飞秒激光氘团簇库仑爆炸引发核聚变的机理研究

在超强飞秒激光与氘团簇的相互作用中，利用库仑爆炸模型，分析了可以引发核聚变的高能氘核产生的机理，提出了氘离子团簇膨胀尺寸与时间的关系式，计算了多种尺寸的氘团簇库仑爆炸时氘核的动能以及氘团簇的解体时间． 关键词： 飞秒强激光 氘团簇 库仑爆炸 核聚变     

超强超短脉冲激光诱发大尺度氘团簇聚变

 利用低温脉冲气阀获得了平均含有3×103氘原子的氘团簇。在飞秒激光装置上实现了氘团簇聚变,每发中子产额为1×10³。中子产额对激光功率密度敏感,保持激光能量不变,随着激光焦斑的变大,DD聚变中子产额逐渐增加,最大值出现在激光焦斑为470 mm时;继续增大激光焦斑,没有观察到中子信号。实验结果还表明激光氘团簇聚变发生的区域主要是激光辐照的等离子体热区,此区域内邻近氘团簇库仑爆炸发射的高能氘离子碰撞引发聚变反应。     

飞秒强激光场中大尺寸氩团簇爆炸机理的实验研究

利用飞行时间谱，研究了在飞秒强激光场（60 fs，2×1016 W/cm2）作用下，大尺寸氩原子团簇Arn（n—=3×103—3×106原子/每团簇）的电离爆炸过程，测量了 团簇爆炸所产生的氩离子的平均能量与团簇尺寸（气体背压）的关系.实验发现，随着气体 背压的升高（团簇尺寸增大），氩离子的平均能量也相应升高.通过分析两个不同几何尺寸 锥形超声喷嘴所产生团簇爆炸后的离子能量，结合Hagena团簇尺寸规律，发现在激光参数保 持不变的情况下，离子的平均能量由团簇尺寸唯一确定.分析表明，团簇尺寸在3×105原 子/每团簇以下时，团簇膨胀的主要机理是库仑爆炸.随着团簇尺寸的进一步增大，团簇膨胀 机理将由库仑爆炸向流体动力学膨胀过渡，在3×105关键词： 原子团簇 飞秒强激光 库仑爆炸 流体动力学膨胀     

SILEX-I装置上激光-团簇聚变实验中子产额测量

 超短超强脉冲激光与CD4团簇相互作用可以产生高能量的氘离子,从而产生DD聚变中子,这种团簇聚变中子源有着非常广阔的应用前景。在SILEX-I 100 TW飞秒激光装置上,超短超强脉冲激光与CD₄团簇相互作用实现了DD核聚变。团簇聚变的中子产额是实验中最为重要的物理量,在实验中采用高灵敏的中子探测器对团簇聚变产生的中子进行了测量,在现有实验条件下测得中子产额为10³。     

氘代乙烷团簇库仑爆炸产生高能氘核和中子的研究

采用简化库仑爆炸模型对强激光脉冲照射氘代乙烷团簇发生的库仑爆炸过程进行数值模拟,研究了氘代乙烷团簇爆炸产生的氘核动能、中子产额与团簇尺寸的关系,且与氘代甲烷团簇产生的氘核动能及中子产额进行了比较.研究表明,尺寸为5 nm的氘代乙烷团簇在发生库仑爆炸后氘核的最大动能为20.96 keV,获得的中子产额为6.31×105,比同尺寸氘代甲烷团簇产生的氘核最大动能及中子产额更大.因此相对于氘代甲烷团簇,大尺寸的氘代乙烷团簇更适合作为激光驱动团簇库仑爆炸获得高额中子的靶材,这与报道的实验推论相一致.     

飞秒强激光脉冲中氩团簇库仑爆炸特性研究

利用Bathe模型,理论模拟了氩团簇在飞秒强激光中(100 fs, 1016 W/cm2)的电离和爆炸过程.研究结果显示,在团簇尺寸较小时,离子平均能量与团簇初始半径平方成正比,爆炸机制为典型的库仑爆炸.随着团簇尺寸的增加,能量增加的速度趋缓并在一定团簇尺寸后趋于饱和.模拟结果与实验数据有较好的吻合.     

