qed corrections to p finite volume effects
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QED corrections to P ( ) : finite volume effects southampton, - PowerPoint PPT Presentation

nazario tantalo nazario.tantalo@roma2.infn.it v.lubicz, g.martinelli, c.t.sachrajda, f.sanfilippo, s.simula, c.tarantino QED corrections to P ( ) : finite volume effects southampton, 27-07-2016 outline P P


  1. nazario tantalo nazario.tantalo@roma2.infn.it v.lubicz, g.martinelli, c.t.sachrajda, f.sanfilippo, s.simula, c.tarantino QED corrections to P − → ℓ ¯ ν ( γ ) : finite volume effects southampton, 27-07-2016

  2. outline ℓ ℓ P − P − • phenomenological motivation ¯ ν ℓ ν ℓ ¯ • infrared-safe measurable observables γ ℓ ℓ • the RM123-SOTON strategy P − P − ν ℓ ¯ ν ℓ ¯ • universality of IR logs and 1 /L terms γ • sums approaching integrals ℓ ℓ P − P − ¯ ν ℓ ¯ ν ℓ • analytical result for ∆Γ pt 0 ( L ) • conclusions & outlooks � 1 c 1 � � � L 2 m 2 ∆Γ 0 ( L ) − ∆Γ 0 ( ∞ ) = c IR log + + O P L 2 Lm P

  3. phenomenological motivations FLAG, arXiv:1607.00299 PDG review, j.rosner, s.stone, r.van de water, 2016 ± ± v.cirigliano et al., Rev.Mod.Phys. 84 (2012) + FLAG average for = + + FLAG average for = + + ETM 14E ETM 14E + FNAL/MILC 14A FNAL/MILC 14A HPQCD 13A HPQCD 13A = MILC 13A MILC 13A ETM 10E ETM 10E FLAG average for = + ℓ FLAG average for = + RBC/UKQCD 14B RBC/UKQCD 14B + RBC/UKQCD 12A RBC/UKQCD 12A Laiho 11 Laiho 11 + MILC 10 MILC 10 MILC 10 MILC 10 + JLQCD/TWQCD 10 JLQCD/TWQCD 10 = RBC/UKQCD 10A RBC/UKQCD 10A PACS-CS 09 P − PACS-CS 09 = JLQCD/TWQCD 09A JLQCD/TWQCD 09A MILC 09A MILC 09A MILC 09A MILC 09A MILC 09 MILC 09 + MILC 09 MILC 09 Aubin 08 Aubin 08 = PACS-CS 08,08A PACS-CS 08,08A RBC/UKQCD 08 RBC/UKQCD 08 HPQCD/UKQCD 07 ¯ ν ℓ HPQCD/UKQCD 07 MILC 04 MILC 04 FLAG average for = FLAG average for = ETM 14D ETM 14D = TWQCD 11 TWQCD 11 ETM 09 ETM 09 = JLQCD/TWQCD 08A JLQCD/TWQCD 08A PDG PDG 120 130 140 145 155 165 MeV • QED corrections are currently estimated in χ -pt • from the last FLAG review we have δ QED Γ[ π − → ℓ ¯ ν ] = 1 . 8% , f π ± = 130 . 2(1 . 4) MeV , δ = 1 . 1% , δ QED Γ[ K − → ℓ ¯ f K ± = 155 . 6(0 . 4) MeV , δ = 0 . 3% , ν ] = 1 . 1% , f + (0) = 0 . 9704(24)(22) , δ = 0 . 3% δ QED Γ[ K → πℓ ¯ ν ] = [0 . 5 , 3]%

  4. the infrared problem • let’s consider the extraction of a matrix-element from an euclidean correlator C ( t, p ) = � 0 | A ( t ) P (0 , p ) | 0 � , t > 0 A P • we know very well what we have to do when there is a mass-gap � P ( 0 ) | P | 0 � e − tmP + R ( t ) , C ( t, 0 ) = � 0 | A | P ( 0 ) � 2 m P R ( t ) = R 1 e − tE 1 + · · · • in presence of electromagnetic interactions, the states A P H | P γ 1 · · · γ n � = �� � P + ( k 1 + · · · k n ) 2 + | k 1 | + · · · + | k n | m 2 | P γ 1 · · · γ n � are degenerate with | P ( 0 ) � in the limit k i �→ 0

  5. infrared-safe measurable observables f.bloch, a.nordsieck, Phys.Rev. 52 (1937) t.d.lee, m.nauenberg, Phys.Rev. 133 (1964) p.p.kulish, l.d.faddeev, Theor.Math.Phys. 4 (1970) • the infrared problem has been analyzed by many authors over the years � × 2 b.p.s • electrically-charged asymptotic states are not eigenstates of the photon-number operator • the perturbative expansion of decay-rates and � cross-sections with respect to α is cumbersome × 3 b.p.s because of the degeneracies • the block & nordsieck approach consists in lifting the degeneracies by introducing an infrared regulator, say m γ , and in computing infrared-safe ( p + k ) 2 + m 2 P = 2 p · k + k 2 ∼ 2 p · k , observables • at any fixed order in α , infrared-safe observables d 4 k � � 1 m P are obtained by adding the appropriate number of � ∼ c IR log , photons in the final states and by integrating over k 2 (2 p · k ) (2 p ℓ · k ) (2 π ) 4 m γ their energy in a finite range, say [0 , ∆ E ] � m γ � m P � � � �� • in this framework, infrared divergences appear at m P � c IR log + log = c IR log intermediate stages of the calculations and cancel m γ ∆ E ∆ E in the sum of the so-called virtual and real contributions

