Rethinking Flavor Physics
|
|
- Vincent Chase
- 5 years ago
- Views:
Transcription
1 Rethinking Flavor Physics René Sondenheimer FSU Jena & L. Egger, A. Maas arxiv: Cold Quantum Coffee, Heidelberg 30th of May 2017
2 LHC works remarkably well Higgs discovery completed SM 2
3 LHC works remarkably well Higgs discovery completed SM No direct signal of BSM physics 2
4 The Standard Model in a nutshell Ɣ 0 e MeV Gauge theory: U(1) 3
5 The Standard Model in a nutshell u +2/3 g 2.3 MeV -1/3 d 4.8 MeV Ɣ 0 0 e MeV Gauge theory: SU(3)C x U(1) 4
6 The Standard Model in a nutshell u +2/3 g 2.3 MeV -1/3 d 4.8 MeV Ɣ 0 0 e -1 W ± MeV 80.4 GeV ν e <2eV Z 91.2 GeV Gauge theory: SU(3)C x SU(2)L x U(1)Y 5
7 The Standard Model in a nutshell +2/3 +2/3 +2/3 u c t g 2.3 MeV GeV GeV -1/3-1/3-1/3 d s b 4.8 MeV 95 MeV 4.18 GeV Ɣ e μ τ -1 W ± MeV MeV 1.78 GeV 80.4 GeV ν e ν μ ν τ Z <2eV <0.17 MeV <15.5 MeV 91.2 GeV Gauge theory: SU(3)C x SU(2)L x U(1)Y 6
8 The Standard Model in a nutshell +2/3 +2/3 +2/3 u c t g 2.3 MeV GeV GeV -1/3-1/3-1/3 d s b 4.8 MeV 95 MeV 4.18 GeV Ɣ MeV MeV 1.78 GeV -1 e μ τ -1 W 80.4 GeV ±1 H ν e ν μ ν τ Z 125 GeV <2eV <0.17 MeV <15.5 MeV 91.2 GeV Gauge theory: SU(3)C x SU(2)L x U(1)Y 7
9 Quantum ChromoDynamics Elementary fields: Quarks and Gluons L = 1 4 Giµ G i µ + q a i /D ab q b + m q q a q a 8
10 Quantum ChromoDynamics Elementary fields: Quarks and Gluons L = 1 4 Giµ G i µ + q a i /D ab q b + m q q a q a Observable states: hadrons q q q q q g g g q q q q q q q q q q q Mesons Baryons Glueballs? Hybrids? Tetraquarks? Pentaquarks? 8
11 Quantum ChromoDynamics Elementary fields: Quarks and Gluons L = 1 4 Giµ G i µ + q a i /D ab q b + m q q a q a Observable states: hadrons q q q q q g g g q q q q q q q q q q q Mesons Baryons Glueballs? Hybrids? Tetraquarks? Pentaquarks? Can we observe a single quark? No. 8
12 Quantum ChromoDynamics Elementary fields: Quarks and Gluons L = 1 4 Giµ G i µ + q a i /D ab q b + m q q a q a Observable states: hadrons q q q q q g g g q q q q q q q q q q q Mesons Baryons Glueballs? Hybrids? Tetraquarks? Pentaquarks? Can we observe a single quark? No. Gauge invariance! 8
13 Higgs-W Subsector Elementary fields: Higgs and W L = 1 4 W iµ W i µ +(D µ ) a (D µ ) a U( a a ) 9
14 Higgs-W Subsector Elementary fields: Higgs and W L = 1 4 W iµ W i µ +(D µ ) a (D µ ) a U( a a ) U L Higgs potential: U = µ ( ) 2 f 9
15 Higgs-W Subsector Elementary fields: Higgs and W L = 1 4 W iµ W i µ +(D µ ) a (D µ ) a U( a a ) U L Higgs potential: U = µ ( ) 2 Expansion around vev: (x) = 1 ' p + (x) 2 v + h(x)+' 0 (x) f 9
16 Higgs-W Subsector Elementary fields: Higgs and W L = 1 4 W iµ W i µ +(D µ ) a (D µ ) a U( a a ) U L Higgs potential: U = µ ( ) 2 Expansion around vev: (x) = 1 ' p + (x) 2 v + h(x)+' 0 (x) f Mass for the W s from the Higgs kinetic term (D µ ) D µ = 1 2 g 2 v 2 4 W i µw iµ
17 Higgs-W Subsector BUT! Elementary states are not gauge invariant Cannot be observable Gauge-invariant states are composite e.g., Higgs-Higgs, W-W, Higgs-W,. W Bound states are not asymptotic states in perturbation theory Why does perturbation theory works at all? Higgs condensate exist only in some gauges Local symmetry breaking vs Elitzur s theorem Elitzur 81 Lee et al 72, Osterwalder&Seiler 77 10
18 Outline Introduction FMS mechanism Implications for Fermions Generations (FMS beyond the standard model) Summary 11
19 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, 81 12
20 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator 12
21 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator O(x) =( )(x) 12
22 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator O(x) =( )(x) 2. Expand Higgs field in correlator in fluctuations around the vev 12
23 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator O(x) =( )(x) 2. Expand Higgs field in correlator in fluctuations around the vev = v + ' ho(x)o(y)i = const. + v 2 hh(x)h(y)i + v 3 h'i + vh' 3 i + h' 4 i 12
24 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator O(x) =( )(x) 2. Expand Higgs field in correlator in fluctuations around the vev = v + ' ho(x)o(y)i = const. + v 2 hh(x)h(y)i + v 3 h'i + vh' 3 i + h' 4 i 3. Perform standard perturbation theory on the right-hand side 12
25 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator O(x) =( )(x) 2. Expand Higgs field in correlator in fluctuations around the vev = v + ' ho(x)o(y)i = const. + v 2 hh(x)h(y)i + v 3 h'i + vh' 3 i + h' 4 i 3. Perform standard perturbation theory on the right-hand side ho(x)o(y)i = v 2 hh(x)h(y)i tl + hh(x)h(y)i 2 tl + O(g 2, ) 12
26 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator O(x) =( )(x) 2. Expand Higgs field in correlator in fluctuations around the vev = v + ' ho(x)o(y)i = const. + v 2 hh(x)h(y)i + v 3 h'i + vh' 3 i + h' 4 i 3. Perform standard perturbation theory on the right-hand side ho(x)o(y)i = v 2 hh(x)h(y)i tl + hh(x)h(y)i 2 tl + O(g 2, ) 4. Compare poles on both sides 12
27 Fröhlich-Morchio-Strocchi mechanism Fröhlich et al 80, Construct a gauge-invariante operator O(x) =( )(x) 2. Expand Higgs field in correlator in fluctuations around the vev = v + ' ho(x)o(y)i = const. + v 2 hh(x)h(y)i + v 3 h'i + vh' 3 i + h' 4 i 3. Perform standard perturbation theory on the right-hand side ho(x)o(y)i = v 2 hh(x)h(y)i tl + hh(x)h(y)i 2 tl + O(g 2, ) 4. Compare poles on both sides Confirmed on the lattice for SU(2)-Higgs theory [Maas 12] 12
