s=2 decay in warped extra dimensions -...
TRANSCRIPT
∆S = 2 decay in Warped Extra Dimensions
Faisal Munir
IHEP, BeijingSupervisor: Cai-Dian Lu
HFCPV
CCNU, WuhanOctober 28, 2017
based on: Chin. Phys. C41 (2017) 053106 [arXiv:1607.07713]
F. Munir (IHEP) New Physics 1 / 14
Outline
Introduction
b → ssd decay in the RS model with custodial protection
b → ssd decay in the bulk-Higgs RS model
Summary
F. Munir (IHEP) New Physics 2 / 14
Introduction to RS model
5D spacetime with warped metric[Randall, Sundrum, Phys. Rev. Lett. 83, 3370 (1999)]
ds2 = e−2kr|φ|ηµνdxµdxν − r2dφ2, φ ∈ [−π, π].
The fundamental scale is MP l, and the effective 4D electroweak scaleis suppressed by a magic exponential
MEW ∼ e−krπMP l ∼ TeV.
natural explanation of gauge hierarchy problem. hierarchical structure of zero mode fermion profiles
Light fermions live close to UV brane.Third generation localized closest to the IR brane.
Kaluza-Klein (KK) excitations live close to the IR brane. Warped extra dimensions with bulk fields have explanation for
fermion masses and CKM hierarchies. Tree level FCNCs (b → ssd).
F. Munir (IHEP) New Physics 3 / 14
b → ssd Channel
Local ∆S = 2 SM effective Hamiltonian for b → ssd transition
H∆S=2eff =
G2F m2
W
16π2
(
VtdV∗
tsVtbV∗
tsS0
(
m2t
m2W
)
+ VcdV∗
csVtbV∗
tsS0
(
m2c
m2W
,m2
t
m2W
))
× [(sd)V −A(sb)V −A]
B(B+ → K+K+π−) < 1.1 × 10−8
[R. Aaij et al. (LHCb), Phys. Lett. B765, 307 (2017)]
b s
ds
u, c, t
u, c, t
W− W+
b → ssd decay with very small strength in the SM serves as asensitive probe for new physics.
B(b → ssd)SM = (2.19 ± 0.38) × 10−12
F. Munir (IHEP) New Physics 4 / 14
b → ssd decay in the RSc model
The RSc model is based on a single warped extra dimension with the bulk gaugegroup
SU(3)c × SU(2)L × SU(2)R × U(1)X × PLR
b → ssd decay receives tree level contributions fromthe Kaluza-Klein (KK) gluons, the heavy KK photons,new heavy electroweak (EW) gauge bosons ZH and Z′,and in principle the Z0 boson.
Custodial protection of the ZbLbL coupling through thediscrete PLR symmetry renders tree-level Z0
contributions negligible.
The effective Hamiltonian for the ∆S = 2 b → ssd
decay with the Wilson coefficients corresponding toµ = O(Mg(1) )
b
s
s
d
G(1)µ
b
s
s
d
Z, Z ′, ZH , A(1)
[H∆S=2eff ]KK =
1
2(Mg(1) )2[CV LL
1 QV LL1 + C
V RR1 Q
V RR1
+ CLR1 Q
LR1 + C
LR2 Q
LR2 + C
RL1 Q
RL1 + C
RL2 Q
RL2 ].