  6. the RM123+SOTON strategy RM123, Phys.Rev. D87 (2013) RM123+SOTON, Phys.Rev. D91 (2015) • we have proposed to compute the leptonic decay-rate of a pseudoscalar meson at O ( α ) ; in this case the infrared-safe observable is obtained by considering the real contributions with a single photon in the final state Γ(∆ E ) = Γ tree + e 2 L →∞ { ∆Γ 0 ( L ) + ∆Γ 1 ( L, ∆ E ) } lim 0 • given a formulation of QED on the finite volume, L acts as an infrared regulator in the previous formula • the finite-volume calculation of the real contribution is challenging: momenta are quantized and one would need very large volumes in order to perform the three-body phase space integral in the soft-photon region with an acceptable resolution; for this reason we have rewritten the previous formula as Γ(∆ E ) = Γ tree + e 2 � ∆Γ 0 ( L ) − ∆Γ pt 0 ( L ) + ∆Γ pt � lim 0 ( L ) + ∆Γ 1 ( L, ∆ E ) 0 L →∞ • ∆Γ pt 0 ( L ) is the virtual decay rate calculated in the effective theory in which the meson is treated as a point-like particle; the so-called structure dependent contributions are given by ∆Γ SD ( L ) = ∆Γ 0 ( L ) − ∆Γ pt 0 ( L ) 0

  7. the RM123+SOTON strategy RM123+SOTON, Phys.Rev. D91 (2015) h.georgi, Ann.Rev.Nucl.Part.Sci. 43 (1993) • the lagrangian of the point-like effective theory is L pt = φ † � − D 2 µ + m 2 � � 2 iG F V CKM f P D µ φ † P ( x ) ¯ ℓ ( x ) γ µ ν ( x ) + h.c. � P ( x ) φ P ( x ) + , P D µ = ∂ µ − ieA µ ( x ) • the matching with the full theory is obtained by using Γ tree 0 G 2 F | V CKM | 2 f 2 � 2 , m ℓ Γ tree ,pt = Γ tree m 3 P r 2 � 1 − r 2 P = r ℓ = 0 ℓ ℓ 0 8 π m P • properly matched effective theories have the same infrared behaviour of the full theory: ∆Γ pt 0 ( L ) has exactly the same infrared divergence of ∆Γ 0 ( L ) and we can write � � ∆ E Γ(∆ E ) = Γ tree + e 2 L →∞ ∆Γ SD ( L ) + e 2 � ∆Γ pt 0 ( m γ ) + ∆Γ pt � lim lim 1 ( m γ , ∆ E ) + O 0 0 mγ →∞ Λ QCD • we have shown that the neglected terms are phenomenologically irrelevant for P = { π, K } and ∆ E ∼ 20 MeV

  8. the RM123+SOTON strategy RM123+SOTON, Phys.Rev. D91 (2015) • in our original proposal we have not performed an analysis of the finite volume corrections affecting ∆Γ 0 ( L ) : we are now going to fill the gap! • the L �→ ∞ asymptotic expansion of the decay rate can be written as � 1 c 1 � � � L 2 m 2 ∆Γ 0 ( L ) − ∆Γ 0 ( ∞ ) = c IR log + + O P L 2 Lm P � 1 c 1 � ∆Γ pt 0 ( L ) − ∆Γ pt � L 2 m 2 � 0 ( ∞ ) = c IR log + + O P L 2 Lm P • in the following, we shall show that the coefficients c IR and c 1 are universal , i.e. they are the same in the full theory and in the point-like approximation • therefore, the finite volume effects on the non-perturbative structure-dependent contributions are � 1 � ∆Γ SD ( L ) − ∆Γ SD ( ∞ ) = O 0 0 L 2 • than we shall give an explicit analytical expression for ∆Γ pt 0 ( L )

  9. universality of IR logs and 1 /L terms 1.0 Ε� 0.02 0.8 Ε� 0.01 0.6 × 0.4 0.2 1 ∼ 2 p · k + k 2 0.0 0.00 0.02 0.04 0.06 0.08 0.10 • to see how this works, let’s consider the contribution to the decay rate coming from the diagrams shown in the figure   d 3 k dk 0 1 1 L αµ ( k ) � �   H αµ ( k, p ) � ∆Γ P ℓ ( L ) − ∆Γ P ℓ ( ∞ ) = − L 3 (2 π ) 3 k 2 2 p ℓ · k + k 2 2 π  k � =0  • infrared divergences and power-law finite volume effects come from the singularity at k 2 = 0 of the integrand and from the QED L prescription k � = 0 • the tensor L αµ is a regular function, it contains the numerator of the lepton propagator and the appropriate normalization factors L αµ ( k ) ≡ L αµ ( k, p ν , p ℓ ) = O (1)

  10. universality of IR logs and 1 /L terms • the hadronic tensor is a QCD quantity that, by neglecting exponentially P, · · · suppressed finite volume effects, is given by � 0 | J α j µ | P � W � d 4 x e ik · x T � 0 | J α H αµ ( k, p ) = i W (0) j µ ( x ) | P ( 0 ) � , P P, · · · ( p + k ) α (2 p + k ) µ � 0 | j µ J α � � W | P � H αµ δ αµ − pt ( k, p ) = f P 2 p · k + k 2 • the point like effective theory is built in such a way to satisfy the same WIs of the full theory k µ H αµ ( k, p ) = − f P p α , H αµ SD ( k, p ) = H αµ ( k, p ) − H αµ k µ H αµ pt ( k, p ) , SD ( k, p ) = 0 • the structure dependent contributions are regular and, since there is no constant two-index tensor orthogonal to k , p · k δ αµ − k α p µ � H αµ F A + ǫ αµρσ p ρ k σ F V + · · · = O ( k ) SD ( k, p ) = �

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