Baryogenesis, EDMs, and The Higgs Boson

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Baryogenesis, EDMs, and The Higgs Boson
M.J. Ramsey-Musolf Wisconsin-Madison
NPAC
Theoretical Nuclear, Particle, Astrophysics
Cosmology
http//www.physics.wisc.edu/groups/particle-theory
/
FNAL Seminar, Oct 2008
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What is the origin of baryonic matter ?
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Baryogenesis Myths

• EW baryogenesis requires a light SUSY Higgs boson
  (mH lt 120 GeV)
• EW baryogenesis requires SUSY with a light RH
  stop
• EDMs have nearly killed EW baryogenesis
• Leptogenesis is the most viable option

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Outline

• Baryogenesis General Features
• Computing YB systematically progress
  challenges
• Illustrative phenomenology in MSSM EDMs,
  Colliders, DM
• Probing EW phase transition w/ Higgs boson
  phenomenology

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Baryogenesis Scenarios
Baryogenesis When? CPV? SUSY? Neutrinos?
?
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Baryogenesis Ingredients
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EW Baryogenesis Standard Model
Anomalous Processes
Different vacua D(BL) DNCS
Sphaleron Transitions
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EW Baryogenesis Standard Model
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Baryogenesis New Electroweak Physics
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EDMs New CPV?

• SM background well below new CPV expectations
• New expts 102 to 103 more sensitive
• CPV needed for BAU?

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EWSB Higgs?

• SM background well below new CPV expectations
• New expts 102 to 103 more sensitive
• CPV needed for BAU?

LEPEWWG
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Baryogenesis EDMs Colliders
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Baryogenesis New Electroweak Physics
90s Cohen, Kaplan, Nelson
Joyce, Prokopec, Turok
Unbroken phase
CP Violation
Theoretical Issues Strength of phase
transition (Higgs sector) Bubble dynamics
(expansion rate) Transport at phase boundary
(non-eq QFT) EDMs many-body physics QCD
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Systematic Baryogenesis
Goal Derive dependence of YB on parameters
Lnew systematically (controlled approximations)

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Quantum Transport Baryogenesis
Electroweak Baryogenesis
Particle Propagation Beyond familiar (Peskin) QFT
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Quantum Transport Baryogenesis
Electroweak Baryogenesis
Scale Hierarchy
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Quantum Transport Equations
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Illustrative Study MSSM
Chargino Mass Matrix
Neutralino Mass Matrix
Resonant CPV M1,2 m
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Baryon Number MSSM
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Resonant CPV Relaxation
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Baryon Number GY
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Baryogenesis tan ? effects
Transport, Spectrum, EDMs
SUSY
Chung,Garbrecht, R-M, Tulin 0808.1144
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Baryogenesis New Electroweak Physics
90s Cohen, Kaplan, Nelson
Joyce, Prokopec, Turok
Unbroken phase
CP Violation
Theoretical Issues Strength of phase
transition (Higgs sector) Bubble dynamics
(expansion rate) Transport at phase boundary
(non-eq QFT) EDMs many-body physics QCD
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EDMs Complementary Searches
Improvements of 102 to 103
Electron
Neutron
Neutral Atoms
Deuteron
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EDMs Theory
Neutron
Neutral Atoms
Deuteron
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EDMs Schiff Moments
One-loop
EDM q, l, n
Chromo-EDM q, n
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One Loop EDMs Baryogenesis
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EDMs in SUSY
One-loop
EDM q, l, n
Chromo-EDM q, n
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EDMs in SUSY
One-loop
EDM q, l, n
Chromo-EDM q, n
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EDM constraints SUSY CPV
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Baryogenesis EDMs Colliders
Cirigliano, Profumo, R-M
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Dark Matter Future Experiments
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EDMs in SUSY Full Two-Loop
Higgs Boson Masses
Li, Profumo, R-M 0608.2693
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EDMs in SUSY Full Two-Loop
Higgs Boson Masses
Stronger limits on ?CPV for light Higgses large
tan?
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Baryogenesis EDMs Colliders
Higgs Boson Masses
Examples w/ tan?20, mstop 150 GeV mA1 TeV,
sin ??0.2 mA1 TeV, sin ??0.05
Stronger limits on ?CPV for light Higgses large
tan?
RH sbottom and stau masses correlated
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Baryogenesis EDMs Colliders
Higgsino Gaugino Mases
Larger mA EDM contours EWB regions contract
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Baryogenesis EDMs Colliders
Res ?? EWB not compatible with dn
Res non-res ?? EWB compatible with future dn ,
light mA, moderate tan?
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Baryogenesis New Electroweak Physics
90s Cohen, Kaplan, Nelson
Joyce, Prokopec, Turok
Unbroken phase
CP Violation
Theoretical Issues Strength of phase
transition (Higgs sector) Bubble dynamics
(expansion rate) Transport at phase boundary
(non-eq QFT) EDMs many-body physics QCD
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Electroweak Phase Transition Higgs
LEP EWWG
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Electroweak Phase Transition Higgs
LEP EWWG
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Electroweak Phase Transition Higgs
LEP EWWG
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The Simplest Extension
Model
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The Simplest Extension, Contd
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Finite Temperature Potential
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Finite Temperature Potential
Potential
Conditions
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Electroweak Symmetry Breaking
Strong first order EWPT
Potential parameters
Small ac limit
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Electroweak Symmetry Breaking
Strong first order EWPT
a1lt0, a2 either sign
a1b3 0, a2 lt 0
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Phenomenology
Colliders
EWPO favors light SM-like scalar
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Phenomenology
Colliders
Z2 Symmetry
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Complex Singlet EWB DM?
Barger, Langacker, McCaskey, R-M Shaugnessy
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Complex Singlet EWB DM?
Barger, Langacker, McCaskey, R-M Shaugnessy
?2 controls ?CDM? EWPT
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Summary

