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Super Exponential Expansion for Dark Energy Model with Variable Λ in f (R, T) Gravity
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the plasma interactive state becomes more stable, otherwise some bit of oscillation is noticed. The stability is seen to depend on the magnetic (M2) and thermal convection (Gr) parameters. Under this condition the signal propagation becomes less diffuse when the frequency of the signal is far greater than the plasma frequency, that is, ω >> p. The study aids our understanding of the effect of coupling frequency on the propagation of satellite signals through the ionosphere.