SUSY QCD. Consider a SUSY SU(N) with F flavors of quarks and squarks
|
|
- Pamela Gibbs
- 5 years ago
- Views:
Transcription
1 SUSY gauge theories
2 SUSY QCD Consider a SUSY SU(N) with F flavors of quarks and squarks Q i = (φ i, Q i, F i ), i = 1,..., F, where φ is the squark and Q is the quark. Q i = (φ i, Q i, F i ), in the antifundamental representation. Note the the bar ( the name not a conjugation, the conjugate fields are ) is part of Q i = (φ i, Q i, F i ), Q i = (φ i, Q i, F i ).
3 SUSY QCD matter content is: SU(N) SU(F ) SU(F ) U(1) B U(1) R Q 1 1 F N F Q 1 1 F N F W =
4 R-charge [R, Q α ] = Q α. chiral supermultiplet: R ψ = R φ 1, normalize the R-charge by Rλ a = λ a, R-charge of the gluino is 1, and the R-charge of the gluon is.
5 Group Theory: Bird Tracks Identify the group generator with a vertex as in Fig.??. a m r ) n (T = n m Figure 1: Bird-track notation for the group generator T a.
6 Bird Tracks quadratic Casimir C 2 (r) and the indext (r) of the representation r, are given diagrammaticly as (T a r ) m l (T a r ) l n = C 2 (r)δ m n, (T a r ) m n (T b r ) n m = T (r)δ ab, m C (r) δ = 2 n n m T(r) δ ab = a b Figure 2:
7 Bird Tracks Contracting the external legs: In the first diagram setting m equal = Figure 3: to n and summing over n yields a factor of d(r). In the second diagram setting a equal to b and summing yields a factor d(ad). d(r)c 2 (r) = d(ad)t (r).
8 Casimirs d( ) = N, d(ad) = N 2 1 T ( ) = 1 2, T (Ad) = N so C 2 ( ) = N 2 1 2N, C 2(Ad) = N.
9 Sum over Generators For the fundamental representation : (T a ) l p(t a ) m n = 1 2 (δl nδ m p 1 N δl pδ m n ). = 1 2 2Ν 1 Figure 4: We can reduce the sums over multiple generators to an essentially topological exercise
10 Anomalies Since we can define an R-charge by taking arbitrary linear combinations of the U(1) R and U(1) B charges we can choose Q i and Q i to have the same R-charge. For a U(1) not be to broken by instanton effects the SU(N) 2 U(1) R anomaly diagram vanishes Figure 5: fermion contributes its R-charge times T (r). Sum over gluino, quarks: 1 T (Ad) + (R 1)T ( ) 2F =, so R = F N F
11 Renormalization group tree-level SUSY: Y = 2g, λ = g 2. For SUSY to be a consistent quantum symmetry these relations must be preserved under RG running. the β function for the gauge coupling at one-loop is β g = µ dg dµ = g3 16π 2 ( 11 3 T (Ad) 2 3 T (F ) 1 3 T (S)) g3 b 16π 2, For SUSY QCD: b = (3N F )
12 where Renormalization group the β function for the Yukawa coupling is : [ ] (4π) 2 β j Y = 1 2 Y 2 (F )Y j + Y j Y 2 (F ) + 2Y k Y j Y k +Y k Tr Y k Y j 3gm{C 2 2 m (F ), Y j }, Y 2 (F ) Y j Y j Y 2 (F )Y j represents the scalar loop corrections to the fermion legs 2Y k Y j Y k contains the 1PI vertex corrections Y k Tr Y k Y j represents fermion loop corrections to the scalar leg C m 2 (F ) is the quadratic Casimir of the fermion fields in the mth gauge group, and represents gauge loop corrections to the fermion legs
13 SUSY QCD RG For SUSY QCD the Yukawa coupling of quark i with color index m, gluino a, and antisquark j with color index n is given by Y jn im,a = 2g(T a ) n mδ j i. Q φ λ Q = Y (Q) 2 λ Q φ λ = Y ( λ) 2 φ Q λ φ = Tr Y Y Figure 6: Feynman diagrams and associated bird-track diagrams. Y 2 (Q) = 2g 2 C 2 ( ), Y 2 (λ) = 2g 2 2F T ( )
14 SUSY QCD RG no scalar corrections corresponding to Y k Y j Y k. As for the fermion loop correction it always has a quark (antisquark) and gluino for the internal lines so we have Y k Tr Y k Y j = Y kq kq im,a (Yfp,b ) Y jn fp,b = 2g2 C 2 ( )(T a ) n mδ j i, gauge loop corrections are {C m 2 (F ), Y j } = (C 2 ( ) + C 2 (Ad))Y j. all the terms in β j Y proportional to C 2( ) cancel: (4π) 2 β j Y = 2g 3 (C 2 ( ) + F + 2C 2 ( ) 3C 2 ( ) 3N) = 2g 3 (3N F ) = 2(4π) 2 β g so the relation between the Yukawa and gauge couplings is preserved under RG running
15 SUSY QCD Quartic RG SUSY also requires the D-term quartic coupling λ = g 2. The auxiliary D a field is given by and the D-term potential is D a = g(φ in (T a ) m n φ mi φ in (T a ) m n φ mi) V = 1 2 Da D a The β function for a quartic scalar coupling at one-loop is (4π) 2 β λ = Λ (2) 4H + 3A + Λ Y 3Λ S, Λ (2) corresponds to the 1PI contribution from the quartic interactions H corresponds to the fermion box graphs A to the two gauge boson exchange graphs Λ Y to the Yukawa leg corrections Λ S corresponds to the gauge leg corrections
16 SUSY QCD Quartic RG (a) (b) (c) (d) (e) + Figure 7:
17 SUSY QCD Quartic RG = 1 4 4Ν 1 4Ν Ν 2 2 Ν 2 = + 2Ν 2 Ν 1 4Ν 2 Figure 8: The bird-track diagram for the sum over four generators quickly reduces to the sum over two generators and a product of identity matrices.
