<p>Hadronic <i>τ</i> decays present an opportunity to determine the isovector part of the hadronic-vacuum-polarization contribution to the anomalous magnetic moment of the muon in a way complementary to <i>e</i><sup>+</sup><i>e</i><sup>−</sup> → hadrons cross sections. However, the required isospin rotation is only exact in the isospin limit, and corrections need to be under control to draw robust conclusions, most notably for <i>τ</i> → <i>ππν</i><sub><i>τ</i></sub> decays to determine the two-pion contribution, <InlineEquation ID="IEq1"> <EquationSource Format="MATHML"><math display="inline"> <msubsup> <mi>a</mi> <mi>μ</mi> <mrow> <mi>HVP</mi> <mo>,</mo> <mi>LO</mi> </mrow> </msubsup> <mfenced close="]" open="[" separators=","> <mi mathvariant="italic">ππ</mi> <mi>τ</mi> </mfenced> </math></EquationSource> <EquationSource Format="TEX">\( {a}_{\mu}^{\textrm{HVP},\textrm{LO}}\left[\pi \pi, \tau \right] \)</EquationSource> </InlineEquation>. In this work, we present a novel analysis of the required radiative corrections using dispersion relations, thereby extending in a model-independent way the previous analysis in chiral perturbation theory (ChPT) beyond the threshold region. In particular, we include the dominant structure-dependent virtual corrections from pion-pole diagrams, leading to sizable changes in the vicinity of the <i>ρ</i>(770) resonance. Moreover, we work out the matching to ChPT and devise a strategy for a stable numerical evaluation of real-emission contributions near the two-pion threshold, which proves important to capture isospin-breaking corrections enhanced by the threshold singularity. For the numerical analysis, we use a dispersive representation of the pion form factor including the <i>ρ</i><sup>′</sup>, <i>ρ</i><sup>′′</sup> resonances, perform fits to the available data sets for the <i>τ</i> → <i>ππν</i><sub><i>τ</i></sub> spectral function, and calculate the corresponding radiative correction factor <i>G</i><sub>EM</sub>(<i>s</i>) in a self-consistent manner. Based on these results, we evaluate the <i>τ</i>-specific isospin-breaking corrections to <InlineEquation ID="IEq2"> <EquationSource Format="MATHML"><math display="inline"> <msubsup> <mi>a</mi> <mi>μ</mi> <mrow> <mi>HVP</mi> <mo>,</mo> <mi>LO</mi> </mrow> </msubsup> <mfenced close="]" open="[" separators=","> <mi mathvariant="italic">ππ</mi> <mi>τ</mi> </mfenced> </math></EquationSource> <EquationSource Format="TEX">\( {a}_{\mu}^{\textrm{HVP},\textrm{LO}}\left[\pi \pi, \tau \right] \)</EquationSource> </InlineEquation>.</p>

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Radiative corrections to τππντ

  • Gilberto Colangelo,
  • Martina Cottini,
  • Martin Hoferichter,
  • Simon Holz

摘要

Hadronic τ decays present an opportunity to determine the isovector part of the hadronic-vacuum-polarization contribution to the anomalous magnetic moment of the muon in a way complementary to e+e → hadrons cross sections. However, the required isospin rotation is only exact in the isospin limit, and corrections need to be under control to draw robust conclusions, most notably for τππντ decays to determine the two-pion contribution, a μ HVP , LO ππ τ \( {a}_{\mu}^{\textrm{HVP},\textrm{LO}}\left[\pi \pi, \tau \right] \) . In this work, we present a novel analysis of the required radiative corrections using dispersion relations, thereby extending in a model-independent way the previous analysis in chiral perturbation theory (ChPT) beyond the threshold region. In particular, we include the dominant structure-dependent virtual corrections from pion-pole diagrams, leading to sizable changes in the vicinity of the ρ(770) resonance. Moreover, we work out the matching to ChPT and devise a strategy for a stable numerical evaluation of real-emission contributions near the two-pion threshold, which proves important to capture isospin-breaking corrections enhanced by the threshold singularity. For the numerical analysis, we use a dispersive representation of the pion form factor including the ρ, ρ′′ resonances, perform fits to the available data sets for the τππντ spectral function, and calculate the corresponding radiative correction factor GEM(s) in a self-consistent manner. Based on these results, we evaluate the τ-specific isospin-breaking corrections to a μ HVP , LO ππ τ \( {a}_{\mu}^{\textrm{HVP},\textrm{LO}}\left[\pi \pi, \tau \right] \) .