Precision calculations of semileptonic B decays
Yu-Ming Wang
Technische Universität München
The 10th TeV Physics Workshop
- 09. 08. 2015
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 1/22
Precision calculations of semileptonic B decays Yu-Ming Wang - - PowerPoint PPT Presentation
Precision calculations of semileptonic B decays Yu-Ming Wang Technische Universitt Mnchen The 10th TeV Physics Workshop 09. 08. 2015 Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 1 / 22 Where do we stand now? Big success of the SM and
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 1/22
CMS Exotica Physics Group Summary – ICHEP , 2014
stopped gluino (cloud) stopped stop (cloud) HSCP gluino (cloud) HSCP stop (cloud) q=2/3e HSCP q=3e HSCP neutralino, ctau=25cm, ECAL time 1 2 3 4 RS1(γγ), k=0.1 RS1(ee,uu), k=0.1 RS1(jj), k=0.1 RS1(WW→4j), k=0.1 1 2 3 4 coloron(jj) x2 coloron(4j) x2 gluino(3j) x2 gluino(jjb) x2 1 2 3 4
RS Gravitons Multijet Resonances Long-Lived Particles
SSM Z'(ττ) SSM Z'(jj) SSM Z'(bb) SSM Z'(ee)+Z'(µµ) SSM W'(jj) SSM W'(lv) SSM W'(WZ→lvll) SSM W'(WZ→4j) 1 2 3 4
Heavy Gauge Bosons
j+MET, SI DM=100 GeV, Λ j+MET, SD DM=100 GeV, Λ γ+MET, SI DM=100 GeV, Λ γ+MET, SD DM=100 GeV, Λ l+MET, ξ=+1, SI DM=100 GeV, Λ l+MET, ξ=+1, SD DM=100 GeV, Λ l+MET, ξ=-1, SI DM=100 GeV, Λ l+MET, ξ=-1, SD DM=100 GeV, Λ 1 2 3 4
Dark Matter
LQ1(ej) x2 LQ1(ej)+LQ1(νj) LQ2(μj) x2 LQ2(μj)+LQ2(νj) LQ3(νb) x2 LQ3(τb) x2 LQ3(τt) x2 LQ3(vt) x2 1 2 3 4
Leptoquarks
e* (M=Λ) μ* (M=Λ) q* (qg) q* (qγ) b* 1 2 3 4
Excited Fermions
dijets, Λ+ LL/RR dijets, Λ- LL/RR dimuons, Λ+ LLIM dimuons, Λ- LLIM dielectrons, Λ+ LLIM dimuons, Λ- LLIM single e, Λ HnCM single μ, Λ HnCM inclusive jets, Λ+ inclusive jets, Λ- 4 8 13 17 21
ADD (γγ), nED=4, MS ADD (ee,μμ), nED=4, MS ADD (j+MET), nED=4, MD ADD (γ+MET), nED=4, MD QBH, nED=4, MD=4 TeV NR BH, nED=4, MD=4 TeV Jet Extinction Scale String Scale (jj)
2 4 5 7 9
Large Extra Dimensions Compositeness
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 2/22
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 3/22
◮ EFT parametrization of BSM physics:
dim4 + ∑ n>4∑ i
(i)
i
◮ Dimension-n operator Q(n)
i
◮ Higher dimension operator Q(n)
i
◮ Two examples: (a) leading NP operators of D = 6 for ∆F = 2 processes
AB,ij =
γ γ α α
d
m ∆
K
ε
K
ε
s
m ∆ &
d
m ∆
ub
V β sin 2
(excl. at CL > 0.95) < 0 β
excluded at CL > 0.95
α β γ
ρ
0.0 0.5 1.0 1.5 2.0
η
0.0 0.5 1.0 1.5
excluded area has CL > 0.95 Winter 14
CKM
f i t t e r
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 4/22
◮ Why are the quark masses (except the top) so small compared with the vev? ◮ Why is the CKM matrix hierarchical? ◮ Why is CKM so different from the PMNS? ◮ Why do we have three families? ◮ Sources of flavor symmetry and violation? Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 5/22
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 6/22
i
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 7/22
0.5 1 1.5
0.5 1 1.5 2
sin 2β B → ρρ B → ρρ ∆md ∆ms & ∆md εK εK |Vub/Vcb| sin 2β α β γ ρ η
excluded area has CL < 0.05
CK M
f i t t e r Winter 2004
γ γ α α
d
m ∆
K
ε
K
ε
s
m ∆ &
d
m ∆
ub
V β sin 2
(excl. at CL > 0.95) < 0 β
excluded at CL > 0.95
α β γ
0.0 0.5 1.0 1.5 2.0
0.0 0.5 1.0 1.5
excluded area has CL > 0.95 Winter 14
CKM
f i t t e r
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 8/22
4
2
2
5 10 15
5
0.5 1
SM from DHMV
[LHCb-CONF-2015-002]
[1407.8526]
RK = B r ( B+ → K+ µ+ µ− ) B r ( B+ → K+ e+ e− )
5 anomaly below 6GeV2 more serious [power corrections].
