Ingoing and outgoing energy fluxes, normalized by the luminosity of an isolated pulsar L0, for both configurations at two different separations.
|L⋆/L0 = 2.8||L⋆/L0 = 3.1|
|3 RLC||Lout/L0 = 2.1||Lout/L0 = 2.3|
|ϵ = 27%||ϵ = 25%|
|L⋆/L0 = 2.5||L⋆/L0 = 3.9|
|1.25 RLC||Lout/L0 = 1.5||Lout/L0 = 2.7|
|ϵ = 40%||ϵ = 30%|
Notes. The luminosities were computed in steady state.
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