÁÛ

2016 ǯ¥Î¡¼¥Ù¥ëʪÍý³Ø¾Þ²òÀ⥻¥ß¥Ê¡¼  Kosterlitz-Thouless ž°Ü¤È Haldane ͽÁÛ 2016 Kosterlitz-Thouless Haldane Dept. of Phys., Kyushu Univ. 2016 11 29 2016 Figure: D.J.Thouless F D.M.Haldane J.M.Kosterlitz TOPOLOGICAL PHASE TRANSITIONS AND TOPOLOGICAL PHASES OF MATTER ( ) ( ) (Dirac,

More information

Meson theory in its developments

Meson theory in its developments Vol. 93 No. 6 (1996), pp.349-399 c 1996 1996 9 2 1997 27 1952 28 1953 2 1990 1 24 1949 11 4 1 5 6 5 1 4 12 10 12 Meson theory in its developments 10 1935 200 10 1 1937 1947 37 1948 27 1952 59 11 3 2 5

More information

1/2 ( ) 1 * 1 2/3 *2 up charm top -1/3 down strange bottom 6 (ν e, ν µ, ν τ ) -1 (e) (µ) (τ) 6 ( 2 ) 6 6 I II III u d ν e e c s ν µ µ t b ν τ τ (2a) (

1/2 ( ) 1 * 1 2/3 *2 up charm top -1/3 down strange bottom 6 (ν e, ν µ, ν τ ) -1 (e) (µ) (τ) 6 ( 2 ) 6 6 I II III u d ν e e c s ν µ µ t b ν τ τ (2a) ( August 26, 2005 1 1 1.1...................................... 1 1.2......................... 4 1.3....................... 5 1.4.............. 7 1.5.................... 8 1.6 GIM..........................

More information

Happy 60th Birthdays! Ishikawa-san & Kawamoto-san

Happy 60th Birthdays! Ishikawa-san & Kawamoto-san Glashow-Weinberg-Salam model on the lattice A construction with exact gauge invariance Y. Kikukawa Institute of Physics, University of Tokyo based on : D. Kadoh and Y.K., JHEP 0805:095 (2008), 0802:063

More information

Hilbert, von Neuman [1, p.86] kt 2 1 [1, 2] 2 2

Hilbert, von Neuman [1, p.86] kt 2 1 [1, 2] 2 2 hara@math.kyushu-u.ac.jp 1 1 1.1............................................... 2 1.2............................................. 3 2 3 3 5 3.1............................................. 6 3.2...................................

More information

,,..,. 1

,,..,. 1 016 9 3 6 0 016 1 0 1 10 1 1 17 1..,,..,. 1 1 c = h = G = ε 0 = 1. 1.1 L L T V 1.1. T, V. d dt L q i L q i = 0 1.. q i t L q i, q i, t L ϕ, ϕ, x µ x µ 1.3. ϕ x µ, L. S, L, L S = Ld 4 x 1.4 = Ld 3 xdt 1.5

More information

(Tokyo Institute of Technology) Seminar at Ehime University ( ) 9 3 U(N C ), N F /2 BPS ( ) 12 5 (

(Tokyo Institute of Technology) Seminar at Ehime University ( ) 9 3 U(N C ), N F /2 BPS ( ) 12 5 ( (Tokyo Institute of Technology) Seminar at Ehime University 2007.08.091 1 2 1.1..................... 2 2 ( ) 9 3 U(N C ), N F 11 4 1/2 BPS ( ) 12 5 ( ) 19 6 Conclusion 23 1 1.1 GeV SU(3) SU(2) U(1): W

More information

重力と宇宙 新しい時空の量子論

重力と宇宙 新しい時空の量子論 Summer Institute at Fujiyoshida, 2009/08/06 KEK/ Conformal Field Theory on R x S^3 from Quantized Gravity, arxiv:0811.1647[hep-th]. Renormalizable 4D Quantum Gravity as A Perturbed Theory from CFT, arxiv:0907.3969[hep-th].

More information

橋本研

橋本研 -Goldstone ( ) 2011 4-2012 3 -Goldstone UV IR SSB+ : Chiral Lagrangian :,... -Goldstone Nambu( 60), Goldstone(61), Nambu, Jona-Lasinio( 61), Goldstone, Salam, Weinberg( 62) Lorentz ( ) = NG 2002~2004?

More information

ʪ¼Á¤Î¥È¥Ý¥í¥¸¥«¥ë¸½¾Ý (2016ǯ¥Î¡¼¥Ù¥ë¾Þ¤Ë´ØÏ¢¤·¤Æ)

ʪ¼Á¤Î¥È¥Ý¥í¥¸¥«¥ë¸½¾Ý  (2016ǯ¥Î¡¼¥Ù¥ë¾Þ¤Ë´ØÏ¢¤·¤Æ) (2016 ) Dept. of Phys., Kyushu Univ. 2017 8 10 1 / 59 2016 Figure: D.J.Thouless F D.M.Haldane J.M.Kosterlitz TOPOLOGICAL PHASE TRANSITIONS AND TOPOLOGICAL PHASES OF MATTER 2 / 59 ( ) ( ) (Dirac, t Hooft-Polyakov)

More information

( ) : (Technocolor)...

