observation of the w b -

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Brad Abbott 1 Observation of the b - Brad Abbott University of Oklahoma On behalf of the DØ Collaboration SLAC January 6, 2009

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Observation of the W b -. Brad Abbott University of Oklahoma On behalf of the D Ø Collaboration. SLAC January 6, 2009. B physics at the Tevatron. Upsilon discovered in 1977 at Fermilab by Lederman et. al. Since then other observations of other B mesons - PowerPoint PPT Presentation

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Page 1: Observation of the  W b -

Brad Abbott 1

Observation of the b-

Brad AbbottUniversity of Oklahoma

On behalf of the DØ Collaboration

SLAC January 6, 2009

Page 2: Observation of the  W b -

Brad Abbott 2

B physics at the Tevatron

• Upsilon discovered in 1977 at Fermilab by Lederman et. al.

• Since then other observations of other B mesons – B+, B0, Bs, Bc

+ (pre Tevatron RunII)

– B* (pre Tevatron RunII), – Bd**(Tevatron RunII)– Bs** (Tevatron RunII)

• Little experimentally known about B baryons

• Only one B baryon known for many years

Summer 1977

Page 3: Observation of the  W b -

Brad Abbott 3

B baryonsCounting only quark content 15 b baryons are expected

Charmless b baryons multiplet

Page 4: Observation of the  W b -

Brad Abbott 4

B baryons more recently

• Prior to Run II only 1 b baryon, b(udb), was considered observed (b J/ )

• However in last 2 years 4 new b baryons have been discovered b

+(uub) b-(ddb) (CDF, 2007)

b-(dsb) (D0/CDF 2007)

b-(ssb) (D0 2008)

Page 5: Observation of the  W b -

Brad Abbott 5

(*)-b in October 2006

CDF announces the observation of the b’s with 1.1 fb-1

PRL 99, 202001 (2007)

Page 6: Observation of the  W b -

Brad Abbott 6

Last year: --bb observation observation

(syst) (stat) 0.09 0.28 0.09 0.08 -

R

5.5ln2ln2

BS

B

L

LL

Signal Significance:

)/()(

) /()(

JBR

JBRR

bb

bb

PRL 99, 052001 (2007)

M(b-)

5792.9 2.5 (stat) 1.7 (syst) MeV/c2

PRL 99, 052002 (2007)

Signal significance = 7.8

CDF

M(b)=5.774 ± 0.019 GeV

Page 7: Observation of the  W b -

Brad Abbott 7

B baryonsVarious predictions for b baryon masses

“Know” approximately where to look and what decay modes are expected

B quark section large at Tevatron(pp bb) = 150 ub @ √s=2 TeV

(e+e- bb) = 7 nb @ √s=Mz

(e+e- bb) = 1 nb @ √s=M(4S)

However large backgrounds make detection challenging

Page 8: Observation of the  W b -

Brad Abbott 8

Tough environment

BaBar

~ 5 tracks/event

Page 9: Observation of the  W b -

Brad Abbott 9

DataTevatron is running well: ~ 5 fb delivered to D0/CDF

D0 Efficiency high: ~ 4.5 fb recorded by each experiment

This analysis

1.3 fb-1

Page 10: Observation of the  W b -

Brad Abbott 10

DØ detector

Large coverage

No particle ID(limited /K separation)

Unprescaled dimuontriggers at all luminosities

Page 11: Observation of the  W b -

Brad Abbott 11

Triggers

• Entire b physics program based on muon triggers (single and dimuon triggers)

• Do not have bandwidth available to trigger on displaced vertices

• Many b physics analyses use dimuon triggers (unprescaled) and search for J/ decaying to .

• Dimuon triggers have several Hz final rate

Page 12: Observation of the  W b -

Brad Abbott 12

B physics program at DØ

Over 34 papers published/accepted for publicationCP violation in Bs decaysFlavor oscillations in Bs decaysBs Branching ratio of Bs Ds*Ds*Bc meson mass/lifetimeDirect CP violation….For full list seehttp://www-d0.fnal.gov/Run2Physics/WWW/results/b.htm

Page 13: Observation of the  W b -

Brad Abbott 13

B baryons at DØb J/

Aids in understanding momentum scale

Possible biases in reconstruction

Lambda long lived so gives practicein reconstructing long lived particles

Discovered that official processing of data inefficient for tracks with large impactparameterTakes a significant time to reconstruct each event andDØ cannot afford to increase reconstruction time forall events

Page 14: Observation of the  W b -

Brad Abbott 14

Data reprocessing

p

When tracks are reconstructed, a maximum impact parameter is required to increase the reconstruction speed and lower the rate of fake tracks.