18 SUSY QCD Quartic RG (φ in (T a ) m n φ mi φ in (T a ) m n φ mi)(φ jq (T a ) p qφ pj φ jq (T a ) p qφ pj), (with flavor indices i j, the case i = j is left as an exercise) we have Λ (2) = ( ) 2F + N 6 N (T a ) m n (T a ) p q + ( ) 1 1 N δ m 2 n δq p, 4H = 8 ( ) N 2 N (T a ) m n (T a ) p q 4 ( ) 1 1 N δ m 2 n δq p, 3A = 3 ( ) N 4 N (T a ) m n (T a ) p q + 3 ( ) 1 1 N δ m 2 n δq p, Λ Y = 4 ( ) N 1 N (T a ) m n (T a ) p q, 3Λ S = 6 ( ) N 1 N (T a ) m n (T a ) p q. individual diagrams that renormalize the gauge invariant, SUSY breaking, operator (φ mi φ mi )(φ pj φ pj ) but the full β function for this operator vanishes and the D-term β function satisfies β λ = β g 2T a T a, β g 2 = 2gβ g. So SUSY is not anomalous at one-loop, and the β functions preserve the relations between couplings at all scales.
19 SUSY RG Figure 9: The couplings remain equal as we run below the SUSY threshold M, but split apart below the non-susy threshold m. If we had added dimension 4 SUSY breaking terms to the theory then the couplings would have run differently at all scales
20 one-loop squark mass Figure 1: The squark loop correction to the squark mass. Σ squark () = ig 2 (T a ) l n(t a ) m l = ig2 16π 2 C 2 ( )δ m n Λ 2 d 4 k (2π) 4 dk 2. i k 2
21 one-loop squark mass Figure 11: The quark gluino loop correction to the squark mass. Σ quark gluino () = ( i 2g) 2 (T a ) l n(t a ) m l ( 1) d 4 k = 2g 2 C 2 ( )δn m d 4 k = 4ig2 16π 2 C 2 ( )δ m n 2k 2 (2π) 4 k 4 Λ 2 dk 2. (2π) Tr ik σ 4 k 2 ik σ k 2
22 one-loop squark mass (a) (b) Figure 12: (a) The squark gluon loop and (b) the gluon loop. Σ quark gluino () = (ig) 2 (T a ) l n(t a ) m l = ξig2 16π 2 C 2 ( )δ m n Λ 2 d 4 k (2π) 4 dk 2, i k k µ ( i) (g µν+(ξ 1) 2 k 2 kµkν k 2 ) k ν Σ gluon () = 1 2 ig2 { (T a ) l n, (T b ) m l = (3+ξ)ig2 16π 2 C 2 ( )δ m n } δ ab g µν d 4 k Λ 2 dk 2. (2π) 4 i k ( i) (g µν+(ξ 1) 2 k 2 kµkν k 2 )
23 one-loop squark mass Adding all the terms together we have Σ() = ( ξ (3 + ξ)) ig2 16π 2 C 2 ( )δ m n Λ 2 dk 2 =. The quadratic divergence in the squark mass cancels! In fact for a massless squark all the mass corrections cancel. This means that in a SUSY theory with a Higgs the Higgs mass is protected from quadratic divergences from gauge interactions as well as from Yukawa interactions
24 Flat directions F < N and the scalar potential is: D a = g(φ in (T a ) m n φ mi φ in (T a ) m n φ mi) V = 1 2 Da D a maximal rank F. In a SUSY vacua: define d n m φ in φ mi d n m = φ in φ mi D a = T am n (d n m d n m) = Since T a is a complete basis for traceless matrices, we must therefore have that the difference of the two matrices is proportional to the identity matrix: d n m d n m = αi
25 Flat directions F < N d n m can be diagonalized by an SU(N) gauge transformation U d U In this diagonal basis there will be at least N F zero eigenvalues d = v 2 1 v v 2 F... where v 2 i. In this basis dn m must also be diagonal, and it must also have N F zero eigenvalues. This tells us that α =, and hence that d n m = d n m
26 Flat directions F < N d n m and d n m are invariant under SU(F ) SU(F ) transformations since φ mi φ mi Vj i, d n m V j i φ in φ mi V i φ jn φ mj = d n m. j, Thus, up to a flavor transformation, we can write v 1... φ = φ = v F D-term potential has flat directions, as we change the VEVs, we move between different vacua with different particle spectra, generically SU(N F ) gauge symmetry.
