the hierarchy problem on neutral - uspfma.if.usp.br/~burdman/talks/pascos15.pdf · gustavo burdman...
TRANSCRIPT
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The Hierarchy Problem on Neutral
Gustavo Burdman University of São Paulo - IAS Princeton
Natural Theories with Colorless Top Partners
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Is the discovery of the Higgs the End of Naturalness ?
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Naturalness and the LHC
Is the Electroweak scale natural ?
• The LHC found the Higgs
• Plus … nothing else.
vEW
Ebounds
MPlanck
Little hierarchy}
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Naturalness and the LHC
Is the Electroweak scale natural ?
• The LHC found the Higgs
• Plus … nothing else.
vEW
Ebounds
MPlanck
Little hierarchy}SM
few TeVEbounds
⇠
Tuned
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Naturalness and the LHC
UV sensitivity of dominated by top quarkm2h
+
) • Top partners X carry color
• Easily produced at the LHC{
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Colorless Top Partners Last refuge of naturalness ?
Top partners need not carry color
If symmetry protecting does not commute with m2h SU(3)c
Exchanges SU(3)c ! SU(3)0
The X’s are charged under SU(3)0
Bounds on not as stringent mX
Colorless X models are more natural
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Colorless Top Partners General idea To solve the Little Hierarchy problem
vEW
Ebounds
MPlanck
Little hierarchy}SM + colorless top partners
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Colorless Top Partners Ingredients for neutral naturalness
• Symmetry protecting the Higgs: spontaneously broken global symmetry, SUSY, …
• Extend the color gauge symmetry to have at least [SU(3)]2
• Either impose a discrete symmetry or orbifold In general, CTP theories can be obtained from orbifolding
N.Craig, S.Knapen, P. Longhi, 1410.6806, 1411.7393
• ModelsTwin Higgs
Folded SUSY
Quirky Little Higgs H. Cai, H.-C. Cheng, J. Terning, 0812.0843
Z. Chacko, H. Goh and R. Harnik, hep-ph/0506256
G.B., Z.Chacko, H. Goh, R. Harnik , hep-ph/0609152
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The Twin Higgs
Higgs is a pNGB of a spontaneously broken global symmetry
SU(4) ! SU(3) 7 NGBs
V (H) = �m2H†H + �(H†H)2
Starting with a fundamental with potential
Z. Chacko, H. Goh and R. Harnik, hep-ph/0506256
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The Twin Higgs
Gauge a subgroup: SU(2)A ⇥ SU(2)B
H =
✓HA
HB
◆
hHiChoose so that stays masslessHA SM Higgs doublet
Gauge interactions break global symmetry explicitly
Quadratically divergent contributions to V
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The Twin Higgs Gauge loops lead to
9
64⇡2g2 ⇤2 H†H is symmetricSU(4)
9
64⇡2
⇣g2AH
†AHA ⇤2
A + g2BH†BHB ⇤2
B
⌘
But imposing a symmetry Z2 gA = gB = g ⇤A = ⇤B,
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The Twin Higgs
E.g. Top Yukawas:
�AHAqAtA + �BHBqBtB
generate
3
8⇡2�2 ⇤2 H†H
Z2
Mirror SM sector
SMA ⇥ SMB
Extend to all SM interactions
3
8⇡2
⇣�2AH
†AHA ⇤2
A + �2BH
†BHB ⇤2
B
⌘
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Twin Higgs in Non-linear Representation
H =
✓HA
HB
◆= e
if ⇧
0
BB@
000f
1
CCA
with
⇧ =
0
BB@
0 0 0 h1
0 0 0 h2
0 0 0 0h⇤1 h⇤
2 0 0
1
CCA
and all the B NGBs were eaten by B gauge bosons
The SM Higgs is h =
✓h1
h2
◆
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�t h qAtA + �t
✓f � 1
2fh†h
◆qBtB
tA
qA
h h�t �t tBqB
h h
�t f
��t/2f
Cancellation
But have colorqB , tB SU(3)B
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Breaking of Symmetry Z2
If is exact Z2 vEW = f
Adding a soft breaking term µ2|HA|2 allows vEW < f
Couplings of the Higgs to SM fields suppressed by
cos ✓ = cos
✓vp2 f
◆
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Twin Higgs Models
Identical Twin:• Complete copy of the SM
• fv' 3� 10 ) ⇤0
QCD > ⇤QCD⇠• Light quarks and leptons
U(1)B• ?
