matter-antimatter differences using muons
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Matter-Antimatter differences using muons. D Ø Result on anomalous Dimuon Charge Asymmetry using Full Tevatron Data Set. G.Borissov, Lancaster University, UK representing D Ø collaboration CERN seminar Geneva, 29 October 2013. Matter-Antimatter imbalance. - PowerPoint PPT PresentationTRANSCRIPT
Matter-Antimatter differencesusing muons
G.Borissov, Lancaster University, UK
representing DØ collaboration
CERN seminarGeneva, 29 October 2013
DØ Result on anomalous Dimuon Charge Asymmetry using Full Tevatron Data Set
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 2
Matter-Antimatter imbalance
• Mystery of imbalance between matter and antimatter in the universe – one of the big questions which need to be addressed by particle physics
• Understanding CP violation and the mechanisms which produce it may be the key to resolving it– CP violation reflects the differences in properties of particles and
antiparticles
– Essential ingredient to explain the imbalance between matter and antimatter
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 3
CP violation
• CP violation is naturally included in the Standard Model (SM) through the complex phase of the CKM mass mixing matrix– The single apex of the
Unitarity triangle is the best confirmation of the SM mechanism of CP violation
• BUT: CP violation accounted for by the SM is not sufficient to explain the observed imbalance between matter and antimatter
• Searching for new sources of CP violation is important to understand the evolution of our universe and test the SM
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 4
Null Test
• "Null test" is the strategy in this search– Measure CP violation in processes where the SM prediction and its
theoretical uncertainty are expected to be small compared to the experimental sensitivity
• In this case, statistically significant deviation of the experimental result from zero would indicate unambiguously the contribution of new physics
• Like-sign dimuon charge asymmetry is a special kind of null test– Subject of this seminar
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 5
Like-sign dimuon charge asymmetry
– N++, N −− − number of events with two muons of the same charge
• Excluding the detector-related effects, this asymmetry can be produced only by CP-violating processes
• Theoretically well predicted quantity– SM expectation and its uncertainty are smaller than the experimental
sensitivity – sensitive null tests
• Inclusive measurement – Large statistics is available
– As yet unknown sources of CP violation could contribute in this asymmetry
NN
NNA
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 6
• Mixing of neutral B0 or Bs0 mesons:
– Produces CP violation in mixing
Known CP-violating processes
BX
X
0)( sB
0)( sB
mix
)()( 0)(
0)(
0)(
0)( XBBXBB ssss
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 7
• Interference of the B0 (Bs0) decays with and without mixing to the
final state accessible to both
– Produces CP violation in interference of decays with and without mixing
• Example: – D(*)+D(*)− produce both μ+ and μ− , but only μ− contributes to the like-sign
dimuon asymmetry
Known CP-violating processes
0)(
0)( ss BB and
XDDDBB (*)(*)(*)00 )( with
mix
CPf
BX 0)( sB
0)( sB 0
)( sB
))(())(( 0)(
0)(
0)(
0)( CPssCPss fBBfBB
interference
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 8
Physics observables
• Asymmetry generated by CP violation in mixing depends on "wrong sign" semileptonic charge asymmetry aq
sl of Bq0 meson (q=d,s)
• Asymmetry generated by CP violation in interference depends on width difference of the Bq0
meson system ΔΓq / Γq
– ΓL , ΓH are the width of light (L) and heavy (H) mass eigenstates of Bq0 system
– Contribution of Bs0 meson is strongly suppressed
– See: GB, B. Hoeneisen, PRD 87, 074020 (2013)
• We extract these quantities from the measured dimuon asymmetry
sdqXBBXBB
XBBXBBa
qqqq
qqqqq ,;)()(
)()(0000
0000
sl
sdqHqLqq ,;,,
