表面活性剂CTAB水溶液中的T2弛豫分散研究

用CPMG脉冲序列测定了表面活性剂十六烷基三甲基溴化铵（CTAB）分子中的氮甲基(N-CH₃)质子的横向弛豫时间（T₂表观）,并发现测得的T₂表观\}与序列中的重聚脉冲间隔时间的一半τ _cp有关,说明存在横向弛豫分散现象. 当在τ_cp≤1 ms时,T₂表观与τ²_cp}呈线性关系;而当τ_cp≥4.6 ms时,T₂表观变得与τ_cp无关. 利用Luz-Meiboom两体化学交换模型计算了不同浓度的CTAB溶液中的N-CH₃质子的本征横向弛豫时间（T₂本征）和化学交换速率k_ex,发现k_ex与T₂本征和自扩散系数D一样,在临界胶束浓度（CMC）附近发生突变. 这个突变反映了CTAB分子在从单体到胶束的转变过程中其动力学特性发生了改变.      

癸基萘磺酸钠胶束中分子动态的质子核磁共振研究

在298、303和313 K下对浓度为0.82 和2.59 mmol/L的癸基萘磺酸钠的重水溶液中质子的自旋-自旋弛豫（T₂）时间进行了测量. 浓度为0.82 mmol/L 的溶液(临界胶束浓度CMC以下)中的所有质子的T₂值均随温度上升而增长，说明整个分子运动变的更自由. 然而，浓度在CMC以上(2.59 mmol/L)时，分子中一部分参与形成栅栏层的质子的T₂值却表现出相反的效应，它们的运动随温度上升而变慢，说明在高温下为防止水分子进入疏水胶束壳内，这些栅栏层的质子堆积的更紧密. 同时分子中其他质子的T₂值随温度上升而增长，表现出正常的分子运动的温度效应.     

向列相液晶电流体不稳定性——偏置电场效应

本文考虑了外电场与液晶盒玻璃片法线成倾角θ₀时,沿面排列的向列相液晶(θ_α<0,σ_α>0)的电流体不稳定性现象。在Dubois-Violette等人的一维理论的基础上,我们获得了直流、正弦波和矩形波三种电场激发下的失稳条件。重要结果包括:(1)电荷弛豫时间随θ₀单调上升。(2)对于MBBA液晶,存在一个临界角θ_c(ω)(ω是外场频率),当θ₀>θ_c(ω) 关键词：     

正十二烷基硫酸钠在聚丙烯酰胺溶液中聚集的1H NMR研究

利用核磁共振自旋-晶格弛豫时间（T₁）、自旋-自旋弛豫时间（T₂）、自扩散系数（D）以及二维核Overhause增强谱（2D NOESY）技术研究了表面活性剂正十二烷基硫酸钠（SDS）在聚丙烯酰胺（PAM）浓度固定为10 g/L水溶液中的聚集. 结合与SDS水溶液体系核磁共振实验数据比较,得到了如下信息：（1） 当溶液中有PAM存在时,SDS分子的运动性下降,临界聚集浓度提前;（2） 随着SDS浓度的增加,PAM分子的自扩散性能下降,同时分子链的柔软性也下降了;（3） 2D NOESY谱结果表明,PAM与SDS分子间未发生直接的缔合作用.     

顺磁金属离子与某些氨基酸分子络合的NMRT1法研究

本文研究了水溶液中微量顺磁离子Fe³⁺和Cu²⁺对蛋白质及多肽结构单元一氨基酸分子纵向弛豫时间T₁的影响,把文献已处理过的金属离子与分子只存在一种络合物种体系的公式,推广到了多个络合物种并存且存在交换的体系中,导出并验证了顺磁弛豫速率R_f。与金属离子浓度C_M成线性关系,较深入地讨论了斜率大小与络合能力、配体浓度的关系.     

