SLIDE 1
'You Better Run' Connecting low-energy Dark Matter searches with high-energy physics
Bradley J. Kavanagh LPTHE & IPhT (CEA/Saclay)
NewDark
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
'You Better Run' Connecting low-energy Dark Matter searches with - - PowerPoint PPT Presentation
'You Better Run' Connecting low-energy Dark Matter searches with - - PowerPoint PPT Presentation
'You Better Run' Connecting low-energy Dark Matter searches with high-energy physics Bradley J. Kavanagh LPTHE & IPhT (CEA/Saclay) Kings College London - 13th June 2016 bradley.kavanagh@lpthe.jussieu.fr @BradleyKavanagh NewDark
SLIDE 2
SLIDE 3
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ
UV this way
mV
Collider searches
∼ 10 TeV
SLIDE 4
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ
UV this way
mV
Collider searches Direct direction
∼ 10 TeV ∼ 1 GeV
SLIDE 5
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ
UV this way
mV
Collider searches Direct direction
∼ 10 TeV ∼ 1 GeV
SLIDE 6
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ
UV this way
mV
Direct direction
∼ 1 GeV
SLIDE 7
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Comparing different searches
ATLAS [1604.07773] Zemeckis, Hanks (1994)
SLIDE 8
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Outline
Simplified Models RG effects in Simplified Models Direct detection constraints on Simplified Models Comparing DD and LHC searches
De Simone, Jacques [1603.08002] Crivellin, D’Eramo, Procura [1402.1173]; D’Eramo, Procura [1411.3342] D’Eramo, Procura [1411.3342]; D’Eramo, BJK, Panci [1605.04917] D’Eramo, BJK, Panci [1605.04917]
SLIDE 9
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Simplified Models
SLIDE 10
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Effective Field Theory
Assume mass of mediator is much larger than momentum transfer integrate out mediator to obtain a contact interaction Only have to deal with two parameters: mχ, Λ
Goodman et al. [1008.1783]
SLIDE 11
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Limits on EFT
ATLAS [1502.01518]
SLIDE 12
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
The problem with EFTs
Frandsen et al. [1204.3839], Buchmueller et al. [1407.8257], Malik et al. [1409.4075], Abdallah et al. [1506.03116], and many others… Buchmueller et al. [1308.6799]
SLIDE 13
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Simplified Models to the rescue
cq cχ
Now have to deal with more parameters: cq, cχ, mχ, mV
Review: De Simone, Jacques [1603.08002] ATLAS [1604.07773]
SLIDE 14
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Our Simplified Model
SLIDE 15
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Vector mediator simplified model
L = LSM + LDM + LV + Jµ
DM Vµ + Jµ SM Vµ
SLIDE 16
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Vector mediator simplified model
LDM ∼ ( |∂µφ|2 − m2
φ |φ|2
complex scalar DM χ
- i/
∂ − mχ
- χ
fermion DM L = LSM + LDM + LV + Jµ
DM Vµ + Jµ SM Vµ
SLIDE 17
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Vector mediator simplified model
L = LSM + LDM + LV + Jµ
DM Vµ + Jµ SM Vµ
LV = −1 4V µνVµν + 1 2m2
V V µVµ
Massive spin-1 mediator V
SLIDE 18
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Jµ
DM ∼
⇢ cφ φ† ← → ∂ µφ complex scalar DM cχV χγµχ + cχA χγµγ5χ fermion DM
Vector mediator simplified model
L = LSM + LDM + LV + Jµ
DM Vµ + Jµ SM Vµ
SLIDE 19
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Vector mediator simplified model
L = LSM + LDM + LV + Jµ
DM Vµ + Jµ SM Vµ
Jµ
SM = 3
X
i=1
h c(i)
q
qi
Lγµqi L + c(i) u ui Rγµui R + c(i) d
di
Rγµdi R + c(i) l
li
Lγµli L + c(i) e
ei
Rγµei R
i
