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Interconnected skyrmions in a nanowire structure: Micromagnetic simulations 纳米线结构中相互连接的天幕:微磁模拟
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-08 DOI: 10.1103/physrevb.110.174415
Taichi Nishitani, Syuta Honda, Hiroyoshi Itoh, Tomokatsu Ohsawa, Masaaki A. Tanaka
The magnetization dynamics of two skyrmions with antiparallel vortex rotations on a nanowire substrate were investigated using micromagnetic simulations. When positioned in proximity, the skyrmions exhibit attractive interactions that decrease their separation distance. This interaction leads to a magnetic energy transition, resulting in the fusion of the two skyrmions into a single connected entity. Applying a static magnetic field aligned with the magnetization direction of the skyrmion cores causes this connected structure to expand, increasing the distance between their cores. Conversely, exposing the connected skyrmions to a specific alternating magnetic field induces resonant oscillations in the core-to-core distance, with the resonance frequency decreasing as the field amplitude increases. The effective mass of the connected skyrmions at resonance is calculated using the resonance frequency. Notably, excessively high amplitudes can cause these oscillations to converge the skyrmions excessively, leading to their annihilation. In simulations involving both static and alternating magnetic fields, separation of the connected skyrmions was not observed. These findings have potential implications for the advancement of technologies utilizing skyrmion numbers for innovative applications.
利用微磁模拟研究了纳米线基底上两个具有反平行涡旋旋转的天元的磁化动力学。当两个天元靠近时,会产生吸引力相互作用,从而减小它们之间的距离。这种相互作用会导致磁能转换,从而使两个天元融合成一个相连的实体。施加与天球离子核心磁化方向一致的静态磁场会导致这种连接结构膨胀,从而增大它们核心之间的距离。相反,将相连的天体置于特定的交变磁场中,则会引起磁芯与磁芯间距离的共振振荡,共振频率随着磁场振幅的增大而降低。利用共振频率可以计算出共振时相连天元的有效质量。值得注意的是,过高的振幅会导致这些振荡过度收敛天元,从而导致天元湮灭。在涉及静态磁场和交变磁场的模拟中,没有观察到连接的天幕分离。这些发现对利用天幕数进行创新应用的技术进步具有潜在影响。
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引用次数: 0
Melting and transport properties ofAl2⁢O3at extreme conditions 极端条件下氧化铝的熔融和传输特性
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-08 DOI: 10.1103/physrevb.110.174107
Maitrayee Ghosh, S. X. Hu, Eric Blackman, Terry-Ann Suer, Shuai Zhang
The high-pressure temperature phase diagram and transport properties of materials are of broad interest to planetary sciences and high-energy-density sciences and applications. Alumina <mjx-container ctxtmenu_counter="133" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(10 0 (9 (3 1 2) 8 (6 4 5)) 7)"><mjx-mrow data-semantic-children="9" data-semantic-content="0,7" data-semantic- data-semantic-owns="0 9 7" data-semantic-role="leftright" data-semantic-speech="left parenthesis upper A l 2 normal upper O 3 right parenthesis" data-semantic-type="fenced"><mjx-mo data-semantic- data-semantic-operator="fenced" data-semantic-parent="10" data-semantic-role="open" data-semantic-type="fence" style="vertical-align: -0.02em;"><mjx-c>(</mjx-c></mjx-mo><mjx-mrow data-semantic-added="true" data-semantic-annotation="clearspeak:unit" data-semantic-children="3,6" data-semantic-content="8" data-semantic- data-semantic-owns="3 8 6" data-semantic-parent="10" data-semantic-role="implicit" data-semantic-type="infixop"><mjx-msub data-semantic-children="1,2" data-semantic- data-semantic-owns="1 2" data-semantic-parent="9" data-semantic-role="unknown" data-semantic-type="subscript"><mjx-mi data-semantic-font="normal" data-semantic- data-semantic-parent="3" data-semantic-role="unknown" data-semantic-type="identifier"><mjx-c noic="true" style="padding-top: 0.706em;">A</mjx-c><mjx-c style="padding-top: 0.706em;">l</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="3" data-semantic-role="integer" data-semantic-type="number" size="s"><mjx-c>2</mjx-c></mjx-mn></mjx-script></mjx-msub><mjx-mo