Effect of Strong Quantizing Magnetic Field on the Transport Properties   of Dense Stellar Plasma
  The transport properties of dense stellar electron-proton plasma is studied following an exact relativistic formalism in presence of strong quantizing magnetic field. The variation of transport coefficients with magnetic field are found to be insensitive for the field strengths $\leq 10^{17}$G, beyond which all of them abruptly go to zero. As a consequence, the electron-proton plasma behaves like a superfluid insulator in presence of ultra-strong magnetic field. 
Soma Manda and Somenath Chakrabarty