Institut für Astrophysik, Georg-August Universität, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany.
Raytheon BBN Technologies, Quantum Engineering and Computing, Cambridge, Massachusetts 02138, USA.
Phys Rev Lett. 2019 Sep 20;123(12):121601. doi: 10.1103/PhysRevLett.123.121601.
Antiferromagnetically doped topological insulators (ATI) are among the candidates to host dynamical axion fields and axion polaritons, weakly interacting quasiparticles that are analogous to the dark axion, a long sought after candidate dark matter particle. Here we demonstrate that using the axion quasiparticle antiferromagnetic resonance in ATIs in conjunction with low-noise methods of detecting THz photons presents a viable route to detect axion dark matter with a mass of 0.7 to 3.5 meV, a range currently inaccessible to other dark matter detection experiments and proposals. The benefits of this method at high frequency are the tunability of the resonance with applied magnetic field, and the use of ATI samples with volumes much larger than 1 mm^{3}.
反铁磁掺杂拓扑绝缘体 (ATI) 是可能存在动力学轴子场和轴子极化激元的候选材料之一,轴子极化激元是一种弱相互作用的准粒子,类似于暗轴子,暗轴子是一种长期以来被寻找的暗物质候选粒子。在这里,我们证明了在 ATI 中使用轴子准粒子反铁磁共振,并结合探测太赫兹光子的低噪声方法,是探测质量为 0.7 到 3.5meV 的轴子暗物质的可行途径,这个质量范围目前是其他暗物质探测实验和方案无法探测到的。这种方法在高频下的优势是可以通过外加磁场来调节共振,以及使用体积比 1mm^{3} 大得多的 ATI 样品。