R型铁氧体BaFe4-xTi2+xO11的化学组态以及磁性行为的研究

本文通过传统的固相反应法制备了R型六角铁氧体BaFe_4-xTi_2+xO₁₁ (x= 0, 0.25, 0.5, 0.75, 1), 并且对它的原子价态以及磁性行为进行了研究. X 射线光电子能谱(XPS)结果显示了随着掺杂含量的增加, 体系中Fe³⁺离子逐渐减少而Fe²⁺离子逐渐增加. 由于具有非对称结构的阻挫晶格中存在各种关联作用的竞争, 使得BaFe_4-xTi_2+xO₁₁体系表现出了复杂的磁有序行为, 在T₁～250 K和T₂～83 K两处存在磁转变. 对这一系列掺杂样品, 在相变温度T₁之上表现顺磁行为, 而在相变温度T₂前后的磁化强度都表现出低场下随磁场的增加快速增加, 高场下则线性变化且在5×10⁴ Oe时还未达到饱和的行为, 表明这一系列掺杂样品是典型的倾斜反铁磁态(canted antiferromagnetic) 或者亚铁磁态.     

嵌段共聚物溶致液晶相中水的2H-NMR动力学分析

采用D₂O 的²H-NMR线型和弛豫分析了PEO-PPO-PEO/D₂O/对二甲苯体系的层状和六角液晶相的动力学行为. 通过实验测得了两个不同体系的自旋 晶格弛豫时间T₁、自旋-自旋弛豫时间T₂和²H-NMR 谱. ²H-NMR 谱均为具有四极劈裂的粉末谱线型，且在谱图的中心，β_LD=54.7°时存在一个倒峰. 倒峰的出现直接表明引起体系中弛豫的主要动力学过程处于极窄化区域. 采用NMR弛豫模型，通过调节动力学参数，使理论模拟的²H-NMR谱、弛豫时间、倒峰的大小与实验的对应量相吻合，求得了体系的动力学参数.     

两个共线Kerr黑洞度规迭加的时空结构

本文利用虚坐标方法研究了两个共线Kerr黑洞迭加的时空结构;首次得到了这种情况下视界以内的时空区域,并给出了2z₀>(M₁²-a₁²)^1/2+(M₂²-a₂²)^1/2时内外无限红移面和奇点随z₀变化的情况。由此我们可以看到,对于角动量平行及反平行的两个共线的全同Kerr解来说,当z₀→(M²-a²)^1/2时,尽管它们视界以外的时空结构分别趋于一个Kerr时空及一个Schwarzschild-NUT时空,但就整个时空结构而言,并非如此。同时,我们还可看到,当2z₀>(M₁²-a₁²)^1/2+(M₂²-a₂²)^1/2时,Einstoin场方程存在无裸奇点(而不是没有奇点)的解。 关键词：     

Nd3+螯合物的含氢有机溶液光谱性能研究

研究了Nd(TTA)₃螯合物溶于二甲基甲酰胺溶剂的光谱性质，溶液中所有氢未置换为氘.测量了这种溶液体系的吸收谱、荧光谱和荧光寿命.在898和1058 nm波长处观察到明显的Nd³⁺荧光特征峰.用Judd-Ofelt理论对吸收谱进行分析计算，得到了三个强度参数Ω_t(t=2,4,6)分别为Ω₂=4.9×10^-20 cm², Ω₄=5.1×10^-20 cm²和Ω₆=2.5×10^-20 cm².利用强度参数计算了⁴F_3/2能级与⁴I_9/2和⁴I_11/2之间的跃迁强度S_ed、自发辐射系数A_ed以及荧光分支比β等，估算了⁴F_3/2能级的辐射跃迁寿命τ_r＝682 μs.实测1058和898 nm波长处荧光寿命τ大约为460和505 μs，因此荧光量子效率分别高达0.67和0.74.荧光量子效率高表明Nd³⁺在这种溶液中无辐射跃迁比较弱；强度参数Ω₂比较大，表明Nd³⁺在溶液中具有不对称配位场环境，不对称的配位场环境可大大促进Nd³⁺吸收激发能量.光谱质量因子Ω₄/Ω₆>1，使得898 nm的辐射强于1058 nm的辐射. 关键词： Nd 有机溶液 光谱性能 Judd-Ofelt理论     

