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ACFI Workshop on Beta decays as a probe of new physics Amherst, Nov 1-3 2018 BSM and beta decay Vincenzo Cirigliano Los Alamos National Laboratory Outline New physics in beta decays: generalities and EFT framework Constraints on


  1. ACFI Workshop on “Beta decays as a probe of new physics” Amherst, Nov 1-3 2018 BSM and beta decay Vincenzo Cirigliano Los Alamos National Laboratory

  2. Outline • New physics in beta decays: generalities and EFT framework • Constraints on non-standard charged current interactions • global analysis of beta decays • collider input: LEP , LHC • comparison of sensitivities • Summary and outlook Special thanks to Martin Gonzalez-Alonso for sharing his slides from the WE-Heraeus-Seminar on “Particle Physics with Cold and UltraCold Neutrons” October 24-26, 2018, Bad Honnef

  3. Semileptonic processes: SM and beyond • In the SM, W exchange ⇒ V-A currents, universality , τ W R , H + , leptoquarks, Z’, SUSY,… G F ~ g 2 V ij /M w2 ~1/v 2 1/ Λ 2

  4. Semileptonic processes: SM and beyond • In the SM, W exchange ⇒ V-A currents, universality SUSY analyses: Bauman, Erler, Ramsey-Musolf, arXiv:1204.0035, , τ … W R , H + , Kurylov & Ramsey-Musolf leptoquarks, hep-ph/0109222. Z’, SUSY,… … Hagiwara et al1995 G F ~ g 2 V ij /M w2 ~1/v 2 1/ Λ 2 … Barbieri et al 1985 … • Broad sensitivity to BSM scenarios • Experimental and theoretical precision at or approaching 0.1% level Probe effective scale Λ in the 5-10 TeV range

  5. Connecting scales — EFT To connect UV physics to neutron and nuclear beta decays, use EFT Matching to BSM scenarios Perturbative matching within SM

  6. Connecting scales — EFT To connect UV physics to neutron and nuclear beta decays, use EFT Matching to BSM scenarios Perturbative matching within SM Hadronic matrix Non-perturbative strong interactions elements Nuclear matrix elements

  7. Effective Lagrangian at E~GeV • New physics effects are encoded in ten quark-level couplings • Quark-level version of Lee-Yang effective Lagrangian, allows us to connect nuclear & high energy probes

  8. Effective Lagrangian at E~GeV Bhattacharya et al., 1110.6448 VC, Graesser, Gonzalez-Alonso 1210.4553 • New physics effects are encoded in ten quark-level couplings Can interfere with SM: linear sensitivity to ε i

  9. Effective Lagrangian at E~GeV Bhattacharya et al., 1110.6448 VC, Graesser, Gonzalez-Alonso 1210.4553 • New physics effects are encoded in ten quark-level couplings Can interfere with SM: linear sensitivity to ε i Interference with SM suppressed by m ν /E: quadratic ~ sensitivity to ε i

  10. Effective Lagrangian at E~GeV Bhattacharya et al., 1110.6448 VC, Graesser, Gonzalez-Alonso 1210.4553 • Work to first order in rad. corr. and new physics Fermi constant extracted fro muon lifetime, possibly “contaminated” by new physics SM rad. corr. ⊃ “large log” ( α / π ) × Log(M Z / μ ) Note: besides the pre-factor, ϵ R appears in nuclear _ Marciano-Sirlin 1981 decays in the combination g A ≡ g A × (1- 2 ϵ R ) Sirlin 1982

  11. How do we probe the ε α ? (1) 1. Differential decay distribution Lee-Yang, 1956 Jackson-Treiman-Wyld 1957 a(g A ), A(g A ) , B(g A , g α ε α ), … isolated via suitable experimental asymmetries Theory input: g V,A,S,T (from lattice QCD) + rad. corr.

  12. Nucleon charges from lattice QCD With estimates of all systematic errors (m q , a, V, excited states) Chang et al. (CalLat) 1805.12030 1% g A g T g S ~5% ~10% Bhattacharya et al. 1806.09006

  13. How do we probe the ε α ? (2) 2. Total decay rates

  14. How do we probe the ε α ? (2) 2. Total decay rates Q-values → Lifetimes, phase space BRs Experimental input

  15. How do we probe the ε α ? (2) 2. Total decay rates Theory input Hadronic / nuclear Lattice QCD, chiral EFT, matrix elements dispersion relations, … and radiative corrections

  16. How do we probe the ε α ? (2) 2. Total decay rates Channel-dependent effective CKM element ~

  17. How do we probe the ε α ? (2) 2. Total decay rates For nuclei, rate traditionally written in terms of “corrected FT values” Nucleus-dependent radiative & “Inner” radiative correction Isospin Breaking correction Δ R V = (2.36 ± 0.04)% [Marciano-Sirlin 2006]

  18. How do we probe the ε α ? (2) 2. Total decay rates For nuclei, rate traditionally written in terms of “corrected FT values” Nucleus-dependent radiative & “Inner” radiative correction Isospin Breaking correction Δ R V = (2.467 ± 0.022)% [Seng et al. 1807.10197]

  19. Snapshot of the field • Experimental precision between ~0.01% and few % Nuclei Gonzalez-Alonso, Naviliat-Cuncic, Severijns, 1803.08732 & M. Gonzalez-Alonso slides

  20. Snapshot of the field • Experimental precision between ~0.01% and few % FT values before including nucleus-dependent radiative “Corrected” FT values correction Hardy-Towner 1411.5987 Gonzalez-Alonso, Naviliat-Cuncic, Severijns, 1803.08732 & M. Gonzalez-Alonso slides

