Study of Higgsinvisible using kinematic fit method applied jet - - PowerPoint PPT Presentation

study of higgs invisible using kinematic fit method
SMART_READER_LITE
LIVE PREVIEW

Study of Higgsinvisible using kinematic fit method applied jet - - PowerPoint PPT Presentation

Study of Higgsinvisible using kinematic fit method applied jet energy resolution of ILD Yu Kato, J.Tian, T.Tanabe, S.Yamashita The Univ. of Tokyo The 55 th General Meeting of ILC Physics Subgroup Feb. 3, 2018 2018/2/3 Outline Study of


slide-1
SLIDE 1

Study of Higgs→invisible using kinematic fit method applied jet energy resolution of ILD

Yu Kato, J.Tian, T.Tanabe, S.Yamashita The Univ. of Tokyo

The 55th General Meeting of ILC Physics Subgroup Feb. 3, 2018

slide-2
SLIDE 2

Outline

pMotivation pIdea for improvement pFlow of study

uEvaluate jet energy resolution ukinematic fit uAnalysis Higgs→invisible

pSummary & Plans

2018/2/3

Study of Higgs->invisible using kinematic fit 2

slide-3
SLIDE 3

lIn SM, Higgs decays invisibly through H → ZZ∗ → 4𝜉 (BR(H → 𝑗𝑜𝑤.)~0.1%) lIf BR(H → 𝑗𝑜𝑤.) exceeds SM prediction , it signifies new physics beyond SM (BSM) lWe estimate SM upper limit of BR(H → 𝑗𝑜𝑤.) lCompare result between left & right polarization

Motivation

2018/2/3

Study of Higgs->invisible using kinematic fit 3

q q

BSM

X X

invisible

Dark Matter… SUSY…

visible 𝐶𝑆 H → XX ~? ? ? %

q q Z Z ν ν ν ν

𝐶𝑆 H → ZZ∗ → 4𝜉 ~0.1% invisible visible Ø A. Ishikawa (Tohoku Univ.), ”Search for Invisible Higgs Decays at the ILC” LCWS2014@Belgrade

Previous study(A.Ishikawa) (95% CL, 250fb-1) left pol. : right pol. 0.95% : 0.69%

slide-4
SLIDE 4

Idea for improvement

2018/2/3

Study of Higgs->invisible using kinematic fit 4

Improve analysis performance

kinematic fit

apply jet energy resolution

method

slide-5
SLIDE 5

Flow of study

Evaluate jet energy resolution

ILD model : ILD_l(s)5_v02 Ø jet energy & cosθ dependence evaluate jet angle resolution also → apply to kinematic fit

kinematic fit

fit variables : constraint : use MarlinKinfit - fitter engine : OPALFitter apply jet resolution Ø check effect & accuracy of fit

Improve analysis performance [BSM search using Higgs→invisible]

2018/2/3

Study of Higgs->invisible using kinematic fit 5

slide-6
SLIDE 6

2018/1/17

ILC実験におけるジェットエネルギー分解能評価 及び kinematic fit 手法の研究 6

Evaluate jet energy resolution

slide-7
SLIDE 7

lILCSoft : v01-19-05 (gcc49) lILDConfig : v01-19-05-p01 lILD models : ILD_l5_o1_v02, (ILD_s5_o1_v02) lsamples : Z→uds (w/o overlay) l jet resolution definition

  • use RMS90 method
  • Energy

𝜏9 𝐹 = RMS90 𝐹

?

𝑛𝑓𝑏𝑜CD 𝐹

?

= 2

  • RMS90 𝐹

??

𝑛𝑓𝑏𝑜CD 𝐹

??

