Radiative Acceleration of Matter and Pressure

Radiative acceleration of matter and pressure is a crucial phenomenon in astrophysics, governing the dynamics of various celestial bodies and environments. It describes the force exerted on matter by radiation, including electromagnetic radiation such as light and other forms of energy emitted by stars and other cosmic sources. This acceleration plays a significant role in shaping the structure and evolution of stars, galaxies, and interstellar mediums, influencing processes like stellar formation, stellar winds, and the dynamics of accretion disks around black holes and other massive objects. Understanding radiative acceleration is essential for comprehending the fundamental mechanisms driving cosmic phenomena.

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