Standard Model Theory of Neutron Beta Decay

Similar documents
Electric Dipole Moments A Theoretical Perspective. Lecture 3 William J. Marciano May 21, 2013

V ud, V us, THE CABIBBO ANGLE, AND CKM UNITARITY Updated March 2012 by E. Blucher (Univ. of Chicago) and W.J. Marciano (BNL)

Radiative Corrections in Free Neutron Decays

Electroweak Theory: 2

Neutron Lifetime & CKM Unitarity: The Standard Model & Beyond

Test of the Standard Model with Kaon decays. Barbara Sciascia LNF-INFN for the Kaon WG, FlaviaNet PhiPsi08 - LNF, 7 April 2008

Low Energy Precision Tests of Supersymmetry

Weak Decays: theoretical overview

Electroweak Physics. Precision Experiments: Historical Perspective. LEP/SLC Physics. Probing the Standard Model. Beyond the Standard Model

Tales From The Dark Side of Particle Physics (The Dark-Light Connection) William J. Marciano

Precision sin 2 θ W (Q 2 ) & Electroweak Physics at The EIC (Electron-Ion Collider) Based on talks at: W&M, Rockefeller, BNL and U.

Lecture 11. Weak interactions

Electroweak Physics: Lecture V

Muonium Decay. Abstract

The Standard Model and Beyond

the role of atom and ion traps

Superb prospects: Physics at Belle II/SuperKEKB

Neutron Beta-Decay. Christopher B. Hayes. December 6, 2012

SECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS

Beyond Standard Model Effects in Flavour Physics: p.1

CKM Unitary tests with Tau decays

Particle Physics: Problem Sheet 5

A model of the basic interactions between elementary particles is defined by the following three ingredients:

Electroweak Theory: 5

Lecture 12 Weak Decays of Hadrons

Weak Decays, CKM, Anders Ryd Cornell University

CKM Matrix and CP Violation in Standard Model

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

The Cabibbo-Kobayashi-Maskawa (CKM) matrix

PoS(CKM2016)028. V ud from Nuclear Beta Decays. J.C. Hardy and I.S. Towner

Shahram Rahatlou University of Rome

TAMU-TRAP facility for Weak Interaction Physics. P.D. Shidling Cyclotron Institute, Texas A&M University

CKM unitarity normalization tests, present and future

OUTLINE. CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion

The MSSM confronts the precision electroweak data and muon g 2. Daisuke Nomura

Recent results from rare decays

- ~200 times heavier than the e GeV µ travels on average. - does not interact strongly. - does emit bremsstrahlung in

Moriond QCD La Thuile, March 14 21, Flavour physics in the LHC era. An introduction. Clara Matteuzzi. INFN and Universita Milano-Bicocca

Unitary Triangle Analysis: Past, Present, Future

Precision Tests of the Standard Model. Yury Kolomensky UC Berkeley Physics in Collision Boston, June 29, 2004

The Muon g 2 Challenging e+e and Tau Spectral Functions

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

Flavour physics Lecture 1

Precision Nuclear Mass Measurements Matthew Redshaw Exotic Beam Summer School, Florida State University Aug 7 th 2015

FLAVOR PHYSICS BEYOND THE STANDARD MODEL

Standard Model of Particle Physics SS 2013

Search for Physics Beyond the Standard Model at B Factories

Abdelhak DJOUADI ( LPT Orsay)

Light hadrons in 2+1 flavor lattice QCD

Electroweak interactions of quarks. Benoit Clément, Université Joseph Fourier/LPSC Grenoble

The CKM matrix elements and their determination. Phil Strother LBL

Advances in Open Charm Physics at CLEO-c

Superallowed Fermi Beta Decay

Theoretical Review on Lepton Universality and LFV

Conference Summary. K.K. Gan The Ohio State University. K.K. Gan Tau2000 1

SO(10) SUSY GUTs with family symmetries: the test of FCNCs

Interactions/Weak Force/Leptons

Measurements of the W Boson Mass and Trilinear Gauge Boson Couplings at the Tevatron

