1) holhraum
黑洞靶
2) black hole
黑洞
1.
Routing algorithm defense against black hole attacks in MANET based on mobile agent;
MANET环境中抵御“黑洞”攻击的路由算法
2.
The energy of scalar particles in a generalized spherical symmetric evaporating charged black hole;
广义球对称带电蒸发黑洞周围时空中标量粒子的能量
3.
Entropy of the scalar field in general accelerating non-stationary black holes with electric charge and magnetic charge;
一般加速带电带磁的动态黑洞中标量场的熵
3) black holes
黑洞
1.
In this method,the adjustable matching threshold is used to greatly reduce the number of black holes,improving fuzzy matching for control parameters with the prescribed fuzzy similarity.
该算法匹配阈值可变,采用调整匹配阈值的方法大幅降低黑洞数量;在满足一定模糊相似度的前提下,实现了带控制参数的模糊匹配,模糊程度可控。
2.
Global solutions of advection dominated accretion- flows (ADAFs) around black holes are presented.
对黑洞径移主导吸积流(ADAF)的整体解作了研究。
3.
The damage to the constant speed of Hawking s radiation done by motion layer around black holes is expounded and it is the important reason for the latter to remain undetectable.
本文论述了黑洞周围运动层对霍金辐射恒定速度的破坏,是后者至今仍无法探测到的重要原因。
4) blackhole
黑洞
1.
A entire study of the spacetime metric and entropy of the system containing a blackhole;
中心黑洞体系球对称度规及熵的整体研究
2.
The entropy of ideal gas which collapses to a blackhole by self-gravitating is studied.
讨论了理想气体自引力坍缩时的熵,得出与黑洞的熵相近的结论,从而说明了黑洞熵的起源。
3.
These security problems were blackhole, denial of service (DoS), routing table overflow, impersonation, power consumption and information disclosure.
针对MANET路由安全的重要性及其脆弱性,从不同角度对MANET的路由层或其它相应层面造成的安全攻击,分类综合出目前网络面临的六大类型的路由安全威胁,即黑洞问题、拒绝服务(DoS)、路由表溢出、伪装欺骗、能源耗竭及信息泄漏。
5) IT black hole
IT黑洞
1.
The appearing of " IT black hole " with the development of the information, makes IT management become one of the hot issues of enterprises instantly , and the key link of the IT manage is whether IT goal of the company conforms with its strategic objective.
伴随信息化的发展而出现的“IT黑洞”,使得IT治理成为当下企业的热门话题之一,而IT治理的核心环节是公司的IT目标是否与战略目标相一致。
2.
The paper briefly analyzed the question of “IT black hole” and reasons that they appeared in the course of Constructing ERP,and put forward a way to solve these questions.
简析了ERP建设中的“IT黑洞”问题及其产生原因,提出了六西格玛法(以下简称6σ法)与ERP集成的解决思路。
6) hohlraum target
黑腔靶
1.
The experimental diagnostics of hot electrons from hohlraum targets irradiated by 1ω_0 light at “Shenguang Ⅱ”;
“神光Ⅱ”基频光黑腔靶实验超热电子诊断
补充资料:黑洞
黑洞 black hole 广义相对论所预言的一种天体。一个质量比太阳大8倍以上的恒星,一般经过超新星爆发留下超过二、三个太阳质量的核,将没有任何力能阻止它继续坍缩。当它的半径小于引力半径rg=2GM/c2(G为万有引力常数,c为光速,M为天体的质量)时,没有任何物质或辐射能够逃逸出来,成为黑洞。黑洞的性质由三个参量来表征,即质量M、角动量J和电荷Q。当J=Q=0时,它是球对称的史瓦西黑洞;当Q=0时,则为轴对称的克尔黑洞。黑洞的性质决定了探测黑洞的困难性。如果向黑洞下落的气体具有较大的角动量,则应绕着黑洞在轨道上旋转,形成一个气盘。气盘中相邻层之间因气体的粘滞性引起的摩擦产生了热能,理论计算表明,气盘应具有很高温度,在X射线波段产生辐射。另一方面,黑洞的质量应大于中子星的质量上限,能够精确确定质量的是双星系统。因此,最有希望找到黑洞的是大质量X射线双星,尤其是天鹅座X-1。这是一个X射线变源,它有一个光学对应体,从这个9等超巨星的光谱得到视向速度的周期性变化,暗示一个不可见伴星的存在。进一步算出它的质量大于4太阳质量,很可能是8太阳质量,大于中子星的上限2~3太阳质量;另一个有希望的黑洞候选者是大麦哲伦云X-3,它也是一个X射线双星,其中不可见天体的质量也是8太阳质量。 |
说明:补充资料仅用于学习参考,请勿用于其它任何用途。
参考词条