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 9
Measurement overview• Measure raw asymmetry A by simple counting of the like-
charge dimuon events
• Identify all background contributions and measure the background asymmetry Abkg directly in data– Background is, by definition, any process producing the dimuon
charge asymmetry and not related to CP violation
– Difference in the interaction of particles and antiparticles with the detector material is the main source of Abkg
• Determine a model-independent asymmetry ACP as:
bkgCP AAA
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 10
Inclusive muon charge asymmetry
• We also measure the inclusive muon charge asymmetry
– n+ (n−) is the number of detected positive (negative) muons
• Measure the background charge asymmetry abkg of inclusive muons directly in data– Background is, by definition, any process producing the inclusive muon
charge asymmetry and not related to CP violation
• Determine a model-independent asymmetry aCP of inclusive muons as:
nn
nna
bkgCP aaa
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 11
Closure test
• The SM expectation of aCP(SM) is much less than ACP(SM) :
• Consistency of measured aCP = a – abkg with zero provides a stringent closure test of our procedure to measure abkg
• It also validates the procedure to measure Abkg
– Sources of the background asymmetries abkg and Abkg are the same
– Their measurement procedure is also the same
)()( SMASMa CPCP
Large collected statistics of events containing muons (~2×109) allows us to test the agreement between a and abkg
with statistical precision of ~3×10-4
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 12
DØ DetectorKey elements for
this measurement:• Muon system• Muon trigger• Solenoid + Toroid• Tracking with precise
vertex detector• interaction• Polarities of magnets
were regularly reversed• Low punch-through• Wide acceptance up to |η|~2
pp
G.Borissov, Matter-Antimatter differences using muons 13
• Polarities of DØ solenoid and toroid were regularly reversed
• Data samples with different magnet polarities are of about thesame size and are added togetherwith proper weights
• This allows to cancel the first order detector effects in the charge asymmetries – Trajectory of the negative particle becomes
exactly the same as the trajectory of the positive particle with the reversed magnet polarity
Reversal of Magnet Polarities
Changing polarities is an important feature of DØ detector, which reduces significantly systematics
in charge asymmetry measurements
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 14
Previous results• DØ published 3 results on this subject
• Last result published in 2011 with 9 fb-1 (PRD 84, 052007,2011):
– aCP is consistent with zero
– ACP significantly deviates from zero
• Interpreting this result as CP violationin B0
(s) mixing we obtain:
– 3.9 σ deviation from the SM– Contribution from CP violation in interference was not included
in this result
)% (syst) (stat) 093.0172.0787.0( ssls
dsld aCaC
)%063.0067.0276.0(
)%079.0042.0034.0(
CP
CP
A
a
(2011) 052007 84, PRD
1; sdssls
dsld CCaCaC
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 15
New measurement
• Increased luminosity from 9.0 fb-1 to 10.4 fb-1
• Detailed study of the dependence of asymmetry on muon impact parameter (IP)
• Detailed study of the dependence of asymmetry on the muon kinematic parameters (pT ,|η|)
• Alternative method to measure the background contribution– Important cross-check of the previously used method
• Additional CP-violating process is included when interpreting the obtained results– CP violation in interference of decays with and without mixing
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 16
IP dependence• Asymmetry aCP is measured in 3 exclusive IP samples
IP sample
muon IP (μm)
IP=1 0 – 50
IP=2 50 – 120
IP=3 120 – 3000
Inclusive muon sample
IP distributions of one muon in the like-sign dimuon sample when the other muon has IP in the IP=1 (full line), IP=2 (dashed line), and IP=3 (dotted line) range.