Physics at the Tevatron. Lecture III

Standard Model & Beyond

Physics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1

PoS(KAON)052. π eν. Prospects for Measurements of the Branching Ratio. Douglas Bryman

Results from B-Physics (LHCb, BELLE)

generation Outline Outline Motivation Electroweak constraints Selected flavor constraints in B and D sector Conclusion Nejc Košnik

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst

The Mystery of Vus from Tau decays. Swagato Banerjee

Weak Interactions: towards the Standard Model of Physics

Little Higgs Models Theory & Phenomenology

Effective Field Theories Beyond the Standard Model

The W-mass Measurement at CDF

LIMIT ON MASS DIFFERENCES IN THE WEINBERG MODEL. M. VELTMAN Institute for Theoretical Physics, University of Utrecht, Netherlands

Parity violation. no left-handed ν$ are produced

Fundamental Symmetries III Muons. R. Tribble Texas A&M University

Flavour Physics at hadron machines

Effective Field Theory

KSETA-Course: Accelelerator-Based Particle Physics

PUZZLING b QUARK DECAYS: HOW TO ACCOUNT FOR THE CHARM MASS

Intense Slow Muon Physics

V cb. Determination of. and related results from BABAR. Masahiro Morii, Harvard University on behalf of the BABAR Collaboration

Particules Élémentaires, Gravitation et Cosmologie Année Le Modèle Standard et ses extensions. The Flavour Sector

SECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS

Flavour Physics. WIN 2015 Heidelberg, Germany, June 8-13, 2015 Tatsuya Nakada. LPHE EPFL Lausanne, Switzerland

Theory of the ElectroWeak Interactions

Problems for SM/Higgs (I)

La Fisica dei Sapori Pesanti

Introduction to Particle Physics. Sreerup Raychaudhuri TIFR. Lecture 5. Weak Interactions

Koji TSUMURA (NTU Nagoya U.) KEK 16-18/2/2012

CKM : Status and Prospects

Fundamental Symmetries - 2

New Physics from Vector-Like Technicolor: Roman Pasechnik Lund University, THEP group

Lepton Universality Tests with Kaons

Interactions/Weak Force/Leptons

RESULTS FROM B-FACTORIES

Flavour Physics Lecture 1

Kaon Decays in the Standard Model

SUSY and Exotics. UK HEP Forum"From the Tevatron to the LHC, Cosener s House, May /05/2009 Steve King, UK HEP Forum '09, Abingdon 1

Two photon exchange: theoretical issues

Standard Model and ion traps: symmetries galore. Jason Clark Exotic Beam Summer School July 28 August 1, 2014

Lecture 23. November 16, Developing the SM s electroweak theory. Fermion mass generation using a Higgs weak doublet

Transcription:

Standard Model Theory of Neutron Beta Decay The Utility of a Δτ n/ τ n measurement to ±0.01%! (Electroweak Radiative Corrections) William J. Marciano November 9, 2012 Santa Fe, NM

Neutron Decay Master Relations 1) V ud 2 = 4908.7(1.9)sec Unc. Radiative Corrections τ n (1+3g A2 ) Same as in Nuclear β Decay 2) τ n = 4908.7(1.9)sec Radiative Corrections Cancel! V ud 2 (1+3g A2 ) 3) (1+3g A2 ) = 4908.7(1.9)sec Radiative Corrections Cancel! V ud 2 τ n Current Δ V ud 2 / V ud 2 = ±0.02% NP = ±0.04% RC Superallowed β Δτ n/ τ n = ±0.12% Δg A2 /g A 2 ±0.20% τ n PDG =880.1(1.1)sec. Recent g A = 1.2755(13) Perkeo II ±0.01% Outstanding/Appropriate Goals for τ n and g A 2

