J. CHARLES (CPT Marseille), H. LACKER (Dresden University),
description
Transcript of J. CHARLES (CPT Marseille), H. LACKER (Dresden University),
Flavour in the
era of the LHC
A Model-Independent Analysis
of New Physics Contributions
in |F| = 2 transitions J. CHARLES (CPT Marseille), H. LACKER (Dresden University),
A. ROBERT, S. MONTEIL (LPC IN2P3 – University Blaise Pascal)
on behalf the CKMfitter group
November 7-10th 2005
Outline – New Physics in |F|=2 transitions1
Part I. Introduction. Part II. Exploring New Physics in Bd mixing. Basic inputs. Adding and measurements. Adding aSL contribution.
Part III. Exploring New Physics in K mixing.
Part IV. Prospective for New Physics in the Bs mixing.
Quality of CKM Standard fit
Standard Model accommodates successfully
all the present flavour data.
2
There is no need a priori for NP contributions in tree-mediated flavour changing processes.
00
0022
BSMeffHB
BfulleffHB
diedr
Modelling New Physics in |B|=2
Assumption no NP in tree-mediated decay amplitudes: |Vub|/|Vcb| and are the main inputs constraining the CKM parameters.
Introduce NP inB=2 transitions accounted for model-independently through two additional parameters.
Is there still room for new physics ?Follow the strategy developed in the paper: The CKMfitter group, Eur. Phys. J. C41 (2005)
Past & present attempts (a selection of)Soares, Wolfenstein, Phys. Rev. D47 (1993)
Grossman, Nir, Worah, Phys. Lett. B407 (1996)Laplace, Ligeti, Nir, Perez, Phys. Rev. D65 (2002)
Ciuchini et al., hep-ph/0307195Bona et al., hep-ph/0509219
3
NP in Bd-Bd mixing (I)
)22cos(
)22sin(
,2
d
d
dd
cbub
mr
VV
• The SM value on 2d=0 is at the border of the CLMax region.
• Shows slight disagreement between Vub and sin(2.
Remove b-> scomponent from the inclusive Vub average Vub=(4.15 ±0.12 ±0.23).10-3
• Any region with 2d > /2 is discarded.
4
NP in Bd-Bd mixing (II)
)(
)22cos(
)22sin(
/2
GGSZGLWADS
mr
VV
d
d
dd
cbub
Adding measurements.
• Two solutions for NP parameters emerge.
• Vub and constrain the CKM parameters.
5
NP in Bd-Bd mixing (III)
Adding measurements.
)222sin(
)22cos(
)22sin(
/2
d
d
d
dd
cbub
mr
VV
The constraint (w/o ) displays also four solutions.
Reinforce the SM region but the preferred NP region is not the one defined by .
6
NP in Bd-Bd mixing (IV)
)222sin(
)(
)22cos(
)22sin(
/2
d
d
d
dd
cbub
GGSZGLWADS
mr
VV
and are of major importance in constraining the NP parameters.
NB: sin(d) is not included. (almost no influence.)
7
NP in Bd-Bd mixing aSL in the game
212
122
12
12SL
2cosIm
2sinRe
d
dSM
d
dSM
rMrMa
Though the experimental precision is far from the prediction, aSL is a crucial input for constraining NP parameters. Only observable depending on both rd
2 and 2d.
(12/M12 is considered here at Leading Order)
aSL= -0.0026 ± 0.0067(HFAG 2005)
8
deg3.52
92.0
2.38.8
73.023.0
2
d
dr
NP parameters extraction
SL
)(
2
)222sin(
)22cos(
)22sin(
/
a
mr
VV
d
GGSZGLWADS
d
d
dd
cbub
The NP solution at has 1-CL < 3%.
9
(Uncertainties are given at 1)
2/BdBd ff 10/
BdBd ff
10/dd BB
Influence of non-pert. hadronic parameters in md
2*22
2
2
)(6
dtbtdtWdBBBF
d rVVxSmBfmG
mdd
• As far as the lattice uncertainties are considered, fBd is the relevant parameter to improve. • A factor 2 has important impact. A factor 10 is not decisive with the current experimental uncertainties of the observables.
