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CURVEDEXTRA-DIMENSIONS
Nicolas
Deutschmann
Work in progress with Giacomo Cacciapaglia and Aldo Deandrea
University of the Witwatersrand, Johannesburg
NITheP, July 22th
2014
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Outline
Introduction: Why 2UED is attractive
Survey of Positively Curved Geometries
A UED model with Bulk fermions
Localizing fermions
Conclusion: A negative future ?
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Introduction: Why 2UED is
attractive
Nicolas Deutschmann Curved Extra-Dimensions 3/25
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Dark Matter!
.
Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
Nicolas Deutschmann Curved Extra-Dimensions 5/25
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Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
Nicolas Deutschmann Curved Extra-Dimensions 5/25
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5/25
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Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
• Neutrinos: See-Saw
Nicolas Deutschmann Curved Extra-Dimensions 5/25
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Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
• Neutrinos: See-Saw
• Dark Matter: often a
by-product of other
models with additional
ad hoc parity (R-parity,
KK-parity...)
Nicolas Deutschmann Curved Extra-Dimensions 5/25
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Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
• Neutrinos: See-Saw
• Dark Matter: often a
by-product of other
models with additional
ad hoc parity (R-parity,
KK-parity...)
Nicolas Deutschmann Curved Extra-Dimensions 5/25
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5/25
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A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
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A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
• The eigenmodes of all fields in Xn create a KK-tower.
Nicolas Deutschmann Curved Extra-Dimensions 6/25
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A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
• The eigenmodes of all fields in Xn create a KK-tower.
• Isometries of Xn: Noether theorem imposes selection rules for
decays
Nicolas Deutschmann Curved Extra-Dimensions 6/25
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A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
• The eigenmodes of all fields in Xn create a KK-tower.
• Isometries of Xn: Noether theorem imposes selection rules for
decays
A stable excitation of a neutral SM field could be Dark Matter!
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Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
2UED
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Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
2UED
Nicolas Deutschmann Curved Extra-Dimensions 7/25
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7/25
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Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
2UED
Nicolas Deutschmann Curved Extra-Dimensions 7/25
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7/25
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Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Nicolas Deutschmann Curved Extra-Dimensions 7/25
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7/25
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Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
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7/25
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Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
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7/25
.
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
Similar tricks for some
R2
/G
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
.
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
Similar tricks for some
R2
/G
Exactly one flat geometry
(Cacciapaglia et al.)
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
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7/25
.
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
Similar tricks for some
R2
/G
Exactly one flat geometry
(Cacciapaglia et al.)
With greater dimensions comes greater freedom
No systematic survey of curved spaces
Nicolas Deutschmann Curved Extra-Dimensions 7/25
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Survey of Positively Curved
Geometries
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Positively curved geometries
.
Uniformization theorem..
.
All positively curved 2D surfaces can be described as S2
/G with
G a discrete subgroup of O(3)
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Positively curved geometries
.
Uniformization theorem..
.
All positively curved 2D surfaces can be described as S2
/G with
G a discrete subgroup of O(3)
First question: Which of these have non-trivial isometries ?
Nicolas Deutschmann Curved Extra-Dimensions 9/25
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Positively curved geometries
.
Uniformization theorem..
.
All positively curved 2D surfaces can be described as S2
/G with
G a discrete subgroup of O(3)
First question: Which of these have non-trivial isometries ?
Fundamental relation:
S ∈ Isom(S2
/G) ⇐⇒ ∀g ∈ G, ∃h ∈ G|S(g(x)) = h(S(x))
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Orbifolds with symmetries
(a) S2
/Cn (b) S2
/Cnh (c) S2
/Sn (d) S2
/Dn
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Orbifolds with symmetries
(a) S2
/Cn (b) S2
/Cnh (c) S2
/Sn (d) S2
/Dn
Next question: Which of this can embed 4D chiral fermions ?
Nicolas Deutschmann Curved Extra-Dimensions 10/25
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Orbifolds with symmetries
(a) S2
/Cn (b) S2
/Cnh (c) S2
/Sn (d) S2
/Dn
Next question: Which of this can embed 4D chiral fermions ?
Nicolas Deutschmann Curved Extra-Dimensions 10/25
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A UED model with Bulk
fermions
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A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Nicolas Deutschmann Curved Extra-Dimensions 12/25
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A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Add an extra U(1) gauge field X
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A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Add an extra U(1) gauge field X
The connection term in the two Weyl spinors of a chiral 6D
spinors become different:
χ = ∂χ + (X + Ω)η η = ∂η + (X − Ω)χ
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A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Add an extra U(1) gauge field X
The connection term in the two Weyl spinors of a chiral 6D
spinors become different:
χ = ∂χ + (X + Ω)η η = ∂η + (X − Ω)χ
If X cancels ±Ω one of the chiralities has a zero-mode.
