Rare decays at LHCb: looking for new physics in b s + - - - PowerPoint PPT Presentation

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Rare decays at LHCb: looking for new physics in b s + - - - PowerPoint PPT Presentation

University of Birmingham School of Physics and Astronomy seminar 4th Nov. 2015 Rare decays at LHCb: looking for new physics in b s + - transitions Luca Pescatore Outline Rare decays: a tool to search for new physics


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SLIDE 1

Luca Pescatore

Rare decays at LHCb:

  • looking for new physics in b→s𝓂+𝓂- transitions

University of Birmingham School of Physics and Astronomy seminar 4th Nov. 2015

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SLIDE 2
  • L. Pescatore

School of Physics seminar

Outline

๏ Rare decays: a tool to search for new physics

✓ Motivation ✓ Theoretical framework ✓ Recent results at LHCb

๏ An analysis of Λb→Λ0μμ decays

✓ Introduction ✓ Differential Branching fraction measurement ✓ Angular analysis

๏ Testing lepton universality with RK*0 ratio

✓ RK and RK* ✓ Measurement description

2

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SLIDE 3
  • L. Pescatore

School of Physics seminar

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The flavour problem and the need for New Physics

The SM is a very successful theory!

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SLIDE 4
  • L. Pescatore

School of Physics seminar

3

The flavour problem and the need for New Physics

The SM is a very successful theory!

Dark matter? Hierarchy problem? Matter antimatter asymmetry?

… but still has its limits …

Include gravity?

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SLIDE 5
  • L. Pescatore

School of Physics seminar

4

Flavour violation in the SM is ruled by the CKM matrix.

The flavour problem and the need for New Physics

Flavour:

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SLIDE 6
  • L. Pescatore

School of Physics seminar

4

Flavour violation in the SM is ruled by the CKM matrix.

The flavour problem and the need for New Physics

Flavour:

First job for LHCb: precision measurement of CKM parameters. It needs a solid basis to go beyond.

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SLIDE 7
  • L. Pescatore

School of Physics seminar

4

Flavour violation in the SM is ruled by the CKM matrix.

The flavour problem and the need for New Physics

Flavour:

Neutrino oscillations? Indicate flavour violation beyond the SM

… then we need beyond the SM physics (BSM)

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SLIDE 8
  • L. Pescatore

School of Physics seminar

4

Flavour violation in the SM is ruled by the CKM matrix.

The flavour problem and the need for New Physics

Flavour:

Neutrino oscillations? Indicate flavour violation beyond the SM

… then we need beyond the SM physics (BSM)

Why does it have a hierarchical structure?

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SLIDE 9
  • L. Pescatore

School of Physics seminar

Why are there 3 families of quarks and leptons?

4

Flavour violation in the SM is ruled by the CKM matrix.

The flavour problem and the need for New Physics

Flavour:

Neutrino oscillations? Indicate flavour violation beyond the SM

… then we need beyond the SM physics (BSM)

Why does it have a hierarchical structure?

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SLIDE 10
  • L. Pescatore

School of Physics seminar

Charged currents: exchange of a W boson →

Only charged currents change flavour in the SM: FCNCs are forbidden at tree level … but it could be different in BSM

← Neutral currents: exchange of a Z/𝛿 boson

4

Flavour violation in the SM is ruled by the CKM matrix.

The flavour problem and the need for New Physics

Flavour:

FCNCs in the SM

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SLIDE 11
  • L. Pescatore

School of Physics seminar

BSM models often predict different amounts of flavour violation than the SM

5

Flavour and BSM physics

BSM models

Can be almost anything as long as compatible with SM → need to constrain the parameter space

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SLIDE 12
  • L. Pescatore

School of Physics seminar

BSM models often predict different amounts of flavour violation than the SM

5

Flavour and BSM physics

BSM models

Can be almost anything as long as compatible with SM → need to constrain the parameter space

MFV models

Can be constrained looking at Bd / Bs ratios FV only from CKM

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SLIDE 13
  • L. Pescatore

School of Physics seminar

BSM models often predict different amounts of flavour violation than the SM

5

Flavour and BSM physics

BSM models

Simplified models

Mid-way model building step: can show the way.

Limited set of parameters = very predictive and easy to compare with measurement

Can be almost anything as long as compatible with SM → need to constrain the parameter space

MFV models

Can be constrained looking at Bd / Bs ratios FV only from CKM

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SLIDE 14
  • L. Pescatore

School of Physics seminar

BSM models often predict different amounts of flavour violation than the SM

5

Flavour and BSM physics

BSM models

Z’ penguins Additional Z’ bosons from a U(1) gauge symmetry

Simplified models

Mid-way model building step: can show the way.

Limited set of parameters = very predictive and easy to compare with measurement

Can be almost anything as long as compatible with SM → need to constrain the parameter space

MFV models

Can be constrained looking at Bd / Bs ratios FV only from CKM

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SLIDE 15
  • L. Pescatore

School of Physics seminar

BSM models often predict different amounts of flavour violation than the SM

5

Flavour and BSM physics

BSM models

Z’ penguins Additional Z’ bosons from a U(1) gauge symmetry Leptoquarks Bosonic particles that carry one lepton and one quark quantum numbers

Simplified models

Mid-way model building step: can show the way.

Limited set of parameters = very predictive and easy to compare with measurement

Can be almost anything as long as compatible with SM → need to constrain the parameter space

MFV models

Can be constrained looking at Bd / Bs ratios FV only from CKM

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SLIDE 16
  • L. Pescatore

School of Physics seminar

6

Rare decays

  • Rare decays: processes suppressed in the SM that can happen only at loop level.
  • Flavour Changing Neutral Currents

→ forbidden at tree level in the SM (e.g b→s or b→d transitions) → branching fractions typically ~10-6 or less → today: mainly dealing with b→s𝓂+𝓂- decays

Penguin diagram W box arXiv:1501.03309

  • New Physics can enter in the loops
  • Very sensitive to new physics effects

→ NP enters at the same level as SM

  • No evidence in direct searches so far

→ loops can probe high energy scales

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SLIDE 17
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

7

  • M(b) << M(W, Z, top) ⇒ an effective theory can be built
  • Separate aptitude calculations into 2 parts:
  • “long-distance”: below b mass scale (known SM physics)
  • “short-distance”: above b mass scale (Z,W and top + all new physics)
  • An example of effective theory is the Fermi-theory of weak interactions

Effective theory

Phys.Lett. B400 (1997) 206–219 arXiv:1501.03309

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SLIDE 18
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

7

  • M(b) << M(W, Z, top) ⇒ an effective theory can be built
  • Separate aptitude calculations into 2 parts:
  • “long-distance”: below b mass scale (known SM physics)
  • “short-distance”: above b mass scale (Z,W and top + all new physics)
  • An example of effective theory is the Fermi-theory of weak interactions

Effective theory

Phys.Lett. B400 (1997) 206–219 arXiv:1501.03309

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SLIDE 19
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

7

  • M(b) << M(W, Z, top) ⇒ an effective theory can be built
  • Separate aptitude calculations into 2 parts:
  • “long-distance”: below b mass scale (known SM physics)
  • “short-distance”: above b mass scale (Z,W and top + all new physics)
  • An example of effective theory is the Fermi-theory of weak interactions

Effective theory

Phys.Lett. B400 (1997) 206–219 arXiv:1501.03309

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SLIDE 20
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

7

  • M(b) << M(W, Z, top) ⇒ an effective theory can be built
  • Separate aptitude calculations into 2 parts:
  • “long-distance”: below b mass scale (known SM physics)
  • “short-distance”: above b mass scale (Z,W and top + all new physics)
  • An example of effective theory is the Fermi-theory of weak interactions

