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1.
磁化水、自来水和蒸馏水的拉曼散射研究   总被引:4,自引:0,他引:4  
对自来水、蒸馏水和磁化水进行了拉曼散射研究。发现:水经磁化后水分子结构未变化,氢键未断裂;磁化效果与磁化时间、磁场强度和磁化方式有关;静态磁化同样有效;水中离子在磁化过程中起重要作用。在离子水化理论基础上,对实验结果和磁化机理作了初步的解释和探讨。对磁水器的设计提出了建议。  相似文献   

2.
以一定速度流过适当强度的磁场后的水称为磁水或磁化水.磁化水在许多情况下呈现出一些值得注意的生物和非生物效应,在工农业、医学和日常生活各方面得到愈来愈广泛的应用,取得了一定的效果.关于磁化水所引起的各种效应的机理也有了多种理论和设想.但是,就目前来看,无论是磁化水的效应及其应用,还是磁化水效应的机理研究方面,都还处于实验和探索的阶段[1].因此,为了给磁化水的应用和进一步发展提供依据,有必要从多方面开展相应的研究工作.本文试图通过水在磁化前后布里渊散射频移的比较,为磁化水的一些应用和机理研究提供一定的依据. 由磁水…  相似文献   

3.
在磁场作用下水的特性的变化和它的变化机理   总被引:7,自引:0,他引:7  
我们研究了在磁场作用下水的光学性质和电学性质等的变化,实验发现它们的这些特性和未受磁场作用的水有重大改变特别是在红外光谱和拉曼光谱中的变化更加明显,这种现象就称为水的磁化。我们从水的中红外光谱得知在3000~3800 cm-1的范围内有奇特的六个峰值存在,从水分子结构和红外光谱的特性出发了解到它们分别代表了自由水分子的OH键的对称与反对称的振动,众多水分子通过氢键连接而成的线性链和环形链的OH键的对称与反对称振动,于是从这个实验我们看到了在这个水中存在有众多水分子结合成的环形氢键链的存在。我们用水分子的极化特性,一阶相变的特性和实验进一步证实了这些环形链的客观存在,根据质子或氢离子在氢键系统中传递理论得知在磁场的罗仑兹力作用下处于水中环形氢键链中质子能够进行传导产生环形电流.这些环形电流象一个分子电流或是个小磁体,它们能彼此相互作用或与外加磁场相互作用,从而改变了水分子的分布和结构状态,导致了水的一些特性的变化,这就是水的磁化的分子机理,我们用这个机理解释了我们从实验中所发现的磁处理过的水的特性如饱和效应和记忆效应等,因此这是非常有趣的实验和现象.  相似文献   

4.
利用有限元法进行数值模拟,研究了悬垂在针尖上的液滴在二阶模态下的振动情况.结果表明,悬垂液滴的固有振动频率与失重下自由液滴的固有振动频率间存在线性关系,该线性关系与液体的表面张力系数、液体的密度和针直径有关,与液体的黏度和"表面张力系数密度之比"无关;在声场的激励下,液滴的位移共振曲线与受迫振动的标准速度共振曲线在形状上一致,并且阻尼系数与黏度、表面张力系数、针直径呈正相关,而与密度、"表面张力系数与密度之比"呈负相关.最后以水为例将模拟结果与实验数据做了对比,两者符合得很好.  相似文献   

5.
氢键效应作为溶液中典型的微观特性直接影响溶液微观结构,并对物理和化学性质产生重要影响。对氢键作用的研究是水科学研究的重要突破口,也使得通过氢键研究水溶液性质成为一种极具优势的研究方法。通过测量不同浓度下的表面张力以及各体系拉曼光谱,研究二甲基亚砜/水、乙腈/水、丙酮/水三种具有典型氢键作用的二元溶液体系。研究了表面张力的变化规律和各体系中的氢键作用,讨论了溶液体系的微观结构变化,解释了氢键作用对表面张力的影响机制。  相似文献   

