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On the role of leptonic CPV phases in cLFV observables

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On the role of leptonic CPV phases in cLFV observables

Jonathan Kriewald

Laboratoire de Physique de Clermont-Ferrand

TAUP 2021TAUP 2021TAUP 2021

Based on: arXiv:2107.06313with A. Abada and A. M. Teixeira 26.8. - 3.9. 2021

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Motivation

Neutrino oscillations first laboratory evidence fornew physics

⇒⇒(Neutral) lepton flavour isviolated, neutrinos aremassive

⇒⇒⇒Massive neutrinos open the door tocLFVand new sources ofCP violation

MinimalSMSMSMmmmννν: massiveDirac neutrinos via Higgs mechanism

accommodateoscillation data;cLFV unobservable, naturalness problem

(Low-scale)seesaw mechanism: heavy neutral leptons (HNL)

HNL: e.g. massiveMajorananeutrinos

LNVandcLFV

LNVobservables crucially depend on CPV phases

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Motivation

Neutrino oscillations first laboratory evidence fornew physics

⇒⇒(Neutral) lepton flavour isviolated, neutrinos aremassive

⇒⇒⇒Massive neutrinos open the door tocLFVand new sources ofCP violation

MinimalSMSMSMmmmννν: massiveDirac neutrinos via Higgs mechanism

accommodateoscillation data;cLFV unobservable, naturalness problem

(Low-scale)seesaw mechanism: heavy neutral leptons (HNL)

HNL: e.g. massiveMajorananeutrinos

LNVandcLFV

LNVobservables crucially depend on CPV phases

10−5 10−4 10−3 10−2 10−1 100

m0/eV 10−5

10−4 10−3 10−2 10−1 100

mee/eV

Excluded by 0νββ

ExcludedbyCosmology

NO IO

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Motivation

Neutrino oscillations first laboratory evidence fornew physics

⇒⇒⇒(Neutral) lepton flavour isviolated, neutrinos aremassive

⇒⇒⇒Massive neutrinos open the door tocLFVand new sources ofCP violation

MinimalSMSMSMmmmννν: massiveDirac neutrinos via Higgs mechanism

accommodateoscillation data;cLFV unobservable, naturalness problem

(Low-scale)seesaw mechanism: heavy neutral leptons (HNL)

HNL: e.g. massiveMajorananeutrinos

LNVandcLFV

LNVobservables crucially depend on CPV phases

10−5 10−4 10−3 10−2 10−1 100

m0/eV 10−5

10−4 10−3 10−2 10−1 100

mee/eV

Excluded by 0νββ

ExcludedbyCosmology

NO IO

Vast model landscape feat. at least 2HNL, at high and low scales

⇒⇒⇒TeVTeVTeV-scaleHNLoffer richcLFVphenomenology; potentially within collider reach

⇒⇒⇒take effective “3+2 model”; analyse effects ofCPV phasesoncLFV observables

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“3+2” toy model

Ignore precise origin ofmmmννν, assume 2 (heavy) Majorana neutrinosNNN4,54,54,5 present

⇒⇒⇒physical neutrino spectrum comprises 5 states (3 light,2 heavy)

Mixing parametrised via 10 mixing anglesθθθαjαjαj, 6 Diracδδδαjαjαj and 4 Majorana phasesϕϕϕjjj

⇒⇒⇒accommodate osc. data in (enlarged) PMNS mixing matrix

“Heavy-light” mixing given by (forcosθα4,5≈1):

U`N

sinθ14e−i(δ14−ϕ4) sinθ15e−i(δ15−ϕ5) sinθ24e−i(δ24−ϕ4) sinθ25e−i(δ25−ϕ5) sinθ34e−i(δ34−ϕ4) sinθ35e−i(δ35−ϕ5)

⇒⇒⇒SM-like (3×3)block no longer unitary, leptonicWWW andZZZ vertices modified Take sterile massesmmm4,54,54,5 atTeV-scale

⇒⇒⇒sizeablecLFVrates @ 1 loop-level, what is the effect ofCPV phases?

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Example: µ µ µ → → → eγ eγ eγ

cLFVprocess mediated byNNN4,54,54,5@ 1 loop-level

BRBR

BR(µ→eγ)∝ |GGGµeγµeγµeγ |2 cLFVform factor including mixing and loop function:

Gµeγ

Gµeγ

Gµeγ = X

i=4,5

Uei

Uei UeiUUUµiµiµi Gγ

m2NNNiii m2W

!

eee

γ γ γ Uµ4,5

Uµ4,5

Uµ4,5 Ue4,5 UUe4,5e4,5 µµµ

N4,5

NN4,54,5

W W

Assumemmm444≈mmm555 andsinθα4≈sinθα51:

|GGGµeγµeγµeγ |2≈4sss214214214sss224224224cos2

δδδ141414+δδδ252525−δδδ151515−δδδ242424

2

Gγ

m2NNNiii m2W

!