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 17
IP dependence
• Asymmetry ACP is measured in 6 non-overlapping samples according to IP1 and IP2 of two muons
IP sample 1st muon IP (μm) 2nd muon IP (μm)
IP1,IP2=11 0 – 50 0 – 50
IP1,IP2=12 0 – 50 50 – 120
IP1,IP2=13 0 – 50 120 – 3000
IP1,IP2=22 50 – 120 50 – 120
IP1,IP2=23 50 – 120 120 – 3000
IP1,IP2=33 120 – 3000 120 – 3000
Like-sign dimuon sample
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 18
(pT , |η|) dependence• Additionally, each IP sample is divided into 9 bins depending on
the muon transverse momentum (pT) and pseudorapidity (η)– General kinematic selection of muons:
• 1.5 < pT < 25 GeV; |η| < 2.2
• pT > 4.2 GeV OR |pZ| > 5.4 GeV
Bin pT (GeV) |η|
1 <5.6 <0.7
2 5.6 – 7.0 <0.7
3 >7.0 <0.7
4 <5.6 0.7 – 1.2
5 >5.6 0.7 – 1.2
6 <3.5 1.2 – 2.2
7 3.5 – 4.2 1.2 – 2.2
8 4.2 – 5.6 1.2 – 2.2
9 > 5.6 1.2 – 2.2
cen
tral
inte
rmed
iate
forw
ard
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 19
Our measurement
• Measure the asymmetry aCP in 3×9 non-overlapping samples of inclusive muon events with different IP and (pT ,|η|)
• Measure the asymmetry ACP in 6×9 samples of like-sign dimuon events with different IP1, IP2 and (pT ,|η|)– Division into the IP samples helps to distinguish between different
CP-violating processes contributing to aCP and ACP
– Background varies considerably in different IP samples
– Division into (pT ,|η|) bins allows a better measurement of background contribution, which can vary significantly in different kinematic regions
– Division into (pT ,|η|) bins also provides a rigorous test of our measurement procedure
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 20
Our measurement
• aCP and ACP are obtained in each in each (pT ,|η|) bin i and in each IP sample :
– Asymmetries ai(IP) and Ai(IP1,IP2) are determined by simple counting of events
– Asymmetries aibkg(IP) and Ai
bkg(IP1,IP2) are measured in data with minimal input from simulation
)IP,(IP)IP,(IP)IP,(IP
(IP)(IP)(IP)
21bkg2121CP
bkgCP
iii
iii
AAA
aaa
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 21
Origin of abkg and Abkg
• The dominant background contribution comes from the charge asymmetry of kaon identified as a muon (K→μ)
• Origin of this asymmetry:– because the reaction K−N→Yπ has no K+N analogue
• K+ meson travels further than K− in the material, and has more chance to – decay K→μν
– punch-through the detector material and produce a signal in muon detector
• Asymmetry of K→μ should be positive
• Asymmetry of π→μ should be significantly smaller– because of the small difference in the (πN) cross section between
positive and negative pions
)()( NKNK N − nucleon
29 October 2013 22
Background asymmetries
• Measure charge asymmetry for each type of particle: aK , aπ , ap
– e.g., aK is measured using kaons from K*0 →K− π+ decay
• Also measure charge asymmetry of muon detection (δ)– using "tag and probe" method and
J/ψ→μ+μ− decay
• Measured directly in data
• Measured in each (pT ,|η|) bin
• Average values:
)%02.013.0(
)%42.343.1(
)%08.006.0(
)%10.010.5(
p
K
a
a
a
central
inte
rmed
iate
forward
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 23
)IP,(IP)IP,(IP)IP,(IP
(IP)(IP)(IP)
21bkg2121CP
bkgCP
iii
iii
AAA
aaa
Background asymmetries
• Background asymmetries in each (pT ,|η|) bin i and each IP sample
– fKi , fπ
i , and fpi are fractions of K→μ, π→μ, p→μ in inclusive muon sample
– FKi , Fπ
i , and Fpi are fractions of K→μ, π→μ, p→μ in dimuon sample
– aμi , Aμ
i are the charge asymmetries of muon detection
iip
ip
iiik
ik
ibkg
iip
ip
iiik
ik
ibkg
AaFaFaFA
aafafafa
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 24
Background fractions
• K→μ, π→μ, p→μ are produced mainly in light quark and gluon jets
• Therefore, their tracks originate from the primary interaction point
• Muons from b-quark decay often have large IP
• Background fractions should decrease significantly in the sample with large IP (IP=3)
),,(
)()()(
sduq
XbbppggXppXqqpp