27 Flat directions F N d n m and d n m are N N positive semi-definite Hermitian matrices of maximal rank N in a SUSY vacuum : d n m d n m = ρi. d n m can be diagonalized by an SU(N) gauge transformation: v 1 2 v 2 2 d =... vn 2 In this basis, d n m must also be diagonal, with eigenvalues v i 2, so v i 2 = v i 2 + ρ.
28 Flat directions F N Since d n m and d n m are invariant under flavor transformations, we can use SU(F ) SU(F ) transformations to put φ and φ in the form v 1... v 1... Φ =....., Φ = v N.... v N Again we have a space of degenerate vacua. At a generic point in the moduli space the SU(N) gauge symmetry is completely broken.
29 The super Higgs mechanism a massless vector supermultiplet eats a chiral supermultiplet to form a massive vector supermultiplet Fayet
30 The super Higgs mechanism Consider the case when v 1 = v 1 = v and v i = v i =, for i > 1 SU(N) SU(N 1) and SU(F ) SU(F ) SU(F 1) SU(F 1). The number of broken gauge generators is N 2 1 ((N 1) 2 1) = 2(N 1) + 1, decompose the adjoint of SU(N) under SU(N 1), we have Ad N = Ad N 1 convenient basis of gauge generators is G A = X, X α 1, X α 2, T a where A = 1,..., N 2 1, α = 1,..., N 1, and a = 1,..., (N 1) 2 1. Xs are the broken generators (span the coset of SU(N)/SU(N 1)), T s are the unbroken SU(N 1) generators
31 The super Higgs mechanism The Xs are analogs of the Pauli matrices: X = 1 2(N 2 N) N , X α 1 = , X α 2 = i.... i.
32 The super Higgs mechanism We can also define raising and lowering operators: X ±α = 1 2 (X α 1 ix α 2 ) so that X +α = , X α =
33 The super Higgs mechanism We can then write the sum of the product of two generators as: G A G A = X X + X +α X α + X α X +α + T a T a Expanding the squark field around its VEV φ φ φ + φ, we have A GA φ = X φ + α X α φ, φ A GA = φ X + φ α X+α, since T a annihilates φ. label the components of the gluino field as G A λ A = X Λ + X +α Λ +α + X α Λ α + T a λ a,
34 The super Higgs mechanism write the quark field as ( ω ψ Q = i ω α Q mi ), Q = ( ω ω α ψ i Q im ), where i is a flavor index, α and m are color indices, Q is a matrix with N 1 rows and F 1 columns, and Q is a matrix with F 1 rows and N 1 columns. fermion mass terms generated by the Yukawa interactions: L F mass = 2g [( φ ( X Λ + φ X +α Λ +α) Q ) ] Q X Λ φ + X α Λ α φ + h.c. ( = gv ω Λ ω Λ ) + ω α Λ +α ω α Λ α + h.c.]. [ N 1 N So we have a Dirac fermion (Λ, (1/ 2)(ω ω )) with mass gv 2(N 1)/N, two sets of N 1 Dirac fermions (Λ +α, ω α ), (Λ α, ω α )) with mass gv, and massless Weyl fermions Q, Q, ψ, ψ, and (1/ 2)(ω + ω )).
35 The super Higgs mechanism decompose the squark field as φ = ( ) h σi, φ = H α φ mi ( h σ i H α φ im ), where φ is a matrix with N 1 rows and F 1 columns. Shifting the scalar field by its VEV so that φ φ + φ we have that the auxiliary D A field is given by D A g = φ G A φ φ G A φ + φ G A φ φ G A φ +φ G A φ φg A φ + φ G A φ φg A φ.
36 The super Higgs mechanism picking out the mass terms in the scalar potential V = 1 2 DA D A : V mass = g2 2 = g2 v 2 2 [ ( ) φ X φ + φ X φ φ X φ φx φ 2 ] +2( φ X +α φ φ X +α φ )(φ X α φ φx α φ ) [ ( h + h (h + h) ] +(H α H α )(H α H α ). (N 1) 2 2(N 2 N) diagonalize the mass matrix: H +α = 1 2 (H α H α ), π +α = 1 2 (H α + H α ), H α = 1 2 (H α H α ), π α = 1 2 (H α + H α ), h = Re(h h), π = Im(h h), Ω = 1 2 (h + h). ) 2
37 The super Higgs mechanism mass terms reduce to V mass = g 2 v 2 [ N 1 N (h ) 2 + H +α H α]. real scalar h with mass gv 2(N 1)/N, a complex scalar H +α (and its conjugate H α ) with mass gv, massless complex scalars σ i, σ i, and Ω. πs become the longitudinal components of the massive gauge bosons, can be removed by going to Unitary gauge
38 The super Higgs mechanism We can write the gauge fields as: G B A B µ = X W µ + X +α W +α µ + X α W α µ + T a A a µ. Then the A 2 φ 2 terms which lead to gauge boson masses are L A 2 φ 2 = g2 A A µ A B ν g µν φ G A G B φ = g 2 g µν φ (X WµX Wν + X +α W µ +α X α Wν α = g 2 v 2 g ( µν N 1 2N W µw ν W ) µ +α Wν α. + X α W α µ X +α W identical term arising from L A2 φ 2 gauge boson Wµ with mass gv 2(N 1)/N, gauge bosons W µ +α and Wµ α with mass gv, the massless gauge bosons A a µ of the unbroken SU(N 1) gauge group. all the particles fall into supermultiplets
39 The super Higgs mechanism v= SU(N) SU(F ) SU(F ) b.d.o.f. Q 1 2NF Q 1 2NF for v we have massive states (in Unitary gauge): SU(N 1) SU(F 1) SU(F 1) b.d.o.f. W W (N 1) W 1 1 4(N 1) massive vector supermultiplet (Wµ, h, Λ, (1/ 2)(ω ω )) 2(N 1) m W = gv N, massive vector supermultiplets (W +α µ, H +α, Λ +α, ω α ) and (W α µ, H α, Λ α, ω α m W ± = gv.
