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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Phys.</journal-id>
<journal-title>Frontiers in Physics</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Phys.</abbrev-journal-title>
<issn pub-type="epub">2296-424X</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">1019881</article-id>
<article-id pub-id-type="doi">10.3389/fphy.2022.1019881</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Physics</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Magnetic anisotropy-controlled vortex nano-oscillator for neuromorphic computing</article-title>
<alt-title alt-title-type="left-running-head">Yun et al.</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/fphy.2022.1019881">10.3389/fphy.2022.1019881</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Yun</surname>
<given-names>Chao</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<xref ref-type="fn" rid="fn1">
<sup>&#x2020;</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Wu</surname>
<given-names>Yu</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="fn" rid="fn1">
<sup>&#x2020;</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Liang</surname>
<given-names>Zhongyu</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1992697/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Yang</surname>
<given-names>Wenyun</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Du</surname>
<given-names>Honglin</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1992691/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Liu</surname>
<given-names>Shunquan</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Han</surname>
<given-names>Jingzhi</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Hou</surname>
<given-names>Yanglong</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/89210/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Yang</surname>
<given-names>Jinbo</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Luo</surname>
<given-names>Zhaochu</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1635778/overview"/>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>State Key Laboratory of Artificial Microstructure and Mesoscopic Physics</institution>, <institution>School of Physics</institution>, <institution>Peking University</institution>, <addr-line>Beijing</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Institute of Condensed Matter Physics and Materials</institution>, <institution>School of Physics</institution>, <institution>Peking University</institution>, <addr-line>Beijing</addr-line>, <country>China</country>
</aff>
<aff id="aff3">
<sup>3</sup>
<institution>School of Materials Science and Engineering</institution>, <institution>Peking University</institution>, <addr-line>Beijing</addr-line>, <country>China</country>
</aff>
<aff id="aff4">
<sup>4</sup>
<institution>Beijing Key Laboratory for Magnetoelectric Materials and Devices</institution>, <addr-line>Beijing</addr-line>, <country>China</country>
</aff>
<aff id="aff5">
<sup>5</sup>
<institution>Collaborative Innovation Center of Quantum Matter</institution>, <addr-line>Beijing</addr-line>, <country>China</country>
</aff>
<aff id="aff6">
<sup>6</sup>
<institution>Peking University Yangtze Delta Institute of Optoelectronics</institution>, <addr-line>Nantong</addr-line>, <country>China</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1468330/overview">Tao Yu</ext-link>, Huazhong University of Science and Technology, China</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1279210/overview">Na Lei</ext-link>, Beihang University, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1970186/overview">Weichao Yu</ext-link>, Fudan University, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1972970/overview">Yong-Chang Lau</ext-link>, Institute of Physics (CAS), China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Chao Yun, <email>yunchao@pku.edu.cn</email>; Zhaochu Luo, <email>zhaochu.luo@pku.edu.cn</email>
</corresp>
<fn fn-type="equal" id="fn1">
<p>
<sup>&#x2020;</sup>These authors have contributed equally to this work</p>
</fn>
<fn fn-type="other">
<p>This article was submitted to Condensed Matter Physics, a section of the journal Frontiers in Physics</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>17</day>
<month>10</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="collection">
<year>2022</year>
</pub-date>
<volume>10</volume>
<elocation-id>1019881</elocation-id>
<history>
<date date-type="received">
<day>15</day>
<month>08</month>
<year>2022</year>
</date>
<date date-type="accepted">
<day>29</day>
<month>09</month>
<year>2022</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2022 Yun, Wu, Liang, Yang, Du, Liu, Han, Hou, Yang and Luo.</copyright-statement>
<copyright-year>2022</copyright-year>
<copyright-holder>Yun, Wu, Liang, Yang, Du, Liu, Han, Hou, Yang and Luo</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>Chiral magnetic vortex has shown great potential for high-density magnetic storage, modern telecommunication and computation devices, thanks to its topological stability and rich dynamic behaviours. Particularly, the synchronization of magnetic vortex nano-oscillators leads to the emergence of fascinating collective phenomena used for microwave generator and neuromorphic computing. In this work, by means of micromagnetic simulations, we create stable chiral magnetic vortices by exploiting the chiral coupling principle and study the gyrotropic motion of the vortex core under spin-transfer torques. The gyrotropic oscillation frequency can be tuned by injecting spin-polarised current as well as the change of the magnetic anisotropy in the vortex area, resulting from the modification of the vortex confine potential and the size of the vortex core. Two vortex nano-oscillators can be synchronized wherein the synchronization state can be modulated by the spin-polarised current and the magnetic anisotropy. Moreover, we demonstrate that the magnetic anisotropy can modify the synchronization patterns when integrating six vortices into an oscillator network, making it potentially serve as an oscillator-based neural network. Our work provides a new route to constructing a flexible oscillator network for neuromorphic computing hardware.</p>
</abstract>
<kwd-group>
<kwd>magnetic vortex oscillator</kwd>
<kwd>chiral coupling</kwd>
<kwd>magnetic anisotropy</kwd>
<kwd>synchronization</kwd>
<kwd>neuromorphic computing</kwd>
</kwd-group>
<contract-num rid="cn001">51731001 11975035 11805006 11675006 52027801 52111530236 52201287 52271160</contract-num>
<contract-num rid="cn002">2021YFB3500300</contract-num>
<contract-sponsor id="cn001">National Natural Science Foundation of China<named-content content-type="fundref-id">10.13039/501100001809</named-content>
</contract-sponsor>
<contract-sponsor id="cn002">National Key Research and Development Program of China<named-content content-type="fundref-id">10.13039/501100012166</named-content>
</contract-sponsor>
</article-meta>
</front>
<body>
<sec id="s1">
<title>Introduction</title>
<p>Polar vortex magnetic texture has nonlinear spin swirling alignment with nontrivial topology. The unique magnetic configuration occurs as a result of the energy competition between various interactions, including magnetic exchange interaction, dipolar interaction, and importantly, the antisymmetric Dzyaloshinskii-Moriya interaction (DMI) [<xref ref-type="bibr" rid="B1">1</xref>&#x2013;<xref ref-type="bibr" rid="B3">3</xref>]. The magnetic vortex, usually with nanoscale dimensions, can have superior stability thanks to the topological protection, and is less prone to defect pinning, which enables the efficient displacement with a low electric current [<xref ref-type="bibr" rid="B4">4</xref>]. The driving current can be as low as 10<sup>6</sup> A/m<sup>2</sup> which is five orders of magnitude lower than the current required for domain-wall motion [<xref ref-type="bibr" rid="B5">5</xref>]. These properties help to realize excellent spintronic devices for high-density data storage, non-volatile logic operation and nanoscale microwave generator [<xref ref-type="bibr" rid="B6">6</xref>, <xref ref-type="bibr" rid="B7">7</xref>]. Moreover, the particle-like characteristic of the magnetic vortex enables the potential application as magnetic synapses [<xref ref-type="bibr" rid="B8">8</xref>]. The local manipulation of creation, motion and deletion of magnetic vortices have been applied to mimic the potentiation and depression behaviours of biological synapses, thus showing great promises for artificial neural networks [<xref ref-type="bibr" rid="B9">9</xref>&#x2013;<xref ref-type="bibr" rid="B11">11</xref>].</p>