(J. S. Marshall and M. A. Thomson, ”Pandora Particle Flow Algorithm”, arXiv:1308.4537 [physics.ins-det])

  • Angle

𝜀𝜚 = RMS90(𝜚IJK − 𝜚MK) 𝜀𝜄 = RMS90(𝜄IJK − 𝜄MK)

2018/2/3

Study of Higgs->invisible using kinematic fit 7

Setting of Evaluation JER

√s [GeV]

30 40 60 91 120 160 200 240 300 350 400 500 l5 [events] 10k 10k 10k 10k 10k 10k 10k 10k 9k 10k 9k 10k s5 [events] 10k 10k 10k 10k 9k 10k 10k 9k 10k 10k 10k 10k

use jet clustering: Durham

Evaluate JER

slide-8
SLIDE 8

ILD model Detailed Baseline Design

2018/2/3

Study of Higgs->invisible using kinematic fit 8

Endcap Barrel θ

ILD_l5_v02 ILD_s5_v02

Evaluate JER

slide-9
SLIDE 9

Result:Energy dependence

2018/2/3

Study of Higgs->invisible using kinematic fit 9

[GeV]

j

E

50 100 150 200 250

) [%]

j

(E

90

) / Mean

j

(E

90

RMS

3 4 5 6 7

sv01-19-05.mILD_l5_o1_v02_nobg

/E = 3.5%

E

σ E /E = 30%/

E

σ Overall :

j

E

  • 1.97 +0.200

j

E 31.3/ | < 0.7 θ Barrel : |cos

j

E

  • 1.91 +0.195

j

E 28.9/ 0.7 ≥ | θ Endcap : |cos

j

E

  • 1.66 +0.184

j

E 33.6/

Evaluate JER

slide-10
SLIDE 10

Result : energy & angle dependence

2018/2/3

Study of Higgs->invisible using kinematic fit 10

| θ |cos

0.2 0.4 0.6 0.8 1

) [%]

j

(E

90

) / Mean

j

(E

90

RMS

5 10 15

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

apply this result to kinematic fit Evaluate JER

slide-11
SLIDE 11

| θ |cos

0.2 0.4 0.6 0.8 1

MC

φ

  • REC

φ = φ δ

0.05 0.1 0.15 0.2 0.25 0.3

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

Angular resolution

2018/2/3

Study of Higgs->invisible using kinematic fit 11

𝜀𝜚 = 𝑆𝑁𝑇CD 𝜚IJK − 𝜚MK 𝜀𝜄 = 𝑆𝑁𝑇CD(𝜄IJK − 𝜄MK)

polar angle azimuth angle

| θ |cos

0.2 0.4 0.6 0.8 1

MC

θ

  • REC

θ = θ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

Durham algorithm

Evaluate JER

For evaluation of angular resolution, use jet clustering.

apply this result to kinematic fit

slide-12
SLIDE 12

2018/1/17

ILC実験におけるジェットエネルギー分解能評価 及び kinematic fit 手法の研究 12

kinematic fit

slide-13
SLIDE 13

Principle of kinematic fit

2018/2/3

Study of Higgs->invisible using kinematic fit 13

seek minimum of under kinematic constraints method of Lagrange multipliers d.o.f.:

kinematic fit

slide-14
SLIDE 14

MarlinKinfit : OPALFitter

2018/2/3

Study of Higgs->invisible using kinematic fit 14 For iterative solution : Taylor-expansion of the constraints

Convergence condition ü 𝜀𝜓R < 0.01% ∩ 𝜀𝐺

V < 10WX

∩ 𝐺

V < 10WR Y 𝜓R

  • r

ü all 𝑔

[ < 10W\ ∩ 𝜀 𝜃, 𝜊, 𝜇 < 10W\

kinematic fit

slide-15
SLIDE 15

ZH processor

pFit variables pZ mass constraint pjet mass constraint pImplement of jet resolution pdegrees of freedom

2018/2/3

Study of Higgs->invisible using kinematic fit 15

| θ |cos

0.2 0.4 0.6 0.8 1

) [%]