28 Fröhlich-Morchio-Strocchi mechanism 13
29 Fröhlich-Morchio-Strocchi mechanism W-Higgs sector of the standard model L = 1 4 W µ W i iµ +(D µ ) D µ U( ) Local SU(2) L Symmetry 13
30 Fröhlich-Morchio-Strocchi mechanism W-Higgs sector of the standard model L = 1 4 W i µ W iµ +(D µ ) D µ U( ) Local SU(2) L Symmetry W µ! UW µ U 1 i g (@ µu)u 1,! U 13
31 Fröhlich-Morchio-Strocchi mechanism W-Higgs sector of the standard model L = 1 4 W i µ W iµ +(D µ ) D µ U( ) Local SU(2) L Symmetry W µ! UW µ U 1 i g (@ µu)u 1,! U Additional global SU(2) cust. symmetry 13
32 Fröhlich-Morchio-Strocchi mechanism W-Higgs sector of the standard model L = 1 4 W i µ W iµ +(D µ ) D µ U( ) Local SU(2) L Symmetry W µ! UW µ U 1 i g (@ µu)u 1,! U Additional global SU(2) cust. symmetry W µ! W µ,! V + W 13
33 Fröhlich-Morchio-Strocchi mechanism W-Higgs sector of the standard model L = 1 4 W i µ W iµ +(D µ ) D µ U( ) Local SU(2) L Symmetry W µ! UW µ U 1 i g (@ µu)u 1,! U Additional global SU(2) cust. symmetry W µ! W µ,! V + W Convenient to rewrite Higgs-Lagrangian 13
34 Fröhlich-Morchio-Strocchi mechanism W-Higgs sector of the standard model L = 1 4 W i µ W iµ +(D µ ) D µ U( ) Local SU(2) L Symmetry W µ! UW µ U 1 i g (@ µu)u 1,! U Additional global SU(2) cust. symmetry W µ! W µ,! V + W Convenient to rewrite Higgs-Lagrangian L =Tr[@ µ µ X] U(TrX X) 13
35 Fröhlich-Morchio-Strocchi mechanism W-Higgs sector of the standard model L = 1 4 W i µ W iµ +(D µ ) D µ U( ) Local SU(2) L Symmetry W µ! UW µ U 1 i g (@ µu)u 1,! U Additional global SU(2) cust. symmetry W µ! W µ,! V + W Convenient to rewrite Higgs-Lagrangian L =Tr[@ µ µ X] U(TrX X) where X = = = v 0 0 v + O(')
36 Fröhlich-Morchio-Strocchi mechanism 14
37 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. 14
38 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. X! U L XU cust 14
39 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. X! U L XU cust W mass: bound state operator in 1- channel 14
40 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. X! U L XU cust W mass: bound state operator in 1- channel Oĩµ =itr( ĩx D µ X) 14
41 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. X! U L XU cust W mass: bound state operator in 1- channel Expand Higgs field: Oĩµ =itr( ĩx D µ X) 14
42 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. X! U L XU cust W mass: bound state operator in 1- channel Expand Higgs field: Oĩµ =itr( ĩx D µ X) hoĩµ(x)o j (y)i = g 2 v 4 hw i µ(x)w j (y)i iĩ j j + O(' 2 ) 14
43 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. X! U L XU cust W mass: bound state operator in 1- channel Expand Higgs field: Oĩµ =itr( ĩx D µ X) hoĩµ(x)o j (y)i = g 2 v 4 hw i µ(x)w j (y)i iĩ j j + O(' 2 ) Pole of bound state the same as for the elementary fields 14
44 Fröhlich-Morchio-Strocchi mechanism Full symmetry acting on the Higgs field: SU(2) L x SU(2)cust. X! U L XU cust W mass: bound state operator in 1- channel Expand Higgs field: Oĩµ =itr( ĩx D µ X) hoĩµ(x)o j (y)i = g 2 v 4 hw i µ(x)w j (y)i iĩ j j + O(' 2 ) Pole of bound state the same as for the elementary fields Mapping of local to global multiplets 14
45 Fermions Fröhlich et al 80 Egger,Maas,RS 17 15
46 Fermions Fröhlich et al 80 Egger,Maas,RS 17 Flavor = weak gauge charge in a given generation 15
47 Fermions Fröhlich et al 80 Egger,Maas,RS 17 Flavor = weak gauge charge in a given generation Necessary to construct suitable gauge-invariant state which emulate elementary fermions 15
48 Fermions Fröhlich et al 80 Egger,Maas,RS 17 Flavor = weak gauge charge in a given generation Necessary to construct suitable gauge-invariant state which emulate elementary fermions O g (x) =X (x)f g (x) 15
49 Fermions Fröhlich et al 80 Egger,Maas,RS 17 Flavor = weak gauge charge in a given generation Necessary to construct suitable gauge-invariant state which emulate elementary fermions O g (x) =X (x)f g (x) State remains custodial doublet 15
50 Fermions Fröhlich et al 80 Egger,Maas,RS 17 Flavor = weak gauge charge in a given generation Necessary to construct suitable gauge-invariant state which emulate elementary fermions O g (x) =X (x)f g (x) State remains custodial doublet E.g., (left-handed) electron and neutrino 15
51 Fermions Fröhlich et al 80 Egger,Maas,RS 17 Flavor = weak gauge charge in a given generation Necessary to construct suitable gauge-invariant state which emulate elementary fermions O g (x) =X (x)f g (x) State remains custodial doublet E.g., (left-handed) electron and neutrino O e = X = e e 2e = v e + O(') 15
52 Fermions Fröhlich et al 80 Egger,Maas,RS 17 Flavor = weak gauge charge in a given generation Necessary to construct suitable gauge-invariant state which emulate elementary fermions O g (x) =X (x)f g (x) State remains custodial doublet E.g., (left-handed) electron and neutrino O e = X = e e 2e = v e + O(') Ordinary states remerge when applying FMS 15
53 Fermions - Quarks Egger,Maas,RS 17 16
54 Fermions - Quarks O ud = X u d = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 16
