Random quadralinear forms and schur product on tensors

In this work, we made progress on the problem that [ symbol: see text] is a Banach algebra under schur product. Our results extend Tonge's results. We also obtained estimates for the norm of the random quadralinear form A:l(r)(M) x l(p)(N) x l(q)(K) x l(s)(H)-->C, defined by: A(e(i), e(j), e(k), e(s))=a(ijks), where the (a(ijks))'s are uniformly bounded, independent, mean zero random variables. We proved that under some conditions [ symbol: see text] is not a Banach algebra under schur product.     

A periodicity of approximately 1 hour in X-ray emission from the active galaxy RE J1034+396

Active galactic nuclei and quasars are thought to be scaled-up versions of Galactic black hole binaries, powered by accretion onto supermassive black holes with masses of 10(6)-10(9) M[symbol: see text], as opposed to the approximately 10 M [symbol: see text] in binaries (here M [symbol: see text] is the solar mass). One example of the similarities between these two types of systems is the characteristic rapid X-ray variability seen from the accretion flow. The power spectrum of this variability in black hole binaries consists of a broad noise with multiple quasi-periodic oscillations superimposed on it. Although the broad noise component has been observed in many active galactic nuclei, there have hitherto been no significant detections of quasi-periodic oscillations. Here we report the discovery of an approximately 1-hour X-ray periodicity in a bright active galaxy, RE J1034+396. The signal is highly statistically significant (at the 5.6 sigma level) and very coherent, with quality factor Q > 16. The X-ray modulation arises from the direct vicinity of the black hole.     

RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system

RR Lyrae pulsating stars have been extensively used as tracers of old stellar populations for the purpose of determining the ages of galaxies, and as tools to measure distances to nearby galaxies. There was accordingly considerable interest when the RR Lyrae star OGLE-BLG-RRLYR-02792 (referred to here as RRLYR-02792) was found to be a member of an eclipsing binary system, because the mass of the pulsator (hitherto constrained only by models) could be unambiguously determined. Here we report that RRLYR-02792 has a mass of 0.26 solar masses M[symbol see text] and therefore cannot be a classical RR Lyrae star. Using models, we find that its properties are best explained by the evolution of a close binary system that started with M[symbol see text] and 0.8M[symbol see text]stars orbiting each other with an initial period of 2.9 days. Mass exchange over 5.4 billion years produced the observed system, which is now in a very short-lived phase where the physical properties of the pulsator happen to place it in the same instability strip of the Hertzsprung-Russell diagram as that occupied by RR Lyrae stars. We estimate that only 0.2 per cent of RR Lyrae stars may be contaminated by systems similar to this one, which implies that distances measured with RR Lyrae stars should not be significantly affected by these binary interlopers.     

A result on character degrees and conjugacy class sizes in finite groups

Let G be a finite group and π be a set of primes including at least two elements. We write cd(G) and cs(G) to denote the set of complex irreducible character degrees and conjugacy class sizes of G , respectively, and write π(m)to denote the set of all prime divisors of a positive integer m . For any 1≠m∈cd(G) and 1≠m∈cs(G), in this note, we shall present the corresponding group structures of finite group G in the case π(m)=π , respectively, which generalizes the result of finite groups with character degrees of two distinct primes. Furthermore, we shall see that the influence of the two sets on the group structure is analogous.     

半群TE(X)中的一个同余

设ＦＸ表示集合上的全变换半群,Ｃｏｎ（Ｓ）表示半群Ｓ上的同余格,对Ｘ上任一非平凡等价关系Ｅ,令ＴＥ（Ｘ）＝（ｆ∈ＦＸ：Ａ↓（ａ,ｂ）∈Ｅ,（ｆ（ａ）,ｆ（ｂ））∈Ｅ）,据「４」,ＴＥ（Ｘ）构成一个α半群,且Ｃｏｎ（ＴＥ（Ｘ））可以 三个互不相交的完全子格,其中的一个为「Ｃ（Ｅ）〈Ｃａ（Ｅ）」,本文 ＴＥ（Ｘ）的同余τ,并证明了当Ｅ为单等价关系时,τ是「Ｃ（Ｅ）,Ｃａ（Ｅ）」中的唯一原子。     

一种有机八氰合钼(Ⅳ)酸盐的合成及晶体结构分析

[M(CN)8]n-(M=Mo,W,Nb;n=3,4)是一类重要的磁性材料构筑单元.化合物(C6H6N3)4[Mo(CN)8].H2O的晶体结构属于三斜晶系的P1-空间群,其不对称单元由1个[Mo(CN)8]4-,4个质子化的苯并三唑有机阳离子C6H6N3+和1个结晶水组成.[Mo(CN)8]4-离子中,Mo中心处于扭曲的反四棱柱配位环境.8个未配位的氰基氮原子作为氢键的受体,有机阳离子上质子化的氮原子和结晶水作为氢键的给体,形成了丰富的氢键作用,这些氢键作用连同部分有机阳离子间的π-π堆积、阴阳离子间的静电力和Van Der Waals力构筑成三维超分子网络.     