Full theory Effective theory

Phys.Lett. B400 (1997) 206–219 arXiv:1501.03309

Short distance contribution associated with GF

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SLIDE 21
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

8

Heff = −4GF √ 2 h λt

q

X Ci(µ)Oi(µ) + λu

q

X Ci(µ)(Oi(µ) − Ou

i (µ))

i

Effective Hamiltonian for b→d and b→s transitions

Phys.Lett. B400 (1997) 206–219

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SLIDE 22
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

8

Heff = −4GF √ 2 h λt

q

X Ci(µ)Oi(µ) + λu

q

X Ci(µ)(Oi(µ) − Ou

i (µ))

i

Short distance physics encoded in the Wilson Coefficients Effective Hamiltonian for b→d and b→s transitions

Phys.Lett. B400 (1997) 206–219

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SLIDE 23
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

8

Heff = −4GF √ 2 h λt

q

X Ci(µ)Oi(µ) + λu

q

X Ci(µ)(Oi(µ) − Ou

i (µ))

i

Long-distance described by a finite set of operators Short distance physics encoded in the Wilson Coefficients Effective Hamiltonian for b→d and b→s transitions

Phys.Lett. B400 (1997) 206–219

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SLIDE 24
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

8

Heff = −4GF √ 2 h λt

q

X Ci(µ)Oi(µ) + λu

q

X Ci(µ)(Oi(µ) − Ou

i (µ))

i

Long-distance described by a finite set of operators Short distance physics encoded in the Wilson Coefficients CKM factors:

λq0

q = Vq0bV ∗ q0q For b→s transitions Vus << Vts

⇒ the second term can be neglected

Effective Hamiltonian for b→d and b→s transitions

Phys.Lett. B400 (1997) 206–219

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SLIDE 25
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

8

Long-distance described by a finite set of operators Short distance physics encoded in the Wilson Coefficients Effective Hamiltonian for b→d and b→s transitions

Contributions to b→s𝓂+𝓂-: ✓O7 : radiative penguin ✓O9,10 : semileptonic decays (Z penguin and W-box)

Heff = −4GF √ 2 h λt

q

X Ci(µ)Oi(µ) + )) i

Left-handed and right-handed

[CiOi + C0

iO0 i] In the SM: C’ ~ ms/mb C

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SLIDE 26
  • L. Pescatore

School of Physics seminar

Theoretical framework:

the effective Hamiltonian

8

Long-distance described by a finite set of operators Short distance physics encoded in the Wilson Coefficients Effective Hamiltonian for b→d and b→s transitions

CSM

7

= −0.3, CSM

9

= 4.2, CSM

10

= −4.2. Ci = CNP

i

+ CSM

i

Heff = −4GF √ 2 h λt

q

X Ci(µ)Oi(µ) + )) i

Left-handed and right-handed

[CiOi + C0

iO0 i] In the SM: C’ ~ ms/mb C

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  • L. Pescatore

School of Physics seminar

9

Calculating exclusive decay amplitudes

A(M ! F) = hM|Heff|Fi = = GF p 2 X V i

CKMCi(µ)hM|Oi(µ)|Fi

The decay amplitude of an exclusive decay → expectation value of Heff given the initial and final states

Perturbative contribution Hadronic matrix elements (form factors) describing the hadronization process. Need to be obtained with non perturbative methods e.g. Lattice QCD Form factors = main source of uncertainty in theory predictions

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  • L. Pescatore

School of Physics seminar

Low q2 region of large hadron recoil

  • photon pole → linked to C7
  • OPE in 1/Eh applies (SCET)
  • up to open-charm threshold

2mc ~ 7GeV2/c4

  • Interval 1-6 GeV2/c4 cleanest

✓ Far from photon pole ✓ Far from charm threshold

] 4 c / 2 [GeV 2 q 5 10 15 20

OPE QCDF

resonances c c broad resonances c c narrow pole photon interference 9
  • 7
[GeV] * K E 1 2

10

Phenomenology of b→s𝓂+𝓂- decays

arXiv:1501.03309

q2 = m(𝓂+𝓂-)2 [GeV2/c2]

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  • L. Pescatore

School of Physics seminar

] 2 c [MeV/
  • µ
+ µ m 3800 4000 4200 4400 4600 ) 2 c Candidates / (25 MeV/ 50 100 150 data total nonresonant interference resonances background LHCb

High q2 region of low hadron recoil

  • can use limit mb→∞
  • OPE in 1/mb applies (HQET)
  • potential contribution from charm

resonances

] 4 c / 2 [GeV 2 q 5 10 15 20

OPE QCDF

resonances c c broad resonances c c narrow pole photon interference 9
  • 7
[GeV] * K E 1 2

10

Phenomenology of b→s𝓂+𝓂- decays

arXiv:1501.03309

q2 = m(𝓂+𝓂-)2 [GeV2/c2]

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  • L. Pescatore

School of Physics seminar

Central q2

  • Dominated by J/ѱ and ѱ(2S)
  • Charm resonances through tree

level b→scc transitions

  • No predictions possible
  • Vetoed experimentally
] 4 c / 2 [GeV 2 q 5 10 15 20

OPE QCDF

resonances c c broad resonances c c narrow pole photon interference 9
  • 7
[GeV] * K E 1 2

10

Phenomenology of b→s𝓂+𝓂- decays

arXiv:1501.03309 b ¯ c

W + c ¯ d/¯ s

} J/ѱ

q2 = m(𝓂+𝓂-)2 [GeV2/c2]

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  • L. Pescatore

School of Physics seminar

11

The LHCb detector

Forward geometry optimised for for b and c decays. Fully instrumented in 2 < η < 5 Cleanest LHC events: <Pile-Up> ~ 2 in Run I 3fb-1 collected: 1fb-1 in 2011 at TeV and 2fb-1 in 2012 at 8TeV

JINST 3 (2008) S08005

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  • L. Pescatore

School of Physics seminar

12

The LHCb detector

VeLo

Silicon tracker → Needed for precise determination of secondary vertices B mesons travel ~1cm into the detector. VeLo is essential to reconstruct secondary vertices of B and D hadrons.

JINST 3 (2008) S08005

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  • L. Pescatore

School of Physics seminar

13

The LHCb detector

RICH

RICH 1: before magnet for 1 < p < 70 GeV/c RICH I1: before magnet for 20 < p < 200 GeV/c Essential to distinguish kinematically similar decays with different final states

JINST 3 (2008) S08005

Provide particle ID

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  • L. Pescatore

School of Physics seminar

14

The LHCb detector

Calorimeters

Example of e/h discrimination PD for charged pions rejection SPD for neutral pions rejection ECAL fully contains electrons HCAL for hadrons ID

JINST 3 (2008) S08005

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  • L. Pescatore

School of Physics seminar

15

The LHCb detector

Muon detector

5 tracking station separated by iron layers Drift tubes in the outer region GEM in the inner region due to higher track density Each station has 95% efficiency. Provides good triggering. Only 10 GeV/c muons pass through.

JINST 3 (2008) S08005

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School of Physics seminar

16

Recent results

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  • L. Pescatore

School of Physics seminar

17

B(Bd/s→μ+μ-)

  • Highly suppressed in the SM FCNC + CKM + helicity
  • Possible tree level BSM contributions ⇒ very sensitive
  • Leptonic decay (no hadronic uncertainties)

→ Very well predicted B(Bs→μμ) = (3.56±0.30)ᐧ10-9

  • Combined measurement by LHCb and CMS
] 2 c [MeV/ µ + µ m 5000 5200 5400 5600 5800 ) 2 c Candidates / (40 MeV/ 2 4 6 8 10 12 14 16 Data Signal and background µ + µ → s B µ + µ → B Combinatorial bkg. Semileptonic bkg. Peaking bkg. CMS and LHCb (LHC run I)

Compatible with the SM. Highly constrains SUSY.

