论文标题

分解质子:与黑暗力量的恋情

Breaking up the Proton: An Affair with Dark Forces

论文作者

Kribs, Graham D., McKeen, David, Raj, Nirmal

论文摘要

$ e^{\ pm} $ off质子的深度非弹性散射对“暗光子”交换的贡献很敏感。使用HERA数据拟合HERA的Parton分布功能,我们可以在Hypercharge和Dark Photon之间的动力学混合和深色光子质量$ \ Lessim 10 $ GEV之间的动力学混合中获得与模型无关的$ε\ Lessim 0.02 $。这略微改善了从Electroweak Precision可观察物获得的结合。对于较高的质量,极限单调削弱; $ε\ Lessim 1 $,黑色光子质量为$ 5 $ tev。利用PDF总和规则,我们证明了深色光子的效果不能(琐碎地)吸收到重新拟合的PDF中,实际上导致了非dglap(Bjorken $ x _ {\ rm b} $ - 独立的)尺度违规行为,可以在数据中提供吸烟枪。 The proposed $e^\pm p$ collider operating at $\sqrt{s} = 1.3$ TeV, LHeC, is anticipated to accumulate $10^3$ times the luminosity of HERA, providing substantial improvements in probing the effects of a dark photon: sensitivity to $ε$ well below that probed by electroweak precision data is possible throughout virtually the entire dark photon mass range, as well as being able to probe to much较高的深色光子块,最高$ 100 $ TEV。

Deep inelastic scattering of $e^{\pm}$ off protons is sensitive to contributions from "dark photon" exchange. Using HERA data fit to HERA's parton distribution functions, we obtain the model-independent bound $ε\lesssim 0.02$ on the kinetic mixing between hypercharge and the dark photon for dark photon masses $\lesssim 10$ GeV. This slightly improves on the bound obtained from electroweak precision observables. For higher masses the limit weakens monotonically; $ε\lesssim 1$ for a dark photon mass of $5$ TeV. Utilizing PDF sum rules, we demonstrate that the effects of the dark photon cannot be (trivially) absorbed into re-fit PDFs, and in fact lead to non-DGLAP (Bjorken $x_{\rm B}$-independent) scaling violations that could provide a smoking gun in data. The proposed $e^\pm p$ collider operating at $\sqrt{s} = 1.3$ TeV, LHeC, is anticipated to accumulate $10^3$ times the luminosity of HERA, providing substantial improvements in probing the effects of a dark photon: sensitivity to $ε$ well below that probed by electroweak precision data is possible throughout virtually the entire dark photon mass range, as well as being able to probe to much higher dark photon masses, up to $100$ TeV.

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