Low energy e - annihilation and τ -lepton decays as a ...
Transcript of Low energy e - annihilation and τ -lepton decays as a ...
O. Shekhovtsova KIPT Kharkov
Ukraine
Cracow, 23.11.2017
NATIONAL SCIENCE CENTERKharkov Institute of Physics and Technology,NAS of Ukraine
Low energy e+ e− - annihilationand τ -lepton decays as a source
information about hadronic interaction
OUTLINE
Muon (g-2): the test of the Standard Model. Current status
Low energy hadronic interaction and Effective Field Theory. Chiral Perturbation Theory and inclusion of resonances
e+e- annihilation into a meson pair, e+e- scattering and hadronic decay modes of �-lepton. Theoretical results and fit to data
Conclusions and perspectives
Standard Model of Elementary Particles
Neutrino oscillations and neutrino masses
Matter-antimatter asymmetry in the Universe
Dark matter and dark energy
…. 2012 by Atlas and CMS the last missing block
the Higgs boson
New Physics ?
Direct search in high energy experiments → no direct signals from LHC so farPrecise low energy measurement of SM parameters
Anomalous Magnetic Momentum of muon: for more than 10 years SM – experiment ~ (2.5 – 4) �
Muon (g-2): the test of the Standard Model.
The magnetic moment of a particle is related to its spin
μ⃗= ge ℏ
2mcS⃗
For Dirac pointlike particle :
g=2
Current status AMM
based on e+e- data → 3.6σ
based on tau – data → 2.4σ
Anomalous magnetic moment (AMM)
Muon (g-2): the test of the Standard Model.
The magnetic moment of a particle is related to its spin
μ⃗= ge ℏ
2mcS⃗
For Dirac pointlike particle :
g=2
Anomalous magnetic moment (AMM)
Current status AMMBNL E821 experiment,completed 2001, published 2006
δaμexp=54⋅10−11
New experiment: Fermilab Muon g-2
Assuming no changes in the (g-2) central value the (exp - theory) discrepancy increases 5σ
Muon (g-2): the test of the Standard Model.
The magnetic moment of a particle is related to its spin
μ⃗= ge ℏ
2mcS⃗
For Dirac pointlike particle :
g=2
Anomalous magnetic moment (AMM)
Current status AMM
What are the SM contributions and their errors? → to get the same precision?
SM VALUE FOR MUON AMM: QED
1 loop
2 loop graphs
………
Recently several independent checks of 4- and 5-loop diagrams: agree with Kinoshita’ results
PRL 109 (2012) 111807
is already reached
SM VALUE FOR MUON AMM: Electro-Weak
is already reached
SM VALUE FOR MUON AMM: Hadronic contribution
L(eading)O(rder) diagrams
H(adronic)V(acuum)P(olarization) H(adronic)L(ight)b(y)L(ight)
... non-perturbative QCD region, the limiting factor of the SM (g-2) prediction
TO APPLY EXPERIMENTAL LOW ENERGY DATA
(LO) Relies on measurements of T(ransition)F(orm)F(actor) in (two-photon) scattering e+e- → e+e- +’
aμHLbL
=(10 .5±26 )⋅10−11
SM VALUE FOR MUON AMM: Hadronic contribution
L(eading)O(rder) diagrams
H(adronic)V(acuum)P(olarization) H(adronic)L(ight)b(y)L(ight)
... non-perturbative QCD region, the limiting factor of the SM (g-2) prediction
TO APPLY EXPERIMENTAL LOW ENERGY DATA
e+e-- → → hadrons(τ→ hadrons + ν
)
dispersion relation+ optical theorem
CVC data
Current status AMM. Summary
692.3 (4.2)
The SM value
Total:(on e+e-)
3.6σ Diff: 28.2 · 10-10
HADRONIC uncertainty dominates!