data-semantic-added="true" data-semantic- data-semantic-operator="infixop,⁢" data-semantic-parent="9" data-semantic-role="multiplication" data-semantic-type="operator"><mjx-c>⁢</mjx-c></mjx-mo><mjx-msub data-semantic-children="4,5" data-semantic- data-semantic-owns="4 5" data-semantic-parent="9" data-semantic-role="latinletter" data-semantic-type="subscript" space="2"><mjx-mi data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="6" data-semantic-role="latinletter" data-semantic-type="identifier"><mjx-c>O</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="6" data-semantic-role="integer" data-semantic-type="number" size="s"><mjx-c>3</mjx-c></mjx-mn></mjx-script></mjx-msub></mjx-mrow><mjx-mo data-semantic- data-semantic-operator="fenced" data-semantic-parent="10" data-semantic-role="close" data-semantic-type="fence" style="vertical-align: -0.02em;"><mjx-c>)</mjx-c></mjx-mo></mjx-mrow></mjx-math></mjx-container> or its various forms (e.g., solutions with other oxides or silicates)
材料的高压温度相图和传输特性对行星科学和高能量密度科学及应用具有广泛的意义。氧化铝(Al2O3)或其各种形态(如与其他氧化物或硅酸盐的溶液)是地球和超地球地幔的重要成分,是动态压缩实验中的常用窗口材料,也是金刚石椭球实验中的标准压力校准器。它的结构和传输特性尤为重要,但在 100 GPa 以上的压力下还没有得到很好的研究。基于广泛的第一性原理分子动力学计算,我们获得了原子水平的结构差异见解,以及在压力为 130-1300GPa 和温度为 4000-20 000 K 时 Al2O3 在几种相中的导电性(𝜎dc)、导热性(𝜅)和反射性的精确结果。我们发现Al2O3的固态到液态变化伴随着绝缘体到半金属的转变,其𝜎dc和𝜅增强,这与其他硅酸盐和氧化物类似,可促进岩质行星内部深处磁场的产生。我们还发现,在 160 GPa 时,固态到固态的转变(从 Rh2O3(II) 到 CaIrO3)伴随着𝜎dc 和𝜅的微小变化,这与之前的预期相反,而另一种更高的压力相变(在 450 GPa 时从 CaIrO3 到 U2S3)则伴随着𝜎dc 和𝜅的增加。此外,我们还发现 Al2O3 中的氧空位可以增强传输特性,但与 MgSiO3 形成溶液对传输特性的影响不大,尤其是在固态时。
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引用次数: 0
On-demand population of Andreev levels by their ionization in the presence of Coulomb blockade 在库仑阻滞作用下,安德烈耶夫电离水平的按需增殖
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-08 DOI: 10.1103/physrevb.110.184508
Pavel D. Kurilovich, Vladislav D. Kurilovich, Aleksandr E. Svetogorov, Wolfgang Belzig, Michel H. Devoret, Leonid I. Glazman
A mechanism to deterministically prepare a nanowire Josephson junction in an odd parity state is proposed. The mechanism involves population of two Andreev levels by a resonant microwave drive breaking a Cooper pair, and a subsequent ionization of one of the levels by the same drive. Robust preparation of the odd state is allowed by a residual Coulomb repulsion in the junction. A similar resonant process can also be used to prepare the junction in the even state. Our theory explains a recent experiment [J. J. Wesdorp et al., Phys. Rev. Lett. 131, 117001 (2023)].
本文提出了一种以确定方式制备奇奇偶态纳米线约瑟夫森结的机制。该机制包括通过打破库珀对的共振微波驱动产生两个安德烈耶夫电平,以及随后通过相同的驱动使其中一个电平电离。结内残余的库仑斥力允许奇数态的稳健制备。类似的共振过程也可以用来制备偶态的结。我们的理论解释了最近的一项实验[J. J. Wesdorp 等人,Phys. Rev. Lett. 131, 117001 (2023)]。
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引用次数: 0
Electronic topological transitions in cadmium under pressure studied via theoretical and experimental x-ray absorption spectroscopy 通过理论和实验 X 射线吸收光谱研究压力下镉的电子拓扑转变
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-07 DOI: 10.1103/physrevb.110.205118
Jasmine K. Hinton, Daniel Schacher, Wonseok Lee, G. Alexander Smith, Emily Siska, Changyong Park, Paul B. Ellison, Scott K. Cushing, Craig P. Schwartz, Keith V. Lawler, Ashkan Salamat
An electronic topological transition (ETT) in cadmium below 1 GPa is investigated in situ with experimental x-ray absorption spectroscopy and projecting calculated core-valence excitons onto the band structure. These projections are a useful application of the Bethe-Salpeter equation approach that considers many-body effects. The method described herein can be used for systems that are otherwise difficult to probe in situ; therefore, it provides a generalizable approach to identifying and understanding ETTs under high pressure. Although pressure-induced ETTs are often probed using indirect structural responses, our own x-ray diffraction and Raman studies suggest a second-order structural transition around 3 GPa but are largely insensitive to or inconclusive for the previously studied ETT in this region.