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Tentative Model
Start by writing the Standard Model Lagrangian in 6D
L = LSM
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Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field
L = LSM −
1
4
XµνXµν
Nicolas Deutschmann Curved Extra-Dimensions 13/25
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Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field
L = LSM −
1
4
XµνXµν
With ⟨X⟩ a magnetic monopole, fixed by GR:
⟨X⟩ =
n
2g
cos θdϕ =
√
2R
κ
cos θdϕ
Nicolas Deutschmann Curved Extra-Dimensions 13/25
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Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field
L = LSM −
1
4
XµνXµν
With ⟨X⟩ a magnetic monopole, fixed by GR:
⟨X⟩ =
n
2g
cos θdϕ =
√
2R
κ
cos θdϕ
How to hide this new gauge boson ?
Nicolas Deutschmann Curved Extra-Dimensions 13/25
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Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field and an additional Higgs field :
L = LSM −
1
4
XµνXµν
+ |DM H|2
+ µ2
|H|2
−
λ
2
|H|4
With ⟨X⟩ a magnetic monopole, fixed by GR:
⟨X⟩ =
n
2g
cos θdϕ =
√
2R
κ
cos θdϕ
How to hide this new gauge boson ?
Nicolas Deutschmann Curved Extra-Dimensions 13/25
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Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent :
Nicolas Deutschmann Curved Extra-Dimensions 14/25
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Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent : Numerical Solution
Nicolas Deutschmann Curved Extra-Dimensions 14/25
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Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent : Numerical Solution
.
Method..
.
Minimization using
Fourier coefficients
Nicolas Deutschmann Curved Extra-Dimensions 14/25
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Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent : Numerical Solution
.
Method..
.
Minimization using
Fourier coefficients
1 2 3 4 5
0.001
0.01
0.1
1
1 2 3 4 5
Mode
Αi
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Effects of the symmetry breaking
• Higgs:
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Effects of the symmetry breaking
• Higgs: O(1/R)
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Effects of the symmetry breaking
• Higgs: O(1/R)
• X: g/R ∼ 10 keV
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Effects of the symmetry breaking
• Higgs: O(1/R)
• X: g/R ∼ 10 keV
Too weak coupling for collider physics.
Compatible with short-range gravity tests
Nicolas Deutschmann Curved Extra-Dimensions 15/25
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Effects of the symmetry breaking
• Higgs: O(1/R)
• X: g/R ∼ 10 keV
Too weak coupling for collider physics.
Compatible with short-range gravity tests
1 10 100 1000
10-2
10-1
100
101
102
103
104
105
106
107
108
109
1010
Excludedby
experiment
Lamoreaux
U.Colorado
Stanford2
Stanford1
U.Washington2
gauged
B#
Yukawamessengers
dilaton
KKgravitons
strange
modulus
gluon
modulus
heavyq
moduli
Stanford3
α
λ (µm)
U.Washington1
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Spectrum of the model
SM Gauge scalar X vector Extra Higgs
0
1
2
3
4
5
6
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Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
Nicolas Deutschmann Curved Extra-Dimensions 17/25
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Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
Nicolas Deutschmann Curved Extra-Dimensions 17/25
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17/25
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Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
.
Tier-1 Excitations..
.
• Need to be pair-produced
• Gluon most likely (massless zero-mode &
QCD)
• Signature: jj + ̸ET
• Loop calculation needed to raise
degeneracy with γ
• Open question: prompt decay to LKK ?
Nicolas Deutschmann Curved Extra-Dimensions 17/25
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17/25
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Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Tier-2 Excitations..
.
• As for Tier-1: Gluon
• If Isom(S2/G) = Z2: Single production
• Need less
√
s
• Striking jj resonance easier to look for
• Sets a limit around 1.5 − 2 TeV
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
.
Tier-1 Excitations..
.
• Need to be pair-produced
• Gluon most likely (massless zero-mode &
QCD)
• Signature: jj + ̸ET
• Loop calculation needed to raise
degeneracy with γ
• Open question: prompt decay to LKK ?
Nicolas Deutschmann Curved Extra-Dimensions 17/25
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17/25
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Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Tier-2 Excitations..
.
• As for Tier-1: Gluon
• If Isom(S2/G) = Z2: Single production
• Need less
√
s
• Striking jj resonance easier to look for
• Sets a limit around 1.5 − 2 TeV
• Constraints can be escaped if S2/G has
a continuous symmetry
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
.
Tier-1 Excitations..
.
• Need to be pair-produced
• Gluon most likely (massless zero-mode &
QCD)
• Signature: jj + ̸ET
• Loop calculation needed to raise
degeneracy with γ
• Open question: prompt decay to LKK ?
