/
14/06/11 Jet physics meeting 14/06/11 Jet physics meeting

14/06/11 Jet physics meeting - PowerPoint Presentation

briana-ranney
briana-ranney . @briana-ranney
Follow
371 views
Uploaded On 2016-04-20

14/06/11 Jet physics meeting - PPT Presentation

VKostyukhin 1 Flavour fractions in di jet system VKostyukhin CLapoire MLehmacher Bonn 140611 Jet physics meeting VKostyukhin 2 Some theory 1 Heavy flavour pair creation ID: 285267

kostyukhin jet meeting physics jet kostyukhin physics meeting vertex model flavour data fit analysis light secondary charm probability heavy

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "14/06/11 Jet physics meeting" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

14/06/11 Jet physics meeting

V.Kostyukhin

1

Flavour fractions in di-jet system

V.Kostyukhin

C.Lapoire

M.Lehmacher

Bonn Slide2

14/06/11 Jet physics meeting

V.Kostyukhin

2

Some theory1) Heavy

flavour

pair creation

Heavy

flavour

production can be approximately described by 3 mechanisms

2)

Flavour

exitation heavy flavour from proton sea or alternatively from initial state showers

3

)

Gluon splitting

g

QQ

in final state

parton

showers

Slide3

14/06/11 Jet physics meeting

V.Kostyukhin

3

Some theory

PYTHIA predictions for inclusive b-jet production (b-quark p

>5GeV)

Similar picture for charmSlide4

14/06/11 Jet physics meeting

V.Kostyukhin

4

Some theory

Only

flavour

pair creation mechanism (1) makes back-to-back jet pairs with identical (heavy)

flavours

. Mainly LO process.

Flavour

exitation

(2) and gluon splitting (3) produce back-to-back heavy+light jet pairs. NLO processes.Even flavour pair creation process contribute to heavy+light

back-to-back pair in NLO, see below

QQ pairs – LO dominant

Q+light

pairs – NLO dominant Slide5

14/06/11 Jet physics meeting

V.Kostyukhin

5

Di-jet flavours

Di-jet (

2 leading jets in event back-to-back) analysis model

includes 6 fractions (full set):

UU (

light+light

) ~85%

CC (

charm+charm) ~1% BB (beaty+beaty) ~0.6% BC (

beauty+charm) ~0.3%

BU (

beauty+light

) ~4%

CU (

charm+light

) ~10%

PYTHIA predictionsSlide6

14/06/11 Jet physics meeting

V.Kostyukhin

6

Di-jet flavours analysis

To distinguish

flavours

the kinematical variables from secondary vertices in jet are used. Many variables were considered.

Optimisation

included

Highest sensitivity to jet

flavour

content

Minimal jet p dependenceStability with respect to detector effectsThe final (minimal) choice includes 2 variables:

“Product” variable

“Boost” variableSlide7

14/06/11 Jet physics meeting

V.Kostyukhin

7

Di-jet flavours analysis

To simplify statistical description and template construction both variables are transformed to be in [0.,1.] range.

“Boost” is the only variable which has the extreme values for charm, not for beauty!

The beauty here is between light and charm. Should facilitate charm separation.

“Product” variable

“Boost” variableSlide8

14/06/11 Jet physics meeting

V.Kostyukhin

8

Di-jet analysis model

Variable definitions (8 in total):

fBB

– fraction of b-jet pairs in 2-jet sample

fCC

– fraction of c-jet pairs in 2-jet sample

fBU

– fraction of b-jet plus u-jet in 2-jet sample

fCU

– fraction of c-jet plus u-jet in 2-jet sample

fBC

– fraction of b-jet plus c-jet in 2-jet sample

f

UU=1.-fBB-fBC-fBU-fCC-fCU

- not independent

v

b

– probability

to reconstruct secondary vertex in b-jet

v

c

– probability to reconstruct secondary vertex in c-jet

v

u

– probability to get fake secondary vertex in u-jet

Templates from MC (boost case):

B(b)

– secondary

vertex

boost

distribution for b-jet

C(b)

– secondary vertex boost distribution for c-jet

U(b)