通过实验 X 射线吸收光谱和将计算出的核价激子投射到能带结构上,对低于 1 GPa 的镉电子拓扑转变 (ETT) 进行了现场研究。这些投影是考虑多体效应的 Bethe-Salpeter 方程方法的有用应用。本文描述的方法可用于难以进行原位探测的系统;因此,它为识别和理解高压下的 ETT 提供了一种可推广的方法。虽然压力诱导的 ETT 通常使用间接结构响应进行探测,但我们自己的 X 射线衍射和拉曼研究表明,在 3 GPa 附近存在二阶结构转变,但对之前研究的该区域的 ETT 基本不敏感或没有结论。
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引用次数: 0
Excitation of fundamental multiple dark solitons from forced biharmonic oscillations in a magnonic active ring 磁子主动环中受迫双谐振荡激发基本多重暗孤子
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-07 DOI: 10.1103/physrevb.110.174413
Alexey B. Ustinov, Leonid S. Vedernikov, Ivan Y. Tatsenko, Andrey A. Stashkevich
This paper reports an experimental demonstration of efficient excitation of fundamental dark spin wave solitons on a magnonic active ring below self-oscillation threshold by means of a biharmonic technique. This technique is shown to be especially appropriate for implementing multisoliton regimes otherwise unattainable. Theoretical analysis has revealed a very important role played by the phase relations between individual harmonics generated nonlinearly in the process of the formation of multiple solitons. The proposed ad hoc approach making use of the inverse Fourier transform has allowed us to elucidate the mechanisms underlying the formation of investigated nonlinear waveforms from their power spectra.
本文报告了通过双谐波技术在自振阈值以下的磁性有源环上高效激发基本暗自旋波孤子的实验演示。实验表明,这种技术特别适用于实现多孤子机制,否则将无法实现。理论分析表明,在形成多孤子的过程中,非线性产生的各个谐波之间的相位关系发挥着非常重要的作用。利用反傅立叶变换的特别方法,我们可以从功率谱中阐明所研究的非线性波形的形成机制。
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引用次数: 0
Limitations of Caldeira-Leggett model for description of phase transitions in superconducting circuits 卡尔代拉-莱格特模型在描述超导电路相变方面的局限性
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-07 DOI: 10.1103/physrevb.110.184505
O. Kashuba, R.-P. Riwar
The inherent complexity of system-bath interactions often requires making critical approximations, which we here show to have a radical influence on the renormalization group flow and the resulting phase diagram. Specifically, for the Caldeira-Leggett model Schmid and Bulgadaev (SB) predicted a phase transition, whose experimental verification in resistive superconducting circuits is currently hotly debated. For normal metal and Josephson junction array resistors, we show that the mapping to Caldeira-Leggett is only exact when applying approximations which decompactify the superconducting phase. We show that there exist treatments that retain phase compactness, which immediately lead to a phase diagram depending on four instead of two parameters. While we still find an SB-like transition in the transmon regime, the critical parameter is controlled exclusively by the capacitive coupling. In contrast, the Cooper pair box maps to the anisotropic Kondo model, where a pseudoferromagnetic phase is not allowed for regular electrostatic interactions.