Nicolas Deutschmann Curved Extra-Dimensions 17/25
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Summing up the model
Spherical Extra-Dimensions are hard to construct.
• Chiral fermions do not come easily
• Need to add two extra-fields: X and H′
• Unsatisfying because
◦ X and H′ are rather untestable
◦ They are ugly
Nicolas Deutschmann Curved Extra-Dimensions 18/25
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Localizing fermions
Nicolas Deutschmann Curved Extra-Dimensions 19/25
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Branes, fat branes and all that
Bottom-up
All but one symmetric
orbifolds have singular
points
• QFT argument:
localized counter-terms
• GR argument: branes
Top-Bottom ∃ explicit
examples of localization:
• RS (not relevant)
• Georgi mechanism on
S1
/Z2
Nice for later if the model
is phenomenologically
relevant.
Nicolas Deutschmann Curved Extra-Dimensions 20/25
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What the model looks like
• Specific orbifold
choice: S2
/S4
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What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
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What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
• 4D Standard model
fermion content with
gauge couplings to the
4D gauge vectors
Nicolas Deutschmann Curved Extra-Dimensions 21/25
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What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
• 4D Standard model
fermion content with
gauge couplings to the
4D gauge vectors
• first tier: unstable
scalars (loop-level)
Nicolas Deutschmann Curved Extra-Dimensions 21/25
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What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
• 4D Standard model
fermion content with
gauge couplings to the
4D gauge vectors
• first tier: unstable
scalars (loop-level)
• second tier: unstable
vectors, stable scalars
(DM)
Nicolas Deutschmann Curved Extra-Dimensions 21/25
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Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level:
• Tier-2 excitations provide resonances:
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon:
• Direct detection:
• Relic density:
Nicolas Deutschmann Curved Extra-Dimensions 22/25
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Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances:
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon:
• Direct detection:
• Relic density:
Nicolas Deutschmann Curved Extra-Dimensions 22/25
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Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon:
• Direct detection:
• Relic density:
Nicolas Deutschmann Curved Extra-Dimensions 22/25
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.
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon: WIMPZILLA!
• Direct detection:
• Relic density:
Nicolas Deutschmann Curved Extra-Dimensions 22/25
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.
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon: WIMPZILLA!
• Direct detection: hard because loop-suppressed
• Relic density:
Nicolas Deutschmann Curved Extra-Dimensions 22/25
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22/25
.
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon: WIMPZILLA!
• Direct detection: hard because loop-suppressed
• Relic density: needs loop calculations
Nicolas Deutschmann Curved Extra-Dimensions 22/25
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.
Conclusion: A negative future ?
Nicolas Deutschmann Curved Extra-Dimensions 23/25
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A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
Nicolas Deutschmann Curved Extra-Dimensions 24/25
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A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
Nicolas Deutschmann Curved Extra-Dimensions 24/25
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24/25
.
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
Nicolas Deutschmann Curved Extra-Dimensions 24/25
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.
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
Nicolas Deutschmann Curved Extra-Dimensions 24/25
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24/25
.
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
• Many features attractive for cosmology (flatness, uniformity,
inflation, ...)
Nicolas Deutschmann Curved Extra-Dimensions 24/25
...
24/25
.
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
• Many features attractive for cosmology (flatness, uniformity,
inflation, ...)
• Topological constraints (genus↔ V/Rn
) make the curvature
radius the only thing to stabilize
Nicolas Deutschmann Curved Extra-Dimensions 24/25
...
24/25
.
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
• Many features attractive for cosmology (flatness, uniformity,
inflation, ...)