– secondary vertex boost distribution for u-jetSlide9

14/06/11 Jet physics meeting

V.Kostyukhin

9

Di-jet analysis model

Case of

2 reconstructed secondary vertices

in

di

-jet event :

Probability

:

2-dim probability density function for the fit :Slide10

14/06/11 Jet physics meeting

V.Kostyukhin

10

Di-jet analysis model

Case of

single reconstructed secondary vertex

in

di

-jet event :

Probability

:

1

-dim probability density function for the fit :Slide11

14/06/11 Jet physics meeting

V.Kostyukhin

11

Di-jet analysis model

2 fitting procedures

are used in analysis:

and B

 are

templated separately and

parametrised with b-splines (1D fit)Joint  & B distributions are used as templates (2D fit)

2D fit has better statistical accuracy due to explicit correlation treatment, but they may be wrong on data so 1D fit is less biased.

More important

is template construction from JX Monte Carlo data samples influence. Splitting of single process into subsamples (JX) results in highly

nonuniform

errors in templates. E.g. few events from J0(low p

sample) with huge weights fall into several template bins. Then these bins get much higher errors and shifted(!!!) in some cases mean. It’s not known

a priori

how to deal correctly with such bins.

The 2 fitting methods use completely different strategies – 1D approach washes out such shifts due to b-

spline

smoothing, 2D fit accepts them.

1D and 2D analysis procedures are far from 100% correlated and then they are used simultaneously for data fitSlide12

14/06/11 Jet physics meeting

V.Kostyukhin

12

Fast simulation model

Heavy

flavour

fractions are small

 fully simulated jet statistics is not enough for validation of analysis properties (bias, error estimations, etc.).

Fast simulation model is developed

All reconstructed secondary vertices in fully simulated jet events are collected into database as a function of jet p

,  and

flavour. Generation procedure:Jet pair is created according to jet p

,  distributions taken from data.

Jet

flavours

are chosen according to the model fractions

fUU,fBB,fCC,fBC,fCU,fBU

From

flavour

content one decides whether secondary vertex is “reconstructed” in each jet according to model efficiencies v

u

,v

c

,v

b

.

If SV is “reconstructed” – its parameters are taken from database according to jet

p

,  (randomly chosen from nearby region).

Finally the recorded SV parameters are smeared with detector resolution to avoid the repetition of exactly the same numbers in generated events due to a single vertex in database chosen several times. Slide13

14/06/11 Jet physics meeting

V.Kostyukhin

13

Fast simulation model

Fast simulation demonstrated that 2010 statistics is not enough for reliable simultaneous estimation of all 8 model parameters.

Then it was chosen to fix 2 SV reconstruction efficiencies on MC values.

Beauty and charm vertex reconstruction efficiencies are chosen to be fixed because they are most precisely predicted by Monte Carlo.

In our analysis of 2010 data we fit simultaneously

6 model parameters (

v

c

,vb are fixed): light jet fake vertex probability (vu

). five

flavour

fractions (

fBB,fBC,fCC,fCU,fBU

)

Both 1D and 2D models with 6 parameters demonstrate correct behavior with fast simulation (next slides…)Slide14

14/06/11 Jet physics meeting

V.Kostyukhin

14

Fast simulation model

2D fitting model performance with fast simulation (200 tries)Slide15

14/06/11 Jet physics meeting

V.Kostyukhin

15

Fast simulation model

2D fitting model pulls with fast simulation (200 tries)Slide16

14/06/11 Jet physics meeting

V.Kostyukhin

16

Data selection

Jets are selected in ID volume |

|<2.1 to guarantee the performance of vertex reconstruction.

Usual jet cleaning cuts are applied on data.

Anti-

kt

R=0.4 jets are used.

Analysis is done in leading jet p

bins . They are chosen to match ATLAS single jet trigger thresholds.The A-D 2010 periods are used for [40,60] and [60,80] bins with L1 jet trigger. For other bins E-I 2010 periods with EF triggers are used.