( ) : (Technocolor)... ( ) 2007.5.14 1 3 1.1............................. 3 1.2 :........... 5 1.3........................ 7 1.4................. 8 2 11 2.1 (Technocolor)................ 11 2.2............................. 12

More information

Chebyshev Schrödinger Heisenberg H = 1 2m p2 + V (x), m = 1, h = 1 1/36 1 V (x) = { 0 (0 < x < L) (otherwise) ψ n (x) = 2 L sin (n + 1)π x L, n = 0, 1, 2,... Feynman K (a, b; T ) = e i EnT/ h ψ n (a)ψ

More information

1 (Contents) (1) Beginning of the Universe, Dark Energy and Dark Matter Noboru NAKANISHI 2 2. Problem of Heat Exchanger (1) Kenji

1 (Contents) (1) Beginning of the Universe, Dark Energy and Dark Matter Noboru NAKANISHI 2 2. Problem of Heat Exchanger (1) Kenji 8 4 2018 6 2018 6 7 1 (Contents) 1. 2 2. (1) 22 3. 31 1. Beginning of the Universe, Dark Energy and Dark Matter Noboru NAKANISHI 2 2. Problem of Heat Exchanger (1) Kenji SETO 22 3. Editorial Comments Tadashi

More information

α : G X (s, A) α s (A) X α s (c 1 A 1 + c 2 A 2 ) = c 1 α s (A 1 )+c 2 α s (A 2 ), α st (A) = α s (α t (A)) G X α 1.1 G α X (IO) 5W1H A A B A B 1.2!?

α : G X (s, A) α s (A) X α s (c 1 A 1 + c 2 A 2 ) = c 1 α s (A 1 )+c 2 α s (A 2 ), α st (A) = α s (α t (A)) G X α 1.1 G α X (IO) 5W1H A A B A B 1.2!? 62 Abstract 0 Coulomb Coulomb Coulomb BCS Higg Cooper 1 G α X, G G = R or Z X X X (A, B) A + B, AB X, K X (c, A) ca X K K = R C K = R or C 1 α : G X (s, A) α s (A) X α s (c 1 A 1 + c 2 A 2 ) = c 1 α s

More information

D-brane K 1, 2 ( ) 1 K D-brane K K D-brane Witten [1] D-brane K K K K D-brane D-brane K RR BPS D-brane

D-brane K 1, 2   ( ) 1 K D-brane K K D-brane Witten [1] D-brane K K K K D-brane D-brane K RR BPS D-brane D-brane K 1, 2 E-mail: sugimoto@yukawa.kyoto-u.ac.jp (2004 12 16 ) 1 K D-brane K K D-brane Witten [1] D-brane K K K K D-brane D-brane K RR BPS D-brane D-brane RR D-brane K D-brane K D-brane K K [2, 3]

More information

Λ(1405) supported by Global Center of Excellence Program Nanoscience and Quantum Physics 2009, Aug. 5th 1

Λ(1405) supported by Global Center of Excellence Program Nanoscience and Quantum Physics 2009, Aug. 5th 1 Λ(1405) supported by Global Center of Excellence Program Nanoscience and Quantum Physics 2009, Aug. 5th 1 S KN Λ(1405) Λ(1405) CDD Nc 2 L = q(i/ m)q P L = 1 2 (1 γ 5), P R = 1 2 (1 + γ 5), q L P L q, q

More information

N = , 4 Introduction 3 1 ADHM Construction Notation Yang-Mills Theory

N = , 4 Introduction 3 1 ADHM Construction Notation Yang-Mills Theory N = 2 2004 8 3, 4 Introduction 3 1 ADHM Construction 5 1.1 Notation..................................... 5 1.2 Yang-Mills Theory............................... 8 1.3 BPST Instanton................................

More information

4/15 No.

4/15 No. 4/15 No. 1 4/15 No. 4/15 No. 3 Particle of mass m moving in a potential V(r) V(r) m i ψ t = m ψ(r,t)+v(r)ψ(r,t) ψ(r,t) = ϕ(r)e iωt ψ(r,t) Wave function steady state m ϕ(r)+v(r)ϕ(r) = εϕ(r) Eigenvalue problem

More information

' , 24 :,,,,, ( ) Cech Index theorem 22 5 Stability 44 6 compact 49 7 Donaldson 58 8 Symplectic structure 63 9 Wall crossing 66 1

' , 24 :,,,,, ( ) Cech Index theorem 22 5 Stability 44 6 compact 49 7 Donaldson 58 8 Symplectic structure 63 9 Wall crossing 66 1 1998 1998 7 20 26, 44. 400,,., (KEK), ( ) ( )..,.,,,. 1998 1 '98 7 23, 24 :,,,,, ( ) 1 3 2 Cech 6 3 13 4 Index theorem 22 5 Stability 44 6 compact 49 7 Donaldson 58 8 Symplectic structure 63 9 Wall crossing

More information

susy.dvi

susy.dvi 1 Chapter 1 Why supper symmetry? 2 Chapter 2 Representaions of the supersymmetry algebra SUSY Q a d 3 xj 0 α J x µjµ = 0 µ SUSY ( {Q A α,q βb } = 2σ µ α β P µδ A B (2.1 {Q A α,q βb } = {Q αa,q βb } = 0