系统-浴相互作用的固有复杂性往往要求进行临界近似,我们在此表明,临界近似对重正化群流和由此产生的相图具有根本性的影响。具体来说,对于卡尔代拉-莱格特模型,施密德和布尔加达耶夫(SB)预言了一种相变,而这种相变在电阻超导电路中的实验验证目前正引起激烈争论。对于普通金属和约瑟夫森结阵列电阻器,我们的研究表明,只有在采用近似方法对超导阶段进行解压缩时,卡尔代拉-莱格特的映射才是精确的。我们的研究表明,存在保留相紧凑性的处理方法,这些方法会立即产生一个取决于四个而非两个参数的相图。虽然我们仍能在跨导机制中发现类似于 SB 的转变,但临界参数完全由电容耦合控制。相比之下,库珀对箱映射到各向异性的近藤模型,在该模型中,常规静电相互作用不允许出现伪铁磁相。
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引用次数: 0
Tunable surface electron gas and effect of phonons inSr2⁢CuO3: A first-principles study Sr2CuO3中的可调谐表面电子气和声子效应:第一原理研究
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-07 DOI: 10.1103/physrevb.110.195121
Xin Du, Hui-Hui He, Xiao-Xiao Man, Zhong-Yi Lu, Kai Liu
While the conducting <mjx-container ctxtmenu_counter="27" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(2 0 1)"><mjx-msub data-semantic-children="0,1" data-semantic- data-semantic-owns="0 1" data-semantic-role="unknown" data-semantic-speech="upper C u upper O 2" data-semantic-type="subscript"><mjx-mi data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="unknown" data-semantic-type="identifier"><mjx-c noic="true" style="padding-top: 0.669em;">C</mjx-c><mjx-c noic="true" style="padding-top: 0.669em;">u</mjx-c><mjx-c style="padding-top: 0.669em;">O</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="integer" data-semantic-type="number" size="s"><mjx-c>2</mjx-c></mjx-mn></mjx-script></mjx-msub></mjx-math></mjx-container> planes in cuprate superconductors have been widely recognized as a crucial component in producing high superconducting <mjx-container ctxtmenu_counter="28" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(2 0 1)"><mjx-msub data-semantic-children="0,1" data-semantic- data-semantic-owns="0 1" data-semantic-role="latinletter" data-semantic-speech="upper T Subscript c" data-semantic-type="subscript"><mjx-mi data-semantic-annotation="clearspeak:simple" data-semantic-font="italic" data-semantic- data-semantic-parent="2" data-semantic-role="latinletter" data-semantic-type="identifier"><mjx-c>𝑇</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em; margin-left: -0.048em;"><mjx-mtext data-semantic-annotation="clearspeak:unit" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="unknown" data-semantic-type="text" size="s" style='font-family: MJX-STX-ZERO, "Helvetica Neue", Helvetica, Roboto, Arial, sans-serif;'><mjx-utext style="font-size: 90.6%; padding: 0.828em 0px 0.221em; width: 4px;" variant="-explicitFont">c</mjx-utext></mjx-mtext></mjx-script></mjx-msub></mjx-math></mjx-container>, recent experimental and theoretical studies on <mjx-container ctxtmenu_counter="29" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(17 (5 0 (4 1 2 3)) 15 (8 6 7) 16 (14 9 (13 10 11 12)))"><mjx-mrow data-semantic-annotation="clearspeak:unit" data-semantic-children="5,8,14" data-semantic-content="15,16" data-semantic- data-semantic-owns="5 15 8 16 14" data-semantic-role="implicit" data-semantic-speech="upper B a Subscript 2 minus x Baseline upper S r Subscript x Baseline upper C u upper O Subscript 3 plus delta" data-semantic-type="infixop"><mjx-msub data-semantic-children="0,4" data-semantic- data-semantic-ow
尽管人们普遍认为铜氧化物超导体中的导电 CuO2 平面是产生高超导𝑇c 的关键组成部分,但最近对 Ba2-𝑥Sr𝑥CuO3+𝛿 的实验和理论研究也引起了人们对一维(1D)铜氧化物中 Cu-O 链重要性的关注。为了更好地理解含有 Cu-O 链的铜氧化物,我们基于自旋极化密度泛函理论计算研究了 Sr2CuO3 块体和薄膜的电子、磁性和声子特性。我们首先再现了块体 Sr2CuO3 的杯状母体化合物的典型莫特绝缘体特征,然后构建了表面暴露有 Cu-O 链的 Sr2CuO3 薄膜,直接研究其特性。与绝缘体相不同,Sr2CuO3 表面显示出有趣的金属特性。进一步的电子结构计算显示,表面 Sr 原子间存在自旋极化电子气,这种电子气强烈依赖于 Cu 自旋链间耦合。此外,涉及链内和链外 O 原子振动的声子模式能在 Sr2CuO3 薄膜表层诱发强烈的电荷和自旋波动,这表明显著的多自由度耦合可能对一维铜氧化物的超导性非常重要。我们的研究提供了有关 Sr2CuO3 中 Cu-O 链性质的全面观点,有助于全面了解一维铜氧化物超导体。
