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Monte Carlo simulations for D = 1, B = 0.9. Top panel: specific heat, magnetization and chirality as a function of temperature. Bottom panel: three snapshots and their corresponding Sq for three different temperatures, indicated as vertical lines in the plots from the top panel. At the lowest simulated temperature, the system is in the ferromagnetic phase, but an intermediate skyrmion gas phase is clearly seen at higher T .

Monte Carlo simulations for D = 1, B = 0.9. Top panel: specific heat, magnetization and chirality as a function of temperature. Bottom panel: three snapshots and their corresponding Sq for three different temperatures, indicated as vertical lines in the plots from the top panel. At the lowest simulated temperature, the system is in the ferromagnetic phase, but an intermediate skyrmion gas phase is clearly seen at higher T .

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Recently, there has been an increased interest in the application of machine learning (ML) techniques to a variety of problems in condensed matter physics. In this regard, of particular significance is the characterization of simple and complex phases of matter. Here, we use a ML approach to construct the full phase diagram of a well known spin mod...

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... their respective S q at different temperatures. In Fig. 2, at B = 0.2, we see that, at low temperature, the system is in a Sp phase, with the typical single-q S q . At higher T , there is nonzero chirality and the snapshots show a Bm phase, which goes from single-q to a less defined S q . A similar behavior is seen at higher fields (B = 0.9) in Fig. 3, but comparing here a ferromagnetic phase at low temperature with an intermediate skyrmion gas phase. In the higher-temperature snapshot, which corresponds to the highest value of the chirality, we can also see that although the system has a net chirality, thermal fluctuations break the skyrmion and less-defined chiral structures are ...
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... account the intermediate phases. On one hand, the system does not present a clear transition between phases with temperature. On the other hand, specially at higher temperatures, these configurations do not have a characteristic structure factor. We illustrate this showing the results of Monte Carlo simulations for D = 1 in Fig. 2 (B = 0.2) and Fig. 3 (B = 0.9). In both cases, we plot the resulting specific heat, and chirality as a function of temperature, and show three different snapshots and their respective S q at different temperatures. In Fig. 2, at B = 0.2, we see that at low temperature the system is in a Sp phase, with the typical single-q S q . At higher T , there is ...
Context 3
... their respective S q at different temperatures. In Fig. 2, at B = 0.2, we see that at low temperature the system is in a Sp phase, with the typical single-q S q . At higher T , there is non-zero chirality and the snapshots show a Bm phase, which goes from single-q to a less defined S q . A similar behavior is seen at higher fields (B = 0.9) in Fig. 3, but comparing here a ferromagnetic phase at low temperature and an intermediate skyrmion gas phase. In the higher temperature snapshot, which corresponds to the highest value of the chirality, we can also see that although the system has a net chirality, thermal fluctuations break the skyrmion and less-defined chiral structures are ...

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... Later, more complicated convolutional neural networks (CNN) were used to study the effect of uniaxial magneto- crystalline anisotropy pointing in the z direction on the phase diagram of a disk-shaped system, 54) and to construct detailed phase diagrams for skyrmion systems including intermediate regions and paramagnetic state. 55) Moreover, it was shown that such an architecture is able to not only determine phase boundaries but also restore various parameters. The authors of Ref. 56 have demonstrated, that a CNN trained on ground state configurations successfully recovers the chirality and magnetization of a given spin texture, as well as the temperature and external magnetic field at which it was stabilized. ...
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