Nature 522 (2015) 68–72, [arXiv:1411.4413].

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SLIDE 38
  • L. Pescatore

School of Physics seminar

18

  • Decay rates of B→K(*)μμ decays: sensitive to new physics entering the loops
  • Single measurements more precise than current world average!
  • All compatible with SM but also all slightly lower.

Extrapolating below J/ѱ assuming distribution as in PRD 61 (2000) 074024

Observables in B→K(*)μμ decays

JHEP 06 (2014) 133, [arXiv:1403.8044]

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SLIDE 39
  • L. Pescatore

School of Physics seminar

19

Observables in B→K(*)μμ decays

  • Large uncertainties in B→K(*) form factors calculations affect predictions

➡ to maximise sensitivity measure asymmetries and ratios where the leading form

factor cancel: e.g. isospin asymmetry

  • Same quark level transition but

charge different light spectator quark

  • AI ~ O(1%) in SM (≠0 for mq/mb corrections)

B0 over B+ lifetimes ratio Two ratios are measured for K and K*

JHEP 06 (2014) 133, [arXiv:1403.8044]

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  • L. Pescatore

School of Physics seminar

20

Observables in B→K(*)μμ decays

  • B+/B0 production asymmetry can bias the result
  • B-factories assumed null B+/B0 production asymmetry
  • LHCb: J/ѱ modes used for normalisation
  • J/ѱ channels have same final daughters → cancellations of systematics
  • A = 0 tested against simplest alternative: constant different than zero.

JHEP 06 (2014) 133, [arXiv:1403.8044]

Compatible with SM within 1.5σ

B → K(∗)µ+µ− B → K(∗)(J/ψ → µ+µ−)

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  • L. Pescatore

School of Physics seminar

21

B0→K*0μμ angular analysis

  • Angular distributions described by 3 angles: θl, θK, ϕ
  • Distributions depend on:

✓ Wilson coefficients: sensitive to new physics :-) ✓ and form factors :-(

  • Measure variables with reduced form factor

uncertainties (JHEP

, 05, 2013, 137)

21

1 dΓ/dq2 d4Γ d cos θld cos θKdφdq2 = 9 32π [3 4(1 − FL) sin2 θK + FL cos2 θK + 1 4(1 − FL) sin2 θK cos 2θl −FL cos2 θK cos 2θl + S3 sin2 θK sin2 θl cos 2φ + S4 sin 2θK sin 2θl cos φ +S5 sin 2θK sin θl cos φ + S6 sin2 θK cos θl + S7 sin 2θK sin θl sin φ +S8 sin 2θK sin 2θl sin φ + S9 sin2 θK sin2 θl sin 2φ]

P 0

(4,5,6,8) =

S(4,5,7,8) p FL(1 − FL)

JHEP 08 (2013) 131, [arXiv:1304.6325]

  • Phys. Rev. Lett. 111 (2013) 191801

FL = fraction of longitudinally polarised dimuons

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  • L. Pescatore

School of Physics seminar

21

B0→K*0μμ angular analysis

  • Angular distributions described by 3 angles: θl, θK, ϕ
  • Distributions depend on:

✓ Wilson coefficients: sensitive to new physics :-) ✓ and form factors :-(

  • Measure variables with reduced form factor

uncertainties (JHEP

, 05, 2013, 137)

21

1 dΓ/dq2 d4Γ d cos θld cos θKdφdq2 = 9 32π [3 4(1 − FL) sin2 θK + FL cos2 θK + 1 4(1 − FL) sin2 θK cos 2θl −FL cos2 θK cos 2θl + S3 sin2 θK sin2 θl cos 2φ + S4 sin 2θK sin 2θl cos φ +S5 sin 2θK sin θl cos φ + S6 sin2 θK cos θl + S7 sin 2θK sin θl sin φ +S8 sin 2θK sin 2θl sin φ + S9 sin2 θK sin2 θl sin 2φ]

P 0

(4,5,6,8) =

S(4,5,7,8) p FL(1 − FL)

JHEP 08 (2013) 131, [arXiv:1304.6325]

  • Phys. Rev. Lett. 111 (2013) 191801
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  • L. Pescatore

School of Physics seminar

22

B0→K*0μμ angular analysis

Many observables found to be in agreement with the SM predictions BUT

Local 3.7σ deviation on P’5 found on 2011 data and confirmed on 2012.

JHEP 08 (2013) 131, [arXiv:1304.6325] LHCb-CONF-2015-002

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  • L. Pescatore

School of Physics seminar

23

Lepton Universality and RH

  • Lepton universality: equality of the EW couplings for leptons
  • Idea: test it using suppressed decays, where there is space for new physics

q2

max ∼ m2 b

q2

min ∼ 4m2 µ
  • Universality → RK ~ 1 with o((mμ/mb)2) corrections (JHEP 12 (2007) 040)
  • Hadronic uncertainties cancel in the ratio

➡ precisely predicted: RK = 1.0 ± 0.0001

Belle ⇒ RK = 0.74+0.46-0.37 BaBar ⇒ RK = 1.03 ± 0.25

PRL 103 (2009) 171801 PRD 86 (2012) 032012

PhysRevLett.113.151601 arXiv:1406.6482

RH = R mb

4m2

µ

dB(B→Hµ+µ−) dq2

R mb

4m2

µ

dB(B→He+e−) dq2

dq2

H = K, K∗0, φ, ...

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  • L. Pescatore

School of Physics seminar

24

The RK measurement

  • The ee channels are the challenge in this analysis:
  • Bremsstrahlung affects the e momentum

→ energy recovered looking at calorimeter hits

  • Low trigger efficiency

→ Use events triggered by the electrons, by the hadrons and by other particles in the event

PhysRevLett.113.151601 arXiv:1406.6482

trigger by electron trigger by hadron trigger by other b
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  • L. Pescatore

School of Physics seminar

25

The ee BR is also reported:

trigger by electron trigger by hadron trigger by other b

← Kµµ triggered by muons 1266 ± 41 evts Kee in 3 categories → 172 + 20 + 62 evts

PhysRevLett.113.151601 arXiv:1406.6482

2.6σ from the SM

The RK measurement

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  • L. Pescatore

School of Physics seminar

26

Global fits

  • Global fits including information from many results combining many observables.

[S. Descotes-Genon et al. PRD 88, 074002] [Altmannshofer et al. arxiv:1411.3161] [Beaujean et al. EPJC 74 2897]

  • A consistent picture can be built putting most results in agreement
  • Possible explanation with Z’ bosons.
  • Based on assumptions

→ we need more data to be sure

¯ Dc2 = 14.0
  • 0.4
  • 0.2
0.0 0.2 0.4
  • 3
  • 2
  • 1
1 2 3 ReHC7 NPL ReHC9 NPL ¯ Dc2 = 15.6
  • 3
  • 2
  • 1
1 2 3
  • 3
  • 2
  • 1
1 2 3 ReHC9 NPL ReHC9 'L ¯ Dc2 = 14.2
  • 3
  • 2
  • 1
1 2 3
  • 3
  • 2
  • 1
1 2 3 ReHC9 NPL ReHC10 NPL

A shift of C9 by -1 is favoured with respect to the SM

Presented at moriond 2015

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  • L. Pescatore

School of Physics seminar

27

The analysis of the rareΛb→Λ0μμ decay

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  • L. Pescatore

School of Physics seminar

28

Rare decays and Λb→Λ0μμ

  • T. Gutsche et al., PRD87 (2013) 074031
  • Λb has non-zero spin:

→ complementary wrt B mesons

  • Particular hadronic physics (heavy quark + diquark)

→ independent form factors

  • Λb→Λ0μμ is a FCNC

b→s transition: rare decay

So why bother?