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引用次数: 0
Magnetism and field-induced effects in the𝑆=52honeycomb lattice antiferromagnetFeP3⁢SiO11 𝑆=52蜂巢晶格反铁磁体FeP3SiO11的磁性和场诱导效应
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-07 DOI: 10.1103/physrevb.110.184402
J. Khatua, M. Gomilšek, Kwang-Yong Choi, P. Khuntia
Quantum magnets based on honeycomb lattices with a low coordination number offer a viable ground to realize exotic emergent quantum excitations and phenomena arising from the interplay between competing magnetic interactions, spin correlations, and spatial anisotropy. However, unlike their low-spin analogs, high-spin honeycomb lattice antiferromagnets have remained comparatively less explored in the context of capturing the classical limits of quantum phenomena. Herein, we report the crystal structure, magnetic susceptibility, specific heat, and electron spin resonance (ESR) measurements, complemented by <i>ab initio</i> density functional theory (DFT) calculations, on polycrystalline samples of <mjx-container ctxtmenu_counter="81" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(7 (2 0 1) 6 (5 3 4))"><mjx-mrow data-semantic-annotation="clearspeak:unit" data-semantic-children="2,5" data-semantic-content="6" data-semantic- data-semantic-owns="2 6 5" data-semantic-role="implicit" data-semantic-speech="upper F e upper P 3 upper S i upper O 11" data-semantic-type="infixop"><mjx-msub data-semantic-children="0,1" data-semantic- data-semantic-owns="0 1" data-semantic-parent="7" data-semantic-role="unknown" data-semantic-type="subscript"><mjx-mi data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="unknown" data-semantic-type="identifier"><mjx-c noic="true" style="padding-top: 0.657em;">F</mjx-c><mjx-c noic="true" style="padding-top: 0.657em;">e</mjx-c><mjx-c style="padding-top: 0.657em;">P</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="integer" data-semantic-type="number" size="s"><mjx-c>3</mjx-c></mjx-mn></mjx-script></mjx-msub><mjx-mo data-semantic-added="true" data-semantic- data-semantic-operator="infixop,⁢" data-semantic-parent="7" data-semantic-role="multiplication" data-semantic-type="operator"><mjx-c>⁢</mjx-c></mjx-mo><mjx-msub data-semantic-children="3,4" data-semantic- data-semantic-owns="3 4" data-semantic-parent="7" data-semantic-role="unknown" data-semantic-type="subscript" space="2"><mjx-mi data-semantic-font="normal" data-semantic- data-semantic-parent="5" data-semantic-role="unknown" data-semantic-type="identifier"><mjx-c noic="true" style="padding-top: 0.673em;">S</mjx-c><mjx-c noic="true" style="padding-top: 0.673em;">i</mjx-c><mjx-c style="padding-top: 0.673em;">O</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="5" data-semantic-role="integer" data-semantic-type="number" size="s"><mjx-c noic="true" style="padding-top: 0.639em;">1</mjx-c><mjx-c style="padding-top: 0.639em;">1</mjx-c></mjx-mn></mjx-script></mjx-msu
基于低配位数蜂巢晶格的量子磁体为实现奇异的新兴量子激元以及竞争磁相互作用、自旋相关性和空间各向异性之间的相互作用所产生的现象提供了一个可行的基础。然而,与低自旋类似物不同,高自旋蜂巢晶格反铁磁体在捕捉量子现象的经典极限方面的探索仍然相对较少。在此,我们报告了对 FeP3SiO11 多晶样品的晶体结构、磁感应强度、比热和电子自旋共振(ESR)测量结果,并辅以原子序数密度泛函理论(DFT)计算,其中 Fe3+ 离子装饰了近乎完美的𝑆=52 蜂窝晶格,组成原子之间没有任何位点紊乱。在 150 K 以上,观察到反铁磁性韦斯温度𝜃CW=-12K,这与 DFT 计算一致,表明存在较强的平面内近邻和较弱的平面间远邻交换相互作用。在 𝑇𝑁=3.5K 时,比热和磁感应强度出现异常,这表明在零场中存在长程有序基态。在𝑇𝑁以上,ESR 证明了短程自旋相关性和不饱和磁熵,而在𝑇𝑁以下,通过幂律比热可以看到非常规激发。在更高的外加磁场中,𝑇𝑁逐渐被抑制,在𝜇0𝐻c2=5.6T时降至零。在 𝜇0𝐻c2 以上,间隙磁子激发导致的比热出现了一个宽广的最大值,这表明在这种蜂巢晶格反铁磁体中出现了一个有趣的近极化态,由无序态包裹。
