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- W2106075428 abstract "Abstract We study tachyonic synchrotron densities of ultra-relativistic electrons in helical motion. There is a longitudinally polarized spectral component due to the negative mass square of the superluminal quanta. The helical pitch-angle scaling of the transversal and longitudinal spectral densities is investigated, in particular the transition from circular to rectilinear motion. The magnetic field induces oscillations along the power-law slopes of the superluminal radiation densities, whose amplitude depends on the pitch angle. At moderate field strength and ultra-relativistic orbital speed, the modulations are tiny, but they become quite pronounced in the surface fields of γ -ray pulsars, resulting in cockscomb distributions. A tachyonic spectral fit to the γ -ray flux of the binary pulsar PSR B1259–63 is performed. The γ -ray wideband of this millisecond pulsar is reproduced by a tachyonic cascade spectrum, capable of generating the spectral curvature in double-logarithmic plots as well as the extended spectral plateau defined by ISGRI, OSSE, COMPTEL, and EGRET flux points." @default.
- W2106075428 created "2016-06-24" @default.
- W2106075428 creator A5072780354 @default.
- W2106075428 date "2007-07-01" @default.
- W2106075428 modified "2023-09-25" @default.
- W2106075428 title "Tachyonic spectral map of a binary pulsar" @default.
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- W2106075428 doi "https://doi.org/10.1016/j.physleta.2007.01.084" @default.
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