Hg原子6^3P1→6^1So态的系际交叉跃迁及其6^1P1态与6^3P1态的组态混合

Hg原子6^3P1→6^1So态253.652nm紫外辐射是系际交叉路迁最著名的一例，可归因于其单重态6^1P1与三重态6^3P1的组合混合。计算结果表明，对于Hg原子6s6p组态，LS耦合方式仍是其较好描述。     

关于电磁打点计时器打双点问题的研究

中学物理实验中所用的电磁打点计时器，如图1所示，额定工作电压为4～6V的交流电，通常工作时，每隔0．02s打一个点．但笔者在指导学生实验中发现，用该仪器验证牛顿第二定律实验时，并未发现图2所示的打双点现象．但用该仪器做验证机械能守恒定律的实验时，却发现打双点现象，这是为什么呢？     

空间波函数的对称性对氦原子双光子双电离过程中电子关联的影响

通过数值求解含时薛定谔方程，研究了氦原子具有对称空间波函数的1s2s 1S态和具有反对称空间波函数的1s2s 3S态分别作为初态的双光子双电离过程. 结果表明，对于初态为单重态1s2s 1S的双光子双电离过程，两个电离电子的能量分布随激光脉冲持续时间的增加呈现由单峰到双峰的变化，这里的单峰和双峰分别意味着两个电离电子主要携带相等和不等的能量；然而对于初态为三重态1s2s 3S的双光子双电离过程，两个电离电子的能量分布随激光脉冲持续时间的增加总是保持双峰结构. 这些结果表明当原子的初态处于反对称空间波函数时，两电子的空间密度分布具有较少的重叠，从而导致电子在超短激光脉冲中电离时电子关联能无法平均分配.     

Ba原子6s5d~3 D与6p5d~3 F态的超精细结构及态间跃迁的同位素移动的直接确定

提出并演示了一种光泵预选态的原子光谱测量方法,并对Ba原子的6s5d3 D态与6p5d3 F态的超精细结构及该跃迁的同位素移动进行了直接测量。首先利用791nm的激光激发Ba原子特定同位素及特定超精细结构的6s6s 1 S0→6s6p3 P1跃迁,并利用6s6p3 P1→6s5d3 D2的自发辐射有选择地分别将这些同位素制备到6s5d3 D2态不同的超精细能级上,再用778nm的激光扫出对应的6s5d3 D2→6p5d3 F2跃迁的荧光光谱,通过这几组光谱之间的对比直接实现了对22条超精细谱线的认定和归属,从而得到了135 Ba和137 Ba的6s5d3 D2能级与6p5d3 F2能级的超精细结构常数及该跃迁的同位素移动。     

锂里德堡态的d-f间隔的共振计算

应用全实加关联方法计算而得到的锂原子的1s2nd (n=3–5) 态 和 1s2nf (n=4–6) 态的能量，我们可以通过量子亏损理论得到量子亏损函数，它随着能量平缓地变化。利用这些函数可以分别构造一个系统方程去求解锂原子1s2nd和 1s2nf (n=7–11)里德堡态的能量和量子亏损。我们计算了nd和nf 中心能级 (n=7–11)的间隔并和文献中已有的实验和理论数据做了比较。     

碳原子1s22s22pns 3P态的能量和波函数

提出了构造碳原子1s22s22pns 3P态波函数的新方法,以Rayleigh-Ritz变分法为基础开发了一套计算碳原子1s22s22pns 3P态波函数和能量的Mathemtica程序,具体计算了碳原子1s22s22pns 3P(n=3-6)态的波函数和非相对论能量及其相对论修正值(包括质量修正、单体达尔文修正、双体达尔文修正、自旋-自旋接触相互作用修正),计算结果与实验值非常接近。     

碳原子1s22s22pns 3P态精细结构的理论计算

提出了构造碳原子1s22s22pns 3P态波函数的新方法,以多电子原子精细结构哈密顿的球张量形式和不可约张量理论为基础,开发了一套计算碳原子1s22s22pns 3P态精细结构的Mathemtica程序,具体计算了碳原子1s22s22pns 3P(n=3-6)态的精细结构(包括自旋-轨道相互作用、自旋-其它轨道相互作用和自旋-自旋相互作用),计算结果与实验值非常接近。     

B2H6分子的几何构型

采用Gaussian 98程序中B3P86，BP86，B3LYP，BLYP，UHF，HF及LSDA等方法，对B_{2Ｈ6分子可能的D3d，D3h，D2d和D2h平面型状态及立体型状态 的几何构型五种情况的1重态及3重态进行了优化，得到该分子基态为1重态，它的电子状态 是^lＡg,B2H6的几何构型仍然是传统的对 称性为乙烯式的D2h结构 ，其构型如图9所示，其能量最低，是－53．5865H.a.u..两个硼原子与四个H原子所在平面 垂直于两个硼原子及另外二个H原子所在平面，二个硼原子之间的距离是R12=0 ．17542nm，B原子及H原子之间的距离是R17=0．13149nm，R13=0． 1188 4nm,它们之间的夹角分别是，∠314=∠526=121．93°，∠817=∠827=96．3°，B2Ｈ6中硼原子采用不等性的sp³轨道和另一硼原子的不等性的sp< sup>3轨道 及氢原子的1s轨道 交互重叠生成桥式三中心双电子键.三中心双电子键比双中心双电子键更为稳定，计算结果 也证实了这一点. 关键词： 2H6')" href="#">B2H6 密度泛函 几何构型 优化}     