超拓扑群

给拓扑群上的超群规定了一种拓扑，使之成为拓扑群。     

关于李世荣的一个定理

本文使用文献[1]的结果,证明了下列定理:定理设G为有限群。假若G的非正规极大子群同阶类类数=2,则(1)若G可解,则|π(r_∞(G))|≤2。(2)若G不可解,则其中Z_2~3为G′φ(G)的极小正规子群,K可解,i=0,1,2,……     

有限群的弱n-Engle条件和p-幂零性

有限群G的一个弱 n-Engle 条件是指：对于G的2个元素x，y和某个非负整数n，[x，ny]∈Z(G)成立，如果存在G的一个子群K满足HK=G和H∩K≤CoreG(H)，则G的一个子群H称为c-可补的，利用极小子群的弱 n-Engle 条件和4阶循环子群的c-可补性，讨论了G的p-幂零性。     

诱导整群环上内自同构的有限群的自同构

设G是有限群,Z是整数环,ZG是G在Z上的整群环,G的所有诱导了ZG上的内自同构的自同构构成了一个群,记为AutZ（G）。令outZ（G）=AutZ（G）/Inn（G）,其中Inn（G）是G的内自同构群。我们证明了如果G有直积分解,那么AutZ（G）和OutZ（G）也有直积分解。作为该结果的一个直接推论,我们得到了G有正规化子性质当且仅当它的直因子有正规化子性质,从而推广了文献[1]中的相应结果。     

Szász算子的收敛速度的估计

本文对[1]及[2]中所给的概率型算子Szász算子S_n(f,x)的收敛速度的估计在Poisson分布下作进一步的改进,得到更精确的系数估计。     

实UFD上的几类格序矩阵代数

设Z是整数环,如果(Mn(Z),+,×,≥)(n≥3)是一个格序环,则它也可以作为Z模有一个含有n2个元的vl-基B.如果B中恰有n2-n-1个幂零元时,本文确定了Mn(Z)上的格序代数的同构类型(见定理3.4),而且我们将该结果推广到实数中一般的唯一因子分解环R上(见定理3.5).另外,如果在Mn(R)上的一个格序代...     

非交换子群共轭类的一个注记

设G是有限群.用τ(G)表示G中非交换子群的共轭类数,π(G)表示G的素因子的集合.对于每个非交换群有τ(G)≥2|π(G)|-2或|π(G)|+1.分析上述不等式中等号成立的有限群的分类.     

广义逆A_(T,S)~(2)的表示与计算

比较系统的总结了AT,S(2)的各种表示,与此同时,给出AT,S(2)的三个新的表达式,AT,S(2)=[E1GA E2]-1[E10]G或AT,S(2)=G(F1 0)-1(AGF1 F2)以及AT,S(2)=-1/β0((GA)s-1+βs-1(GA)s-2+…+β2(GA)+β1In)G=-1/β0G((AG)s-1+βs-1(AG)s-2+…+β2(AG)+β1In)利用前两种表达式,我们给出AT,S(2)逆的Gauss-Jordan消去法的求法.     

链直积上的明聚点

本文得到了完全分配格是[1]中定义的分子格的一个充要条件,并在没有补映射的情况下,借助余拓扑将[4]中提出的明聚点、明导集概念及其一系列重要性质推广到链直积。     

半群上的L－Fuzzy同余关系

先引入半群Ｓ上的Ｌ－Ｆｕｚｚｙ同余关系的概念，进而讨论Ｌ－Ｆｕｚｚｙ同余关系的几个基本性质，然后证明半群Ｓ上的所有Ｌ－Ｆｕｚｚｙ同余关系作成一个格，同时证明群Ｇ上所有Ｌ－Ｆｕｚｚｙ同余关系作成一个模格．     

关于q－基本群和内7－闭可解群的构造

研究内ｐ－闭群和ｑ－基本群的构造是一个很活跃的课题，对于ｐ＝２，３，５的内ｐ－闭群的构造已经被确定（见［１，２，３，４或５］）。文［６］研究过２－基本群，文［５，定理１．１］列出了ｑ－基本群的一些重要性质，本文首先推广［５，定理１，１］的一个结果，进而确定ｑ－基本群和内７－闭可解群的构造。     

仿射Weyl群(E～)6的a值5的左胞腔

Coxeter群的胞腔是1979年Kazhdan和Lusztig中定义的，这些胞腔理论在代数群的表示理论中发挥了重要的作用。对一些特殊的情况，胞腔的分类已经明确地给出了，例如，对于秩为2的群参见，对于An^-参见，对于a值4的典范型和或参见.本文利用时俭益的运算算法给出了仿射Weyl群E6^-的a值等于5的所有左胞腔。     

关于q－基本群和内7－闭可解群的构造

研究内ｐ－闭群和ｑ－基本群的构造是一个很活跃的课题，对于ｐ＝２，３，５的内ｐ－闭群的构造已经被确定（见［１，２，３，４或５］）。文［６］研究过２－基本群，文［５，定理１．１］列出了ｑ－基本群的一些重要性质，本文首先推广［５，定理１，１］的一个结果，进而确定ｑ－基本群和内７－闭可解群的构造。