Chacko, Goh, Harnik
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Twin Higgs and Higgs Physics
All Higgs couplings to SM states suppressed by cos ✓
�(pp ! ⇢) = �SM (pp ! h)cos
2 ✓
E.g.:
cos
2 ✓�(⇢ ! Ai) = �SM (h ! SMi)
Invisible width
�(⇢ ! B) = �SM (h) sin2 ✓ �
� < 1 vEW < fwith for
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Prediction Identical Twin
Higgs couplings G.B., Z.Chacko, R.Harnik, L. Lima, C. Verhaaren, 1411.3310
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Fraternal Twin: Twin Higgs Models
•Only minimal fermion content to solve hierarchy problemQ3, tR, bR, L
3, ⌧R 3rd generation twin fermions
•Higgs glueballs SM
Craig, Katz, Strassler, Sundrum, 1501.05310
c⌧0 ⇠ 18m⇥✓10 GeV
m0
◆7
⇥✓
f
750 GeV
◆4
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Twin Higgs Dark Matter
Twin strong sector generates a higher strong scale
⇤0QCD > ⇤QCD⇠
Possible Asymmetric Dark Matter candidate
mn ' few mn)
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Twin Higgs Dark Matter
Twin strong sector generates a higher strong scale
⇤0QCD > ⇤QCD⇠
Possible Asymmetric Dark Matter candidate
mn ' few mn)
M. Farina, 1506.03520
Lux
CDMSlite
SuperCDMS
10.05.03.0 7.010-47
10-45
10-43
10-41
10-39
10-37
mDM @GeVD
sSI@cm
-2 D
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Fraternal Twin Higgs Dark Matter Asymmetric DM: I. Garcia, R. Lasemby, J. March-Rusell, 1505.07410
Twin bottom baryons �b
Thermal Relic (TWIMP ?)
I. Garcia, R. Lasemby, J. March-Rusell, 1505.07109
Mostly ⌧
N. Craig, A. Katz, 1505.07113
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Colorless Top Partners in Supersymmetry
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Folded Supersymmetry
Cancellation of top divergence
HuHu�t �t
q
u
Hu Hu
�2t
q, u
• Squarks need to be charged under SU(2)L
• Need not be charged under SU(3)c
G.B., Z.Chacko, H. Goh, R. Harnik , hep-ph/0609152
But how ?
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Bifold Protection
S Qi Qi� i = 1 . . . , NU(N)Global
is quadratically divergentM2S
• Supersymmetrize
• Duplicate index running in loop: i = 1, . . . ., 2N
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• Theory is invariant under
Z2R{fermions odd
bosons even
Bifold Protection • Define
� =
0
BBBBBBBB@
+1. . .
+1�1
. . .�1
1
CCCCCCCCA
1...N
N + 1...
2N
Z2� Qi ! ��Qi{S ! S
Qi ! ��⇤ Qi
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Bifold Protection
q1...qN
q1...qN
qN+1...
q2N
qN+1...
q2N
+1
�1
+1�1
Z2�
Z2R
Project out states odd under Z2� ⇥ Z2ROrbifold projection:
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Bifold Protection Project out states odd under Z2� ⇥ Z2R
q1...qN
q1...qN
qN+1...
q2N
qN+1...
q2N
+1
�1
+1�1
Z2�
Z2R
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Bifold Protection Accidental SUSY: spectrum not supersymmetric
But still cancels one-loop quadratic divergence
+q1...qN
qN+1...
q2N
S S S S
j = N + 1, . . . , 2Ni = 1, . . . , N
qiqj
M.Bershadsky, A.Johansen, hep-th/9803248;Large-N orbifold correspondence:
S.Kachru, E. Silverstein, hep-th/9802183;
M.Schmaltz, hep-th/9805218
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Realistic Folded SUSY Model
Orbifold so that:
qB , uBqA, uA + remain in the spectrum
No gauginos
Yukawas obey
(�t hu qA uA + h.c.) + �2t |qB hu|2 + �2
t |uB |2 |hu|2
Accidental SUSY still protects m2h
Gauge symmetry:SU(3)A ⇥ SU(3)B ⇥ Z2 ⇥ SU(2)L ⇥ U(1)Y
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Folded SUSY UV Completion
SUSY broken by BCs (Scherk-Schwarz)
BCs break at Z2 ⇡R
Can be realized in 5D compactified on S1/Z2
SU(3)A ⇥ SU(3)B ⇥ Z2
SU(2)L ⇥ U(1)Y
0 ⇡R
HU , HD
QA, QB , UA, UB , DA, DB
LA, LB , EA, EB
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Folded SUSY Spectrum
• Scalar zero modes from
• Fermion zero modes from
QA, UA, DA, LA, EA
QB , UB , DB , LB , EB
• Localize Higgses at y = 0
�(y)�t {Q3AHUU3A +Q3BHUU3B}
generates desired Yukawas at low energies
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Folded SUSY Spectrum
m2Q = K
1
4⇡4
✓4
3g23 +
3
4g22 +
1
36g21
◆1
R2
m2U = K
1
4⇡4
✓4
3g23 +
4
9g21
◆1
R2
m2D = K
1
4⇡4
✓4
3g23 +
1
9g21
◆1
R2
m2L = K
1
4⇡4
✓3
4g22 +
1
4g21
◆1
R2
m2E = K
1
4⇡4g21
1
R2
