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Schroedinger-Zitterbewegung Radiation

机译:薛定inger颤抖运动辐射

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Zitterbewegung is the quiver motion with frequency (such that its energy is slightly greater than 1 MeV) and Compton-wavelength amplitude discovered by Schroedinger in his 1930 solution of the time-dependent Dirac equation for a free electron. It is shown in this paper that it is possible to interpret Zitterbewegung as a radiative component of the time-dependent Dirac solution which is consistent with the long-known relationship between Dirac’s and Maxwell’s equations. Experimental evidence is cited for this interpretation in the form of extragalactic background gamma radiation which shows up as a bump near 1 MeV in the observed background spectrum. This background – called here Schroedinger-Zitterbewegung radiation – could exist due to the presence of copious free electrons in intergalactic space mostly in the form of ionized hydrogen.
机译:施特丁格(Schitteredwegung)是颤动运动,其频率(使能量略大于1 MeV)和施罗丁格在1930年的自由电子随时间的狄拉克方程的解中发现的康普顿波长幅度。本文表明,有可能将Zitterbewegung解释为与时间相关的Dirac解的辐射分量,这与Dirac方程和Maxwell方程之间的已知关系一致。这种解释的实验证据是银河外背景伽马辐射的形式,在观察到的背景光谱中显示为接近1 MeV的隆起。这种背景(这里称为Schroedinger-Zitterbewegung辐射)可能由于存在于星际空间中的大量自由电子(主要是电离氢的形式)而存在。

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