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ParityViolation with Electrons: Theoretical Perspectives

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Title: ParityViolation with Electrons: Theoretical Perspectives


1
Parity-Violation with Electrons Theoretical
Perspectives
M.J. Ramsey-Musolf
2
PV Past, Present, Future
3
PV Past, Present, Future
4
PV Past, Present, Future
5
Quarks, Gluons, the Light Elements
Lattice QCD
6
Strange Quarks in the NucleonWhat have we
learned?
Jaffe 89 Hammer, Meissner, Drechsel 95
  • Dispersion Relations
  • Narrow Resonances
  • High Q2 ansatz

7
Strange Quarks in the NucleonWhat have we
learned?
8
Strange Quarks in the Nucleon What have we
learned?
  • Strange quarks dont appear in Quark Model
    picture of the nucleon
  • Perturbation theory may not apply

?QCD / ms 1 No HQET
mK / ?c 1/2 ?PT ?
  • Symmetry is impotent

J?s J?B 2 J?EM, I0
9
Q2 -dependenceof GsM
10
Lattice Computations
See also Leinweber et al
Dong, Liu, Williams (1998)
Lewis, Wilcox, Woloshyn (2003)
  • Quenched QCD
  • Wilson fermions
  • 2000 gauge configurations
  • 60-noise estimate/config
  • Quenched QCD
  • Wilson fermions
  • 100 gauge configurations
  • 300-noise estimate/config

11
Lattice Computations
Leinweber et al
12
What ?PT can (cannot) say
Ito, R-M Hemmert, Meissner, Kubis
Hammer, Zhu, Puglia, R-M
Strange magnetism as an illustration
13
What ?PT can (cannot) say
Strange magnetism as an illustration
14
Dispersion theory
Jaffe Hammer,
Drechsel, R-M
15
Dispersion theory
Hammer R-M
16
Dispersion theory
Hammer R-M
17
Dispersion theory
Models expt suggest cancellations
18
Combining ?PT, dispersion theory, lattice QCD
SAMPLE
19
Radiative Corrections the Hadronic Weak
Interaction
  • GAe
  • N !D
  • PV p photo- and electro-production (threshold)
  • Vector analyzing power (gg)

20
at Q20.1 (GeV/c)2
  • s-quarks contribute less than 5 (1s) to the
    protons magnetic form factor.
  • protons axial structure is complicated!

R. Hasty et al., Science 290, 2117 (2000).
21
Axial Radiative Corrections
22
Anapole Effects
Hadronic PV
Cant account for a large reduction in GeA
23
Nuclear PV Effects
PV NN interaction
Carlson, Paris, Schiavilla Liu,
Prezeau, Ramsey-Musolf
24
SAMPLE Results
R. Hasty et al., Science 290, 2117 (2000).
at Q20.1 (GeV/c)2
  • s-quarks contribute less than 5 (1s) to the
    protons magnetic moment.

200 MeV update 2003 Improved EM radiative
corr. Improved acceptance model Correction for p
background
125 MeV no p background similar sensitivity to
GAe(T1)
E. Beise, U Maryland
25
Transition Axial Form Factor
Off Diagonal Goldberger-Treiman Relation
26
Measuring GAND(Q2)
27
Weak interactions of s-quarks are puzzling
Hyperon weak decays
28
Weak interactions of s-quarks are puzzling
29
Weak interactions of s-quarks are puzzling
Resonance saturation
Holstein Borasoy
S11 Roper
30
Weak interactions of s-quarks are puzzling
Resonance saturation
Holstein Borasoy
S11 Roper
31
Weak interactions of s-quarks are puzzling
32
We have a DS0 probe
Use PV to filter out EM transition
Zhu, Maekawa, Holstein, MR-M
33
We have a DS0 probe
Naïve dimensional analysis (NDA)
Resonance saturation
34
Measuring dD
35
N!D Transition
36
Vector Analyzing Power
  • T-odd, P-even correlation
  • Doubly virtual compton scattering (VVCS) new
    probe of nucleon structure
  • Implications for radiative corrections in
    other processes GEp/GMp, b-decay
  • SAMPLE, Mainz, JLab experiments

37
Vector Analyzing Power
Vg VVCS Re Mg(MggboxMggcross) Rosenbluth Im
MgMggbox VAP
VW,Z Electroweak VVCS Re MV(MVgboxMVgcross) b-
decay, RA, Im MVMVgbox b-decay
T-violation
38
Vector Analyzing Power
39
Vector Analyzing Power
40
Radiative Corrections the Hadronic Weak
Interaction
  • GAe
  • N !D
  • PV p photo- and electro-production (threshold)
  • Vector analyzing power (gg)

41
Weak Mixing Angle Scale Dependence
Czarnecki, Marciano Erler, Kurylov, MR-M
42
Comparing Qwe and QWp
Kurylov, Su, MR-M
43
Comparing Qwe and QWp
Erler, Kurylov, R-M
44
Additional PV electron scattering ideas
Czarnecki, Marciano Erler et al.
45
Comparing Qwe and QWp
Kurylov, R-M, Su
??? SUSY dark matter
46
Comparing AdDIS and Qwp,e
47
Comparing Qwe and QWp
Kurylov, R-M, Su
??? SUSY dark matter
48
Higher Twist Pollution
49
Higher Twist Pollution
50
Tasks for the modern era future
Strange quarks
  • Finish the experimental program
  • Credible, unquenched lattice calculations

Rad corrections
  • Further tests of electroweak VVCS with N!D, VAP
  • Theory quark mass (mp) dependence
  • Measure dD

SM new physics
  • DIS-Parity Is there significant I-violation as
    suggested by NuTeV?
  • Theory how big is twist pollution?
  • Theory relating rn(r) APV

Hardronic PV
  • Lots of new expt theory.
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