bsm and beta decay
play

BSM and beta decay Vincenzo Cirigliano Los Alamos National - PowerPoint PPT Presentation

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

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend