Electric Dipole Moments and Sources of CP violation
σ σ
Jordy de Vries, UMass Amherst, RIKEN BNL Research Center Goals
§ Goal 1: A crash course in Electric Dipole Moments
• What are EDMs and why do people bother to find them? • Overview of EDM theory and experimental landscape (I’m a theorist…)
§ Goal 2: Put EDMs in a broader context (LHC/flavor/….)
• How do EDM measurements complement other searches ?
Excellent reviews: Pospelov/Ritz ‘05, Engel/van Kolck/Ramsey Musolf ’13 Outline
§ Part I: What are EDMs and why do (should) we care ?
§ Part II: Sources of CP violation: an EFT approach §
§ Part III: Classes of EDM searches + theoretical interpretation Magnetic dipole moments
• Let’s remind ourselves about magnetic dipole moments • Particle at rest with spin (i.e. electron) in magnetic field is described by ω ! ! eg ! ! µ = H = −µ (S ⋅ B) S = σ / 2 2m ! B ! Spin Magnetic Field σ
Magnetic dipole moment
• The B-field puts a torque on the system à spin precession ω = 2µB sinθ
• Dirac equation predicts tree-level magnetic moment Magnetic dipole moments Aµ
µ 1 eu¯(p0) u(p)A e ( † )A † B µ ! 0 2m · e e
µ ! ! eg • Dirac predicts: H = − (σ ⋅ B) µ = g =2 2 2m
• g is the gyromagnetic ratio (clasically g=1), triumph of QM ! -11 • Electron magnetic moment ~ e/me ~ 10 e cm ~ 100 e fm
• Measurements in 1940’s: ge = 2*(1.00118+-0.00003)….. • Enter Quantum Field Theory
↵ a = em + (↵2 ) e 2⇡ O em Magnetic Electric dipole moments
• Let’s remind ourselves about electric dipole moments • A particle with spin (i.e. neutron) in an electric field is described by ω ! ! ! ! H = −d (S ⋅ E) S = σ / 2 ! E! B ! Hamiltonian Spin Electric Field σ
Magnetic Electric dipole moment
• The E-field puts a torque on the system à spin precession
ω = 2µB sinθ ω = 2dE sinθ
• How large is the electric dipole moment ? Electric dipole moments
• We already exhausted the Dirac equation… No EDM there ? • Can we understand this ? ! ! ! ! H = −µ (S ⋅ B) − d (S ⋅ E)
• Perform a Time-reversal (T) transformation ! ! ! ! ! S → −S Spin like angular momentum ~ L ~ r × p ! ! ! ijk B → −B B ∝ε Fjk ~ ∂ j Ak → (+∂ j )(−Ak ) ! ! ! E → E E ∝ F0i ~ ∂0 Ai → (−∂0 )(−Ai ) ! ! ! ! H = −µ (S ⋅ B) −+ d (S ⋅ E) CP violation in the Standard Model • We can try to calculate EDMs from SM CKM phase
1 L = − Ψσ µν (µ +iγ 5d)ΨF dip 2 µν
e d e u,c,t γ γ γ W+- e u,c,t e d
e md αweak * αem µ ∝ (V V ) µ = d = 0 2 qd qd 2m e 2π mW 2π ∗ � ~ �� � � = 0 SM CKM EDMs (too many acronyms!)
• At two loops: individual diagrams contribute but sum vanishes
• dq (2 loops) = 0, somewhat unexpected !