  • Can give complementary results → angular analysis
  • Can give independent verifications of results in B physics
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School of Physics seminar

29

Reconstructing Λ0 in LHCb

  • Decay reconstructed using the Λ0 →pπ mode
  • Λ0 is a long-lived particle and can fly a few meters into the detector
  • Can be reconstructed from 2 types of tracks: long and downstream
  • Characterised by different resolution and decay kinematics
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School of Physics seminar

29

Reconstructing Λ0 in LHCb

  • Decay reconstructed using the Λ0 →pπ mode
  • Λ0 is a long-lived particle and can fly a few meters into the detector
  • Can be reconstructed from 2 types of tracks: long and downstream
  • Characterised by different resolution and decay kinematics

✓ Long tracks with hits in the VELO

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School of Physics seminar

29

Reconstructing Λ0 in LHCb

  • Decay reconstructed using the Λ0 →pπ mode
  • Λ0 is a long-lived particle and can fly a few meters into the detector
  • Can be reconstructed from 2 types of tracks: long and downstream
  • Characterised by different resolution and decay kinematics

✓ Downstream tracks without hits in the VELO ✓ Long tracks with hits in the VELO

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School of Physics seminar

30

Selection

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School of Physics seminar

30

Selection

DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
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School of Physics seminar

30

Selection

DIRA

DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
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School of Physics seminar

30

Selection

1 c 1 c m B/D p p

DIRA

DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
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School of Physics seminar

30

Selection

PID using information from RICH and muon detector 1 c 1 c m B/D p p

DIRA

DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
slide-58
SLIDE 58
  • L. Pescatore

School of Physics seminar

30

Selection

Momenta help distinguishing combinatorial PID using information from RICH and muon detector 1 c 1 c m B/D p p

DIRA

DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
slide-59
SLIDE 59
  • L. Pescatore

School of Physics seminar

30

Selection

Neural Network: NeuroBayes Training: signal MC and sideband background Momenta help distinguishing combinatorial PID using information from RICH and muon detector 1 c 1 c m B/D p p

DIRA

DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
slide-60
SLIDE 60
  • L. Pescatore

School of Physics seminar

30

Selection

Neural Network: NeuroBayes Training: signal MC and sideband background A.U. 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 0.1 0.2 0.3 0.4 0.5 signal background Momenta help distinguishing combinatorial PID using information from RICH and muon detector 1 c 1 c m B/D p p

DIRA

DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
slide-61
SLIDE 61
  • L. Pescatore

School of Physics seminar

30

Selection

Neural Network: NeuroBayes Training: signal MC and sideband background A.U. 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 0.1 0.2 0.3 0.4 0.5 signal background Momenta help distinguishing combinatorial PID using information from RICH and muon detector 1 c 1 c m B/D p p

DIRA

MVA cut 0.2 0.4 0.6 0.8 1 S+B S/ 1 2 3 4 5 6 sig = 5.893062e+00

Optimisation

Maximised :
  • Significance at high q2
  • Punzi FoM at low q2
(best for unobserved signals) P = S nσ/2 + √ B DecayTreeFitter: χ2 of a kinematically constrained refit ] 2 c ) [MeV/ µ µ Λ m( 5500 5550 5600 5650 5700 A.U. 1000 2000 3000 4000 5000 6000 7000 8000 Not constrained Constrained
slide-62
SLIDE 62
  • L. Pescatore

School of Physics seminar

Mass fits:Λb→Λ0(J/ѱ→μμ)

31

]

2

c ) [MeV/ µ µ Λ M(

5400 5600 5800 6000

2

c Candidtates per 10 MeV/

10

2

10

3

10

4

10 LHCb

KS

simulated shape

Combinatorial

exponential

Signal

sum of two Crystal Ball functions

Same signal shape used for rare and resonant channels

slide-63
SLIDE 63
  • L. Pescatore

School of Physics seminar

Λb→Λ0μμ branching fraction

32

  • Already observed at CDF (PRL 107 2011 201802) and LHCb (PLB725 2013 25)

but only in the high q2 region, above ѱ(2S)

  • Analysis on 3fb-1: ~300 observed events
] 2 c ) [MeV/ µ µ Λ M( 5400 5600 5800 6000 2 c Candidates per 30.0 MeV/ 20 40 60 80 100 120 140 160 180 200 LHCb

Branching ratio:

Inner error: stati + syst Outer error: including normalisation (dominant)

] 4 c / 2 [GeV 2 q 5 10 15 20 ]
  • 1
) 4 c / 2 (GeV
  • 7
[10 2 q ) / d µ µ Λ → b Λ dB( 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 LHCb SM prediction Data

1.1 < q2 < 6.0 0.09 + 0.06

− 0.05 (stat) + 0.01 − 0.01 (syst) + 0.02 − 0.02 (norm)

15.0 < q2 < 20.0 1.18 + 0.09

− 0.08 (stat) + 0.03 − 0.03 (syst) + 0.27 − 0.27 (norm)

First observation at 3σ level at low q2

[15-20] GeV2/c4 Prediction: PRD 87 (2013) 074502

JHEP 1506 (2015) 115, [arXiv:1503.07138]

slide-64
SLIDE 64
  • L. Pescatore

School of Physics seminar

Angular analysis

33

dΓ dq2d cos θ` ∝ 3 8(1 + cos θ`)(1 − fL) + A`

F B cos θ` + 3

4fL sin2 θ`

New!

dΓ dq2d cos θh ∝ (1 + 2Ah

FB cos θh)

  • Differential rates

as a function of the angles

In Λb rest frame

JHEP 1506 (2015) 115, [arXiv:1503.07138]

  • First measurement of angular observables for this decay
  • In Λb→Λ0μμ the Λ0 decays weakly (v/s in B→K*μμ the K* decays strongly)

→ the hadronic side asymmetry is also interesting

  • Fit one-dimensional angular distributions
slide-65
SLIDE 65
  • L. Pescatore

School of Physics seminar

Angular analysis

33

dΓ dq2d cos θ` ∝ 3 8(1 + cos θ`)(1 − fL) + A`

F B cos θ` + 3

4fL sin2 θ`

New!

Forward-backward asymmetry in the dimuon system

dΓ dq2d cos θh ∝ (1 + 2Ah

FB cos θh)

  • In Λb rest frame

JHEP 1506 (2015) 115, [arXiv:1503.07138]

  • First measurement of angular observables for this decay
  • In Λb→Λ0μμ the Λ0 decays weakly (v/s in B→K*μμ the K* decays strongly)

→ the hadronic side asymmetry is also interesting

  • Fit one-dimensional angular distributions
slide-66
SLIDE 66
  • L. Pescatore

School of Physics seminar

Angular analysis

33

dΓ dq2d cos θ` ∝ 3 8(1 + cos θ`)(1 − fL) + A`

F B cos θ` + 3

4fL sin2 θ`

New!

Fraction of longitudinally polarised dimuons

dΓ dq2d cos θh ∝ (1 + 2Ah

FB cos θh)

  • In Λb rest frame

JHEP 1506 (2015) 115, [arXiv:1503.07138]

  • First measurement of angular observables for this decay
  • In Λb→Λ0μμ the Λ0 decays weakly (v/s in B→K*μμ the K* decays strongly)

→ the hadronic side asymmetry is also interesting

  • Fit one-dimensional angular distributions
slide-67
SLIDE 67
  • L. Pescatore

School of Physics seminar

Angular analysis

33

dΓ dq2d cos θ` ∝ 3 8(1 + cos θ`)(1 − fL) + A`

F B cos θ` + 3

4fL sin2 θ`

New!

