Analyses demonstrate pulsar emission patterns based on time-density gradients, indicating a novel mechanism.
This paper demonstrates that the extreme collimation of electromagnetic radiation in pulsars is a direct consequence of the relativistic time-density gradient (∆ft) between the rotational poles and the equator. By analyzing the Crab Pulsar (PSR B0531+21), we show that energy emission follows the path of maximum temporal density.
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Christian Krebs (2026) studied this question.
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