Refs: A. Sirlin RMP 50, 573 (1978) + earlier work WJM & A. Sirlin, PRL 56, 22 (1986); ibid 96, 032002 (2006) A. Czarnecki, WJM, A. Sirlin, PRD 70, 093006 (2004) Also see the classic: D. Wilkinson, NP SU(2) L xu(1) Y Standard Model Electroweak Radiative Corrections to µ eν e ν µ and n peν e both Infinite but renormalized using (G F0 G µ ) Quark mixing divergences absorbed in V 0 ud V ud maintaining Unitarity The CKM Quark Mixing Matrix: V ud V us V ub V CKM = V cd V cs V cb V td V ts V tb 3x3 Unitary Matrix Unitarity V ud 2 + V us 2 + V ub 2 =1 Any Apparent Deviation from 1 Implies New Physics at the tree or quantum loop level

Short-distance behavior of µ and β decays differ due to weak hypercharges of µ L (Y=-1) and d L. (Y=+1/3). Different anomalous dimensions! Muon Decay Γ 0 (µ eνν)=f(m e2 /m µ2 )G 0 F 2 m µ5 /192π 3 = 1/τ µ 0 Neutron Decay Γ 0 (n peν)=fg 0 F 2 V 0 ud 2 m e5 (1+3g A2 )/2π 3 =1/τ n 0 F(x)=1-8x+8x 3 -x 4-12x 2 lnx Phase Space Factor f=1.6887 phase space factor, including Fermi function proton recoil, finite nucleon size Uncertainty O(few x10-5 ) Other Effects: Weak Magnetism, Induced Pseudoscalar etc. negligible g A and τ n important for: Unitarity test, solar neutrino flux, reactor neutrino flux, primordial abundances, spin content of proton, Goldberger-Treiman/Muon Capture, Bjorken Sum Rule, lattice benchmark Must be precisely determined!

Electroweak Radiative Corrections to Muon Decay Virtual One Loop Corrections + Inclusive Bremsstrahlung Absorb Ultraviolet divergences and some finite parts in G 0 F =g 0 2 /4 2m 2 W0 G µ τ µ -1 = Γ(µ + e + ν e ν µ (γ)) F(m e2 /m µ2 )G µ2 m µ5 [1+RC]/192π 3 RC =α/2π(25/4-π 2 )(1+α/π[2/3ln(m µ /m e )-3.7) ] Fermi Th. Defines G µ Other SM and New Physics radiative corrections absorbed into G µ. Eg. Top Mass, Higgs Mass, Technicolor, Susy,W* MuLAN experiment at PSI (Complete) World Ave. τ µ+ =2.1969803(22)x10-6 sec 1ppm! Most precise lifetime ever measured gives: G µ =1.1663787(6)x10-5 GeV -2 precise & important

Electroweak Radiative Corrections to Neutron Beta Decay Include Virtual Corrections + Inclusive Bremsstrahlung Normalize using G µ from the muon lifetime Absorbs Ultraviolet Divergences & some finite parts 1/τ n = fg µ2 V ud 2 m e5 (1+3g A2 )(1+RC)/2π 3 f=1.6887 (Includes Fermi Function etc. not Rad. Corr.) RC calculated for (Conserved) Vector Current since it is not renormalized by strong interaction at zero momentum transfer. Same RC used to define g A : [A(g A )=(1.001)Aexp ] RC=α/2π[<g(E m )>+3ln(m Z /m p )+ln(m Z /m A )+2C+A QCD ] + higher order O(α/π) 2 g(e e )=Universal Sirlin Function (1967) from Vector Current A. Sirlin, PRD 164, 1767 (1967).