• Topological constraints (genus↔ V/Rn
) make the curvature
radius the only thing to stabilize
• Quantum corrections could play a significant role as Mpl goes
down
Nicolas Deutschmann Curved Extra-Dimensions 24/25
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Thank you for your attention
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"Curved extra-dimensions" by Nicolas Deutschmann (Institut de Physique Nucleaire de Lyon, France)

  • 1. .. CURVEDEXTRA-DIMENSIONS Nicolas Deutschmann Work in progress with Giacomo Cacciapaglia and Aldo Deandrea University of the Witwatersrand, Johannesburg NITheP, July 22th 2014 Nicolas Deutschmann Curved Extra-Dimensions 1/25 ... 1/25
  • 2. . Outline Introduction: Why 2UED is attractive Survey of Positively Curved Geometries A UED model with Bulk fermions Localizing fermions Conclusion: A negative future ? Nicolas Deutschmann Curved Extra-Dimensions 2/25 ... 2/25
  • 3. . Introduction: Why 2UED is attractive Nicolas Deutschmann Curved Extra-Dimensions 3/25 ... 3/25
  • 5. . Ad hoc parities Many theoretically satisfying solutions to the short-comings of the Standard Model Nicolas Deutschmann Curved Extra-Dimensions 5/25 ... 5/25
  • 6. . Ad hoc parities Many theoretically satisfying solutions to the short-comings of the Standard Model • Hierarchy: SuSy, RS, Little Higgs Nicolas Deutschmann Curved Extra-Dimensions 5/25 ... 5/25
  • 7. . Ad hoc parities Many theoretically satisfying solutions to the short-comings of the Standard Model • Hierarchy: SuSy, RS, Little Higgs • Neutrinos: See-Saw Nicolas Deutschmann Curved Extra-Dimensions 5/25 ... 5/25
  • 8. . Ad hoc parities Many theoretically satisfying solutions to the short-comings of the Standard Model • Hierarchy: SuSy, RS, Little Higgs • Neutrinos: See-Saw • Dark Matter: often a by-product of other models with additional ad hoc parity (R-parity, KK-parity...) Nicolas Deutschmann Curved Extra-Dimensions 5/25 ... 5/25
  • 9. . Ad hoc parities Many theoretically satisfying solutions to the short-comings of the Standard Model • Hierarchy: SuSy, RS, Little Higgs • Neutrinos: See-Saw • Dark Matter: often a by-product of other models with additional ad hoc parity (R-parity, KK-parity...) Nicolas Deutschmann Curved Extra-Dimensions 5/25 ... 5/25
  • 10. . A potential solution in the UED frame work Universal Extra-Dimensions: all fields propagate in the bulk • (4 + n)D space: M4 × Xn a compact space Nicolas Deutschmann Curved Extra-Dimensions 6/25 ... 6/25
  • 11. . A potential solution in the UED frame work Universal Extra-Dimensions: all fields propagate in the bulk • (4 + n)D space: M4 × Xn a compact space • The eigenmodes of all fields in Xn create a KK-tower. Nicolas Deutschmann Curved Extra-Dimensions 6/25 ... 6/25
  • 12. . A potential solution in the UED frame work Universal Extra-Dimensions: all fields propagate in the bulk • (4 + n)D space: M4 × Xn a compact space • The eigenmodes of all fields in Xn create a KK-tower. • Isometries of Xn: Noether theorem imposes selection rules for decays Nicolas Deutschmann Curved Extra-Dimensions 6/25 ... 6/25
  • 13. . A potential solution in the UED frame work Universal Extra-Dimensions: all fields propagate in the bulk • (4 + n)D space: M4 × Xn a compact space • The eigenmodes of all fields in Xn create a KK-tower. • Isometries of Xn: Noether theorem imposes selection rules for decays A stable excitation of a neutral SM field could be Dark Matter! Nicolas Deutschmann Curved Extra-Dimensions 6/25 ... 6/25
  • 14. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED 2UED Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 15. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions 2UED Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 16. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions Classical trick on S1 /Z2 for a chiral zero-mode (unique) 2UED Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 17. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions Classical trick on S1 /Z2 for a chiral zero-mode (unique) No symmetry 2UED Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 18. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions Classical trick on S1 /Z2 for a chiral zero-mode (unique) No symmetry 2UED With greater dimensions comes greater freedom Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 19. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions Classical trick on S1 /Z2 for a chiral zero-mode (unique) No symmetry 2UED Chiral fermions, but constructed from both left- and right-handed Weyls With greater dimensions comes greater freedom Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 20. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions Classical trick on S1 /Z2 for a chiral zero-mode (unique) No symmetry 2UED Chiral fermions, but constructed from both left- and right-handed Weyls Similar tricks for some R2 /G With greater dimensions comes greater freedom Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 21. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions Classical trick on S1 /Z2 for a chiral zero-mode (unique) No symmetry 2UED Chiral fermions, but constructed from both left- and right-handed Weyls Similar tricks for some R2 /G Exactly one flat geometry (Cacciapaglia et al.) With greater dimensions comes greater freedom Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 22. . Why go to curved (n ≥ 2) UED ? Two limiting factors: Isometries and fermions 1UED Odd dimensions: no chiral fermions Classical trick on S1 /Z2 for a chiral zero-mode (unique) No symmetry 2UED Chiral fermions, but constructed from both left- and right-handed Weyls Similar tricks for some R2 /G Exactly one flat geometry (Cacciapaglia et al.) With greater dimensions comes greater freedom No systematic survey of curved spaces Nicolas Deutschmann Curved Extra-Dimensions 7/25 ... 7/25
  • 23. . Survey of Positively Curved Geometries Nicolas Deutschmann Curved Extra-Dimensions 8/25 ... 8/25
  • 24. . Positively curved geometries . Uniformization theorem.. . All positively curved 2D surfaces can be described as S2 /G with G a discrete subgroup of O(3) Nicolas Deutschmann Curved Extra-Dimensions 9/25 ... 9/25
  • 25. . Positively curved geometries . Uniformization theorem.. . All positively curved 2D surfaces can be described as S2 /G with G a discrete subgroup of O(3) First question: Which of these have non-trivial isometries ? Nicolas Deutschmann Curved Extra-Dimensions 9/25 ... 9/25
  • 26. . Positively curved geometries . Uniformization theorem.. . All positively curved 2D surfaces can be described as S2 /G with G a discrete subgroup of O(3) First question: Which of these have non-trivial isometries ? Fundamental relation: S ∈ Isom(S2 /G) ⇐⇒ ∀g ∈ G, ∃h ∈ G|S(g(x)) = h(S(x)) Nicolas Deutschmann Curved Extra-Dimensions 9/25 ... 9/25
  • 27. . Orbifolds with symmetries (a) S2 /Cn (b) S2 /Cnh (c) S2 /Sn (d) S2 /Dn Nicolas Deutschmann Curved Extra-Dimensions 10/25 ... 10/25
  • 28. . Orbifolds with symmetries (a) S2 /Cn (b) S2 /Cnh (c) S2 /Sn (d) S2 /Dn Next question: Which of this can embed 4D chiral fermions ? Nicolas Deutschmann Curved Extra-Dimensions 10/25 ... 10/25
  • 29. . Orbifolds with symmetries (a) S2 /Cn (b) S2 /Cnh (c) S2 /Sn (d) S2 /Dn Next question: Which of this can embed 4D chiral fermions ? Nicolas Deutschmann Curved Extra-Dimensions 10/25 ... 10/25
  • 30. . A UED model with Bulk fermions Nicolas Deutschmann Curved Extra-Dimensions 11/25 ... 11/25
  • 31. . A gauge field to kill the connection Method from Randjbar-Daemi, Salam and Strathdee Nicolas Deutschmann Curved Extra-Dimensions 12/25 ... 12/25
  • 32. . A gauge field to kill the connection Method from Randjbar-Daemi, Salam and Strathdee Add an extra U(1) gauge field X Nicolas Deutschmann Curved Extra-Dimensions 12/25 ... 12/25
  • 33. . A gauge field to kill the connection Method from Randjbar-Daemi, Salam and Strathdee Add an extra U(1) gauge field X The connection term in the two Weyl spinors of a chiral 6D spinors become different: χ = ∂χ + (X + Ω)η η = ∂η + (X − Ω)χ Nicolas Deutschmann Curved Extra-Dimensions 12/25 ... 12/25
  • 34. . A gauge field to kill the connection Method from Randjbar-Daemi, Salam and Strathdee Add an extra U(1) gauge field X The connection term in the two Weyl spinors of a chiral 6D spinors become different: χ = ∂χ + (X + Ω)η η = ∂η + (X − Ω)χ If X cancels ±Ω one of the chiralities has a zero-mode. Nicolas Deutschmann Curved Extra-Dimensions 12/25 ... 12/25
  • 35. . Tentative Model Start by writing the Standard Model Lagrangian in 6D L = LSM Nicolas Deutschmann Curved Extra-Dimensions 13/25 ... 13/25
