Effective Field Theory and EDMs

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ACFI EDM School November 2016 Effective Field Theory and EDMs Vincenzo Cirigliano Los Alamos National Laboratory 1

Lecture III outline EFT approach to physics beyond the Standard Model Standard Model EFT up to dimension 6: guided tour Simple examples of matching CP violating dimension-6 operators contributing to EDMs Classification Evolution from the BSM scale to hadronic scale 2

Effective theory for new physics (and EDMs) 3

EDMs and new physics EDMs are a powerful probe of high-scale new physics Quantitative connection of EDMs with high scale models requires Effective Field Theory tools M vew UV new physics: Supersymmetry, Extended Higgs sectors, Dark sectors: effects below current sensitivity ** LeDall-Pospelov-Ritz 1505.01865 1/Coupling 4

Connecting EDMs to UV new physics RG EVOLUTION (perturbative) MATRIX ELEMENTS (non-perturbative) Multi-scale problem: need RG evolution of effective couplings & hadronic / nuclear / molecular calculations of matrix elements 5

Connecting EDMs to UV new physics RG EVOLUTION (perturbative) MATRIX ELEMENTS (non-perturbative) In this lecture we will cover the EFT analysis connecting physics between the new physics scale Λ and the hadronic scale Λhad ~ 1 GeV 6

The low-energy footprints of LBSM At energy E exp << MBSM, new particles can be integrated out Generate new local operators with coefficients ~ g k /(MBSM) n vew Familiar example: g W g q 2 << MW 2 GF ~ g 2 /Mw 2 Effective Field Theory emerges as a natural framework to analyze low-e implications of classes of BSM scenarios and inform model building 7

Why use EFT for new physics General framework encompassing classes of models Efficient and rigorous tool to analyze experiments at different scales (from collider to table-top) The steps below UV matching apply to all models: can be done once and for all Very useful diagnosing tool in this pre-discovery phase :) Inform model building (success story is SM itself**) EFT and UV models approaches are not mutually exclusive 8

**EFT for β decays and the making of the Standard Model 9

EFT framework Assume mass gap MBSM > GF -1/2 ~ vew Degrees of freedom: SM fields (+ possibly νr) Symmetries: SM gauge group; no flavor, CP, B, L EFT expansion in E/M BSM, MW/MBSM [Oi (d) built out of SM fields] [ Λ MBSM ] 10

Guided tour of Leff Dim 5: only one operator Weinberg 1979 11

Guided tour of Leff Dim 5: only one operator Weinberg 1979 Violates total lepton number Generates Majorana mass for L-handed neutrinos (after EWSB) See-saw : 11

Guided tour of Leff Dim 6: many structures (59, not including flavor) No fermions Two fermions Four fermions 12

Guided tour of Leff Dim 6: affect many processes B violation Gauge and Higgs boson couplings Weinberg 1979 Wilczek-Zee1979 Buchmuller-Wyler 1986,... Grzadkowski-Iskrzynksi- Misiak-Rosiek (2010) EDMs, LFV, qfcnc,... g-2, Charged Currents, Neutral Currents,... EFT used beyond tree-level: one-loop anomalous dimensions known 13 Alonso, Jenkins, Manohar, Trott 2013

Examples of matching Explicit examples of matching from full model to EFT Dim 5: Heavy R-handed neutrino φ φ L λ ν T ν R M R -1 ν R λ ν L g g ~ λ ν T M R -1 λ ν 14

Examples of matching Explicit examples of matching from full model to EFT Dim 5: Triplet Higgs field φ µ T φ T g L i YT L j g ~ µ T M T -2 Y T 15

More on matching We just saw two simple examples of matching calculation in EFT: To a given order in E/MR,T, determine effective couplings (Wilson coefficients) from the matching condition Afull = AEFT with amplitudes involving light external states We did matching at tree-level, but strong and electroweak higher order corrections can be included Full theory Effective theory 16

More on matching We just saw two simple examples of matching calculation in EFT: In some cases Afull starts at loop level (highly relevant for EDMs) MSSM = C Function of SUSY coupling and masses 17

CP-violating operators contributing to EDMs: from BSM scale to hadronic scale 18

Dim-6 CPV operators When including flavor indices, at dimension=6 there are 2499 independent couplings of which 1149 CP-violating!! Alonso et al.2014 A large number of them contributes to EDMs Leading flavor-diagonal CP odd operators contributing to EDMs have been identified, neglecting 2nd and 3rd generation fermions** Dekens-DeVries 1303.3156 Engel, Ramsey-Musolf, Van Kolck 1303.2371 **Caveat: (i) strange quark can t really be ignored; (ii) new physics could couple predominantly to heavy quarks; (iii) flavor-changing operators can contribute to EDMs (multiple insertions) 19

High-scale effective Lagrangian CPV BSM dynamics dictated by: Here follow notation of: Engel, Ramsey-Musolf, Van Kolck 1303.2371 20

High-scale effective Lagrangian CPV BSM dynamics dictated by: Here follow notation of: Engel, Ramsey-Musolf, Van Kolck 1303.2371 non-relativistic limit Elementary fermion (chromo)-electric dipole 20

High-scale effective Lagrangian CPV BSM dynamics dictated by: Here follow notation of: Engel, Ramsey-Musolf, Van Kolck 1303.2371 21

High-scale effective Lagrangian CPV BSM dynamics dictated by: Here follow notation of: Engel, Ramsey-Musolf, Van Kolck 1303.2371 21

High-scale effective Lagrangian CPV BSM dynamics dictated by: Here follow notation of: Engel, Ramsey-Musolf, Van Kolck 1303.2371 21

High-scale effective Lagrangian CPV BSM dynamics dictated by: Here follow notation of: Engel, Ramsey-Musolf, Van Kolck 1303.2371 21