j

(E

90

) / Mean

j

(E

90

RMS

5 10 15

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

MC

θ

  • REC

θ = θ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

MC

φ

  • REC

φ = φ δ

0.05 0.1 0.15 0.2 0.25 0.3

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

q q X X

invisible !" H → XX ~???%

kinematic fit

slide-16
SLIDE 16

Result:accuracy of fit

2018/2/3

Study of Higgs->invisible using kinematic fit 16

2

χ

500 1000 1500 2000

Events / 2.00

1 10

2

10

3

10

4

10

sv01-19-05.mILD_o1_v05.eL.pR

OPALFitter fit success : 99.85 % mean = 14.453 sigma = 46.970

sv01-19-05.mILD_o1_v05.eL.pR

fit probability

Fit Probability

0.2 0.4 0.6 0.8 1

Events / 0.01

2

10

3

10

4

10

sv01-19-05.mILD_o1_v05.eL.pR

OPALFitter fit success : 99.85 % mean = 0.278 sigma = 0.313

sv01-19-05.mILD_o1_v05.eL.pR

←peak around0

fit with well-estimated errors →normal distributed between 0 and 1

a possibility of underestimating parameter error χ2 distribution

Mean:14.5 Ndof :1 Mean > Ndof

kinematic fit

slide-17
SLIDE 17

Result:Recoil mass

2018/2/3

Study of Higgs->invisible using kinematic fit 17 Recoil Mass [GeV]

100 110 120 130 140 150 160

Events / 0.50 GeV

200 400 600

sv01-19-05.mILD_o1_v05.eL.pR

OPALFitter success : 99.85 %

before fit: mean = 130.1 sigma = 12.076 after fit: mean = 129.0 sigma = 10.496 Recoil Mass [GeV]

100 110 120 130 140 150 160

Events / 0.50 GeV

1000 2000 3000 4000

sv01-19-05.mILD_o1_v05.eL.pR

MC: mode = 125.2 sigma = 6.379

OPALFitter success : 99.85 %

sv01-19-05.mILD_o1_v05.eL.pR

Recoil Mass Relative Error

1 − 0.5 − 0.5 1

Events / 0.01

200 400 600 800 1000 1200

sv01-19-05.mILD_o1_v05.eL.pR

OPALFitter success : 99.85 %

before fit: mean = 8.4e-03 sigma = 8.8e-02 after fit: mean = -3.3e-04 sigma = 6.9e-02

sv01-19-05.mILD_o1_v05.eL.pR

↓ISR effect

improve recoil mass resolution ~20%

kinematic fit

slide-18
SLIDE 18

Problems : Z mass distribution

2018/2/3

Study of Higgs->invisible using kinematic fit 18

[GeV]

Z

M

70 80 90 100 110 120

Events / 0.50 GeV

1 10

2

10

3

10

4

10

sv01-19-05.mILD_o1_v05.eL.pR

OPALFitter success : 99.85 %

MC: mean = 90.9 sigma = 5.338 before fit: mean = 90.7 sigma = 10.091 after fit: mean = 91.3 sigma = 1.271

Error???

kinematic fit

slide-19
SLIDE 19

the Cause:

2018/2/3

Study of Higgs→invisible using kin-fit applied JER of ILD 19

kinematic fit

[GeV]

Z

M

70 80 90 100 110 120

Events / 0.50 GeV

1 10

2

10

3

10

4

10

sv01-19-05.mILD_o1_v05.eL.pR

NewtonFitter success : 99.35 %

MC: mean = 90.9 sigma = 5.486 before fit: mean = 90.4 sigma = 9.516 after fit: mean = 91.2 sigma = 0.077

[GeV]

Z

M

70 80 90 100 110 120

Events / 0.50 GeV

1 10

2

10

3

10

4

10

sv01-19-05.mILD_o1_v05.eL.pR

OPALFitter success : 99.85 %

MC: mean = 90.9 sigma = 5.338 before fit: mean = 90.7 sigma = 10.091 after fit: mean = 91.3 sigma = 1.271

OPALFitter NewtonFitter Approximate calculation of constraint in OPALFitter

slide-20
SLIDE 20

2018/1/17

ILC実験におけるジェットエネルギー分解能評価 及び kinematic fit 手法の研究 20

Search for BSM using H→invisible

slide-21
SLIDE 21

Analysis

lSimulation set up

  • Generator: WHIZARD 1.95
  • Samples: DBD sample + Dirac sample ( ebeW → qqH, H → ZZ∗ → 4ν )
  • Detector: ILD full simulation ( ILD_o1_v05 )
  • 𝑡
  • = 250 GeV, ∫𝑀𝑒𝑢 = 250 fb-1 , 𝑄

