Title: Nuclear Science
1Nuclear Science the New Standard Model
Neutrinos Fundamental Symmetries in the Next
Decade
Fifty years of PV in nuclear physics
Solar ns the neutrino revolution
Michael Ramsey-Musolf, INPC 2007
2Fundamental Symmetries Cosmic History
3Fundamental Symmetries Cosmic History
4Fundamental 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?
5Opportunity Unique role for low energy studies
in the LHC era
(and beyond!)
6 Primary Scientific Questions
7Specific Opportunities
- Major Discovery Potential
- 0nbb-decay EDM
- Precision measurements
- Neutrino mixing hierarchy
- Weak decays, PVES, gm-2
- Electroweak probes of QCD
- PVES, Hadronic PV, nN scatt
8The Origin of Matter Energy
Baryogenesis When? CPV? SUSY? Neutrinos?
?
9Baryogenesis Ingredients
Sakharov Criteria
- B violation
- C CP violation
- Nonequilibrium dynamics
Sakharov, 1967
10Leptogenesis
110nbb-Decay LNV? Mass Term?
Dirac
Majorana
120nbb Mechanism mn
Impt to know if RPV interactions exist and, if
so, what magnitude
13Lepton Flavor Number Violation
MEG Bm!eg 5 x 10-14
Mu2e Bm!e 5 x 10-17
Also PRIME
14Lepton Flavor Number Violation
Raidal, Santamaria Cirigliano, Kurylov, R-M,
Vogel
MEG Bm!eg 5 x 10-14
Logarithmic enhancements of R
Mu2e Bm!e 5 x 10-17
15Baryogenesis New Electroweak Physics
90s Cohen, Kaplan, Nelson
Joyce, Prokopec, Turok
Unbroken phase
CP Violation
16EDM Probes of New CP Violation
17EDMs New CPV?
Improvements of 102 to 103
Electron
Neutron
Neutral Atoms
Deuteron
18Baryogenesis EDMs Colliders
19Precision Probes of New Symmetries
New Symmetries
- Origin of Matter
- Unification gravity
- Weak scale stability
- Neutrinos
20Precision Neutrino Property Studies
Mixing, hierarchy, CPV
Long baseline oscillation studies CPV? Normal or
Inverted ?
21Precision Neutrino Property Studies
Solar Neutrinos
KamLAND
Borexino
CLEAN
LENS
22Neutrino Mass Magnetic Moments
Bell, Cirigliano, Gorshteyn,R-M, Vogel, Wang,
Wise Davidson, Gorbahn, Santamaria
How large is mn ?
Experiment mn lt (10-10 - 10-12) mB e
scattering, astro limits
Radiatively-induced mn
Both operators chiral odd
23Weak decays new physics
24Correlations in Muon Decay mn
Model Independent Analysis
2005 Global fit Gagliardi et al.
Model Dependent Analysis
25Weak Mixing in the Standard Model
26Probing SUSY with PV Electron Scattering
27Muon Anomalous Magnetic Moment
3.4 s !
28Uncovering the New Standard Model
Baryon asymmetry?
Lepton Number Violation ?
Neutrino Mass ? Mixing ? Sterile ns ?
What is the New Standard Model ?
New Forces?
Weak Scale CP- Violation ?
Supersymmetry ? Extra Dimensions ?
Baryon asymmetry?
29Back Matter
30Neutrino Mass Magnetic Moments
Majorana vs Dirac mn ?
Effective theory for E lt L
Dirac
Majorana
31Neutrino Mass Magnetic Moments
Majorana vs Dirac mn ?
Naturalness bounds on CW,B
Dirac
Majorana
7D mixing
5D matching