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THEORETICAL PREDICTIONS FOR COLLIDER SEARCHES

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1. THEORETICAL PREDICTIONS. FOR COLLIDER SEARCHES 'Big' and ' ... Degrassi-Heinemeyer-Hollik-Slavich-Weiglein. Mc 103.5 GeV. 9. Giusti-Romanino-Strumia ... – PowerPoint PPT presentation

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Title: THEORETICAL PREDICTIONS FOR COLLIDER SEARCHES


1
THEORETICAL PREDICTIONSFOR COLLIDER SEARCHES
G.F. Giudice CERN
  • Big and little hierarchy problems
  • Supersymmetry
  • Little Higgs
  • Extra dimensions

2
HIERARCHY PROBLEM
no fine-tuning a LSM lt TeV Big hierarchy
between LSM and MPl Cosmological constant a Cut
off of quartic divergences at Llt10-3 eV
3
LITTLE HIERARCHY
10 5.6 9.2 9.7 4.6 7.3
6.1 4.3 4.5 3.2
6.4 9.3 5.0 12.4
4
LSMlt1 TeV, LLHgt5-10 TeV Little hierarchy
between LSM and LLH a
  • New physics at LSM is weakly interacting
  • No (sizable) tree-level contributions from new
    physics at LSM
  • Strongly-interacting physics can only occur at
    scales larger than LLH
  • Successful new physics at LSM has to pass
    non-trivial tests

5
SUPERSYMMETRY
  • can be extended to MPl
  • Link with quantum gravity
  • Successful scenario for GUT

exp
exp
Ghilencea-Ross
6
UNIFICATION WITHOUT DESERT
Dienes-Dudas-Gherghetta
  • Accelerated running from extra dimensions
  • or from gauge group replication
  • Different tree-level expression for sin2qW
  • GUT trace over
    GUT irrep
  • Little running needed

Arkani Hamed-Cohen-Georgi
Dimopoulos-Kaplan
7
SUPERSYMMETRY
  • Gauge-coupling unification
  • Radiative EW breaking
  • Light Higgs
  • Satisfies little hierarchy LLH4pLSM
  • Dark matter
  • Sparticles have not been observed
  • Susy-breaking sector unspecified

?
?
8
Mc gt 103.5 GeV
Degrassi-Heinemeyer-Hollik-Slavich-Weiglein
9
Giusti-Romanino-Strumia
10
Supersymmetry-breaking sector unspecified
  • Susy flavour violations ? gauge, gaugino
    mediation
  • Connection with gravity _ supergravity, anomaly
    mediation
  • problem _ supergravity
  • Predictivity _ gauge,
    gaugino, anomaly med.

Scenarios with different spectra and different
experimental signals
11
NEW INGREDIENTS FROM EXTRA DIMENSIONS
y
Scherk-Schwarz breaking
R
Supersymmetry is broken
Non-local susy breaking _ involves global
structure At short distances (ltR), susy-breaking
effects are suppressed
12
NEW INGREDIENTS FROM EXTRA DIMENSIONS
Orbifold projection
Z2 y g-y cos(ny/R)
sin(ny/R)
-
n0
n1
Chiral theories
n1
n2
n2
0
0
pR
pR
13
AN INTERESTING EXAMPLE
Barbieri-Hall-Nomura
  • 5D SUSY SM compactified on S1/(Z2Z2)
  • Different susy breaking at each boundary
  • effective theory non-susy
  • (susy recovered at dltR)
  • Higgs boson mass (rather) insensitive to UV
  • mH 127 10 GeV
  • Large corrections to Dr ?
  • UV completion at L 5 TeV ?