Jj, 𝑄Jk = −0.8, +0.3 , (+0.8, −0.3)

lFlow of analysis

1. Reconstruction : “PandoraPFA”

  • Isolated lepton tagging

2. 2 jet clustering : “Durham algorithm”

  • Forced 2 jet clustering
  • 3. kinematic fit

4. Event selection

  • Assume BR(H→invisible) = 10%

5. Estimate upper limit of BR.

  • Template method: BR(H→invisible) = [1,2,…10%]

2018/2/3

Study of Higgs->invisible using kinematic fit 21

“Left” “Right”

Higgs→invisible

slide-22
SLIDE 22

Signal

ü2jet & missing E ü𝑁oo ≈ 𝑁q : 𝐶𝑆 Z → 𝑟𝑟 ~70% ü𝑁IJKt[u ≈ 𝑁v[wwx üs channel process

2018/2/3

Study of Higgs->invisible using kinematic fit 22

q q X X

invisible 𝐶𝑆 H → XX ~? ? ? %

Main background

ZZ semi-leptonic WW semi-leptonic ννZ semi-leptonic

Higgs→invisible

slide-23
SLIDE 23

Cut table

𝑄

Jj, 𝑄Jk = −0.8, +0.3

2018/2/3

Study of Higgs->invisible using kinematic fit 23

w/o kinematic fit w/ kinematic fit

Higgs→invisible

cut condition cut condition cut condition S/√S+B S/√S+B S/√S+B signal signal signal all bkg all bkg all bkg common part common part

slide-24
SLIDE 24

Cut table

𝑄

Jj, 𝑄Jk = +0.8, −0.3

2018/2/3

Study of Higgs->invisible using kinematic fit 24

w/o kinematic fit w/ kinematic fit

Higgs→invisible

cut condition cut condition cut condition S/√S+B S/√S+B S/√S+B signal signal signal all bkg all bkg all bkg common part common part

slide-25
SLIDE 25

[GeV]

kf recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

500 1000 1500 2000 2500

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (-0.8,+0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/ kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

[GeV]

kf recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

200 400 600 800

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (+0.8,-0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/ kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

[GeV]

recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

500 1000 1500 2000 2500

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (-0.8,+0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/o kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

[GeV]

recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

200 400 600 800

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (+0.8,-0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/o kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

2018/2/3

25

Left polarization Right polarization

Study of Higgs->invisible using kinematic fit

Result:Recoil mass distribution

significance=15.54 significance=20.81 significance=19.72 significance=16.26 w/o kinematic fit w/ kinematic fit

Higgs→invisible

slide-26
SLIDE 26

[GeV]

kf recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

500 1000 1500 2000 2500

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (-0.8,+0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/ kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

[GeV]

kf recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

200 400 600 800

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (+0.8,-0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/ kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

[GeV]

recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

500 1000 1500 2000 2500

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (-0.8,+0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/o kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

[GeV]

recoil

M

100 110 120 130 140 150 160

Events / 2.00 GeV

200 400 600 800

, Cut: No.1~No.9

  • 1

dt = 250 fb L

) = (+0.8,-0.3),

+

,Pe

  • = 250 GeV, (Pe

s

w/o kinematic fit inv. → H BR = 10% qqH,SM ZZ WW Z ν ν

  • ther bkg

2018/2/3

26

Left polarization Right polarization

Study of Higgs->invisible using kinematic fit

Result : Upper limit of BR (95% CL)

UL=0.89±0.44% UL=0.59±0.29% UL=0.63±0.32% UL=0.84±0.42% w/o kinematic fit w/ kinematic fit

Higgs→invisible

slide-27
SLIDE 27

Summary

2018/2/3

Study of Higgs->invisible using kinematic fit 27

Recoil Mass [GeV]

100 110 120 130 140 150 160

Events / 0.50 GeV

200 400 600

sv01-19-05.mILD_o1_v05.eL.pR

OPALFitter success : 99.85 %

before fit: mean = 130.1 sigma = 12.076 after fit: mean = 129.0 sigma = 10.496

| θ |cos

0.2 0.4 0.6 0.8 1

) [%]

j

(E

90

) / Mean

j

(E

90

RMS

5 10 15

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

UL of BR [%] (95%CL) Left polarization Right polarization Previous study 0.95 0.69 w/o kinematic fit 0.89±0.44 0.63±0.32 w/ kinematic fit 0.84±0.42 0.59±0.29