It is heavy to expect a missed SM effect as large as (200-300)·10 -11 , i.e. logical posibilities:
Some experimental issue → new independent measurement by Fermilab Muon g-2
Current status AMM. Summary
692.3 (4.2)
The SM value
Total:(on e+e-)
3.6σ Diff: 28.2 · 10-10
HADRONIC uncertainty dominates!
It is heavy to expect a missed SM effect as large as (200-300)·10 -11 , i.e. logical posibilities:
Some experimental issue → new independent measurement by Fermilab Muon g-2
NP beyond the Standard Model → no evidence about NP from LHC
Current status AMM. Summary
692.3 (4.2)
The SM value
Total:(on e+e-)
3.6σ Diff: 28.2 · 10-10
HADRONIC uncertainty dominates!
It is heavy to expect a missed SM effect as large as (200-300)·10 -11 , i.e. logical posibilities:
Some experimental issue → new independent measurement by Fermilab Muon g-2
NP beyond the Standard Model → no evidence about NP from LHC
Coherent combination of small effects in theory and experiment that reduces the discrepancy - mainly due to hadronic contribution: non direct estimation based on e+e- (tau) data - model dependent data analysis of hadronic interaction at low energies more precise experimental results and reliable theoretical model
Measured experimental distributions
“Bare” hadronic form factors/ cross section
Theoretical Model inspired by QCD :
hadronic form factors
Low energy data as input in HVP and HLbL
HVP and HLbL
estimation
Low energy hadronic interaction and Effective Field Theory
The QCD Lagrangian
with covariant derivative
The behaviour of the QCD strong coupling :
1 = (2 n
f – 33)/6
1 < 0 for n
f < 17
the coupling increases when the energy decreases :- asymptotic freedom at high energies - confiment at low energies: below ~1 GeV is to big to apply perturbative theory methods
For low energies (quark, gluons) → (new objects?/ light mesons) QCD → EFT ChPT that rem
The QCD Lagrangian
For u/d/s quarks for the energy about 1GeV the main part
with a small perturbation
For the chiral components
[the chiral components mixed only in ] Chiral invariant
is invariant under
whereas the ground state shows
Spontaneous symmetry breaking of chiral symmetry → 8 Goldstone bosons
The light pseudoscalar octet (, K, ) the best candidates for them.
Finite u/d/s quark masses → finite masses of Goldstone bosons
Stefan Scherer, hep-ph/0210398Introduction to Chiral Perturbation Theory
A theory that obeys for Lagrangian
and
for the ground states → Chiral Perturbation Theory
A natural choice the lightest pseudoscalar octet (, K, )
Chiral Perturbation Theory and inclusion of resonances
+ … , 10 terms
, 97 terms
p2/(4 F)2 < 1 p < M
770 MeV
p ~ Mresonance has to be included
The object is SU(3) matrix
Nambu-Goldstone boson of SSB of massless QCD
A series by a small parameter p2/(4 F)2
Chiral and gauge invariant Lagrangian with the minimal number of derivatives
LEC’s determined by low energy phenomenology, high energy behaviour of Green functions.
e.g. : →
Inclusion of resonances. Resonance Chiral Theory
From p ~ Mthe resonances have to be included
80’s Gasser&Leutwyler O(p2) chiral invariant Lagrangian with -resonance → generalization V, A, S, P in 90’s → Resonance Chiral Theory
R= V, A, S, P
Satisfies low (ChPT, by constraction) and high (QCD, by LEC’ resonance) energy limits → was applied for study of e+e- →hadrons and hadronic decays of tau-lepton
2 ways to realize A, V: vector and tensor formalisms, LEC’s depend on a chosen formalism
Tensor formalism
chiral and gauge invariant Lagrangian with the minimal number of derivatives
Single, lightest octet resonances(two-pion FF → p4 GB LECs = 0)
Measured experimental distributions
Monte Carlo generators:a technique to integrate restricted phase space;
a quality depends on used input (both theory and exp
data
Theoretical Model inspired by QCD :
hadronic form factors
fitting procedure:
limitations: syst err., reduced dimensionality, folded backgrounds
Theo
r diff
dis
tr li
mita
tions
:
unce
rtain
ass
umpt
ions
Fitt
ed m
odel
par
amet
ers do results of fitted theoretical model
represent results of measurements ???
