Baryogenesis, EDMs, and The Higgs Boson - PowerPoint PPT Presentation

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Baryogenesis, EDMs, and The Higgs Boson

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Explaining non-zero rB requires CP-violation and a scalar ... Chiral Relaxation. Strong sphalerons. Producing nL = 0. SCPV. GM , GH , GY , GSS. Approximations ... – PowerPoint PPT presentation

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Title: Baryogenesis, EDMs, and The Higgs Boson


1
Baryogenesis, EDMs, and The Higgs Boson
Higgs Phenomenology
Baryogenesis
  • V. Cirigliano LANL
  • C. Lee LBL
  • S. Tulin Caltech
  • S. Profumo UC Santa Cruz
  • G. Shaugnessy Wisconsin
  • V. Barger Wisconsin
  • P. Langacker IAS
  • M. McCaskey Wisconsin
  • D. OConnell IAS
  • G. Shaugnessy Wisconsin
  • M. Wise Caltech

PRD 71 075010 (2005) PRD 73 115009 (2006)
JHEP 0607002 (2006 ) JHEP 0807010 (2007)
PRD 75 037701 (2007) arXiv 0706.4311 hep-ph
2
What is the origin of baryonic matter ?
3
Outline
  • Baryogenesis General Features
  • Probing EW phase transition w/ Higgs boson
    phenomenology
  • Computing YB systematically progress
    challenges
  • Illustrative phenomenology in MSSM EDMs, DM,
    Colliders

4
The Origin of Matter Energy
Baryogenesis When? CPV? SUSY? Neutrinos?
?
5
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

6
Baryogenesis Ingredients
7
EW Baryogenesis Standard Model
Anomalous Processes
Different vacua D(BL) DNCS
Sphaleron Transitions
8
EW Baryogenesis Standard Model
9
Baryogenesis New Electroweak Physics
Unbroken phase
CP Violation
10
EDMs New CPV?
  • SM background well below new CPV expectations
  • New expts 102 to 103 more sensitive
  • CPV needed for BAU?

11
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
(numerical) Transport at phase boundary (non-eq
QFT) EDMs many-body physics QCD
12
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
13
Electroweak Phase Transition Higgs
LEP EWWG
14
Electroweak Phase Transition Higgs
LEP EWWG
15
Electroweak Phase Transition Higgs
LEP EWWG
16
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
17
The Simplest Extension
Model
18
The Simplest Extension, Contd
19
Finite Temperature Potential
20
Finite Temperature Potential
Potential
Conditions
21
Symmetry Breaking
Two Cases for ltSgtat high T
Vmin 0
Vmin V0 lt 0
22
Electroweak Symmetry Breaking
Critical Temperature
LEP allowed models TC 100 GeV
V0 / TC4 ltlt 1
23
Electroweak Symmetry Breaking
Strong first order EWPT
Potential parameters
Small ac limit
24
Electroweak Symmetry Breaking
Strong first order EWPT
a1lt0, a2 either sign
a1b3 0, a2 lt 0
25
Phenomenology EWPO
Electroweak Precision Observables (EWPO)
Oblique parameters
Similar for S,U
26
Phenomenology EWPO contd
Electroweak Precision Observables (EWPO)
Oblique parameters
Global fit (GAPP)
27
Phenomenology
Colliders
EWPO favors light SM-like scalar
28
Phenomenology
Colliders
Z2 Symmetry
29
LHC Phenomenology

Barger, Langacker, McCaskey, R-M, Shaughnessy
Discovery Potential
30
LHC Phenomenology

Barger, Langacker, McCaskey, R-M, Shaughnessy
Discovery Potential
31
ILC Phenomenology

(also WWF, ZZF)
32
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

33
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
34
Systematic Baryogenesis
Goal Derive dependence of YB on parameters
Lnew systematically (controlled approximations)

35
Quantum Transport Baryogenesis
Electroweak Baryogenesis
Particle Propagation Beyond familiar (Peskin) QFT
36
Quantum Transport Baryogenesis
Electroweak Baryogenesis
Scale Hierarchy
37
Quantum Transport Equations
38
Illustrative Study MSSM
Chargino Mass Matrix
Neutralino Mass Matrix
Resonant CPV M1,2 m
39
EDMs Baryogenesis
40
EDMs in SUSY
One-loop
EDM q, l, n
Chromo-EDM q, n
41
EDMs in SUSY
One-loop
EDM q, l, n
Chromo-EDM q, n
42
EDM constraints SUSY CPV
43
Baryogenesis EDMs Colliders
Cirigliano, Profumo, R-M
44
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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