Terry Kammash - NASA's Institute for Advanced Concepts
Terry Kammash - NASA's Institute for Advanced Concepts
Terry Kammash - NASA's Institute for Advanced Concepts
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Physics ContinuedEnergy conservation <strong>for</strong> electrons in cloudPE=KEPE≈πe 2 n b h 2KE=( γ b -1)m o c 2where γ b =Relativistic ParameterHence:h=√(γ b -1)m o c 2 /πe 2 n b = =√(γ b -1)/πr e n bWhere: r e =classical electron radiusr e =e 2 /m o c 2 =2.8×10 -13Substituting into exp. <strong>for</strong> E z we getE z =2c√πm o (γ b -1)n b