6.
关于磁化水性质的实验研究   总被引:4,自引:0,他引:4  
王信良  徐国勇 《物理》1992,21(2):113-114
水在磁场中流动或静止处理,其理化性质都会发生变化,但两种处理方式生产的磁化水性质有显著差异.磁化水的表面张力系数随磁处理时间的延长先增大、再减小、再增大.煮沸后冷却不影响磁水的作用.  相似文献   

7.
王彬  谢文楷 《物理学报》2007,56(12):7138-7146
利用磁化等离子体介电张量和纵向场分量法对任意大小轴向磁场中等离子体填充耦合腔慢波结构进行场分析,得到磁化等离子体填充电子注通道电磁波场分量的轴对称精确解.在此基础上,建立耦合腔分区模型、采用场匹配方法建立色散方程,并数值计算得出不同等离子体密度及磁场下的耦合腔色散曲线.对不同密度等离子体填充情况下的耦合腔色散特性、混合模式的形成机理以及等离子体空间电荷波进行了分析讨论. 关键词: 耦合腔慢波结构 等离子体 混合模式 色散特性  相似文献   

8.
宋冬灵  明亮  单昊  廖天河 《物理学报》2016,65(2):27102-027102
磁星是一类由磁场供能、强磁化的中子星,其内部磁场远高于电子的量子临界磁场.本文通过引入电子朗道能级的稳定性系数g_n,讨论了在磁星环境下电子的朗道能级的稳定性及其对电子费米能E_F(e)的影响;研究发现,磁场越强,电子的朗道能级越不稳定,最大的朗道能级级数n_(max)越小;朗道能级数n越大,能级稳定性系数g_n越小.根据朗道能级的稳定性系数g_n随磁场的增加而减小的要求,电子费米能表达式的磁场指数β必须是正数.通过引入Dirac-δ函数,推导出超强磁场下的简并的、相对论电子费米能的一般表达式,修正了E_F(e)的特解.新的特解给出磁场指数β=1/6;特解的适用范围ρ≥10~7g·cm~(-3),Bcr≤B≤10~(17)G.本文结果将有助于中子星内部弱相互作用过程(包括修正的URCA反应和电子俘获)和磁星磁热演化机理的研究.  相似文献   

9.
王兆军  吕国梁  朱春花  张军 《物理学报》2011,60(4):49702-049702
中子星内部的电子处于高度简并或完全简并的状态,电子磁矩(包括内禀磁矩和朗道反磁矩)的取向不是随机的,而是呈现出极强的磁化行为.考虑了磁化后的磁诱导方程要改写,改写后的方程添加了新的磁场生成项,更重要的改变是等效磁扩散系数变小了(顺磁情况),在临界情况(等效扩散系数等于零),磁场在磁生成项的作用下增加直到抑制机理出现,朗道反磁矩就是在这个时候变得越来越重要.磁场增加的最终结果使中子星局域磁场成为振荡的,对外看来有可能成为磁星. 关键词: 中子星 简并 磁化  相似文献   

10.
伍岳  肖立业 《物理学报》2022,(13):360-365
超导体在旋转过程中会在其内部产生磁场,称为London磁场.目前,包括London理论和G-L理论在内的多种理论都对London磁场的产生机理进行了解释.从本质上,这些理论解释大多认为旋转超导体最外层超导电子运动滞后并由此出现净余电流,而London磁场则是由旋转超导体表面的净余电流产生的.然而,关于旋转超导体最外层超导电子运动滞后的原因,目前仍没有明确的理论解释.本文通过对旋转系中带电粒子,以及旋转超导体中超导电子的贝里相位进行了理论分析,结果表明旋转状态下超导电子的贝里曲率与London磁场具有相同的表达形式,表明London磁场可视为A-B效应的逆效应,也即基于贝里相位的一种宏观量子效应.  相似文献   