团簇在超强超短脉冲激光场中的演化

 利用低温脉冲气阀产生氘团簇束,在SILEX-Ⅰ激光装置上开展实验,研究氘团簇在超强超短脉冲激光场中的演化过程,获得了数十keV的高能氘离子,这些氘离子的能谱分布与库仑爆炸模型计算结果一致。实验结果表明,在一定的激光功率密度条件下,团簇的平均尺度决定了释放出高能离子的能谱分布。激光辐照团簇后,通过阈上电离部分电子逃逸团簇,随着初始电离电子屏蔽作用加强,碰撞电离变成了团簇的主要电离机制。     

4s和4p半核态引入价态(导致杂化指数降低)可以减弱Mon (n=2∽18)团簇的二聚体现象的第一性原理研究

钼团簇因具有独特的结构、电子和物理化学性质,被期待在未来的纳米科技中扮演重要角色,但是它们的基态结构至今还存在争议. 本研究采用粒子群优化(CALYPSO)方法对Mo_n (n=2∽18)团簇的晶体结构进行全局域能量最小化搜索,并结合第一性原理方法进一步优化. 计算表明：当4s和4p半核态不作为价态时,Mo_n (n=2∽18)团簇有明显的二聚体趋势,原子数为偶数的团簇往往是“幻数”团簇,具有较高的稳定性;但是,将4s和4p电子作为价电子后,平均杂化指数H_sp、H_sd和H_pd显著降低,二聚体趋势急剧减弱. 本文报道了Mo_n(n=11,14,15)团簇的新基态结构,证明了半核态对于Mo_n团簇是十分重要的.     

第一性原理计算ZrnFe(n=2—13)团簇的基态结构及其磁性

从第一性原理出发，利用密度泛函理论中的广义梯度近似对Zr_nFe(n=2—13)团簇进行了结构优化、能量和频率计算.在充分考虑自旋多重度的前提下，对每一具体尺寸的团簇，得到了多个平衡构型，并根据能量高低确定了团簇的基态结构.综合团簇的结合能、二阶能量差分以及团簇的最高占据轨道和最低未占据轨道间的能隙可知Zr₅Fe，Zr₇Fe和Zr₁₂Fe团簇的稳定性相对较高，Zr₁₂Fe团簇的结构是具有I_h对称性的正二十面体，而且Zr₁₂Fe的稳定性在所有团簇中是最高的.另外，不仅Zr₅Fe，Zr₇Fe和Zr₁₂Fe团簇的稳定性相对较高，而且它们均为磁性团簇(而Zr_n团簇的磁矩在n≥5时已经发生了淬灭)，由此可知通过选择合适的掺杂元素可能得到高稳定的磁性团簇.从Mulliken布居分析结果可知，除了在Zr₁₂Fe团簇中Fe原子失去少量电荷外，其他团簇中Fe原子均从Zr原子那里得到了一定量电荷，即Fe原子在Zr_nFe(n=2—13，n≠12)团簇中是电子受体.     

特定位点上CO2与(TiO2)n团簇相互作用的第一性原理研究

本文基于密度泛函理论系统地研究了(TiO₂)_n团簇上二氧化碳(CO₂)的吸附和活化性质. 计算结果表明,CO₂更倾向于吸附在(TiO₂)_n团簇的桥氧原子上,形成“化学吸附”碳酸盐络合物. 而CO更倾向于吸附到末端Ti-O的Ti原子上. 发现计算得到的碳酸盐振动频率值与实验获得的结果非常吻合,这表明配合物中CO₂的几何构型与其线性型相比,有微小的弯转. 通过对电子结构、电荷密度、电离势、HOMO-LUMO以及态密度的分析,证实了CO₂与团簇之间的电荷转移以及相互作用. 从预测的能量分布图来看,(TiO₂)_n团簇上的CO₂活化与结构密切有关,相比于块体的TiO₂,CO₂在团簇结构上更易于吸附和活化.     

Ultrafast nuclear dynamics and non-uniform Coulomb explosion of heteroclusters

This paper reports on some unique features of the ion spatial distribution, energetics and time-resolved dynamics in Coulomb explosion of multicharged light-heavy heteroclusters, consisting of light, low-charge and heavy, high-charge, ions, e.g. hydroiodic acid [image omitted] and its isotopic substituents [image omitted] and [image omitted]. In these clusters, extreme multielectron ionization in ultraintense laser fields (peak intensity I = 1015 - 1020 W cm-2) results in highly charged heavy ions, e.g. qI ? 7 at I = 6×1015 W cm-2 and qI = 25 at I = 1019 W cm-2. Molecular dynamics simulations based on the cluster vertical ionization (CVI) initial conditions, together with complete simulations involving both electron and nuclear dynamics of heteroclusters subjected to a Gaussian laser pulse, which were conducted for Coulomb explosion of [image omitted] and [image omitted] ionic clusters, reveal expanding, thin, two-dimensional spherical shells of the light D+ or H+ ions, with the monolayer expansion occurring on the femtosecond time scale. The expanding spherical nanoshells of light ions are analogous to a 'soap bubble', characterized by negative surface tension and driven by Coulomb pressure. The energetic data for the light ions reveal high energies with a narrow energy distribution, characterized by a lower energy cut-off, e.g. average energy Eav = 23 keV at width ΔE/Eav = 0.16, and a cut-off energy of EMIN = 19.2 keV for Coulomb explosion of [image omitted] clusters. These dynamic, structural and energetic data for exploding multicharged light-heavy heteroclusters arise from kinematic overrun effects of the light ions.     

