| 预测某些中子星的构成组份 |
| |
| 引用本文： | 李思农. 预测某些中子星的构成组份[J]. 科学技术与工程, 2010, 10(25) |
| |
| 作者姓名： | 李思农 |
| |
| 作者单位： | |
| |
| 摘 要： | 在理论上对中子星的构成组份以及中子星物质的不可压缩性进行不同的设定,通过计算得到一系列对应的中子星质量理论最大值。将这些计算值与观测值进行对比,可预测出某些中子星的构成组份。
|
| 关 键 词： | 中子星 组份 最大质量 |
| 收稿时间： | 2010-06-05 |
| 修稿时间： | 2010-06-11 |
Compositions of Some Neutron Stars |
| |
| Li Si Nong. Compositions of Some Neutron Stars[J]. Science Technology and Engineering, 2010, 10(25) |
| |
| Authors: | Li Si Nong |
| |
| Affiliation: | Department of Physics,Jinan University,Guangzhou 510632,P.R.China |
| |
| Abstract: | We got a series of maximum masses of neutron stars by presuming different compositions appearing in these neutron stars and different incompressibility of neutron star matter, respectively. And comparing these theoretical results to the observed value by astrophysicists we predict the composition of each specific neutron star. |
| |
| Keywords: | neutron stars composition maximum mass |
| 本文献已被 CNKI 万方数据 等数据库收录！ |
| 点击此处可从《科学技术与工程》浏览原始摘要信息 |
|
点击此处可从《科学技术与工程》下载全文 |
