1)Hawking temperatureHawking温度
1.Using the Tortoise coordinate transformation and the Dirac field equation near the event horizon,the Hawking temperature of Kinnersley black hole is obtained.采用Tortoise坐标变换,约化视界面附近Dirac场方程,得到Kinnersley黑洞的Hawking温度。
2.This paper presents that using the Tortoise coordinate transformation and the Klein-Gorden field equation near the event horizon,the Hawking temperature of black hole is obtained.采用Tortoise坐标变换,约化视界面附近Klein-Gorden方程,得到黑洞的Hawking温度。
3.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;并用薄膜模型计算了黑洞熵,得到了熵与视界面积成正比的Bekenstein关系。
2)hawking radiationHawking辐射
1.Damour-Ruffini method and nonthermal Hawking radiation from Reissner-Nordstrom black hole;Damour-Ruffini方法和Reissner-Nordstrom黑洞的非热Hawking辐射
2.Hawking radiation of massive scalor particles fromthe 5-dimensional rotating black hole;5维转动黑洞中有质量标量粒子的Hawking辐射
3.A new method for exploring the black hole Hawking radiation—— the quantum statistical method;探讨黑洞Hawking辐射的新方法——量子统计法
英文短句/例句
1.The Hawking Radiation of Black Holes and Casimir Effect of Massive Scalar Field;黑洞的Hawking辐射与有质量标量场的Casimir效应
2.Horizon and Hawking Radiation of the Uniformly Rectilinearly Accelercting Rindier Observer with Electric Charge;荷电匀加速度直线运动的Rindler观者的视界和Hawking辐射
3.A Study of Gravity and Thermodynamics of Horizons and Quantum Tunneling Method of Hawking Radiation and Related Research引力和视界热力学及Hawking辐射量子隧穿方法的相关研究
4.Hawking Radiation as Tunneling of General Static Spherically Symmetric Black Holes一般静态球对称黑洞的Hawking隧穿辐射
5.imb Radiance Infrared Radiometer (LRIR)临边辐射红外辐射仪
6.background radiation背景辐射，本底辐射
7.nuclear radiation, X-rays.核辐射和x光辐射。
8.spectral radiation exitance光谱辐（射）出（射）度
9.To send out rays or waves.放射，辐射发出射线或波
10.bolometric standard irradiance测辐射热标准辐照度
11.isotropic radiator各向同性辐射体;全方位辐射器;全向辐射器
12.absorbed dose of radiation吸收剂量（辐射的）
13.radial ply tyreph.1. 辐射层轮胎
14.sievert [radiation quantity]希沃特〔辐射剂量〕
15.density meter(of ionizing radiation)（电离辐射）密度计
16.satellite actinometry卫星辐射测量（学）
17.(nuclear)radiation transducer [sensor]（核）辐射式传感器
18.classical theory of radiation古典派辐射(学)说
相关短句/例句
hawking radiationHawking辐射
1.Damour-Ruffini method and nonthermal Hawking radiation from Reissner-Nordstrom black hole;Damour-Ruffini方法和Reissner-Nordstrom黑洞的非热Hawking辐射
2.Hawking radiation of massive scalor particles fromthe 5-dimensional rotating black hole;5维转动黑洞中有质量标量粒子的Hawking辐射
3.A new method for exploring the black hole Hawking radiation—— the quantum statistical method;探讨黑洞Hawking辐射的新方法——量子统计法
3)Bekenstein-Hawking entropyBekenstein-Hawking熵
1.The result shows that the tunneling rate of particle at the event horizon and the cosmic horizon is relevant to Bekenstein-Hawking entropy,and the radiation spectrum is not strictly pure thermal.结果表明在能量守恒的条件下,此黑洞事件视界和宇宙视界处粒子的隧穿率与Bekenstein-Hawking熵有关,真实的辐射谱不再是严格的纯热谱,这是对Hawking纯热谱的正确修正。
2.The result shows that the tunneling rate at the event horizon of the black hole is relevant to Bekenstein-Hawking entropy and the exact radiation spectrum is not pure thermal one when the self-gravitation and energy conservation are taken into consideration.当考虑粒子的自引力作用和能量守恒时,Gibbons-Maeda dilation黑洞视界处的粒子隧穿率与Bekenstein-Hawking熵有关,黑洞真实的辐射谱不再是严格的纯热谱。
3.The result shows that when energy conservation is taken into consideration,the tunneling rate of the radiation particle is related to the change of Bekenstein-Hawking entropy and the radiation spectrum is not pure thermal,but satisfies an underlying unitary theory.结果表明,在能量守恒的条件下,此黑洞事件视界处粒子的隧穿率与Bekenstein-Hawking熵变有关,真实的辐射谱不再是纯热谱,但满足量子力学中的么正性原理。
4)Hawking absorptionHawking吸收
1.After especially considering the Hawking absorption of the black hole, Planck absolute entropy of the charged black hole has been given out.基于严格求解 Dirac方程 ,全面研究了双视界面黑洞内、外视界附近的量子热效应 ,特别是考虑到黑洞内视界的 Hawking吸收后 ,成功的给出了荷电黑洞的普朗克绝对
2.After especially considering the Hawking absorption of the black hole,we give Planck absolute entropy of the charged black hole.基于严格求解Dirac方程 ,全面研究了双视界面黑洞内、外视界附近的量子热效应 ,特别是考虑到黑洞内视界的Hawking吸收后 ,成功的给出了荷电黑洞的普郎克绝对
5)Hawking effectHawking效应
1.The Hawking effect,event horizon and corresponding temperature of a uniformly accelerating,non stationary,charged black hole are given.给出了匀加速荷电黑洞的Hawking效应和事件视界及相应温度。
2.The Hawking effect in a general spherically symmetric non stationary space time can be considered as a compensate effect of the time scale transformation.一般球对称动态时空中的Hawking效应可看作时间尺度变换下的补偿效应 。
3.Like a stationary space-time, the Hawking effect can be regarded as a compensate effect of the scale transformation of coordinate time in the non-stationary VaidyaSchwarzschild-de sitter space-time- One of the pure-gauge potentials represents the Hawking temperature and the other the change rate of the temperature.同稳态时空一样，动态Vaidya-Schwarzschild－deSitter时空中的Hawking效应可看作时间尺度变换下的补偿效应，补偿场纯规范势的一个分量表征黑洞温度，另一个表征黑洞温度变化率。
6)Gibbons-Hawking effectGibbons-Hawking效应
延伸阅读
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