Title: Future Directions in Parity Violation: From Quarks to the Cosmos
1Future Directions in Parity Violation From
Quarks to the Cosmos
many students, post-docs, collaborators, and
colleagues
PAVI 06 MHLOS
2Fundamental Symmetries Cosmic History
What are the fundamental symmetries that have
governed the microphysics of the evolving
universe?
- Parity violation as a probe of the
protons internal structure (sea quarks, twist) - Parity violation as probe of the hadronic weak
interaction - Parity violation as a probe of additional
symmetries of the early universe
3Fundamental Symmetries Cosmic History
4Fundamental Symmetries Cosmic History
SM unfinished business
What is the internal landscape of the proton?
Sea quarks, gluons, qq, qqg correllations
5Probing the strange sea with PV
GMs 0.28 /- 0.20 GEs -0.006 /- 0.016 3
/- 2.3 of proton magnetic moment 20 /- 15
of isoscalar magnetic moment 0.2 /- 0.5 of
Electric distribution
Consistent with s-quark contributions to mP JP
but smaller than early theoretical expectations
Preliminary
Courtesy of Kent Pashke (U Mass)
6Probing Higher Twist Beyond the Parton Model
2xF1 Experimental Status
Data from JLab E94-110 (nucl-ex/0410027,
submitted to PRL) Courtesy C Keppel
7n 2 Cornwall-Norton Moments
F2
F2, F1 in excellent agreement with NNLO TM
above Q2 2 GeV2 No (or canceling) higher
twists Yet, dominated by large x and resonance
region Remove known HT (a bit novel), the
elastic, and there is no more down to Q2 0.5
GeV2 The case looks different for FL (data or
curve?)
2xF1
FL
8Probing Higher Twist with PV
9Fundamental Symmetries Cosmic History
SM unfinished business
How do weak interactions of hadrons reflect the
weak qq force ? Are QCD symmetries (chiral,
large NC,) applicable? Is there a long range
weak NN interaction?
10Weak Interactions of Hadrons Strange?
Hyperon weak decays
11Weak Interactions of Hadrons Strange?
12Weak Interactions of S0 Hadrons Strange?
What does QCD predict ?
13Weak Interactions of S0 Hadrons Strange?
Use parity-violation to filter out EM strong
interactions
Desplanques, Donoghue, Holstein (DDH)
14Is the weak NN force short range ?
15Is the weak NN force short range ?
16Hadronic PV Effective Field Theory
PV Potential
Long Range
Short Range
Medium Range
Zhu, Maekawa, Holstein, R-M, van Kolck 05 R-M
Page 06
17Hadronic PV Effective Field Theory
PV Current Operators
Long Range
Medium Range
Short Range
18Hadronic PV Few-Body Systems
Pionless theory
Ab initio few-body calcs
19Hadronic PV Theoretical Challenges
20Hadronic PV 0n bb - decay
21Hadronic PV 0n bb - decay
22Hadronic PV as a probe
- Determine VPV through O (p) from PV low-energy
few-body studies where power counting works - Re-analyze nuclear PV observables using this VPV
- If successful, we would have some indication
that operator power counting works in nuclei - Apply to 0nbb-decay
Prezeau, R-M, Vogel
23Fundamental Symmetries Cosmic History
Puzzles the Standard Model cant solve
- Origin of matter
- Unification gravity
- Weak scale stability
- Neutrinos
What are the symmetries (forces) of the early
universe beyond those of the SM?
24PV as a Probe of New Symmetries
Puzzles the Standard Model cant solve
- Origin of matter
- Unification gravity
- Weak scale stability
- Neutrinos
What are the implications of mn and PV expts for
possible new symmetries forces?
25PV as a Probe of New Symmetries
Unseen Forces Supersymmetry ?
- Unification gravity
- Weak scale stability
- Origin of matter
- Neutrinos
26PV Correlations in Muon Decay mn
27PV Correlations in Muon Decay mn
Model Independent Analysis
2005 Global fit Gagliardi et al.
Model Dependent Analysis
28Weak decays new physics
29Weak decays PV
30Weak decays PV
31Weak decays PV Correlations
32Probing SUSY with PV eN Interactions
??? SUSY dark matter
?? -gt e??e
Kurylov, Su, MR-M
33Probing SUSY with PV eN Interactions
34Probing SUSY with PV eN Interactions
Kurylov, R-M, Su
??? SUSY dark matter
35Fundamental Symmetries Cosmic History
Baryogenesis When? SUSY? Neutrinos? CPV?
WIMPy D.M. Related to baryogenesis?
New gravity? Lorentz violation? Effects on CMB?
?
36What is the origin of baryonic matter ?
37Baryogenesis New Electroweak Physics
90s Cohen, Kaplan, Nelson
Joyce, Prokopec, Turok
Unbroken phase
CP Violation
38EDM Probes of New CP Violation
39Baryogenesis Dark Matter MSSM
Chargino Mass Matrix
Neutralino Mass Matrix
40EDM constraints SUSY CPV
41Dark Matter Future Experiments
42EDMs, Baryogenesis, Dark Matter
- Continued progress in performing
systematic computations of the baryon asymmetry - Continued scrutiny of QCD nuclear
structure uncertainties in EDM computations - Comprehensive phenomenology with other models
of new CPV (extended Higgs sector) - Funding for experiments !
43Future Directions
- Parity violation in electron scattering and
hadronic interactions will continue to provide
new insights into protons internal structure
and weak qq interactions - PV in weak decays and electron scattering will
continue to provide insights into new physics
(SUSY, ns, Higgs) that will complement LHC, ILC
probes - PVTV will provide powerful probe of the origin
of baryonic matter and non-baryonic dark matter
Considerable theoretical and experimental
challenges and opportunities remain PAVI must
go on!