F. Munir (IHEP) New Physics 5 / 14
b → ssd decay in the RSc model
QV LL1 = (sγµPLb)(sγµPLd),
QV RR1 = (sγµPRb)(sγµPRd),
QLR1 = (sγµPLb)(sγµPRd),
QLR2 = (sPLb)(sPRd),
QRL1 = (sγµPRb)(sγµPLd),
QRL2 = (sPRb)(sPLd),
[CV LL1 (M
g(1) )]G = 23
pUV2∆sb
L∆sd
L,
[CV RR1 (M
g(1) )]G = 23
pUV2∆sb
R∆sd
R,
[CLR1 (M
g(1) )]G = − 13
pUV2∆sb
L∆sd
R,
[CLR2 (M
g(1) )]G = −2pUV2∆sb
L∆sd
R,
[CRL1 (M
g(1) )]G = − 13
pUV2∆sb
R∆sd
L,
[CRL2 (M
g(1) )]G = −2pUV2∆sb
R∆sd
L,
[∆CV LL1 (M
g(1) )]EW = 2[∆sbL
(Z(1))∆sdL
(Z(1)) + ∆sbL
(Z(1)
X)∆sd
L(Z
(1)
X)],
[∆CV RR1 (M
g(1) )]EW = 2[∆sbR
(Z(1))∆sdR
(Z(1)) + ∆sbR
(Z(1)
X)∆sd
R(Z
(1)
X)],
[∆CLR1 (M
g(1) )]EW = 2[∆sbL
(Z(1))∆sdR
(Z(1)) + ∆sbL
(Z(1)
X)∆sd
R(Z
(1)
X)],
[∆CRL1 (M
g(1) )]EW = 2[∆sbR
(Z(1))∆sdL
(Z(1)) + ∆sbR
(Z(1)
X)∆sd
L(Z
(1)
X)],
[∆CV LL1 (M
g(1) )]QED = 2[∆sbL
(A(1))][∆sdL
(A(1))],
[∆CV RR1 (M
g(1) )]QED = 2[∆sbR
(A(1))][∆sdR
(A(1))],
[∆CLR1 (M
g(1) )]QED = 2[∆sbL
(A(1))][∆sdR
(A(1))],
[∆CRL1 (M
g(1) )]QED = 2[∆sbR
(A(1))][∆sdL
(A(1))],
F. Munir (IHEP) New Physics 6 / 14
b → ssd decay in the RSc model
CV LL1 (Mg(1) ) = [0.67 + 0.02 + 0.56]∆sb
L ∆sdL = 1.25∆sb
L ∆sdL ,
CV RR1 (Mg(1) ) = [0.67 + 0.02 + 0.98]∆sb
R ∆sdR = 1.67∆sb
R ∆sdR ,
CLR1 (Mg(1) ) = [−0.333 + 0.02 + 0.56]∆sb
L ∆sdR = 0.25∆sb
L ∆sdR ,
CRL1 (Mg(1) ) = [−0.333 + 0.02 + 0.56]∆sb
R ∆sdL = 0.25∆sb
R ∆sdL ,
After RG running of the Wilson coefficients to a low energy scaleµb = 4.6 GeV, the decay width in the RSc model
Γ =m5
b
3072(2π)3(Mg(1))4[16(|CV LL
1 (µb)|2 + |CV RR
1 (µb)|2)
+ 12(|CLR1 (µb)|2 + |CRL
1 (µb)|2) + 3(|CLR2 (µb)|
2 + |CRL2 (µb)|
2)
− 2Re(CLR1 (µb)C
∗LR2 (µb) + CLR
2 (µb)C∗LR1 (µb)
+ CRL1 (µb)C∗RL
2 (µb) + CRL2 (µb)C∗RL
1 (µb))].
F. Munir (IHEP) New Physics 7 / 14
b → ssd decay in the bulk-Higgs RS model
The bulk-Higgs RS model is based on the 5D gauge groupSU(3)c × SU(2)V × U(1)Y , where all the fields propagate in the 5Dspacetime.
b → ssd decay in the bulk-Higgs RS model results from tree-level
exchanges of Kaluza-Klein gluons and photons, the Z0 boson andthe Higgs boson as well as their KK excitations and the extendedscalar fields φZ(n).
We consider the summation over the contributions from the entire KKtowers, with the lightest KK states having mass Mg(1) ≈ 2.45 MKK.
[H∆S=2eff ]KK =
5∑
n=1
[CnOn + CnOn],
O1 = (sLγµbL)(sLγµdL),
O2 = (sRbL)(sRdL),
O3 = (sαRb
βL)(sβ
RdαL),
O4 = (sRbL)(sLdR),
O5 = (sαRb
βL)(sβ
LdαR).