Forward-backward asymmetry in the hadronic system

dΓ dq2d cos θh ∝ (1 + 2Ah

FB cos θh)

  • In Λb rest frame

JHEP 1506 (2015) 115, [arXiv:1503.07138]

  • First measurement of angular observables for this decay
  • In Λb→Λ0μμ the Λ0 decays weakly (v/s in B→K*μμ the K* decays strongly)

→ the hadronic side asymmetry is also interesting

  • Fit one-dimensional angular distributions
slide-68
SLIDE 68
  • L. Pescatore

School of Physics seminar

l θ cos
  • 1
  • 0.5

0.5 1

Candidates per 0.2 10 20 30 40 50 60 70 LHCb

Angular analysis

34

New!

h θ cos
  • 1
  • 0.5

0.5 1

Candidates per 0.2 10 20 30 40 50 60 70 80 90

LHCb

15 < q2 < 20 GeV2/c4

PDF tot(cos θi) = [f theory(cos θi) + f bkg(cos θi)] × ε(cos θi)

Most challenging due to asymmetric acceptance.

Dimuon system Hadronic system

JHEP 1506 (2015) 115, [arXiv:1503.07138]

  • First measurement of angular observables for this decay
  • In Λb→Λ0μμ the Λ0 decays weakly (v/s in B→K*μμ the K* decays strongly)

→ the hadronic side asymmetry is also interesting

  • Fit one-dimensional angular distributions
slide-69
SLIDE 69
  • L. Pescatore

School of Physics seminar

] 4 c / 2 [GeV 2 q 5 10 15 20 h FB A
  • 0.5
  • 0.4
  • 0.3
  • 0.2
  • 0.1
0.1 0.2 0.3 0.4 0.5 LHCb SM prediction Data ] 4 c / 2 [GeV 2 q 5 10 15 20 l FB A
  • 1
  • 0.8
  • 0.6
  • 0.4
  • 0.2
0.2 0.4 0.6 0.8 1 LHCb SM prediction Data

Angular analysis: results

35

  • Only where the signal significance is above 3σ
  • Physical boundaries in the parameter-space:

→ using Feldman-Cousins inspired “plug-in” method

  • l
FB A
  • 0.5
0.5 L f 0.2 0.4 0.6 0.8 1 LHCb 4 c / 2 [15.0,20.0] GeV

Leptonic asymmetry Hadronic asymmetry

  • AhFB is in good agreement with SM prediction
  • AlFB is compatible within 2 sigma but consistently

above the prediction → Could be due large contributions.

cc

Physical region

New!

Two-dimensional 68% CL region JHEP 1506 (2015) 115, [arXiv:1503.07138] Theory: arXiv:1401.2685

slide-70
SLIDE 70
  • L. Pescatore

School of Physics seminar

36

Testing lepton universality: RK*

slide-71
SLIDE 71
  • L. Pescatore

School of Physics seminar

37

RK*: making RK stronger and more

  • Amplitudes for different B→H𝓂𝓂 are described by different

combinations of left- and right-handed (C and C’) Wilson coefficients

  • Therefore sensitive to different kind of new physics

RK and RK* give complementary information!

RH = R mb

4m2

µ

dB(B→Hµ+µ−) dq2

R mb

4m2

µ

dB(B→He+e−) dq2

dq2

H = K, K, K∗0

JHEP 1502 (2015) 055 [arXiv:1411.4773]

slide-72
SLIDE 72
  • L. Pescatore

School of Physics seminar

38

Selection for RK*

  • Neural Network (similarly to Λb→Λ0μμ)
  • PID from variables combining information from RICH, calorimeters,

muon detector and tracking Cuts on combinations of correct ID and mis-ID variables to exploit the full PID power.

Kaon ID efficiency: ~ 95 % for ~ 5 % π→K mis-id probability Muon ID efficiency: ~ 97 % for 1-3 % π→μ mis-id probability

slide-73
SLIDE 73
  • L. Pescatore

School of Physics seminar

39

Peaking backgrounds

Other decays may mimic the decays of interest: ✓ B+→K+μμ plus a random pion ✓ Bs→ϕμμ with ϕ→KK and a K misidentified as a π ✓ Λb decays with misidentified or misreconstructed particles

  • Not peaking: need to be modelled in the fit

3-body Kμμ invariant mass shows a narrow B+ peak easy to remove

slide-74
SLIDE 74
  • L. Pescatore

School of Physics seminar

39

Peaking backgrounds

Other decays may mimic the decays of interest: ✓ B+→K+μμ plus a random pion ✓ Bs→ϕμμ with ϕ→KK and a K misidentified as a π ✓ Λb decays with misidentified or misreconstructed particles

  • Not peaking: need to be modelled in the fit

We give the identify of a K to the pion and recalculate the mass. A peak is present in a limited region of the plane

slide-75
SLIDE 75
  • L. Pescatore

School of Physics seminar

40

The HOP cut for electrons

Correct electron momentum assuming the energy is lost due to bremsstrahlung

pcorr

x,y,x =

pK∗0

T

pee

T

! pmeas

x,y,z

pK∗0

T

= −pee

T then recompute the 4-body mass

Backgrounds have low values of corrected masses which allows to separate the signal.

slide-76
SLIDE 76
  • L. Pescatore

School of Physics seminar

41

Charmonium channels

  • Charmonium channels B→K*(J/ѱ→𝓂𝓂) peak in the q2 spectrum.
  • Naturally distinguished from the rare channels by the q2 binning

[0.1,1,1,2,4,6,8] - J/ѱ - [11,12.5] - ѱ(2S) - [15,16,18,20] µµ ee

Resonant samples used as high statistics control samples.

slide-77
SLIDE 77
  • L. Pescatore

School of Physics seminar

42

Mass fits: B0→K*0(J/ѱ→μμ)

] 2 ) [Mev/c µ µ π m(K 5200 5300 5400 5500 5600 5700 5800 2 Candidtates per 10 Mev/c 1 10 2 10 3 10 4 10 5 10 0.0001 ± = -0.0055 KstJPsMM comb b 0.01 ± = 5280.88 KstJPsMM_MC m 73.7 ± = 2191.6 Bs2KstJPs N 456.1 ± = 13850.4 Lb2pKJPs N 363.8 ± = 10197.0 comb N 599.7 ± = 333917.2 ψ J/ N 0.002 ± = 1.140 scale JPs σ
  • Sig. KstJPsMM
  • Bkg. Bs2KstJPs
  • Bkg. Lb2pKJPs
  • Bkg. comb
5200 5300 5400 5500 5600 5700 5800 Pulls 5 − 5
  • Resonant and rare samples fit simultaneously → some shape parameters shared

Signal: sum of two Crystal Ball functions Λb decays: modelled with a simulated shape Bs→K*μμ: same shape as signal but shifted in mass Combinatorial: exponential

  • A kinematic fit is used to constrain the Jpsi

mass improving the B0 mass resolution

slide-78
SLIDE 78
  • L. Pescatore

School of Physics seminar

43

Electron channels: trigger

Simultaneous fit to the three trigger categories

  • The trigger categories (with different mass shapes and efficiencies)

✓ L0E ⇒ triggered by the electron ✓ L0H ⇒ triggered by the hadron and not the electron ✓ L0I ⇒ triggered by other particles in the event (and not the first two)