DNA平衡离子凝聚的动态光散射分析

利用动态光散射技术系统地研究了不同化合价的平衡离子氯化钠 (Na⁺)、氯化镁 (Mg²⁺)、三氯六氨络合钴 ([Co(NH₃)₆]³⁺) 和精胺 ([C₁₀N₄H₃₀]⁴⁺) 与DNA之间的相互作用. 实验结果显示, 当缓冲液中只包含Na⁺ 或Mg²⁺, 且浓度c≥ 5 mM时, DNA电泳迁移率之比约为2:1; 当缓冲液单独包含Na⁺或[Co(NH₃)₆]³⁺, 且浓度c≥ 5 mM时, DNA 的电泳迁移率之比约为4.5:1. 而当平衡离子的化合价为4时, 观察到DNA的电泳迁移率由负变正, 意味着发生了电荷反转. 在平衡离子浓度c<5 mM时, 随着离子浓度的增大, 迁移率之比逐渐增大. 对于一价或二价平衡离子情形, 实验结果与Manning的平衡离子凝聚理论的预言相符. 对于三价平衡离子, 实验结果与理论值有明显偏离. 而对于四价离子, 由于发生了DNA电荷逆转, 基于平均场的平衡离子凝聚理论失效. 另外, 通过原子力显微镜观察到当平衡离子的化合价大于等于3 时, DNA分子的构型发生变化. 因此, 自由溶液中的聚电解质的构型和离子关联效应在聚电解质迁移过程中起重要作用. 关键词： 电泳迁移率 平衡离子 动态光散射 DNA     

Phase transition behavior of hydrogen bonded liquid crystal (6BA)<Subscript>2</Subscript>-(BPy)<Subscript><Emphasis Type="Bold">x</Emphasis></Subscript> as studied by <Superscript>2</Superscript>H NMR

The thermal properties and the orientational order of hydrogen-bonded liquid crystals (6BA)₂-(BPy)_0.4 and (6BA)₂-(BPy)_0.3 (6BA: 4-n-hexylbenzoicacid, BPy: 4,4’-bipyridine) were investigated by DSC and ²H NMR. On cooling, isotropic liquid - liquid crystal phase transition temperatures were T _C= 409 and 405 K for (6BA)₂-(BPy)_0.4 and (6BA)₂-(BPy)_0.3, respectively. Thermal anomalies in the liquid crystal phase were observed at T _LC1= 402 and T _LC2= 375 K for (6BA)₂-(BPy)_0.4 and at T _LC1= 398 and T _LC2= 375 K for (6BA)₂-(BPy)_0.3. For (6BA)₂-(BPy)_0.4, only the smectic component was created above T _LC1. In addition, the nematic component was created below T _LC1. The nematic component gradually changed to the smectic component with decreasing temperature and only the smectic component was observed below T _LC2. For (6BA)₂-(BPy)_0.3, only the nematic component was created above T _LC2. The phase transition from the nematic phase to the smectic phase took place at around T _LC2.     

Causes of the Metamagnetism in a Disordered EuMn<Subscript>0.5</Subscript>Co<Subscript>0.5</Subscript>O<Subscript>3</Subscript> Perovskite

The magnetic properties of the EuMn_0.5Co_0.5O₃ perovskite synthesized under various conditions are studied in fields up to 140 kOe. The sample synthesized at T = 1500°C is shown to exhibit a metamagnetic phase transition, which is irreversible below T = 40 K, and the sample synthesized at T = 1200°C demonstrates the field dependence of magnetization that is typical of a ferromagnet. Both samples have T_C = 123 K and approximately the same magnetization in high magnetic fields. The metamagnetism is assumed to be related to a transition from a noncollinear ferromagnetic phase to a collinear phase, and the presence of clusters with ordered Co²⁺ and Mn⁴⁺ ions leads to ferromagnetism. The noncollinear phase is formed due to the competition between positive Co²⁺–Mn⁴⁺ and negative Mn⁴⁺–Mn⁴⁺ and Co²⁺–Co²⁺ interactions, which make almost the same contributions, and to the existence of a high magnetic anisotropy.     

Pressure Effects on Submicrosecond Phospholipid Dynamics Using a Long-Lived Fluorescence Probe

