Tachyon Dynamics - for Neutrinos?

C. Schwartz
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引用次数: 17

Abstract

Following earlier studies that provided a consistent theory of kinematics for tachyons (faster-than-light particles) we here embark on a study of tachyon dynamics, both in classical physics and in the quantum theory. Examining a general scattering process we come to recognize that the labels given to "in" and "out" states are not Lorentz invariant for tachyons; and this lets us find a sensible interpretation of negative energy states. For statistical mechanics, as well as for scattering problems, we study what should be the proper expression for density of states for tachyons. We review the previous work on quantization of a Dirac field for tachyons and go on to expand earlier considerations of neutrinos as tachyons in the context of cosmology. We stumble into the realization that tachyon neutrinos would contribute to gravitation with the opposite sign compared to tachyon antineutrinos. This leads to the gobsmacking prediction that the Cosmic Neutrino Background, if they are indeed tachyons, might explain both phenomena of Dark Matter and Dark Energy. This theoretical study also makes contact with the anticipated results from the experiments KATRIN and PTOLEMY, which focus on beta decay and neutrino absorption by Tritium.
速子动力学-中微子?
根据早期的研究,提供了一个一致的理论,为速子(比光快的粒子)的运动学,我们在这里着手研究速子动力学,在经典物理学和量子理论。考察一般的散射过程,我们认识到给“入”和“出”态的标签对速子来说不是洛伦兹不变的;这让我们找到负能态的合理解释。对于统计力学和散射问题,我们研究速子态密度的适当表达式。我们回顾了之前关于狄拉克场对速子的量子化的工作,并继续扩展了在宇宙学背景下中微子作为速子的早期考虑。我们偶然意识到,与快子反中微子相比,快子中微子对引力的贡献是相反的。这导致了一个令人震惊的预测:宇宙中微子背景,如果它们确实是超光速粒子,可能会解释暗物质和暗能量的现象。本理论研究也与KATRIN和PTOLEMY实验的预期结果相联系,这两个实验的重点是氚的β衰变和中微子吸收。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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