10
2/dd BB 10/dd BB
Alternative parametrization of NP in |B|=2
))1(
Im(
)1(22
1
212
12
2
2
d
d
d
id
SM
SM
SL
id
SMd
idd
ehMa
ehArg
mehm
)1( 21212
didSM ehMM
Without and aSL constraints
Isolate the pure NP contributionfrom (SM+NP) terms:
11
With and aSL constraints
Agashe et al. hep-ph/0509117
65.006.008.0
dh
Allowing in addition NP in K-K mixing (I)
00
00
Im
Im
KSMeffHK
KfulleffHK
rK
KK
d
d
d
dd
cbub
r
a
GGSZGLWADS
mr
VV
SL
2
)222sin(
)(
)22cos(
)22sin(
/
45.046.0
09.1
deg1.41.9
8.42
76.025.0
92.02
K
d
d
r
r
12
(1)
Allowing in addition NP in K-K mixing (II)
13
The NP region at 2d=/2 in Bd mixing implies also NP in K mixing corresponding to K< 0
14 NP in Bs mixing Prospective study (I)
s~ can be extracted from
the global Standard Model fit.
The angle governing the mixing in the Bs system is already known to good precision in the SM
sins =
*
*
argtstb
cscbs
VV
VV
15 NP in Bs mixing Prospective study (I)
NP in Bs mixing (B=2 and S=2) is accounted for model-independently through two additional parameters, akin to the Bd system :
00
00
SM
full22
ss
ss
BeffHB
BeffHBs
iesr
KDB
KDB
BJBJB
A
DBm
d
sss
csss
smix
sss
(*)
-1
fromdeg859
fromdeg14572
and / ,/ combinedfrom
028.0036.0)2sin(
fromps 011.0000.20
)22sin(
)22sin(
2
ss
ss
ss mr
• LHCb expected sensitivities correspond to 2 fb-1 (See Talks of O.Schneider & L.Fernandez):
NP in Bs mixing Prospective study (II)16
deg6.17.1
1.02
11.009.0
01.12
s
sr
(1)
)22sin(
)22sin(
)222sin(
ysensitivit LHCb Adding
)(
)22cos(
)22sin(
/
2
2
SL
2
ss
ss
ss
KK
d
d
d
dd
cbub
mr
r
a
GGSZGLWADS
mr
VV
10s
CONCLUSIONS17
• Bd mixing: which room for new physics ? ... Not much.
• K mixing: the only constraint is from k under constrained pb as far as specific NP phase & modulus are considered.
• Bs mixing: LHCb will immediately see NP if O(10°).
APPENDIX
I Main inputs to the fit
|Vub| (average) = (4.15 ± 0.12 ± 0.23).10-3
|Vcb| (incl) = (41.58 ± 0.45 ± 0.58).10-3
|Vcb| (excl) = (41.4 ± 2.1).10-3
|K| = (2.282 ± 0.017).10-3
md = (0.509 ± 0.004) ps-1
sin(2) = 0.687 ± 0.032
S+-= -0.50 ± 0.12
C+- = -0.37 ± 0.10
C00 = -0.28 ± 0.39
B,all charge Inputs to isospin analysisS+-
L = -0.22 ± 0.22C+-
L = -0.02 ± 0.17BL,all charge Inputs to isospin analysisB3 Time dependent Dalits analysis
BD(*) K(*)(-) Inputs to GLW,ADS & GGSZ analysis
mK = (3.490 ± 0.006).10-12 MeV
BK = 0.79 ± 0.04 ± 0.09
mK+ =(493.677 ± 0.016) MeV
fK= 159.8 ± 1.5 MeV
tt= 0.5765 ± 0.0065
ct= 0.47 ± 0.04
B(MS) = 0.551 ± 0.007
fBd√Bd =(223 ± 33 ± 12) MeV
aSL= - 0.0026 ± 0.0067
II measurements
Adding B
22
2
2
22
2
18
)( ubB
B
BBF Vfm
mm
mGBBR
• Powerful in the future for constraining the SM region.• Potential annihilation by means of H+ prevents for considering this input in the analysis.
With md, removethe fB dependence
III