⇒⇒⇒Rate depends onDirac phases, fullcancellationforδδδ141414+δδδ252525−δδδ151515−δδδ242424=π Other form factors more complicated,ZZZ-penguin and boxes also depend onϕϕϕ4,54,54,5

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Effects of Dirac phases

Simplified approach onµµµ−−−eeeflavour violatingobservables µ→3e

µ→3e

µ→3eadditionally dependsZZZ-penguins and box-diagrams

Takesinθα4= sinθα5 andmmm444=mmm555= (1,5,10) TeV, onlyδδδ1414146= 0:

0 1 2 3 4 5 6

δ14 10−18

10−17 10−16 10−15 10−14 10−13 10−12

AKT 2107.06313

BR(µeγ) BR(µee+e) BR(Z→e±µ)

⇒⇒Strong cancellation forδδδ141414=πin all observables(similar results forδ24, δ15, δ25)

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Effects of Majorana phases

Simplified approach onµµµ−−−eeeflavour violatingobservables

Takesinθα4= sinθα5 andmmm444=mmm555= (1,5,10) TeV, onlyϕϕϕ4446= 0:

0 1 2 3 4 5 6

ϕ4 10−14

10−13

AKT 2107.06313

BR(µeγ) BR(µee+e) BR(Z→e±µ)

⇒⇒Variational behaviour amplified with increasingmmm4,54,54,5

⇒⇒Photon penguin independent ofϕϕϕ444 (analytically expected)

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Joint behaviour of Dirac and Majorana CPV phases

Simplified approach onµµµ−−−eeeflavour violatingobservables

Takesinθα4= sinθα5 andmmm444=mmm555= (1,5,10) TeV, varyϕϕϕ444, fixδδδ141414=π:

0 1 2 3 4 5 6

ϕ4 10−22

10−20 10−18 10−16 10−14

AKT 2107.06313

BR(µeγ) BR(µ→ee+e) BR(Ze±µ)

⇒⇒⇒Cancel dipole contributions, presence ofϕϕϕ4446= 0enhancesZZZ-penguin and boxes

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Joint behaviour of Dirac and Majorana CPV phases (continued)

Neutrinolessµµµ−−−eeeconversion in nuclei, process depends on all topologies and phases Takesinθα4= sinθα5 andmmm444=mmm555= 1 TeV, vary 2 phases at a time:

0 1 2 3 4 5 6

δ14 0

1 2 3 4 5 6

ϕ4

10−19 10−18 10−17 10−16 10−15 10−14 10−13

CR(µe,Al)

⇒Varying onlyϕϕϕ444 can lead to strong cancellations as well, interference of contributions

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Joint behaviour of Dirac and Majorana CPV phases (continued)

Neutrinolessµµµ−−−eeeconversion in nuclei, process depends on all topologies and phases Takesinθα4= sinθα5 andmmm444=mmm555= 1 TeV, vary 2 phases at a time:

0 1 2 3 4 5 6

δ34 0

1 2 3 4 5 6

ϕ4

10−19 10−18 10−17 10−16 10−15 10−14 10−13

CR(µe,Al)

⇒⇒⇒Sum over allflavoursinZZZ-vertex⇒⇒⇒dependence onδδδ343434

⇒⇒Interference of contributions can be constructive, leading toenhancements!

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Towards realistic scenarios

ForTeVTeVTeV-scaleHNLseveral indirect constraints apply (besidescLFV):

◦ Lepton Universality:WWW→`ν,ZZZ→`+`,ratiosof leptonic Meson decays, ratios of (semi-leptonic)τττ-lepton decays,CKMunitarity ...

◦ LNV: neutrinoless double beta decay

◦ Perturbative Unitarity: ΓNNN4,54,54,5/mNNN4,54,54,5≤1/2

◦ Electroweak Precision: mWWW,GF,Γ(ZZZ →invisibles)

Constraintsindependent ofCPV phases

⇒Randomly scanconstrainedparameter space withθθθα4α4α4≈ ±θθθα5α5α5 andmmm444=mmm555= 1TeVTeVTeV

⇒⇒

⇒For each point vary phasesδδδα4α4α4andϕϕϕ444 randomly and on a grid

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Breaking correlations

Effective couplingGGGM MM MM M ofMuMuMu−−−MuMuMuoscillation (µµµ+++eee→→→µµµeee+++) only depends on boxes Bothµµµ→→→eγeγeγandGGGM MM MM M only depend onθθθ14,514,514,5 andθθθ24,524,524,5⇒⇒⇒expect strong correlation

10−25 10−23 10−21 10−19 10−17 10−15 10−13 10−11

BR(µeγ)

10−25 10−23 10−21 10−19 10−17 10−15

|GMM|

MEG II MEG AKT 2107.06313

blue: all phases vanishing;

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Breaking correlations

Effective couplingGGGM MM MM M ofMuMuMu−−−MuMuMuoscillation (µµµ+++eee→→→µµµeee+++) only depends on boxes Bothµµµ→→→eγeγeγandGGGM MM MM M only depend onθθθ14,514,514,5 andθθθ24,524,524,5⇒⇒⇒expect strong correlation

10−25 10−23 10−21 10−19 10−17 10−15 10−13 10−11

BR(µeγ)

10−25 10−23 10−21 10−19 10−17 10−15

|GMM|

MEG II MEG AKT 2107.06313

blue: all phases vanishing;orange: random phases;

⇒⇒⇒Presence of phasesbreaks correlation!

