Abstract：In General Ralativity it is indicated that gravitational collapse can draw some massive celestial bodies(stars) to form black holes if their mass(of these stars) is bigger than double mass of the Sun. If the quantum effect is considered in strong gravitational field, a black hole will radiate "particles" by the calculation from Quantum Fields in Curved Spacetime. There is a kind of model called Moving Mirror which can be used to descride some physical situations in the outside spacetime of the black hole's event horizon and could simplify their some physical processes and corresponding physical explanations. We submit a special model (a special trajectory being assigned) and use it to Schwarzschild black hole. Our calculation demonstrates that the particles spectrum of the Moving Mirror is the same as that of the black hole out of its event horizon.
收稿日期: 1994-02-25
引用本文:
万影 周并举. 黑洞与运动镜的辐射[J]. , 1994, 33(2): 0-0.
万影 周并举. RADIATION FROM BLACK HOLES AND FROM MOVING MIRRORS. , 1994, 33(2): 0-0.