2 2 mc ↵sGF 21 • At three loops: d m 10 e fm d ' d 108⇡5 JCP ' 2 5 = c c c s s s sin 3 10 JCP 12 23 13 12 23 13 ' · • Electron EDM even at 4 loops !! � ≅ 10 � �� • Compare with magnetic moment: µ 100 e fm e ' • CKM EDMs are really very very small • Nucleon EDMs more complicated but also small Note: actual size of SM SM size of actual Note: 5 6 to orders Upperbound nEDM 10^ [e cm] With linear extrapolation: CKM neutron EDM in 2075…. EDM in CKM neutron extrapolation: linear With Standard Model suppression below nEDM upper bound bound upper has large uncertainty large has u freach! Out of “Here be dragons” “Here Baker et al ’ 06 ‘15 Strong CP violation ‘t Hooft ’76, ‘78
• Second source: QCD theta-term. (Later more detail). • Due to complicated vacuum structure of QCD
• Causes a ‘new’ CP-violating interaction with coupling constant θ
µnab ! ! q e GµnGab (in QED ~ E ⋅ B )
• Size of θ is unknown, one of the SM parameters
€ The strong CP problem If θ ~ 1
More details on calculation later Upperbound Upperbound nEDM 10^ [e cm]
Sets θ upper bound: θ < 10-10 Is there a reason for this suppression? Axions? Is θ=0 exact, or merely very small? Measurement of a nonzero EDM
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BSM sources of Standard Model: CP-violation θ-term SUSY, Left-Right, 2HDM,…
For the forseeable future: EDMs are ‘background-free’ searches for new physics Measurement of a nonzero EDM
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BSM sources of Standard Model: CP-violation θ-term SUSY, Left-Right, 2HDM,…
Collider/flavor input Matter/Antimatter asymmetry (electroweak baryogenesis) Very active experimental field
System Group Limit C.L. Value Year 205Tl Berkeley 1.6 × 10−27 90% 6.9(7.4) × 10−28 2002 e YbF Imperial 10.5 × 10−28 90 −2.4(5.7)(1.5) × 10−28 2011 ThO ACME 1.1 × 10−29 90 4.3(3.1)(2.6) × 10−30 2018 HfF+ Boulder 1.3 × 10−28 90 0.9(7.7)(1.7) × 10−29 2017 n Sussex-RAL-ILL 3.0 × 10−26 90 0.2(1.5)(0.7) × 10−26 2006 129Xe UMich 4.8 × 10−27 95 0.26(2.3)(0.7) × 10−27 2019 199Hg UWash 7.4 × 10−30 95 -2.2(2.8)(1.5) × 10−30 2016 225Ra Argonne 1.4 × 10−23 95 4(6.0)(0.2) × 10−24 2016
muon E821 BNL g−2 1.8 × 10−19 95 0.0(0.2)(0.9) × 10−19 2009
+ new electron, muon, neutron, proton, Xe, Ra, Rn ….. experiments
• Why do experiments on so many different systems? • How do the different limits compare? • How to interpret the limits or a future signal? Measuring EDMs • General idea now. Later more.
σ B E B E σ
T/CP
= + d ~ E d ~ B Hd e · m ·
−28 • Note d =10 e cm E =100 kV / cm δω ~ 10−7 rad / s ~ 1 rad / year CP violation beyond the SM
• We saw that CKM EDMs are too small to be measured • We have the theta term, but that seems small for some reason… • Why bother with measuring further ?
• EDMs can be much larger in models of new physics, even at high scales • CKM EDMs are small because of the peculiar SM flavor structure • Need at least 3 loops to get an EDM (big suppression)
• NOT GENERAL at all. In many BSM models, EDMs at tree- or one- loop level. Much larger EDMs ! Example: the MSSM
Slide from Altmannshofer, 2014 The SUSY/LR CP problem
• CPV phase already at one-loop ! • Typical size of EDM
↵ n m d em e sin e ⇠ ⇡ ⇤2 ⇣ ⌘ If phase = O(1): Λ > 30 TeV (n=1) There are clever ways to avoid this !
uL d + L • In left-right symmetric models WL
+ L = i⌅(¯uR µdR)(¯uL µdL)+h.c. W d R u R R Ξ~ sin � /Λ € € € • Tree-level CP violation, EDMs probe ~50 TeV scale € € € The EDM metromap Outline
§ Part I: What are EDMs and why do (should) we care ?