15 independent, SU(2)L x U(1)Y gauge-invariant couplings
SLIDE 20
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Calculating the direct detection rate
SLIDE 21
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Direct detection
mχ & 1 GeV v ∼ 10−3
DM
Rate driven by coupling of DM to light quarks (u, d, s): Look for low energy - O(keV) - recoils of detector nuclei χγµχ qγµq χγµγ5χ qγµγ5q χγµχ qγµγ5q χγµγ5χ qγµq
SLIDE 22
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Direct detection
mχ & 1 GeV v ∼ 10−3
DM
Rate driven by coupling of DM to light quarks (u, d, s): Look for low energy - O(keV) - recoils of detector nuclei χγµχ qγµq χγµγ5χ qγµγ5q χγµχ qγµγ5q χγµγ5χ qγµq Standard SI Standard SD
SLIDE 23
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Connecting high and low scales
Define couplings at high energy scale (mediator mass), but need to calculate direct detection rate at low energy
Kopp et al. [0907.3159], Frandsen et al. [1207.3971], Haisch, Kahlhoefer [1302.4454], Kopp et al. [1401.6457], Crivellin, Haisch [1408.5046]
Running can change the DD rate by orders of magnitude. Examples in specific models:
- Use EFT techniques and RG flow to study
the effects for general interactions
- Include all relevant DD interactions (not just
naive ‘leading order’)
SLIDE 24
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ mV
SMχ ⇠⇠ EW SMχ
D’Eramo, Procura [1411.3342]
NREFT
SLIDE 25
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ mV
SMχ ⇠⇠ EW SMχ
Integrate out vector mediator
D’Eramo, Procura [1411.3342]
NREFT
SLIDE 26
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ mV
SMχ ⇠⇠ EW SMχ
Integrate out vector mediator
D’Eramo, Procura [1411.3342]
NREFT
c(i)
V,A u = ±c(i) q
+ c(i)
u
2 c(i)
V,A d = ±c(i) q
+ c(i)
d
2 c(i)
V,A e = ±c(i) l
+ c(i)
e
2
Matching at EWSB
SLIDE 27
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ mV
SMχ ⇠⇠ EW SMχ
Integrate out vector mediator Run down to electroweak scale
D’Eramo, Procura [1411.3342]
NREFT
SLIDE 28
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ mV
SMχ ⇠⇠ EW SMχ
Integrate out vector mediator Run down to electroweak scale Match onto EW-broken theory
D’Eramo, Procura [1411.3342]
NREFT
SLIDE 29
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ mV
SMχ ⇠⇠ EW SMχ
Integrate out vector mediator Run down to electroweak scale Match onto EW-broken theory Run down to nuclear scale
D’Eramo, Procura [1411.3342]
NREFT
SLIDE 30
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
E
mN mZ mV
SMχ ⇠⇠ EW SMχ
NREFT Integrate out vector mediator Run down to electroweak scale Match onto EW-broken theory Run down to nuclear scale Match onto nucleon couplings Calculate direct detection rate
D’Eramo, Procura [1411.3342]
SLIDE 31
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
RGE effects
As we move between the different scales, we have to take into account the running of the couplings, due only to loops of Standard Model particles, e.g.
Self-renormalisation Operator mixing
SLIDE 32
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
RGE effects
As we move between the different scales, we have to take into account the running of the couplings, due only to loops of Standard Model particles, e.g. The running doesn’t depend on the properties of the Dark Sector.
Self-renormalisation Operator mixing
SLIDE 33
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
RGE effects
As we move between the different scales, we have to take into account the running of the couplings, due only to loops of Standard Model particles, e.g. The running doesn’t depend on the properties of the Dark Sector.
Self-renormalisation Operator mixing
Y O U H A V E T O R U N !
