On Modified Yukava Screening in Dense Hydrogen Plasma

The plasma of low and moderate non-ideality is of interest in solar and stellar plasma.The previous research of modeling a collective plasma influence onto the emitter in plasma was conducted with the modeling of electron screening influence by the usage of Debye screening mechanism.Although this was a known erroneous presumption a preliminary results has shown a expected behavior in respect to particles in plasma densities as well as temperatures that was present in modeled plasma.The more thorough research has shown that the modified Yukava type screening is more applicable.Here are presented preliminary results of plasma influence onto the emitter potential in pure hydrogen plasma.This is the further step in development of more detailed analysis of collective phenomena in area of moderate to dense plasma influence.