  • Yields parameterised as a function of a common parameter:

➡ Allows to get a combined result directly out of the fit ➡ More stable fit as it gathers information form 3 samples at once

slide-79
SLIDE 79
  • L. Pescatore

School of Physics seminar

44

Electron channels: signal description

  • Mass shapes depend on how many bremsstrahlung photons are recovered

✓ Fit simulation split in brem categories ✓ Take from simulated fractions of 0, 1 and 2 𝛿 ✓ Build a combined PDF

] 2 ee) [MeV/c π m(K 4800 5000 5200 5400 5600 5800 6000 6200 2 Candidtates per 20 MeV/c 200 400 600 800 1000 1200 1400 1600 1800 2000 2200 2400 0.004 ± = 0.145 KstJPsEE_0g_L0E α 1.1 ± = 5247.0 KstJPsEE_0g_L0E m 0.6 ± = 25.1 KstJPsEE_0g_L0E σ Chi2/NDF = 64.37 / 37.00
  • Sig. KstJPsEE
4800 5000 5200 5400 5600 5800 6000 Pulls 5 − 5 ] 2 ee) [MeV/c π m(K 4800 5000 5200 5400 5600 5800 6000 6200 2 Candidtates per 20 MeV/c 500 1000 1500 2000 2500 3000 3500 4000 0.03 ± = 0.39 KstJPsEE_1g_L0E α 0.04 ± = 0.88 KstJPsEE_1g_L0E gauss f 1.7 ± = 5246.2 KstJPsEE_1g_L0E m 31.0 ± = 5314.4 KstJPsEE_1g_L0E gauss m 2.3 ± = 46.0 KstJPsEE_1g_L0E σ 8.1 ± = 99.1 KstJPsEE_1g_L0E gauss σ Chi2/NDF = 6309.06 / 47.00
  • Sig. KstJPsEE
4800 5000 5200 5400 5600 5800 6000 Pulls 5 − 5 ] 2 ee) [MeV/c π m(K 4800 5000 5200 5400 5600 5800 6000 6200 2 Candidtates per 20 MeV/c 200 400 600 800 1000 1200 1400 1600 1800 0.1 ± = 0.6 KstJPsEE_2g_L0E α 0.1 ± = 0.7 KstJPsEE_2g_L0E gauss f 1.5 ± = 5258.3 KstJPsEE_2g_L0E m 38.4 ± = 5345.7 KstJPsEE_2g_L0E gauss m 5.7 ± = 50.5 KstJPsEE_2g_L0E σ 10.2 ± = 85.4 KstJPsEE_2g_L0E gauss σ Chi2/NDF = 52.76 / 45.00
  • Sig. KstJPsEE
4800 5000 5200 5400 5600 5800 6000 Pulls 5 − 5

0𝛿: simple CB 1𝛿: CB+gauss 2𝛿: CB+gauss

slide-80
SLIDE 80
  • L. Pescatore

School of Physics seminar

45

Electron channels: background description

  • Combinatorial: exponential
  • Background from higher hadronic and leptonic resonances
  • Leak of the J/ѱ and ѱ(2S) tails into the rare intervals

Modelled with simulated distributions Only resonant channel

B→(Y→KπX)(J/ѱ→ee) B→(K*→Kπ)(Y->J/ѱ→ee)

slide-81
SLIDE 81
  • L. Pescatore

School of Physics seminar

46

Mass fits: B0→K*0(J/ѱ→ee)

Simultaneous fit to the three trigger categories, resonant and rate samples: shape parameters are shared.

] 2 c ee) [MeV/ π m(K 5100 5150 5200 5250 5300 5350 5400 5450 5500 5550 5600 2 c Candidtates per 10 MeV/ 1 10 2 10 3 10
  • Sig. KstPsiEE
  • Bkg. comb

Fitting also ѱ(2S) events as they can leak into the high q2 rare interval.

] 2 c ee) [MeV/ π m(K 4600 4800 5000 5200 5400 5600 5800 6000 6200 2 c Candidtates per 34 MeV/ 1000 2000 3000 4000 5000 6000 7000
  • Sig. KstJPsEE
  • Bkg. comb
  • Bkg. leakPsi
  • Bkg. Lb2pKJPs
  • Bkg. misRecoKst
  • Bkg. misRecoJPs
  • Bkg. Bs2KstJPs
slide-82
SLIDE 82
  • L. Pescatore

School of Physics seminar

47

J/ѱ sanity check

No new physics expected in the resonant channels Good agreement is found → almost ready to get the results out! → Ratio between them corrected for efficiency should be 1

slide-83
SLIDE 83
  • L. Pescatore

School of Physics seminar

48

Result and systematics

Result as a double ratio over the resonant channels → similar kinematics cancels systematic uncertainties in efficiency determination

Systematics

Results not approved yet, but soon!

  • Choice of signal and background PDFs
  • Bin migration modelling
slide-84
SLIDE 84
  • L. Pescatore

School of Physics seminar

49

Thank you for listening!

  • Many interesting results from the RD group at LHCb
  • Updated B(Λb→Λ0μμ): uncertainties improved by a factor of ~3
  • First evidence of signal al low q2
  • First measurement of angular observables
  • Testing Lepton Universality with RK*
  • Results coming soon!

Summary

slide-85
SLIDE 85
  • L. Pescatore

School of Physics seminar

Backup

50

slide-86
SLIDE 86
  • L. Pescatore

HEPFT, 2014 Rare decays at LHCb

q2 spectrum DNA

51

Blake, Gershon & Hiller: arXiv:1501.03309v1

slide-87
SLIDE 87
  • L. Pescatore

School of Physics seminar

  • Lepton side PDF has physical boundaries → can bias the uncertainties
  • Nuisance parameters treated with the plug-in method (arXiv:1109.0714)

Based on toy experiments

Well defined frequentist coverage

  • Systematics:
  • Effect of a non-flat efficiency on the integration of the full 5D angular PDF
  • Data-MC discrepancies (MC used for most of the efficiencies)
  • Particular choice of background parameterisation
  • Effect of finite angular resolution → asymmetric bin migration

52

Angular analysis: uncertainties

afb
  • 0.8
  • 0.6
  • 0.4
  • 0.2
0.2 0.4 0.6 0.8 fL 0.2 0.4 0.6 0.8 1

Dark area: region of the parameter space where the PDF is positive.

Statistical uncertainties treated with likelihood ordering method

slide-88
SLIDE 88
  • L. Pescatore

HEPFT, 2014 Rare decays at LHCb

Feldman-Cousins method

  • Feldman-Cousins method plug-in method to extract confidence bands
  • Choose Parameters of Interest (PoI) and fit data with PoI free and fixed
  • Generate toys with PoI fixed to tested values and nuisance parameters (all other parameters)

from fixed fit on data.

  • Fit toys with free and fixed PoI
  • Look how may times log likelihood ratio

in data is smaller than MC

  • Scan values to look for 68%, 95% etc.

53

Statistica Sinica 19 (2009) 301
  • Starts to be widely used in LHCb
  • Allows to consider nuisance parameters: no confidence belt
  • Guarantees full coverage
  • Returns 2-side intervals and upper limits in a unified approach
arXiv:1109.0714v1

arXiv:physics/9711021

slide-89
SLIDE 89
  • L. Pescatore

School of Physics seminar

  • Events generated in a q2 can be

reconstructed in an other.