More information

02-量子力学の復習

02-量子力学の復習 4/17 No. 1 4/17 No. 2 4/17 No. 3 Particle of mass m moving in a potential V(r) V(r) m i ψ t = 2 2m 2 ψ(r,t)+v(r)ψ(r,t) ψ(r,t) Wave function ψ(r,t) = ϕ(r)e iωt steady state 2 2m 2 ϕ(r)+v(r)ϕ(r) = εϕ(r)

More information

July 28, H H 0 H int = H H 0 H int = H int (x)d 3 x Schrödinger Picture Ψ(t) S =e iht Ψ H O S Heisenberg Picture Ψ H O H (t) =e iht O S e i

July 28, H H 0 H int = H H 0 H int = H int (x)d 3 x Schrödinger Picture Ψ(t) S =e iht Ψ H O S Heisenberg Picture Ψ H O H (t) =e iht O S e i July 8, 4. H H H int H H H int H int (x)d 3 x Schrödinger Picture Ψ(t) S e iht Ψ H O S Heisenberg Picture Ψ H O H (t) e iht O S e iht Interaction Picture Ψ(t) D e iht Ψ(t) S O D (t) e iht O S e ih t (Dirac

More information

D.dvi

D.dvi 2005 3 3 1 7 1.1... 7 1.2 Brane... 8 1.3 AdS/CFT black hole... 9 1.4... 10 2 11 2.1 Kaluza-Klein... 11 2.1.1 Kazula-Klein 4... 11 2.1.2 Kaluza-Klein... 13 2.2 Brane... 14 2.2.1 Brane 4... 14 2.2.2 Bulk

More information

Big Bang Planck Big Bang 1 43 Planck Planck quantum gravity Planck Grand Unified Theories: GUTs X X W X 1 15 ev 197 Glashow Georgi 1 14 GeV 1 2

Big Bang Planck Big Bang 1 43 Planck Planck quantum gravity Planck Grand Unified Theories: GUTs X X W X 1 15 ev 197 Glashow Georgi 1 14 GeV 1 2 12 Big Bang 12.1 Big Bang Big Bang 12.1 1-5 1 32 K 1 19 GeV 1-4 time after the Big Bang [ s ] 1-3 1-2 1-1 1 1 1 1 2 inflationary epoch gravity strong electromagnetic weak 1 27 K 1 14 GeV 1 15 K 1 2 GeV

More information

b.dvi

b.dvi , 0 1 2 1.1 [2, 3] : : : : : : : : : : : : : : : : 3 2, 6 2.1 : : : : : : : : : : : : : : : 7 2.2 : : : : : : : : : : : : : : : : : : : 15 2.3, : : : : 18 3 23 4 31 5 35 6 46 6.1 Borel. : : : : : : : :

More information

hidaka2

hidaka2 -Goldstone ( ) 様々な物理状態 自発的対称性の破れ 並進対称性 U(1)ゲージ対称性 並進対称性 CC by-sa Didier Descouens ガリレイ対称性 CC by-sa Mai-Linh Doan CC by-sa Roger McLassus 並進対称性 スピン対称性 カイラル対称性 CC by-sa Aney SU(2)xU(1) ゲージ対称性 CC by-sa Elijah

More information

熱場

熱場 -Goldstone ( ) 様々な物理状態 自発的対称性の破れ 並進対称性 U(1)ゲージ対称性 並進対称性 CC by-sa Didier Descouens ガリレイ対称性 CC by-sa Mai-Linh Doan 並進対称性 スピン対称性 CC by-sa Roger McLassus カイラル対称性 CC by-sa Aney CC by-sa Elijah van der Giessen

More information

2 2 Belavin Polyakov Zamolodchikov (BPZ) 1984 [13] 2 BPZ BPZ Virasoro [16][18] [20], [30], [47] [1][6] [8][10], [11], [12] Affine [6],GKO [2] W

2 2 Belavin Polyakov Zamolodchikov (BPZ) 1984 [13] 2 BPZ BPZ Virasoro [16][18] [20], [30], [47] [1][6] [8][10], [11], [12] Affine [6],GKO [2] W SGC -83 2 2 Belavin Polyakov Zamolodchikov (BPZ) 1984 [13] 2 BPZ BPZ 1 3 4 Virasoro [16][18] [20], [30], [47] [1][6] [8][10], [11], [12] Affine [6],GKO [2] W [14] c = 1 CFT [8] Rational CFT [15], [56]

More information

·«¤ê¤³¤ß·²¤È¥ß¥ì¥Ë¥¢¥àÌäÂê

·«¤ê¤³¤ß·²¤È¥ß¥ì¥Ë¥¢¥àÌäÂê .. 1 10-11 Nov., 2016 1 email:keiichi.r.ito@gmail.com, ito@kurims.kyoto-u.ac.jp ( ) 10-11 Nov., 2016 1 / 45 Clay Institute.1 Construction of 4D YM Field Theory (Jaffe, Witten) Jaffe, Balaban (1980).2 Solution