Barbieri-Hall-Marandella-Nomura-Okui-Oliver-Papucc
i
14
  • Mass spectrum is non-supersymmetric
  • one Higgs and two sparticles for each SM
    particle
  • LSP stable stop with mass 210 GeV

15
USING WARPED DIMENSIONS
Gherghetta-Pomarol
  • Susy-breaking in Higgs sector is non-local _
    finite effects
  • AdS/CFT _ SM non-susy
  • Higgs sector susy bound states of spontaneously
    broken CFT
  • Light Higgs higgsino
  • New CFT states at L-1 TeV
  • Considerable fine tuning

SM
Susy breaking
Higgs sector
16
SUPERSYMMETRY CONCLUSIONS
  • Susy at EW scale can be realized in very
    different ways
  • ETmiss
  • ETmiss g
  • ETmiss l
  • Stable charged particle
  • Nearly-degenerate
  • Stable stop
  • Partial susy spectrum

17
HIGGS AS PSEUDOGOLDSTONE BOSON
Gauge, Yukawa and self-interaction are large
non-derivative couplings _ Violate global
symmetry and introduce quadratic div.
18
LITTLE HIGGS
Arkani Hamed-Cohen-Georgi
A less ambitious programme Explain only little
hierarchy At LSM new physics cancels one-loop
power divergences
Collective breaking many (approximate) global
symmetries preserve massless Goldstone boson
19
  • It can be achieved with gauge-group replication
  • Goldstone bosons in
  • gauged subgroups, each
    preserving a non-linear global symmetry
  • which breaks all
    symmetries
  • Field replication Ex. SU2 gauge with F1,2
    doublets such that V(F1F1,F2F2) and F1,2
    spontaneously break SU2
  • Turning off gauge coupling to F1 _
  • Local SU2(F2) global SU2(F1) both spont. broken

Kaplan-Schmaltz
20
Realistic models are rather elaborate Effectively
, new particles at the scale f LSM canceling
(same-spin) SM one-loop divergences with
couplings related by symmetry Typical
spectrum Vectorlike charge 2/3 quark
Arkani Hamed-Cohen-Georgi-Katz-Nelson-Gregoire-Wac
ker-Low-Skiba-Smith-Kaplan-Schmaltz-Terning
Gauge bosons EW triplet singlet Scalars
(triplets ?)
21
Bounds from Tevatron limits on new gauge bosons
EW data (Dr from new gauge
and top)
Csaki-Hubisz-Kribs-Meade-Terning
In minimal model
Variations significantly reduce the fine tuning
22
HIGGS AS EXTRA-DIM COMPONENT OF GAUGE FIELD
  • AM (Am,A5), A5 g A5 ?5 L forbids
    m2A52
  • Correct Higgs quantum numbers by projecting out
    unwanted states with orbifold
  • Yukawa couplings
  • Quartic couplings
  • Do not reintroduce quadratic divergences

Csaki-Grojean-Murayama Burdman-Nomura Scrucca-Sero
ne-Silvestrini
23
FLAT Arkani
Hamed-Dimopoulos-Dvali
WARPED Randall-Sundrum
24
Contact interactions (loop dominates over tree if
gravity is strong)
Higgs-radion mixing
25
Graviton emission Tree-level graviton
exchange Graviton loops Gauge/graviton
loop G.G.-Strumia
26
v
Gravitational scattering G.G.-Rattazzi-Wells
Black-hole production Giddings-Thomas,
Dimopoulos-Landsberg
27
SM PARTICLES IN EXTRA DIMENSIONS
  • Gauge bosons in 5D
  • Direct indirect limits Mc gt 6.8 TeV
    Cheung-Landsberg
  • At LHC up to 13-15 TeV
  • Weaker bounds in universal extra dimensions
  • After compactification, momentum conservation
    in 5th dim _ KK number conserved
  • KK particles pair produced no tree-level
    exchange
  • Mc gt 0.3 TeV
    Appelquist-Cheng-Dobrescu

28
CONCLUSIONS
  • Many open theoretical options for new physics at
    EW scale
  • Direct searches precision measurements _ no
    existing theory is completely free of fine-tuning

Connection with MPl Gauge coupling unification
  • LLH or LSM _ Need for UV

  • completion at L
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