Yb原子里德伯态及价态的场电离阈

用偏振激光两步激发得到Yb原子不同|m|值的里德伯态和4f~(13)5d6s6p价态,采用脉冲场电离方法测定了6sns~1S_0(n=21—28),m=0和6snd~1D_2(n=20—27),|m|=0,1各里德伯态及4f~(13)5d6s6p价态的电离阈值。引入stark有效量子数n_s对电离阈值作了计算。对实验和计算结果作了对比分析。讨论了场电离过程中价态与里德伯态之间的相互作用及其对电离阈值的影响。 关键词：     

类锂体系激发态的精确判据

利用Gálvez Porras关于原子体系电子在核处密度和径向期待值的精确不等式，分别建立了波函数的两套精确判据，它们是独立于能量判据之外的检验波函数精确度的判据. 以类锂体系激发态为研究对象，首先对1s2 3s态的电子在核处密度和径向期待值的上界进行了检查，然后对锂原子1s2 3s态在不同计算方法下由电子在核处密度上界定义的R6值和的上界定义的R4值分别进行了测试，同时还对锂原子双激发态的电子在核处密度和径向期待值的上界进行了检验. 研究表明这两套不等式都可作为原子体系各种能态波函数的精确判据. 关键词： 电子在核处密度 径向期待值 全实加关联 精确判据     

Doppler-free spectroscopy of mercury at 253.7 nm using a high-power, frequency-quadrupled, optically pumped external-cavity semiconductor laser

We have developed a stable, high-power, single-frequency optically pumped external-cavity semiconductor laser system and generate up to 125 mW of power at 253.7 nm using successive frequency doubling stages. We demonstrate precision scanning and control of the laser frequency in the UV to be used for cooling and trapping of mercury atoms. With active frequency stabilization, a linewidth of <60 kHz is measured in the IR. Doppler-free spectroscopy and stabilization to the 6(1)S(0)-6(3)P(1) mercury transition at 253.7 nm is demonstrated. To our knowledge, this is the first demonstration of Doppler-free spectroscopy in the deep UV based on a frequency-quadrupled, high-power (>1 W) optically pumped semiconductor laser system. The results demonstrate the utility of these devices for precision spectroscopy at deep-UV wavelengths.     

Narrow-band UV radiation (250–260 nm) from intracavity doubling a single-mode ring dye laser

Generation of continuous-wave, tunable UV radiation (250–260 nm) by intracavity doubling a coumarin-515 ring dye laser is described. A cooled (200–280 K) ADP crystal with end faces cut at Brester's angle is placed inside the laser ring cavity which has been compensated for astigmatism and coma. UV output powers at 254 nm of 120 μW and 60 μW are achieved with the laser operating multimode (bandwidth ? 20 GHz) and single-mode (bandwidth ? 50 MHz), respectively. Continuous single-mode scans over the 253.7 nm mercury profile demonstrate sub-Doppler resolution of the Hg 6s6p ³P^O₁ - 6s²¹S₀ transition.     

750 mW continuous-wave solid-state deep ultraviolet laser source at the 253.7 nm transition in mercury

A high-power continuous-wave coherent light source at 253.7 nm is described. It is based on a solid-state Yb:YAG disk laser with two successive frequency doubling stages and is capable of generating stable output powers of up to 750 mW. Spectroscopy of the 6 (1)S(0)-6 (3)P(1) transition of mercury has been demonstrated.     

Airborne-mercury detection by resonant UV laser pumping

Optical pumping of the Hg(0) (6s (1)S(0) --> 6p (3)P(1)) transition at 253.7 nm (in air) leads to extremely fast energy transfer and strong laser-induced-fluorescence (LIF) from the Hg(0) (7s(3)S(1) --> 6p (3)P(2)) green transition at 546.2 nm, which is not directly populated by the laser. Ionization occurs simultaneously and becomes particularly strong at reduced background pressures. These observations are consistent with the existence of a multiphoton process followed by electron collisional excitation. Preliminary studies are made to evaluate these phenomena for detecting elemental airborne mercury by LIF and point monitoring with an ionization detector. Measured sensitivities of 2 and 10 parts in 10(9) (ppb), respectively, at 0.1-Torr air pressure are projected to increase to 1 x 10(-4) and 1 x 10(-5) ppb after relevant system optimization.     