More information

DaisukeSatow.key

DaisukeSatow.key Nambu-Goldstone Fermion in Quark-Gluon Plasma and Bose-Fermi Cold Atom System ( /BNL! ECT* ") : Jean-Paul Blaizot (Saclay CEA #) ( ) (SUSY) = b f b f 2 (SUSY) Q: supercharge b f b f SUSY: [Q, H]=0 Supercharge

More information

09kyoto

09kyoto F [ ] F [ ] Nambu( 60), Goldstone(61), Nambu Jona-Lasinio( 61), Goldstone, Salam, Weinberg( 62). N NG = N BS NG : CC by-sa Aney CC by Zouavman Le Zouave CC by-sa Roger McLassus U(1) CC by-sa Aney -Goldstone

More information

nenmatsu5c19_web.key

nenmatsu5c19_web.key KL π ± e νe + e - (Ke3ee) Ke3ee ν e + e - Ke3 K 0 γ e + π - Ke3 KL ; 40.67(%) Ke3ee K 0 ν γ e + π - Ke3 KL ; 40.67(%) Me + e - 10 4 10 3 10 2 : MC Ke3γ : data K L real γ e detector matter e e 10 1 0 0.02

More information

スライド タイトルなし

スライド タイトルなし 006 8 (g cm -3 ) 1 ~10-8 cm ~10-1 cm 10 14 (n) 10 15 ~10-13 cm (p) (q) RGB uds... (contd.) 0 ~ fm np nn,pp (contd.) 1 GeV 100 GeV 1 TeV RI FAIR GSI RHIC BNL LHC CERN (contd.) T < 9 ~ 10 K (contd.) (k B

More information

0. Intro ( K CohFT etc CohFT 5.IKKT 6.

0. Intro ( K CohFT etc CohFT 5.IKKT 6. E-mail: sako@math.keio.ac.jp 0. Intro ( K 1. 2. CohFT etc 3. 4. CohFT 5.IKKT 6. 1 µ, ν : d (x 0,x 1,,x d 1 ) t = x 0 ( t τ ) x i i, j, :, α, β, SO(D) ( x µ g µν x µ µ g µν x ν (1) g µν g µν vector x µ,y

More information

QCD

QCD QCD 2014 2 26 25 2 (Quantum ChromoDynamisc, QCD) QCD QCD QCD 1 1 QCD QCD QCD QCD QCD QCD QCD QCD QCD QCD low-lying Dirac mode Polyakov loop Dirac mode Polyakov loop low-lying Dirac mode low-lying Dirac

More information

7 π L int = gψ(x)ψ(x)φ(x) + (7.4) [ ] p ψ N = n (7.5) π (π +,π 0,π ) ψ (σ, σ, σ )ψ ( A) σ τ ( L int = gψψφ g N τ ) N π * ) (7.6) π π = (π, π, π ) π ±

7 π L int = gψ(x)ψ(x)φ(x) + (7.4) [ ] p ψ N = n (7.5) π (π +,π 0,π ) ψ (σ, σ, σ )ψ ( A) σ τ ( L int = gψψφ g N τ ) N π * ) (7.6) π π = (π, π, π ) π ± 7 7. ( ) SU() SU() 9 ( MeV) p 98.8 π + π 0 n 99.57 9.57 97.4 497.70 δm m 0.4%.% 0.% 0.8% π 9.57 4.96 Σ + Σ 0 Σ 89.6 9.46 K + K 0 49.67 (7.) p p = αp + βn, n n = γp + δn (7.a) [ ] p ψ ψ = Uψ, U = n [ α

More information

2 I II T.-P. Cheng and L.-F. Li, Gauge theory of elementary particle physics (Oxford university press, 1984) H. Georgi, Weak Interactio

2 I II T.-P. Cheng and L.-F. Li, Gauge theory of elementary particle physics (Oxford university press, 1984) H. Georgi, Weak Interactio 1 2006 6 23 HP 1998 1995 1998 1999 M. Veltman, Facts and Mysteries in Elementary Particle Physics, (World Scientific, 2003). 1986 1993 1995 2000 2000 2002 1986 I II 1992 J. J. Sakurai, Advanced Quantum

More information

2 5W1H = a) [ ]= (= ) : b) [ ] : c) [ ] = (to characterize the observed system) : d) [ ] (: ) 2

2 5W1H = a) [ ]= (= ) : b) [ ] : c) [ ] = (to characterize the observed system) : d) [ ] (: ) 2 1 vs. 90 mescoscopic physics 1 2 5W1H = a) [ ]= (= ) : b) [ ] : c) [ ] = (to characterize the observed system) : d) [ ] (: ) 2 (: ) [1]: 1. Newton =[( ) vs. ] (a) =0 x v ( p = mv) [ a), b), c)] (b) = :

More information

PowerPoint Presentation

PowerPoint Presentation 2010 KEK (Japan) (Japan) (Japan) Cheoun, Myun -ki Soongsil (Korea) Ryu,, Chung-Yoe Soongsil (Korea) 1. S.Reddy, M.Prakash and J.M. Lattimer, P.R.D58 #013009 (1998) Magnetar : ~ 10 15 G ~ 10 17 19 G (?)