SLIDE 34
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
runDM - a code for the RGE
Mathematica and Python versions available at: https://github.com/bradkav/runDM/
SLIDE 35
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
runDM - a code for the RGE
Mathematica and Python versions available at: https://github.com/bradkav/runDM/
Input: DM-SM couplings at high energy scale Output: DM-SM couplings at another arbitrary energy scale OR DM-nucleon couplings at direct detection scale
SLIDE 36
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Direct detection constraints
SLIDE 37
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Results I - quarks vector
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµχ ¯ fγµf
LUX 2014 LZ projected
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµui + diγµdii
SLIDE 38
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Results I - quarks vector
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµχ ¯ fγµf
LUX 2014 LZ projected
c(q)
V
∼ 1 + # e2 16π2 ln(mV /mN)
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµui + diγµdii
SLIDE 39
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Results I - quarks vector
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµχ ¯ fγµf
LUX 2014 LZ projected
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµγ5χ ¯ fγµf
LUX 2014 L Z p r
- j
e c t e d
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµui + diγµdii
SLIDE 40
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV]
L U X 2 1 4 LZ projected
Flavor universal: Quarks only ¯ χγµγ5χ ¯ fγµγ5f
Results II - quarks axial-vector
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµγ5ui + diγµγ5dii
No running Running
SLIDE 41
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Aside: SM axial-vector current
But only for coupling to AV current of SM fermions!
JDM µ qγµγ5q
SLIDE 42
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV]
L U X 2 1 4 LZ projected
Flavor universal: Quarks only ¯ χγµγ5χ ¯ fγµγ5f
Results II - quarks axial-vector
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµγ5ui + diγµγ5dii
No running Running
SLIDE 43
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµγ5χ ¯ fγµγ5f
L U X 2 1 4 L Z p r
- j
e c t e d
c(q)
A ∼ 1 + #
λ2
b,t
16π2 ln(mV /mN)
Results II - quarks axial-vector
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµγ5ui + diγµγ5dii
No running Running
SLIDE 44
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV]
LUX 2014 LZ projected
Flavor universal: Quarks only ¯ χγµχ ¯ fγµγ5f
Results II - quarks axial-vector
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµγ5ui + diγµγ5dii
No running Running
SLIDE 45
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Results II - quarks axial-vector
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµγ5ui + diγµγ5dii
10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµχ ¯ fγµγ5f
LUX 2014 L Z p r
- j
e c t e d
c(q)
V
∼ 0 + # λ2
b,t
16π2 ln(mV /mN)
No running Running
SLIDE 46
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµχ ¯ fγµγ5f
LUX 2014 L Z p r
- j
e c t e d
10 102 103 104 Dark Matter mass mχ [GeV] 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµγ5χ ¯ fγµγ5f
L U X 2 1 4 L Z p r
- j
e c t e d
Results II - quarks axial-vector
LEFT = − 1 m2
V
JDM µ
3
X
i=1
h uiγµγ5ui + diγµγ5dii
No running Running
SLIDE 47
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV] Third Generation ¯ χγµχ ¯ fγµγ5f 10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV] Third Generation ¯ χγµγ5χ ¯ fγµγ5f
Results III - 3rd Generation axial-vector
LEFT = − 1 m2
V
JDM µ ⇥ tγµγ5t + bγµγ5b + τγµγ5τ ⇤
SLIDE 48
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV] Third Generation ¯ χγµχ ¯ fγµγ5f
LUX 2014 LZ projected
10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV] Third Generation ¯ χγµγ5χ ¯ fγµγ5f
LUX 2014 L Z p r
- j
e c t e d
Results III - 3rd Generation axial-vector
LEFT = − 1 m2
V
JDM µ ⇥ tγµγ5t + bγµγ5b + τγµγ5τ ⇤
SLIDE 49
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Comparing DD and LHC searches
SLIDE 50