<p>The magnetic vortex has rich dynamic behaviours with a broad frequency range from 0.1&#x2013;100&#xa0;GHz [<xref ref-type="bibr" rid="B12">12</xref>&#x2013;<xref ref-type="bibr" rid="B14">14</xref>]. Response dynamics of magnetic vortices under external fields can be classified into two modes: breath mode and gyration mode. On one hand, the dynamical shrinkage/expansion of the vortex texture can be manipulated by perpendicular a. c. Magnetic field [<xref ref-type="bibr" rid="B15">15</xref>, <xref ref-type="bibr" rid="B16">16</xref>], a. c. Current [<xref ref-type="bibr" rid="B17">17</xref>], or spin-orbital torques [<xref ref-type="bibr" rid="B17">17</xref>, <xref ref-type="bibr" rid="B18">18</xref>]. On the other hand, since the inherent dynamics of magnetic vortex is gyrotropic, self-sustained magnetic oscillation can be obtained <italic>via</italic> spin transfer torques that compensate the intrinsic magnetic damping, which suggests great potential for applications in spin-torque nano-oscillators [<xref ref-type="bibr" rid="B13">13</xref>, <xref ref-type="bibr" rid="B14">14</xref>, <xref ref-type="bibr" rid="B19">19</xref>, <xref ref-type="bibr" rid="B20">20</xref>]. The radio-frequency oscillation gives an electric power output in the pico-watt to nano-watt range [<xref ref-type="bibr" rid="B21">21</xref>, <xref ref-type="bibr" rid="B22">22</xref>], which can be further enhanced by placing the nano-oscillators in arrays or networks. In such nano-oscillators, the interactions between the individual vortex nano-oscillator result in the phase locking, with all nano-oscillators oscillating in a common frequency, termed as synchronization [<xref ref-type="bibr" rid="B23">23</xref>]. Synchronization between magnetic nano-oscillators usually occurs as a result of exchange interactions in close proximity [<xref ref-type="bibr" rid="B24">24</xref>, <xref ref-type="bibr" rid="B25">25</xref>], long-range dipolar coupling [<xref ref-type="bibr" rid="B14">14</xref>, <xref ref-type="bibr" rid="B23">23</xref>, <xref ref-type="bibr" rid="B26">26</xref>, <xref ref-type="bibr" rid="B27">27</xref>], propagating spin waves [<xref ref-type="bibr" rid="B28">28</xref>] or emitted power through microwave currents [<xref ref-type="bibr" rid="B29">29</xref>]. The phase locking can act as an &#x2018;anchor&#x2019; to stablise the self-sustained oscillations that is crucial for radio-frequency applications. More importantly, the nonlinear dynamics of synchronized magnetic nano-oscillators enables the development of neuromorphic computing architectures, particularly associative memories with information encoding in the individual phases of large scale arrays of interacting nano-oscillators [<xref ref-type="bibr" rid="B14">14</xref>]. Intercorrelated magnetic vortex oscillators provide extended possibilities to embrace the dynamical nature of the brains through interactions [<xref ref-type="bibr" rid="B14">14</xref>, <xref ref-type="bibr" rid="B30">30</xref>&#x2013;<xref ref-type="bibr" rid="B32">32</xref>], aiming to solve complex problems efficiently within small networks. The synchronization can also mimic the periodic spiking and synaptic communication of neurons. A coupled network of spin-torque nano-oscillators can learn to perform computational tasks through synchronization, for applications in speech, pattern recognition, where each synchronization pattern can be used directly as an output for the neural networks [<xref ref-type="bibr" rid="B31">31</xref>, <xref ref-type="bibr" rid="B33">33</xref>]. Therefore, finding an efficient way to manipulate the synchronization is crucial for magnetic vortex oscillator-based neuromorphic computing devices.</p>
<p>The nonlinear dynamics of magnetic vortex oscillators results in easy adaption of their frequencies to the external stimuli or other associative oscillators. The modified dynamics of individual oscillator can in turn influence the synchronization [<xref ref-type="bibr" rid="B14">14</xref>], and hence large varieties of synchronization patterns can be obtained when different external stimuli are implemented. Indeed, magnetic field and spin-polarised current have been reported to successfully tune the dynamic properties of magnetic vortex nano-oscillators [<xref ref-type="bibr" rid="B19">19</xref>, <xref ref-type="bibr" rid="B20">20</xref>, <xref ref-type="bibr" rid="B34">34</xref>, <xref ref-type="bibr" rid="B35">35</xref>]. Since the oscillation frequency depends on the vortex potential energy, the magnetic anisotropy of the vortex region, which directly influences the magnetic anisotropy energy, can provide a new route to modulating the oscillation dynamics. In experiment, the magnetic anisotropy can be readily modified <italic>via</italic> voltage controlled perpendicular magnetic anisotropy (VCMA) effect [<xref ref-type="bibr" rid="B36">36</xref>&#x2013;<xref ref-type="bibr" rid="B39">39</xref>].</p>
<p>In this work, using micromagnetic simulation, we introduce magnetic anisotropy as a degree of freedom to manipulate the oscillation dynamics and the synchronization of magnetic vortices. The vortex structure for a single oscillator is generated through chiral coupling principle between adjacent regions with in-plane (IP) and out-of-plane (OOP) anisotropy inside a magnetic vortex, and is stabilised <italic>via</italic> interfacial DMI. Although magnetic vortex can be formed and the oscillation and synchronization phenomena can be realized without DMI [<xref ref-type="bibr" rid="B12">12</xref>, <xref ref-type="bibr" rid="B34">34</xref>, <xref ref-type="bibr" rid="B40">40</xref>, <xref ref-type="bibr" rid="B41">41</xref>], the presence of DMI, on the other hand, has been reported to obtain a large frequency and can protect the magnetic texture of the magnetic vortex under a large spin current, thus making the vortex more stable and favouring the development of microwave signal generator [<xref ref-type="bibr" rid="B42">42</xref>]. Also, DMI can help to realize small magnetic nano-oscillators (as small as 10&#xa0;nm) [<xref ref-type="bibr" rid="B43">43</xref>, <xref ref-type="bibr" rid="B44">44</xref>]. The DMI-stabilised chirally coupled nanomagnets have been experimentally demonstrated to realize current-driven domain-wall logic, synthetic antiferromagnets and Ising-like artificial spin ices [<xref ref-type="bibr" rid="B45">45</xref>&#x2013;<xref ref-type="bibr" rid="B48">48</xref>]. Here, by altering the magnetic anisotropy of the vortex region from IP to OOP, i.e. by increasing the value of magnetic anisotropy constant, we show that the oscillation frequency of a magnetic vortex increases significantly. This magnetic anisotropy-dependence of the oscillation dynamics can be used to modulate the synchronization of two vortex oscillators, based on which we design an oscillator network which is capable of programming synchronization configurations used for pattern recognition. As compared to the spin-current-based vortex oscillator reported previously, here magnetic anisotropy is introduced as a new degree of freedom to tune the dynamics, and the mechanism for dynamics modulation is explained in a more comprehensive way. Moreover, the spin current and the magnetic anisotropy can be combined to tune the synchronization configuration and potentially provide extended flexibility for neuromorphic computing.</p>
</sec>
<sec sec-type="methods" id="s2">
<title>Methods</title>
<p>To study the oscillation dynamics of the magnetic vortex, micromagnetic simulations were carried out with the MuMa&#xd7;3 code [<xref ref-type="bibr" rid="B49">49</xref>] using a computation box with 2 &#xd7; 2 &#xd7; 1&#xa0;nm<sup>3</sup> discretization. The MuMax3 utilises the Landau&#x2013; Lifshitz&#x2013;Gilbert&#x2013;Slonczewski (LLG) equation as the basic formalism for describing the low-energy magnetisation dynamics (for details, see <xref ref-type="app" rid="app1">Appendix A</xref>). The magnetic parameters are taken from the experimentally reported chirally coupled nanomagnet based on Pt/Co/AlOx multilayer, with a saturation magnetisation <italic>M</italic>