More information

φ 4 Minimal subtraction scheme 2-loop ε 2008 (University of Tokyo) (Atsuo Kuniba) version 21/Apr/ Formulas Γ( n + ɛ) = ( 1)n (1 n! ɛ + ψ(n + 1)

φ 4 Minimal subtraction scheme 2-loop ε 2008 (University of Tokyo) (Atsuo Kuniba) version 21/Apr/ Formulas Γ( n + ɛ) = ( 1)n (1 n! ɛ + ψ(n + 1) φ 4 Minimal subtraction scheme 2-loop ε 28 University of Tokyo Atsuo Kuniba version 2/Apr/28 Formulas Γ n + ɛ = n n! ɛ + ψn + + Oɛ n =,, 2, ψn + = + 2 + + γ, 2 n ψ = γ =.5772... Euler const, log + ax x

More information

『共形場理論』

『共形場理論』 T (z) SL(2, C) T (z) SU(2) S 1 /Z 2 SU(2) (ŜU(2) k ŜU(2) 1)/ŜU(2) k+1 ŜU(2)/Û(1) G H N =1 N =1 N =1 N =1 N =2 N =2 N =2 N =2 ĉ>1 N =2 N =2 N =4 N =4 1 2 2 z=x 1 +ix 2 z f(z) f(z) 1 1 4 4 N =4 1 = = 1.3

More information

Euler, Yang-Mills Clebsch variable Helicity ( Tosiaki Kori ) School of Sciences and Technology, Waseda Uiversity (i) Yang-Mills 3 A T (T A) Poisson Ha

Euler, Yang-Mills Clebsch variable Helicity ( Tosiaki Kori ) School of Sciences and Technology, Waseda Uiversity (i) Yang-Mills 3 A T (T A) Poisson Ha Euler, Yang-ills Clebsch variable Helicity Tosiaki Kori ) School of Sciences and Technology, Waseda Uiversity i) Yang-ills 3 A T T A) Poisson Hamilton ii) Clebsch parametrization iii) Y- Y-iv) Euler,v)

More information

CP-PACS CP-PACS CP-PACS : 2048PU+128IOU 614GFLOPS peak 128GByte memory 1058GByte disk 1992 1996 SR2201 : 1996 8 9 CP-PACS Top 500 List ranking No. 1 November 1996 Linpack 368.2Gflops No. 24 Novermber 1999

More information

G (n) (x 1, x 2,..., x n ) = 1 Dφe is φ(x 1 )φ(x 2 ) φ(x n ) (5) N N = Dφe is (6) G (n) (generating functional) 1 Z[J] d 4 x 1 d 4 x n G (n) (x 1, x 2

G (n) (x 1, x 2,..., x n ) = 1 Dφe is φ(x 1 )φ(x 2 ) φ(x n ) (5) N N = Dφe is (6) G (n) (generating functional) 1 Z[J] d 4 x 1 d 4 x n G (n) (x 1, x 2 6 Feynman (Green ) Feynman 6.1 Green generating functional Z[J] φ 4 L = 1 2 µφ µ φ m 2 φ2 λ 4! φ4 (1) ( 1 S[φ] = d 4 x 2 φkφ λ ) 4! φ4 (2) K = ( 2 + m 2 ) (3) n G (n) (x 1, x 2,..., x n ) = φ(x 1 )φ(x

More information

Chadwick [ 1 ] 1919,, electron number Q kinetic energy [MeV] 8.1: 8.1, 1 internal conversion electron E γ E e =

Chadwick [ 1 ] 1919,, electron number Q kinetic energy [MeV] 8.1: 8.1, 1 internal conversion electron E γ E e = 8 8.1 8.1.1 1 Chadwick [ 1 ] 1919,, electron number Q 0.0 0. 0.4 0.6 0.8 1.0 kinetic energy [MeV] 8.1: 8.1, 1 internal conversion electron E γ E e = E γ φ φ E e X 153 154 8, 3 H 3 He, ( ) 3 H( 1 ) 3 He(

More information

Dirac 38 5 Dirac 4 4 γ µ p µ p µ + m 2 = ( p µ γ µ + m)(p ν γ ν + m) (5.1) γ = p µ p ν γ µ γ ν p µ γ µ m + mp ν γ ν + m 2 = 1 2 p µp ν {γ µ, γ ν } + m

Dirac 38 5 Dirac 4 4 γ µ p µ p µ + m 2 = ( p µ γ µ + m)(p ν γ ν + m) (5.1) γ = p µ p ν γ µ γ ν p µ γ µ m + mp ν γ ν + m 2 = 1 2 p µp ν {γ µ, γ ν } + m Dirac 38 5 Dirac 4 4 γ µ p µ p µ + m 2 p µ γ µ + mp ν γ ν + m 5.1 γ p µ p ν γ µ γ ν p µ γ µ m + mp ν γ ν + m 2 1 2 p µp ν {γ µ, γ ν } + m 2 5.2 p m p p µ γ µ {, } 10 γ {γ µ, γ ν } 2η µν 5.3 p µ γ µ + mp

More information

V(x) m e V 0 cos x π x π V(x) = x < π, x > π V 0 (i) x = 0 (V(x) V 0 (1 x 2 /2)) n n d 2 f dξ 2ξ d f 2 dξ + 2n f = 0 H n (ξ) (ii) H