Subleading

jet p

is also restricted in analysis to decrease systematic due to p

dependence of templates

. Slide17

14/06/11 Jet physics meeting

V.Kostyukhin

17

Vertex reconstruction efficiencies

The efficiencies are obtained as weighted average over all JX PYTHIA samples. Slide18

14/06/11 Jet physics meeting

V.Kostyukhin

18

Vertex asymmetry

The amount of reconstructed secondary vertices in leading and

subleading

jets is

DIFFERENT

in

di

-jet event.

One of the reasons is the semileptonic

decays of heavy flavours. Jet energy disappears with neutrino, what automatically makes the heavy flavour jet subleading.

Qualitatively described by MC

BUT

DISAGREE(!!!)

with data quantitatively Slide19

14/06/11 Jet physics meeting

V.Kostyukhin

19

Vertex asymmetry

The SV asymmetry is coming from mixed

heavy+light

jet pairs.

Reason of data-MC discrepancy here could be either bad description of

semileptonic

decays in PYTHIA or bad description of gluon splitting (also causes jet energy loss)

Asymmetry is added to the fitting model. The exact reason is unclear (doesn’t seem PYTHIA problem, but…) then for baseline result the asymmetry is fixed on MC values.

Changes due to free asymmetry parameter in the are taken as

systematics.Slide20

14/06/11 Jet physics meeting

V.Kostyukhin

20

Data fit quality

Example: data description in [80,120] GeV bin with 2D fitSlide21

14/06/11 Jet physics meeting

V.Kostyukhin

21

Fit results

Data in each p

bin are fitted with 1D and 2D methods.

Fit results are combined with error dependent weights.

Statistical error in bin is calculated from 1D and 2D errors assuming 100% correlation between them.

First – probability to get fake vertex in light jet :

̶̶̶ data fit

̶̶̶ Monte Carlo (PYTHIA)Leading jet p

 GeVSlide22

14/06/11 Jet physics meeting

V.Kostyukhin

22

Fit results

Fitted

di

-jet

flavour

fractions compared with PYTHIA predictions

̶̶̶ data fit

̶̶̶ Monte Carlo

(PYTHIA)Leading jet p GeVLeading jet p GeV

fUU

fraction is estimated from others

fUU

=1-fBB-fBC-fCC-fBU-fCUSlide23

14/06/11 Jet physics meeting

V.Kostyukhin

23

Fit results

Fitted

di

-jet

flavour

fractions compared with other generators. MC boxes represent statistical errors. At particle jet level MC band should be much more narrow. Slide24

14/06/11 Jet physics meeting

V.Kostyukhin

24

Unfolding to particle jet level

Exists, but requires some final polishing.

That’s why not presented here.

However changes in

flavour

fractions are very small just because they are

ratios

!Slide25

14/06/11 Jet physics meeting

V.Kostyukhin

25

Systematics

Systematic due to SV asymmetry discrepancy between data and MC.

Is checked by leaving free the b-jet asymmetry in the fit.Slide26

14/06/11 Jet physics meeting

V.Kostyukhin

26

Systematics

Systematic due to template shape description.

Done by using templates made from

inclusive

jets.

No

di

-jet selection, much bigger statistics, different production mechanisms.

Different MC statistics produces additional statistical fluctuations, so the average shift for all p

 bins is taken as systematic of give model parameter.

To be completed with another MC generators…Slide27

14/06/11 Jet physics meeting

V.Kostyukhin

27

Systematics

Systematic due to charm and beauty vertex reconstruction efficiencies.

Can be estimated from data using the tight link between these efficiencies and fake vertex probability in light jet.

Due to vertex reconstruction algorithm they are controlled by single parameter. Then data-MC difference in fake vertex probability can be translated to

v

c

/

v

b

uncertainties.They are estimated to be 1.1% for charm and 2% for beauty To be completed with another MC generators…

Changes in results due to simultaneous change of

v

c

by 1.1% and

v

b

by 2% Slide28

14/06/11 Jet physics meeting

V.Kostyukhin

28

Status

The measurements are done and now they are under final polishing.

Systematic needs to be completed with different MC generators. Corresponding MC samples are being processed right now.

Backup note should be finished soon.