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Magneto-Optical Trap of Cesium Atoms 被引量:5
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作者 GAN Jian-hua LI Yi-min +3 位作者 CHEN Xu-zong LIU Hai-feng YANG Dong-hai WANG Yi-qiu 《Chinese Physics Letters》 SCIE CAS CSCD 1996年第11期821-824,共4页
We have trapped a cold sample of cesium atoms in a magneto-optical trap.The damped harmonic force of magneto-optical trap was used to capture and trap the cesium atoms directly from a room temperature vapor.About 1.5&... We have trapped a cold sample of cesium atoms in a magneto-optical trap.The damped harmonic force of magneto-optical trap was used to capture and trap the cesium atoms directly from a room temperature vapor.About 1.5×10^(7) cesium atoms with a density of 3×10^(9) atoms/cm^(3) formed a 4mm^(3) cesium atomic cloud with temperature below 500μK. 展开更多
关键词 HARMONIC CESIUM MAGNETO
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Energy Dependence of Profile Width in Short Gamma-Ray Bursts
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作者 YANG Yu-xuan CHE Hai-hong +1 位作者 WU Mei CAO Sheng-lin 《Chinese Physics Letters》 SCIE CAS CSCD 1997年第10期797-800,共4页
Using the high time-resolution and 64ms resolution data of the burst and transient source experiment,we performed an autocorrelation analysis of the energy dependence of burst pulse width in short gamma-ray bursts.A m... Using the high time-resolution and 64ms resolution data of the burst and transient source experiment,we performed an autocorrelation analysis of the energy dependence of burst pulse width in short gamma-ray bursts.A method free from potential cosmological effects has been proposed.This allows us to use a sample with a size comparable to that used for long and bright bursts.Our result shows that the profiles of short bursts exhibit a very good power-law between profile width and photon energy,with an index~-0.3.This result is consistent with a united origin of the bimodal distribution. 展开更多
关键词 RESOLUTION MODAL transient
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Characterization of Frequency Stability:Analysis in Time Domain in Time Domain
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作者 卫国 《Science China Mathematics》 SCIE 1993年第3期338-345,共8页
A new model of noise processes,the so-called dynamic model,is presentedin which all the five noise processes(White PW,White FM,Random Walk FM,FlickerPM and Flieker FM)are involved.Withsuch a model and a special method... A new model of noise processes,the so-called dynamic model,is presentedin which all the five noise processes(White PW,White FM,Random Walk FM,FlickerPM and Flieker FM)are involved.Withsuch a model and a special method,the autocorrelationfunctions of the five noise processes are deduced. 展开更多
关键词 FREQUENCY STABILITY noise MODEL AUTOCORRELATION FUNCTION
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Line profiles of the two-phase medium broad-line region in active galactic nuclei
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作者 薛随建 林宣滨 +1 位作者 程福臻 John Kwan 《Science China Mathematics》 SCIE 1996年第8期883-896,共14页
In the framework of BLR in AGNs, i.e. large number of small, cold and dense emission-line clouds immerging in an intercloud hot medium, a delicate radiation model for a typical emission cloud is established, in which ... In the framework of BLR in AGNs, i.e. large number of small, cold and dense emission-line clouds immerging in an intercloud hot medium, a delicate radiation model for a typical emission cloud is established, in which the backside photoionization of the cloud against the central continuum source by the scattered diffuse continuum in the hot medium is considered. Under the assumption of the radial kinematics of the BLR clouds, the line profiles for the two important UV emission-lines, Lya and CIV/11549 are computed; and based on these calculations, various physical factors that affect the properties of the emission-line profiles are discussed. It is concluded that: (i) when the BLR clouds is inflow, there exists a confining hot medium with density around 2 x 105 cm-3. In this case, theoretical line profiles agree well with the observational; (ii) both symmetric Lya and nearly symmetric CIV line profiles show blue velocity shifts, the quantities of which are sensitive to the cutoff of the outer radius of the BLR. It is suggested that this cutoff effect is physical background to explain the observations that high ionization lines in the spectra of AGNs have some systematic blue shifts relative to those low ionization lines which usually characterize their source system velocities. 展开更多
关键词 active GALACTIC NUCLEI (AGNs) BROAD LINE region (BLR) EMISSION LINE profiles.
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Kinematic Models of BLR Gas and Line Profiles of HeIλ5876 and Hβ in AGNs
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作者 薛随建 程福臻 John Kwan 《Science China Mathematics》 SCIE 1994年第4期487-496,共10页
The present paper derives the modified expression of broad emission line profiles for the kinematic model of radiation pressure driving BLR gas outflow in the BLR, and discusses the intrinsic emission difference betwe... The present paper derives the modified expression of broad emission line profiles for the kinematic model of radiation pressure driving BLR gas outflow in the BLR, and discusses the intrinsic emission difference between the two lines HeIλ5876 and Hβ. It is shown that the fact that the observed line width of HeIλ5876 is broader than that of Hβ cannot be explained by W. G. Mathews’ modified model. For comparison, line profiles of gravitational infall model and orbital disk model are also calculated; the latter is in good agreement with the observations. Thereupon, conclusion is reached that gravitational infall is an important process in the BLR gas motion. 展开更多
关键词 AGNS broad-line REGION (BLR) broad-line profiles.
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