α/2π <g(e m =1.292579MeV)>=0.015056 long distance loops and brem. averaged over the decay spectrum. Independent of Strong Int. up to O(E e /m P ) g(e e ) also applies to Nuclei A. Sirlin (1967) Uncertainty < 10-5 3α/2πln(m Z /m p ) short-distance (Vector) log not renormalized by strong int. [α/2π[ln(m Z /m A )+2C+A QCD ] Induced by axial-current loop Includes hadronic uncertainty m A =1.2GeV long/short distance matching scale (factor 2 m A unc.) C=0.8g A (µ N +µ P )=0.891 (long distance γw Box diagram) WJM&A.Sirlin(1986) A QCD = -α s /π(ln(m Z /m A )+cons)=-0.34 QCD Correction [α/πln(m Z /m)] n leading logs summed via renormalization group, (+0.0016) Next to leading short distance logs ~ -0.0001, and -α 2 ln(m p /m e )=-0.00043 estimated (for neutron decay) Czarnecki, WJM, Sirlin (2004) 1+RC=1.0390(8) main unc. from m A matching short and long distance γw (VA) Box. Unc*. ±8x10-4 vs future (discussed here ±0.1sec) τ n ±1.1x10-4 goal. * Note, unc. cancels in neutron vs nuclear beta decays eg V ud

γw Box Diagram

2006 Improvement WJM & A. Sirlin 1.) Use large N QCD Interpolator to connect long-short distances 2.) Relate neutron beta decay to Bjorken Sum Rule (N F =3) 1-α s /π 1-α s (Q 2 )/π-3.583(α s (Q 2 )/π) 2-20.212(α s (Q 2 )/π) 3-175.7 (α s (Q 2 )/π) 4 (Baikov,Chetyrkin and Kuhn) Negligible Effect The extra QCD corrections lead to a matching between short and long distance corrections at about Q 2 =(0.8GeV) 2 Very little change in size of RC, but uncertainties reduced by a factor of 2 (perhaps 3)! (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) Unc. Reduced to ±3.9x10-4 (about 3x τ n goal).

RC Error Budget 1) Neglected Two Loop Effects: ±0.0001 conservative 2) Long Distance α/πc~α/π (0.75g A (µ N +µ 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 ΔV ud =±0.00019 More Aggressive Analysis ΔV ud =±0.00013 (1/2 conservative) only about 2xτ n goal of ±0.1sec. (well matched)

Superallowed (0 + 0 + ) Beta Decays & V ud RC same as in Neutron Decay but with <g(e m )> averaged Nuclear decay spectrum, C modified by Nucleon-Nucleon Interactions and +Z α 2 ln(m p /m e ) corrections (opposite sign from neutron) ft= V ud 2 (2984.5s)(1+RC)(1+NP corr.) Nuclear Physics (NP) isospin breaking effects (Hardy & Towner Calculations: See later critique) ft values + RC for 13 precisely measured nuclei found to be consistent with CVC: Average V ud

Superallowed Nuclear Beta Decays RC Uncertainty-Same as Neutron Decay Nuclear Unc. - Significantly Reduced (2006-08) Nuclear Coulomb Corrections Improved V ud = 0.97425(11) Nuc (19) RC (2008 Hardy and Towner Update) (0.97418((13)(14)(19) in PDG08) (0.97377(11)(15)(19) in PDG06) (0.97340(80) in 2004) Factor of 3 worse

The Kaon Revolution of 2004-2005 (Starting with BNL E865) +FNAL, Frascati & CERN BR(K πeν) increased by 6%! All Major K L BRs Changed! ε K changed by 3.7σ! Now Based on: Γ(K πlν) exp & Γ(K µν)/γ(π µν) exp + Lattice Matrix Elements f + (0)=0.960(5) & f K /f π =1.193(6) 2010 Flavianet Analysis Currently: V us =0.2253(13) from K πlν Vector V us =0.2252(13) from K µν Axial-Vector V us =0.2253(9) Kaon Average (was ~0.220 pre 2004) (Watch for lattice updates)