On the energy dependence of the yield of doubly charged negative ions during the capture of free electrons by C60(CF3)12 trifluoromethylfullerene molecules

Peaks of C₆₀(CF₃) _n ^2? doubly charged negative ions (n = 6–12) have been observed in the mass spectra of the resonance electron capture by trifluoromethylfullerene C₆₀(CF₃)₁₂ molecules. It has been established that these ions are formed owing to the attachment of two free isoenergetic electrons. The autodetachment of an extra electron has been detected for the doubly charged molecular ions (n = 12). It has been established from the observation of the delayed fragmentation of the most abundant ions with n = 8 and 10 that the doubly charged negative ions, like their singly charged analogs, are metastable with respect to the separation of the CF₃ fragment(s). The yield of doubly charged negative ions has been obtained as a function of the electron energy. By comparing them with the analogous dependences for the singly charged ions, the specific features have been revealed which were associated with the presence of the repulsive Coulomb barrier and the regular effect of the doubled energy of two additional electrons on the energy dependence of the dissociative decay of the doubly charged negative ions. The absolute cross section for the formation of the C₆₀(CF₃) ₁₀ ^2? ions has been measured. At the energy of their yield maximum near the 5 eV, it is ～1 × 10^?19 cm².     

Synthesis and regularities of combustion of acetoxymethylnitroamines. Impact sensitivity of secondary alkylnitroamines

The use of the nitrolysis of cyclic amines and of the direct synthesis from primary nitroamines made it possible to obtain acetates of methylolnitroamines of general formula AcO(CH₂NNO₂) _n R(n = 1–6). A number of high explosives, nitroamines, were synthesized: DNA ((CH₃NNO₂)₂CH₂), DMNA ((CH₃)₂NNO₂), DNA-2 ((CH₃NNO₂CH₂)₂), TRIS ((CH₃NNO₂CH₂)₂NNO₂), and TETRA ((CH₃NNO₂CH₂NNO₂)₂CH₂). The regularities of the combustion of the synthesized compounds were studied, and their characteristics were compared. Stress curve measurements were used to estimate the impact sensitivity of alkylnitroamines. A number of basic macroscopic characteristics of the nitroamines studied and nitroamine-ammonium perchlorate mixtures, including the heat of explosion. For comparison, the characteristics of regular high explosive are given.     

Study of background processes with the formation of neutrons in nuclear reactions in the energy range of 26–32 kev

The nature of background processes accompanying astrophysical nuclear reactions induced by hydrogen, helium, and neon ions in deuterated targets with small cross sections has been studied in calculations and experiments. The experiments have been performed at a Hall pulsed plasma accelerator in the ion energy range of 26–32 keV. The yield of background neutrons and γ-quanta with energies below 4 MeV in the proton-induced D(p, γ)³He reaction is primarily due to the presence of a natural impurity of gaseous deuterium in gaseous hydrogen and the chain of D(D, ³He)n → (n, γ) or (n, n'γ) reactions. A small contribution comes from the chain of D(¹H, ¹H)D → D(D, ³He)n → (n, γ) or (n, n'γ) reactions. It has been shown that background neutrons and γ-quanta from the D(4He, γ)6Li reaction are entirely due to the chain of D(⁴He, ⁴He)D → D(D, ³He)n → (n, γ) or (n, n'γ) reactions. It has been shown that the yield of neutrons and γ-ray photons detected at the interaction of neon ions with deuterated targets is also entirely due to the chain of elastic- scattering reactions of neon ions on deuterons in the target and to subsequent inelastic processes of interaction of deuterons accelerated at elastic scattering with other deuterons of the target. The main contribution to the yields of background neutrons and γ-quanta comes from doubly charged neon ions. The main conclusion is that the explanation of the yield of neutrons and γ-quanta at the interaction of hydrogen, helium, and neon ions with deuterated targets does not require “exotic” theoretical models.     

Processes of ordering of structural elements, critical and noncritical parameters of phase transitions in the (NH4)3WO3F3 crystal

The structure of the low-temperature triclinic phase of the (NH₄)₃WO₃F₃ crystal has been determined and the structure of the cubic phase of this crystal has been refined from data of an X-ray diffraction experiment performed for a powder sample. The profile and structural parameters have been refined according to the procedure implemented in the DDM program. The results obtained have been discussed with invoking the group-theoretical analysis of the complete order parameter condensate, which takes into account the critical and noncritical atomic orderings and allows one to interpret the obtained experimental data. It has been found that the symmetry transformation in the crystal can be schematically represented in the following form: Fm[`3]m(Z = 4) ? P[`1](Z = 1) ? P[`1](Z = 6)Fm\bar 3m(Z = 4) \to P\bar 1(Z = 1) \to P\bar 1(Z = 6). This transformation is accompanied by the complete ordering of WO₃F₃ polyhedra and the displacement of NH₄ ions.     

