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Theory Beyond the Standard Model (model building) Ann Nelson, August 4, 2013 Theory Community Issues Panel Sunday, August 4, 2013 Why build (new) models? ideas are cheap. we need models H. Georgi baryogenesis, dark matter,


  1. Theory Beyond the Standard Model (model building) Ann Nelson, August 4, 2013 Theory Community Issues Panel Sunday, August 4, 2013

  2. Why build (new) models? “ideas are cheap. we need models” H. Georgi • baryogenesis, dark matter, hierarchy, strong CP , m ν , flavor, unification • connect theory to phenomenology • explicit, motivated, consistent, inspiring, predictive • discover new mechanisms • new phenomena • inspire great experiments • inspire new experimental analyses Sunday, August 4, 2013

  3. inspiration • …..LHC • GUTs inspire proton decay search • proton decay searches find SN1987A neutrinos and discover atmospheric neutrino oscillations • Large extra dimensions inspire torsion balance short distance tests of Newton’s law • discover that laws of gravity do not change on submillimeter scale • axions inspire microwave cavity expts Sunday, August 4, 2013

  4. Track Record • Theorists have been immensely successful at discovering good/correct models • Standard Model • Neutrino seesaw • “We have a very limited palette” - Sidney Coleman • Terrible track record at guessing parameters • top mass, Vcb, neutrino mixing, neutrino mass Sunday, August 4, 2013

  5. LHC era • “All your models are wrong” “we just need models to cover the signature space” • range of models cover many triggers and analyses • Large number of exotic models hugely expands breadth and interest of LHC • “hidden valley” → long lived particle triggers • History: expect surprises in the parameters • may need the right model to correlate different categories of events to get a discovery • some motivated reasons susy could be “stealthy” Sunday, August 4, 2013

  6. Landscape of known and unknown unknowns LHC Energy Standard Model hidden sector? Gravity Dark Stuff Stronger coupling to Standard Model Sunday, August 4, 2013

  7. Intensity frontier/neutrino physics • dark energy scale ~ neutrino mass ~ M w2 /M Pl ~ one motivated range for m 3/2 ~ short distance gravity test scale • just as strong reasons to think about new, weakly coupled low scale physics as new TeV physics • naturalness • dark sector • experimental hints • guaranteed BSM: m ν is new physics Sunday, August 4, 2013

  8. New phenomena in neutrino sector • LBNE has a great “bread and butter physics” program • measuring CPV, mass hierarchy (analogous to LHC measurement of Higgs properties) • Needs a “new physics” complement • neutrinos are a possible portal to any hidden sector containing light fermion X • l H X operator is renormalizable • X mixes with neutrinos, is ‘sterile neutrino’ • X can have other interactions, be part of dark matter and/or dark energy ‘sector’ Sunday, August 4, 2013

  9. exotic ν physics • possible connection with dark energy (MaVaNs) • ‘sterile neutrinos’ with parameters “forbidden” by cosmology and astrophysics • nonunitary in neutrino mixing matrix • nonstandard CPV • anomalous dependence on L/E • anomalous matter effects Sunday, August 4, 2013

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