1.The thesis studies the solution of Dirac equation in the non-static and spherically symmetric black hole, it change into the form of tortoise coordinate by employing the tortoise coordinate transformation. Then this changes into standard wavw equation near the event horizons and gwts Hawking radiation temperature of Dirac particles near the event horizons, which successfully obtains Hawking thermal spectrum formula.
在动态球对称黑洞时空中求解狄拉克方程,采用了Tortoise坐标变换将狄拉克方程变成Tortoise坐标下的形式,在视界面附近化成了标准的波动方程,得到在视界面附近狄拉克粒子的Hawking辐射温度,成功地导出了Hawking热谱公式.
2.Under a new Tortoise coordinate transformation, by reducing and solving the Klein-Gordon equation near the event horizon, the Hawking radiation is studied.
采用一种新的Tortoise坐标变换 ,通过约化和求解视界附近的Klein Gordon方程 ,得到了黑洞的Hawking热谱和Hawking温度 .
3.By means of the Dirac equation and the generalized Tortoise coordinate variation, the event horizon equation and Hawking temperature of the black hole are obtained directly, and finally the Hawking radiation formula of the Dirac particles is educed.
从Dirac四分量方程出发 ,经广义Tortoise坐标变换 ,直接导出黑洞的事件视界面方程及温度函数 ,并最终获得了Dirac粒子的热谱公式 .
4.With the null tetrad,the Dirac equation is reduced and solved near the event horizon in the static space-time with an internal global monopole when the tortoise coordinate is adopted. The Hawking temperature and the formula of thermal spectrum of the Dirace particles are derived.
利用零标架,采用Tortoise 坐标,在具有整体单极时空中,将Dirac 方程在事件视界附近化为波动方程,并得到了出射波和入射波,导出了Hawking 温度和Dirac 粒子的热谱公式.
5.Asymptotically solutions of the Klein-Gorden equation in region near event horizon of a uniformaly accelerating charged black hole are obtained by using generalized tortoise coordinate. The location of the event horizon and the Hawking temperature of the hole are given. In the appropriate limits, the results reduce to that of the Reissuer-Nordstrom, Schwarzschild and F-Z accelerating black hole.
利用推广的Tortoise坐标，得到了在加速荷电黑洞视界邻域内Klein－Gorden方程的渐近解．求出了事件视界的位置和Hawking温度．结果表明：由于黑洞的加速作用，事件的形状不再是球对称的．在一定的条件下，所得结果退为Reissner－Nordstrm黑洞，Schwarzschile黑洞和F－Z加速黑洞结果．
6.By means of the dirac equation and the generalized tortoise coordinate variation we directly ob- tained the location of event horizon of black hole with electric-magnetic charge.
从Dirac四分量旋量方程出发，经广义Tortoise坐标变换，直接导出含有双荷子球对称黑洞的视界面位置。
7.Under a new tortoise coordinate transformation,Hawking temperature of the Vaidya black hole is calculated by reducing the Klein-Gordon equation near the event horizon.
采用一种新的Tortoise坐标变换,约化视界附近Klein-Gordon方程,得到了黑洞的Hawking温度;
8.Research on the Event Horizon Surface Gravity of Kerr-Newman-de Sitter Black Hole by Using a New Tortoise Coordinate Transformation
在一种新的Tortoise坐标变换下研究Kerr-Newman-de Sitter黑洞的视界表面引力
9.The location of event horizon and surface gravity near event horizon of Kerr black hole are given directly by Dirac equation htrough generalized Tortoise translation.
从 Dirac方程出发 ,经广义 Tortoise坐标变换后 ,在视界曲面附近求解 ,直接导出Kerr黑洞的视界位置及视界表面重力 ,证明了 Kerr黑洞的视界是球对称的
10.4Never ever attempt to hibernate a tortoise which you suspect is ill. To put a sick or underweight tortoise into hibernation is to condemn it to certain death.
不要忘了，通常越小的龟龟越容易在冬眠中夭亡。非常小的龟龟需要短期的，非常小心控制下的冬眠。