<sub>S</sub> &#x3d; 1.0&#xa0;MA/m, exchange constant <italic>A</italic> &#x3d; 16&#xa0;pJ/m, interfacial DMI constant <italic>D</italic> &#x3d; &#x2212;1.5&#xa0;mJ/m<sup>&#x2212;2</sup> favouring left-handed chirality, uniaxial anisotropy constant of the OOP region <italic>K</italic>
<sub>0</sub> &#x3d; 7.03 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>2</sup>, and Gilbert damping constant <italic>&#x3b1;</italic> &#x3d; 0.01. A circular region with a diameter of 100&#xa0;nm (named as vortex region hereafter) is embedded inside the computation box with a fixed OOP magnetic anisotropy (named as OOP region hereafter) to form the vortex-like magnetic texture. To reach the vortex-like magnetic texture, the magnetisation in the OOP region is set to the &#x2b;<italic>z</italic> direction, while the magnetisation in the vortex region is set to its opposite direction, after which the system is relaxed. Self-sustained oscillation of the vortex core is then obtained by injecting a spin polarised current along the &#x2b;<italic>z</italic> direction in the vortex region. The <italic>x</italic> component of the average magnetisation (<italic>M</italic>
<sub>Vx</sub>) in the vortex region, which is closely correlated to the oscillation of the core, is used to illustrate the dynamic behaviour of the vortex [<xref ref-type="bibr" rid="B50">50</xref>]. The oscillation frequency is obtained from the frequency spectra converted <italic>via</italic> fast Fourier transformation (FFT) on the time-dependent <italic>M</italic>
<sub>Vx</sub> with the simulation running over a period of 150&#xa0;ns. To study the influence of anisotropy on the oscillation frequency, the magnetic anisotropy constant of the vortex region is varied from 0. To study the synchronization phenomena. Several vortices are separated with each other by a certain distance to create a network. The synchronization spectra are obtained by superimposing the frequency spectra of each single vortex. When mutual phase-locking occurs, the spectra exhibit a strengthened intensity with a common shared peak, otherwise separated peaks with much weaker intensities are observed. All the simulations are performed at zero absolute temperature without considering the thermal magnetisation fluctuations.</p>
</sec>
<sec sec-type="results|discussion" id="s3">
<title>Results and discussions</title>
<sec id="s3-1">
<title>Single oscillator</title>
<p>We first consider the dynamics of a single vortex. As shown in <xref ref-type="fig" rid="F1">Figure 1</xref>, a circular region with variable magnetic anisotropy (vortex region) is embedded in a slab with a fixed uniaxial OOP anisotropy (OOP region). When the uniaxial magnetic anisotropy constant of the vortex region (<italic>K</italic>
<sub>V</sub>) is initially set to be 0, the vortex region has an IP anisotropy, and the chiral vortex magnetic texture is stabilised by the interfacial DMI: <bold>
<italic>H</italic>
</bold>
<sub>DM</sub> &#x3d; &#x2013;<bold>
<italic>D</italic>
</bold>
<sub>
<italic>ij</italic>
</sub> &#xb7; (<bold>
<italic>m</italic>
</bold>
<sub>
<italic>i</italic>
</sub> &#xd7; <bold>
<italic>m</italic>
</bold>
<sub>
<italic>j</italic>
</sub>) where <bold>
<italic>D</italic>
</bold>
<sub>
<italic>ij</italic>
</sub> denotes the DMI vector of interfacial-type DMI, and the DMI energy is given by <inline-formula id="inf1">
<mml:math id="m1">
<mml:mrow>
<mml:msub>
<mml:mi>U</mml:mi>
<mml:mrow>
<mml:mi>D</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>I</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>D</mml:mi>
<mml:mo>&#x222b;</mml:mo>
<mml:mi>d</mml:mi>
<mml:mi>V</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>x</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>x</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>y</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>y</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>. Unlike the symmetric exchange interaction that favours collinear alignment of magnetic moments, DMI prefers an orthogonal arrangement between the neighbouring spins [<xref ref-type="bibr" rid="B45">45</xref>], and here in the Pt/Co/AlO<sub>x</sub> system it gives a fixed left-handed chirality determined by the negative sign of the Dzyaloshinskii vector <bold>
<italic>D</italic>
</bold>
<sub>ij</sub>. Hence, the chiral coupling generates skyrmion-like spin texture in the vortex region which induces a core pointing along the OOP direction opposite to that in the outside OOP regions [<xref ref-type="bibr" rid="B23">23</xref>, <xref ref-type="bibr" rid="B50">50</xref>]. The equilibrium position of the core in the absence of external stimulus is located in the geometry centre of the vortex region for a relatively large DMI strength (&#x7c;<bold>
<italic>D</italic>
</bold>
<sub>ij</sub>&#x7c;&#x2265;0.75&#xa0;mJ/m<sup>2</sup>) [<xref ref-type="bibr" rid="B50">50</xref>] (<xref ref-type="fig" rid="F1">Figure 1A</xref>). When the DMI strength is too small, the equilibrium position of the core is at a finite distance away from the centre, whereas the vortex texture may turn into helical state for a large DMI strength [<xref ref-type="bibr" rid="B50">50</xref>, <xref ref-type="bibr" rid="B51">51</xref>]. In order to stimulate the gyrotropic motion of the vortex core with STT, a spin-polarised current is perpendicularly injected in the vortex region. The self-sustained oscillation can only be obtained when the current is injected here in the &#x2b;<italic>z</italic> direction, while the current injected in the -<italic>z</italic> direction breaks the balance between the forces (<xref ref-type="fig" rid="F1">Figure 1B</xref>). Due to the rapid dissipation of the injected current and the much lower SOT current-to-spin conversion efficiency <italic>cf.</italic> the STT current-to-spin conversion efficiency [<xref ref-type="bibr" rid="B52">52</xref>, <xref ref-type="bibr" rid="B53">53</xref>], the SOT spin current generated in Pt is negligible as compared to the spin current generated <italic>via</italic> STT and not considered in our structure. In order to quickly reach the steady precession state, a preset process is needed [<xref ref-type="bibr" rid="B54">54</xref>&#x2013;<xref ref-type="bibr" rid="B56">56</xref>], which is done here by a applying a magnetic field of 5&#xa0;mT parallel to the plane to preset the vortex core away from the geometry centre. The magnetic field is then removed. If there is no external stimulus, the vortex core relaxes back to the centre following a damped gyrotropic trajectory (black curve in <xref ref-type="fig" rid="F2">Figure 2A</xref> and left inset of <xref ref-type="fig" rid="F2">Figure 2B</xref>). In the presence of STT, the energy dissipation can be counter-balanced by injecting a continuous spin-polarised current in the plain normal direction (<italic>z</italic> direction) through an OOP magnetized top layer <italic>via</italic> a magnetic tunnelling junction in adjacent to the magnetic disk in experiments (<xref ref-type="fig" rid="F1">Figure 1B</xref>). When the current density <italic>J</italic> is above a threshold, self-sustained oscillation of the core with a finite distance away from the geometry centre can be obtained (red curve in <xref ref-type="fig" rid="F2">Figure 2A</xref> and middle inset in <xref ref-type="fig" rid="F2">Figure 2B</xref>). As shown by the snapshots taken from different time for the oscillation at <italic>J</italic> &#x3d; 5.5 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> (insets of <xref ref-type="fig" rid="F2">Figure 2A</xref>), all vortex cores keep the same distance away from the geometry centre. <xref ref-type="fig" rid="F2">Figure 2B</xref> shows the spectra for oscillation frequency as a function of spin current <italic>J</italic> when <italic>K</italic>
<sub>V</sub> &#x3d; 0. The oscillation frequency increases with the increase of <italic>J</italic>, while a larger current (above 1.35 &#xd7; 10<sup>9</sup> A/m<sup>2</sup>) destroys the self-sustained oscillation, leading to the collapse of the vortex structure (blue curve in <xref ref-type="fig" rid="F2">Figure 2A</xref> and right inset of <xref ref-type="fig" rid="F2">Figure 2B</xref>). When <italic>K</italic>
