Misra Subhradeep, Stern Michael, Umansky Vladimir, Bar-Joseph Israel
Department of Condensed Matter Physics, Weizmann Institute of Science, Rehovot 7610001, Israel.
Department of Physics and Center for Quantum Entanglement Science and Technology, Bar-Ilan University, Ramat-Gan 5290002, Israel.
Proc Natl Acad Sci U S A. 2022 Aug 9;119(32):e2203531119. doi: 10.1073/pnas.2203531119. Epub 2022 Aug 3.
We show that a Bose-Einstein condensate consisting of dark excitons forms in GaAs coupled quantum wells at low temperatures. We find that the condensate extends over hundreds of micrometers, well beyond the optical excitation region, and is limited only by the boundaries of the mesa. We show that the condensate density is determined by spin-flipping collisions among the excitons, which convert dark excitons into bright ones. The suppression of this process at low temperature yields a density buildup, manifested as a temperature-dependent blueshift of the exciton emission line. Measurements under an in-plane magnetic field allow us to preferentially modify the bright exciton density and determine their role in the system dynamics. We find that their interaction with the condensate leads to its depletion. We present a simple rate-equations model, which well reproduces the observed temperature, power, and magnetic-field dependence of the exciton density.
我们表明,由暗激子组成的玻色-爱因斯坦凝聚体在低温下于砷化镓耦合量子阱中形成。我们发现,该凝聚体延伸超过数百微米,远超出光激发区域,并且仅受台面边界限制。我们表明,凝聚体密度由激子间的自旋翻转碰撞决定,这种碰撞将暗激子转化为亮激子。在低温下该过程的抑制导致密度增加,表现为激子发射线的温度依赖性蓝移。在面内磁场下的测量使我们能够优先改变亮激子密度并确定它们在系统动力学中的作用。我们发现它们与凝聚体的相互作用导致凝聚体耗尽。我们提出了一个简单的速率方程模型,该模型很好地再现了所观察到的激子密度的温度、功率和磁场依赖性。