F. Munir (IHEP) New Physics 8 / 14
b → ssd decay in the bulk-Higgs RS model
C1 =4πL
M2KK
(∆D)23 ⊗ (∆D)21[αs
2(1 −
1
Nc
) + αQ2d +
α
s2wc2
w
(T d3 − Qds2
w)2],
C1 =4πL
M2KK
(∆d)23 ⊗ (∆d)21[αs
2(1 −
1
Nc) + αQ2
d +α
s2wc2
w
(−Qds2w)2],
C4 = −4πLαs
M2KK
(∆D)23 ⊗ (∆d)21 −L
πβM2KK
(Ωd)23 ⊗ (ΩD)21,
C4 = −4πLαs
M2KK
(∆d)23 ⊗ (∆D)21 −L
πβM2KK
(ΩD)23 ⊗ (Ωd)21,
C5 =4πL
M2KK
(∆D)23 ⊗ (∆d)21[αs
Nc
− 2αQ2d +
2α
s2wc2
w
(T d3 − Qds2
w)(Qds2w)],
C5 =4πL
M2KK
(∆d)23 ⊗ (∆D)21[αs
Nc
− 2αQ2d +
2α
s2wc2
w
(T d3 − Qds2
w)(Qds2w)],
F. Munir (IHEP) New Physics 9 / 14
b → ssd decay in the bulk-Higgs RS model
(∆D)23 ⊗ (∆d)21 → (U†
d)2i(Ud)i3(∆Dd)ij (W
†
d)2j (Wd)j1,
(∆Dd)ij =F 2(cQi
)
3 + 2cQi
3 + cQi+ cdj
2(2 + cQi+ cdj
)
F 2(cdj)
3 + 2cdj
,
(ΩD)23 ⊗ (Ωd)21 → (U†
d)2i(Wd)j3(ΩDd)ijkl(W
†
d)2k(Ud)l1,
(ΩDd)ijkl =π(1 + β)
4L
F (cQi)F (cdj
)
2 + β + cQi+ cdj
(Yd)ij (Y†
d)kl
1
×(4 + 2β + cQi
+ cdj+ cdk
+ cQl)
4 + cQi+ cdj
+ cdk+ cQl
F (cdk)F (cQl
)
2 + β + cdk+ cQl
,
The decay width in the bulk-Higgs RS model
Γ =m5
b
3072(2π)3[64(|C1(µb)|2 + |C1(µb)|2)
+ 12(|C4(µb)|2 + |C4(µb)|2 + |C5(µb)|2 + |C5(µb)|2)
+ 4Re(C4(µb)C∗5 (µb) + C∗
4 (µb)C5(µb)
+ C4(µb)C∗5 (µb) + C∗
4 (µb)C5(µb))].
F. Munir (IHEP) New Physics 10 / 14
Phenomenological bounds on RS models
The RSc modelConstraint from tree-level analysis of the S and T parameters
[Malm, Neubert, Novotny, Schmell, JHEP 01 (2014) 173]
Mg(1) > 4.8 TeV (95% CL).
[Malm, Neubert, Schmell, JHEP 02 (2015) 008]
Stringent bounds emerge from the signal rates for pp → h → ZZ∗, W W ∗, at95% CL
Mg(1) |custodial RS
brane-Higgs > 22.7 TeV × (y⋆
3), M
g(1) |custodial RSnarrow bulk-Higgs
> 13.2 TeV × (y⋆
3)
F. Munir (IHEP) New Physics 11 / 14
Branching ratio of b → ssd in the RSc model
∆MK , ǫK and ∆MBs
constraints
KK gluons dominant
Comparable ZH andZ ′ contributions
F. Munir (IHEP) New Physics 12 / 14
Branching ratio in the bulk-Higgs RS model
broad Higgs profile
β = 1
narrow Higgs profile
β = 10
F. Munir (IHEP) New Physics 13 / 14
Summary
In both models, the main contribution to the b → ssd decay comesfrom tree level exchanges of KK gluons, while in the RSc model thecontributions from the new heavy EW gauge bosons ZH and Z ′ cancompete with the KK-gluon contributions.
We employed renormalization group runnings of the Wilsoncoefficients with NLO QCD factors in both models.
The RSc model enhances the branching ratio, compared to the SMresult, by two order of magnitude for some points in the parameterspace with y⋆ = 1.5.
In the bulk-Higgs RS model with β = 10, it is possible to achieve anorder of magnitude enhancement of the branching ratio for some ofthe parameter points.
THANK YOU!
F. Munir (IHEP) New Physics 14 / 14