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 25
Charge asymmetry of inclusive muons aCP
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 26
Background fractions
• Measured directly in data
• Measure in each (pT ,|η|) bin and in each IP sample
• Alternative independent method is used to cross check the measurement
• Background vary by a factor >7 between IP=1 (low IP) and IP=3 (high IP)
– Only statistical uncertainties are shown
IP=1 IP=2 IP=3
fK, (%) 20.30±0.34 7.71±0.24 2.69±0.14
fπ, (%) 39.13±2.09 15.39±0.83 5.32±0.30
fp, (%) 0.73±0.21 0.28±0.09 0.08±0.09
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 27
Contributions to Background asymmetry
– Only statistical uncertainties are given
• Contribution from K→μ dominates in the samples with low IP
• Background is considerably reduced for IP=3
• For IP=3 the kaon and muon detection asymmetries have approximately the same magnitude
IP=1 IP=2 IP=3
K→μ (%) +1.037±0.029 +0.385±0.017 +0.134±0.010
π→μ (%) −0.022±0.040 −0.019±0.016 −0.007±0.006
p→μ (%) −0.010±0.012 −0.004±0.005 −0.001±0.001
aμ (%) −0.050±0.009 −0.102±0.017 −0.128±0.021
abkg (%) +0.954±0.053 +0.250±0.027 −0.001±0.023
a (%) +0.930±0.003 +0.277±0.006 −0.049±0.005
29 October 2013 28
Asymmetry aCP
• Raw asymmetry is large for IP=1 sample
• Background asymmetryexplains it
• aCP is consistent with zero for all IP samples
(IP)(IP)(IP) bkgCP aaa
Sample a (%) abkg (%) aCP (%)
All IP +0.670±0.002 +0.702±0.042 −0.032±0.042±0.061
IP=1 +0.930±0.003 +0.954±0.053 −0.024±0.053±0.075
IP=2 +0.277±0.006 +0.259±0.027 +0.018±0.028±0.024
IP=3 −0.049±0.005 −0.001±0.023 −0.048±0.024±0.011
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 29
SM expectation
• SM expectation for the inclusive muon asymmetry aCP is ~10-5
• It is strongly suppressed by the large fraction of non-CP violating processes contributing to the inclusive muon sample– e.g. c→μX or b→μX without oscillation
• Consistency of aCP with zero is an important "closure test" to verify our procedure of background measurement
We observe this consistency in all IP samples, while the raw asymmetry varies considerably and even changes the sign
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 30
Closure test: IP=1
• Test consistency with zero of ai
CP for all (pT ,|η|) bins
• Raw asymmetry varies by more than 1.5%
• Background asymmetry abkg explains these variations
• Asymmetry aCP is consistent with zero within 0.05%
χ2=7.54/8 d.o.f
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 31
Closure test: IP=2
• Test consistency with zero of ai
CP for all (pT ,|η|) bins
• Raw asymmetry varies by more than 1%
• Background asymmetry abkg explains these variations
• Asymmetry aCP is consistent with zero within 0.03%
χ2=3.48/8 d.o.f
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 32
Closure test: IP=3
• Test consistency with zero of ai
CP for all (pT ,|η|) bins
• Raw asymmetry varies by more than 0.5%
• Background asymmetry abkg explains these variations
• Asymmetry aCP is consistent with zero within 0.05%
χ2=10.8/8 d.o.f
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 33
Conclusions on aCP
• Measurement of aCP confirms a validity of our procedure of background measurement– Background varies considerably in different (pT ,|η|) bins
– Background changes by a factor >7 between different IP samples
– Still we get a consistent result: a and abkg agree within 0.03%
• This closure test validates our procedure of the background measurement
• Provides confidence in the measurement of like-sign dimuon asymmetry ACP where the same method of background measurement is used
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 34
Charge asymmetry of like-sign dimuons ACP
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 35
Dependence on (pT ,|η|)
• There is an overall deviationfrom zero of ACP
– This value is shown in the last bin
– Only statistical uncertainties are shown in the plot
• Raw asymmetry A varies considerably in (pT ,|η|) bins
