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用Newman-Penrose形式,研究了球对称动态时空中的引力、电磁、标量和Dirac场,表明量子能层会影响动态黑洞的辐射机制.与Kerr能层和电磁势产生的经典效应不同,这个效应的特征是辐射机制明显依赖于自旋态.By means of the Newman-Penrose formalism,the gravitational,electromagnetic, scalar and Dirac fields in spherically symmetric non-static space-times are discussed.It is shown that the quantum ergosphere can influence the radiative mechanism of a non-static black hole.The character of the effect is that the radiative mechanism is obviously dependent on the spin state,which differs from the classical effects due to the Kerr ergosphere and the electromagnetic potential.
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