<sub>V</sub> increases to 4 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, the frequency of the whole spectra increases and the modulation of oscillation frequency occurs at a higher current (<xref ref-type="fig" rid="F2">Figure 2C</xref>). The detailed mechanism for the modulation in oscillation frequency will be discussed later.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Schematic illustration of a magnetic vortex structure where circular vortex regions with tunable anisotropy are surrounded by regions with fixed out-of-plane (OOP) anisotropy and a core with out-of-plane magnetisation is induced: <bold>(A)</bold> in equilibrium and <bold>(B)</bold> in oscillation under spin-polarised current. The insets show the magnetisation configuration of the simulated area. Magnetisation along the &#x2b;<italic>z</italic> and&#x2013;<italic>z</italic> direction is indicated in white and black, while the magnetisation direction in the vortex region is given by the colour wheel. Scale bar: 50&#xa0;nm.</p>
</caption>
<graphic xlink:href="fphy-10-1019881-g001.tif"/>
</fig>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>
<bold>(A)</bold> Oscillation amplitudes of <italic>x</italic> component of average magnetisation in the vortex when the spin polarised current <italic>J</italic> &#x3d; 0 (black), <italic>J</italic> &#x3d; 5.5 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> (red) and <italic>J</italic> &#x3d; 2.05 &#xd7; 10<sup>9</sup> A/m<sup>2</sup> (blue). Dependence of oscillation frequency on <italic>J</italic> for <bold>(B)</bold> the anisotropy constant of vortex region <italic>K</italic>
<sub>V</sub> &#x3d; 0 and <bold>(C)</bold> <italic>K</italic>
<sub>V</sub> &#x3d; 4 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>. <bold>(D)</bold> Oscillation amplitudes of <italic>x</italic> component of average magnetisation in the vortex region when <italic>K</italic>
<sub>V</sub> &#x3d; 0 (black) and <italic>K</italic>
<sub>V</sub> &#x3d; 3 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> (red) for <italic>J</italic> &#x3d; 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>. Dependence of oscillation frequency on <italic>K</italic>
<sub>V</sub> for <bold>(E)</bold> <italic>J</italic> &#x3d; 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> and <bold>(F)</bold> <italic>J</italic> &#x3d; 1.35 &#xd7; 10<sup>9</sup> A/m<sup>2</sup>. <bold>(G)</bold> Dependence of the potential energy (<italic>U</italic>) on the variation of the core displacement (&#x7c;<bold>
<italic>X</italic>
</bold>&#x7c;) at different <italic>K</italic>
<sub>V</sub> values. <bold>(H)</bold> The change of upper limit current density (<italic>J</italic>
<sub>C</sub>) for the self-sustained oscillation with the change in <italic>K</italic>
<sub>V</sub>.</p>
</caption>
<graphic xlink:href="fphy-10-1019881-g002.tif"/>
</fig>
<p>Note that the required STT current density (10<sup>8</sup>&#x2013;10<sup>9</sup> A/m<sup>2</sup>) is much lower than the spin-orbital-torque (SOT) current density (10<sup>11</sup> A/m<sup>2</sup>) in a similar structure [<xref ref-type="bibr" rid="B57">57</xref>] which is due to the following reasons: First, the charge-to-spin conversion efficiency in the STT (around 0.5 in Pt/Co system [<xref ref-type="bibr" rid="B52">52</xref>]) is usually higher as compared to SOT (around 0.1 in Pt [<xref ref-type="bibr" rid="B53">53</xref>]). Second, the spin current drives a gyrotropic motion of magnetic oscillator around the equilibrium spin texture, while the SOT switching needs to overcome the magnetic anisotropy and rotate the magnetisation for 180&#xb0;. So the oscillation spin current density is lower than that for switching the magnetisation. Meanwhile, we have not considered the pinning effect which may increases the required spin current density in the real devices.</p>
<p>To study the influence of magnetic anisotropy on the dynamic behaviour of a single vortex, we fix the electric current <italic>J</italic> &#x3d; 8.0 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> and vary the magnetic anisotropy constant <italic>K</italic>
<sub>V</sub> from 0. When <italic>K</italic>
<sub>V</sub> is equal to 0, due to chiral coupling the vortex region forms a stable skyrmion-like spin texture with a small OOP core (left inset of <xref ref-type="fig" rid="F2">Figure 2E</xref>) as a result of exchange singularity [<xref ref-type="bibr" rid="B23">23</xref>, <xref ref-type="bibr" rid="B50">50</xref>]. The self-sustained oscillation, as shown in <xref ref-type="fig" rid="F2">Figure 2D</xref> (curve in black for <italic>K</italic>
<sub>V</sub> &#x3d; 0), has a constant amplitude with a fixed period of 32.6&#xa0;ns, corresponding to a frequency of 306&#xa0;MHz. With the increase of <italic>K</italic>
<sub>V</sub>, the oscillation frequency first increases slowly when <italic>K</italic>
<sub>V</sub> &#x3c;3 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, and then increases drastically when <italic>K</italic>
<sub>V</sub> &#x3e;3 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> (<xref ref-type="fig" rid="F2">Figure 2E</xref>). Meanwhile, the size of the vortex core, as shown in the middle and right inset of <xref ref-type="fig" rid="F2">Figure 2E</xref> (for <italic>K</italic>
<sub>V</sub> &#x3d; 4 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>), undergoes a significant expansion. The red oscillation curve in <xref ref-type="fig" rid="F2">Figure 2D</xref> (representing the oscillation at <italic>K</italic>
<sub>V</sub> &#x3d; 3 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>), as compared to the black curve (<italic>K</italic>
<sub>V</sub> &#x3d; 0) has a shorter oscillation period (25&#xa0;ns) with a larger frequency (400&#xa0;MHz). The oscillation amplitude, which is proportional to the average magnetisation of the vortex region, also decreases, due to the expansion of the core region and the reduction of the IP magnetised region. Interestingly, when <italic>K</italic>
<sub>V</sub> is beyond a critical point of &#x223c;5.8 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, the spectra intensity gradually vanishes, indicating the breakdown of the self-sustained oscillation. As shown in the right inset of <xref ref-type="fig" rid="F2">Figure 2E</xref>, the size of OOP core enlarges to be almost equal to the vortex region when <italic>K</italic>
<sub>V</sub> &#x3d; 5.8 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, resulting in the annihilation of the vortex structure. A similar phenomenon is observed when <italic>J</italic> is increased to 13.5 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> (<xref ref-type="fig" rid="F2">Figure 2F</xref>), where the frequency increases less rapidly with the increasing of <italic>K</italic>
<sub>V</sub>, with a peak reaching at a similar <italic>K</italic>
<sub>V</sub> &#x3d; 5.8 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> before the vortex structure collapses. The annihilation of the vortex structure due to the modification of magnetic anisotropy has been realized experimentally through VCMA effects [<xref ref-type="bibr" rid="B36">36</xref>, <xref ref-type="bibr" rid="B37">37</xref>, <xref ref-type="bibr" rid="B58">58</xref>, <xref ref-type="bibr" rid="B59">59</xref>], where a well-defined IP anisotropy in the radial vortex region is crucial for maintaining the noncolinear spin texture of vortex structure through DMI. When <italic>K</italic>
<sub>V</sub> increases, the antisymmetric DMI is gradually taken over by the symmetric exchange interaction, while the latter favours a colinear and parallel spin alignment between adjacent regions, which eventually results in the collapse of the noncolinear vortex spin texture.</p>
<p>To further understand the tunable dynamic behaviour of the vortex oscillation under the influence of <italic>J</italic> and <italic>K</italic>
<sub>V</sub>, we refer to the centre-of-mass dynamics of the magnetic vortex oscillator, which has been well-modelled by the single collective variable Thiele equation [<xref ref-type="bibr" rid="B60">60</xref>&#x2013;<xref ref-type="bibr" rid="B62">62</xref>].<disp-formula id="e1">
<mml:math id="m2">
<mml:mrow>
<mml:mi mathvariant="bold-italic">G</mml:mi>