Evaluate jet energy resolution

ILD model : ILD_l(s)5_v02 Ø jet energy & cosθ dependence evaluate jet angle resolution also → apply to kinematic fit

kinematic fit

fit variables : constraint : MarlinKinfit : OPALFitter apply jet resolution

Higgs→invisible

Estimate upper limit of BR(H→inv.) Check effect by kinematic fit

slide-28
SLIDE 28

今後の課題

ジェットエネルギー分解能評価

  • エンドキャップ部分のより精細な評価 ← 統計量の増加
  • cジェット、bジェット評価の追加
  • ジェットクラスタリングを用いた評価:
  • ジェット質量(または運動量)依存性の追加

kinematic fit

  • フィッティング精度の改善:分解能をスケールする
  • soft constraintの実装:Zボソンの自然幅を考慮
  • 他の物理過程への応用

Higgs→invisible崩壊分岐比の上限推定

  • 反跳質量以外のフィット後の変数を事象選別に使用
  • 推定に用いる反跳質量領域の最適化
  • より高度な手法を用いて上限評価

ex.) profile likelihood ratio

2018/2/3

Study of Higgs->invisible using kinematic fit 28

slide-29
SLIDE 29

backup

2018/2/3

Study of Higgs->invisible using kinematic fit 29

slide-30
SLIDE 30

2018/2/3

Study of Higgs→invisible using kin-fit applied JER of ILD 30

slide-31
SLIDE 31

2018/2/3

Study of Higgs->invisible using kinematic fit 31

slide-32
SLIDE 32

2018/2/3

Study of Higgs->invisible using kinematic fit 32

slide-33
SLIDE 33

Angular resolution

2018/2/3

Study of Higgs->invisible using kinematic fit 33

𝜀𝜚 ∗ 𝑡𝑗𝑜𝜄 = 𝑆𝑁𝑇CD{ 𝜚IJK − 𝜚MK 𝑡𝑗𝑜𝜄} 𝜀𝜄 = 𝑆𝑁𝑇CD(𝜄IJK − 𝜄MK)

polar angle azimuth angle

| θ |cos

0.2 0.4 0.6 0.8 1

θ *sin φ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

MC

θ

  • REC

θ = θ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

Durham algorithm

Evaluate JER

For evaluation of angular resolution, use jet clustering.

apply this result to kinematic fit

slide-34
SLIDE 34

Compare with

2018/2/3

Study of Higgs->invisible using kinematic fit 34

| θ |cos

0.2 0.4 0.6 0.8 1

) [%]

j

(E

90

) / Mean

j

(E

90

RMS

5 10 15

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

) [%]

j

(E

90

) / Mean

j

(E

90

RMS

5 10 15

sv01-19-05.mILD_s5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

[GeV]

j

E

50 100 150 200 250

) [%]

j

(E

90

) / Mean

j

(E

90

RMS

3 4 5 6 7

|<0.7 θ sv01-19-05 |cos

mILD_l5_o1_v02_nobg

j

E

  • 1.91 +0.195

j

E 28.9/ mILD_s5_o1_v02_nobg

j

E

  • 1.59 +0.199

j

E 27.6/ /E = 3.5%

E

σ

エネルギー分解能の定義 RMS90 ヒストグラム内の90%の事象が含まれる 最小の領域における標準偏差を用いる ILD_l5_v02 ILD_s5_v02

slide-35
SLIDE 35

| θ |cos

0.2 0.4 0.6 0.8 1

θ *sin φ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

θ *sin φ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_s5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

極角分解能

2018/2/3

Study of Higgs->invisible using kinematic fit 35

| θ |cos

0.2 0.4 0.6 0.8 1

MC

θ

  • REC

θ = θ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

MC

θ

  • REC

θ = θ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_s5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