§ Part II: Sources of CP violation: an EFT approach §
§ Part III: Classes of EDM searches + theoretical interpretation Heavy BSM physics and the SM EFT
• Assume BSM fields exists but are heavy à Integrate them out
Fermi’s theory:
• We don’t need ‘high-energy details’, the W boson, at low energies ! Energy SM fields Λ BSM fields
Effective operators E << Λ 1 exp ~ Λn Buchmuller & Wyler ‘86 Standard Model EFT Gradzkowski et al ’10 Many others • To stay model independent: add all EFT operators (infinite…)
1) Degrees of freedom: Full SM field content 2) Symmetries: Lorentz, SU(3)xSU(2)xU(1) 1 1 L = L + L + L +! new SM Λ 5 Λ2 6 • Low-energy effects suppressed by (E/Λ)^n
Advantages: General framework, no need to specify a BSM model Keep constraints from gauge invariance and EWSB Great tool to analyze experiments at different scales
Disadvantages: Many operators at relevant order Might not be valid for LHC physics if scale too low Not applicable for light BSM physics Typical Energy Scale Beyond-the-SM ? Λ physics ? TeV EFT operators
LEFF RG flow
M ~ v ~ M EW Z,W,H,t Integrate out heavy SM fields 100 GeV L' EFF RG flow
~ 2 F ~ M Λ χ π π N Nonperturbative QCD regimes 1 GeV
L'''EFF Lattice QCD + chiral effective field theory
100 MeV - eV EDMs Typical Energy Scale Beyond-the-SM ? Λ physics ? TeV EFT operators
LHC physics LEFF RG flow
M ~ v ~ M EW Z,W,H,t Integrate out heavy SM fields 100 GeV L' EFF RG flow B + D flavor physics
~ 2 F ~ M Λ χ π π N Nonperturbative QCD regimes 1 GeV
L'''EFF Lattice QCD + chiral effective field theory
100 MeV - eV EDMs + Kaons + beta + …. Examples of EFT operators: dipoles
EDMs and MDMs appear in the SMEFT Lagrangian at dimension-six
MCP � � � � � + ℎ. �. → � � � � +ℎ. �. ? TeV
€ B, W One-loop QCD mixing q, l q’, l’ H H
Electron (muon, tau) Quark chromo-EDM Quark EDM EDM
1 GeV e e Weinberg PRL ’89 Gluon chromo-EDM Braaten et al PRL ’90
d f abcε µναβ Ga Gb Gc λ w αβ µλ ν Weinberg operator
MCP ? TeV
€ QCD RGE mixing
1 GeV Weinberg PRL ’89 Gluon chromo-EDM Braaten et al PRL ’90
d f abcε µναβ Ga Gb Gc λ w αβ µλ ν Weinberg operator
µν MCP CG tLσ tR Gµνϕ + h. c. ? TeV Threshold contributions from heavy CEDMs
€ mQ Q QCD RGE mixing
1 GeV Modified Yukawa couplings
† C y t t ! ( ) h.c. L = C m t t (vh + h2 + )+ h.c. Λ Y t L Rϕ ϕ ϕ + Y t L R !