<mml:mo>&#xd7;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2b;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:mi>U</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mi>D</mml:mi>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mi>T</mml:mi>
<mml:mi>T</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:math>
<label>(1)</label>
</disp-formula>
</p>
<p>The first term represents the gyrotropic force (also termed as Magnus force), where <inline-formula id="inf2">
<mml:math id="m3">
<mml:mrow>
<mml:mi mathvariant="bold-italic">G</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mn>4</mml:mn>
<mml:mi>&#x3c0;</mml:mi>
<mml:mi>Q</mml:mi>
<mml:msub>
<mml:mi>&#x3bc;</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
<mml:mi>d</mml:mi>
<mml:msub>
<mml:mi>M</mml:mi>
<mml:mi>S</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mi>&#x3b3;</mml:mi>
</mml:mfrac>
<mml:msub>
<mml:mi mathvariant="bold-italic">e</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the gyrovector, with skyrmion number <italic>Q</italic> &#x3d; &#xb1;1 for isolated skyrmion. <italic>M</italic>
<sub>S</sub> is the saturation magnetisation, <italic>d</italic> is the film thickness, <inline-formula id="inf3">
<mml:math id="m4">
<mml:mrow>
<mml:mi>&#x3b3;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the gyromagnetic ratio, <inline-formula id="inf4">
<mml:math id="m5">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3bc;</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the vacuum permeability and <inline-formula id="inf5">
<mml:math id="m6">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">e</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the unit vector. The rigid profile of the vortex core is described by its position <bold>
<italic>X</italic>
</bold> &#x3d; <italic>X</italic> (<italic>x</italic>(t), <italic>y</italic>(t)) in the plane, and its velocity is given by <inline-formula id="inf6">
<mml:math id="m7">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula>. The gyrotropic force is radial outward which primarily acts to expel the core to the outer shell of the vortex [<xref ref-type="bibr" rid="B62">62</xref>]. The second term represents the repulsive (or restoring) force which originates from the edge effect: when the core moves close to the boundary of the vortex structure, the magnetic charges distributed at the cylindrical side wall will generate a centripetal confine potential <italic>U</italic> (<bold>
<italic>X</italic>
</bold>) to regulate the core inside the vortex region [<xref ref-type="bibr" rid="B63">63</xref>]. As can be seen from the form, this second term <inline-formula id="inf7">
<mml:math id="m8">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:mi>U</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula> represents a conservative force acting on the vortex core that is derived from the total free energy of the system [<xref ref-type="bibr" rid="B13">13</xref>]. The edge-induced repulsive force together with the remanent gyrotropic force provide the centripetal force to sustain the circular motion of the core [<xref ref-type="bibr" rid="B54">54</xref>], as illustrated in <xref ref-type="fig" rid="F1">Figure 1B</xref>. The last two terms in <xref ref-type="disp-formula" rid="e1">Eq. (1)</xref> represent the damping force and spin transfer forces, respectively [<xref ref-type="bibr" rid="B54">54</xref>]. The spin polarised current perpendicular to the layers results in a torque force on the vortex core, which can be balanced by the dissipative force, and, in overall, they jointly support orbital motion of the vortex core [<xref ref-type="bibr" rid="B23">23</xref>]. It is worthwhile to mention that <xref ref-type="disp-formula" rid="e1">Eq. (1)</xref> describes an intrinsically non-Newtonian dynamics, which means that the response of the vortex core to a conservative force is gyrotropic, i.e. in a direction perpendicular to the force, instead of accelerating in a direction collinear with the force. This gyrotropic dynamics therefore underpins the persistent oscillations of the vortex core under the four different contributions [<xref ref-type="bibr" rid="B13">13</xref>], as depicted in <xref ref-type="fig" rid="F1">Figure 1B</xref>.</p>
<p>We first consider the role of spin polarised current <italic>J</italic>. As discussed above, the confining potential provides an inward radial repulsive force (second term in <xref ref-type="disp-formula" rid="e1">Eq. 1</xref>) to confine the vortex inside the vortex region, while the spin transfer torque (STT force, the last term in <xref ref-type="disp-formula" rid="e1">Eq. (1)</xref>) arising from <italic>J</italic> tends to drive the core outward toward the edge, so does the gyrotropic force (first term in <xref ref-type="disp-formula" rid="e1">Eq. (1)</xref>). With the increase in <italic>J</italic>, the radius of the steady state orbit increases (as shown in the middle inset of <xref ref-type="fig" rid="F2">Figure 2B</xref> in comparison with the left inset), as a larger dissipation rate is required to compensate the increase in spin torques [<xref ref-type="bibr" rid="B50">50</xref>]. The gyrotropc force increases as well to counterbalance the increase in the STT force, resulting in the increase in the velocity of the core <inline-formula id="inf8">
<mml:math id="m9">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula> [<xref ref-type="bibr" rid="B64">64</xref>]. This entails higher oscillation frequencies above the intrinsic resonance frequency (<xref ref-type="fig" rid="F2">Figures 2B,C</xref>). On the other hand, the radial inward repulsive force has an upper limit because of the limited confine potential <italic>U</italic> (<bold>
<italic>X</italic>
</bold>) [<xref ref-type="bibr" rid="B62">62</xref>]. The increase in <italic>J</italic> therefore leads to a growing outward net force to push the core towards the boundary. When <italic>J</italic> reaches a critical value, the core cannot be confined inside the vortex region and eventually be pushed out (as shown in the right inset of <xref ref-type="fig" rid="F2">Figure 2B</xref>), leading to the collapse of the vortex spin texture [<xref ref-type="bibr" rid="B62">62</xref>]. To more effectively confine the core and maintain the vortex, the upper critical current density should be increased. This can be done by increasing the edge potential using nanoring with high perpendicular magnetic anisotropy [<xref ref-type="bibr" rid="B62">62</xref>]. As discussed below, the increase in the <italic>K</italic>
<sub>V</sub> in the vortex region can serve as an alternative stabiliser to increase the confine potential.</p>
<p>We now turn to understand the role of <italic>K</italic>
<sub>V</sub> on the oscillation dynamics. The intrinsic oscillation frequency is determined by the curvature of the confining potential at the equilibrium core position in the absence of STT force [<xref ref-type="bibr" rid="B50">50</xref>]. We first calculate the relative potential energy of system (<italic>U</italic>-<italic>U</italic>
<sub>0</sub>, where <italic>U</italic>
<sub>0</sub> is the potential energy when the core is in the centre) with respect to different core distances from the centre (&#x7c;<bold>
<italic>X</italic>
</bold>&#x7c;) at different <italic>K</italic>
<sub>V</sub> values in the absence of STT (<xref ref-type="fig" rid="F2">Figure 2G</xref>). Since the equilibrium position of the core is in the centre, <italic>U</italic>-<italic>U</italic>
<sub>0</sub> increases when the core displaces away from the centre. Interestingly, when <italic>K</italic>
<sub>V</sub> increases, <italic>U</italic>-<italic>U</italic>
<sub>0</sub> increases more rapidly with displacement, especially at large <italic>K</italic>
<sub>V</sub> values, indicating that the potential energy becomes higher when the core has the same displacement. This, on one hand, directly increases the slope of the curve as observed in <xref ref-type="fig" rid="F2">Figure 2G</xref>, corresponding to an enhanced <inline-formula id="inf9">
<mml:math id="m10">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:mi>U</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula>, and causes the increase of the repulsive force (second term in <xref ref-type="disp-formula" rid="e1">Eq. 1</xref>). The increase in the repulsive force can in turn be counterbalanced by increasing the gyrotropic force (first term in <xref ref-type="disp-formula" rid="e1">Eq. 1</xref>) when <italic>J</italic> is fixed, as long as self-sustained oscillation is maintained. The increase in gyrotropic force eventually leads to the increase in the velocity <inline-formula id="inf10">
