Transport Theory for EW Baryogenesis & Leptogenesis · 3 Transport Issues • How robustly can one...
Transcript of Transport Theory for EW Baryogenesis & Leptogenesis · 3 Transport Issues • How robustly can one...
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Transport Theory for EWBaryogenesis & Leptogenesis
M.J. Ramsey-MusolfWisconsin-MadisonU Mass-Amherst
Snowmass CSS, August 2013
Amherst Center forFundamental Interactions
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Key Points
• Robust tests of low-scale baryogenesis scenarios !Refine theoretical machinery for computingasymmetries in out-of-equilibrium contexts
• Pioneering work utilized conventional Boltzmannframework
• Recent advances exploiting Schwinger-Keldysh/CTP formulation are providing a moresystematic treatment
• Considerable room for future theoretical progressexists
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Transport Issues
• How robustly can one predict charge asymmetries ( nleft, Yl , YX…) ?
• What is the role of CP-conserving dynamics ?
• CPV sources in EWB (MSSM…)
• CPV decays in leptogenesis (soft lepto)
• Particle number changing rxns in EWB
• Washout in leptogenesis, asym DM…
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Outline
I. Transport dynamics in CTP
II. CPV sources in EWB & softLeptogenesis
III. Particle number changing reactionsin EWB
IV. Flavored CPV & EWB
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
!
˜ G (x, y) = P"a (x)"b* (y) # ab =
Gt (x, y) $G<(x,y)G>(x, y) $Gt (x, y)
%
& '
(
) *
CTP or Schwinger-Keldysh Green’s functions
• Appropriate for evolution of “in-in” matrix elements
• Contain full info on number densities: nαβ• Matrices in flavor space: (e,µ,τ) , ( tL, tR ), …
~ ~
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
= + + …
!
˜ G
!
˜ G 0 +
!
˜ G 0
!
˜ G 0
!
˜ "
!
˜ G (x, y) = P"a (x)"b* (y) # ab =
Gt (x, y) $G<(x,y)G>(x, y) $Gt (x, y)
%
& '
(
) *
CTP or Schwinger-Keldysh Green’s functions
• Appropriate for evolution of “in-in” matrix elements
• Contain full info on number densities: nαβ• Matrices in flavor space: (e,µ,τ) , ( tL, tR ), …
~ ~
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Systematic Baryo/leptogenesis:
Scale Hierarchies
Thermal, but not too dissipative
Gradient expansion
Quasiparticle description
εw = vw (kw / ω ) << 1
εp = Γp / ω << 1
Plural, but not too flavored
εcoll = Γcoll / ω << 1
εosc = Δω / T << 1
EW Baryogenesis Leptogenesis
εLNV = ΓLNV / ΓΗ < 1
Gradient expansion
Quasiparticle description
εp = Γp / ω << 1
Thermal, but not too dissipative
εcoll = Γcoll / ω << 1
! power counting
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
Kinetic eq (approx) in Wigner space: Lowest non-trivial order in grad’s
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
Diagonal after rotation to local mass basis:
!
M 2 X( ) =U + m2 X( )U
!
"µ X( ) =U +#µU~ ~( tL, tR ) ! ( t1, t2 )
~ ~
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
Flavor oscillations: flavor off-diag densities
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
CPV in m2(X): for EWB, arises from spacetimevarying complex phase(s) generated byinteraction of background field(s) (Higgs vevs)with quantum fields
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
CPV in m2(X): for EWB, arises from spacetimevarying complex phase(s) generated byinteraction of background field(s) (Higgs vevs)with quantum fields
How large is CPV source ? Riotto; Carena et al;Prokopec et al; Cline et al; Konstandin et al; Cirigliano etal; Kainulainen….
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
CPV in m2(X): for EWB, arises from spacetimevarying complex phase(s) generated byinteraction of background field(s) (Higgs vevs)with quantum fields
✔
✔ = recent progressResonant enhancement ofCPV sources for small εosc
Cirigliano et al
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CPV Sources: EW BaryogenesisCPV Sources: how large a sinφCPV necessary ?
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
VEV insert approx
• Riotto• Carena et al• Cirigliano et al
Resummed vevs
• Konstandin,Prokpec, Schmidt
Resummed vevs
• Cirigliano et al
Large resonantenhancement butnot realistic insmall εosc regime
Exact solution in two-flavor toy model:large resonantenhancement
Small resonanteffect but neglecteddiffusion and off-diag Σii Gij terms
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CPV Sources: EW BaryogenesisCPV Sources: how large a sinφCPV necessary ?