  • E.g. Due to bremsstrahlung
  • Can cause bias is the migration
  • f events is asymmetric
  • We generate events with

different models to verify how much we are sensitive to this

54

Bin migration

1 10 2 10 3 10 4 10 ] 4 c / 2 [GeV rec 2 q 2 4 6 8 10 12 14 16 18 20 ] 4 c / 2 [GeV gen 2 q 2 4 6 8 10 12 14 16 18 20 ] 4 c / 2 [GeV 2 q 5 10 15 20 model / default 0.5 1 1.5 2 2.5 Ball-Zwicky Melikhov Stech Colangelo QCD Melikhov lattice
slide-90
SLIDE 90
  • L. Pescatore

School of Physics seminar

55

] 2 c ee) [MeV/ π m(K 4600 4800 5000 5200 5400 5600 5800 6000 6200 2 c Candidtates per 34 MeV/ 2000 4000 6000 8000 10000
  • Sig. KstJPsEE
  • Bkg. comb
  • Bkg. leakPsi
  • Bkg. Lb2pKJPs
  • Bkg. misRecoKst
  • Bkg. misRecoJPs
  • Bkg. Bs2KstJPs
] 2 c ee) [MeV/ π m(K 4600 4800 5000 5200 5400 5600 5800 6000 6200 2 c Candidtates per 34 MeV/ 1000 2000 3000 4000 5000 6000 7000
  • Sig. KstJPsEE
  • Bkg. comb
  • Bkg. leakPsi
  • Bkg. Lb2pKJPs
  • Bkg. misRecoKst
  • Bkg. misRecoJPs
  • Bkg. Bs2KstJPs

HOP cut effect HOP No HOP

slide-91
SLIDE 91
  • L. Pescatore

School of Physics seminar

In the high q2 region - above ѱ(2S) - due to threshold effect the combinatorial is not exponential

56

Combinatorial background for high q2

]

2

) [MeV/c ll π M(K

5000 5500 6000

A.U.

0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 ee - MVA < 0.8
  • MVA < 0.8
µ µ
  • MVA < 0.1
µ µ

By inverting the MVA cut one selects only combinatorial background!

slide-92
SLIDE 92
  • L. Pescatore

School of Physics seminar

57

The flavour problem and the need for New Physics

Assumed to be conserved in all SM interactions due to experimental evidence

μ→eee BR < 1.2 × 10-11

Nucl.Phys. B299 (1988) 1

μ→e𝛿 BR < 1.0 × 10-12

Phys.Rev. D65 (2002) 112002 [hep-ex/0111030] Ann.Rev.Nucl.Part.Sci. 58 (2008) 315–341

Flavour:

slide-93
SLIDE 93
  • L. Pescatore

School of Physics seminar

Wilson coefficients

58

The effective theory matched with the full SM calculation at the EW scale (µW) Renormalization equations allow to evolve to different scales. Any particle above the b mass, including Z, W and t, affects at least one coefficient.

  • New physics enters into Wilson coefficients as additive factors.

CSM

7

= −0.3, CSM

9

= 4.2, CSM

10

= −4.2. Ci = CNP

i

+ CSM

i

hep-ph/9806471.

slide-94
SLIDE 94
  • L. Pescatore

School of Physics seminar

59

Operators

A complete basis is given by: ✓O1,2 : tree level ✓O3-6 and O8 : mediated by gluons ✓O7 : radiative penguin ✓O9,10 : semileptonic decays (Z penguin and W-box)

O7 = mb

e (¯

sµνPRb)Fµν O9 = (¯ sµPLb)(¯ `µ`), O10 = (¯ sµPLb)(¯ `µ5`)

Separating left-handed and right-handed components:

Right-handed operators can be obtained swapping PR and PL

Heff = 4GF √ 2 VtbV ⇤

ts

αe 4π

10

X

i=1

[CiOi + C0

iO0 i] Suppressed C’ ~ ms/mb C

arXiv:1501.03309

slide-95
SLIDE 95
  • L. Pescatore

School of Physics seminar

59

Operators

A complete basis is given by: ✓O1,2 : tree level ✓O3-6 and O8 : mediated by gluons ✓O7 : radiative penguin ✓O9,10 : semileptonic decays (Z penguin and W-box)

O7 = mb

e (¯

sµνPRb)Fµν O9 = (¯ sµPLb)(¯ `µ`), O10 = (¯ sµPLb)(¯ `µ5`)

Separating left-handed and right-handed components:

Right-handed operators can be obtained swapping PR and PL

Heff = 4GF √ 2 VtbV ⇤

ts

αe 4π

10

X

i=1

[CiOi + C0

iO0 i] Suppressed C’ ~ ms/mb C

arXiv:1501.03309

slide-96
SLIDE 96
  • L. Pescatore

School of Physics seminar

59

Operators

A complete basis is given by: ✓O1,2 : tree level ✓O3-6 and O8 : mediated by gluons ✓O7 : radiative penguin ✓O9,10 : semileptonic decays (Z penguin and W-box)

O7 = mb

e (¯

sµνPRb)Fµν O9 = (¯ sµPLb)(¯ `µ`), O10 = (¯ sµPLb)(¯ `µ5`)

Separating left-handed and right-handed components:

Right-handed operators can be obtained swapping PR and PL

Heff = 4GF √ 2 VtbV ⇤

ts

αe 4π

10

X

i=1

[CiOi + C0

iO0 i] Suppressed C’ ~ ms/mb C

arXiv:1501.03309

slide-97
SLIDE 97
  • L. Pescatore

School of Physics seminar

60

… and a lot more from RDWG

Analysis semileptonic Bs decays e.g. Bs→ϕμμ

JHEP 07 (2013) 084, [arXiv:1305.2168]

Majorana neutrino and

PRL 112 (2014) 131802

lepton flavour violation searches

PRL 111 (2013) 141801

  • PRL. 111 (2013) 141801

arXiv:1506.08777

slide-98
SLIDE 98
  • L. Pescatore

School of Physics seminar

61

The LHCb detector

Tracking system

TT → before magnet OT → after magnet

  • Precision:

0.4% at 5 GeV/c 1% at 200 GeV/c

  • Silicon strip and drift chambers

Magnet

Power: 4 Tm Polarity periodically reversed to reduce systematics

JINST 3 (2008) S08005

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SLIDE 99
  • L. Pescatore

HEPFT, 2014 Rare decays at LHCb

IP𝛙2 and DIRA

62

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SLIDE 100
  • L. Pescatore

School of Physics seminar

63

Global fit results

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SLIDE 101
  • L. Pescatore

HEPFT, 2014 Rare decays at LHCb

Using J/ѱΛ for cross-check

64

LHCB-PAPER-2015-009 Λ

θ cos

  • 1
  • 0.5
0.5 1

Candidates per 0.1

100 200 300 400 500 600 700 LHCb l

θ cos

  • 1
  • 0.5
0.5 1

Candidates per 0.1

50 100 150 200 250 300 350 400 450 LHCb

Leptonic angle Hadronic angle

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SLIDE 102
  • L. Pescatore

HEPFT, 2014 Rare decays at LHCb

l θ cos
  • 1
  • 0.5
0.5 1
  • Tot. eff. (A.U.)
0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 LHCb simulation h θ cos
  • 1
  • 0.5
0.5 1
  • Tot. eff. (A.U.)
0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 LHCb simulation l θ cos
  • 1
  • 0.5
0.5 1
  • Tot. eff. (A.U.)
0.1 0.2 0.3 0.4 0.5 LHCb simulation h θ cos
  • 1
  • 0.5
0.5 1
  • Tot. eff. (A.U.)
0.1 0.2 0.3 0.4 0.5 0.6 LHCb simulation

Angular acceptances

65

LHCB-PAPER-2015-009

In LHCb long-lived particles, like Λ0, can be reconstructed with hits in the VELO (log)

