Theory Beyond the Standard Model (model building) Ann Nelson, - - PowerPoint PPT Presentation

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Theory Beyond the Standard Model (model building) Ann Nelson, - - PowerPoint PPT Presentation

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,


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SLIDE 1

Theory Beyond the Standard Model (model building)

Ann Nelson, August 4, 2013 Theory Community Issues Panel

Sunday, August 4, 2013

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SLIDE 2

“ideas are cheap. we need models”

  • H. Georgi
  • baryogenesis, dark matter, hierarchy, strong CP

, mν, flavor, unification

  • connect theory to phenomenology
  • explicit, motivated, consistent, inspiring, predictive
  • discover new mechanisms
  • new phenomena
  • inspire great experiments
  • inspire new experimental analyses

Why build (new) models?

Sunday, August 4, 2013

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SLIDE 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

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SLIDE 4
  • 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

Track Record

Sunday, August 4, 2013

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SLIDE 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

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SLIDE 6

Landscape of known and unknown unknowns

Stronger coupling to Standard Model Energy

Standard Model Gravity Dark Stuff

hidden sector? LHC

Sunday, August 4, 2013

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SLIDE 7

Intensity frontier/neutrino physics

  • dark energy scale ~ neutrino mass

~ Mw2/MPl~ one motivated range for m3/2 ~ 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: mν is new physics

Sunday, August 4, 2013

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SLIDE 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

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SLIDE 9

exotic νphysics

  • 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