Unraveling Energy Flow in Starbursts Through the Poynting Vector
The Poynting vector, defined as the directional energy flux of electromagnetic fields, serves as a foundational concept in understanding how energy propagates through astrophysical plasmas—especially in extreme environments like starburst galaxies. In these regions, where intense stellar formation triggers violent outflows and powerful radiation, electromagnetic energy transport becomes pivotal. The vector captures not only the
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