Study of low energy hadronic data
Application of RChL for hadronic FFs
Hadronic Light by Light → Transition Form factors
LO
0
Experimentally measured TFF
Ti(x,y,z) kinematical functions
Where to measure TFF’s
Two-photon exchange in e+e- collisions
Single-Tag measurements (BaBar, Belle)
Double-Tag measurementsReconstruct both scattered lepton. Not measured yet!
For any setup: Measured cross section → MC (th. model) → TFF
TFF model for both virtualities
RChL with n resonance octets vector formulation n = 1, 2, 3
P = 0’
Chiral approach with vector resonances for pion and eta (eta’) mesons
H. Czyz, S. Ivashyn, A. Korchin, O.S., PRD 85 (2012) 094010
QCD driven behaviour(n+1) equations → 2n – (n+1) = (n-1) to be fitted
One-octet ansatz
no free parameters
116 exp points
Two-octet ansatz
1 parameter to fit →
PDG
Fit 116 exp points
Three-octet ansatz
2 parameters to fit strong correlation!!!
Two-octet ansatz included in EKHARAhttp://prac.us.edu.pl/~ekhara/
Contradictsother exp.
Belle2012 , to be included !
BaBar arXiv: 0905.4778
Influence of BaBar selection rules on the measured cross section
d(full) – d(approx)) /d(approx)
d(approx) = d(q22 = 0)
Dependence on Q2 for TFF’s. Not taking into account → a fake Q2 dependence for TFF
TFF of - mesons bigger (up to 6.5% ) than BaBar claims (4.6%)
EKHARA installed in BES III
Hadronic Vacuum Polarization → Hadronic e+e- cross section
How to estimate HVP
above ~ 1.8 GeV QCD is applied + narrow resonances ( J/ , Y)
Below ~ 1.8 GeV data for e+e-
had have to be “bare” → without RC
Two ways to measure (/ scan) had :
- direct scanning (Novosibirsk)
- radiative return (KLOE Frascati : + –)
Radiator function = QED RC analytically / by MC destroyed by FSR (models)
IDEAL
FSR is suppressed for small angle analysis < 15 ; 45 <
< 135
is not suppressed for large angle analysis 45 < < 135
Photon radiation in e+ e-- → P1 P2
ISR defined only by 1 Lorentz structure
(multiplied the pion FF)
FSRdefined by ? Lorentz structures
(multiplied by hadronic FF )
FSR tensor: general structure
charge congjugation, photon crossing symmetry, gauge invariance and one photon real → 3 Lorentz structures → Hadronic Form factors
Hadronic Form factors model dependent
Final state radiation in e+ e-- → P1 P2
below and about 1GeV
Vector resonance contribution
Scalar resonance contribution
Bremsstrahlung process (only for + – )
P1 P2 = (+ 000)
Calculation was done within RChL
S. Dubinsky et al. EPJC 40; S. Eidelman et al EPJC 69;G. Pancheri et al PLB 642; O. S. Comp. Phys. Comm 18-
Numerical results
neutral modes
Clear signal of Vector resonance mechanism
~ no Vector resonance mechanism
Numerical results +
PHOKHARA 6.1: KLOE study
PHOKHARA 6.1 MC of KLOE to study FSR; syst uncertainty related with FSR in a_mu^had
Forward- Backward asymmetry, large angle analysis
NLO HVP to muon AMM
aμhad ,γ=
α 2
3π2 ∫4mπ
2
smax
dss
R γ ( s )K ( s ) , R γ ( s )=σπ +π− ,γ (s )
σ μ+ μ−(s )
much below current experimental precision
diff sQED and RChL
>Ecut
estimation within sQED·VMD : 4.3·10 -11 (exp 4.9·10 -11)