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引用次数: 0
Ferromagnetic ferroelectricity due to the Kugel-Khomskii mechanism of orbital ordering assisted by atomic Hund's second rule effects 库格尔-霍姆斯基轨道有序机制在原子亨德第二规则效应辅助下产生的铁磁铁电性
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-07 DOI: 10.1103/physrevb.110.205116
I. V. Solovyev, R. Ono, S. A. Nikolaev
The exchange interactions in insulators depend on the orbital state of magnetic ions, obeying certain phenomenological principles, known as Goodenough-Kanamori-Anderson rules. Particularly, the ferro order of alike orbitals tends to stabilize antiferromagnetic interactions, while the antiferro order of unlike orbitals favors ferromagnetic interactions. The Kugel-Khomskii theory provides a universal view on such coupling between spin and orbital degrees of freedom, based on the superexchange processes: namely, for a given magnetic order, the occupied orbitals tend to arrange in a way to further minimize the exchange energy. Then, if two magnetic sites are connected by the spatial inversion, the antiferro orbital order should lead to the ferromagnetic coupling <i>and</i> break the inversion symmetry. This constitutes the basic idea of our work, which provides a pathway for designing ferromagnetic ferroelectrics: the rare but fundamentally and practically important multiferroic materials. After illustrating the basic idea on toy-model examples, we propose that such behavior can be indeed realized in the van der Waals ferromagnet <mjx-container ctxtmenu_counter="652" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(2 0 1)"><mjx-msub data-semantic-children="0,1" data-semantic- data-semantic-owns="0 1" data-semantic-role="unknown" data-semantic-speech="upper V upper I 3" data-semantic-type="subscript"><mjx-mi data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="unknown" data-semantic-type="identifier"><mjx-c noic="true" style="padding-top: 0.657em;">V</mjx-c><mjx-c style="padding-top: 0.657em;">I</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="integer" data-semantic-type="number" size="s"><mjx-c>3</mjx-c></mjx-mn></mjx-script></mjx-msub></mjx-math></mjx-container>, employing for this analysis the realistic model derived from first-principles calculations for magnetic <mjx-container ctxtmenu_counter="653" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(3 0 2 1)"><mjx-mrow data-semantic-annotation="clearspeak:simple;clearspeak:unit" data-semantic-children="0,1" data-semantic-content="2" data-semantic- data-semantic-owns="0 2 1" data-semantic-role="implicit" data-semantic-speech="3 d" data-semantic-type="infixop"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="3" data-semantic-role="integer" data-semantic-type="number"><mjx-c>3</mjx-c></mjx-mn><mjx-mo data-semantic-added="true" data-semantic- data-semantic-operator="infixop,⁢" data-semantic-parent="3" data-semantic-role="multiplicat
绝缘体中的交换相互作用取决于磁性离子的轨道状态,服从某些现象学原理,即古德诺-卡纳莫里-安德森规则。特别是,相同轨道的铁阶倾向于稳定反铁磁相互作用,而不相同轨道的反铁阶则有利于铁磁相互作用。库格尔-霍姆斯基(Kugel-Khomskii)理论以超交换过程为基础,为自旋和轨道自由度之间的这种耦合提供了一种普遍的观点:即对于给定的磁序,被占据的轨道倾向于以进一步最小化交换能的方式排列。那么,如果两个磁性位点通过空间反转相连,反铁氧体轨道阶应导致铁磁耦合并打破反转对称性。这就是我们工作的基本思想,它为设计铁磁性铁电体提供了一条途径:这是一种罕见但具有重要基础和实际意义的多铁电体材料。在用玩具模型举例说明基本思想之后,我们提出这种行为确实可以在范德瓦耳斯铁磁体 VI3 中实现,并在分析中采用了根据磁性 3𝑑 带的第一原理计算得出的现实模型。我们认为,造成亨德第二规则的原子内相互作用与晶体场相反,倾向于恢复 VI3 中离子𝑑2 态的轨道退变性,从而为激活轨道有序的库格尔-霍姆斯基机制提供了必要的灵活性。在蜂巢晶格中,这种轨道排序打破了反转对称性,稳定了铁磁-铁电基态。对称性的打破导致了磁化的倾斜,而磁化可进一步受磁场控制,从而产生巨大的电极化变化。
