论文标题

使用C $^{\ Star} $调整QCD+QED模拟$边界条件

Tuning of QCD+QED simulations with C$^{\star}$ boundary conditions

论文作者

Altherr, Anian, Bushnaq, Lucius, Campos, Isabel, Catillo, Marco, Cotellucci, Alessandro, Dale, Madeleine, Fritzsch, Patrick, Gruber, Roman, Lücke, Jens, Marinkovic, Marina, Patella, Agostino, Tantalo, Nazario, Tavella, Paola

论文摘要

我们通过使用OpenQ $^\ star $ d代码为RC $^\ star $ Collaboration的持续努力进行更新,以生成完全动态的QCD+QED合奏。将模拟调整为pions $ m_ {π^{\ pm}} \大约400 $ meV的pions pions的U-对称点($ m_d = m_s $)。光中膜的分裂用作三个可观察的可观察物之一,并固定为$ m_ {k^{0}} - m_ {k^{\ pm}} \大约5 $ meV和$ m_ {k^{0}}} - m_ {k^{k^{k^{\ pm pm}} $α_ {\ text {r}} \大约α_ {\ text {phys}} $和$α_r\ of5.5α_{phys} $。将三个独立的夸克质量调整为所需的恒定物理线条特别具有挑战性。我们将定义所选的耐加率的重量化方案,并将基于质量重新加权和线性插值的组合提出调整策略,以探索参数空间。我们将评论有限体积效应,将两个不同卷上的介子质量与$ m_ {π^{\ pm}} l \ 3.2 $和$ m_ {π^{\ pm}} l \ l \ 5.1 $进行比较。我们还将提供有关我们更新策略的一些技术细节,以计算费米子Pfaffian的迹象,该符号在存在C $^\ star $边界条件的情况下代替标准费米子决定因素。有关配置产生的更多技术细节,请参见J.Lücke的诉讼程序

We give an update on the ongoing effort of the RC$^\star$ collaboration to generate fully dynamical QCD+QED ensembles with C$^\star$ boundary conditions using the openQ$^\star$D code. The simulations were tuned to the U-symmetric point ($m_d = m_s$) with pions at $m_{π^{\pm}} \approx 400$ MeV. The splitting of the light mesons is used as one of three tuning observables and fixed to $m_{K^{0}} - m_{K^{\pm}} \approx 5$ MeV and $m_{K^{0}} - m_{K^{\pm}} \approx 25$ MeV on ensembles with renormalized electromagnetic coupling $α_{\text{R}} \approx α_{\text{phys}}$ and $α_R \approx 5.5α_{phys}$ respectively. The tuning of the three independent quark masses to the desired lines of constant physics is particularly challenging. We will define the chosen hadronic renormalization scheme, and we will present a tuning strategy based on a combination of mass reweighting and linear interpolation to explore the parameter space. We will comment on finite-volume effects comparing meson masses on two different volumes with $m_{π^{\pm}} L \approx 3.2$ and $m_{π^{\pm}} L \approx 5.1$. We will also provide some technical details on our updated strategy to calculate the sign of the fermionic Pfaffian, which arises in presence of C$^\star$ boundary conditions in place of the standard fermionic determinant. More technical details on the generation of the configurations can be found in J. Lücke's proceedings

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