<mml:math id="m11">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="bold-italic">X</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula> and hence the oscillation frequency of the vortex core increases (<xref ref-type="fig" rid="F2">Figures 2E,F</xref>). On the other hand, the increase in confine potential caused by the increase in <italic>K</italic>
<sub>V</sub> requires a larger STT current to maintain the oscillation, which elevates the upper limit of the critical current density (<italic>J</italic>
<sub>C</sub>) for the self-sustained oscillation before the annihilation occurs. <xref ref-type="fig" rid="F2">Figure 2H</xref> shows the <italic>J</italic>
<sub>C</sub> under a 150 ns running interval: when <italic>K</italic>
<sub>V</sub> increases from 0 to 5 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, <italic>J</italic>
<sub>C</sub> increases monotonically from 1.35 &#xd7; 10<sup>9</sup> A/m<sup>2</sup> to 4.25 &#xd7; 10<sup>9</sup> A/m<sup>2</sup>.</p>
<p>The potential energy is closely correlated to the evolution of the vortex structure. As mentioned above, the vortex core expands rapidly when <italic>K</italic>
<sub>V</sub> increases (insets in <xref ref-type="fig" rid="F2">Figure 2E</xref>), which leads to the shrinkage of the noncolinear spin region. The enlarged OOP core and the reduced vortex area make it more difficult for the core to move, and thus a higher exchange energy is needed, which results in the increase in the overall potential energy and the oscillation frequency. Hence, the tuning of the oscillation frequency by <italic>K</italic>
<sub>V</sub> is understood.</p>
</sec>
<sec id="s3-2">
<title>Synchronization of two oscillators</title>
<p>We next turn to investigate how the spin current and magnetic anisotropy affect the mutual interactions for a couple of oscillators. In the simulation, two vortex oscillators are placed with a given distance, while the <italic>J</italic> and <italic>K</italic>
<sub>V</sub> are varied (<xref ref-type="fig" rid="F3">Figure 3A</xref>). As mentioned earlier, interacting non-identical oscillators with different intrinsic frequencies tend to undergo resonance at a common frequency when their oscillation frequencies are within an certain locking range, resulting in the synchronization phenomena [<xref ref-type="bibr" rid="B23">23</xref>, <xref ref-type="bibr" rid="B50">50</xref>]. <xref ref-type="fig" rid="F3">Figure 3B</xref> shows the synchronization spectra as a function of the current density for a pair of oscillators (named as one and 2) with a 100&#xa0;nm distance when <italic>K</italic>
<sub>V</sub> &#x3d; 0. When the spin polarised current of oscillator 1 (<italic>J</italic>
<sub>1</sub>) is fixed at 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> and that of oscillator 2 (<italic>J</italic>
<sub>2</sub>) varies from 0 to 1.25 &#xd7; 10<sup>9</sup> A/m<sup>2</sup>, two distinct frequency peaks are observed at small <italic>J</italic>
<sub>2</sub>, and then they merge into one peak with an enhanced intensity, undergoing synchronization when <italic>J</italic>
<sub>2</sub> ranges between 6 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> and 1 &#xd7; 10<sup>9</sup> A/m<sup>2</sup>. The merged peak diverge again when <italic>J</italic>
<sub>2</sub> &#x3e; 1 &#xd7; 10<sup>9</sup> A/m<sup>2</sup>. In order to study the influence of magnetic anisotropy on the synchronization, the magnetic anisotropy constant in the vortex region of oscillator 1 (<italic>K</italic>
<sub>V1</sub>) is fixed at 1 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> while that of oscillator (<italic>K</italic>
<sub>V2</sub>) varies from 0 to 3 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>. We first study the case where different currents are injected into the two oscillators: <italic>J</italic>
<sub>1</sub> (8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>) &#x2260; <italic>J</italic>
<sub>2</sub> (6.5 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>). As shown in <xref ref-type="fig" rid="F3">Figure 3C</xref>, the two oscillators synchronize with each other when <italic>K</italic>
<sub>V2</sub> ranges from 6 &#xd7; 10<sup>4</sup>&#xa0;J/m<sup>3</sup> to 1.5 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>. The synchronized region &#x394;<italic>K</italic>
<sub>V2</sub>, defined as the length of the interval between the starting and ending point of <italic>K</italic>
<sub>V2</sub> of the synchronization region, is estimated to be 0.9 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>. It is noteworthy that the frequency spectra and synchronization region keep unchanged when the two different oscillators swap their relative positions, as shown in <xref ref-type="fig" rid="F3">Figure 3D</xref>, indicating that the contributions from two oscillators are switchable with regard to position.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>
<bold>(A)</bold> Schematic illustration for the synchronization of two non-identical vortex nano-oscillators with varying spin polarised current density (<italic>J</italic>) and anisotropy constant of the vortex region (<italic>K</italic>
<sub>V</sub>). <bold>(B)</bold> Synchronization frequency spectra for two oscillators separated by a distance of 100&#xa0;nm with varying <italic>J</italic> when the <italic>K</italic>
<sub>V</sub> for both oscillators are 0. The injected current density for oscillator 1 (<italic>J</italic>
<sub>1</sub>) is fixed at 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> while that of oscillator 2 (<italic>J</italic>
<sub>2</sub>) is varied. <bold>(C)</bold> Synchronization frequency spectra for two oscillators separated by a distance of 100&#xa0;nm with varying <italic>K</italic>
<sub>V</sub> when the <italic>J</italic> for both oscillators are fixed at 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>. The anisotropy constant of the vortex region for oscillator 1 (<italic>K</italic>
<sub>V1</sub>) is fixed at 1 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> while that of oscillator 2 (<italic>K</italic>
<sub>V2</sub>) is varied. <bold>(D)</bold> Synchronization frequency spectra when oscillator one and two switch their positions.</p>
</caption>
<graphic xlink:href="fphy-10-1019881-g003.tif"/>
</fig>
<p>The synchronization of nano-oscillators in this system can be realized through propagating spin waves or dipolar interactions [<xref ref-type="bibr" rid="B14">14</xref>], where the distance between the oscillators plays a crucial role to determine the synchronization stability and coupling strength [<xref ref-type="bibr" rid="B50">50</xref>]. Here, to better understand the distance effect, the separation between the oscillators is varied from 60 to 150&#xa0;nm. <xref ref-type="fig" rid="F4">Figures 4A&#x2013;C</xref> show the synchronization spectra with a distance of 60, 80 and 100&#xa0;nm, respectively, for <italic>J</italic>
<sub>1</sub> (8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>) &#x2260; <italic>J</italic>
<sub>2</sub> (6.5 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>) (termed as &#x2018;nonequal case&#x2019;) and <xref ref-type="fig" rid="F4">Figures 4D&#x2013;F</xref> show the respective spectra for <italic>J</italic>
<sub>1</sub> (8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>) &#x3d; <italic>J</italic>
<sub>2</sub> (8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>) (termed as &#x2018;equal case&#x2019;). In both cases, the synchronization range &#x394;<italic>K</italic>
<sub>V2</sub> decreases with the increase in separation distance (<xref ref-type="fig" rid="F4">Figure 4G</xref>), which could be attributed to the decay in coupling strength [<xref ref-type="bibr" rid="B50">50</xref>]. Interestingly, the decrease in &#x394;<italic>K</italic>
<sub>V2</sub> for the nonequal case is much more rapid than the equal case: at a small distance of 60&#xa0;nm, &#x394;<italic>K</italic>
