This note shows that the nontrivial third order cohomology cycle for gauge group implies the existence of anomalous associative law and consequently anomaly for Jacobi identity.

Many scientists hypothesized that the presence of oxygen is necessary for the formation and stabilization of the metastable high T_c A15 Nb₃Ge phase in Nb-Ge films. In our previous work we proposed that a certain amount of Nb₅Ge₃ may play a role in stabilizing the high T_c A15 phase. New experimental results of induction measurement on the Nb-Ge films support our proposal.

A class of spatially dependent exact solutions of the Boltzmann equation for a gas of monatomic Maxwell molecules is obtained and discussed. The similarity solution describing a gas uni-formly flying away proposed by Bobylev¹ is included in this class as a special case.

Possibilities of (8.32) being an 0⁺⁺ or 0^-+ Higgs are examined. Possible mixrings between Higgs and corresponding bottomia are considered. It seems that the ratio B_r[ T ( 2s ) → γ ]/ B_r[ T ( 1s ) → γ ]<0.22 could hardly be understood if is an 0^-+ Higgs, but may be understood if is an 0⁺⁺ Higgs.

Based on the argument that the bag radius of a bounded nucleon is larger than that of a free one due to the change of vacuum property in nucleus, a good fit is obtained for the EMC effect.

A convenient method is presented to compute the moments of the distribution amplitude for pion and a possible model form is proposed to fit the experimental data.

The temperature dependence of magnetization- and strain-induced magnetic anisotropy constants is reported in two nearly non-magnetostrictive CoFeSiB based metallic glasses. It is in accordance with the single-ion theory of uniaxial magnetic anisotropy. It seems that this theory can be regarded as a basis for discussing the nature of induced magnetic anisotropy in some metallic glasses.

The magnetic moments and Curie temperatures of amorphous Fe_90-XCo_XZr₁₀(0x90) alloys have been measured experimentally. For x 30, the great enhancement of the magnetic moment is explained by the increase of magnetic moment of iron atoms and the existence of two magnetic regions, while the increase of the Curie temperature with Co content is interpreted by the interactions of Fe-Co atoms which will be larger than that of Fe-Fe and Co-Co.

NdFeB permanent magnets of (BH)_max = 41MGOe were prepared by powder metallurgy. A typical specimen, Nd_16.4Fe_76.6B₇ alloy, was measured and analyzed. The crystallization process of this alloy near 1400K appeared very complicated. Non-uniform distribution of Nd atoms in the alloy shows that a second phase may exist. At low temperatures the easy direction for magnetization will become canting.

We have observed the granular deposition of metallic Li on the α-LiIO₃ surface in contact with the cathode of DC field by a scanning electron microscope. The relationship between the accumulation lines of space charges und the ionic transportation along c-axis is discussed.

A study of the anisotropy of primary cosmic rays is presented. The expression of the anisotropy was derived in a model of discrete sources in an infinite galaxy. Using these derived formulas, the amplitudes of the first harmonic anisotropy caused by eleven supernovae nearby the Earth were calculated individually and the trend of the resultant anisotropy was investigated. It was found that the expected results can account for the power law of E^0.5 of the anisotropy above an energy 5x10¹⁵eV, and the Compton-Getting effect is responsible for the anisotropies in the energy range 10¹¹-10¹⁴eV. Furthermore, we have got the streaming velocity of 35km/s with respect to the cosmic ray background.

In this paper, we point out that the spectrum of the quasar UM663 can not be explained by photoionization models; on the contrary, it can be explained by the theory of Cerenkov line radiation. The Cerenkov redshift Δλ_c( 24Å )of the emission line Lα of this quasar has been estimated from the position of Nv absorption line in the Lα-Nv profile.

The pressure dependence of deep energy levels associated with substitutional point defects in GaP is investigated using an approach proposed before. A deep level can be driven out of the gap into the valence bands, if this level is caused by a P-substitutional defect and located sufficiently close to the valence band maxim in the unpressurized solid. No deep level can be driven into the gap from the conduction bands by the pressure. The theoretical calculations are in good agreement with the experimental results.