Abstract

The light axial-vector resonances $a_1(1260)$ and $b_1(1235)$ are explored in Nf=2 lattice QCD by simulating the corresponding scattering channels $\rho\pi$ and $\omega\pi$. Interpolating fields $\bar{q} q$ and $\rho\pi$ or $\omega\pi$ are used to extract the s-wave phase shifts for the first time. The $\rho$ and $\omega$ are treated as stable and we argue that this is justified in the considered energy range and for our parameters $m_\pi\simeq 266~$MeV and $L\simeq 2~$fm. We neglect other channels that would be open when using physical masses in continuum. Assuming a resonance interpretation a Breit-Wigner fit to the phase shift gives the $a_1(1260)$ resonance mass $m_{a1}^{res}=1.435(53)(^{+0}_{-109})$ GeV compared to $m_{a1}^{exp}=1.230(40)$ GeV. The $a_1$ width $\Gamma_{a1}(s)=g^2 p/s$ is parametrized in terms of the coupling and we obtain $g_{a_1\rho\pi}=1.71(39)$ GeV compared to $g_{a_1\rho\pi}^{exp}=1.35(30)$ GeV derived from $\Gamma_{a1}^{exp}=425(175)$ MeV. In the $b_1$ channel, we find energy levels related to $\pi(0)\omega(0)$ and $b_1(1235)$, and the lowest level is found at $E_1 \gtrsim m_\omega+m_\pi$ but is within uncertainty also compatible with an attractive interaction. Assuming the coupling $g_{b_1\omega\pi}$ extracted from the experimental width we estimate $m_{b_1}^{res}=1.414(36)(^{+0}_{-83})$.

Highlights

  • Our simulation is the first attempt at extracting the s-wave scattering phase shifts for ρπ or ωπ channels in lattice QCD

  • In the b1 channel, we find energy levels related to π(0)ω(0) and b1(1235), and the lowest level is found at E1 mω + mπ but is within uncertainty compatible with an attractive interaction

  • We estimate the expected energy shift a∆E1 ≃ −0.01 based on gbe1xωpπ, Breit-Wigner dependence (6.4), the Luscher relation (6.2) and the value of mrbe1s (7.1) determined below; note that this shift is smaller than the uncertainty of the ground state energy level in the b1 channel and comparable to the uncertainty in amω

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Summary

Lattice setup

Due to the limited data for just a single ensemble, our determination of the lattice spacing a reported in [3] results from taking a typical value of the Sommer parameter r0. The sea and valence quarks obey periodic boundary conditions in space. Valence quark propagators periodic and anti-periodic in time are combined into so-called “P + A” propagators, which effectively extends the time direction to 2NT = 64 [3]. The rather small volume V = 163 × 32 (L ≃ 2 fm) simplifies the use of the powerful full distillation method [29], which allows for the computation of all contractions for the correlation matrix with qq and V π interpolators. A small box has the advantage that the effect of ρ → 2π and ω → 3π is less significant in our simulation with total momentum zero

Discussion of assumptions
Energies in a1 and b1 channels
Analysis of the b1 channel
Conclusions and outlook
A Wick contractions and the correlation matrix
The ωπ s-wave correlation matrix

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