• Asymmetry Abkg explains thesevariations
2 entries per each dimuon event
)%055.0064.0235.0()IP all( CPA
χ2=7.6/8 d.o.f
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 36
Measurements in IP samples
χ2=6.8/8 d.o.f
χ2=5.0/8 d.o.f
χ2=5.0/8 d.o.f
χ2=5.8/8 d.o.f
χ2=7.5/8 d.o.f
χ2=3.5/8 d.o.f
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 37
Measurements in IP samples• Same pattern is observed for the
measurements in different IP1, IP2 samples
– good stability of ACP in (pT ,|η|) bins
– Overall shift of ACP
• Deviation from zero of the combination of all our asymmetrymeasurements (3 aCP and 6 ACP) is
9/5.36d.o.f./2
Strong evidence (4.1 σ) of non-zero charge asymmetry
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 38
Stability in time
• We published several papers on the dimuon asymmetry
• The result on the residual dimuon asymmetry is very stable – Change of luminosity 1.0 → 10.4 fb-1
– Change of the analysis method
arXiv:1310.0447[hep-ex]
PRD74, 092001 (2006)
PRD82, 032001 (2010)
PRD84, 052007 (2011)
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 39
Comparison with the SM• Two SM contributions to the dimuon asymmetry are expected:
– CP violation in mixing– CP violation in interference of decays with and without mixing
• Second contribution is dominant– For all IP:
– The second contribution was established just recently [ GB, B. Hoeneisen, PRD 87, 074020 (2013) ]
– It was not considered in our previous publications
4int4mix
int5mix
10)8.05.3()(;10)1.08.0()(
0)(;10)2.08.0()(
SMASMA
SMaSMa
CPCP
CPCP
)()()(
)()(intmix
mix
SMASMASMA
SMaSMa
CPCPCP
CPCP
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 40
Comparison with the SM
• Comparing 9 measurements (3 measurements of aCP and 6 measurements of ACP) with the SM prediction we get:
3.6 standard deviations from the SM prediction
9/0.31d.o.f./2
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 41
Interpretation• If we assume that the measured charge asymmetries are produced
by CP violation in mixing and CP violation in interference, we can extract ad
sl, assl, and ΔΓd/Γd
– Asymmetries depend linearly on them
– Coefficients Kd, Ks, and KΓ are different in different IP sub-samples
– These coefficients are determined using the MC input and measured quantities
d
dss
dd
ss
dd
KaKaKA
akaka
)IP,IP()IP,IP()IP,IP()IP,IP(
)IP()IP()IP(
21sl21sl2121CP
slslCP
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 42
Results
• We get:
– deviates from the SM prediction by 3.0 σ
• Result is consistent with independent DØ measurements of– ad
sl : PRD 86, 072009 (2012)
– assl : PRL 110, 011801 (2013)
)%38.150.0(
)%99.082.0(
)%43.062.0(
d
d
ssl
dsl
a
a
muon asymmetry 66.0
03.0
61.0
,
,
,
s
d
sd
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 43
Impact of ΔΓd / Γd
• The contribution of CP violation in interference depends on the value of ΔΓd / Γd
• This quantity is measured experimentally with poor precision
• SM expectation:
• Contrarily to other quantities, NP contribution to ΔΓd / Γd is not experimentally constrained yet
210)8.15.1(( WA),experimentd
d
210)08.042.0(SM)( d
d
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 44
Example of impact of ΔΓd / Γd
• Deviation from SM is sensitive to the value of ΔΓd / Γd
• Using the WA value of ΔΓd / Γd instead of the SM, we get:
– In this example the deviation from the SM prediction for ad
sl , assl is 1.9 σ
(fixed) 0150.0
79.0
)%74.035.0(
)%42.062.0(
,
d
d
sd
ssl
dsl
a
a
Independent measurements of ΔΓd / Γd are required
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 45
Combination with other DØ results
• Combining our 3 results (see figure) we get more precise values:
– Deviates from the SM prediction by 3.1 σ
• The measurements are consistent– χ2/d.o.f. = 4.4/2
)%15.179.0(
)%58.033.1(
)%29.009.0(
d
d
ssl
dsl
a
a
The most precise measurement of these quantities so far in a single experiment
55.0
24.0
34.0
,
,
,
s
d
sd
G.Borissov, Matter-Antimatter differences using muons 46