- CVC to estimate HVP of AMM
to estimate HVP of AMM
TAUOLA (Monte Carlo generator for tau decay modes)
R. Decker, S.Jadach, M.Jezabek, J.H.Kuhn, Z. Was, Comp. Phys. Comm. 76 (1993) 361; ibid 70 (1992) 69, ibid 64 (1990) 275
Later: Cleo parametrization for 0 0 (Phys Rev D61, 012002)
Hadronic FF within VMD
3 scalar modes BW(V1)*BW(V2) , reproduces LO ChPT limit
RChL hadronic form factors for main 2P and 3P modes
KK →88% of tau hadronic width
Hadronic Decay Modes of tau
2P: 2 FFs (Lorentz structures)3P : 4 FFs (Lorentz structures)
RChL
RChL vs VMD
VMD
ChPT at least up to NLO + correct QCD behaviour
ChPT LO + correct QCD behaviour
wrong ChPT NLO
O.S, T. Przedzinski, P. Roig, Z. Was PRD D86
Based on the theoretically predicted values for the RChL
Deviation from the PDG central values 1-20% (exception 25-40% for KK mode)
Adding (1400) and (1700)
Fitting to BaBar preliminary data for mode
Fitting to Belle data for 0mode
RChL TAUOLA is used by LHCb
…… Belle II
Belle parametrization RChL
To get agreement we HAD to add sigma meson (phenomenologically)
I.Nugent et al PRD 88 OS JETP 102
CONCLUSIONS:
Hadronic contribution to muon AMM is the main restriction to its SM estimation
HVP and HlLbL estimated on the basis of experimental data
e+ e-- → hadrons ( →
+ hadrons) and e+ e-- →e+ e-- + hadrons
Data analysis equires theoretical calculations of Hadronic FF within
a QCD inspired model Resonance Chiral Lagrangian approach:
e+ e-- → (FSR) ; e+ e-- → ;) ;
t → nt + (2 ; 3 ; K K )
Implementation of the Hadronic FF in : PHOKHARA, EKHARA, TAUOLA
BaBar, KLOE BES Belle, LHCb
Fit of theoretical spectra within RChL to KLOE, Belle, BaBar data
PERSPECTIVES:
Belle II : Phase III Early 2019 start of data taking with the complete Belle II detectorintegrated luminosity: 50 ab -1 (50 x Belle)
Wide physics program: WG 8 “Low multiplicity & tau ” - gamma-gamma physics (TFF 1 and 2 mesons) - tau physics - low energy e + e -- → hadrons (radiative return)
Official MC: EKHARA, PHOKHARA, TAUOLA
Continuous work on: new theoretical results update of MC based on new theoretical results advanced fitting strategy to get hadronic model parameters
Update our knowledge about hadronic interactions (pole masses and vertex constants) → more precise estimation of HVP and HlbL of muon AMM to be compatible
New E989 (g-2)_mu in Fermilab (first physics run 2018, late 2018 - early 2019 BNL to
reproduce statistics ) with precision 1.6 · 10 -11
Measured experimental distributions
Monte Carlo generators:a technique to integrate restricted phase space;
a quality depends on used input (both theory and exp
data
Theoretical Model inspired by QCD :
hadronic form factors
My participation in study of hadronization
details can be found in ….
fitting procedure:
List of publications:
BACK SLIDES
Current status AMM. Summary
692.3 (4.2)
The SM value
Total:(on e+e-)
3.6σ
New experiment: Fermilab Muon g-2
Assuming no changes in the (g-2) central value the (exp - theory) discrepancy increases 5σ
Diff: 28.2 · 10-10
HADRONIC uncertainty dominates! Non direct estimation!!