V(x) m e V 0 cos x π x π V(x) = x < π, x > π V 0 (i) x = 0 (V(x) V 0 (1 x 2 /2)) n n d 2 f dξ 2ξ d f 2 dξ + 2n f = 0 H n (ξ) (ii) H 199 1 1 199 1 1. Vx) m e V cos x π x π Vx) = x < π, x > π V i) x = Vx) V 1 x /)) n n d f dξ ξ d f dξ + n f = H n ξ) ii) H n ξ) = 1) n expξ ) dn dξ n exp ξ )) H n ξ)h m ξ) exp ξ )dξ = π n n!δ n,m x = Vx)

More information

N=1 N=1 QCD N=1 non-abelian QCD X 0

N=1 N=1 QCD N=1 non-abelian QCD X 0 2 945207 18 9 22 N=1 N=1 QCD N=1 non-abelian QCD X 0 1 3 2 7 2.1..................................... 7 2.2.................................. 8 2.3............ 10 2.4 moduli...............................

More information

( ) 1 (Quantum Field Theory) = Maxwell Dirac Quantum Electro-Dynamics (QED) 1

( ) 1 (Quantum Field Theory) = Maxwell Dirac Quantum Electro-Dynamics (QED) 1 ( ) 1 (Quantum Field Theory) = Maxwell Dirac Quantum Electro-Dynamics (QED) 1 = 2 Key words = : = : = UV divergence = IR divergence massless ( photons) 3 QFT = : a = ( ) Λ = 1/a = = UV cut-off λ( a) QFT

More information

3 exotica

3 exotica ( / ) 2013 2 23 embedding tensors (non)geometric fluxes exotic branes + D U-duality G 0 R-symmetry H dim(g 0 /H) T-duality 11 1 1 0 1 IIA R + 1 1 1 IIB SL(2, R) SO(2) 2 1 9 GL(2, R) SO(2) 3 SO(1, 1) 8

More information

a L = Ψ éiγ c pa qaa mc ù êë ( - )- úû Ψ 1 Ψ 4 γ a a 0, 1,, 3 {γ a, γ b } η ab æi O ö æo ö β, σ = ço I α = è - ø çèσ O ø γ 0 x iβ γ i x iβα i

a L = Ψ éiγ c pa qaa mc ù êë ( - )- úû Ψ 1 Ψ 4 γ a a 0, 1,, 3 {γ a, γ b } η ab æi O ö æo ö β, σ = ço I α = è - ø çèσ O ø γ 0 x iβ γ i x iβα i 解説 4 matsuo.mamoru jaea.go.jp 4 eizi imr.tohoku.ac.jp 4 maekawa.sadamichi jaea.go.jp i ii iii i Gd Tb Dy g khz Pt ii iii Keywords vierbein 3 dreibein 4 vielbein torsion JST-ERATO 1 017 1. 1..1 a L = Ψ

More information

Mathews Grant J. (University of Notre Dame) Boyd Richard N. (Lawrence Livermore National Laboratory) 2009/5/21

Mathews Grant J. (University of Notre Dame) Boyd Richard N. (Lawrence Livermore National Laboratory) 2009/5/21 Mathews Grant J. (University of Notre Dame) Boyd Richard N. (Lawrence Livermore National Laboratory) 2009/5/21 Abstract strongly interacting massive particles (SIMPs, X) Big Bang (BBN) X heavy colored

More information

スライド 1

スライド 1 @ ( based on M.H., C.Sasaki and W.Weise, arxiv:0805.4792, arxiv:0807.1417 see also G.E.Brown, M.H., J.W.Holts, M.Rho and C.Sasaki, arxiv:0804.3196 M.H. and C.Sasaki, Phys. Rev. D74, 114006 (2006) M.H.

More information

Anderson ( ) Anderson / 14

Anderson ( ) Anderson / 14 Anderson 2008 12 ( ) Anderson 2008 12 1 / 14 Anderson ( ) Anderson 2008 12 2 / 14 Anderson P.W.Anderson 1958 ( ) Anderson 2008 12 3 / 14 Anderson tight binding Anderson tight binding Z d u (x) = V i u

More information

,, Andrej Gendiar (Density Matrix Renormalization Group, DMRG) 1 10 S.R. White [1, 2] 2 DMRG ( ) [3, 2] DMRG Baxter [4, 5] 2 Ising 2 1 Ising 1 1 Ising

,, Andrej Gendiar (Density Matrix Renormalization Group, DMRG) 1 10 S.R. White [1, 2] 2 DMRG ( ) [3, 2] DMRG Baxter [4, 5] 2 Ising 2 1 Ising 1 1 Ising ,, Andrej Gendiar (Density Matrix Renormalization Group, DMRG) 1 10 S.R. White [1, 2] 2 DMRG ( ) [3, 2] DMRG Baxter [4, 5] 2 Ising 2 1 Ising 1 1 Ising Model 1 Ising 1 Ising Model N Ising (σ i = ±1) (Free