Neutral atom frequency reference in the deep ultraviolet with fractional uncertainty = 5.7×10(-15)

We present an assessment of the (6s2) (1)S0 ? (6s6p)(3)P0 clock transition frequency in 199Hg with an uncertainty reduction of nearly 3 orders of magnitude and demonstrate an atomic quality factor Q of ～10(14). The 199Hg atoms are confined in a vertical lattice trap with light at the newly determined magic wavelength of 362.5697±0.0011 nm and at a lattice depth of 20E(R). The atoms are loaded from a single-stage magneto-optical trap with cooling light at 253.7 nm. The high Q factor is obtained with an 80 ms Rabi pulse at 265.6 nm. We find the frequency of the clock transition to be 1,128,575,290,808,162.0±6.4(syst)±0.3(stat) Hz (i.e., with fractional uncertainty=5.7×10(-15)). Neither an atom number nor second order Zeeman dependence has yet been detected. Only three laser wavelengths are used for the cooling, lattice trapping, probing, and detection.     

VUV photometric comparison between an absolute flux detector and standards traceable to the NBS

An absolute flux detector obtained by means of the calibration cross, has been compared with a standard source at 253.7 nm and a calibrated photodiode in the range of 135.4 to 253.7 nm, both standards traceable to the NBS.     

冷端温度对无极灯253.7nm共振谱线的影响

无极灯是一种长寿命、低汞害、无频闪的新型电光源,其光效在很大程度上取决于253.7nm共振谱线的辐射效率。通过原子发射光谱分析,实验研究了冷端温度对253.7nm共振谱线的影响规律。研究发现,253.7nm共振谱线的辐射效率随冷端温度变化近似呈正态分布,即无极灯工作存在一个最佳冷端温度。运用气体放电理论对实验结果进行了定性分析,对无极灯光效的提高具有指导意义。     

铟网位置对无极灯253.7 nm共振谱线的影响

无极灯是一种基于高频电磁感应和无极气体放电的新型电光源,由Hg 253.7 nm共振谱线激发荧光粉进而发出可见光。通过原子发射光谱分析,实验研究了铟网位置对Hg 253.7 nm共振谱线的影响规律。研究发现,Hg 253.7 nm共振谱线的相对强度,当铟网位于耦合线圈两端时最强,位于耦合线圈中部时较弱,远离耦合线圈时最弱。并推断,存在一个最佳的铟网位置,对应最高的发光效率。结合Maxwell 3D有限元仿真,从气体放电角度对实验结果进行了定性分析,对无极灯模型设计与参数优化具有指导意义。     

Study of the dependence of the radiative properties of high-frequency electrodeless lamps in an Hg-Ar mixture on the pressure of mercury vapor

The radiative characteristics of high-frequency electrodeless lamps in a mixture of mercury and argon have been studied theoretically and experimentally as functions of the cold spot temperature (the pressure of mercury vapor). The intensity of the mercury lines at 404.7, 435.8, and 546.1 nm, corresponding to the triplet transition (7³ S ₁-6³ P _0,1,2) in the visible spectral region, as well as the intensity of the UV resonance line (6³ P ₁-6¹ S ₀) at 253.7 nm, has been measured. A model describing the physical processes in the discharge plasma and including the kinetics of excited states of mercury and argon atoms has been suggested. The parameters of the discharge plasma and the electromagnetic field have been calculated self-consistently through the numerical solution of the system of equations of electron density and energy balance and population balance of excited levels of argon and mercury atoms, as well as the Maxwell equations. The model developed has allowed us to calculate the intensities of the mercury emission lines at 253.7, 404.7, 435.8, and 546.1 nm and to compare the results with experimental data. The relative intensities of the mercury spectral lines corresponding to the triplet transition 7³ S ₁-6³ P _0,1,2 have been calculated for the first time on the basis of a self-consistent model of the discharge.     

Comparative Study of the Ratio Spectra Derivative Spectrophotometry,Derivative Spectrophotometry and Vierordt's Method Appued to the Analysis of Lisinopril and Hydrochlorothiazide in Tablets

Abstract

Three new spectrophotometric methods are described for the determination of lisinopril and hydrochlorothiazide in their binary mixturer: First derivative spectrophotometry ratio spectra derivative and Vierordt's method. The procedures do not require any prior separation. In the derivative spectrophotometry, the dA/dλ values in the first derivative spectra of the mixture were measured at 269.6 nm for lisinopril and at 279.8 nm for hydrochlorothiazide. The calibration graphs were linear in the range 25.56–129.50 μg.ml^?1 for lisinopril and 10.60–139.80 μg.ml^?1 for hydrochlorothiazide. In ratio spectra derivative spectrophotometry, the calibration graphs for 15.68–129.50 μg.ml^?1 lisinopril and for 5.98–139.80 μg.ml^?1 hydrochlorothiazide were obtained by measuring the signals at 253.7 nm and 243.6 nm for lisinopril and at 280.1 nm and 270.8 nm for hydrochlorothiazide. In Vierordt's method, A¹ ₁ (1 %, 1 cm) values of lisinopril and hydrochlorothiazide were determined at 259.8 nm and 272.7 nm in the zero-order spectra. The quantity of both compounds were calculated by using the A¹ ₁ (1 %, 1cm) values. The methods were successfully applied to a pharmaceutical formulation for determination of both active compounds.