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Breaking correlations

Effective couplingGGGM MM MM M ofMuMuMu−−−MuMuMuoscillation (µµµ+++eee→→→µµµeee+++) only depends on boxes Bothµµµ→→→eγeγeγandGGGM MM MM M only depend onθθθ14,514,514,5 andθθθ24,524,524,5⇒⇒⇒expect strong correlation

10−25 10−23 10−21 10−19 10−17 10−15 10−13 10−11

BR(µeγ)

10−25 10−23 10−21 10−19 10−17 10−15

|GMM|

MEG II MEG AKT 2107.06313

blue: all phases vanishing;orange: random phases;green: phases grid scan

⇒⇒⇒Presence of phasesbreaks correlation!

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Breaking correlations (continued)

Bothµµµ−−−eeeconversion andµµµ→→→3e3e3edominated byZZZ-penguins, expect strong correlation

10−27 10−25 10−23 10−21 10−19 10−17 10−15 10−13

BR(µee+e)

10−26 10−24 10−22 10−20 10−18 10−16 10−14 10−12

CR(µe,Al)

COMET, Mu2e SINDRUM II (Au)

Mu3e

SINDRUM AKT 2107.06313

blue: all phases vanishing;orange: random phases;green: phases grid scan

⇒⇒⇒Hypothetical signal e.g. only inµµµ→→→3e3e3edoes not disfavourHNL models!

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General view on parameter space

Scanθθθα4α4α4 andθθθα5α5α5 independently, randomly varyall phases,(apply all constraints) Mass splitting varied within inΓΓΓNNN4,54,54,5,m4= 1 TeV,m5−m4∈(40 MeV,210 GeV)

10−23 10−21 10−19 10−17 10−15 10−13 10−11

BR(µeγ)

10−22 10−20 10−18 10−16 10−14 10−12

CR(µe,Al)

AKT 2107.06313

COMET, Mu2e SINDRUM II (Au)

MEG II MEG

⇒⇒⇒Sizeableµµµ→→→eγeγeγrate possible withoutµµµ−−−eeeconversion and vice versa!

⇒⇒⇒Effects ofCPV phasessignificant!

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Summary & Conclusion

Presence ofCPVMajorana and Dirac phases can suppress and enhance the rate of cLFVobservables with significant impact on the interpretation of future data:

PP(1(0) 0)

P1(10):Enhancingrates to future sensitivities inµτµτµτ-sector

PPP(2(2(00)) 0)

2 :Enhancingrates inµeµeµe-sector

PP(3(0) 0)

P3(30):Suppressingrates inµeµeµe-sector

⇒⇒⇒PresenceCPV phases: data needs to be interpreted carefully

◦◦◦Non-observation of a certain observable does not (necessarily) disfavourHNLmodels

◦◦◦Sizeable mixing angles possible, if phases lead to suppression ofcLFV

◦◦◦CPV phasesneed to be consistently included in phenomenological analyses ofHNL

You cannot spell flavour without

CP Violation!

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Summary & Conclusion

Presence ofCPVMajorana and Dirac phases can suppress and enhance the rate of cLFVobservables with significant impact on the interpretation of future data:

PP(1(0) 0)

P1(10):Enhancingrates to future sensitivities inµτµτµτ-sector

PPP(2(2(00)) 0)

2 :Enhancingrates inµeµeµe-sector

PP(3(0) 0)

P3(30):Suppressingrates inµeµeµe-sector

⇒⇒⇒PresenceCPV phases: data needs to be interpreted carefully

◦◦◦Non-observation of a certain observable does not (necessarily) disfavourHNLmodels

◦◦◦Sizeable mixing angles possible, if phases lead to suppression ofcLFV

◦◦◦CPV phasesneed to be consistently included in phenomenological analyses ofHNL

You cannot spell flavour without

CP Violation!

(20)

Summary & Conclusion

Presence ofCPVMajorana and Dirac phases can suppress and enhance the rate of cLFVobservables with significant impact on the interpretation of future data:

PP(1(0) 0)

P1(10):Enhancingrates to future sensitivities inµτµτµτ-sector

PPP(2(2(00)) 0)

2 :Enhancingrates inµeµeµe-sector

PP(3(0) 0)

P3(30):Suppressingrates inµeµeµe-sector

⇒⇒⇒PresenceCPV phases: data needs to be interpreted carefully

◦◦◦Non-observation of a certain observable does not (necessarily) disfavourHNLmodels

◦◦◦Sizeable mixing angles possible, if phases lead to suppression ofcLFV

◦◦◦CPV phasesneed to be consistently included in phenomenological analyses ofHNL

You cannot spell flavour without

CP Violation!

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Thank you!!!

µ

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