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Magnetic properties of the David star in the 2D-Kagome lattice
Philosophical Magazine ( IF 1.6 ) Pub Date : 2021-01-26 , DOI: 10.1080/14786435.2021.1876266
Nermin Kahveci Yağcı 1
Affiliation  

ABSTRACT

We investigate the magnetisation and internal energy of the David star in the Kagome lattice by the effective field theory developed by Kaneyoshi. First-order, Second-order and successive phase transitions are observed for different spin-down orientations. Spin-down orientation of identical atoms causes a second-order phase transition, spin-down orientation of different atoms causes a first-order and successive phase transitions. Minimum internal energy is obtained as UDavid star =−5 for all spin-up orientations, whereas it increases (UDavid star > −5) for at least one spin-down orientation. For spin-down orientation of A↑–A↓, internal energy becomes zero at a certain temperature and we call this temperature ‘zero internal energy temperature (Tzie)’. At T < Tzie=1.99, internal energy is positive, whereas it is negative for other spin states. Therefore, spin-induced minimum internal energy broken is observed except for all spin-up (A↑, B↑ and C↑) cases.



中文翻译:

2D-Kagome晶格中David恒星的磁性

摘要

我们根据Kaoshioshi开发的有效场论研究了Kagome晶格中David恒星的磁化和内部能量。对于不同的向下旋转方向,观察到一阶,二阶和连续相变。相同原子的自旋向下取向导致二阶相变,不同原子的自旋向下取向引起一阶及连续相变。对于所有向上旋转方向,当U David star  = -5时,获得最小内部能量,而内部能量增加(U David star > -5)至少有一个向下旋转方向。对于A↑–A↓的向下旋转方向,在一定温度下内部能量变为零,我们将此温度称为“零内部能量温度(Tzie)”。当T  <Tzie = 1.99时,内部能量为正,而其他自旋态则为负。因此,除了所有自旋(A↑,B↑和C↑)情况,都观察到了自旋引起的最小内能断裂。

更新日期:2021-01-26
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