  • 36. . Tentative Model Start by writing the Standard Model Lagrangian in 6D with the new gauge field L = LSM − 1 4 XµνXµν Nicolas Deutschmann Curved Extra-Dimensions 13/25 ... 13/25
  • 37. . Tentative Model Start by writing the Standard Model Lagrangian in 6D with the new gauge field L = LSM − 1 4 XµνXµν With ⟨X⟩ a magnetic monopole, fixed by GR: ⟨X⟩ = n 2g cos θdϕ = √ 2R κ cos θdϕ Nicolas Deutschmann Curved Extra-Dimensions 13/25 ... 13/25
  • 38. . Tentative Model Start by writing the Standard Model Lagrangian in 6D with the new gauge field L = LSM − 1 4 XµνXµν With ⟨X⟩ a magnetic monopole, fixed by GR: ⟨X⟩ = n 2g cos θdϕ = √ 2R κ cos θdϕ How to hide this new gauge boson ? Nicolas Deutschmann Curved Extra-Dimensions 13/25 ... 13/25
  • 39. . Tentative Model Start by writing the Standard Model Lagrangian in 6D with the new gauge field and an additional Higgs field : L = LSM − 1 4 XµνXµν + |DM H|2 + µ2 |H|2 − λ 2 |H|4 With ⟨X⟩ a magnetic monopole, fixed by GR: ⟨X⟩ = n 2g cos θdϕ = √ 2R κ cos θdϕ How to hide this new gauge boson ? Nicolas Deutschmann Curved Extra-Dimensions 13/25 ... 13/25
  • 40. . Higgs Mechanism in a Monopole Background Need to find the minimum |DM H|2 − µ2 |H|2 + λ 2 |H|4 A priori θ-dependent : Nicolas Deutschmann Curved Extra-Dimensions 14/25 ... 14/25
  • 41. . Higgs Mechanism in a Monopole Background Need to find the minimum |DM H|2 − µ2 |H|2 + λ 2 |H|4 A priori θ-dependent : Numerical Solution Nicolas Deutschmann Curved Extra-Dimensions 14/25 ... 14/25
  • 42. . Higgs Mechanism in a Monopole Background Need to find the minimum |DM H|2 − µ2 |H|2 + λ 2 |H|4 A priori θ-dependent : Numerical Solution . Method.. . Minimization using Fourier coefficients Nicolas Deutschmann Curved Extra-Dimensions 14/25 ... 14/25
  • 43. . Higgs Mechanism in a Monopole Background Need to find the minimum |DM H|2 − µ2 |H|2 + λ 2 |H|4 A priori θ-dependent : Numerical Solution . Method.. . Minimization using Fourier coefficients 1 2 3 4 5 0.001 0.01 0.1 1 1 2 3 4 5 Mode Αi Nicolas Deutschmann Curved Extra-Dimensions 14/25 ... 14/25
  • 44. . Effects of the symmetry breaking • Higgs: Nicolas Deutschmann Curved Extra-Dimensions 15/25 ... 15/25
  • 45. . Effects of the symmetry breaking • Higgs: O(1/R) Nicolas Deutschmann Curved Extra-Dimensions 15/25 ... 15/25
  • 46. . Effects of the symmetry breaking • Higgs: O(1/R) • X: g/R ∼ 10 keV Nicolas Deutschmann Curved Extra-Dimensions 15/25 ... 15/25
  • 47. . Effects of the symmetry breaking • Higgs: O(1/R) • X: g/R ∼ 10 keV Too weak coupling for collider physics. Compatible with short-range gravity tests Nicolas Deutschmann Curved Extra-Dimensions 15/25 ... 15/25
  • 48. . Effects of the symmetry breaking • Higgs: O(1/R) • X: g/R ∼ 10 keV Too weak coupling for collider physics. Compatible with short-range gravity tests 1 10 100 1000 10-2 10-1 100 101 102 103 104 105 106 107 108 109 1010 Excludedby experiment Lamoreaux U.Colorado Stanford2 Stanford1 U.Washington2 gauged B# Yukawamessengers dilaton KKgravitons strange modulus gluon modulus heavyq moduli Stanford3 α λ (µm) U.Washington1 Nicolas Deutschmann Curved Extra-Dimensions 15/25 ... 15/25
  • 49. . Spectrum of the model SM Gauge scalar X vector Extra Higgs 0 1 2 3 4 5 6 Nicolas Deutschmann Curved Extra-Dimensions 16/25 ... 16/25
  • 50. . Some Experimental Remarks . X boson properties .. . • Interacts too weakly for colliders • Can decay into neutrinos (Γ ≃ 10−11 eV) • Not a good DM candidate Nicolas Deutschmann Curved Extra-Dimensions 17/25 ... 17/25
  • 51. . Some Experimental Remarks . X boson properties .. . • Interacts too weakly for colliders • Can decay into neutrinos (Γ ≃ 10−11 eV) • Not a good DM candidate . Extra-Higgs .. . No direct SM interaction so not expected at colliders Decay mostly into X pairs Nicolas Deutschmann Curved Extra-Dimensions 17/25 ... 17/25
  • 52. . Some Experimental Remarks . X boson properties .. . • Interacts too weakly for colliders • Can decay into neutrinos (Γ ≃ 10−11 eV) • Not a good DM candidate . Extra-Higgs .. . No direct SM interaction so not expected at colliders Decay mostly into X pairs . Tier-1 Excitations.. . • Need to be pair-produced • Gluon most likely (massless zero-mode & QCD) • Signature: jj + ̸ET • Loop calculation needed to raise degeneracy with γ • Open question: prompt decay to LKK ? Nicolas Deutschmann Curved Extra-Dimensions 17/25 ... 17/25