Comparison with other experiments
• Other measurementsBaBar, Belle: ad
sl PRL 111, 101802 (2013), HFAG, arXiv:1207.1158 [hep-ex]
LHCb: assl arXiv:1308.1048 [hep-ex]
Belle: ΔΓd / Γd PRD 85, 071105 (2012)
• Our combination of all world results gives:
– Deviates by 2.9 σ from the SM prediction
• Good consistency of all measurements– χ2/d.o.f. = 4.3/3
)%91.051.1(
)%43.083.0(
)%21.009.0(
d
d
ssl
dsl
a
a
47.0
23.0
25.0
,
,
,
s
d
sd
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 47
Conclusions• Measurements of aCP and ACP in
different IP samples are obtained
• Evidence with confidence 4.1 σ of deviation of muon asymmetry from zero
• Our results deviate from the SM prediction by 3.6 σ
• Available in arXiv: 1310.0447[hep-ex]
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 48
Backup slides
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 49
Measurement of kaon asymmetry
• Define sources of kaons:
• Require that the kaon is identified as a muon
• Build the mass distribution separately for positive and negative kaons
• Compute asymmetry in the number of observed events
KK
KK
)1020(
0*
→ K+ K− decay
N(K+→μ+) + N(K−→μ−)
N(K+→μ+) − N(K−→μ−)
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 50
Alternative method to measure background
• Up to now we used the fraction of K*0 to measure the fraction of K→μ events in our sample (K*0 method)
• Recently we developed an independent method to measure background using local muon variables (LV method)
• Background muons come from K→μν and π→μν decays
• When we reconstruct a muon, the charged track in the central tracker is associated with the local track in the muon detector
• If a muon comes from kaon or pion decay, the track parameters of the central track and local track are different
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 51
Local variables• Distribution of local variables is significantly different for
signal (S muons) and background (L muons)
• It is very similar for K→μ and π→μ because of similar origin
centrallocal PPX / |)()(| centrallocalY
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 52
Measuring the fraction of background
• Use the templates for L muons and S muons to measure the total background fraction
• Templates are obtained in data
• Background fraction is measured independently for each (pT, |η|) bin
• Here the example of the fit for bin 2 is presented
• Ratio π/K is fixed to the expected value
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 53
Comparison of two methods• Use local variables (LV) of muon detector to measure background
• Compare it with the "K*0" method used so far in the dimuon papers
• Very good agreement between two methods, including the IP dependence
• Uncertainties for both methods do not include the systematics
• Systematics for two methods is different and independent
Method All IP IP=1 IP=2 IP=3
Local variables (%) 42.56±0.87 55.10±0.94 22.73±1.15 8.51±0.14
K*0 method (%) 46.73±1.76 60.19±2.21 23.38±1.01 8.09±0.47
relative difference (%)
−8.92±3.90 −8.46±3.71 −2.78±6.47 5.19±6.35
Background fraction in the inclusive muon sample
LV method is used as an important cross check of the K*0 method, providing the estimate of its systematic uncertainty
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 54
World Average Inputs• Direct measurements of as
sl= (-0.50 ± 0.52)%
– D0: Phys. Rev. Lett., 110, 011801 (2013) assl= (-1.12 ± 0.76)%
– LHCb: arXiv:1308.1048 assl= (-0.06 ± 0.63)%
• Direct measurements of adsl= (+0.23 ± 0.26)%
– Previous B-Factory Results (HFAG) adsl= (-0.05± 0.56)%
– D0: Phys. Rev. D 86, 072009 (2012) adsl= (+0.68± 0.47)%
– New BaBar: Phys. Rev. Lett. 111, 101802 (2013) adsl= (+0.06 ± 0.38)%
• Direct Measurement of ΔΓ/Γ = (+1.5± 1.8)%– Previous B-Factory Results (HFAG)
• Combined with the muon asymmetries using 3-dimensional χ2 minimisation and the correlations.
29 October 2013 G.Borissov, Matter-Antimatter differences using muons 55
WA Combination Plots