55 Fermions - Quarks O ud = X u = d 2u 1d u 1u + = v + O(') 2d d Egger,Maas,RS 17 Quark sector different from lepton sector, bound in hadrons 16
56 Fermions - Quarks O ud = X u d = 2u 1u + 1d 2d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction = v u d + O(') Egger,Maas,RS 17 16
57 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 16
58 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 c ijkl q i q j q k X ĩl or q i q j q k X ĩi X jj X kk 16
59 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 c ijkl q i q j q k X ĩl or q i q j q k X ĩi X jj X kk c ijkl = a 1 ij kl + a 2 ik jl + a 3 jk il and ĩ =1 16
60 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 c ijkl q i q j q k X ĩl or q i q j q k X ĩi X jj X kk Proton: c ijkl = a 1 ij kl + a 2 ik jl + a 3 jk il and ĩ =1 16
61 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 c ijkl q i q j q k X ĩl or q i q j q k X ĩi X jj X kk Proton: c ijkl = a 1 ij kl + a 2 ik jl + a 3 jk il and ĩ =1 Some mesons are weak-gauge singlets, e.g., 16
62 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 c ijkl q i q j q k X ĩl or q i q j q k X ĩi X jj X kk Proton: c ijkl = a 1 ij kl + a 2 ik jl + a 3 jk il and ĩ =1 Some mesons are weak-gauge singlets, e.g.,! meson (ūu + dd) 16
63 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 c ijkl q i q j q k X ĩl or q i q j q k X ĩi X jj X kk Proton: c ijkl = a 1 ij kl + a 2 ik jl + a 3 jk il and ĩ =1 Some mesons are weak-gauge singlets, e.g.,! meson (ūu + dd) Not true for all mesons, e.g., pions 16
64 Fermions - Quarks O ud = X u d Quark sector different from lepton sector, bound in hadrons Hadrons singlets of strong interaction, not necessarily of weak interaction Obvious for baryons (strong indices suppressed) = 2u 1u + 1d 2d = v u d + O(') Egger,Maas,RS 17 c ijkl q i q j q k X ĩl or q i q j q k X ĩi X jj X kk Proton: c ijkl = a 1 ij kl + a 2 ik jl + a 3 jk il and ĩ =1 Some mesons are weak-gauge singlets, e.g.,! meson (ūu + dd) Not true for all mesons, e.g., pions 16 + : Ō ud 2 O ud 1 ( du)
65 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 17
66 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin 17
67 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space 17
68 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects 17
69 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects Speculation(!): 3 generations could be internal excitations of a single generation 17
70 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects Speculation(!): 3 generations could be internal excitations of a single generation SM effective theory of excitation spectrum 17
71 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects Speculation(!): 3 generations could be internal excitations of a single generation SM effective theory of excitation spectrum X Q E = T T Q E Q E = 2u E 2d E + 1 d E 1u E 17
72 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects Speculation(!): 3 generations could be internal excitations of a single generation SM effective theory of excitation spectrum Ground state: X Q E = T T Q E Q E = 2u E 2d E + 1 d E 1u E 17
73 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects Speculation(!): 3 generations could be internal excitations of a single generation SM effective theory of excitation spectrum X Q E = T T Q E Q E = 2u E 2d E + 1 d E 1u E Ground state: d =( Q E ) g 17
74 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects Speculation(!): 3 generations could be internal excitations of a single generation SM effective theory of excitation spectrum X Q E = T T Q E Q E = 2u E 2d E + 1 d E 1u E Ground state: d =( Q E ) g higher excitations: 17
75 Generations as excitation spectra (speculation!) Egger,Maas,RS 17 Flavor identity from combination of generation and weak isospin Difference: Yukawa and weak interactions cannot be simultaneously diagonal in generation space Flavor distinguishes between inter- and intrageneration effects Speculation(!): 3 generations could be internal excitations of a single generation SM effective theory of excitation spectrum X Q E = T T Q E Q E = 2u E 2d E + 1 d E 1u E Ground state: higher excitations: d =( Q E ) g s =( Q E ), b =( Q E ) 17
76 Gauge-invariant perturbation theory Egger,Maas,RS 17 Lepton collision as probing experiment of the bound state structure M = ho e 2 (p 1 )Ō e 2 (p 2 )O f (q 1 )Ōf (q 2 )i v 4 he + e ffi + he + e ihhh ffi +... Final state μ b t 1.00 dσ Full dσ Perturbative s 18
77 BSM - Grand Unified theories Maas,Törek 16 Maas,Törek,RS, in preparation 19
78 BSM - Grand Unified theories Maas,Törek 16 Maas,Törek,RS, in preparation SU(N) gauge theory + Higgs in fundamental representation Perturbative mass spectrum: 2N - 1 massive gauge bosons (N-1) 2-1 massless gauge bosons 1 massive scalar Higgs boson 19
79 BSM - Grand Unified theories Maas,Törek 16 Maas,Törek,RS, in preparation SU(N) gauge theory + Higgs in fundamental representation Perturbative mass spectrum: 2N - 1 massive gauge bosons (N-1) 2-1 massless gauge bosons 1 massive scalar Higgs boson Local and global symmetry group do not match for N > 2 19