<sub>V2</sub> of the nonequal case is similar to that of the equal case, both having a large synchronization interval of &#x223c;3 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>; in contrast, when the distance increases to 150&#xa0;nm, &#x394;<italic>K</italic>
<sub>V2</sub> for the equal case keeps at a sizable value 1.7 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, while for the nonequal case it decays to 0.1 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>. This stark difference is a clear indication of the faster decay for the overall strength of oscillator interaction with the increase in separation distance when the two current densities are different, which could be due to the relative contribution from different source of interaction (dipolar interaction or spin wave propagation) changes when the current density and distance are different.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>
<bold>(A</bold>&#x2013;<bold>C)</bold> Influence of oscillator distance on the synchronization frequency spectra for two oscillators with varying anisotropy (<italic>K</italic>
<sub>V</sub>) when the current density (<italic>J</italic>) for the two oscillators are nonequal (<italic>J</italic>
<sub>1</sub> &#x3d; 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> and <italic>J</italic>
<sub>2</sub> &#x3d; 6.5 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>): <bold>(A)</bold> D &#x3d; 100&#xa0;nm <bold>(B)</bold> D &#x3d; 80&#xa0;nm and <bold>(C)</bold> D &#x3d; 60&#xa0;nm. The anisotropy constant of the vortex region for oscillator 1 (<italic>K</italic>
<sub>V1</sub>) is fixed at 1 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> while that of oscillator 2 (<italic>K</italic>
<sub>V2</sub>) is varied. <bold>(D</bold>&#x2013;<bold>F)</bold> Influence of oscillator distance on the synchronization frequency spectra for two oscillators with varying anisotropy (<italic>K</italic>
<sub>V</sub>) when the current density (J) for both oscillators are equal (<italic>J</italic>
<sub>1</sub> &#x3d; <italic>J</italic>
<sub>2</sub> &#x3d; 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>): <bold>(A)</bold> D &#x3d; 100&#xa0;nm <bold>(B)</bold> D &#x3d; 80&#xa0;nm and <bold>(C)</bold> D &#x3d; 60&#xa0;nm. The anisotropy constant of the vortex region for oscillator 1 (<italic>K</italic>
<sub>V1</sub>) is fixed at 1 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> while that of oscillator 2 (<italic>K</italic>
<sub>V2</sub>) is varied. <bold>(G)</bold> The change of synchronization range with varying the distance of the two oscillators. The error bar is taken as the interval of the variation of the anisotropy constant in the simulation.</p>
</caption>
<graphic xlink:href="fphy-10-1019881-g004.tif"/>
</fig>
</sec>
<sec id="s3-3">
<title>Synchronization of multiple oscillators for neural networks</title>
<p>The synchronization of nano-oscillators is of great interest for neuromorphic computing. As a proof-of-concept demonstration, we design a neural network comprised of six vortex oscillators (A, B and 1, 2, 3, 4) (<xref ref-type="fig" rid="F5">Figure 5A</xref>), and explore the ability of coupled vortex nano-oscillators to work as a model system for neuromorphic computing <italic>via</italic> anisotropy control. <xref ref-type="fig" rid="F5">Figure 5B</xref> shows the schematic for the intercorrelation between oscillators, neurons, inputs and outputs. The oscillators are separated from each other with a certain distance, with 1&#x2013;4 (output neurons) surrounded by A and B (input oscillators), so that all oscillators can be mutually interacted with each other. As shown below, the change in <italic>K</italic>
<sub>V</sub> of the two input oscillators can modify the synchronization configurations of the whole neural network, mimicking the conversion of encoded inputs to classified output signals <italic>via</italic> programmable weighting mechanism [<xref ref-type="bibr" rid="B30">30</xref>]. Hence, the synchronization configuration between the six oscillators is interpreted here as the output signal.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>
<bold>(A)</bold> Configuration of the neural network with two input oscillators <bold>(A,B)</bold> and four neuron oscillators (1,2,3,4). <bold>(B)</bold> Schematic illustration for the intercorrelation between the oscillators, neurons, inputs and outputs. <bold>(C)</bold> The output frequencies of the oscillators, for the case of <italic>K</italic>
<sub>VA</sub> &#x3d; 2.4 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, <italic>K</italic>
<sub>VB</sub> &#x3d; 1.6 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>. <italic>J</italic> and for all the oscillators are fixed at 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>, and <italic>K</italic>
<sub>V</sub> for neurons 1,2,3,4 are 1.1 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, 0.8 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, 1.2 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, 0.9 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, respectively. <bold>(D)</bold> 2D synchronization map with varying <italic>K</italic>
<sub>VA</sub> and <italic>K</italic>
<sub>VB</sub> when <italic>J</italic>
<sub>B</sub> &#x3d; 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>. <bold>(E)</bold> 2D synchronization map with varying <italic>K</italic>
<sub>VA</sub> and <italic>K</italic>
<sub>VB</sub> when <italic>J</italic>
<sub>B</sub> &#x3d; 9 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>.</p>
</caption>
<graphic xlink:href="fphy-10-1019881-g005.tif"/>
</fig>
<p>To begin with, we set up one input signal using the magnetic anisotropy of either oscillator A or B (<italic>K</italic>
<sub>VA</sub> or <italic>K</italic>
<sub>VB</sub>), and then increase to two input signals by adopting both <italic>K</italic>
<sub>VA</sub> and <italic>K</italic>
<sub>VB</sub>. The current density <italic>J</italic> for all the oscillators is set to be 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>, and the <italic>K</italic>
<sub>V</sub> for the output neurons 1, 2, 3, and four are set to be 1.1 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, 0.8 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, 1.2 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, 0.9 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, respectively. When <italic>K</italic>
<sub>VA</sub> and <italic>K</italic>
<sub>VB</sub> are varied from 0 to 4 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, the frequency patterns of the neural network are converged and allocated to different synchronization configurations appearing at different <italic>K</italic>
<sub>VA</sub> and <italic>K</italic>
<sub>VB</sub> values. For example, when <italic>K</italic>
<sub>VA</sub> &#x3d; 2.4 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup> and <italic>K</italic>
<sub>VB</sub> &#x3d; 1.6 &#xd7; 10<sup>5</sup>&#xa0;J/m<sup>3</sup>, five oscillators (1, 2, 3, 4 and B) are synchronized into one common frequency (<xref ref-type="fig" rid="F5">Figure 5C</xref>) during a running period of 50&#xa0;ns, corresponding to an output synchronization code of (1234B). A total of 13 output patterns are obtained, as represented by 13 different colours organised into a two-dimensional colour map (<xref ref-type="fig" rid="F5">Figure 5D</xref>), while only up to six configurations can be recognised with one input (either <italic>K</italic>
<sub>VA</sub> or <italic>K</italic>
<sub>VB</sub>). Interestingly, when <italic>J</italic>
<sub>B</sub> changes to 9 &#xd7; 10<sup>8</sup> A/m<sup>2</sup>, the synchronization pattern is modified (<xref ref-type="fig" rid="F5">Figure 5E</xref>): the synchronization codes (124B), (134, 2AB) and (124B, 3A) that appear in the case of <italic>J</italic>
<sub>B</sub> &#x3d; 8 &#xd7; 10<sup>8</sup> A/m<sup>2</sup> now disappear, while another three codes (13A, 24), (134, 2A) and (124) emerge. This indicates that current can work jointly with the magnetic anisotropy to modulate the output synchronization patterns.</p>
<p>In the proof-of-concept neural network shown in <xref ref-type="fig" rid="F5">Figure 5</xref>, we have six oscillators, each having independent current density and magnetic anisotropy. The neural network hence has twelve variables. Two variables (<italic>K</italic>
<sub>VA</sub> and <italic>K</italic>