CURRENT STATUS of CKM Unitarity V ud 2 + V us 2 + V ub 2 =0.9999(4) Vud (4) Vus =0.9999(6) Outstanding Agreement With Unitarity Confirms CVC & SM Radiative Corrections: 2αln(m Z /m p )/π+ +3.6% at 60 sigma level! Naively Fits m Z =90(7)GeV vs 91.1875GeV (Direct) Comparison of G µ with other measurements (normalization) constrains or unveils New Physics New Physics Constraints-Implications: Exotic Muon Decays, W*bosons, SUSY, Technicolor, Z Bosons, H ±, Heavy Quark/Lepton Mixing

Comparisons can be viewed as a probe of differences among Fermi Constants µ e Decay G µ =1.1663787(6)x10-5 GeV -2 τ µ Decay G F =1.1678000(26000)x10-5 GeV -2 τ e Decay G F =1.1675000(26000)x10-5 GeV -2 Tests e-µ-τ Universality Agreement Constrains Heavy Lepton Mixing CKM Unitarity: G F CKM =1.1663000(3000)x10-5 GeV -2 Best After τ µ! Agreement Constrains: Exotic Muon Decays, Heavy Quark Mixing, W* (extra dim., Sequential ),SUSY Loops, H -, (Squarks vs Sleptons), Z,

Exotic Muon Decays: µ eν e ν µ wrong neutrinos! BR 0.001 (95%CL) Potential Background Uncertainty For Neutrino Oscillations At Neutrino Factory Heavy Quark Mixing (e.g. E6 D L singlets) V ud 0.03 Similar Heavy Lepton Constraint Seems unlikely, since V ub =0.003

W* Excited KK Bosons or sequential W (different µ & β) 4(m W /m W* ) 2 =0.0001(6), m W* >6TeV? Unless Cancellation with muon decay? (1TeV extra dim. Unlikely?) LHC sequential W? 2 Higgs Doublets Charged Higgs H ± m H± 5.6tanβ (From K µν)

Superallowed Beta Decay Issue Isospin Breaking Coulomb Corrections of Hardy and Towner questioned by: G. Miller & A. Schwenk N. Auerbach H. Liang et al. Hardy and Towner (1-δ C ) correction increases V ud δ C ~0.2-1.6% Correction Recent Claims δ C is smaller due to nuclear radial excitations smaller V ud =0.97425 0.9730 (Liang, Giai, Meng) V ud 2 + V us 2 + V ub 2 reduced to (roughly) 0.9975? Unitarity Lost? Issue needs complete quantitative resolution ( Experimentally Addressed by Hardy & Towner)

Neutron Decay (n peν) & V ud V ud 2 = 4908.7(1.9)sec Master Relation τ n (1+3g A2 ) Measure τ n and g A G A /G V (decay asymmetries) 2008 PDG τ n ave =885.7(8)sec, g A ave =1.2695(29) V ud ave =0.9746(4) τn (18) ga (2) RC reasonable but 2012 τ n PDG 880.1(1.1)sec? & g A 1.2755(13) Perkeo II V ud =0.9739(6) τn (8) ga (2) RC Agrees with superallowed! 0 + 0 + Nuclear Beta V ud =0.97425(22) (Are τ n & g A both shifting?) History g A =1.18 1.23 1.25 1.26 1.27 1.275? Many New τ n & g A Experiments Planned

2012 PDG (Confusion) 2010 PDG τ n ave =885.7(8)sec, g A ave =1.2695(28) 2012 PDG τ n ave =880.1(1.1)sec, g A ave =Deferred (1.275?) Should expect g A =1.275 Independent of Radiative Corrections! Experimental measurements of g A and τ n will test Nuclear Coulombic corrections.

Conclusion

Goals 1) Extraction of g A from τ n &V ud (nuclear) independent of radiative corrections unc! τ n to±0.1 sec + V ud = 0.97425(11) Nuc Δg A to ±0.0001! 2) V ud comparison of neutron and nuclear beta decays ( V ud = 0.97425(11) Nuc (19) RC ) suggests τ n should be measured to ±0.1sec ΔV ud ±0.000055! Good Luck