11.
The properties of water and their changes under the action of a magnetic field were gathered by the spectrum techniques of infrared, Raman, visible, ultraviolet and X-ray lights, which may give an insight into molecular and atomic structures of water. It was found that some properties of water were changed, and a lot of new and strange phenomena were discovered after magnetization. Magnetized water really has magnetism, which has been verified by a peak shift of X-ray diffraction of magnetized water + Fe3O4 hybrid relative to that of pure water + Fe3O4 hybrid, that is a saturation and memory effect. The properties of infrared and ultraviolet absorptions, Raman scattering and X-ray diffraction of magnetized water were greatly changed relative to those of pure water; their strengths of peaks were all increased, the frequencies of some peaks did also shift, and some new peaks, for example, at 5198, 8050 and 9340 cm−1, occurred at 25°C after water was magnetized. In the meanwhile, the magnetized effects of water are related to the magnetized time, the intensity of an externally applied magnetic field, and the temperature of water, but they are not a linear relationship. The study also showed a lot of new and unusual properties of magnetized water, for example, the six peaks in 3000–3800 cm−1 in infrared absorption, the exponential increase of ultraviolet absorption of wave with the decreasing wavelength of light of 200–300 nm, the frequency-shifts of peaks, a strange irreversible effect in the increasing and decreasing processes, as well as a stronger peak of absorption occurring at 50°C, 70°C and 80°C, the existence of many models of motion from 85°C to 95°C in 8000–10000 cm−1, and so on. These results show that the molecular structure of water is very complicated, which needs further study. Furthermore, the macroscopic feature of mechanics, for instance, surface tension force of magnetized water, was also measured. Experiments discovered that the size in contact angles of magnetized water on the surface of hydrophobic materials decreases, thus the surface tension force of magnetized water decreases relative to that of pure water. It is seen from the above results that the clustering structure of hydrogen-bonded chains and polarization effects of water molecules are enhanced after magnetization. These results are helpful in revealing the mechanism of magnetization of water. Supported by the National Basic Research Program of China (Grant No. 2007CB936103)  相似文献   

12.
We explore the end point of the helical instability in a finite density, finite magnetic field background discussed by Kharzeev and Yee. The nonlinear solution is obtained and identified with the(magnetized) chiral density wave phase in the literature. We find there are two branches of solutions, which match the two unstable modes found before. At large chemical potential and magnetic field, the magnetized chiral density wave can be thermodynamically preferred over the chirally symmetric phase and chiral symmetry breaking phase. Interestingly, we find an exotic state with vanishing chemical potential at large magnetic field. We also attempt to clarify the role of anomalous charge in the holographic model.  相似文献   

13.
We have developed a simple numerical model for simulating domains as well as remanence and viscosity curves in the slow dynamics regime, for thin films characterized by perpendicular magnetization and irregular domain configurations due to strong disorder. The physical system is represented as constituted of identical switching units, described by proper switching field distributions and energy barrier laws for pinning and nucleation processes. The model also includes an effective field which accounts for magnetic forces proportional to magnetization, on average. Simulations of DCD curves show that when the reversal of magnetization is governed by pinning, the coercive field depends on the physical size of the film area on which the external field is applied. In the case of viscosity phenomena described by a linear energy barrier law associated with a single predominant reversal process (pinning or nucleation), universal viscosity curves can be generated by properly transforming the DCD curve of the system. We also demonstrate that a reduction of the maximum viscosity coefficient can coexist with a reduction of the energy barrier heights.  相似文献   

14.
In this paper we investigate the non-perturbative generation of an anomalous magnetic moment for massless fermions in the presence of an external magnetic field. In the context of massless QED in a magnetic field, we prove that the phenomenon of magnetic catalysis of chiral symmetry breaking, which has been associated in the literature with dynamical mass generation, is also responsible for the generation of a dynamical anomalous magnetic moment. As a consequence, the degenerate energy of electrons in Landau levels higher than zero exhibits Zeeman splitting. We explicitly report the splitting for the first Landau level and find the non-perturbative Lande g-factor and Bohr magneton. We anticipate that a dynamically generated anomalous magnetic moment will be a universal feature of theories with magnetic catalysis. Our findings can be important for condensed planar systems as graphene, as well as for highly magnetized dense systems as those forming the core of compact stars.  相似文献   