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
LHC mono-X searches
ATLAS [1604.07773]
LAV = gχVµ χγµγ5χ + gqVµ X
q
qiγµγ5qi
SLIDE 51
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’ 1 10 102 103 104
Dark Matter mass mχ [GeV]
10−43 10−42 10−41 10−40 10−39 10−38 10−37
σSD (DM-neutron) [cm2] gq = 0.25, gχ = 1.0
Axial Vector Mediator
LUX 2016 ATLAS monojet
1 10 102 103 104
Dark Matter mass mχ [GeV]
10−43 10−42 10−41 10−40 10−39 10−38 10−37
σSD (DM-proton) [cm2] gq = 0.25, gχ = 1.0
Axial Vector Mediator
L U X 2 1 6 PICO-2L ATLAS monojet
LHC mono-X searches
LAV = gχVµ χγµγ5χ + gqVµ X
q
qiγµγ5qi
SLIDE 52
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’ 1 10 102 103 104
Dark Matter mass mχ [GeV]
10−43 10−42 10−41 10−40 10−39 10−38 10−37
σSD (DM-proton) [cm2] gq = 0.25, gχ = 1.0
Axial Vector Mediator
L U X 2 1 6 P I C O
- 2
L ATLAS monojet ATLAS monojet (with running)
1 10 102 103 10−43 10−42
1 10 102 103 104
Dark Matter mass mχ [GeV]
10−43 10−42 10−41 10−40 10−39 10−38 10−37
σSD (DM-neutron) [cm2] gq = 0.25, gχ = 1.0
Axial Vector Mediator
L U X 2 1 6 ATLAS monojet ATLAS monojet (with running)
1 10 102 103 10−43 10−42
LHC mono-X searches
LAV = gχVµ χγµγ5χ + gqVµ X
q
qiγµγ5qi
SLIDE 53
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Isospin violation
LAV = gχVµ χγµγ5χ + gqVµ X
q
qiγµγ5qi
10 102 103 104 105 Mediator mass mV [GeV] 0.0 0.5 1.0 1.5 2.0 2.5 σN
SD(with running)/σN SD(without running)
p r
- t
- n
neutron
Flavor universal: Quarks only ¯ χγµγ5χ ¯ fγµγ5f
C(N)
A
= gq 2 4 X
q=u,d,s
∆(N)
q
3 5 + 3gq 2π ⇣ ∆(N)
d
+ ∆(N)
s
− ∆(N)
u
⌘ [αt ln(mV /mZ) − αb ln(mV /µN)]
SLIDE 54
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Other interactions
Goodman et al. [1008.1783]
Standard SI Standard SD
SLIDE 55
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Other interactions
Goodman et al. [1008.1783]
SLIDE 56
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Other interactions
Goodman et al. [1008.1783]
10 102 103 104 Dark Matter mass mχ [GeV] 1 10 102 103 104 105 106 Mediator mass mV [GeV] Flavor universal: Quarks only ¯ χγµχ ¯ fγµγ5f
LUX 2014 L Z p r
- j
e c t e d
SLIDE 57
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Caveats
If we add extra degrees of freedom, the phenomenology may be different
E.g. Jackson et al. [1303.4717]
May want to include mass and/or kinetic mixing of the mediator
Langacker [0801.1345]
LKM ∼ ✏ZµνV µν but we expect this to strengthen the limits In general, we need to worry about the UV completion (e.g. anomaly cancellation, Higgling of the U(1)’, etc.) But if we stick to the Simplified Model framework, our results are valid - and unavoidable!
SLIDE 58
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Summary
Need to take into account separation of scales RGE (use runDM code) Low-E couplings changed and new operators induced limits on heavy mediators affected (sometimes by OoM!) Running is important for search complementarity
- req. for translating LHC searches into DD plane
Isospin violation (factor of ~few) is automatic arising only from SM loops
SLIDE 59
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Summary
Need to take into account separation of scales RGE (use runDM code) Low-E couplings changed and new operators induced limits on heavy mediators affected (sometimes by OoM!) Running is important for search complementarity
- req. for translating LHC searches into DD plane
Isospin violation (factor of ~few) is automatic arising only from SM loops
YOU HAVE TO RUN!
SLIDE 60
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Backup slides
SLIDE 61
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Scalar Mediators
Crivellin, D’Eramo, Procura [1402.1173]
Interactions through a scalar mediator appear at dimension-7, with rates typically suppressed by the quark mass
Buckley et al. [1410.6497]
SLIDE 62
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’
Scalar mediator: 750 GeV
D’Eramo, de Vries, Panci [1601.01571]
Substantial RG effects!
SLIDE 63
Bradley J Kavanagh (LPTHE & IPhT) King’s College London - 13th June 2016 ‘You Better Run’