PULSARS

作品数:382被引量:269H指数:7
导出分析报告
相关领域:天文地球更多>>
相关作者:王洪光杨信男更多>>
相关机构:中国科学院新疆天文台国家天文台北京大学广州大学更多>>
相关期刊:《Science China Mathematics》《Chinese Physics B》《Bulletin of the Chinese Academy of Sciences》《现代物理知识》更多>>
相关基金:国家自然科学基金国家重点基础研究发展计划国家高技术研究发展计划上海市自然科学基金更多>>
-

检索结果分析

结果分析中...
选择条件:
  • 期刊=Chinese Physics Cx
条 记 录,以下是1-6
视图:
排序:
Pulsars as candidates of LHAASO sources J2226+6057,J1908+0621,and J1825-1326:The leptonic origin
《Chinese Physics C》2023年第6期161-166,共6页常哲 况宇庭 张旭坤 周敬之 
Supported by the National Nature Science Foundation of China(12075249,11690022);the Key Research Program of the Chinese Academy of Sciences(XDPB15)。
Recently,from 12γ-ray Galactic sources,the LHAASO has detected ultrahigh-energy photons up to 1.4 PeV.Theγ-ray spectra of the sources J2226+6057,J1908+0621,and J1825-1326 and the suggested origin pulsars near the so...
关键词:GAMMA-RAYS cosmic rays acceleration of particles PULSARS 
Binding energy produced within the framework of the accretion of millisecond pulsars
《Chinese Physics C》2023年第4期11-15,共5页Ali Taani 
The role and implication of binding energy through the accretion-induced collapse(AIC)of accreting white dwarfs(WDs)for the production of millisecond pulsars(MSPs)are investigated.The binding energy model is examined ...
关键词:binding energy PULSARS EVOLUTION kinematics and dynamics 
Particles accelerated in Hertzian magnetic dipole field of a pulsar
《Chinese Physics C》2021年第11期136-142,共7页Zhe Chang Qing-Hua Zhu 
Supported by grants from NSFC(11675182,11690022)。
Supernova remnants are supposed to be the most possible sources of cosmic rays.However,alternative sources of cosmic rays,such as an active galactic nucleus,gamma-ray bursts,and pulsars,have not be excluded.In this st...
关键词:PULSARS cosmic rays acceleration of particles 
Spontaneous magnetization of solid quark-cluster stars
《Chinese Physics C》2016年第9期75-81,共7页来小禹 徐仁新 
Supported by 973 Program(2012CB821801);West Light Foundation(XBBS-2014-23);National Natural Science Foundation of China(11203018,11225314,11365022);Science Project of Universities in Xinjiang(XJEDU2012S02);Doctoral Science Foundation of Xinjiang University(BS120107)
Pulsar-like compact stars usually have strong magnetic fields, with strengths from -10^8 to -10^12 G on the surface. How such strong magnetic fields can be generated and maintained is still an unsolved problem,which i...
关键词:PULSARS strange stars magnetic fields 
A corresponding-state approach to quark-cluster matter
《Chinese Physics C》2014年第5期38-47,共10页郭彦君 来小禹 徐仁新 
Supported by National Basic Research Program of China(2012CB821800);National Natural Science Foundation of China(11225314,11203018);National Fund for Fostering Talents of Basic Science(NFFTBS)(J1030310/J1103205)
The state of super-dense matter is essential for us to understand the nature of pulsars; however, non- perturbative quantum chromodynamics makes it very difficult to make direct calculations of the state of cold matte...
关键词:PULSARS neutron stars elementary particles 
Quark-clustering in cold quark matter
《Chinese Physics C》2010年第9期1331-1334,共4页来小禹 徐仁新 
Supported by NSFC (10778611,10973002);National Basic Research Program of China (2009CB824800) and LCWR (LHXZ200602)
Quarks are proposed to be grouped together to make quark-clusters due to the strong interaction in cold quark matter at a few nuclear densities,because a weakly coupling treatment of the interaction between quarks the...
关键词:quark matter neutron stars PULSARS nuclear matter quantum chromodynamics 
检索报告 对象比较 聚类工具 使用帮助 返回顶部