Title: Baryogenesis, EDMs, and The Higgs Boson
1Baryogenesis, 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
2What is the origin of baryonic matter ?
3Outline
- Baryogenesis General Features
- Probing EW phase transition w/ Higgs boson
phenomenology - Computing YB systematically progress
challenges - Illustrative phenomenology in MSSM EDMs, DM,
Colliders
4The Origin of Matter Energy
Baryogenesis When? CPV? SUSY? Neutrinos?
?
5Baryogenesis 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
6Baryogenesis Ingredients
7EW Baryogenesis Standard Model
Anomalous Processes
Different vacua D(BL) DNCS
Sphaleron Transitions
8EW Baryogenesis Standard Model
9Baryogenesis New Electroweak Physics
Unbroken phase
CP Violation
10EDMs New CPV?
- SM background well below new CPV expectations
- New expts 102 to 103 more sensitive
- CPV needed for BAU?
11Baryogenesis 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
12Baryogenesis 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
13Electroweak Phase Transition Higgs
LEP EWWG
14Electroweak Phase Transition Higgs
LEP EWWG
15Electroweak Phase Transition Higgs
LEP EWWG
16Extending 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
17The Simplest Extension
Model
18The Simplest Extension, Contd
19Finite Temperature Potential
20Finite Temperature Potential
Potential
Conditions
21Symmetry Breaking
Two Cases for ltSgtat high T
Vmin 0
Vmin V0 lt 0
22Electroweak Symmetry Breaking
Critical Temperature
LEP allowed models TC 100 GeV
V0 / TC4 ltlt 1
23Electroweak Symmetry Breaking
Strong first order EWPT
Potential parameters
Small ac limit
24Electroweak Symmetry Breaking
Strong first order EWPT
a1lt0, a2 either sign
a1b3 0, a2 lt 0
25Phenomenology EWPO
Electroweak Precision Observables (EWPO)
Oblique parameters
Similar for S,U
26Phenomenology EWPO contd
Electroweak Precision Observables (EWPO)
Oblique parameters
Global fit (GAPP)
27Phenomenology
Colliders
EWPO favors light SM-like scalar
28Phenomenology
Colliders
Z2 Symmetry
29LHC Phenomenology
Barger, Langacker, McCaskey, R-M, Shaughnessy
Discovery Potential
30LHC Phenomenology
Barger, Langacker, McCaskey, R-M, Shaughnessy
Discovery Potential
31ILC Phenomenology
(also WWF, ZZF)
32Scalar 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
33Baryogenesis 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
34Systematic Baryogenesis
Goal Derive dependence of YB on parameters
Lnew systematically (controlled approximations)
35Quantum Transport Baryogenesis
Electroweak Baryogenesis
Particle Propagation Beyond familiar (Peskin) QFT
36Quantum Transport Baryogenesis
Electroweak Baryogenesis
Scale Hierarchy
37Quantum Transport Equations
38Illustrative Study MSSM
Chargino Mass Matrix
Neutralino Mass Matrix
Resonant CPV M1,2 m
39EDMs Baryogenesis
40EDMs in SUSY
One-loop
EDM q, l, n
Chromo-EDM q, n
41EDMs in SUSY
One-loop
EDM q, l, n
Chromo-EDM q, n
42EDM constraints SUSY CPV
43Baryogenesis EDMs Colliders
Cirigliano, Profumo, R-M
44Summary
- 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