Zero-mode Folded sfermions: A. Delgado, A. Pomarol, M Quiros, hep-ph/9812489
plus Yukawa contributions for 3rd generation
m2Q3
= K�2t
8⇡4
1
R2m2
U3= K
�2t
4⇡4
1
R2
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Folded SUSY
vEW
1
R
Accidental SUSY
5D SUSY
⇤
1
R⇠ (5� 7) TeV
⇤R < 4⇠
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Folded SUSY Signals
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Folded SUSY Signals at the LHC
Electroweak pair production of F-squarks
But mT � ⇤0QCD ' few GeV they do not hadronize
q
q⇤
p p
“squirks” have to come back for annihilation
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Squirk Annihilation
q
q
W±⇤ u
d
W±
�
• Annihilation is prompt
• Onium is in s-wave before annihilation
G.B., Z.Chacko, H.Goh, R. Harnik, C. Krenke, 0805.4667
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Bounds from the LHC
Assumes• No smearing
�• No decay
mT >{ 320445465
GeV}
mT
Direct search betterthan Higgs couplings
G.B., Z.Chacko, R.Harnik, L. Lima, C. Verhaaren, 1411.3310
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Folded Sleptons (G.B., R. D'Agnolo, 150x.xxxx)
In the minimal model, lepton hypermultiplets
LA(1, 1, 2,�1/2) LB(1, 1, 2,�1/2)
EA(1, 1, 1, 1) EB(1, 1, 1, 1)
Zero modes: Leptons F-sleptons
Lightest F-slepton is stable ! Need to add preserving HDOs Z2
�(y)
Zd✓2
✓UAUADAEB
⇤+
UBUBDBEA
⇤
◆E.g.
Highly displaced vertices
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-5
-4
-3
-2
-10
1
23
4
56
7
0 10 20 30 40 50 60
500
1000
1500
2000
500
1000
1500
2000
2500
m0 (GeV)
mt(GeV
)[FoldedSUSY]
mT(GeV
)[TwinHiggs
]Figure 4. Contours show log
10
c⌧/m, where c⌧ is the mean decay length of the lightest glueball state 0
++.Computed with Eq. (3.13) in Folded SUSY Eq. (3.8) and Twin Higgs Eq. (3.12) theories. The blue bandscorrespond to the shift of the contours resulting from the 25% uncertainty in the total 0
++ width.
where Br(h ! gg)SM
⇡ 8.6%.The coupling ratio ↵B
s (mh)/↵As (mh) depends on the mirror sector spectrum between m
0
and mh.Ignoring threshold effects below mh, it can be estimated by solving Eq. (3.2) for µB
pole
and evolvingto µ = mh:
↵Bs (mh)
�1
=
b
2⇡log
mh
µBpole
, where µBpole
= µApole
· m0
a0
(rSM0
)
�1
. (3.17)
The minimal assumption is b = 11, corresponding to no mirror sector matter below mh. This isalmost required by LEP limits for Folded SUSY and Quirky Little Higgs. The resulting coupling ratio�↵Bs (mh)/↵A
s (mh)�2 is shown as the green band in Fig. 5 (left), ranging from about 1 to 2.5 for m
0
from 10 to 60 GeV. For a likely Fraternal Twin Higgs scenario, with a single mirror bottom below mh
(assumed for illustrative purposes to be close to m0
in mass), the ratio is only about 10% higher dueto the negative contribution to b, as indicated by the purple band. If much more matter is present therecan be significant enhancement, as shown by the red band for all mirror quarks being close in mass tom
0
except the mirror top. However, as illustrated by Fig. 3 (bottom), in Twin Higgs scenarios this isonly compatible with glueball masses below 25 GeV.
3.5 Estimating 0
++ production
Owing to the vastly different lifetimes of the glueball states, we need to estimate the exclusive pro-duction rate of 0
++ from exotic Higgs decays, since it will likely be the only glueball state thatdecays observably (though there can be exceptions). This requires detailed knowledge of pure-glue
– 16 –
Folded SUSY Glueball Decays
D. Curtin, 1506.06141
Will start being competitive at HL-LHC
![Page 41: The Hierarchy Problem on Neutral - USPfma.if.usp.br/~burdman/talks/pascos15.pdf · Gustavo Burdman University of São Paulo - IAS Princeton Natural Theories with Colorless Top Partners](https://reader034.vdocuments.net/reader034/viewer/2022042811/5fa4dd0968aba930900a435b/html5/thumbnails/41.jpg)
Summary •We still have natural theories of EWSB not ruled out by data
•Signals at colliders are different
•The LHC has sensitivity for a lot of the parameter space
• But not impossible that HL-LHC ends and some "natural" parameter space still there (e.g. Identical Twin Higgs)
•All these theories have low cutoffs (< 20 TeV)
Experiment: Higher energies
Theory: UV completions
•Interesting for DM model building (especially ADM)