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Supersymmetry

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Spurion. Supersymmetry is broken either by an F-component of a chiral superfield. fi=q2Fi ... Spurion operators. Spurion z =fi/M=q2Fi/M generates soft terms ... – PowerPoint PPT presentation

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Title: Supersymmetry


1
Supersymmetry
  • Hitoshi Murayama
  • Taiwan Spring School
  • March 29, 2002

2
Electroweak Symmetry Breaking
  • In the MSSM, electroweak symmetry does not get
    broken
  • Only after supersymmetry is broken, Higgs can
    obtain a VEV vmSUSY
  • Regard EWSB as a consequence of supersymmetry
    breaking
  • EW symmetry and hierarchy protected by
    supersymmetry

3
Origin of Hierarchy
  • vltltMPl because vmSUSYltltMPl
  • Why mSUSYltltMPl?
  • Idea dimensional transmutation
  • SUSY broken by strong gauge dynamics with
  • Dynamical supersymmetry breaking

4
Dynamical Supersymmetry Breaking
  • Simplest example SO(10) with one 16
  • No moduli space, cant analyze with Seibergian
    techniques
  • non-calculable (Affleck-Dine-Seiberg)
  • Add one 10, make it massive and decouple
  • When M100, moduli space spanned by 161610, 102,
    generically SO(10)?SO(7)
  • SO(7) gaugino condensation generates dynamical
    superpotential
  • Add WM10102, lifts moduli space, breaks SUSY
  • Decouple 10 smoothly(HM)

5
Izawa-Yanagida-Intriligator-Thomas model
  • Sp(Nc) gauge theory with NfNc1
  • Quantum modified moduli space
  • Pf M L2Nf for mesons MijQiQj
  • Add superpotential with singlets Sij
  • WSij QiQj forces Mij0
  • Contradiction ? no SUSY vacua

6
Issue of mediation
  • Many gauge theories that break SUSY dynamically
    known
  • The main issue how do we communicate the SUSY
    breaking effects to the MSSM? mediation

7
Spurion
  • Supersymmetry is broken either by an F-component
    of a chiral superfield
  • fiq2Fi?0
  • or a D-component of a vector superfield
  • Vq2D?0
  • Once they are frozen at their expectation values,
    they can be viewed as spurions of supersymmetry
    breaking order parameters

8
Soft supersymmetry breaking
  • Purpose of supersymmetry is to protect hierarchy
  • Arbitrary terms in Lagrangian that break
    supersymmetry reintroduce power divergences
  • Soft supersymmetry breaking classified
  • mll, m2ijfifj, Aijkfjfjfk, Bijfjfj, Cifj
  • Dark horse terms (not always allowed)
  • fjfjfk, lyj, yiyj

9
Spurion operators
  • Spurion z fi/Mq2Fi/M generates soft terms
  • M is the mediation scale where the effects of
    SUSY breaking are communicated
  • m ll ?d2q z c Wa Wa
  • m2ijfifj ?d4q zz cijfifj
  • Aijkfjfjfk ?d2q z cijkfjfjfk
  • Bijfjfj ?d2q z cijfjfj
  • Cifj ?d2q z cifj
  • Coefficients c are random at this point

10
Supersymmetric flavor problem
  • Random SUSY breaking excluded by FCNC constraints
  • Consider scalar down quarks
  • Take the off-diagonal terms to be perturbation

11
Supersymmetric flavor problem
  • Random SUSY breaking excluded by FCNC constraints
  • Want a reason why off-diagonal terms are
    suppressed

_
K0
K0
12
Two possible directions
  • Develop a theory of flavor that predicts not only
    the pattern of Yukawa matrices (masses, mixings),
    but also soft masses
  • Develop a theory of mediation mechanism of
    supersymmetry breaking that predicts
    (approximately) flavor-blind soft masses

13
Gravity Mediation
14
Supergravity
  • Specify Kähler potential K and superpotential W
  • Minimal supergravity
  • Kz2?ifi2 WWh(z)Wo(f)
  • SUSY broken if FzzWWz?0, W?0
  • ?Universal scalar mass, trilinear couplings etc

15
Lore
  • Got universal scalar mass!
  • Of course, because gravity doesnt distinguish
    flavor
  • Wrong!
  • Minimal is a choice to obtain canonical kinetic
    terms with no Planck-suppressed corrections
  • But in general there are such corrections in
    non-renormalizable theory and SUGRA not minimal

16
Problems with Minimal SUGRA
  • There is no fundamental reason to believe that
    Kähler potential in effective theory of quantum
    gravity is strictly minimal
  • In many string compactifications, it isnt
  • Direct coupling of observable fields with moduli
    in Käler potential that depend on their modular
    weights
  • Thought to be an ad hoc convenient choice, not a
    theory of mediation
  • But phenomenologically excellent start point,
    explaning EWSB, dark matter, absence of FCNC

17
Problems with general SUGRA
  • There may be arbitrary coupling between hidden
    and observable fields in Kähler potential under
    no control
  • Generically, soft masses expected to be
    arbitrary, with flavor violation
  • m2ijfifj ?d4q zz cij fifj
  • Phenomenogically disaster