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 9/22
ub
2
< 12 GeV
2
Khodjamirian et al. q
0.06 + 0.37 - 0.32 ± 3.41
2
< 16 GeV
2
Ball-Zwicky q
0.06 + 0.59 - 0.40 ± 3.58
2
> 16 GeV
2
HPQCD q
0.08 + 0.61 - 0.40 ± 3.52
2
> 16 GeV
2
FNAL/MILC q
0.08 + 0.37 - 0.31 ± 3.36
PDG 2014
ub
)
e
CLEO (E
0.50 + 0.31 - 0.36 ± 4.28
)
2
, q
X
BELLE sim. ann. (m
0.47 + 0.28 - 0.30 ± 4.49
)
e
BELLE (E
0.46 + 0.27 - 0.29 ± 4.93
)
e
BABAR (E
0.26 + 0.27 - 0.33 ± 4.54
)
max h
, s
e
BABAR (E
0.22 + 0.33 - 0.38 ± 4.53
BELLE multivariate (p*)
0.27 + 0.20 - 0.22 ± 4.49
<1.55)
X
BABAR (m
0.20 + 0.28 - 0.27 ± 4.30
<1.7)
X
BABAR (m
0.23 ± 0.22 ± 4.04
>8)
2
<1.7, q
X
BABAR (m
0.23 + 0.26 - 0.28 ± 4.30
<0.66)
+
BABAR (P
0.25 + 0.28 - 0.27 ± 4.15
BABAR (p*>1GeV)
0.24 + 0.19 - 0.21 ± 4.32
BABAR (p*>1.3GeV)
0.27 + 0.20 - 0.21 ± 4.32
Average +/- exp + th. - th.
0.16 + 0.21 - 0.22 ± 4.45
PDG14 Bosch, Lange, Neubert and Paz (BLNP) Phys.Rev.D72:073006,2005 /dof = 9.0/11 (CL = 62.00 %)
2
χ
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 10/22
¯ B π ℓ νℓ b u
Bπ(q2)
B −m2 π
Bπ(q2) m2 B −m2 π
F|Vub|2
B
l )2 |
l
B |
Bπ(q2)|2 + 3m2 l
B −m2 π)2 |f 0 Bπ(q2)|2
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 11/22
B +m2 π −q2
π
B
π
B
πh πh
π −p2)
Bπ(n·p)+f 0 Bπ(n·p)
ωs
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 12/22
B u
B (ω′)
Bπ(n·p)
Bπ(n·p)+O(αs).
B (ω) =
B (ω) defined in a similar way.]
B (ω′) at NLO must be IR finite.
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 13/22
¯ d bv
µ +Π(1) µ +... = ΦB ⊗T
B ⊗T(0) +
B ⊗T(1) +Φ(1) B ⊗T(0)
B ⊗T(1) = Π(1) µ −Φ(1) B ⊗T(0) . Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 14/22
µ,weak
s CF
b +i0][l2 +i0]
B,weak ⊗T(0)
s CF
β α = − i ˜
B (ω)n
B (ω)¯
B (ω)γµ ⊥
⊥
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 15/22
k=±
B (ω,µ)
k=±
B (ω,µ).
n bv +....
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 16/22
B (ω,µ)
B (ω,µ)
B (ω′,µ)
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 17/22
π /(n·pωM)
Bπ(n·p), f 0 Bπ(n·p)
B,eff(ω′,µ)+
B,eff(ω′,µ)
B,eff(ω′,µ)+C(−)(n·p,µ)φ− B (ω′,µ)
B,eff(ω′,µ) = 0 + αs CF
ω′
B (ω,µ) ,
B,eff(ω′,µ) = φ− B (ω′,µ)+ αs CF
B (ω,µ)
ω′ dω
B (ω,µ)
QCD/mb). Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 18/22
B,I(ω,µ0) = ω
B,II(ω,µ0) =
B,III(ω,µ0) = 2ω2
1
B,IV(ω,µ0) =
Bπ(q2) less model dependent.
Bπ(q2 = 0) = 0.28±0.03
−30 MeV ,
−35 MeV ,
−30 MeV ,
−30 MeV .
2 4 6 8 0.0 0.2 0.4 0.6 0.8 q2 GeV2 fB Π
q2
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 19/22
fB Π
q20
LL NLL NLO 1.0 1.2 1.4 1.6 1.8 2.0 0.1 0.2 0.3 0.4 0.5 Μ GeV fB Π
q2NLL fB Π q2LL
2 4 6 8 0.4 0.6 0.8 1.0 1.2 1.4 q2 GeV2
◮ Dominant radiative effect from the NLO QCD correction instead of the QCD resummation. ◮ Resummation improvement does stabilize the factorization scale dependence. ◮ Radiative effect can induce 20 % reduction of the form factor. Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 20/22
Bπ(q2):
Bπ(q2) from B-
f BΠ
q2
2 4 6 8 10 12 0.0 0.2 0.4 0.6 0.8 1.0 q2 GeV2
−0.38
−0.42
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 21/22
Yu-Ming Wang (TUM) B decays Beijing, 09. 08. 2015 22/22