The effects of applied external hydrostatic pressure on submicrosecond lipid motions in DPPC⁴ bilayers have been examined using coronene (a long-lived planar fluorescent molecule) and DPH. Steady-state fluorescence emission anisotropy (EA) values () obtained for probe-labeled DPPC SUVs measured at different fixed temperatures above T _c as a function of increasing hydrostatic pressure reveal pressure-induced lipid phase transition profiles. For coronene-labeled samples, the observed lipid melt profiles are broad and shifted to higher midpoint EA pressure values (P _1/2) compared with corresponding DPH-labeled SUVs at the same temperature. The data suggest lipid motions occurring on the submicrosecond time scale, detected only by using a long-lived fluorescence probe, which occur well above the normally reported fluid–gel lipid phase transition. Slopes of the pressure-to-temperature equivalence plots (dP _1/2/dT = 39 bar/K) obtained for DPH-or coronene-labeled DPPC SUVs are identical within experimental error and reflect probe independence. For DPH, the slope of the P _1/2(T) plot provides the expected phase transition phospholipid volume change. However, intercept values (at P _1/2 = 1 bar) or apparent phase transition temperatures obtained from the equivalence plots for the two probes are not equal. Differences appear to arise due to the very disparate fluorescence lifetime values of the two probes, which result in rotational sensitivity of coronene to gel lipid volume fluctuations occurring during the extended time window provided by coronene fluorescence.     

Physical properties and phase diagram of the magnetic compound Cr<Subscript>0.26</Subscript>NbS<Subscript>1.74</Subscript> at high pressures

We report the results of a study of magnetic, electrical, and thermodynamic properties of a single crystal of the magnetic compound Cr_0.26NbS_1.74 at ambient and high pressures. Results of the measurements of magnetization as a function of temperature reveal the existence of a ferromagnetic phase transition in Cr_0.26NbS_1.74. The effective number of Bohr magnetons per Cr atom in the paramagnetic phase of Cr_0.26NbS_1.74 is µ_eff ≈ 4.6µB, which matches the literature data for Cr1/3NbS2. Similarly, the effective number of Bohr magnetons per Cr atom in the saturation fields is rather close in both substances and corresponds to the number of magnetons in the Cr⁺³ ion. In contrast to the stoichiometric compound, Cr_0.26NbS_1.74 does not show a metamagnetic transition, that indicates the lack of a magnetic soliton. A high-pressure phase diagram of the compound reveals the quantum phase transition at T = 0 and P ≈ 4.2 GPa and the triple point situated at T ≈ 20 K and P ≈ 4.2 GPa.     

Current-conducting properties of paper consisting of multiwall carbon nanotubes

Electrical conductivity σ(T) of the paper consisting of multiwalled carbon nanotubes (MWCNTs) is studied in the temperature range 4.2-295 K, and its magnetoresistivity ρ(B) at various temperatures in magnetic fields up to 9 T is analyzed. The temperature dependence of the paper electrical conductivity σ(T) exhibits two-dimensional quantum corrections to the conductivity below 10 K. The dependences of negative magnetoresistivity ρ(B) measured at various temperatures are used to estimate the wavefunction phase breakdown length L _φ of conduction electrons and to obtain the temperature dependence L _φ = constT ^?p/2, where p ≈ 1/3. Similar dependences of electrical conductivity σ(T), magnetoresistivity ρ(B), and phase breakdown length L _φ(T) are detected for the initial MWCNTs used to prepare the paper.     

Crystal structure and structural transition caused by charge-transfer phase transition for iron mixed-valence complex (n-C3H7)4N[FeFe(dto)3] (dto=C2O2S2)

(n-C₃H₇)₄N[Fe^IIFe^III(dto)₃] shows a new type of first order phase transition called charge-transfer phase transition around 120 K, where the charge transfer between Fe^II and Fe^III occurs reversibly. Recently, we have succeeded in obtaining single crystals of the title complex and determined the crystal structure at room temperature. Crystal data: space group P6₃, Z=2. Moreover, we have investigated the structural transition caused by the charge-transfer phase transition by means of powder X-ray diffraction measurement. When the temperature is decreased, the a-axis, which corresponds to the hexagonal ring size in two-dimensional honeycomb network structure of [Fe^IIFe^III(dto)₃]_∞, contracts by 0.1 Å at the charge-transfer transition temperature (T_CT), while the c-axis, perpendicular to the honeycomb network layer, elongates by 0.1 Å at T_CT. Consequently, when the temperature is decreased, the unit cell volume decreases without noticeable anomaly around T_CT, which is responsible for the quite small vibrational contribution to the entropy change, compared with usual spin crossover transition. Thus, the charge-transfer phase transition around 120 K for (n-C₃H₇)₄N[Fe^IIFe^III(dto)₃] is regarded as spin entropy driven phase transition.     