Evolution to low-e: generalities 1. Evolution of effective couplings with energy scale Operators in L eff depend on the energy scale μ at which they are renormalized (i.e. the UV divergences are removed) To avoid large logs, μ should be of the order of the energy probed Physical results should not depend on the arbitrary scale The couplings C i depend on μ in such a way to guarantee this! 22

Evolution to low-e: generalities 2. As one evolves the theory to low energy, need to remove ( integrate out ) heavy particles In our case, in the evolution of Leff we encounter the electroweak scale: remove top quark, Higgs, W, Z b and c quark thresholds 23

Dipole operators Λ g, B, W f = q, e CEDM renormalization vew g,γ CEDM mixing into EDM ΛHad f = q, e 24

Dipole operators Λ g, B, W f = q, e CEDM renormalization vew g,γ CEDM mixing into EDM ΛHad f = q, e 24

Three gauge bosons Λ g g g vew Weinberg mixing into CEDM g g ΛHad g g q q New structure at low-energy 25

Dipole and three-gluon mixing Rosetta stone Effect of mixing is important Dekens-DeVries 1303.3156 26

Four fermion operators (1) Λ vew Diagonal QCD evolution of scalar and tensor quark bilinears ΛHad mixes into lepton dipoles 27

Four fermion operators (2) Λ vew ΛHad 4-quark operators mix among themselves and into quark dipoles 28

Induced 4-quark operator Λ vew ΛHad 29

Induced 4-quark operator Λ vew ΛHad + color-mixed structure induced by QCD corrections 29

Gauge-Higgs operators Λ vew ΛHad g,γ f = q, e Mix into quark CEDM, quark EDM, electron EDM 30

and more Λ t B, W t For example: top quark electroweak dipoles induce at two loops electron and quark EDMs strongest constraints (by three orders of magnitude)! vew t γ ΛHad f = q, e VC, W. Dekens, J. de Vries, E. Mereghetti 1603.03049, 1605.04311 31

and more EDM physics reach vs flavor and collider probes C γ = c γ + i c~ γ Bound on top EDM improved by three orders of magnitude: dt < 5 10-20 e cm Dominated by eedm LHC sensitivity (pp jet t γ) and LHeC dt ~10-17 e cm [Fael-Gehrmann 13, Bouzas-Larios 13] VC, W. Dekens, J. de Vries, E. Mereghetti 1603.03049 32

Low-energy effective Lagrangian When the dust settles, at the hadronic scale we have: 33

Low-energy effective Lagrangian When the dust settles, at the hadronic scale we have: Electric and chromo-electric dipoles of fermions J E J Ec 33

Low-energy effective Lagrangian When the dust settles, at the hadronic scale we have: Electric and chromo-electric dipoles of fermions Gluon chromo-edm (Weinberg operator) J E J Ec 33

Low-energy effective Lagrangian When the dust settles, at the hadronic scale we have: Electric and chromo-electric dipoles of fermions Gluon chromo-edm (Weinberg operator) Semi-leptonic (3) and four-quark (2 SP + 2 LR ) J E J Ec Their form (and number) is strongly constrained by SU(2) gauge invariance Explicit form of operators given in previous slides 33

Low-energy effective Lagrangian When the dust settles, at the hadronic scale we have: Generated by a variety of BSM scenarios MSSM MSSM 2HDM Quark EDM and chromo-edm See Lecture IV for detailed discussion 34

Low-energy effective Lagrangian When the dust settles, at the hadronic scale we have: Generated by a variety of BSM scenarios MSSM 2HDM Weinberg operator See Lecture IV for detailed discussion 35

Low-energy effective Lagrangian When the dust settles, at the hadronic scale we have: Important points: Each BSM scenario generate its own pattern of operators (and hence of EDM signatures ) Within a model, relative importance of operators depends on various parameters (masses, etc) So, in a post-discovery scenario, a combination of EDMs will allow us to learn about underlying sources of CP violation 36

But we are not done yet RG EVOLUTION (perturbative) MATRIX ELEMENTS (non-perturbative) Multi-scale problem: need RG evolution of effective couplings & hadronic / nuclear / molecular calculations of matrix elements 37

But we are not done yet RG EVOLUTION (perturbative) MATRIX ELEMENTS (non-perturbative) Multi-scale problem: need RG evolution of effective couplings & hadronic / nuclear / molecular calculations of matrix elements 38

But we are not done yet RG EVOLUTION (perturbative) MATRIX ELEMENTS (non-perturbative) Multi-scale problem: need RG evolution of effective couplings & hadronic / nuclear / molecular calculations of matrix elements 39

Next step: from quarks and gluons to hadrons Leading pion-nucleon CPV interactions characterized by few LECs Electron and Nucleon EDMs γ T-odd P-odd pionnucleon couplings π Short-range 4N and 2N2e coupling e e N N N N N N To be discussed in Lectures VI, VII, VIII 40

Backup slides 41

Standard Model building blocks 42

Standard Model Lagrangian EWSB 43

Counting operators at low scale Engel, Ramsey-Musolf, Van Kolck 1303.2371 44

Renormalization group Large logs (from widely separated scales) spoil validity of perturbation theory NLO N 2 LO N 3 LO Ordinary pert. theory proceeds by rows : NLO, N 2 LO,... RGE re-organize the expansion by columns : LL, NLL,... 45

RGEs: exploit the fact that physics does not depend on the renormalization scale - Bare operators do not depend on μ (subtraction scale) - Physical amplitudes do not depend on μ 46

In general, need to solve: 47

In general, need to solve: One-loop beta functions: Needed input: γi (0) anomalous dimensions for relevant operators 48