40 The super Higgs mechanism for v also have the massless states: SU(N 1) SU(F 1) SU(F 1) b.d.o.f. Q 1 2(N 1)(F 1) Q 1 2(N 1)(F 1) ψ 1 1 2(F 1) ψ 1 1 2(F 1) S quark chiral supermultiplet Q = (φ, Q ) gauge singlets ψ = (σ, ψ) and S = (1/ 2)(h + h), (1/ 2)(ω + ω ) In both cases (v = and v ) a total of 2(N 2 1) + 4F N b.d.o.f. (and, of course, the same number of fermionic degrees of freedom).
Lecture 5 The Renormalization Group
Lecture 5 The Renormalization Group Outline The canonical theory: SUSY QCD. Assignment of R-symmetry charges. Group theory factors: bird track diagrams. Review: the renormalization group. Explicit Feynman
More informationLecture 6 The Super-Higgs Mechanism
Lecture 6 The Super-Higgs Mechanism Introduction: moduli space. Outline Explicit computation of moduli space for SUSY QCD with F < N and F N. The Higgs mechanism. The super-higgs mechanism. Reading: Terning
More informationThe Affleck Dine Seiberg superpotential
The Affleck Dine Seiberg superpotential SUSY QCD Symmetry SUN) with F flavors where F < N SUN) SUF ) SUF ) U1) U1) R Φ, Q 1 1 F N F Φ, Q 1-1 F N F Recall that the auxiliary D a fields: D a = gφ jn T a
More informationLecture 7: N = 2 supersymmetric gauge theory
Lecture 7: N = 2 supersymmetric gauge theory José D. Edelstein University of Santiago de Compostela SUPERSYMMETRY Santiago de Compostela, November 22, 2012 José D. Edelstein (USC) Lecture 7: N = 2 supersymmetric
More informationLecture 7 SUSY breaking
Lecture 7 SUSY breaking Outline Spontaneous SUSY breaking in the WZ-model. The goldstino. Goldstino couplings. The goldstino theorem. Reading: Terning 5.1, 5.3-5.4. Spontaneous SUSY Breaking Reminder:
More informationSeiberg Duality: SUSY QCD
Seiberg Duality: SUSY QCD Outline: SYM for F N In this lecture we begin the study of SUSY SU(N) Yang-Mills theory with F N flavors. This setting is very rich! Higlights of the next few lectures: The IR
More informationIntroduction to Supersymmetry
Introduction to Supersymmetry Unreasonable effectiveness of the SM L Yukawa = y t H 0 t L t R + h.c. H 0 = H 0 + h 0 = v + h 0 m t = y t v t, L t R h 0 h 0 Figure 1: The top loop contribution to the Higgs
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 informationAnomaly and gaugino mediation
Anomaly and gaugino mediation Supergravity mediation X is in the hidden sector, P l suppressed couplings SUSY breaking VEV W = ( W hid (X) + W vis ) (ψ) f = δj i ci j X X ψ j e V ψ 2 i +... Pl τ = θ Y
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 informationLecture 12 Holomorphy: Gauge Theory
Lecture 12 Holomorphy: Gauge Theory Outline SUSY Yang-Mills theory as a chiral theory: the holomorphic coupling and the holomorphic scale. Nonrenormalization theorem for SUSY YM: the gauge coupling runs
More informationNTNU Trondheim, Institutt for fysikk
NTNU Trondheim, Institutt for fysikk Examination for FY3464 Quantum Field Theory I Contact: Michael Kachelrieß, tel. 99890701 Allowed tools: mathematical tables Some formulas can be found on p.2. 1. Concepts.
More informationSolutions to gauge hierarchy problem. SS 10, Uli Haisch
Solutions to gauge hierarchy problem SS 10, Uli Haisch 1 Quantum instability of Higgs mass So far we considered only at RGE of Higgs quartic coupling (dimensionless parameter). Higgs mass has a totally
More informationFunctional determinants
Functional determinants based on S-53 We are going to discuss situations where a functional determinant depends on some other field and so it cannot be absorbed into the overall normalization of the path
More informationWeek 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books
Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books Burgess-Moore, Chapter Weiberg, Chapter 5 Donoghue, Golowich, Holstein Chapter 1, 1 Free field Lagrangians
More informationTheory of Elementary Particles homework VIII (June 04)
Theory of Elementary Particles homework VIII June 4) At the head of your report, please write your name, student ID number and a list of problems that you worked on in a report like II-1, II-3, IV- ).