• EW baryogenesis remains a viable and testable
  mechanism for producing the observed baryon
  asymmetry
• Extensions of the Higgs sector of the SM can
  readily yield a strong 1st order EWPT, and these
  extensions can be probed at LHC and ILC
• Weve made progress in computing YB
  systematically, but challenges remain no ones
  (yet) perfect !
• EDM searches provide our most powerful probe of
  new EW CPV needed for YB

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Back Matter
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Baryogenesis EDMs Transport
Higgs Boson Masses
Stronger limits on ?CPV for light Higgses large
tan?
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Dark Matter Neutrinos in the Sun
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Dark Matter Relic Abundance
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Phenomenology EWPO
Electroweak Precision Observables (EWPO)
Oblique parameters
Similar for S,U
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Phenomenology EWPO contd
Electroweak Precision Observables (EWPO)
Oblique parameters
Global fit (GAPP)
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Quantum Transport Equations
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SUSY Baryogenesis Colliders
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LHC Phenomenology

Barger, Langacker, McCaskey, R-M, Shaughnessy
Discovery Potential
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LHC Phenomenology

Barger, Langacker, McCaskey, R-M, Shaughnessy
Discovery Potential
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LHC Phenomenology, contd

Barger, Langacker, McKaskey, R-M, Shaughnessy
Determining x
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ILC Phenomenology

(also WWF, ZZF)
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Scalar Sector the EWPT

• Simple extensions of the SM scalar sector (xSM)
  w/ small number of d.o.f. can readily lead to a
  strong, 1st order EWPT as needed for EW
  baryogenesis
• EWPT viable xSM can allow for heavier SM-like
  Higgs consistent with EWPO
• EWPT xSM can readily probed at the LHC and ILC
  using Higgs boson searches
• One can obtain an analytic criteria for
  parameters of xSM needed for 1st order EWPT that
  provides guidance for specific model realizations

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Symmetry Breaking
Two Cases for ltSgtat high T
Vmin 0
Vmin V0 lt 0
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Electroweak Symmetry Breaking
Critical Temperature
LEP allowed models TC 100 GeV
V0 / TC4 ltlt 1
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Extending the Higgs Sector
Ando, Barger, Langacker, Profumo, R-M,
Shaugnessy, Tulin
SUSY Beyond the MSSM
L soft
GUTs SU(5) example
Fileviez Perez, Patel, R-M
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SUSY Baryogenesis Colliders
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EDM constraints SUSY CPV
One-loop de slepton mass
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EDM constraints SUSY CPV
One-loop vs. Two-loop EDMs
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EDM constraints SUSY CPV
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Extending the Higgs Sector GUTs
SU(5) w/ extended Higgs sector
Implications

• Strong 1st order EWPT w/o SUSY ?
• New sources of CPV?
• Light triplet Higgs
• Light leptoquarks (unification)

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One-loop Finite T Contributions
Cylindrical Co-ordinates
Coleman-Weinberg
One-loop finite T
Ring sum plasma screening
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What is the origin of baryonic matter ?
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• Can an augmented Higgs sector
• Generate a strong 1st order EWPT ?
• Allow for a heavier SM-like Higgs than in the
  MSSM ?
• Alleviate the tension between direct Higgs
  search bounds and the EWPO ?
• Be discovered at the LHC ?
• Can its necessary characteristic probed at the
  LHC and a future ee- collider ?

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Cosmic Energy Budget
gg fusion at LHC