论文标题
通过使用局部加速电位
Spatial separation of degenerate components of magnon Bose-Einstein condensate by using a local acceleration potential
论文作者
论文摘要
镁的Bose-Einstein凝结(BEC)是在室温下可观察到的少数宏观量子现象之一。由于交换和磁偶极相互作用的竞争,最小能量磁蛋白状态是双重变性的,对应于两个反平行的非零波动器。相应地,Magnon BEC与其他冷凝物基本不同,因为它同时在+/- K_min上进行。 BEC的退化和其两个组成部分之间的相互作用对冷凝物特性具有重大影响。两种冷凝物的相位锁定导致形成冷凝水密度和量化涡流的常驻波。另外,据信这两个组分之间的相互作用对于相对于真实空间崩溃的凝结物稳定很重要。因此,创建非分类的单组分冷凝物的可能性是决定理解镁质BEC的基本物理学的可能性。在这里,我们在实验上证明了一种方法,该方法允许人们完成这项具有挑战性的任务。我们表明,可以通过使用局部脉冲磁场在真实空间中使用归化凝结物的两个组件的分离来实现这一目标,从而使它们的运动沿相反的方向引起。因此,在一定的延迟之后,对应于不同组分的两个云在真实空间中变得很好分开。我们发现,云的运动可以基于磁化分散特征的特殊性来很好地描述。此外,我们表明,在运动过程中,冷凝水云收获了非固定镁,从而导致凝结物耗竭的部分补偿。
Bose-Einstein condensation (BEC) of magnons is one of few macroscopic quantum phenomena observable at room temperature. Due to competition of the exchange and the magnetic dipole interactions the minimum-energy magnon state is doubly degenerate and corresponds to two antiparallel non-zero wavevectors. Correspondingly, magnon BEC differs essentially from other condensates, since it takes place simultaneously at +/-k_min. The degeneracy of BEC and interaction between its two components have significant impact on the condensate properties. Phase locking of the two condensates causes formation of a standing wave of the condensate density and quantized vortices. Additionally, interaction between the two components is believed to be important for stabilization of the condensate with respect to the real-space collapse. Thus, the possibility to create a non-degenerate, single-component condensate is decisive for understanding of underlying physics of magnon BEC. Here, we experimentally demonstrate an approach, which allows one to accomplish this challenging task. We show that this can be achieved by using a separation of the two components of the degenerate condensate in the real space by applying a local pulsed magnetic field, which causes their motion in the opposite directions. Thus, after a certain delay, the two clouds corresponding to different components become well separated in the real space. We find that the motion of the clouds can be described well based on the peculiarities of the magnon dispersion characteristics. Additionally, we show that, during the motion, the condensate cloud harvests non-condensed magnons, which results in a partial compensation of the condensate depletion.