  • r without hits in the VELO (downstream).
  • Up- and down-stream events are characterised by different efficiency and resolution
  • A simultaneous fit is performed on the two categories

Long Long Downstream Downstream

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SLIDE 103
  • L. Pescatore

HEPFT, 2014 Rare decays at LHCb

Results tables

66

LHCB-PAPER-2015-009

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SLIDE 104
  • L. Pescatore

HEPFT, 2014 Rare decays at LHCb

Confidence regions

67

LHCB-PAPER-2015-009 l FB A
  • 0.5
0.5 L f 0.2 0.4 0.6 0.8 1 LHCb 4 c / 2 [11.0,12.5] GeV l FB A
  • 0.5
0.5 L f 0.2 0.4 0.6 0.8 1 LHCb 4 c / 2 [15.0,16.0] GeV l FB A
  • 0.5
0.5 L f 0.2 0.4 0.6 0.8 1 LHCb 4 c / 2 [16.0,18.0] GeV l FB A
  • 0.5
0.5 L f 0.2 0.4 0.6 0.8 1 LHCb 4 c / 2 [18.0,20.0] GeV
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SLIDE 105
  • L. Pescatore

School of Physics seminar

fL values

68

]

4

c /

2

[GeV

2

q

5 10 15 20

L

f

0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

LHCb

LHCB-PAPER-2015-009
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SLIDE 106
  • L. Pescatore

School of Physics seminar

69

  • Young but growing sector. Recent measurements at LHCb:
  • Lifetime: 1.482 ± 0.021 ps (PRL 111 (2013) 102003)
  • Polarisation: 0.06 ± 0.09 (PLB 724 (2013) 27)
  • Mass: 5619.44 ± 0.51 (PRL 110 (2013) 182001)
  • Hadronization fraction: (PRD 85 (2012) 032008)

fΛ/fd = (0.387 ± 0.043) + (0.067 ± 0.017)(η - 3,198)

Progress with Λb

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SLIDE 107
  • L. Pescatore

School of Physics seminar

Angular analysis

70

New!

LHCB-PAPER-2015-009 l

θ cos

  • 1
  • 0.5
0.5 1

Candidates per 0.2

10 20 30 40 50 LHCb Preliminary

15 < q2 < 20 GeV2/c4

PDF tot(cos θi) = [f theory(cos θi) + f bkg(cos θi)] × ε(cos θi)

  • In Λb→Λ0µµ the Λ0 decays weakly

→ unlike for B decays the hadronic side asymmetry is also interesting

  • Measure two forward-backward asymmetries: in dimuon and Λ0 system
  • Selection based on a Neural Network using the NeuroBayes package
  • Fit one-dimensional angular distributions
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SLIDE 108
  • L. Pescatore

School of Physics seminar

Angular analysis

70

New!

LHCB-PAPER-2015-009 Λ

θ cos

  • 1
  • 0.5
0.5 1

Candidates per 0.2

10 20 30 40 50 60 70 80 LHCb Preliminary

15 < q2 < 20 GeV2/c4

PDF tot(cos θi) = [f theory(cos θi) + f bkg(cos θi)] × ε(cos θi)

  • In Λb→Λ0µµ the Λ0 decays weakly

→ unlike for B decays the hadronic side asymmetry is also interesting

  • Measure two forward-backward asymmetries: in dimuon and Λ0 system
  • Selection based on a Neural Network using the NeuroBayes package
  • Fit one-dimensional angular distributions
slide-109
SLIDE 109
  • L. Pescatore

School of Physics seminar

Λb→Λ0µµ branching ratio

71

  • Already observed at CDF (PRL 107 2011 201802) and LHCb (PLB725 2013 25) but only

in the low q2 region

  • Reconstructed using the Λ→pπ mode
  • J/ѱΛ as normalisation to limit systematics
  • Analysis on 3fb-1: ~300 observed events
  • Peaking background from B→KS decays

modelled in fit.

LHCB-PAPER-2015-009 to be submitted to JHEP ] 2 c ) [MeV/ µ µ Λ M( 5400 5600 5800 6000 2 c Candidates per 30.0 MeV/ 20 40 60 80 100 120 140 160 180 200 LHCb

Branching ratio:

First observation at 3σ level at low q2

] 4 c / 2 [GeV 2 q 5 10 15 20
  • 3
10 ⋅ 2 q ) / d µ µ Λ → b Λ )) dB( Λ ψ J/ → b Λ (1 / B( 0.05 0.1 0.15 0.2 0.25 LHCb

Relative branching fraction

Inner error: total systematic Outer error: statistical (dominant)

preliminary

1.1 < q2 < 6.0 0.09 + 0.06

− 0.05 (stat) + 0.01 − 0.01 (syst) + 0.02 − 0.02 (norm)

15.0 < q2 < 20.0 1.18 + 0.09

− 0.08 (stat) + 0.03 − 0.03 (syst) + 0.27 − 0.27 (norm) preliminary
slide-110
SLIDE 110
  • L. Pescatore

School of Physics seminar

Λb→Λ0µµ branching ratio

71

  • Already observed at CDF (PRL 107 2011 201802) and LHCb (PLB725 2013 25) but only

in the low q2 region

  • Reconstructed using the Λ→pπ mode
  • J/ѱΛ as normalisation to limit systematics
  • Analysis on 3fb-1: ~300 observed events
  • Peaking background from B→KS decays

modelled in fit.

LHCB-PAPER-2015-009 to be submitted to JHEP ] 2 c ) [MeV/ µ µ Λ M( 5400 5600 5800 6000 2 c Candidates per 30.0 MeV/ 20 40 60 80 100 120 140 160 180 200 LHCb

Branching ratio:

preliminary

Absolute branching fraction

Inner error: stati + syst Outer error: including normalisation (dominant)

Compatible with the SM within 1.5σ.

Prediction: PRD 87 (2013) 074502 ] 4 c / 2 [GeV 2 q 5 10 15 20 ]
  • 1
) 4 c / 2 (GeV
  • 7
[10 2 q ) / d µ µ Λ → b Λ dB( 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 LHCb SM prediction Data preliminary

1.1 < q2 < 6.0 0.09 + 0.06

− 0.05 (stat) + 0.01 − 0.01 (syst) + 0.02 − 0.02 (norm)

15.0 < q2 < 20.0 1.18 + 0.09

− 0.08 (stat) + 0.03 − 0.03 (syst) + 0.27 − 0.27 (norm) preliminary
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SLIDE 111
  • L. Pescatore

School of Physics seminar

72

PID using information from RICH and muon detector

DIRA

DecayTreeFitter: χ2 of a kinematically constrained refit MVA cut 0.2 0.4 0.6 0.8 1 S+B S/ 1 2 3 4 5 6 sig = 5.893062e+00 Flight distance

Efficiency evaluated

Training: signal MC and sideband background Maximised :
  • Significance at high q2
  • Punzi FoM at low q2
(best for unobserved signals) P = S nσ/2 + √ B Optimisation A.U. 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 0.1 0.2 0.3 0.4 0.5 signal background Momenta help distinguishing combinatorial arXiv:1211.6759 1 c 1 c m B/D p p ) 2 mass (MeV/c b Λ 5500 5550 5600 5650 5700 1000 2000 3000 4000 5000 6000 7000 8000 ) 2 mass (MeV/c b Λ 5500 5550 5600 5650 5700 500 1000 1500 2000 2500 3000 3500 4000 (LHCB-PAPER-2015-009) ] 4 c / 2 [GeV 2 q 5 10 15 20 Relative efficiency 0.4 0.5 0.6 0.7 0.8 0.9 1 1.1 1.2 1.3 1.4 long downstream LHCb simulation prelimin

Selection