More information8.821 F2008 Lecture 5: SUSY Self-Defense
8.8 F008 Lecture 5: SUSY Self-Defense Lecturer: McGreevy Scribe: Iqbal September, 008 Today s lecture will teach you enough supersymmetry to defend yourself against a hostile supersymmetric field theory,
More information+ µ 2 ) H (m 2 H 2
I. THE HIGGS POTENTIAL AND THE LIGHT HIGGS BOSON In the previous chapter, it was demonstrated that a negative mass squared in the Higgs potential is generated radiatively for a large range of boundary
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 informationReφ = 1 2. h ff λ. = λ f
I. THE FINE-TUNING PROBLEM A. Quadratic divergence We illustrate the problem of the quadratic divergence in the Higgs sector of the SM through an explicit calculation. The example studied is that of the
More informationLectures on Supersymmetry I
I Carlos E.M. Wagner HEP Division, Argonne National Laboratory Enrico Fermi Institute, University of Chicago Ecole de Physique de Les Houches, France, August 5, 005. PASI 006, Puerto Vallarta, Mexico,
More informationm f f unchanged under the field redefinition (1), the complex mass matrix m should transform into
PHY 396 T: SUSY Solutions or problem set #8. Problem (a): To keep the net quark mass term L QCD L mass = ψ α c m ψ c α + hermitian conjugate (S.) unchanged under the ield redeinition (), the complex mass
More informationSymmetry Groups conservation law quantum numbers Gauge symmetries local bosons mediate the interaction Group Abelian Product of Groups simple
Symmetry Groups Symmetry plays an essential role in particle theory. If a theory is invariant under transformations by a symmetry group one obtains a conservation law and quantum numbers. For example,
More informationA New Regulariation of N = 4 Super Yang-Mills Theory
A New Regulariation of N = 4 Super Yang-Mills Theory Humboldt Universität zu Berlin Institut für Physik 10.07.2009 F. Alday, J. Henn, J. Plefka and T. Schuster, arxiv:0908.0684 Outline 1 Motivation Why
More informationQuantum Field Theory. and the Standard Model. !H Cambridge UNIVERSITY PRESS MATTHEW D. SCHWARTZ. Harvard University
Quantum Field Theory and the Standard Model MATTHEW D. Harvard University SCHWARTZ!H Cambridge UNIVERSITY PRESS t Contents v Preface page xv Part I Field theory 1 1 Microscopic theory of radiation 3 1.1
More informationNTNU Trondheim, Institutt for fysikk
FY3464 Quantum Field Theory II Final exam 0..0 NTNU Trondheim, Institutt for fysikk Examination for FY3464 Quantum Field Theory II Contact: Kåre Olaussen, tel. 735 9365/4543770 Allowed tools: mathematical
More informationIntroduction to Instantons. T. Daniel Brennan. Quantum Mechanics. Quantum Field Theory. Effects of Instanton- Matter Interactions.
February 18, 2015 1 2 3 Instantons in Path Integral Formulation of mechanics is based around the propagator: x f e iht / x i In path integral formulation of quantum mechanics we relate the propagator to
More informationParticle Physics I Lecture Exam Question Sheet
Particle Physics I Lecture Exam Question Sheet Five out of these 16 questions will be given to you at the beginning of the exam. (1) (a) Which are the different fundamental interactions that exist in Nature?
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 informationVector Mesons and an Interpretation of Seiberg Duality
Vector Mesons and an Interpretation of Seiberg Duality p. 1/?? Vector Mesons and an Interpretation of Seiberg Duality Zohar Komargodski Institute for Advanced Study, Princeton 1010.4105 Vector Mesons and
More informationSupersymmetry Breaking
Supersymmetry Breaking LHC Search of SUSY: Part II Kai Wang Phenomenology Institute Department of Physics University of Wisconsin Madison Collider Phemonology Gauge Hierarchy and Low Energy SUSY Gauge
More informationN=1 Global Supersymmetry in D=4
Susy algebra equivalently at quantum level Susy algebra In Weyl basis In this form it is obvious the U(1) R symmetry Susy algebra We choose a Majorana representation for which all spinors are real. In
More informationQuantum Field Theory III
Quantum Field Theory III Prof. Erick Weinberg April 5, 011 1 Lecture 6 Let s write down the superfield (without worrying about factors of i or Φ = A(y + θψ(y + θθf (y = A(x + θσ θ A + θθ θ θ A + θψ + θθ(
More informationChern-Simons Theory and Its Applications. The 10 th Summer Institute for Theoretical Physics Ki-Myeong Lee
Chern-Simons Theory and Its Applications The 10 th Summer Institute for Theoretical Physics Ki-Myeong Lee Maxwell Theory Maxwell Theory: Gauge Transformation and Invariance Gauss Law Charge Degrees of
More informationSM, EWSB & Higgs. MITP Summer School 2017 Joint Challenges for Cosmology and Colliders. Homework & Exercises
SM, EWSB & Higgs MITP Summer School 017 Joint Challenges for Cosmology and Colliders Homework & Exercises Ch!"ophe Grojean Ch!"ophe Grojean DESY (Hamburg) Humboldt University (Berlin) ( christophe.grojean@desy.de
More information6.1 Quadratic Casimir Invariants
7 Version of May 6, 5 CHAPTER 6. QUANTUM CHROMODYNAMICS Mesons, then are described by a wavefunction and baryons by Φ = q a q a, (6.3) Ψ = ǫ abc q a q b q c. (6.4) This resolves the old paradox that ground