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
VEV insert approx
• Riotto• Carena et al• Cirigliano et al
Resummed vevs
• Konstandin,Prokpec, Schmidt
Resummed vevs
• Cirigliano et al
Large resonantenhancement butnot realistic insmall εosc regime
Exact solution in two-flavor toy model:large resonantenhancement
Small resonanteffect but neglecteddiffusion and off-diag Σii Gij terms
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CPV Sources: EW BaryogenesisCPV Sources: how large a sinφCPV necessary ?
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
VEV insert approx
• Riotto• Carena et al• Cirigliano et al
Resummed vevs
• Konstandin,Prokpec, Schmidt
Resummed vevs
• Cirigliano et al
Large resonantenhancement butnot realistic insmall εosc regime
Exact solution in two-flavor toy model:large resonantenhancement
Small resonanteffect but neglecteddiffusion and off-diag Σii Gij terms
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CPV Sources: EW BaryogenesisCPV Sources: how large a sinφCPV necessary ?
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
VEV insert approx
• Riotto• Carena et al• Cirigliano et al
Resummed vevs
• Konstandin,Prokpec, Schmidt
Resummed vevs
• Cirigliano et al
Neglect o-d Σii Gijterms & approx Λ
Fullsolution
Large resonantenhancement butnot realistic insmall εosc regime
Exact solution in two-flavor toy model:large resonantenhancement
Small resonanteffect but neglecteddiffusion and off-diag Σii Gij terms
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CPV Sources: EW BaryogenesisCPV Sources: how large a sinφCPV necessary ?
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
VEV insert approx
• Riotto• Carena et al• Cirigliano et al
Resummed vevs
• Konstandin,Prokpec, Schmidt
Resummed vevs
• Cirigliano et al
Neglect o-d Σii Gijterms & approx Λ
Fullsolution
Large resonantenhancement butnot realistic insmall εosc regime
Exact solution in two-flavor toy model:large resonantenhancement
Small resonanteffect but neglecteddiffusion and off-diag Σii Gij terms
Next steps:
1. Apply to realistic model (MSSM)
2. Fermions
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
Leptogenesis
CPV decays
Washout
Flavor sensitive rxns
Gauge interactions
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CPV Asymmetries: Soft LeptogenesisFormalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
Soft Leptogenesis 0901.0008,1009.0003, 1107.5312
Including finite-T statistics for externalstates in Boltzmann equations
Sizeable Yl withTeV scale dof:
Interestingphenomenology ?
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CPV Asymmetries: Soft LeptogenesisFormalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
Soft Leptogenesis 1307.0524, Garbrecht & MR-M
Vanishing Yl : canceling contributions when stat’s included on all lines
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Systematic Baryo/leptogenesis:Formalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
EW Baryogenesis
ACPBSM ! ACP
SM
“Superequilibrium”
Diffusion
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Collision Terms: Transfer ReactionsFormalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
MSSM: ~ 30 Coupled Eqns
Topological transitions
MSSM: Chung, Garbrecht, R-M, Tulin ‘09
Bubble interior
Bubble exterior
LH leptons
LH quarksLH fermions
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Collision Terms: Transfer ReactionsFormalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
MSSM: ~ 30 Coupled Eqns
Thanks: B. Garbrecht
Topological transitions
MSSM: Chung, Garbrecht, R-M, Tulin ‘09
Bubble interior
Bubble exterior
LH leptons
LH quarksLH fermions
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Collision Terms: Transfer ReactionsFormalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
Small tanβ
tanβ=20
muon g-2 !
Chung, Garbrecht, R-M, Tulin
MSSM: ~ 30 Coupled Eqns
Thanks: B. Garbrecht
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New Direction: Flavored CPV & EWBFormalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
General 2HDM
?
!(x)bs
Liu, R-M, Shu ‘11;see also Tulin &Winslow ‘11; Clineet al ‘11
Combinationof Hu,d vevs
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New Direction: Flavored CPV & EWBFormalism: Kadanoff-Baym to Boltzmann
Kinetic eq (approx) in Wigner space:
!
2k " #X G< k,X( ) = $i M 2 X( ),G< k,X( )[ ] $ 2 k " %,G< k,X( )[ ] + & G k,X( )[ ]
General 2HDM
Liu, R-M, Shu ‘11;see also Tulin &Winslow ‘11; Clineet al ‘11
constant nB / s
LHCb
Tevatron w/osame-sign Aµµ
Tevatron: same-sign Aµµ
included
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Outlook
• Robust tests of low-scale baryogenesis scenarios !Refine theoretical machinery for computingasymmetries in out-of-equilibrium contexts
• Important for evaluating viability of TeV scalescenarios in light of phenomenological input: EDMs,flavored CPV, precision tests (g-2,…)
• Recent advances exploiting Schwinger-Keldysh/CTP formulation are providing a moresystematic treatment
• Considerable room for future theoretical progressexists: fermion CPV sources, low-scaleleptogenesis…