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Neutron Decay Electroweak Radiative Corrections Preliminary Update. ( Implications for the neutron lifetime puzzle) Czarnecki , WJM & A. Sirlin Response to Dispersion Relations Results Seng , Gorchtein , Patel & Ramsey- Musolf PRL Hardy Fest 2019 William J. Marciano
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Neutron Decay Electroweak Radiative Corrections Preliminary Update (Implications for the neutron lifetime puzzle) • Czarnecki, WJM & A. Sirlin Response to Dispersion Relations Results Seng, Gorchtein, Patel & Ramsey-Musolf PRL Hardy Fest 2019 William J. Marciano January 7, 2019
John Hardy Celebration More than 50 years of Research and Leadership Distinguished Professor Famous Collaboration with Ian Towner Experimentalist + Theorist Combo Champions of Superallowed Beta Decays Many Honors: Bonner Prize etc. Authority on Vud = 0.97420(21)(2018 PDG) Will it Survive? “I come to praise Caesar, not to bury him”
Beta decay npeν Wγ BoxSeng, Gorchtein, Patel & Ramsey-MusolfDispersion Relations come to beta decayCongratulations: Major DevelopmentΔRV=0.02361(38) 0.02467(22)Vud=0.97420(21) 0.97370(15) lasting?
Seng, Gorchtein, Patel & Ramsey–Musolf PRL (2018) “Reduced Hadronic Uncertainties in the determination of Vud” Radiative Corrections: Axial Induced part via Dispersion Relation. Claim our RC=0.02361(38) 0.02467(22) |Vud|=0.97420(21) 0.97370(14) |Vud|2+|Vus|2 =0.9994(4)(2)0.9984(3)(2) 4 sigma deviation from unitarity
Work in Progress with A. Czarnecki & A. Sirlin Radiative Corrections to Neutron Decay Preliminary Unsanctioned Update MS(2006) SGPR-M(2018) CMS(2019) RC = 3.89(4)% 3.99(2)% 3.93(3)% Vud = 0.97420(21) 0.97370(14) 0.97400(18) (0.97392)* (0.97422)* *Seng, Gorchtein, Ramsey-MusolfNuclear Quenching My Guess Vud=0.97425(13), n = 878.2(7)sec Based on Vus via Kμ2/πμ2 (very clean theory)
Electroweak Radiative Corrections to Neutron Beta Decay Include Virtual Corrections + Inclusive Bremsstrahlung Normalize using G from the muon lifetime Absorbs Ultraviolet Divergences & some finite parts 1/n= fG2|Vud|2me5(1+3gA2)(1+RC)/23 f=1.6887(1) (Includes Fermi Function etc. not Rad. Corr.) RC calculated for (Conserved) Vector Current. Same RC used to define gA:[A(gA)=(1.001)Aexp] RC=/2[<g(Em)>+3ln(mZ/mp)+ln(mZ/mA)+2C+AQCD] + higher order O(/)2 g(Ee)=Universal Sirlin Function from Vector Current A. Sirlin, PRD 164, 1767 (1967).
/2 <g(Em=1.292579MeV)>=0.015056 long distance loops and brem. averaged over the decay spectrum. Independent of Strong Int. up to O(Ee/mP) g(Ee) also applies to Nuclei A. Sirlin (1967) Uncertainty < 10-5 3/2ln(mZ/mp) short-distance (Vector) log notrenormalized by strong int. [/2[ln(mZ/mA)+2C+AQCD] Induced by axial-current loop Includes hadronic uncertainty mA=1.2GeV long/short distance matching scale (factor 2 mA unc.) C=0.8gA(N+P)=0.891 (long distance W Box diagram) WJM&A.Sirlin(1986) AQCD= -s/(ln(mZ/mA)+cons)=-0.34 QCD Correction [/ln(mZ/m)]n leading logs summed via renormalization group, (+0.0016) Next to leading short distance logs ~ -0.0001, and -2ln(mp/me)=-0.00043 estimated (for neutron decay) Czarnecki, WJM, Sirlin (2004) 1+RC=1.0390(8) main unc. from mA matching short and long distance W (VA) Box. Unc*. ±8x10-4 vs future (±0.1sec goal) n ±1.1x10-4 goal. * Note, unc. cancels in neutron vs nuclear beta decays eg Vud
2006 Improvement WJM & A. Sirlin 1.) Use large NQCD Interpolator to connect long-short distances 3 Resonances & 3 Matching Conditions 2.) Relate neutron beta decay to Bjorken Sum Rule (NF=3) 1-s/ 1-s(Q2)/-3.583(s(Q2)/)2-20.212(s(Q2)/)3 The extra QCD corrections lead to a matching between short and long distance Born corrections at about Q2=(0.8GeV)2 Very little change in size of RC, but uncertainties reduced by a factor of 2.! (Both Prescriptions Agree) 1+RC= 1.0390(8)1.03886(39) for Neutron Beta Decay Reduction by 1.4x10-4 (Same for 0+0+ beta decays) .