More informationChiral Symmetry Breaking from Monopoles and Duality
Chiral Symmetry Breaking from Monopoles and Duality Thomas Schaefer, North Carolina State University with A. Cherman and M. Unsal, PRL 117 (2016) 081601 Motivation Confinement and chiral symmetry breaking
More informationSupersymmetric Gauge Theories in 3d
Supersymmetric Gauge Theories in 3d Nathan Seiberg IAS Intriligator and NS, arxiv:1305.1633 Aharony, Razamat, NS, and Willett, arxiv:1305.3924 3d SUSY Gauge Theories New lessons about dynamics of quantum
More informationNon-Supersymmetric Seiberg duality Beyond the Planar Limit
Non-Supersymmetric Seiberg duality Beyond the Planar Limit Input from non-critical string theory, IAP Large N@Swansea, July 2009 A. Armoni, D.I., G. Moraitis and V. Niarchos, arxiv:0801.0762 Introduction
More informationGauge-Higgs Unification on Flat Space Revised
Outline Gauge-Higgs Unification on Flat Space Revised Giuliano Panico ISAS-SISSA Trieste, Italy The 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions Irvine,
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 informationDynamical supersymmetry breaking, with Flavor
Dynamical supersymmetry breaking, with Flavor Cornell University, November 2009 Based on arxiv: 0911.2467 [Craig, Essig, Franco, Kachru, GT] and arxiv: 0812.3213 [Essig, Fortin, Sinha, GT, Strassler] Flavor
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 informationVacuum Energy and Effective Potentials
Vacuum Energy and Effective Potentials Quantum field theories have badly divergent vacuum energies. In perturbation theory, the leading term is the net zero-point energy E zeropoint = particle species
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 informationSpontaneous breaking of supersymmetry
Spontaneous breaking of supersymmetry Hiroshi Suzuki Theoretical Physics Laboratory Nov. 18, 2009 @ Theoretical science colloquium in RIKEN Hiroshi Suzuki (TPL) Spontaneous breaking of supersymmetry Nov.
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 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 informationMinimal Supersymmetric Standard Model (MSSM). Nausheen R. Shah
Minimal Supersymmetric Standard Model (MSSM). Nausheen R. Shah June 8, 2003 1 Introduction Even though the Standard Model has had years of experimental success, it has been known for a long time that it
More informationRoni Harnik LBL and UC Berkeley
Roni Harnik LBL and UC Berkeley with Daniel Larson and Hitoshi Murayama, hep-ph/0309224 Supersymmetry and Dense QCD? What can we compare b/w QCD and SQCD? Scalars with a chemical potential. Exact Results.
More informationEDMs from the QCD θ term
ACFI EDM School November 2016 EDMs from the QCD θ term Vincenzo Cirigliano Los Alamos National Laboratory 1 Lecture II outline The QCD θ term Toolbox: chiral symmetries and their breaking Estimate of the
More informationSymmetries, Groups Theory and Lie Algebras in Physics
Symmetries, Groups Theory and Lie Algebras in Physics M.M. Sheikh-Jabbari Symmetries have been the cornerstone of modern physics in the last century. Symmetries are used to classify solutions to physical
More informationTextbook Problem 4.2: We begin by developing Feynman rules for the theory at hand. The Hamiltonian clearly decomposes into Ĥ = Ĥ0 + ˆV where
PHY 396 K. Solutions for problem set #11. Textbook Problem 4.2: We begin by developing Feynman rules for the theory at hand. The Hamiltonian clearly decomposes into Ĥ = Ĥ0 + ˆV where Ĥ 0 = Ĥfree Φ + Ĥfree
More informationNon Abelian Higgs Mechanism
Non Abelian Higgs Mechanism When a local rather than global symmetry is spontaneously broken, we do not get a massless Goldstone boson. Instead, the gauge field of the broken symmetry becomes massive,
More information1 Susy in 4d- Notes by Horatiu Nastase A very basic introduction (survival guide)
1 Susy in 4d- Notes by Horatiu Nastase A very basic introduction (survival guide) 1.1 Algebras 2-component notation for 4d spinors ( ) ψα ψ = χ α (1) C matrix ( ɛαβ 0 C AB = 0 ɛ α β ) ; ɛ αβ = ɛ α β =
More informationTHE STANDARD MODEL. II. Lagrangians 7 A. Scalars 9 B. Fermions 10 C. Fermions and scalars 10
THE STANDARD MODEL Contents I. Introduction to the Standard Model 2 A. Interactions and particles 2 B. Problems of the Standard Model 4 C. The Scale of New Physics 5 II. Lagrangians 7 A. Scalars 9 B. Fermions
More informationGAUGE THEORY AMPLITUDES, SCALAR GRAPHS AND TWISTOR SPACE
GAUGE THEORY AMPLITUES, SCALAR GRAPHS AN TWISTOR SPACE VALENTIN V. KHOZE epartment of Physics and IPPP University of urham urham, H1 3LE United Kingdom We discuss a remarkable new approach initiated by
More informationSUSY Breaking in Gauge Theories
SUSY Breaking in Gauge Theories Joshua Berger With the Witten index constraint on SUSY breaking having been introduced in last week s Journal club, we proceed to explicitly determine the constraints on
More informationDonoghue, Golowich, Holstein Chapter 4, 6
1 Week 7: Non linear sigma models and pion lagrangians Reading material from the books Burgess-Moore, Chapter 9.3 Donoghue, Golowich, Holstein Chapter 4, 6 Weinberg, Chap. 19 1 Goldstone boson lagrangians
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 informationQED and the Standard Model Autumn 2014
QED and the Standard Model Autumn 2014 Joel Goldstein University of Bristol Joel.Goldstein@bristol.ac.uk These lectures are designed to give an introduction to the gauge theories of the standard model
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 informationPhysics at e + e - Linear Colliders. 4. Supersymmetric particles. M. E. Peskin March, 2002
Physics at e + e - Linear Colliders 4. Supersymmetric particles M. E. Peskin March, 2002 In this final lecture, I would like to discuss supersymmetry at the LC. Supersymmetry is not a part of the Standard
More informationTwo Examples of Seiberg Duality in Gauge Theories With Less Than Four Supercharges. Adi Armoni Swansea University
Two Examples of Seiberg Duality in Gauge Theories With Less Than Four Supercharges Adi Armoni Swansea University Queen Mary, April 2009 1 Introduction Seiberg duality (Seiberg 1994) is a highly non-trivial
More informationGoldstone Bosons and Chiral Symmetry Breaking in QCD
Goldstone Bosons and Chiral Symmetry Breaking in QCD Michael Dine Department of Physics University of California, Santa Cruz May 2011 Before reading this handout, carefully read Peskin and Schroeder s
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 informationSupersymmetry, Dark Matter, and Neutrinos
Supersymmetry, Dark Matter, and Neutrinos The Standard Model and Supersymmetry Dark Matter Neutrino Physics and Astrophysics The Physics of Supersymmetry Gauge Theories Gauge symmetry requires existence
More informationDefining Chiral Gauge Theories Beyond Perturbation Theory
Defining Chiral Gauge Theories Beyond Perturbation Theory Lattice Regulating Chiral Gauge Theories Dorota M Grabowska UC Berkeley Work done with David B. Kaplan: Phys. Rev. Lett. 116 (2016), no. 21 211602
More informationt Hooft Anomaly Matching for QCD
UCB-PTH-97-3 LBNL-41477 t Hooft Anomaly Matching for QCD John Terning Department of Physics, University of California, Berkeley, CA 9470 and Theory Group, Lawrence Berkeley National Laboratory, Berkeley,
More informationMasses and the Higgs Mechanism
Chapter 8 Masses and the Higgs Mechanism The Z, like the W ± must be very heavy. This much can be inferred immediately because a massless Z boson would give rise to a peculiar parity-violating long-range
More informationIntroduction to Supersymmetry
Introduction to Supersymmetry I. Antoniadis Albert Einstein Center - ITP Lecture 5 Grand Unification I. Antoniadis (Supersymmetry) 1 / 22 Grand Unification Standard Model: remnant of a larger gauge symmetry
More informationThe rudiments of Supersymmetry 1/ 53. Supersymmetry I. A. B. Lahanas. University of Athens Nuclear and Particle Physics Section Athens - Greece
The rudiments of Supersymmetry 1/ 53 Supersymmetry I A. B. Lahanas University of Athens Nuclear and Particle Physics Section Athens - Greece The rudiments of Supersymmetry 2/ 53 Outline 1 Introduction
More information2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC)
2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC) hep-th/0606045 Success of 2T-physics for particles on worldlines. Field theory version of 2T-physics. Standard Model in 4+2 dimensions.
More informationUniversal Extra Dimensions
Universal Extra Dimensions Add compact dimension(s) of radius R ~ ant crawling on tube Kaluza-Klein tower of partners to SM particles due to curled-up extra dimensions of radius R n = quantum number for
More informationAn Introduction to Dynamical Supersymmetry Breaking
An Introduction to Dynamical Supersymmetry Breaking Thomas Walshe September 28, 2009 Submitted in partial fulfillment of the requirements for the degree of Master of Science of Imperial College London
More informationSpectral action, scale anomaly. and the Higgs-Dilaton potential
Spectral action, scale anomaly and the Higgs-Dilaton potential Fedele Lizzi Università di Napoli Federico II Work in collaboration with A.A. Andrianov (St. Petersburg) and M.A. Kurkov (Napoli) JHEP 1005:057,2010
More informationAn extended standard model and its Higgs geometry from the matrix model
An extended standard model and its Higgs geometry from the matrix model Jochen Zahn Universität Wien based on arxiv:1401.2020 joint work with Harold Steinacker Bayrischzell, May 2014 Motivation The IKKT
More informationSupersymmetric Gauge Theories, Matrix Models and Geometric Transitions
Supersymmetric Gauge Theories, Matrix Models and Geometric Transitions Frank FERRARI Université Libre de Bruxelles and International Solvay Institutes XVth Oporto meeting on Geometry, Topology and Physics:
More informationS-CONFINING DUALITIES
DIMENSIONAL REDUCTION of S-CONFINING DUALITIES Cornell University work in progress, in collaboration with C. Csaki, Y. Shirman, F. Tanedo and J. Terning. 1 46 3D Yang-Mills A. M. Polyakov, Quark Confinement
More informationKaluza-Klein Masses and Couplings: Radiative Corrections to Tree-Level Relations
Kaluza-Klein Masses and Couplings: Radiative Corrections to Tree-Level Relations Sky Bauman Work in collaboration with Keith Dienes Phys. Rev. D 77, 125005 (2008) [arxiv:0712.3532 [hep-th]] Phys. Rev.