80 BSM - Grand Unified theories Maas,Törek 16 Maas,Törek,RS, in preparation SU(N) gauge theory + Higgs in fundamental representation Perturbative mass spectrum: 2N - 1 massive gauge bosons (N-1) 2-1 massless gauge bosons 1 massive scalar Higgs boson Local and global symmetry group do not match for N > 2 1 neutral bound state in 0+ channel = Higgs 19
81 BSM - Grand Unified theories Maas,Törek 16 Maas,Törek,RS, in preparation SU(N) gauge theory + Higgs in fundamental representation Perturbative mass spectrum: 2N - 1 massive gauge bosons (N-1) 2-1 massless gauge bosons 1 massive scalar Higgs boson Local and global symmetry group do not match for N > 2 1 neutral bound state in 0+ channel = Higgs Only 1 bound state in 1- channel (U(1) singlet) i D µ 19
82 BSM - Grand Unified theories Maas,Törek 16 Maas,Törek,RS, in preparation SU(N) gauge theory + Higgs in fundamental representation Perturbative mass spectrum: 2N - 1 massive gauge bosons (N-1) 2-1 massless gauge bosons 1 massive scalar Higgs boson Local and global symmetry group do not match for N > 2 1 neutral bound state in 0+ channel = Higgs Only 1 bound state in 1- channel (U(1) singlet) i D µ 1- states with open U(1) quantum number? abc a (D µ ) b (D D ) c (for SU(3)) 19
83 Summary Observable spectrum must be gauge invariant Non-Abelian gauge theory: composite operator FMS mechanism provides a mapping of the local to the global multiplets Gauge-invariant perturbation theory as a tool BSM model building may be affected Same results in leading order for the standard model Verification requieres non-perturbative methods 20
On the observable spectrum of theories with a Brout-Englert-Higgs effect
On the observable spectrum of theories with a Brout-Englert-Higgs effect René Sondenheimer FSU Jena & L. Egger, A. Maas arxiv:1701.02881 & A. Maas, P.Törek arxiv:1709.07477, arxiv:1710.01941 Higgs Couplings
More informationThe physical spectrum of theories with a Brout-Englert-Higgs effect
The physical spectrum of theories with a Brout-Englert-Higgs effect Pascal Törek with Axel Maas and René Sondenheimer University of Graz Alps 2018, Obergurgl, 18 th of April, 2018 [1709.07477 and 1804.04453]
More informationThe Strong Interaction and LHC phenomenology
The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Lecture 2: The QCD Lagrangian, Symmetries and Feynman Rules
More informationIntroduction to the Standard Model New Horizons in Lattice Field Theory IIP Natal, March 2013
Introduction to the Standard Model New Horizons in Lattice Field Theory IIP Natal, March 2013 Rogerio Rosenfeld IFT-UNESP Lecture 1: Motivation/QFT/Gauge Symmetries/QED/QCD Lecture 2: QCD tests/electroweak
More informationA model of the basic interactions between elementary particles is defined by the following three ingredients:
I. THE STANDARD MODEL A model of the basic interactions between elementary particles is defined by the following three ingredients:. The symmetries of the Lagrangian; 2. The representations of fermions
More informationThe Physics Of Yang-Mills-Higgs Systems
The Physics Of Yang-Mills-Higgs Systems Beyond Perturbation Theory Axel Maas 9 th of January 2014 University of Heidelberg Germany Overview Yang-Mills-Higgs theory Overview Yang-Mills-Higgs theory Physical
More informationLecture III: Higgs Mechanism
ecture III: Higgs Mechanism Spontaneous Symmetry Breaking The Higgs Mechanism Mass Generation for eptons Quark Masses & Mixing III.1 Symmetry Breaking One example is the infinite ferromagnet the nearest
More informationMesons beyond the quark-antiquark picture: glueballs, hybrids, tetraquarks - part 1 - Francesco Giacosa
Mesons beyond the quark-antiquark picture: glueballs, hybrids, tetraquarks - part 1-55 Cracow School of Theoretical Physics 20 28/6/2015, Zakopane, Poland Outline The Lagrangian of QCD and its symmetries
More informationNew Physics from Vector-Like Technicolor: Roman Pasechnik Lund University, THEP group
New Physics from Vector-Like Technicolor: Roman Pasechnik Lund University, THEP group CP3 Origins, September 16 th, 2013 At this seminar I will touch upon... σ 2 Issues of the Standard Model Dramatically
More informationLecture 19. November 2, Comments on HW3. Introduction to EWK symmetry breaking. Hydro Model of a Quark-Gluon Plasma Tianyu Dai
Lecture 19 November 2, 2017 Comments on HW3 Introduction to EWK symmetry breaking Hydro Model of a Quark-Gluon Plasma Tianyu Dai 1 Class Plans Date Lecture Essay presentation (15 minutes) Nov. 2 19 Tianyu
More informationHunting New Physics in the Higgs Sector
HS Hunting New Physics in the Higgs Sector SM Higgs Sector - Test of the Higgs Mechanism Oleg Kaikov KIT, Seminar WS 2015/16 Prof. Dr. M. Margarete Mühlleitner, Dr. Roger Wolf, Dr. Hendrik Mantler Advisor:
More informationFor Review Only. General Structure of Democratic Mass Matrix of Lepton Sector in E 6 Model. Canadian Journal of Physics
General Structure of Democratic Mass Matrix of Lepton Sector in E 6 Model Journal: Canadian Journal of Physics Manuscript ID cjp-2017-0783.r1 Manuscript Type: Article Date Submitted by the Author: 08-Jan-2018
More informationQuark Model. Ling-Fong Li. (Institute) Note 8 1 / 26
Quark Model Ling-Fong Li (Institute) Note 8 1 / 6 QCD Quark Model Isospin symmetry To a good approximation, nuclear force is independent of the electric charge carried by the nucleons charge independence.
More informationLecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM
Lecture 03 The Standard Model of Particle Physics Part II The Higgs Boson Properties of the SM The Standard Model So far we talked about all the particles except the Higgs If we know what the particles
More informationStrongly Coupled Dark Matter at the LHC
Strongly Coupled Dark Matter at the LHC Graham Kribs University of Oregon Appelquist et al (LSD Collaboration): 1402.6656; 1503.04203; 1503.04205 GK, Adam Martin, Ethan Neil, Bryan Ostdiek, Tom Tong [in
More informationThis means that n or p form a doublet under isospin transformation. Isospin invariance simply means that. [T i, H s ] = 0
1 QCD 1.1 Quark Model 1. Isospin symmetry In early studies of nuclear reactions, it was found that, to a good approximation, nuclear force is independent of the electromagnetic charge carried by the nucleons
More informationPhysics 4213/5213 Lecture 1
August 28, 2002 1 INTRODUCTION 1 Introduction Physics 4213/5213 Lecture 1 There are four known forces: gravity, electricity and magnetism (E&M), the weak force, and the strong force. Each is responsible
More informationPatrick Kirchgaeßer 07. Januar 2016
Patrick Kirchgaeßer 07. Januar 2016 INSTITUTE OF EXPERIMENTAL PARTICLE PHYSICS (IEKP) PHYSICS FACULTY KIT Universität des Landes Baden-Württemberg und nationales Forschungszentrum in der Helmholtz-Gemeinschaft
More informationThe Standard Model and Beyond
The Standard Model and Beyond Nobuchika Okada Department of Physics and Astronomy The University of Alabama 2011 BCVSPIN ADVANCED STUDY INSTITUTE IN PARTICLE PHYSICS AND COSMOLOGY Huê, Vietnam, 25-30,
More informationNovember 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model
Scalar from November 24, 2014 1 2 3 4 5 What is the? Gauge theory that explains strong weak, and electromagnetic forces SU(3) C SU(2) W U(1) Y Each generation (3) has 2 quark flavors (each comes in one
More informationIntroduction to the SM (5)
Y. Grossman The SM (5) TES-HEP, July 12, 2015 p. 1 Introduction to the SM (5) Yuval Grossman Cornell Y. Grossman The SM (5) TES-HEP, July 12, 2015 p. 2 Yesterday... Yesterday: Symmetries Today SSB the
More informationThe Standard Model and beyond
The Standard Model and beyond In this chapter we overview the structure of the Standard Model (SM) of particle physics, its shortcomings, and different ideas for physics beyond the Standard Model (BSM)
More informationNon-Abelian SU(2) H and Two-Higgs Doublets
Non-Abelian SU(2) H and Two-Higgs Doublets Technische Universität Dortmund Wei- Chih Huang 25 Sept 2015 Kavli IPMU arxiv:1510.xxxx(?) with Yue-Lin Sming Tsai, Tzu-Chiang Yuan Plea Please do not take any
More informationIntroduction to Quantum Chromodynamics (QCD)
Introduction to Quantum Chromodynamics (QCD) Jianwei Qiu Theory Center, Jefferson Lab May 29 June 15, 2018 Lecture One The plan for my four lectures q The Goal: To understand the strong interaction dynamics
More informationDirections for BSM physics from Asymptotic Safety
Bad Honnef- 21.6.2018 Directions for BSM physics from Asymptotic Safety phenomenology connecting theory to data Gudrun Hiller, TU Dortmund q f e DFG FOR 1873 et 1 Asymptotic Safety pheno for cosmology
More informationA String Model for Preons and the Standard Model Particles. Abstract
March 5, 013 A String Model for Preons and the Standard Model Particles Risto Raitio 1 030 Espoo, Finland Abstract A preon model for standard model particles is proposed based on spin 1 fermion and spin
More informationGauge coupling unification without leptoquarks Mikhail Shaposhnikov
Gauge coupling unification without leptoquarks Mikhail Shaposhnikov March 9, 2017 Work with Georgios Karananas, 1703.02964 Heidelberg, March 9, 2017 p. 1 Outline Motivation Gauge coupling unification without
More informationE 6 Spectra at the TeV Scale
E 6 Spectra at the TeV Scale Instituts-Seminar Kerne und Teilchen, TU Dresden Alexander Knochel Uni Freiburg 24.06.2010 Based on: F. Braam, AK, J. Reuter, arxiv:1001.4074 [hep-ph], JHEP06(2010)013 Outline
More informationBaryon and Lepton Number Violation at the TeV Scale
Baryon and Lepton Number Violation at the TeV Scale S. Nandi Oklahoma State University and Oklahoma Center for High Energy Physics : S. Chakdar, T. Li, S. Nandi and S. K. Rai, arxiv:1206.0409[hep-ph] (Phys.
