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    EQUATIONS OF MOTION FOR RELATIVISTIC CORRECTIONS WITH THE RADIATIVE FORCE
    含辐射作用力的相对论改正运动方程
    SEVERAL PROBLEMS IN THE NUMERICAL INTEGRATION FOR THE EQUATIONS OF CELESTIAL MOTIONS
    关于数值求解天体运动方程的几个问题
    THE PERTURBATION SOLUTION TO THE EQUATIONS OF SATELLITE MOTION
    卫星运动方程的摄动解法
    Relativistic Celestial Mechanics and Post-Newtonian Equations of Motion
    相对论天体力学和后牛顿运动方程
    The Second-order Post-Newtonian Equations of Light Ray
    二阶后牛顿光线方程
    Statistical Entropy and Thermodynamics Equations of the Black Hole of Kerr-Newman
    Kerr-Newman黑洞的统计熵及黑洞热力学方程
    According to conservation equations of mass, momentum and energy, and equation of polytropic expanding process, we studied heating and cooling mechanism of gas and found the equation of the gas temperature of the envelopes.
    我们研究了拱星包层气体的加热机制和致冷原因,根据拱星包层气体的质量、动量和能量守恒方程及多方膨胀过程方程,通过计算得到了拱星包层气体温度所满足的温度方程
    The decoupling treatment overcomes such difficulties as small domain and slow speed of convergence encountered in numerically solving the differential equations of the problem, and naturally provides a guess solution which is needed in Henyey method.
    这样的一个退耦处理,有利于克服以前在数值解这类问题时常常遇到的收敛域小和收敛速度慢等困难,并且为数值解方程时所采用的Henyey方法提供了一个自然和方便的初始猜测解。
    The equations of motion of elliptic restricted problem of three bodies with variable mass according to n =1(k = 0, q =1/2) were derived more recently[5]. We have expanded the main sequence star to n = 2(k = 1, q = 3/2), n = 3(k = 2, q = 6/2) and n = 4(k = 3, q = 7/2) in this paper.
    较近期的关于可变质量的椭圆型限制性三体问题的运动方程[5]是对于n=1的情况,本文把星序数n扩充到2,3及4,对于每一种n,分别建立了可变质量的椭圆型限制性三体问题的运动方程
    In this paper, the iterative method is taken to establish and calculate the 2PN equations of light ray.
    在此建议采用迭代的方法来推导2PN光线方程.
    The 2PN equations of light ray in the solar-system have been deduced from the metric tensor and Christoffel symbols.
    从度规和Christoffel记号出发推导太阳系中的2PN光线方程.
    When the higher-order terms are neglected, the 2PN equations of light ray reduce to the 1PX equations which widely appeared in many textbooks.
    当忽略掉更高阶的项时,2PN光线方程将回到在很多教科书中广泛出现的1PN光线方程.
    Based on the nonlinear equations of the theory of density wave, the evolutionary direction and the observable conditions on spiral galaxies may be derived by the qualitative analysis theory.
    基于密度波理论的非线性方程,用定性分析理论可导出旋涡星系的演化方向和由观测可得到的演化条件.
    The energy level equations of scalar particles starting are derived out from Hamilton-Jacobin equation by using general Tortoise transformation.
    从Hamilton-Jacobin方程出发,通过广义Tortoise变换推导出该时空中标量粒子的能级方程;
    We also derive out the energy level equations of scalar particles starting from Hamilton-Jacobin equation by using general Tortoise transformation.
    从Hamilton- Jacobin方程出发,通过广义Tortoise变换推导出该时空中标量粒子的能级方程;
    THE PERTURBATION EQUATIONS OF THE ELEMENTS OF VINTI'S INTERMEDIATE
    Vinti型中间轨道根数的摄动方程
    ON FURTHER RESEARCH FOR EQUATIONS OF MOTION FOR ELLIPTIC RESTRICTED PROBLEM OF THREE BODIES WITH VARIABLE MASS
    关于可变质量的椭圆型限制性三体问题运动方程的再探讨
    Application of Maple Software in Gerneral Relativity ——First Post Newtonian Equations of Motion for Binary Systems
    Maple在广义相对论中的应用——双星系统1-PN近似运动方程
    ON THE PROBLEM IN SOLVING THE EQUATIONS OF THE MOTION OF AN ARTIFICIAL SATELLITE BY NUMERICAL METHODS
    关于数值求解卫星运动微分方程中的一个问题
    PROPERTIES OF NEUTRON STARS WITH NEW EQUATIONS OF STATE
    新状态方程下中子星的性质
 

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