<sub>VB</sub>) can act as inputs and tune the synchronization patterns as the outputs (<xref ref-type="fig" rid="F5">Figure 5D</xref>). We also found that the synchronization pattern changes when the current density of one oscillator is changed (<xref ref-type="fig" rid="F5">Figures 5E</xref> vs <xref ref-type="fig" rid="F5">5D</xref>), indicating that the output depends on the combination of all variables. When two variables (<italic>K</italic>
<sub>VA</sub>, <italic>K</italic>
<sub>VB</sub>) are defined as the inputs, the combination of the rest ten variables (<italic>K</italic>
<sub>V1</sub> &#x2026; <italic>K</italic>
<sub>V4</sub>, <italic>J</italic>
<sub>1</sub>, &#x2026; , <italic>J</italic>
<sub>4</sub> and <italic>J</italic>
<sub>A</sub>, <italic>J</italic>
<sub>B</sub>) can be defined as the weight and bias. When these ten parameters are changed, the weight and bias are changed, resulting in a different output pattern (as shown in <xref ref-type="fig" rid="F5">Figures 5D,E</xref>). Therefore, we can train the neural network to get a target output pattern by adjusting the weight and bias parameters <italic>via</italic> a learning rule.</p>
</sec>
</sec>
<sec sec-type="conclusion" id="s4">
<title>Conclusion</title>
<p>We propose a spintronic nano-oscillator based on the tunable magnetic anisotropy of a polar vortex magnetic structure. The increase of the magnetic anisotropy in the vortex region, which modifies the confine potential and the topology of the magnetic vortex texture, brings the oscillation frequency to higher values and increase the upper critical limit of the spin-polarised currents. The change in oscillation frequency can modify the synchronization between a pair of oscillators. Making use of the tunable dynamics, we show that a designed network of tunable magnetic vortex oscillators can serve as a model system for neuromorphic computing, which is capable to recognise different output synchronization configurations when the magnetic anisotropies of vortices are encoded as inputs. We also found that the output patterns are modified when the spin-polarised current changes. Since both the magnetic anisotropy and spin-polarised current can be experimentally tuned, our model system possesses great potential as a hardware for neuromorphic computing with large flexibility.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s5">
<title>Data availability statement</title>
<p>The data presented in the study are deposited in the Zendo repository, accession number: <ext-link ext-link-type="uri" xlink:href="https://zenodo.org/deposit/7149131">https://zenodo.org/deposit/7149131</ext-link>.</p>
</sec>
<sec id="s6">
<title>Author contributions</title>
<p>ZLu and CY conceived and designed the project. CY, ZLi, and ZLu performed the simulation. CY and YW analysed the simulation data. CY and ZLu worked on the manuscript. All authors are contributed to the discussion on the data and revision of the manuscript.</p>
</sec>
<ack>
<p>The authors acknowledge funding from the National Natural Science Foundation of China (Grant Nos. 51731001, 52201287, 52271160, 11975035, 11805006, 11675006, 52027801, 52111530236), the National Key Research and Development Program of China (Grant No. 2021YFB3500300) and the China-Germany Collaboration Project (M-0199). CY acknowledges the funding from Boya postdoctoral fellowship, Peking University for support of the research.</p>
</ack>
<sec sec-type="COI-statement" id="s7">
<title>Conflict of interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s8">
<title>Publisher&#x2019;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
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<app-group>
<app id="app1">
<title>Appendix A: Basic formalism of the Mumax software</title>
<p>The MuMax3 code is based on the low-energy magnetisation dynamics in strong ferromagnets, which is well-described by the Landau&#x2013;Lifshitz&#x2013;Gilbert&#x2013;Slonczewski (LLG) equation [<xref ref-type="bibr" rid="B65">65</xref>, <xref ref-type="bibr" rid="B66">66</xref>]<disp-formula id="eA1">
<mml:math id="m12">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="bold-italic">m</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>&#x3b3;</mml:mi>
<mml:msub>
<mml:mi>&#x3bc;</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
<mml:mi mathvariant="bold-italic">m</mml:mi>
<mml:mo>&#xd7;</mml:mo>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>f</mml:mi>
<mml:mi>f</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mi mathvariant="bold-italic">m</mml:mi>
<mml:mo>&#xd7;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="bold-italic">m</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>J</mml:mi>
<mml:mi mathvariant="bold-italic">m</mml:mi>
<mml:mo>&#xd7;</mml:mo>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi mathvariant="bold-italic">m</mml:mi>
<mml:mo>&#xd7;</mml:mo>
<mml:mi mathvariant="bold-italic">p</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(A1)</label>
</disp-formula>where <bold>
<italic>m</italic>
</bold> &#x3d; <inline-formula id="inf11">
<mml:math id="m13">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mover accent="true">
<mml:mi>M</mml:mi>
<mml:mo>&#x2192;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mi>M</mml:mi>
<mml:mi>S</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula> is the normalised spin vector, <italic>M</italic>
<sub>S</sub> is the saturation magnetisation, <italic>&#x3b3;</italic> is the gyromagnetic ratio, <inline-formula id="inf12">
<mml:math id="m14">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3bc;</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the vacuum permeability, <bold>
<italic>p</italic>
</bold> is the electron polarization unit vector, <italic>J</italic> is the current density. The first term on the right hand side describes the precession of magnetisation induced by the local effective magnetic field<disp-formula id="eA2">
<mml:math id="m15">
<mml:mrow>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>f</mml:mi>
<mml:mi>f</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mfrac>
<mml:mn>1</mml:mn>
<mml:mrow>
<mml:msub>
<mml:mi>&#x3bc;</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
<mml:msub>
<mml:mi>M</mml:mi>
<mml:mi>S</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>U</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi mathvariant="bold-italic">m</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
<label>(A2)</label>
</disp-formula>where <italic>U</italic> is the free energy of the system. <inline-formula id="inf13">
<mml:math id="m16">
<mml:mrow>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>f</mml:mi>
<mml:mi>f</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> includes the perpendicular uniaxial magnetic anisotropy field, the exchange field, the demagnetization field, and field induced by the interfacial form of the Dzyaloshinskii&#x2013;Moriya interaction (DMI). In a continuous magnetization model, the DMI energy is given by<disp-formula id="eA3">
<mml:math id="m17">
<mml:mrow>
<mml:msub>
<mml:mi>U</mml:mi>
<mml:mrow>
<mml:mi>D</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>I</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>D</mml:mi>
<mml:mo>&#x222b;</mml:mo>
<mml:mi>d</mml:mi>
<mml:mi>V</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>x</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>x</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>y</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>y</mml:mi>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:msub>
<mml:mi>m</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b4;</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(A3)</label>
</disp-formula>where <italic>D</italic> is the DMI constant and <italic>m</italic>
<sub>x</sub>, <italic>m</italic>
<sub>y</sub>, <italic>m</italic>
<sub>z</sub> are the components of the normalized magnetization vector <bold>
<italic>m</italic>
</bold>. The second term on the right is the Gilbert term representing viscous damping, where <italic>&#x3b1;</italic> is the Gilbert damping constant. The third term on the right hand is the Slonczewski term describing the torque arising from the coupling between the local magnetisation and the spin-polarised current flowing perpendicular to the film plane.</p>
</app>
</app-group>
</back>
</article>