15.
李郝  杨鑫  张正平 《物理学报》2021,(7):215-222
为利用太赫兹波解决飞行器再入过程遇到的“黑障”问题,以散射矩阵方法为基础,分别以非均匀磁化等离子体的磁化方向、电子密度、外加磁场强度和碰撞频率为变量,研究了垂直入射情形下它们对太赫兹波传输行为的影响.结果表明:这些参数对太赫兹波传输性能影响明显,例如按某一方向改变磁化角度对左极化和右极化太赫兹波的传输功率有相反的影响;降低磁化强度能一定程度地避开等离子体对右极化波的吸收;而降低碰撞频率能缩小等离子体对右极化波的吸收频带.通过调整这些参数,有望在一定程度上缓解黑障现象.  相似文献   

16.
We report the first demonstration of magnetically induced transmission in an opaque magnetized plasma. Magnetically induced transmission in a plasma is a classical analog to the electromagnetically induced transparency in atomic systems. The transmission of radiation through an axially magnetized plasma is obtained by applying an additional one dimensional transverse spatial periodic magnetic field. The transverse-periodic magnetic field uncouples the right-hand electromagnetic wave from interacting with plasma electrons, rendering the plasma band-stop transparent. This provides means to control the extent of absorption of electromagnetic radiation in magnetized plasma.  相似文献   

17.
The properties of obliquely propagating ion-acoustic waves have been investigated in multi-ions magnetized plasma comprising of inertial, positively and negatively charged ion fluids, trapped electrons, and negatively charged stationary heavy ions. The propagation of the waves is oblique to the ambient magnetic field which is along the z-direction. Only fast type of modes exists in the linear regime. The reductive perturbation method was adopted to derive the Korteweg– de Vries (KdV) and Burger equations, as well as the solitary and shock wave solutions of the evolved equations, have been used to analyze the properties of the small but finite amplitude waves. The effects of the constituent plasma parameters, namely, the trapping effect of electrons, the electron degenerate temperature and the viscosity coefficient on the dynamics of the small amplitude solitary and shock waves have been examined. The influence of the magnetic field and the obliquity parameter on the propagation characteristics of ion-acoustic waves are discussed.  相似文献   

18.
段萍  李肸  鄂鹏  卿绍伟 《物理学报》2011,60(12):125203-125203
为进一步研究霍尔推进器壁面二次电子发射对推进器性能的影响,采用流体模型数值模拟了二次电子磁化效应的等离子体鞘层特性.得到二次电子磁化鞘层的玻姆判据.讨论了不同的磁场强度和方向、二次电子发射系数以及不同种类等离子体推进器的鞘层结构.结果表明:随器壁二次电子发射系数的增大,鞘层中粒子密度增加,器壁电势升高,鞘层厚度减小;鞘层电势及粒子密度随着磁场强度和方位角的增加而增加;而对于不同种类的等离子体,壁面电势和鞘层厚度也不同.这为霍尔推进器的磁安特性实验提供了理论解释. 关键词: 霍尔推进器 磁鞘 二次电子  相似文献   

19.
C P SINGH 《Pramana》2014,83(1):63-81
In this paper, we study anisotropic Bianchi-V Universe with magnetic field and bulk viscous fluid in string cosmology. Exact solutions of the field equations are obtained by using the equation of state (EoS) for a cloud of strings, and a relationship between bulk viscous coefficient and scalar expansion. The bulk viscous coefficient is assumed to be inversely proportional to the expansion scalar. It is interesting to examine the effects of magnetized bulk viscous string model in early and late stages of evolution of the Universe. This paper presents different string models like geometrical (Nambu string), Takabayasi (p-string) and Reddy string models by taking certain physical conditions. We discuss the nature of classical potential for viscous fluid with and without magnetic field. The presence of bulk viscosity stops the Universe from becoming empty in its future evolution. It is observed that the Universe expands with decelerated rate in the presence of viscous fluid with magnetic field whereas, it expands with marginal inflation in the presence of viscous fluid without magnetic field. The other physical and geometrical aspects of each string model are discussed in detail.  相似文献   

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