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Nuclear Science

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Title: Nuclear Science


1
Nuclear 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
2
Fundamental Symmetries Cosmic History
3
Fundamental Symmetries Cosmic History
4
Fundamental 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?
5
Opportunity Unique role for low energy studies
in the LHC era
(and beyond!)
6
Primary Scientific Questions
7
Specific 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

8
The Origin of Matter Energy
Baryogenesis When? CPV? SUSY? Neutrinos?
?
9
Baryogenesis Ingredients
Sakharov Criteria
  • B violation
  • C CP violation
  • Nonequilibrium dynamics

Sakharov, 1967
10
Leptogenesis
11
0nbb-Decay LNV? Mass Term?
Dirac
Majorana
12
0nbb Mechanism mn
Impt to know if RPV interactions exist and, if
so, what magnitude
13
Lepton Flavor Number Violation
MEG Bm!eg 5 x 10-14
Mu2e Bm!e 5 x 10-17
Also PRIME
14
Lepton 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
15
Baryogenesis New Electroweak Physics
90s Cohen, Kaplan, Nelson
Joyce, Prokopec, Turok
Unbroken phase
CP Violation
16
EDM Probes of New CP Violation
17
EDMs New CPV?
Improvements of 102 to 103
Electron
Neutron
Neutral Atoms
Deuteron
18
Baryogenesis EDMs Colliders
19
Precision Probes of New Symmetries
New Symmetries
  • Origin of Matter
  • Unification gravity
  • Weak scale stability
  • Neutrinos

20
Precision Neutrino Property Studies
Mixing, hierarchy, CPV
Long baseline oscillation studies CPV? Normal or
Inverted ?
21
Precision Neutrino Property Studies
Solar Neutrinos
KamLAND
Borexino
CLEAN
LENS
22
Neutrino 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
23
Weak decays new physics
24
Correlations in Muon Decay mn
Model Independent Analysis
2005 Global fit Gagliardi et al.
Model Dependent Analysis
25
Weak Mixing in the Standard Model
26
Probing SUSY with PV Electron Scattering
27
Muon Anomalous Magnetic Moment
3.4 s !
28
Uncovering 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?
29
Back Matter
30
Neutrino Mass Magnetic Moments
Majorana vs Dirac mn ?
Effective theory for E lt L
Dirac
Majorana
31
Neutrino Mass Magnetic Moments
Majorana vs Dirac mn ?
Naturalness bounds on CW,B
Dirac
Majorana
7D mixing
5D matching
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