But for particles like the b-,

this requirement could result in missing the and proton

tracks from the and - decays

Page 15: Observation of the  W b -

Brad Abbott 15

Reprocessing J/ sample

• Since interesting decays all have a J/ only reconstruct subset of data

• Much smaller sample and can be reconstructed in a reasonable time (few months)

Page 16: Observation of the  W b -

Brad Abbott 16

Increase of reconstruction efficiency

0

SK p

Opening up the IP cut: (Before) ( After )GeV GeV GeV

D0 D0 D0

Page 17: Observation of the  W b -

Brad Abbott 17

Similarities of decays

b J/ b J/

Techniques learned in measuring b led to observation of b in 2007

Apply same idea to searching for b

Use techniques learned from b to help in searching for b

“extra pion”

Page 18: Observation of the  W b -

Brad Abbott 18

Search for the -b(bss)

bss quarks combination Mass is predicted to be

5.94 - 6.12 GeV

0.83<(-b)<1.67 ps

(prediction)

M(-b) > M(b)

Page 19: Observation of the  W b -

Brad Abbott 19

--

b

+

-

-

p

K-

~3 cm

~5 cm

Similar decay topologiesb J/ b J/

Page 20: Observation of the  W b -

Brad Abbott 20

Slight differences

• c() = 7.89 cm• c() = 2.46 cm• Lifetime(b) = 1.42 ps• Lifetime(b)= .84-1.69 ps (predicted)• Mass(b) = 5.792 GeV• Mass(b) = 5.94-6.12 GeV (predicted)

• Much more difficult to reconstruct than

Page 21: Observation of the  W b -

Brad Abbott 21

vs reconstruction →p decays:

– pT(p)>0.7 GeV

– pT()>0.3 GeV

- → decays:– pT()>0.2 GeV

– Transverse decay length>0.5 cm

– Collinearity>0.99

)( p

D0

D0

reconstruction

Black symbols: right sign combinationsGreen/red symbols: wrong sign combinations

Page 22: Observation of the  W b -

Brad Abbott 22

reconstruction

• Need to clean up mass peak

• First clean up peak

• Apply Boosted Decision Trees to further clean up sample

Page 23: Observation of the  W b -

Brad Abbott 23

optimization

Apply a cut on proper decay length significance

( decay length significance > 10)

D0 Before cut

Page 24: Observation of the  W b -

Brad Abbott 24

reconstruction

• Minimum selection cuts: +K vertex

reconstructed– Transverse decay

length significance>4– Proper decay length

uncertainty<0.5 cm

Wrong-sign

events+K+

Right-sign events(+K-)

D0

PDG mass value

Page 25: Observation of the  W b -

Brad Abbott 25

Boosted Decision Trees (BDT)

• 20 input variables and - vertex

quality, decay lengths and decay kinematics

• For training we use MC signal and background from wrong-sign events (J/(K+)).

• Most important variables: pT(K)

pT(p)

pT()

decay length

Page 26: Observation of the  W b -

Brad Abbott 26

- after BDT selection

- signal much

cleaner

D0

Signal yield approximately the sameBackgrounds greatly reduced

Page 27: Observation of the  W b -

Brad Abbott 27

Contamination due to --

• There is a reflection due to assigning a pion as a kaon.

• Remove by requiring M()>1.34.

Page 28: Observation of the  W b -

Brad Abbott 28

- after BDT selection and removing decays

Wrong-sign combination events

Page 29: Observation of the  W b -

Brad Abbott 29

Final b optimization

• Optimized for the efficiency

• Further reduce background (based on level we observe in the wrong-sign combinations.)

• Uncertainty on b proper decay length < .03 cm

b transverse momentum greater than 6 GeV

J/ and in same hemispere

Page 30: Observation of the  W b -

Brad Abbott 30

Mass ResolutionPDGPDG

JJJ MMMMMM ///

= 80 MeV = 34 MeV

“poor man’s” way to reduce mass resolution

Page 31: Observation of the  W b -

Brad Abbott 31

Look where we don’t expect any signal

• After “optimize” J/+ decays by using wrong-sign combination events: <0.03 cm

J/ and in the same hemisphere

pT(J/+)>6 GeV

30 events remain

Page 32: Observation of the  W b -

Brad Abbott 32

Side band control samples

DØ DØ

Page 33: Observation of the  W b -

Brad Abbott 33

Summary of all control samples

No excess is observed in any MC sample after selection criteria applied.

)))((())((/

)))((())((/

))((/0*

pJ

KKJB

pJ

b

S

b

Study known decays using MC samples with statistics larger than data set

Page 34: Observation of the  W b -

Brad Abbott 34

“Open Box” and look at right-sign combinations

Excess of events

79 events selected

Page 35: Observation of the  W b -

Brad Abbott 35

Mass measurement

• Fit:Unbinned log-

likelihood fitGaussian signal, flat

backgroundNumber of

background/signal events are floating parametersNumber of signal events: 17.8 ±

4.9

Mean of the Gaussian: 6.165 ± 0.010(stat) GeV

Width of the Gaussian fixed (MC): 0.034 GeV

Page 36: Observation of the  W b -

Brad Abbott 36

Signal Significance

• Two likelihood fits are performed to estimate the significance:1.Signal + background hypothesis (LS+B)

2.Only background hypothesis (LB)

• We evaluate the significance:

• Significance of the observed signal: 5.4

BS

B

L

LL ln2ln2

Page 37: Observation of the  W b -

Brad Abbott 37

Consistency check: Increase pT(B)

