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Ultra-high energy physics and standard basic principles - Do Planck units really make sense?

机译:超高能物理和标准基本原理-普朗克单元真的有意义吗?

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It has not yet been elucidated whether the observed flux suppression for ultra-high energy cosmic rays (UHECR) at energies above ? 4 x 1019 eV is a signature of the Greisen-Zatsepin-Kuzmin (GZK) cutoff or a consequence of other phenomena. In both cases, violations of the standard fundamental principles of Physics can be present and play a significant role. They can in particular modify cosmic-ray interactions, propagation or acceleration at very high energy. Thus, in a long-term program, UHECR data can hopefully be used to test relativity, quantum mechanics, energy and momentum conservation, vacuum properties... as well as the elementariness of standard particles. Data on cosmic rays at energies ? 1020 eV may also be sensitive to new physics generated well beyond Planck scale. A typical example is provided by the search for possible signatures of a Lorentz symmetry violation (LSV) associated to a privileged local reference frame (the "vacuum rest frame", VRF). If a VRF exists, the internal structure of standard particles at ultra-high energy can undergo substantial modifications. Similarly, the conventional particle symmetries may cease to be valid at such energies instead of heading to a grand unification and the structure of vacuum may no longer be governed by standard quantum field theory. Then, the question whether the notion of Planck scale still makes sense clearly becomes relevant and the very grounds of Cosmology can undergo essential modifications. UHECR studies naturally interact with the interpretation of WMAP and Planck observations. Recent Planck data analyses tend to confirm the possible existence of a privileged space direction. If the observed phenomenon turns out to be a signature of the spinorial space-time (SST) we suggested in 1996-97, then conventional Particle Physics may correspond to the local properties of standard matter at low enough energy and large enough distances. This would clearly strengthen the cosmological relevance of UHECR phenomenology and weaken the status of the Planck scale hypothesis. Another crucial observation is that, already before incorporating standard matter and relativity, the SST geometry naturally yields a H t = 1 law where t is the age of the Universe and H the ratio between relative speeds and distances at cosmic scale. As standard cosmology is not required to get such a fundamental result, the need for a conventional Planck scale is far from obvious and the study of UHECR can potentially yield evidence for an alternative approach including new physics and new ultimate constituents of matter. UHECR may in particular allow to explore the possible indications of the existence of a transition scale at very high energy where the standard laws would start becoming less and less dominant and new physics would replace the conventional fundamental principles. We discuss prospects of searches for potential signatures of such a phenomenon.
机译:尚未阐明在能量高于时对超高能宇宙射线(UHECR)观察到的通量抑制作用吗? 4 x 1019 eV是Greisen-Zatsepin-Kuzmin(GZK)截止值或其他现象的结果。在这两种情况下,都可能出现违反物理标准基本原理的现象,并起着重要作用。它们尤其可以在非常高的能量下修改宇宙射线的相互作用,传播或加速。因此,在长期计划中,UHECR数据有望用于测试相对论,量子力学,能量和动量守恒,真空性质...以及标准粒子的元素。关于宇宙射线能量的数据? 1020 eV也可能对远远超出普朗克规模的新物理学敏感。通过搜索与特权本地参考帧(“真空休止帧”,VRF)关联的洛伦兹对称违例(LSV)的可能特征来提供典型示例。如果存在VRF,则超高能的标准颗粒的内部结构可能会发生重大变化。类似地,常规的粒子对称性可能在这种能量下不再有效,而不是完全统一,并且真空结构可能不再受标准量子场论控制。然后,普朗克量表的概念是否仍然有意义的问题就变得很相关,宇宙学的基础可以进行本质的修改。 UHECR研究自然与WMAP和Planck观测结果的解释相互作用。最近的普朗克数据分析倾向于确认特权空间方向的可能存在。如果观察到的现象证明是我们在1996-97年提出的脊柱时空(SST)的特征,那么常规的粒子物理学可能在能量足够低且距离足够大的情况下对应于标准物质的局部性质。这显然会加强UHECR现象学的宇宙学相关性,并削弱普朗克量表假设的地位。另一个至关重要的观察结果是,在纳入标准物质和相对论之前,SST几何学自然就产生了H t = 1律,其中t是宇宙的年龄,H是宇宙尺度上相对速度和距离之比。由于不需要标准宇宙学来获得这样的基本结果,对常规普朗克标度的需求就不那么明显了,对UHECR的研究可以为包括新物理和新的物质终极成分的替代方法提供证据。特别是,UHECR可能允许探索在非常高的能量下存在过渡尺度的可能迹象,在该尺度上,标准定律将开始越来越占主导地位,而新的物理学将取代常规的基本原理。我们讨论了寻找这种现象的潜在特征的前景。

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