名师点评

近日,家中装修,购置了一台价值上千元的大彩灯。这盏灯可谓是华丽至极:整灯呈圆锥形,直径有一米左右,周围用变换光的材料磨成棱锥,将上百个棱锥围在圆锥周围,就如那魔幻飞碟般奇丽。     

热中子星r-mode 不稳定性的研究

理论上,不稳定的中子星r-mode 能辐射可探测的引力波。采用具有超软对称能的非对称核物质物态方程,并考虑非牛顿引力效应影响,数值计算了由于CFS(Chandrasekhar-Friedmann-Schutz) 不稳定性引起的年轻热中子星的r-mode 不稳定窗口,给出了引力辐射时标和耗散时标随温度的变化关系。利用中子星观测对非牛顿引力参数的约束,给出了热中子星在高温区不稳定窗口边界的约束,并发现较大的非牛顿引力参数对应着较宽的r-mode 不稳定窗口。研究结果可为地面引力辐射探测提供有意义的参考。Theoritically, instable r-mode in neutron star may radiate detectable gravitational waves. In this work,considering the non-Newtonian gravity proposed in the grand unification theories, we numerically calculate the CFS instabilities of r-mode s in the hot neutron stars by using an equation of state with super-soft symmetry energies. The changes of the gravitational radiation time scales and the viscous time scales versus the stellar temperatures are obtained.And according to the constraint of the neutron star observation on the parameter of non-Newtonian gravity, the constraint on the boundary of the instability window is also given. It is found that a stronger non-Newtonian gravity corresponds with a wider r-mode instability window. These results may provide interesting reference for the gravitational wave detection.     

Gravitational waves from the axial perturbations of hyperon stars

The eigen-frequencies of the axial w-mode oscillations of hyperon stars are examined.It is shown that as the appearance of hyperons softens the equation of state of the super-density matter,the frequency of gravitational waves from the axial w-mode of hyperon star becomes smaller than that of a traditional neutron star at the same stellar mass.Moreover,the eigenfrequencies of hyperon stars also have scaling universality.It is shown that the EURO thirdgeneration gravitational-wave detector has the potential to detect the gravitational-wave signal emitted from the axial w-mode oscillations of a hyperon star.     

牢骚

“我真不明白,难道是命中注定,让我们一生都得呆在这儿受罪吗?”又是它们,又是那山上的大石块们在发牢骚了。终于有一天,靠山的小镇上的人们从山上把这些大石块搬运下山,石块们不知道发生了什么事,反正不呆在山上     

R-mode Instability of Neutron Star with Non-Newtonian Gravity

The Chandrasekhar-Friedmann-Schutz(CFS) instabilities of r-modes for canonical neutron stars(1.4 M ⊙) with rigid crusts are investigated by using an equation of state of asymmetric nuclear matter with super-soft symmetry energy,where the non-Newtonian gravity proposed in the grand unification theories is also considered.Constrained by the observations of the masses and the spin frequencies for neutron stars,the boundary of the r-mode instability window for a canonical neutron star is obtained,and the results show that the observed neutron stars are all outside the instability window,which is consistent with the theoretical expectation.In addition,an upper limit of the non-Newtonian gravity parameters is also given.     

中华鳖病原菌菌种的分离鉴定及多重PCR的初步建立

对患病中华鳖心脏、肝脏、肠道中分离得到的疑似致病菌株进行常规生理生化鉴定,同时采用分子生物学鉴定方法,设计细菌16srDNA保守区通用引物,进行基因扩增及序列比对,建立并优化多重PCR反应条件.分离鉴定出4种病原菌:迟钝爱德华氏菌(Edwardsiella tarda,Et)、嗜水气单胞菌(Aeromonas hydrophila,Ah)、维氏气单胞菌(Aeromonas veronii,Av)、弗氏柠檬酸杆菌(Citrobacter freundii,Cf).多重PCR检测体系敏感性与特异性良好,证明多重PCR是一种能快速准确鉴定多种中华鳖致病菌的方法,且操作简单、灵敏度高、稳定性和重复性好.     

承诺

五月的阳光暖意融融,温柔地向人们微笑,让人心中也如五月阳光般暖意融融,我迈着轻快的步子,向着楼前一家新开的“令你满意”商店走去……     

考虑非牛顿引力下的快速转动混合星性质

计算和讨论了考虑非牛顿引力下的快速转动混合星结构与性质,包括质量-半径关系、Kepler转速、转动惯量、引力红移以及转动动能和引力结合能之比等.结果表明,转动将有效地增大混合星能支持的最大质量,Kepler转速下能支持的最大质量比静态时增加20%左右;转动对于考虑非牛顿引力的混合星整体结构性质(包括质量-半径关系、转动惯量、转动动能和引力结合能之比等)具有明显的影响,但对极向引力红移影响相对较小.