Quantum electrodynamic corrections to the 23S1 → 11S0 + one photon transition rate in helium and helium-like lons

The order (Zα)⁵, α(Zα)⁴, and α(Zα)⁴ log(Zα) energy denominator and recoil corrections to the leading order (Zα)⁴ decay amplitude for the 2³S₁ → 1¹S₀ + one photon transition are considered. It is found that order α(Zα)⁴ terms arise in the individual diagrams but exactly cancel upon summation. In view of the results of this and other recent theoretical work it is concluded that the rates predicted by pure quantum electrodynamics are known to considerable precision. The recent discrepancy between theory and experiment in the decay rate for several helium-like ions appears to have been resolved by placing the detector farther downstream from the foil where the metastable states are produced. At present, all the experimental values are in good agreement with the theory.     

Ignition curves for deuterium/helium-3 fuel in spherical tokamak reactor

In this paper, ignition curve for deuterium /helium-3 fusion reaction is studied. Four fusion reactions are considered. Zero-dimensional model for the power balance equation has been used. The closed ignition curves for ρ=constant (ratio of particle to energy confinement time) have been derived. The results of our calculations show that ignited equilibria for deuterium /helium-3 fuel in a spherical tokamak is only possible for ρ= 5.5 and 6. Then, by using the energy confinement scaling and parameters of the spherical tokamak reactor, the plasma stability limits have been obtained in n_e, T plane and, to determine the thermal instability of plasma, the time-dependent transport equations have been solved.     

Fragmentation of polyatomic ions produced by electron-loss collisions of butane and isobutane molecules with ions of kiloelectronvolt energy

Fragmentation accompanying the loss of electrons by butane and isobutane (C₄H₁₀) molecules in collisions with energy H⁺, He²⁺, and Ar⁶⁺ ions of kiloelectronvolt energies is studied. The electron density functional technique is applied to C _n H_2n+2 alkane molecules and their respective C _n H _2n+2 ⁺ ions to carry out quantum-chemical calculations of the atomic spacing, electron total energy for the initial configuration of the ionizing molecules and ions in the ground state, and atomic bond breaking energy necessary to produce different ion fragments. The fragmentation energy is correlated with the fragmentation probability. It is shown that the relative cross sections of ion fragmentation depend primarily on the related energy consumption. However, the process cross section is also strongly affected by the initial configuration of C₄H₁₀ isomer molecules, as well as by the amount of dangling and arising atomic bonds involved in the formation of each ion fragment.     

Energy efficiency of femtosecond laser ablation of polymer materials

We present the results of an experimental study of the ablation spectral energy thresholds for a number of polymer materials ((C₂F₄) _n , (CH₂O) _n ) exposed to femtosecond (τ_0.5 ~ 45–70 fs) laser pulses (λ ~ 266, 400, 800 nm) under atmospheric conditions and under vacuum (p ~ 10–2 Pa). We have analyzed the energy thresholds and the efficiency of optical, thermophysical, and gasdynamic processes in laser ablation vs. the laser pulse duration and photon energy.     

Anregung und Schädigung der Lumineszenz von CaWO4 und ZnS/Ag durch Ionen

The luminescence-response of ZnS/Ag and CaWO₄ to ion-bombardement and the deterioration of luminescence under prolonged irradiation was determined as a function of ion-energyE, ion-massM _i and beam-densityI. The variation of lightoutput with ion-energy is of the formJ ₀=C. (E-E ₀) ⁿ withn=2 (ZnS/Ag) or lower values (CaWO₄). The luminescence-response to ions of various mass was found to decrease generally with growing mass, but to be nearly constant to ions of middle atomic weight (ZnS/Ag). The luminescence-efficiency, caused by ions of energy greater than 5 keV, is independent of beam-density within the whole range studied here (maximum 3 · 10^?7 A · cm^?2), but it diminishes in the caseE=5 keV for values ofI above 6 · 10^?8 A · cm^?2. The deterioration-effect grows, except in the case of He⁺-ions, the lightest ions used here, with ion-energy. It also increases by substituting Ne⁺- for He⁺-ions, but remains nearly independent of mass (CaWO₄) or diminishes with growing ion-mass (ZnS/Ag), if the ions are heavier than Ne⁺-ions. Increasing beam-density leads to a reduced deterioration of ZnS/Ag-luminescence, yet has no influence to that of CaWO₄.