More informationThe mass of the Higgs boson
The mass of the Higgs boson LHC : Higgs particle observation CMS 2011/12 ATLAS 2011/12 a prediction Higgs boson found standard model Higgs boson T.Plehn, M.Rauch Spontaneous symmetry breaking confirmed
More informationThe symmetries of QCD (and consequences)
The symmetries of QCD (and consequences) Sinéad M. Ryan Trinity College Dublin Quantum Universe Symposium, Groningen, March 2018 Understand nature in terms of fundamental building blocks The Rumsfeld
More informationAstronomy, Astrophysics, and Cosmology
Astronomy, Astrophysics, and Cosmology Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson IX April 12, 2016 arxiv:0706.1988 L. A. Anchordoqui (CUNY)
More informationElectroweak and Higgs Physics
Electroweak and Higgs Physics Lecture 2 : Higgs Mechanism in the Standard and Supersymmetric Models Alexei Raspereza DESY Summer Student Program Hamburg August 2017 Standard Model (Summary) Building blocks
More informationCurrent knowledge tells us that matter is made of fundamental particle called fermions,
Chapter 1 Particle Physics 1.1 Fundamental Particles Current knowledge tells us that matter is made of fundamental particle called fermions, which are spin 1 particles. Our world is composed of two kinds
More informationFlavor Physics in the multi-higgs doublet models induced by the left-right symmetry
Flavor Physics in the multi-higgs doublet models induced by the left-right symmetry Yoshihiro Shigekami KEK HUST ( 華中科技大学 ), Wuhan ( 武漢 ) Syuhei Iguro (Nagoya U.), Yu Muramatsu (CCNU), Yuji Omura (Nagoya
More informationLecture 2: The First Second origin of neutrons and protons
Lecture 2: The First Second origin of neutrons and protons Hot Big Bang Expanding and cooling Soup of free particles + anti-particles Symmetry breaking Soup of free quarks Quarks confined into neutrons
More informationParticle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden
Particle Physics Tommy Ohlsson Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden International Baccalaureate T. Ohlsson (KTH) Particle Physics 1/
More informationINTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS
INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS Class Mechanics My office (for now): Dantziger B Room 121 My Phone: x85200 Office hours: Call ahead, or better yet, email... Even better than office
More informationFundamental Forces. David Morrissey. Key Concepts, March 15, 2013
Fundamental Forces David Morrissey Key Concepts, March 15, 2013 Not a fundamental force... Also not a fundamental force... What Do We Mean By Fundamental? Example: Electromagnetism (EM) electric forces
More informationLittle Higgs Models Theory & Phenomenology
Little Higgs Models Theory Phenomenology Wolfgang Kilian (Karlsruhe) Karlsruhe January 2003 How to make a light Higgs (without SUSY) Minimal models The Littlest Higgs and the Minimal Moose Phenomenology
More informationLecture 23. November 16, Developing the SM s electroweak theory. Fermion mass generation using a Higgs weak doublet
Lecture 23 November 16, 2017 Developing the SM s electroweak theory Research News: Higgs boson properties and use as a dark matter probe Fermion mass generation using a Higgs weak doublet Summary of the
More informationBeyond Standard Model Effects in Flavour Physics: p.1
Beyond Standard Model Effects in Flavour Physics: Alakabha Datta University of Mississippi Feb 13, 2006 Beyond Standard Model Effects in Flavour Physics: p.1 OUTLINE Standard Model (SM) and its Problems.
More informationS 3 Symmetry as the Origin of CKM Matrix
S 3 Symmetry as the Origin of CKM Matrix Ujjal Kumar Dey Physical Research Laboratory October 25, 2015 Based on: PRD 89, 095025 and arxiv:1507.06509 Collaborators: D. Das and P. B. Pal 1 / 25 Outline 1
More informationLe Modèle Standard et ses extensions
Particules Élémentaires, Gravitation et Cosmologie Année 2007-08 08 Le Modèle Standard et ses extensions Cours III: 15 février f 2008 Weak Interactions: from Fermi s s model to a gauge theory 15 fevrier
More information12.2 Problem Set 2 Solutions
78 CHAPTER. PROBLEM SET SOLUTIONS. Problem Set Solutions. I will use a basis m, which ψ C = iγ ψ = Cγ ψ (.47) We can define left (light) handed Majorana fields as, so that ω = ψ L + (ψ L ) C (.48) χ =
More informationThe Higgs Boson and Electroweak Symmetry Breaking
The Higgs Boson and Electroweak Symmetry Breaking 1. Minimal Standard Model M. E. Peskin Chiemsee School September 2014 The Higgs boson has an odd position in the Standard Model of particle physics. On
More informationQuark Model History and current status
Quark Model History and current status Manon Bischoff Heavy-Ion Seminar 2013 October 31, 2013 Manon Bischoff Quark Model 1 Outline Introduction Motivation and historical development Group theory and the
More informationMass. Chris Quigg Fermi National Accelerator Laboratory
Mass Chris Quigg Fermi National Accelerator Laboratory YITP@40 Stony Brook 4 May 2007 I. Newton (1687) Mass: the quantity of matter arising from its density and bulk conjointly F = ma + Universal Gravitation
More informationThe Physics of Heavy Z-prime Gauge Bosons
The Physics of Heavy Z-prime Gauge Bosons Tevatron LHC LHC LC LC 15fb -1 100fb -1 14TeV 1ab -1 14TeV 0.5TeV 1ab -1 P - =0.8 P + =0.6 0.8TeV 1ab -1 P - =0.8 P + =0.6 χ ψ η LR SSM 0 2 4 6 8 10 12 2σ m Z'
More informationThe Scale-Symmetric Theory as the Origin of the Standard Model
Copyright 2017 by Sylwester Kornowski All rights reserved The Scale-Symmetric Theory as the Origin of the Standard Model Sylwester Kornowski Abstract: Here we showed that the Scale-Symmetric Theory (SST)
More informationHadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora
Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora Hadron Physics & QCD Part 1: First Encounter With Hadrons: Introduction to Mesons & Baryons, The Quark
More informationFlavour physics Lecture 1
Flavour physics Lecture 1 Jim Libby (IITM) XI th SERC school on EHEP NISER Bhubaneswar November 2017 Lecture 1 1 Outline What is flavour physics? Some theory and history CKM matrix Lecture 1 2 What is
More informationStandard Model & Beyond
XI SERC School on Experimental High-Energy Physics National Institute of Science Education and Research 13 th November 2017 Standard Model & Beyond Lecture III Sreerup Raychaudhuri TIFR, Mumbai 2 Fermions
More informationNeutrino Masses SU(3) C U(1) EM, (1.2) φ(1, 2) +1/2. (1.3)
Neutrino Masses Contents I. The renormalizable Standard Model 1 II. The non-renormalizable Standard Model III. The See-Saw Mechanism 4 IV. Vacuum Oscillations 5 V. The MSW effect 7 VI. Experimental results
More informationPossible Color Octet Quark-Anti-Quark Condensate in the. Instanton Model. Abstract
SUNY-NTG-01-03 Possible Color Octet Quark-Anti-Quark Condensate in the Instanton Model Thomas Schäfer Department of Physics, SUNY Stony Brook, Stony Brook, NY 11794 and Riken-BNL Research Center, Brookhaven
More informationLecture 16 V2. October 24, 2017
Lecture 16 V2 October 24, 2017 Recap: gamma matrices Recap: pion decay properties Unifying the weak and electromagnetic interactions Ø Recap: QED Lagrangian for U Q (1) gauge symmetry Ø Introduction of
More informationDark matter and IceCube neutrinos
IL NUOVO CIMENTO 38 C (2015) 31 DOI 10.1393/ncc/i2015-15031-4 Colloquia: IFAE 2014 Dark matter and IceCube neutrinos R. Biondi Dipartimento di Scienze Fisiche e Chimiche, Università degli Studi di L Aquila,
More informationPHYSICS PARTICLE. An Introductory Course of. Palash B. Pal. CRC Press. Saha Institute of Nuclear Physics. Kolkata, India. Taylor &.