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引用次数: 0
Neural network enabled molecular dynamics study ofHfO2phase transitions 神经网络支持的二氧化铪相变分子动力学研究
IF 3.7 2区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-11-07 DOI: 10.1103/physrevb.110.174105
Sebastian Bichelmaier, Jesús Carrete, Georg K. H. Madsen
The advances of machine-learned force fields have opened up molecular dynamics (MD) simulations for compounds for which <i>ab initio</i> MD is too resource intensive and phenomena for which classical force fields are insufficient. Here we describe a neural-network force field parametrized to reproduce the <mjx-container ctxtmenu_counter="23" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(5 (2 0 1) 4 3)"><mjx-mrow data-semantic-annotation="clearspeak:unit" data-semantic-children="2,3" data-semantic-content="4" data-semantic- data-semantic-owns="2 4 3" data-semantic-role="implicit" data-semantic-speech="normal r squared upper S upper C upper A upper N" data-semantic-type="infixop"><mjx-msup data-semantic-children="0,1" data-semantic- data-semantic-owns="0 1" data-semantic-parent="5" data-semantic-role="latinletter" data-semantic-type="superscript"><mjx-mrow><mjx-mi data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="latinletter" data-semantic-type="identifier"><mjx-c>r</mjx-c></mjx-mi></mjx-mrow><mjx-script style="vertical-align: 0.363em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="integer" data-semantic-type="number" size="s"><mjx-c>2</mjx-c></mjx-mn></mjx-script></mjx-msup><mjx-mo data-semantic-added="true" data-semantic- data-semantic-operator="infixop,⁢" data-semantic-parent="5" data-semantic-role="multiplication" data-semantic-type="operator"><mjx-c>⁢</mjx-c></mjx-mo><mjx-mi data-semantic-font="normal" data-semantic- data-semantic-parent="5" data-semantic-role="unknown" data-semantic-type="identifier" space="2"><mjx-c noic="true" style="padding-top: 0.669em;">S</mjx-c><mjx-c noic="true" style="padding-top: 0.669em;">C</mjx-c><mjx-c noic="true" style="padding-top: 0.669em;">A</mjx-c><mjx-c style="padding-top: 0.669em;">N</mjx-c></mjx-mi></mjx-mrow></mjx-math></mjx-container> potential energy landscape of <mjx-container ctxtmenu_counter="24" ctxtmenu_oldtabindex="1" jax="CHTML" overflow="linebreak" role="tree" sre-explorer- style="font-size: 100.7%;" tabindex="0"><mjx-math data-semantic-structure="(2 0 1)"><mjx-msub data-semantic-children="0,1" data-semantic- data-semantic-owns="0 1" data-semantic-role="unknown" data-semantic-speech="upper H f upper O 2" data-semantic-type="subscript"><mjx-mi data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="unknown" data-semantic-type="identifier"><mjx-c noic="true" style="padding-top: 0.713em;">H</mjx-c><mjx-c noic="true" style="padding-top: 0.713em;">f</mjx-c><mjx-c style="padding-top: 0.713em;">O</mjx-c></mjx-mi><mjx-script style="vertical-align: -0.15em;"><mjx-mn data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-sema
机器学习力场的进步为分子动力学(MD)模拟开辟了新的途径,可以模拟那些因ab initio MD过于耗费资源而无法进行的化合物,以及那些经典力场无法充分模拟的现象。在此,我们描述了一种神经网络力场,其参数化的目的是重现 HfO2 的 r2SCAN 势能图。基于等温-等压(𝑁𝑃𝑇)集合的自动可微分实现,以及灵活的单元波动,我们研究了 HfO2 的相空间。我们发现晶格常数和 X 射线衍射实验数据具有极佳的预测能力。在 2000 K 左右的温度下,可以清楚地看到单斜相的转变,这与现有的实验数据和以前的计算结果一致。晶格常数的另一个突然变化发生在 3000 K 左右。虽然由此产生的晶格常数更接近立方体,但它们表现出很小的四方畸变,而且体积没有相关变化。我们的研究表明,这种高温结构与现有的高温衍射数据一致。
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引用次数: 0
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Physical Review B
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