RC Error Budget 1) Neglected Two Loop Effects: 0.0001 conservative 2) Long Distance /C~/ (0.75gA(N+P))=0.0020 Assumed Uncertainty 10%0.0002 reasonable? 3) Long-Short Distance Loop Matching: 0.8GeV<Q<1.5GeV 100% 0.0003 conservative? Total RC Error 0.00038 Vud=±0.00019 More Aggressive Analysis Vud=±0.00013 (1/2 conservative) only about 2xn goal of ±0.1sec. (well matched)
Dispersion Relation Approach to Box DiagramSeng, Gorchtein, Patel & Ramsey-Musolf PRL M&S2006(xα/π) S,G.P&R-M2018(xα/π) Perturbation 1.85 1.87 Born 0.83(8) 0.91(5) Interpolator 0.14(14) 0.48(7) Total 2.82(16) 3.26(9) 1+RC 1.03886(38) 1.03992(22) Universal RC 0.02361(38) 0.02467(22)
2019 Update Czarnecki, WJM & Sirlin 1.) Relate neutron beta decay to Bjorken Sum Rule (NF=3) 1-s/ 1-s(Q2)/-3.583(s(Q2)/)2-20.212(s(Q2)/)3 -175.7(s(Q2)/)4 (Baikov,Chetyrkin,Kuhn) 4 loops! = 1 - αBj(Q2)/πphysical coupling perturbative F(Q2) = 1/Q2( 1-Bj(Q2)/) for Q2>Q20 =1.125GeV2 non-perturbative Light Front Holography (LFH) Bj(Q2)/ =exp(-Q2/Q20) Q2≤Q20 Bj(0)/ = 1 AdS F(0)=1/Q20 =0.89GeV-2 The extra QCD correction leads to a matching between short and long distance couplings at about Q2=1.125GeV2
Running QCD Coupling from Bj sum rule data Brodsky, Duer et al.
γW Box RC: Bj Function Approach 1 • Q2 Domain Integral (xα/π) 0<Q2<Q20 0.20 New Effect Q20<Q2<2.25GeV2 0.125 2.25GeV2<Q2<∞ 1.83 ZW Box 0.06 Born 0.856 Σ not Q0 sensitiveMidway 3.07 Total (New) 3.32 DR (2018) 2.82 MS (2006)
2. Large Nc QCD Approach (new) Infinite sum of Vector and Axial-Vector Resonances Use 3 Resonances + 3 Matching Conditions F(Q2) = __ A__ + B + C____ Q2+m2ρ Q2+m2A Q2+m2ρ’ mρ =0.776GeV mA =1.230GeV mρ’ =1.465GeV 1. Integral m2c- ∞ equals Bj Function Integral 2. No 1/Q4 terms in large Q2 limit 3. F(0) =3/4gA(κ2n/mn2-κ2p/mp2) GDH Sum Rule ≈ 0.30GeV-2 (1/Nc0 large Nc limit)?
3 Resonance Solution for F(0)=0.3GeV-2 • A =-1.0603 • B =+5.7820 • C = -3.7783 • Integral 0 –m2c=0.23α/π • Total =2.98α/π (close to 2006) • Average of 2 Approaches=3.02α/π • DR=3.26α/π
Update Summary and Implications DR: 1 + RC=1.03886(38) 1.03992(22) “New Physics” Hint or something else? CMS Preliminary Update Based on 4 loop Bj Function & Q2 integration to 0 • Bj function F(0)=0.89GeV-2 1+RC =1.03944(30) • Large N 3 Resonances F(0)=0.30GeV-2 1+RC= 1.03932(30) Average 1.03938(30) Vud=0.9740(11)(15)
Comments on DR Results 1. Difference with CMS only ~ 0.05% 2. Is ZW Box included? Added 0.01% 3. Validity of GLS sum rule low Q2 data 4. Possible Double Counting? 5. Born Uncertainty? Alternative Issues with Bj & Interpolator? Try method elsewhere More complicated low Q2 behavior
Fornal-Grinstein Solution BR(ndark particles) ~ 1% BR(npeν)=0.9999(7) + 1.30(gA-1.2755) Total exotic n decay BR < 0.27% at 95%CL For Fornal-Grinstein Solution to be valid, post 2002 gA asymmetry values from PERKEOII and UCNA must be wrong (significant tension) PerkeoIII BR(n”new physics”) < 0.10% 95%CL
Recent gA =1.2764(6) Perkeo III Result Post 2002 gAave=1.2762(5) n = 878.2(7)s Neutron Lifetime Problem nbeam =888.0(2.0)s ntrap=879.4(6)s Could Both Be Right? ntrap(ave)=879.4(6) good agreement BR(any exotic n decay)< 0.10% (95% C.L.) Requires “Creative” Theorists