18
Remedy by flavor symmetry
  • We need theory of flavor anyway
  • The issue of flavor-violating soft masses is
    intimately tied to the origin of flavor, Yukawa
    couplings
  • Seek for a common theory that solves the problem

19
Flavor-blind Mediation Mechanisms
  • Gauge Mediation
  • Gaugino Mediation
  • Anomaly Mediation

20
Gauge Mediation
21
Dine-Nelson-Shirman model
  • Dynamical supersymmetry breaking sector
  • Take SU(5) with 105
  • (non-calculable DSB model
  • add massive 55 and can show DSB HM)
  • break it to SU(4)?U(1) with non-anomalous global
    U(1)m
  • (624-31-8)1 (4-114)-3
  • W 4-1 4-3 14 14 14 1-8
  • breaks supersymmetry dynamically
  • gauge global U(1)m as messenger U(1)
  • Problem with FY D-term for messenger U(1) ?
    solved by changing the DSB model to SU(6)?U(1)
  • (Dine, Nelson, Nir, Shirman)

22
Dine-Nelson-Shirman model
  • Messenger sector
  • a pair f? charged under messenger U(1)
  • NF pairs of FF (55) under SU(5)
    ?SU(3)?SU(2)?U(1)
  • Wl1Sff-l2SFFl3S3
  • f? acquire negative mass-squred from two-loops
    in messenger U(1) interaction
  • triggers S to acquire both A- and F-component
    VEVs
  • gives both mass and B-term to FF
  • Ml2ltSgt, MBl2ltFSgt

23
Dine-Nelson-Shirman model
  • Because FF are charged under the standard model
    gauge groups, their one-loop diagrams generate
    gaugino masses, and two-loop diagrams generate
    scalar masses
  • Generated scalar masses flavor-blind, because
    gauge interactions do not distinguish flavor

24
Dine-Nelson-Shirman model
  • Lightest Supersymmetry Particle gravitino
  • In general, a cosmological problem (overclosure)
  • (de Gouvêa, Moroi, HM)
  • Collider signatures may be unique
  • Bino ? gravitino photon
  • Decay length may be microns to km
  • Should not have any new flavor physics below the
    mediation scale to screw-up flavor-blindness of
    soft masses

25
Direct Gauge Mediation
  • Too many sectors to worry about!
  • DSB sector Sp(4) with 5 flavors charged under
    SU(5) (HM)

26
Gaugino Mediation
  • (Kaplan, Kribs, Schmaltz)
  • (Chacko, Luty, Nelson, Ponton)
  • DSB in another brane
  • Gauge multiplet in the bulk
  • Gauge multiplet learns SUSY breaking first,
    obtains gaugino mass
  • MSSM at the compactification scale with gaugino
    mass only
  • Scalar masses generated by RGE

27
Gaugino Mediation
  • Phenomenology similar to minimal supergravity
    with zero universal scalar mass
  • Gravitino heavy less harmful
  • Needs high (GUT scale) compactification to jack
    up slepton mass high enough
  • Should not have any new flavor physics below the
    compactification scale to screw-up
    flavor-blindness of soft masses

28
Anomaly Mediation
  • (Randall, Sundrum)
  • (Giudice, Luty, HM, Rattazzi)
  • Try not to mediate
  • Zen of SUSY breaking
  • If no coupling between DSB and MSSM, there is no
    supersymmetry breaking at tree-level
  • But divergence of supercurrent in the same
    multiplet as the trace of energy momentum tensor
  • Conformal anomaly induces supersymmetry breaking

29
Weyl compensator formalism
  • Conformal Supergravity fixed by Weyl
    compensator F
  • The only communication of SUSY breaking is
    through the auxiliary component of Fq2F
  • ?d4q FF ff ?d2q F3 (M f2l f3)
  • Scale f?f/F
  • ?d4q ff ?d2q (F M f2l f3)
  • Only dimensionful parameters acquire SUSY
    breaking
  • Massless theory ? no SUSY breaking

30
Conformal Anomaly
  • Any (non-finite) theory needs a regulator with an
    explicit mass scale
  • Pauli-Villars with heavy regulator mass
  • DRED with renormalization scale m
  • (Boyda, HM, Pierce)
  • Regulator receives SUSY breaking
  • SUSY breaking induced by regulator effect anomaly

31
Anomaly Mediation
  • Anomaly mediation predicts SUSY breaking with
    theory given at the scale of interest
  • UV insensitivity
  • Can be checked explicitly by integrating out
    heavy fields that their loops exactly cancel the
    differences in b-functions anomalous dimensions
  • (Giudice, Luty, HM, Rattazzi)
  • (Boyda, HM, Pierce)
  • SUSY breakings always stay on the RGE trajectory

32
Too predictive!
  • Anomaly mediation highly predictive with only one
    parameter overall scale
  • Slepton mass-squareds come out negative
  • Phenomenologically dead on start
  • Remedies
  • Add uinversal scalar mass
  • Cause symmetry breaking via SUSY breaking
  • Destroys UV insensitivity