More information

格子QCD実践入門

格子QCD実践入門 -- nakamura at riise.hiroshima-u.ac.jp or nakamura at an-pan.org 2013.6.26-27 1. vs. 2. (1) 3. QCD QCD QCD 4. (2) 5. QCD 2 QCD 1981 QCD Parisi, Stamatescu, Hasenfratz, etc 2 3 (Cut-Off) = +Cut-Off a p

More information

untitled

untitled 1 Constructive field theory and renormalization group Hiroshi WATANABE 1 2001 7,. 1 2 2 Euclidean field theory 3 2.1...................................... 4 2.2..................................... 6 3

More information

( ) Note (e ) (µ ) (τ ) ( (ν e,e ) e- (ν µ, µ ) µ- (ν τ,τ ) τ- ) ( ) ( ) (SU(2) ) (W +,Z 0,W ) * 1) 3 * 2) [ ] [ ] [ ] ν e ν µ ν τ e

( ) Note (e ) (µ ) (τ ) ( (ν e,e ) e- (ν µ, µ ) µ- (ν τ,τ ) τ- ) ( ) ( ) (SU(2) ) (W +,Z 0,W ) * 1) 3 * 2) [ ] [ ] [ ] ν e ν µ ν τ e ( ) Note 3 19 12 13 8 8.1 (e ) (µ ) (τ ) ( (ν e,e ) e- (ν µ, µ ) µ- (ν τ,τ ) τ- ) ( ) ( ) (SU(2) ) (W +,Z 0,W ) * 1) 3 * 2) [ ] [ ] [ ] ν e ν µ ν τ e µ τ, e R, µ R, τ R (1a) L ( ) ) * 3) W Z 1/2 ( - )

More information

Part I Review on correlation functions of the XXZ spin chain (1) H. Bethe(1930): Exact solutions of the one-dimensional Heisenberg model (XXX spin cha

Part I Review on correlation functions of the XXZ spin chain (1) H. Bethe(1930): Exact solutions of the one-dimensional Heisenberg model (XXX spin cha Part I Review on correlation functions of the XXZ spin chain (1) H. Bethe(1930): Exact solutions of the one-dimensional Heisenberg model (XXX spin chain) (2) C.N. Yang and C.P. Yang (1966): the ground

More information

/ Christopher Essex Radiation and the Violation of Bilinearity in the Thermodynamics of Irreversible Processes, Planet.Space Sci.32 (1984) 1035 Radiat

/ Christopher Essex Radiation and the Violation of Bilinearity in the Thermodynamics of Irreversible Processes, Planet.Space Sci.32 (1984) 1035 Radiat / Christopher Essex Radiation and the Violation of Bilinearity in the Thermodynamics of Irreversible Processes, Planet.Space Sci.32 (1984) 1035 Radiation and the Continuing Failure of the Bilinear Formalism,

More information

ssastro2016_shiromizu

ssastro2016_shiromizu 26 th July 2016 / 1991(M1)-1995(D3), 2005( ) 26 th July 2016 / 1. 2. 3. 4. . ( ) 1960-70 1963 Kerr 1965 BH Penrose 1967 Hawking BH Israel 1971 (Carter)-75(Robinson) BH 1972 BH theorem(,, ) Hawk 1975 Hawking

More information

スライド 1

スライド 1 Determination of KN compositeness of the Λ(1405) resonance from its radiative decay Takayasu SEKIHARA (KEK) in collaboration with Shunzo KUMANO (KEK) 1. Introduction 2. Formulation of Λ(1405) radiative

More information

QMI13a.dvi

QMI13a.dvi I (2013 (MAEDA, Atsutaka) 25 10 15 [ I I [] ( ) 0. (a) (b) Plank Compton de Broglie Bohr 1. (a) Einstein- de Broglie (b) (c) 1 (d) 2. Schrödinger (a) Schrödinger (b) Schrödinger (c) (d) 3. (a) (b) (c)

More information

phaleron decoupling and E hase transitio 2/45

phaleron decoupling and E hase transitio 2/45 1/45 phaleron decoupling and E hase transitio 2/45 Sphaleron σφαλϵρos = ready-to-fall, deceitful [cf. a sphalt] [Klinkhamer and Manton, Phys. Rev. D30 ('84)] 4-dim. SU(2) gauge + 1-doublet Higgs 2-dim.

More information

1 (Contents) (4) Why Has the Superstring Theory Collapsed? Noboru NAKANISHI 2 2. A Periodic Potential Problem

1 (Contents) (4) Why Has the Superstring Theory Collapsed? Noboru NAKANISHI 2 2. A Periodic Potential Problem 7 1 2017 3 2017 3 18 1 (Contents) 1. 2 2. (4) 13 3. 1 20 4. 25 5. 28 6. 29 1. Why Has the Superstring Theory Collapsed? Noboru NAKANISHI 2 2. A Periodic Potential Problem in Quantum Mechanics (4) Kenji

More information

nakayama.key

nakayama.key 2017/11/1@Flavor Physics Workshop 2017 Contents CP 1932 10 4 p + p! p + p + p + p P. Blasi, 1311.7346 d d. 10 Gpc 10 0 Cohen, De Rujula, Glashow (1997) d B0 Flux [photons cm -2 s -1 MeV -1 sr -1