An Introductory Course of PARTICLE PHYSICS Palash B. Pal Saha Institute of Nuclear Physics Kolkata, India W CRC Press Taylor &. Francis Croup Boca Raton London New York CRC Press is an imprint of the &
More informationIsospin. K.K. Gan L5: Isospin and Parity 1
Isospin Isospin is a continuous symmetry invented by Heisenberg: Explain the observation that the strong interaction does not distinguish between neutron and proton. Example: the mass difference between
More informationElementary Particles, Flavour Physics and all that...
Elementary Particles, Flavour Physics and all that... 1 Flavour Physics The term Flavour physics was coined in 1971 by Murray Gell-Mann and his student at the time, Harald Fritzsch, at a Baskin-Robbins
More informationTwo-Higgs-Doublet Model
Two-Higgs-Doublet Model Logan A. Morrison University of California, Santa Cruz loanmorr@ucsc.edu March 18, 016 Logan A. Morrison (UCSC) HDM March 18, 016 1 / 7 Overview 1 Review of SM HDM Formalism HDM
More informationF. Börkeroth, F. J. de Anda, I. de Medeiros Varzielas, S. F. King. arxiv:
F. Börkeroth, F. J. de Anda, I. de Medeiros Varzielas, S. F. King S FLASY 2015 arxiv:1503.03306 Standard Model Gauge theory SU(3)C X SU(2)L X U(1)Y Standard Model Gauge theory SU(3)C X SU(2)L X U(1)Y SM:
More informationParticle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry
Particle Physics JJ Thompson discovered electrons in 1897 Rutherford discovered the atomic nucleus in 1911 and the proton in 1919 (idea of gold foil expt) All science is either physics or stamp collecting
More informationG2 gauge theories. Axel Maas. 14 th of November 2013 Strongly-Interacting Field Theories III Jena, Germany
G2 gauge theories Axel Maas 14 th of November 2013 Strongly-Interacting Field Theories III Jena, Germany Overview Why G2? Overview Why G2? G2 Yang-Mills theory Running coupling [Olejnik, Maas JHEP'08,
More informationProblems for SM/Higgs (I)
Problems for SM/Higgs (I) 1 Draw all possible Feynman diagrams (at the lowest level in perturbation theory) for the processes e + e µ + µ, ν e ν e, γγ, ZZ, W + W. Likewise, draw all possible Feynman diagrams
More informationNeutrino Masses and Dark Matter in Gauge Theories for Baryon and Lepton Numbers
Neutrino Masses and Dark Matter in Gauge Theories for Baryon and Lepton Numbers DPG Frühjahrstagung 014 in Mainz Based on Phys. Rev. Lett. 110, 31801 (013), Phys. Rev. D 88, 051701(R) (013), arxiv:1309.3970
More informationTwo models with extra Higgs doublets and Axions
Two models with extra Higgs doublets and Axions H Serôdio (KAIST) 4 th KIAS Workshop Particle Physics and Cosmology, 30 October 2014 In collaboration with: Alejandro Celis, Javier Fuentes-Martin Works:
More informationTheory toolbox. Chapter Chiral effective field theories
Chapter 3 Theory toolbox 3.1 Chiral effective field theories The near chiral symmetry of the QCD Lagrangian and its spontaneous breaking can be exploited to construct low-energy effective theories of QCD
More informationUnification without Doublet-Triplet Splitting SUSY Exotics at the LHC
Unification without Doublet-Triplet Splitting SUSY Exotics at the LHC Jürgen Reuter Carleton University, Ottawa University of Freiburg W. Kilian, J. Reuter, PLB B642 (2006), 81, and work in progress (with
More informationfrom exact asymptotic safety to physics beyond the Standard Model
from exact asymptotic safety to physics beyond the Standard Model Daniel F Litim Heidelberg, 9 Mar 2017 DF Litim 1102.4624 DF Litim, F Sannino, 1406.2337 AD Bond, DF Litim, 1608.00519 AD Bond, G Hiller,
More informationDouble Higgs production via gluon fusion (gg hh) in composite models
Double Higgs production via gluon fusion (gg hh) in composite models Ennio Salvioni CERN and University of Padova based on work in collaboration with C.Grojean (CERN), M.Gillioz (Zürich), R.Gröber and
More informationThe Standard Model of particle physics and beyond
The Standard Model of particle physics and beyond - Lecture 3: Beyond the Standard Model Avelino Vicente IFIC CSIC / U. Valencia Physics and astrophysics of cosmic rays in space Milano September 2016 1
More informationLectures on Chiral Perturbation Theory
Lectures on Chiral Perturbation Theory I. Foundations II. Lattice Applications III. Baryons IV. Convergence Brian Tiburzi RIKEN BNL Research Center Chiral Perturbation Theory I. Foundations Low-energy
More informationHiggs Property Measurement with ATLAS
Higgs Property Measurement with ATLAS Haijun Yang (on behalf of the ATLAS) Shanghai Jiao Tong University Hadron Collider Physics Symposium HCP 2012, Kyoto University, Japan November 12-16, 2012 Observation
More informationEffective Theory for Electroweak Doublet Dark Matter
Effective Theory for Electroweak Doublet Dark Matter University of Ioannina, Greece 3/9/2016 In collaboration with Athanasios Dedes and Vassilis Spanos ArXiv:1607.05040 [submitted to PhysRevD] Why dark
More informationThe Higgs discovery - a portal to new physics
The Higgs discovery - a portal to new physics Department of astronomy and theoretical physics, 2012-10-17 1 / 1 The Higgs discovery 2 / 1 July 4th 2012 - a historic day in many ways... 3 / 1 July 4th 2012
More informationElectroweak physics and the LHC an introduction to the Standard Model
Electroweak physics and the LHC an introduction to the Standard Model Paolo Gambino INFN Torino LHC School Martignano 12-18 June 2006 Outline Prologue on weak interactions Express review of gauge theories
More informationExotic scalars. Stefania Gori. Second MCTP Spring Symposium on Higgs Boson Physics. The University of Chicago & Argonne National Laboratory
Exotic Exotic scalars scalars and and the the Higgs Higgs to to gamma gamma -- gamma gamma rate rate Stefania Gori The University of Chicago & Argonne National Laboratory Second MCTP Spring Symposium on
More informationCritical lines and points. in the. QCD phase diagram
Critical lines and points in the QCD phase diagram Understanding the phase diagram Phase diagram for m s > m u,d quark-gluon plasma deconfinement quark matter : superfluid B spontaneously broken nuclear
More informationWeak interactions and vector bosons
Weak interactions and vector bosons What do we know now about weak interactions? Theory of weak interactions Fermi's theory of weak interactions V-A theory Current - current theory, current algebra W and
More informationIllustration of the Emergence of Fundamental Forces
Copyright 2017 by Sylwester Kornowski All rights reserved Illustration of the Emergence of Fundamental Forces Sylwester Kornowski Abstract: Here, within the Scale-Symmetric Theory (SST), we illustrate
More informationThe Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten
Lecture 4 QCD as a Gauge Theory Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local
More informationThe Strong Interaction and LHC phenomenology
The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Introduction and motivation: QCD and modern high-energy physics
More informationChapter 1. Introduction
Chapter 1 Introduction 1.1 Fundamental Forces Particle physics is concerned with the fundamental constituents of matter and the fundamental forces through which the fundamental constituents interact among
More informationStrongly coupled gauge theories: What can lattice calculations teach us?