More informationQuantum Field Theory 2 nd Edition
Quantum Field Theory 2 nd Edition FRANZ MANDL and GRAHAM SHAW School of Physics & Astromony, The University of Manchester, Manchester, UK WILEY A John Wiley and Sons, Ltd., Publication Contents Preface
More informationThe Higgs Mechanism and the Higgs Particle
The Higgs Mechanism and the Higgs Particle Heavy-Ion Seminar... or the Anderson-Higgs-Brout-Englert-Guralnik-Hagen-Kibble Mechanism Philip W. Anderson Peter W. Higgs Tom W. B. Gerald Carl R. François Robert
More informationTHE STANDARD MODEL AND THE GENERALIZED COVARIANT DERIVATIVE
THE STANDAD MODEL AND THE GENEALIZED COVAIANT DEIVATIVE arxiv:hep-ph/9907480v Jul 999 M. Chaves and H. Morales Escuela de Física, Universidad de Costa ica San José, Costa ica E-mails: mchaves@cariari.ucr.ac.cr,
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 informationModels of Neutrino Masses
Models of Neutrino Masses Fernando Romero López 13.05.2016 1 Introduction and Motivation 3 2 Dirac and Majorana Spinors 4 3 SU(2) L U(1) Y Extensions 11 4 Neutrino masses in R-Parity Violating Supersymmetry
More informationAspects of N = 2 Supersymmetric Gauge Theories in Three Dimensions
hep-th/9703110, RU-97-10, IASSNS-HEP-97/18 Aspects of N = 2 Supersymmetric Gauge Theories in Three Dimensions O. Aharony 1, A. Hanany 2, K. Intriligator 2, N. Seiberg 1, and M.J. Strassler 2,3 1 Dept.
More informationHiggs Boson Phenomenology Lecture I
iggs Boson Phenomenology Lecture I Laura Reina TASI 2011, CU-Boulder, June 2011 Outline of Lecture I Understanding the Electroweak Symmetry Breaking as a first step towards a more fundamental theory of
More informationJuly 2, SISSA Entrance Examination. PhD in Theoretical Particle Physics Academic Year 2018/2019. olve two among the three problems presented.
July, 018 SISSA Entrance Examination PhD in Theoretical Particle Physics Academic Year 018/019 S olve two among the three problems presented. Problem I Consider a theory described by the Lagrangian density
More informationAxial symmetry in the chiral symmetric phase
Axial symmetry in the chiral symmetric phase Swagato Mukherjee June 2014, Stoney Brook, USA Axial symmetry in QCD massless QCD Lagrangian is invariant under U A (1) : ψ (x) e i α ( x) γ 5 ψ(x) μ J 5 μ
More informationKonishi Anomaly. 32π 2 ǫκλµν F κλ F µν. (5)
Konishi Anomaly Consider the SQED with massless charged fields A and B. Classically, it has an axial symmetry A e +iϕ A, B e +iϕ B and hence a conserved axial current J ax = Ae +2gV A + B e 2gV B, () D
More informationAnomalies and discrete chiral symmetries
Anomalies and discrete chiral symmetries Michael Creutz BNL & U. Mainz Three sources of chiral symmetry breaking in QCD spontaneous breaking ψψ 0 explains lightness of pions implicit breaking of U(1) by
More informationAnomaly. Kenichi KONISHI University of Pisa. College de France, 14 February 2006
Anomaly Kenichi KONISHI University of Pisa College de France, 14 February 2006 Abstract Symmetry and quantization U A (1) anomaly and π 0 decay Origin of anomalies Chiral and nonabelian anomaly Anomally
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 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 informationLecture 24 Seiberg Witten Theory III
Lecture 24 Seiberg Witten Theory III Outline This is the third of three lectures on the exact Seiberg-Witten solution of N = 2 SUSY theory. The third lecture: The Seiberg-Witten Curve: the elliptic curve
More informationAxions Theory SLAC Summer Institute 2007
Axions Theory p. 1/? Axions Theory SLAC Summer Institute 2007 Helen Quinn Stanford Linear Accelerator Center Axions Theory p. 2/? Lectures from an Axion Workshop Strong CP Problem and Axions Roberto Peccei
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 informationFinding the Higgs boson
Finding the Higgs boson Sally Dawson, BN XIII Mexican School of Particles and Fields ecture 1, Oct, 008 Properties of the Higgs boson Higgs production at the Tevatron and HC Discovery vs spectroscopy Collider
More informationGrand Unification. Strong, weak, electromagnetic unified at Q M X M Z Simple group SU(3) SU(2) U(1) Gravity not included
Pati-Salam, 73; Georgi-Glashow, 74 Grand Unification Strong, weak, electromagnetic unified at Q M X M Z Simple group G M X SU(3) SU() U(1) Gravity not included (perhaps not ambitious enough) α(q ) α 3
More informationParticle Physics 2018 Final Exam (Answers with Words Only)
Particle Physics 2018 Final Exam (Answers with Words Only) This was a hard course that likely covered a lot of new and complex ideas. If you are feeling as if you could not possibly recount all of the
More information