rare b decays chris parkes supa postgraduate lectures introduction radiative decays b s b d ...

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Rare B Decays Chris Parkes SUPA Postgraduate Lectures •Introduction •Radiative decays bs bd •Electroweak Penguin b sl + l - •Rate •Forward backward asymmetry •Final states with neutrinos

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Page 1: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Rare B Decays

Chris Parkes

SUPA Postgraduate Lectures

•Introduction•Radiative decays

bsbd

•Electroweak Penguin b sl+l-

•Rate•Forward backward asymmetry

•Final states with neutrinos

Page 2: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

B mesons / Baryons

• Masses known to a few MeV

00 ,, sBBB and various excitations

CB

• Baryonsb

• In spectator model b lifetimes would all be the same– Non-spectator effects give rise to a hierarchy

Theory and experimental pattern in agreement

Evidence 1998Accurate Mass 2005

Page 3: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

What do we mean by a rare B-decay ?

• All decays ‘rare’ as decays out of generation

b

t

s

c

d

u

• Flavour Changing Neutral Currents (FCNC) are even more suppressed as forbidden at tree level in SM– bs– bd

• Rare in this context means not bc

Page 4: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Feynman Diagrams for B Processes

Page 5: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

FCNC B decays

• Forbidden at tree level in SM

• Occur via Penguin / Box diagrams

• Sensitive to New Physics heavy particles – SUSY, non-SM Higgs

Page 6: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Operator Product Expansion (OPE)• A method of formulating an effective theory of the interaction

Feynman diagram full process description

OrEffective point-like vertex

e.g.

decay

Contains : 1)CKM elements VCKM

2)Matrix Element Operators non-perturbative - Lattice Calculations, HQET

3)Wilson Coupling Coefficients Ci (there are 10)Aim to measure these – sensitive to new physics

• Form an effective weak Hamiltonian, effective vertices multiplied by effective coupling constants

Page 7: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

bs

Page 8: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Discovery of bs, B K*

• FCNC

• CLEO, 1993 (PRL 71,674)

Later extended to inclusive bs rate measurementRate sensitive to new physics

Page 9: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 10: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 11: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 12: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Current Result (BaBar/Belle)

Page 13: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

bd

Page 14: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 15: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Discovery of bd

Page 16: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

And… bd gluon (g )ss

Page 17: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 18: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 19: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 20: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Forward Backward Asymmetry of leptonssensitive to New Physics, determine C7 C9 C10

Page 21: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Determined with low precisionRequires a larger data sampleLHCb or Super-B Factory

Page 22: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Channels with neutrinos

Page 23: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 24: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 25: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward
Page 26: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

B(s)+-

Page 27: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

B(s)+-

•Really really rare!

SM box SM Penguin

•Sensitive to New Physics

in SUSY models

Page 28: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

B(s)+-

•Unique Experimental signature•Easy to identify / trigger – good for ATLAS/CMS

•Really really rare! •Needs LHC data sample for SM•Bs 3.5x10-9, •Bd 1.0x10-10

Current limits from Tevatron

Page 29: Rare B Decays Chris Parkes SUPA Postgraduate Lectures Introduction Radiative decays b  s  b  d  Electroweak Penguin b  sl + l - Rate Forward backward

Information Sources

• Varenna CP violation school 2005– http://varenna05.pi.infn.it/– Slides taken from talks of:– Rare B Decays – H. Aihara

• OPE & Wilson Coefficients, A. Buras hep-ph/9806471