NP beyond the Standard Model
It is heavy to expect a missed SM effect as large as (200-300)·10 -11 , i.e. logical posibilities:
Some experimental issue → new measurement by Fermilab Muon g-2
Coherent combination of small effects in theory and experiment that reduces the discrepancy - mainly due to hadronic contribution: non direct estimation based on e+e- (tau) data
Hadronic Light by Light
F.Jegerlehner&A.Nyfeller https://arxiv.org/pdf/0902.3360.pdf
n resonance octet
Similar for and H. Czyz et al, PRD 85 (2012) 094010
High energy behaviour of TFF
leads to restrictions for couplings
(n+1) equations → 2n – (n+1) = (n-1) constants to be fitted to data
n = 1 all parameters fixed, n = 2 - ONE to fit
The resonance masses from PDG
The slope of TFF’s at the origin
E799 experiment
Crystall Ball
SINDRUM I
NA60
http://prac.us.edu.pl/~ekhara/
Monte Carlo generator EKHARA
As a default two-octet parametrization
Not done yet
Comparison with measured cross section
BABAR event selection 0 : q22< 0.18 GeV2 q2
2< 0.38 GeV2
Discrepancy only with BaBar 2009
Bremsstrahlung (sQEDVMD)
But how good is
this approximation?
F(s) F(s)
F(s)
RChL
sQEDsQED
Beyond sQEDBeyond sQED
sQED VMD is reasonable for the final state
But what about final state ?
Can we use for FSR the same value of F(s) as for
S. Dubinsky et al, EPJC40(2005) 41
Charge asymmetry
big enough contribution due to RPT !
almost negligiblealmost negligible
s=1 GeV2FSR as background to ISR
RT parametrization
Tauola 2013 : inclusion of sigma meson
Tauola 2013 : inclusion of sigma meson
* alpha, beta are related for PT - correct inclusion based on PT structure* inclusion tensor resonances in RT framework J.J Sanz Cillero, O.S.
CLEO parametrization
F5
V
RT parametrization
OZI
Also K*(1400), (1450)
Also No yet and KKK modes with RT TAUOLA CPC
I. Nugent (BaBar Colaboration)
Tau Workshop, Cracow, 2013
RT TAUOLA (default) no OZI contribution
Not in TAUOLA
Goal of Fermilab E989
• A factor of 4 reduction in total error in aover BNL (0.54 ppm)
± 0.54 ppm total error
• Two things to notice:– statistical error dominates– systematic error is only 2.5 to 3 times larger than E989 goal
• How to improve:– get a hotter beam (Fermilab) (21 × statistics of BNL)– improve everything in systematics, which have many contributing factors
• Fermilab Goal: Equal statistical and systematic errors– ± 70 ppb for a and p. total: ± 100 ppb
– ± 100 ppb for statistics– Total error 140 ppb ( 0.14 ppm)
B. Lee Roberts - PhiPsi 2016- Mainz 26 June 2017 72
Fermilab Timescale
• This Year:– We are in first commissioning now until 7 July– We will turn back on in November and finish comissioning– US budget willing, we will then move to production running
• Anticipated results: (≃ 1, 5, 25 × BNL data set)– A BNL level data set should obtained relative quickly.
• We will stop data collection, and re-blind and keep running.• BNL level result perhaps by late 2018, early 2019.
– The next data set should give us half the BNL error– The final data set should give us one-fourth the BNL error.
B. Lee Roberts - PhiPsi 2016- Mainz 26 June 2017 73
June 2017 ~ 700,000 positrons (~2 weeks)
B. Lee Roberts - PhiPsi 2016- Mainz 26 June 2017 74
Particle: q = Qe moving in a magnetic field: momentum turns with cyclotron frequency C,
spin turns with S
Spin turns relative to the momentum with a
B. Lee Roberts - PhiPsi 2016- Mainz 26 June 2017 75
Spin Motion in a Magnetic Field
In a storage ring, we need vertical focusing
B. Lee Roberts - PhiPsi 2016- Mainz 26 June 2017 76
With an electric quadrupole field for vertical focusing and the magic 0
Measure two quantities
where B is expressed in terms of the Larmor frequency of a free proton