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1引言设A是n阶非负方阵.设矩阵方程(1)AXA=A,(2)XAX=X,(3)(AX)~T= AX,(4)(XA)~T=XA,(5)AX=XA.A具有非负广义逆是指存在非负方阵X满足方程(1)~(4),并记为A~(?).A具有非负群逆是指存在非负方阵X满足方程(1),(2),(5),并记为A~#.在A~(?)存在的前提下,两者相同的充分必要条件有(a)AA~(?)=A~(?)A;(b)A~(?)=p(A),其 相似文献
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Quantum Inequality for Negative Energy Density States of Massive Dirac Field in Four-Dimensional Spacetime 下载免费PDF全文
Negative energy density and the quantum inequality are examined for the Dirac field. A proof is given of the quantum inequality for negative energy densities in the massive Dirac field produced by the superposition of two single particle electron states. 相似文献
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Zuo LIU Zhen De WU 《数学学报(英文版)》2005,21(5):997-1000
Let κ be non-negative integer. The unoriented bordism classes, which can be represented as [RP(ξ^κ)] where ξ^κ is a k-plane bundle, form an ideal of the unoriented bordism ring MO.. A group of generators of this ideal expressed by a base of MO. and a necessary and sufficient condition for a bordism class to belong to this ideal are given. 相似文献
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An experimental method for investigating the effect of medium boundary on distributions of light in the biological tissue phantom intralipid is presented. Measurements of distributions of light in intralipid-10% suspensions at 633 nm are described, in which a narrow collimated beam is incident on the surface of the phantoms and into the different depths inside of the phantoms. The experimental results show that the effect of the boundary of the medium on the curves geometry of light distributions is trivial, but the effect on intensity of scattering light is obvious, the maximal relative change of the energy fluence reaches 53.8% and the position of the peak of the energy fluence curve has a shift of 1.1 mm in the reverse direction of incident light for the phantom with albedo a=0.998, and the effect of the boundary is decreased with the increase of the absorption coefficients of tissue phantoms. The experimental results were analysed by the diffusion theory. These studies will be helpful for further understandings of the relation between the boundary of biological tissue and the distribution of light in tissue. 相似文献
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Temporal Skewness of Electromagnetic Pulsed Waves Propagating Through Random Media with Ebedded Irregularity slab 下载免费PDF全文
《中国物理快报》2003,20(3):370-373
Electromagnetic pulsed waves can be distorted in the propagation through random media,and their energy distributions change along the leading and trailing edge of the waveform,which can be presented by the temporal skewness.The skewness presents asymmetry and is treated by the third-order temporal moment,in which an analytic solution for the two-frequency mutual coherence function is obtained recently.Then,transionospheric pulses are discussed in details,Both theoretical analysis and numerical computation indicate that the contributions from scattering and dispersion of irregularities dominate over those of background,so the latter can be neglected in most cases.Also,the temporal skewness of a transionopheric pulse is negative and energy is shifted to the leading edge. 相似文献
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Using Schroedinger-Maxwell formalism, we propose and analyse a cw four-wave mixing (FWM) scheme for the generation of coherent light in a five-level double-∧ atomic system based on electromagnetically induced transparency. We derive the corresponding explicit analytical expressions for the generated FWM field. The influence of hyperfine sublevel on the amplitude of the generated FWM field is predicted in detail. We also give a brief discussion on the experimental realization of the proposed scheme. 相似文献
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Specific Angular Momentum Distribution of Disc Galaxies Formed in Preheated Intergalactic Media 下载免费PDF全文
LUOZhi-Jian FULi-Ping SHUCheng-Gang 《中国物理快报》2004,21(7):1409-1412
Assuming that baryons within a galactic halo have the same specific angular momentum as the dark matter where they locate initially and a disc forms due to the gas cooling and condensation with the conservation of angular momentum, we investigate the angular momentum distribution in a resulting galactic disc under the new preheated galaxy formation model suggested by Mo and Mao (Mon. Not. R. Astron. Soc. 333 (2002) 768).Compared with the observational results, it can be concluded that the preheated galaxy formation model can match current observations. This model can be a good approach to solve the problems of both the angular momentum catastrophe and the mismatch of angularomomentum profiles in current disc galaxy formation models. 相似文献