  • 53. . Some Experimental Remarks . X boson properties .. . • Interacts too weakly for colliders • Can decay into neutrinos (Γ ≃ 10−11 eV) • Not a good DM candidate . Tier-2 Excitations.. . • As for Tier-1: Gluon • If Isom(S2/G) = Z2: Single production • Need less √ s • Striking jj resonance easier to look for • Sets a limit around 1.5 − 2 TeV . Extra-Higgs .. . No direct SM interaction so not expected at colliders Decay mostly into X pairs . Tier-1 Excitations.. . • Need to be pair-produced • Gluon most likely (massless zero-mode & QCD) • Signature: jj + ̸ET • Loop calculation needed to raise degeneracy with γ • Open question: prompt decay to LKK ? Nicolas Deutschmann Curved Extra-Dimensions 17/25 ... 17/25
  • 54. . Some Experimental Remarks . X boson properties .. . • Interacts too weakly for colliders • Can decay into neutrinos (Γ ≃ 10−11 eV) • Not a good DM candidate . Tier-2 Excitations.. . • As for Tier-1: Gluon • If Isom(S2/G) = Z2: Single production • Need less √ s • Striking jj resonance easier to look for • Sets a limit around 1.5 − 2 TeV • Constraints can be escaped if S2/G has a continuous symmetry . Extra-Higgs .. . No direct SM interaction so not expected at colliders Decay mostly into X pairs . Tier-1 Excitations.. . • Need to be pair-produced • Gluon most likely (massless zero-mode & QCD) • Signature: jj + ̸ET • Loop calculation needed to raise degeneracy with γ • Open question: prompt decay to LKK ? Nicolas Deutschmann Curved Extra-Dimensions 17/25 ... 17/25
  • 55. . Summing up the model Spherical Extra-Dimensions are hard to construct. • Chiral fermions do not come easily • Need to add two extra-fields: X and H′ • Unsatisfying because ◦ X and H′ are rather untestable ◦ They are ugly Nicolas Deutschmann Curved Extra-Dimensions 18/25 ... 18/25
  • 56. . Localizing fermions Nicolas Deutschmann Curved Extra-Dimensions 19/25 ... 19/25
  • 57. . Branes, fat branes and all that Bottom-up All but one symmetric orbifolds have singular points • QFT argument: localized counter-terms • GR argument: branes Top-Bottom ∃ explicit examples of localization: • RS (not relevant) • Georgi mechanism on S1 /Z2 Nice for later if the model is phenomenologically relevant. Nicolas Deutschmann Curved Extra-Dimensions 20/25 ... 20/25
  • 58. . What the model looks like • Specific orbifold choice: S2 /S4 Nicolas Deutschmann Curved Extra-Dimensions 21/25 ... 21/25
  • 59. . What the model looks like l=0 l=2 l=3 m=0m=-2 m=2 l=1 • Specific orbifold choice: S2 /S4 • 6D QCD+EW Nicolas Deutschmann Curved Extra-Dimensions 21/25 ... 21/25
  • 60. . What the model looks like l=0 l=2 l=3 m=0m=-2 m=2 l=1 • Specific orbifold choice: S2 /S4 • 6D QCD+EW • 4D Standard model fermion content with gauge couplings to the 4D gauge vectors Nicolas Deutschmann Curved Extra-Dimensions 21/25 ... 21/25
  • 61. . What the model looks like l=0 l=2 l=3 m=0m=-2 m=2 l=1 • Specific orbifold choice: S2 /S4 • 6D QCD+EW • 4D Standard model fermion content with gauge couplings to the 4D gauge vectors • first tier: unstable scalars (loop-level) Nicolas Deutschmann Curved Extra-Dimensions 21/25 ... 21/25
  • 62. . What the model looks like l=0 l=2 l=3 m=0m=-2 m=2 l=1 • Specific orbifold choice: S2 /S4 • 6D QCD+EW • 4D Standard model fermion content with gauge couplings to the 4D gauge vectors • first tier: unstable scalars (loop-level) • second tier: unstable vectors, stable scalars (DM) Nicolas Deutschmann Curved Extra-Dimensions 21/25 ... 21/25
  • 63. . Phenomenology Two competing constraints: LHC v.s. Dark Matter . LHC constraints.. . • Tier-1 excitations couple at loop level: • Tier-2 excitations provide resonances: . Dark matter.. . Likely DM candidate: scalar Tier-2 photon: • Direct detection: • Relic density: Nicolas Deutschmann Curved Extra-Dimensions 22/25 ... 22/25
  • 64. . Phenomenology Two competing constraints: LHC v.s. Dark Matter . LHC constraints.. . • Tier-1 excitations couple at loop level: sub-dominant a priori • Tier-2 excitations provide resonances: . Dark matter.. . Likely DM candidate: scalar Tier-2 photon: • Direct detection: • Relic density: Nicolas Deutschmann Curved Extra-Dimensions 22/25 ... 22/25