方位角分解能 𝜀𝜚 ∗ 𝑡𝑗𝑜𝜄 = 𝑆𝑁𝑇CD{ 𝜚IJK − 𝜚MK 𝑡𝑗𝑜𝜄}

𝜀𝜄 = 𝑆𝑁𝑇CD(𝜄IJK − 𝜄MK)

ILD_l5_v02 ILD_s5_v02 ILD_l5_v02 ILD_s5_v02

slide-36
SLIDE 36

極角分解能

2018/2/3

Study of Higgs->invisible using kinematic fit 36

| θ |cos

0.2 0.4 0.6 0.8 1

MC

θ

  • REC

θ = θ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

MC

θ

  • REC

θ = θ δ

0.02 0.04 0.06 0.08

sv01-19-05.mILD_s5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

方位角分解能

| θ |cos

0.2 0.4 0.6 0.8 1

MC

φ

  • REC

φ = φ δ

0.05 0.1 0.15 0.2 0.25 0.3

sv01-19-05.mILD_l5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

| θ |cos

0.2 0.4 0.6 0.8 1

MC

φ

  • REC

φ = φ δ

0.05 0.1 0.15 0.2 0.25 0.3

sv01-19-05.mILD_s5_o1_v02_nobg

15GeV 20GeV 30GeV 45.5GeV 60GeV 80GeV 100GeV 120GeV 150GeV 175GeV 200GeV 250GeV

𝜀𝜚 = 𝑆𝑁𝑇CD(𝜚IJK − 𝜚MK) 𝜀𝜄 = 𝑆𝑁𝑇CD(𝜄IJK − 𝜄MK)

ILD_l5_v02 ILD_s5_v02 ILD_l5_v02 ILD_s5_v02

slide-37
SLIDE 37

Event Selection

  • 1. isolated lepton veto
  • 2. loose restriction

[transverse di-jet momentum, di-jet invariant mass, recoil

mass from di-jet]

  • 3. number of PFOs and charged tracks: Npfo, Ntrack
  • 4. di-jet (Z) pt: PtZ
  • 5. di-jet mass: MZ
  • 6. di-jet polar angle: θZ
  • 7. recoil mass: Mrecoil
  • 8. multi-variate analysis: Boosted Decision Tree(BDT)

method

2018/2/3

Study of Higgs->invisible using kinematic fit 37

slide-38
SLIDE 38

生成断面積とモンテカルロサンプル

2018/2/3

Study of Higgs->invisible using kinematic fit 38

slide-39
SLIDE 39

How to set UL [Statistical method]

l Template

Ø Assume BR(H→invisible)=[1,2,…,10]% -> Event selection Ø Get # of events (NS+B) in window range (Mrecoil∈[120,140] GeV) Ø Generate Poisson distribution of NS+B -> Get 95% CL limit (NUL) Ø Repeat for each BR(H→invisible)=[1,2,…,10]% -> Get calibration line between NUL and UL

l Toy MC

Ø Fit template bkg -> Generate pseudo experiment by fluctuated bkg function Ø Get # of events (NS+B) in window range (Mrecoil∈[120,140] GeV) Ø Translate NS+B into UL of BR(H→invisible) using calibration line Ø Repeat 10000 times -> Obtain UL distribution 2016/12/9 @LCWS2016

BSM search using Higgs to invisible decay 39

NS+B NUL UL NS+B

slide-40
SLIDE 40

Result of Mrec dist. [Ecm = 250 GeV, 250 fb-1,BR(H->inv.)=10%]

2018/2/3

40

No. Cut No. Cut 1 Isolated lepton veto 5 80 < di-jet invariant mass < 100 2 Loose Cut (Ptz,Mz,Mrecoil) 6 | di-jet polar angle |< 0.9 3 #pfo >15 & #all_track > 6 & # track_in_one_jet > 1 7 100 < recoil mass < 160 4 20 GeV < di-jet Pt < 80 GeV 8 BDT cut

MVA input variables

di-jet inv. mass

  • ne jet

polar angle

di-jet polar angle

another jet polar angle

TMVA v-4.2.0

Study of Higgs->invisible using kinematic fit

Right

significance: 19.7 efficiency: 65.9%

signal bkg

Left

significance: 15.5 efficiency: 63.5%

signal bkg