Temperature dependence of Mn2+ EPR in Sn2P2S6 near the phase transition

The X-band EPR spectrum of Mn²⁺ in Sn₂P₂S₆ was studied in the temperature rangeT=223–363 K. At room temperature the spin-Hamiltonian constants areg=2.00±0.01,B ₂ ⁰ =(163±3)·10^?4 cm^?1,B ₂ ² =(159±3)·10^?4 cm^?1,A=?(75±1)·10^?4 cm^?1. The effect of the invariance in temperature of the resonance magnetic fields in the narrow temperature rangeT=337–340 K and the model of the paramagnetic centre are discussed. According to EPR data a phase transition occurs atT=337 K. This transition from the paraelectric phase to the ferroelectric one is accompanied by a dramatic change in value of the spin-Hamiltonian constantB ₂ ⁰ .     

Magnetization of La- and Ce-doped CaMnO<Subscript>3</Subscript> manganite single crystals in a strong magnetic field

Studies of the magnetization curves of electron-doped single-crystal manganites Ca_{1 ? x} Ln _x MnO₃ (Ln = La³⁺, Ce⁴⁺; x ≤ 0.12) in strong pulsed magnetic fields of up to 350 kOe have revealed a metamagnetic transition in Ca_0.9Ce_0.1MnO₃ in the temperature range 77–190 K. The critical transition fields increase to ～350 kOe with the temperature decreasing to 100 K. The spin polarization is ～50% of the theoretical value. These results are interpreted as due to “melting” of the orbital/charge ordering below the temperature T _OO/CO = 185 K = T _N (of the C type AFM phase); this entails a decrease in the volume of the ordered phase with localized carriers and an increase in the volume of the ferromagnetic phase with delocalized carriers. The temperature and field dependences of the magnetization are used to compare two manganite systems in the region of the two-phase magnetic state.     

High-resolution spectroscopy of HoFe<Subscript>3</Subscript>(BO<Subscript>3</Subscript>)<Subscript>4</Subscript> crystal: a study of phase transitions

The transmission spectra of HoFe₃(BO₃) multiferroic single crystals are studied by optical Fourier-transform spectroscopy at temperatures of 1.7–423 K in polarized light in the spectral range 500–10 000 cm^–1 with a resolution up to 0.1 cm^–1. A new first-order structural phase transition close to the second-order transition is recorded at T_c = 360 K by the appearance of a new phonon mode at 976 cm^–1. The reasons for considerable differences in T_c for different samples of holmium ferroborate are discussed. By temperature variations in the spectra of the f–f transitions in the Ho³⁺ ion, we studied two magnetic phase transitions, namely, magnetic ordering into an easy-plane structure as a second-order phase transition at T_N = 39 K and spin reorientation from the ab plane to the c axis as a first-order phase transition at T_SR = 4.7 ± 0.2 K. It is shown that erbium impurity in a concentration of 1 at % decreases the spin-reorientation transition temperature to T_SR = 4.0 K.     

The big bang as a result of the first-order phase transition driven by a change of the scalar curvature in an expanding early Universe: The “hyperinflation” scenario

We suggest that the Big Bang could be a result of the first-order phase transition driven by a change in the scalar curvature of the 4D spacetime in an expanding cold Universe filled with a nonlinear scalar field φ and neutral matter with an equation of state p = νε (where p and ε are the pressure and energy density of the matter, respectively). We consider the Lagrangian of a scalar field with nonlinearity φ⁴ in a curved spacetime that, along with the term–ξR|φ|² quadratic in φ (where ξ is the interaction constant between the scalar and gravitational fields and R is the scalar curvature), contains the term ξRφ₀(φ + φ⁺) linear in φ, where φ₀ is the vacuum mean of the scalar field amplitude. As a consequence, the condition for the existence of extrema of the scalar-field potential energy is reduced to an equation cubic in φ. Provided that ν > 1/3, the scalar curvature R = [κ(3ν–1)ε–4Λ] (where κ and Λ are Einstein’s gravitational and cosmological constants, respectively) decreases with decreasing ε as the Universe expands, and a first-order phase transition in variable “external field” parameter proportional to R occurs at some critical value R _c < 0. Under certain conditions, the critical radius of the early Universe at the point of the first-order phase transition can reach an arbitrary large value, so that this scenario of unrestricted “inflation” of the Universe may be called “hyperinflation.” After the passage through the phase-transition point, the scalar-field potential energy should be rapidly released, which must lead to strong heating of the Universe, playing the role of the Big Bang.