  • 65. . Phenomenology Two competing constraints: LHC v.s. Dark Matter . LHC constraints.. . • Tier-1 excitations couple at loop level: sub-dominant a priori • Tier-2 excitations provide resonances: R ≥ 1.5 TeV . Dark matter.. . Likely DM candidate: scalar Tier-2 photon: • Direct detection: • Relic density: Nicolas Deutschmann Curved Extra-Dimensions 22/25 ... 22/25
  • 66. . Phenomenology Two competing constraints: LHC v.s. Dark Matter . LHC constraints.. . • Tier-1 excitations couple at loop level: sub-dominant a priori • Tier-2 excitations provide resonances: R ≥ 1.5 TeV . Dark matter.. . Likely DM candidate: scalar Tier-2 photon: WIMPZILLA! • Direct detection: • Relic density: Nicolas Deutschmann Curved Extra-Dimensions 22/25 ... 22/25
  • 67. . Phenomenology Two competing constraints: LHC v.s. Dark Matter . LHC constraints.. . • Tier-1 excitations couple at loop level: sub-dominant a priori • Tier-2 excitations provide resonances: R ≥ 1.5 TeV . Dark matter.. . Likely DM candidate: scalar Tier-2 photon: WIMPZILLA! • Direct detection: hard because loop-suppressed • Relic density: Nicolas Deutschmann Curved Extra-Dimensions 22/25 ... 22/25
  • 68. . Phenomenology Two competing constraints: LHC v.s. Dark Matter . LHC constraints.. . • Tier-1 excitations couple at loop level: sub-dominant a priori • Tier-2 excitations provide resonances: R ≥ 1.5 TeV . Dark matter.. . Likely DM candidate: scalar Tier-2 photon: WIMPZILLA! • Direct detection: hard because loop-suppressed • Relic density: needs loop calculations Nicolas Deutschmann Curved Extra-Dimensions 22/25 ... 22/25
  • 69. . Conclusion: A negative future ? Nicolas Deutschmann Curved Extra-Dimensions 23/25 ... 23/25
  • 70. . A Brighter Horizon: Hyperbolic Extra-Dimensions • Fermions behave much more nicely: there is a massless mode Nicolas Deutschmann Curved Extra-Dimensions 24/25 ... 24/25
  • 71. . A Brighter Horizon: Hyperbolic Extra-Dimensions • Fermions behave much more nicely: there is a massless mode • Much more freedom: arbitrary high volumes for a given curvature radius Nicolas Deutschmann Curved Extra-Dimensions 24/25 ... 24/25
  • 72. . A Brighter Horizon: Hyperbolic Extra-Dimensions • Fermions behave much more nicely: there is a massless mode • Much more freedom: arbitrary high volumes for a given curvature radius • Mass gap protected by curvature radius Nicolas Deutschmann Curved Extra-Dimensions 24/25 ... 24/25
  • 73. . A Brighter Horizon: Hyperbolic Extra-Dimensions • Fermions behave much more nicely: there is a massless mode • Much more freedom: arbitrary high volumes for a given curvature radius • Mass gap protected by curvature radius • Can pull down Mpl while keeping MKK high enough Nicolas Deutschmann Curved Extra-Dimensions 24/25 ... 24/25
  • 74. . A Brighter Horizon: Hyperbolic Extra-Dimensions • Fermions behave much more nicely: there is a massless mode • Much more freedom: arbitrary high volumes for a given curvature radius • Mass gap protected by curvature radius • Can pull down Mpl while keeping MKK high enough • Many features attractive for cosmology (flatness, uniformity, inflation, ...) Nicolas Deutschmann Curved Extra-Dimensions 24/25 ... 24/25
  • 75. . A Brighter Horizon: Hyperbolic Extra-Dimensions • Fermions behave much more nicely: there is a massless mode • Much more freedom: arbitrary high volumes for a given curvature radius • Mass gap protected by curvature radius • Can pull down Mpl while keeping MKK high enough • Many features attractive for cosmology (flatness, uniformity, inflation, ...) • Topological constraints (genus↔ V/Rn ) make the curvature radius the only thing to stabilize Nicolas Deutschmann Curved Extra-Dimensions 24/25 ... 24/25
  • 76. . A Brighter Horizon: Hyperbolic Extra-Dimensions • Fermions behave much more nicely: there is a massless mode • Much more freedom: arbitrary high volumes for a given curvature radius • Mass gap protected by curvature radius • Can pull down Mpl while keeping MKK high enough • Many features attractive for cosmology (flatness, uniformity, inflation, ...) • Topological constraints (genus↔ V/Rn ) make the curvature radius the only thing to stabilize • Quantum corrections could play a significant role as Mpl goes down Nicolas Deutschmann Curved Extra-Dimensions 24/25 ... 24/25
  • 77. . Thank you for your attention Nicolas Deutschmann Curved Extra-Dimensions 25/25 ... 25/25