Significance > 6

Page 38: Observation of the  W b -

Brad Abbott 38

Look back plots

D0

D0

See consistent yields

Page 39: Observation of the  W b -

Brad Abbott 39

Another consistency check

We can compare proper decay length of sample with MC sample with a lifetime of 1.54 ps

We do not know the lifetime of the b

We do not have enough events to measure the lifetime of the b

Page 40: Observation of the  W b -

Brad Abbott 40

Alternative Cuts Based Analysis (CBA)

Variable BDT CBApT() (GeV) >0.2 and input to BDT >0.2

pT(p) (GeV) >0.2 and input to BDT >0.7

pT(K) (GeV) input to BDT >0.3

collinearity input to BDT >0.99

Transverse decay length (cm)

input to BDT >0.5

Proper decay length uncertainty (cm)

<0.3 <0.3

Variables selected based on relative importance in BDT

performance

Page 41: Observation of the  W b -

Brad Abbott 41

Cut Based Analysis

Number of signal events: 15.7 ± 5.3

Mean of the Gaussian: 6.177 ± 0.015(stat) GeV

Width of the Gaussian fixed (MC): 0.034 GeV

Signal significance reduced to 3.9 due to increased background

Page 42: Observation of the  W b -

Brad Abbott 42

BDT or Cut Base Analysis

After removing duplicate events and combining analyses we observe 25.5 ± 6.5 events. Significance: 5.4

Cut based and BDT can select different events. Overlap is ~ 50%

Page 43: Observation of the  W b -

Brad Abbott 43

Signal confirmed without BDT.

• BDT vs CBA– Consistent number of

observed signal candidates

– Consistent mass– Consistent

reconstruction efficiencies

– BDT has better background rejection power.

Page 44: Observation of the  W b -

Brad Abbott 44

Systematic uncertainties on the mass

• Fitting models– Linear background instead of flat background gives

negligible change.– Varying the signal Gaussian width between 28 – 40

MeV resulted in a 3 MeV uncertainty• Momentum scale correction:

– Fit to the b mass peak in data gives a 4 MeV uncertainty.

• Event selection:– Varying selection criteria and from the mass shift observed

between the cut-based and BDT analysis gives a 12 MeV uncertainty.

Page 45: Observation of the  W b -

Brad Abbott 45

b mass

M(b)=6.165 ± 0.010(stat) ± .013(stat) GeV

A little on the high side of the predictions1-2

Page 46: Observation of the  W b -

Brad Abbott 46

Production rate

)()(32.080.0)/()(

)/()( 14.022.0 syststat

JBrbf

JBrbf

bb

bb

To determine production rate we normalize to b

)(

)(

)(

)(

)/()(

)/()(

b

b

b

b

bb

bb

N

N

JBrbf

JBrbf

2.06.1)(

)(

b

b

The systematic uncertainty includes contributions from the signal yields as well as selection efficiencies

Determined from MC

Page 47: Observation of the  W b -

Brad Abbott 47

Production rate

8.9)/(

)/(

: (1997) 2799 56, D Rev. Phys. From

J

J

b

b

ps 42.1)( 28.024.0

b

theory

ps 67.1)(83.0 b

ps) 67.1)(( 062.0

ps) 83.0)(( 126.0

)(

)(

b

b

b

b

bf

bf

14.007.0)(

)(

b

b

bf

bf

Spin of b = ½ Spin of b = 3/2

Page 48: Observation of the  W b -

Brad Abbott 48

Summary of b

Number of signal events: 17.8 ± 4.9 (stat) ± 0.8(syst)

Mass: 6.165 ± 0.010(stat) ± 0.013(syst) GeV

Significance= 5.4

arXiv:0808.4142(2008) PRL 101, 232002 (2008)

Page 49: Observation of the  W b -

Brad Abbott 49

Summary of b

14.007.0)(

)(

b

b

bf

bf

Consistent with expectations

)()(32.080.0)/()(

)/()( 14.022.0 syststat

JBrbf

JBrbf

bb

bb

Page 50: Observation of the  W b -

Brad Abbott 50

Future plans

• Reprocess Run IIb data– Lots more data (1.3 pb-1Run IIa vs 3.2 pb-1

Run IIb) – Much higher instantaneous luminosities so

much larger combinatorial background– Layer 0 silicon

• Begin searches for other B baryons

Page 51: Observation of the  W b -

Brad Abbott 51

Other possible B baryons(need a J/ to trigger)

0cb(dcb) 0

c J/ +

cb(ucb) +c J/

0bb(ubb) 0

b J/low rate

-bb(dbb) -

b J/low rate

0cb(scb) 0

c J/

Page 52: Observation of the  W b -

Brad Abbott 52

Backup

Page 53: Observation of the  W b -

Brad Abbott 53

Event display of b candidate

Page 54: Observation of the  W b -

Brad Abbott 54

Boosted Decision Trees (BDT)

• All variables are on - or its decay products.

• For training we use MC signal and background from wrong-sign events (J/(K+)).