| Dynamical Behavior of Core ~3 He Nuclear Reaction-Diffusion Systems and Sun′s Gravitational Field |
| |
| 引用本文： | 杜九林,申洪.Dynamical Behavior of Core ~3 He Nuclear Reaction-Diffusion Systems and Sun′s Gravitational Field[J].天津大学学报(英文版),2005(1). |
| |
| 作者姓名： | 杜九林 申洪 |
| |
| 作者单位： | School of Sciences，Tianjin University，Tianjin 300072，China，Department of Physics，Gannan Teachers College，Ganzhou 330047，China |
| |
| 基金项目： | Supportedbytheprojectof“985”ProgramofTianjinUniversity. |
| |
| 摘 要： | IthasbeenlongunderstoodthatthegravityplaysavitalroleinsuchinstabilityofhydrodynamicsastheBenardconvection. Itisworthnoticing, forareac tion diffusionsystem, thegravityfieldcouldbringaboutinhomogeneityinspace, leadingtothebreakofspacesymmetryandthenintroducingthepreferenceforstates1]. Intheinteriorofastar, thecorenuclearreactionsareaffectedalwaysbythegravitationalfield,thepressure, thediffusionofparticlesandthemotionoffluid, amongwhichthegravitationalfieldwasbe lievedtobeareasonfordrivingt…
|
| 本文献已被 CNKI 等数据库收录！ |
|