  21. Snapshot of the field • Experimental precision between ~0.01% and few % Gonzalez-Alonso, Naviliat-Cuncic, Severijns, 1803.08732 & M. Gonzalez-Alonso slides

  22. Results of global fit to low-E data Gonzalez-Alonso, Naviliat-Cuncic, Severijns, 1803.08732 • Standard Model fit ( λ = g A /g V ) Radiative corrections ( Δ R ) Experimental • Fit driven by F t’s (0 + → 0 + ) λ and τ n (not A n ) V ud (1+ Δ R ) 1/2

  23. Results of global fit to low-E data Gonzalez-Alonso, Naviliat-Cuncic, Severijns, 1803.08732 • Standard Model fit ( λ = g A /g V ) New Radiative corrections ( Δ R ) Experimental [Seng et al. 1807.10197] • Fit driven by F t’s (0 + → 0 + ) λ and τ n (not A n ) V ud (1+ Δ R ) 1/2

  24. Results of global fit to low-E data Gonzalez-Alonso, Naviliat-Cuncic, Severijns, 1803.08732 • Fit including BSM couplings (driven by F t’s (0 + → 0 + ) , τ n , and A n ) 2nd error: Δ R , g A , g S , and g T 1st error: experimental ~2 % → ~ 0.5% ** ~0.2 % ~0.1 % ** CalLat 1805.12030

  25. Cabibbo universality test Extraction dominated by K decays: Extraction dominated by 0 + → 0 + nuclear transitions K →π e ν & K →μν vs π→μν (V us /V ud ) FLAVIANET report 1005.2323 and refs therein Hardy-Towner 1411.5987 CKM 2016 Lattice QCD input from FLAG 1607.00299 and refs therein + MILC 2018 1809.02827

  26. Cabibbo universality test _ V us from K → μν V us 0.02% Δ CKM = - (4 ± 5) ∗ 10 -4 ~ 1 σ K → μν Δ CKM = - (12 ± 6) ∗ 10 -4 ~ 2 σ V us from K → π l ν K → π l ν unitarity 0 + → 0 + 0.4% _ V ud

  27. Cabibbo universality test _ V us from K → μν V us 0.02% Δ CKM = - (4 ± 5) ∗ 10 -4 ~ 1 σ K → μν Δ CKM = - (12 ± 6) ∗ 10 -4 ~ 2 σ V us from K → π l ν Hint of something [ ε ’s ≠ 0] or SM theory input? K → π l ν unitarity 0 + → 0 + 0.4% Worth a closer look: at the level of the best LEP EW _ precision tests, V ud probing scale Λ ~10 TeV

  28. Cabibbo universality test _ V us from K → μν V us 0.02% Δ CKM = - (14 ± 4) ∗ 10 -4 ~3.5 σ K → μν Δ CKM = - (22 ± 5) ∗ 10 -4 ~4.5 σ V us from K → π l ν With new radiative corrections K → π l ν [Seng et al. 1807.10197] unitarity 0 + → 0 + 0.4% _ V ud

  29. Impact of neutrons • Independent extraction of V ud @ 0.02% requires: Czarnecki, Marciano, Sirlin 1802.01804 δ g A /g A ~0.15% → 0.03% δτ n ~ 0.35 s ( δ a/a , δ A/A ~ 0.14%) δτ n / τ n ~ 0.04 % δ A/A < 0.2% can be reached UCN τ @ LANL [ τ n ~ 877.7(7)(3)s] by PERC, UCNA+ is almost there, will reach δτ n ~ 0.2 s δ a/a ~ 0.1% at Nab 1707.01817

  30. Interplay with High Energy physics • Need to know high-scale origin of the various ε α Match SM-EFT and SM-EFT’ • Model-independent statements possible in “heavy BSM” scenarios: M BSM > TeV → new physics looks point-like at collider VC, Gonzalez-Alonso, Jenkins 0908.1754

  31. Interplay with High Energy physics • Need to know high-scale origin of the various ε α ε L,R originate from SU(2)xU(1) invariant vertex corrections Gauge invariance u i d j E.g. from W L -W R mixing in Left-Right symmetric models VC, Gonzalez-Alonso, Jenkins 0908.1754

  32. Interplay with High Energy physics • Need to know high-scale origin of the various ε α ε S,P ,T and one contribution to ε L,R originate from SU(2)xU(1) ε L arise from SU(2)xU(1) invariant invariant vertex corrections 4-fermion operators u i u i d j d j … VC, Gonzalez-Alonso, Jenkins 0908.1754

  33. Interplay with High Energy physics • Need to know high-scale origin of the various ε α ε S,P ,T and one contribution to ε L,R originate from SU(2)xU(1) ε L arise from SU(2)xU(1) invariant invariant vertex corrections 4-fermion operators u i u i d j d j • LEP: • Strong constraints (<0.1%) on L-handed vertex corrections (Z-pole) • Weaker constraints on 4-fermion interactions ( σ had ) • What about LHC?

  34. LHC sensitivity: 4-fermions Bhattacharya et al., 1110.6448, VC, Graesser, Gonzalez-Alonso 1210.4553 • The effective couplings ε α contribute to the process pp → e ν + X • No excess events in transverse mass distribution: bounds on ε α m T (GeV) m T (GeV)

  35. LHC sensitivity: vertex corrections S. Alioli, VC, W. Dekens, J. de Vries, E. Mereghetti 1703.04751 • Vertex corrections inducing ε L,R in the SM- EFT involve the Higgs field (due to SU(2) ε L gauge invariance) ε R • Can be probed at the LHC by associated Higgs + W production q H ε L,R W ε L,R q’ W

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