Strongly coupled gauge theories: What can lattice calculations teach us? Anna Hasenfratz University of Colorado Boulder Rencontres de Moriond, March 21 216 Higgs era of particle physics The 212 discovery
More informationLecture 9 Valence Quark Model of Hadrons
Lecture 9 Valence Quark Model of Hadrons Isospin symmetry SU(3) flavour symmetry Meson & Baryon states Hadronic wavefunctions Masses and magnetic moments Heavy quark states 1 Isospin Symmetry Strong interactions
More informationThe Phases of QCD. Thomas Schaefer. North Carolina State University
The Phases of QCD Thomas Schaefer North Carolina State University 1 Motivation Different phases of QCD occur in the universe Neutron Stars, Big Bang Exploring the phase diagram is important to understanding
More information8.882 LHC Physics. Higgs Physics and Other Essentials. [Lecture 22, April 29, 2009] Experimental Methods and Measurements
8.882 LHC Physics Experimental Methods and Measurements Higgs Physics and Other Essentials [Lecture 22, April 29, 2009] Organization Next week lectures: Monday 2pm and Tuesday 9:30am (which room?) Project
More informationThe Role and Discovery of the Higgs
The Role and Discovery of the Higgs David Clarke Abstract This paper summarizes the importance of the Higgs boson in QFT and outlines experiments leading up to the discovery of the Higgs boson. First we
More informationRichard Williams. Hèlios Sanchis-Alepuz
Richard Williams Hèlios Sanchis-Alepuz Introduction 2 Idea: Information on hadron properties encoded in Green s functions EM form-factors Dyson-Schwinger Approach Nonpert. Covariant Multi-scale Symmetries
More informationFlavor, Minimality and Naturalness in Composite Higgs Models
eth zurich Flavor, Minimality and Naturalness in Composite Higgs Models Adrián Carmona Bermúdez Institute for Theoretical Physics, ETH Zurich In collaboration with F. Goertz A naturally light Higgs without
More information1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles
1 Introduction The purpose of this chapter is to provide a brief introduction to the Standard Model of particle physics. In particular, it gives an overview of the fundamental particles and the relationship
More informationThe SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry Breaking Gell-Mann Okubo Mass Formulae Quark-Mo
Lecture 2 Quark Model The Eight Fold Way Adnan Bashir, IFM, UMSNH, Mexico August 2014 Culiacán Sinaloa The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry
More informationFermion Mixing Angles and the Connection to Non-Trivially Broken Flavor Symmetries
Fermion Mixing ngles and the Connection to Non-Trivially Broken Flavor Symmetries C. Hagedorn hagedorn@mpi-hd.mpg.de Max-Planck-Institut für Kernphysik, Heidelberg, Germany. Blum, CH, M. Lindner numerics:.
More informationPHYSICS BEYOND SM AND LHC. (Corfu 2010)
PHYSICS BEYOND SM AND LHC (Corfu 2010) We all expect physics beyond SM Fantastic success of SM (LEP!) But it has its limits reflected by the following questions: What is the origin of electroweak symmetry
More informationLecture 8. September 21, General plan for construction of Standard Model theory. Choice of gauge symmetries for the Standard Model
Lecture 8 September 21, 2017 Today General plan for construction of Standard Model theory Properties of SU(n) transformations (review) Choice of gauge symmetries for the Standard Model Use of Lagrangian
More informationFundamental Particles and Forces
Fundamental Particles and Forces A Look at the Standard Model and Interesting Theories André Gras PHYS 3305 SMU 1 Overview Introduction to Fundamental Particles and Forces Brief History of Discovery The
More informationFundamental Symmetries - 2
HUGS 2018 Jefferson Lab, Newport News, VA May 29- June 15 2018 Fundamental Symmetries - 2 Vincenzo Cirigliano Los Alamos National Laboratory Plan of the lectures Review symmetry and symmetry breaking Introduce
More information1/N Expansions in String and Gauge Field Theories. Adi Armoni Swansea University
1/N Expansions in String and Gauge Field Theories Adi Armoni Swansea University Oberwoelz, September 2010 1 Motivation It is extremely difficult to carry out reliable calculations in the strongly coupled
More informationDEEP INELASTIC SCATTERING
DEEP INELASTIC SCATTERING Electron scattering off nucleons (Fig 7.1): 1) Elastic scattering: E = E (θ) 2) Inelastic scattering: No 1-to-1 relationship between E and θ Inelastic scattering: nucleon gets
More information