g, γ g t Barr, Zee ’90 t Barr-Zee diagrams g, γ g mt g QCD RGE mixing
γ γ 1 GeV e e Many more… But when the dust settles….. γ
Few GeV QCD + + + + (θ-term) Four-quark Quark EDM Quark C-EDM Gluon C-EDM operators (semi-)leptonic interactions JdV et al ‘12 ‘13 Ramsey-Musolf/Chupp ‘13 γ e e
` e e Electron EDM q q
• Any BSM model at high scales with CP-violation can be described at low energies by O(10) CPV operators (integrated out high-energy details !) • Different BSM model, different relevant operators Intermediate summary • Parametrized BSM CP violation in terms of dim6 operators • Evolved them to lower energies to ~ 1 GeV • O(10) operators left: theta, (C)EDMs, Weinberg, Four-fermion • Important: different BSM models à different EFT operators
1. Standard Model: only theta has a chance to be measured 2. 2-Higgs doublet model: quark+electron EDM, CEDMs, Weinberg (exact hierarchy depends on detail of models) 3. Split SUSY: only electron + quark EDMs (ratio fixed) 4. Left-right symmetric models: FQ operators, way smaller (C)EDMs 5. Leptoquark: FQ + semi-leptonic operators
• Now we must calculate EDMs. Not easy, since EDMs involve horrible objects (for a particle physicist) such as nucleons, atoms, and molecules Outline
§ Part I: What are EDMs and why do (should) we care ?
§ Part II: Sources of CP violation: an EFT approach §
§ Part III: Classes of EDM searches + theory interpretation The ‘easy case’: (semi-)leptonic CP violation
(semi-)leptonic interactions Few GeV γ e e
` e e Electron EDM q q
Hadronization (known matrix elements
e e N = nucleon ` < GeV e e (neutron, proton) Electron EDM N N Probing semi-leptonic operators System Group Limit C.L. Value Year 205Tl Berkeley 1.6 × 10−27 90% 6.9(7.4) × 10−28 2002 e YbF Imperial 10.5 × 10−28 90 −2.4(5.7)(1.5) × 10−28 2011 ThO ACME 1.1 × 10−29 90 4.3(3.1)(2.6) × 10−30 2018 HfF+ Boulder 1.3 × 10−28 90 0.9(7.7)(1.7) × 10−29 2017
• Why these complicated systems ? Cannot use free electrons…. • Look at neutral systems with unpaired electron (paramagnetic) • Why not simply use Hydrogen ? Probing semi-leptonic operators System Group Limit C.L. Value Year 205Tl Berkeley 1.6 × 10−27 90% 6.9(7.4) × 10−28 2002 e YbF Imperial 10.5 × 10−28 90 −2.4(5.7)(1.5) × 10−28 2011 ThO ACME 1.1 × 10−29 90 4.3(3.1)(2.6) × 10−30 2018 HfF+ Boulder 1.3 × 10−28 90 0.9(7.7)(1.7) × 10−29 2017
Schiffs theorem: the electron cloud will rearrange so that the nucleus does not ‘feel’ an external E-field. The EDMs of the nucleus and electron are screened (clasical argument but works in QM as well)! E Probing the electron EDM
System Group Limit C.L. Value Year 205Tl Berkeley 1.6 × 10−27 90% 6.9(7.4) × 10−28 2002 e YbF Imperial 10.5 × 10−28 90 −2.4(5.7)(1.5) × 10−28 2011 ThO ACME 1.1 × 10−29 90 4.3(3.1)(2.6) × 10−30 2018 HfF+ Boulder 1.3 × 10−28 90 0.9(7.7)(1.7) × 10−29 2017
Schiff Theorem: EDMs of charged constituents are screened in a neutral atom Schiff, ‘63 • Assumption : non-relativistic constituents • Invalid in heavy atoms/molecules 3 2 dA (de ) = KAde KA∝ Z αem Sandars ’65
−25 Bound on atomic Tl EDM : d 205Tl < 9 ⋅10 e cm Regan et al ’02 Strong enhancement! dA (de ) = KAde KTl= −(570±20) −27 de <1.6 ⋅10 e cm State-of-the-art: polar molecules Liu,Kelly ‘92, Dzuba, ‘09, Porsev et al ’12, Mayer ’09 Polar molecules: Convert small external to huge internal field
# & de ΔEYbF = (15± 2)⋅GeV % (+O(CS ) $ e cm ' Ε eff # & Εext de ΔEThO = (80 ±10)⋅GeV % (+O(CS ) $ e cm '