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arXiv 1007.2269hep-ph
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洛伦兹破坏对甚高能光子天体物理传播的影响

Lorentz violation effects on astrophysical propagation of very high energy photons

Lijing Shao, Bo-Qiang Ma

摘要:

对正则能量-动量色散关系$E^2=p^2+m^2$进行了修正,得到了一些量子引力(QG)候选模型的洛伦兹破坏(LV)预言.因此,新的现象超出了标准模型的预测。特别是,LV的存在高度影响来自遥远星系的具有非常高能量的天体物理光子的传播。在本文中,我们回顾了更新的理论和实验结果,这一主题。我们将效应分为三类:(i)不同能量的光子之间的时间滞后;(ii)光子衰减阈值能量以上的光子通量截止,$γ\rightarrow e^++e^-$ ;(iii)由于背景光的吸收,多TeV光子和EeV光子光谱中的新模式。正如我们所看到的,LV对天体物理光子的影响的细节在很大程度上取决于LV参数的“相空间”。从观测的角度来看,现有的和即将出现的仪器有望研究这些现象,并对LV问题和QG理论有所启发。最后对超高能宇宙射线(UHECR)的最新进展和制约因素进行了全面的讨论。

英文摘要:

Lorentz violation (LV) is predicted by some quantum gravity (QG) candidates, wherein the canonical energy-momentum dispersion relation, $E^2=p^2+m^2$, is modified. Consequently, new phenomenons beyond the standard model are predicted. Especially, the presence of LV highly affects the propagation of astrophysical photons with very high energies from distant galaxies. In this paper, we review the updating theoretical and experimental results on this topic. We classify the effects into three categories: (i) time lags between photons with different energies; (ii) a cutoff of photon flux above the threshold energy of photon decay, $γ\rightarrow e^++e^-$; (iii) new patterns in the spectra of multi-TeV photons and EeV photons, due to the absorption of background lights. As we can see, the details of LV effects on astrophysical photons depend heavily on the "phase space" of LV parameters. From observational aspects, nowadays available and upcoming instruments can study these phenomenons hopefully, and shed light onto LV issues and QG theories. The most recent progresses and constraints on the ultra-high energy cosmic rays (UHECRs) are also fully discussed.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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