33
Viable UV-insensitiveAnomaly Mediation
  • Add U(1)B-L and U(1)Y D-terms
  • Three SUSY-breaking parameters now
  • Can show that UV-insensitive
  • (Arkani-Hamed, Kaplan, HM, Nomura)

34
Conformal sequestering
  • Inspiration from AdS/CFT correspondence
  • Make hidden sector nearly superconformal
  • Dangerous coupling between hidden and observable
    fields suppressed because Kähler potential of
    hidden fields flow to IR fixed point (Luty,
    Sundrum)
  • Can be extended to include U(1) breaking sector
    to make the scenario phenomenologically viable
    (Harnik, HM, Pierce)

35
U(1) breaking sector
  • SO(5) theory with 6 spinors, no mass parameters
  • Gauge SU(4)?SU(2)?U(1) subgroup of global SU(6)
    symmetry
  • Quantum modified moduli space breaks U(1) (and
    also SU(4)?Sp(2))
  • D-term non-calculable because compositeness
    scale Lv U(1)-breaking scale
  • Can be made calculable within the same
    universality class by (1) additional flavor Lgtgtv
    or (2) additional colorflavor Lltltv to show D?0
  • Can be used to generate right-handed neutrino
    mass
  • (Harnik, HM, Pierce)

36
SUSY spectra
37
Models of Flavor
38
Question of Flavor
  • What distinguishes different generations?
  • Same gauge quantum numbers, yet different
  • Hierarchy with small mixings
  • ? Need some ordered structure
  • Probably a hidden flavor quantum number
  • ? Need flavor symmetry
  • Flavor symmetry must allow top Yukawa
  • Other Yukawas forbidden
  • Small symmetry breaking generates small Yukawas

39
Broken Flavor Symmetry
  • Flavor symmetry broken by a VEV ???0.02
  • SU(5)-like
  • 10(Q, uR, eR) (2, 1, 0)
  • 5(L, dR) (1, 1, 1)
  • mumcmt md2ms2mb2 me2mm2mt2 ?4 ?2 1

40
Not bad!
  • mb mt, ms mm, md me _at_MGUT
  • mumcmt md2ms2mb2 me2mm2mt2

41
New Data from Neutrinos
  • Neutrinos are already providing significant new
    information about flavor symmetries
  • If LMA, all mixing except Ue3 large
  • Two mass splittings not very different
  • Atmospheric mixing maximal
  • Any new symmetry or structure behind it?

42
Is There A StructureIn Neutrino Masses Mixings?
  • Monte Carlo random complex 3?3 matrices with
    seesaw mechanism
  • (Hall, HM, Weiner Haba, HM)

43
Anarchy
  • No particular structure in neutrino mass matrix
  • All three angles large
  • CP violation O(1)
  • Ratio of two mass splittings just right for LMA
  • Three out of four distributions OK
  • Reasonable
  • ? Underlying symmetries dont distinguish 3
    neutrinos.

44
Anarchy is Peaceful
  • Anarchy (Miriam-Webster)
  • A utopian society of individuals who enjoy
    complete freedom without government
  • Peaceful ideology that neutrinos work together
    based on their good will
  • Predicts large mixings, LMA, large CP violation
  • sin22q13 just below the bound
  • Ideal for VLBL experiments
  • Wants globalization!

45
More flavor parameters
  • Squarks, sleptons also come with mass matrices
  • Off-diagonal elements violate flavor suppressed
    by flavor symmetries
  • Look for flavor violation due to SUSY loops
  • Then look for patterns to identify symmetries
  • ? Repeat Gell-MannOkubo!
  • Need to know SUSY masses

46
To Figure It Out
  • Models differ in flavor quantum number
    assignments
  • Need data on sin22q13, solar neutrinos, CP
    violation, B-physics, LFV, EWSB, proton decay
  • Archaeology
  • We will learn insight on origin of flavor by
    studying as many fossils as possible
  • cf. CMBR in cosmology

47
More FossilsLepton Flavor Violation
  • Neutrino oscillation
  • ? lepton family number is not conserved!
  • Any tests using charged leptons?
  • Top quark unified with leptons
  • Slepton masses split in up- or neutrino-basis
  • Causes lepton-flavor violation (Barbieri, Hall)
  • predict B(t?mg), B(m?eg), m?e at interesting (or
    too-large) levels

48
Barbieri, Hall, Strumia
49
More FossilsQuark Flavor Violation
  • Now also large mixing between nt and nm
  • (nt, bR) and (nm , sR) unified in SU(5)
  • Doesnt show up in CKM matrix
  • But can show up among squarks
  • CP violation in Bs mixing (Bs?J/y f)
  • Addtl CP violation in penguin b?s (Bd?f Ks)
  • (Chang, Masiero, HM)

50
Conclusions
  • Dynamical supersymmetry breaking successfully
    produces hierarchy
  • Various mediation mechanisms
  • Gravity mediation flavor symmetry
  • Gauge mediation
  • Anomaly mediation
  • Gaugino mediation
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