More information

遍歴電子磁性とスピン揺らぎ理論 - 京都大学大学院理学研究科 集中講義

遍歴電子磁性とスピン揺らぎ理論 - 京都大学大学院理学研究科 集中講義 email: takahash@sci.u-hyogo.ac.jp August 3, 2009 Title of Lecture: SCR Spin Fluctuation Theory 2 / 179 Part I Introduction Introduction Stoner-Wohlfarth Theory Stoner-Wohlfarth Theory Hatree Fock Approximation

More information

arxiv: v1(astro-ph.co)

arxiv: v1(astro-ph.co) arxiv:1311.0281v1(astro-ph.co) R µν 1 2 Rg µν + Λg µν = 8πG c 4 T µν Λ f(r) R f(r) Galileon φ(t) Massive Gravity etc... Action S = d 4 x g (L GG + L m ) L GG = K(φ,X) G 3 (φ,x)φ + G 4 (φ,x)r + G 4X (φ)

More information

TeV b,c,τ KEK/ ) ICEPP

TeV b,c,τ KEK/ ) ICEPP TeV b,c,τ KEK/ ) ICEPP 2 TeV TeV ~1930 ~1970 ~2010 LHC TeV LHC TeV LHC TeV CKM K FCNC K CP violation c b, τ B-B t B CP violation interplay 6 Super B Factory Super KEKB LoI (hep-ex/0406071) SLAC Super B

More information

宇宙の背景輻射 現在 150億年 50億年 星や銀河の 形成 自然界には4つの力 3つの分岐点が今回のシリーズの目標 3K LHC温度 1016K (10-12 ~ 10-14s) 10億年 (2) GUTへの挑戦 超対称性による大統一 3000K 30万年 原子 分子の形成 3分 原子核の形成 10-10 秒 弱い相互作用が分離 3つの力が分離する 量子重力の世界 10-34 秒 10-43 秒

More information

1. Introduction overview of baryogenesis. Anomalous Baryon Number Nonconservation 3. Sphaleron Process 4. Requirements for EW Baryogenesis 5. Leptogen

1. Introduction overview of baryogenesis. Anomalous Baryon Number Nonconservation 3. Sphaleron Process 4. Requirements for EW Baryogenesis 5. Leptogen 1/73 1. Introduction overview of baryogenesis. Anomalous Baryon Number Nonconservation 3. Sphaleron Process 4. Requirements for EW Baryogenesis 5. Leptogenesis 6. Discussions Sphaleron process and Leptogenesis

More information

Black-Scholes [1] Nelson [2] Schrödinger 1 Black Scholes [1] Black-Scholes Nelson [2][3][4] Schrödinger Nelson Parisi Wu [5] Nelson Parisi-W

Black-Scholes [1] Nelson [2] Schrödinger 1 Black Scholes [1] Black-Scholes Nelson [2][3][4] Schrödinger Nelson Parisi Wu [5] Nelson Parisi-W 003 7 14 Black-Scholes [1] Nelson [] Schrödinger 1 Black Scholes [1] Black-Scholes Nelson [][3][4] Schrödinger Nelson Parisi Wu [5] Nelson Parisi-Wu Nelson e-mail: takatoshi-tasaki@nifty.com kabutaro@mocha.freemail.ne.jp

More information

Norisuke Sakai (Tokyo Institute of Technology) In collaboration with M. Eto, T. Fujimori, Y. Isozumi, T. Nagashima, M. Nitta, K. Ohashi, K. Ohta, Y. T

Norisuke Sakai (Tokyo Institute of Technology) In collaboration with M. Eto, T. Fujimori, Y. Isozumi, T. Nagashima, M. Nitta, K. Ohashi, K. Ohta, Y. T Norisuke Sakai (Tokyo Institute of Technology) In collaboration with M. Eto, T. Fujimori, Y. Isozumi, T. Nagashima, M. Nitta, K. Ohashi, K. Ohta, Y. Tachikawa, D. Tong, M. Yamazaki, and Y. Yang 2008.3.21-26,

More information

Chern-Simons Jones 3 Chern-Simons 1 - Chern-Simons - Jones J(K; q) [1] Jones q 1 J (K + ; q) qj (K ; q) = (q 1/2 q

Chern-Simons   Jones 3 Chern-Simons 1 - Chern-Simons - Jones J(K; q) [1] Jones q 1 J (K + ; q) qj (K ; q) = (q 1/2 q Chern-Simons E-mail: fuji@th.phys.nagoya-u.ac.jp Jones 3 Chern-Simons - Chern-Simons - Jones J(K; q) []Jones q J (K + ; q) qj (K ; q) = (q /2 q /2 )J (K 0 ; q), () J( ; q) =. (2) K Figure : K +, K, K 0

More information

QCD ( ), ( ) 8 23 Typeset by FoilTEX

QCD ( ), ( ) 8 23 Typeset by FoilTEX QCD ( ), ( ) 8 23 Typeset by FoilTEX Introduction:QCD Phase diagram of QCD system Critical end point Quark Gluon Plasma T c Temperature 1st order phase transition line Hadron 0 CSC 0 Chemical potential

More information

19 /

19 / 19 / 1 1.1............................... 1. Andreev............................... 3 1.3..................................... 3 1.4..................................... 4 / 5.1......................................

More information