论文标题
扩展宇宙边界处的费米亚生产:冷原子引力类似物
Fermion production at the boundary of an expanding universe: a cold-atom gravitational analogue
论文作者
论文摘要
我们研究了弗里德曼 - 罗伯逊 - 骑行时期宇宙粒子产生的宇宙学粒子产生现象,重点是(1+1)维度的情况,在这种情况下,量表因子的演变是由jackiw-teitelboim重力的方程式设置的。作为迈向这种现象的量子模拟的第一步,我们考虑了两个可能的晶格正规化,这使我们能够探索粒子产生和拓扑现象的相互作用,并在边界的空间中探索。特别是,对于迪拉克场的Wilson型离散化,由中间扩展连接的渐近Minkowski真空对应于对称性保护的拓扑结构地面,并以零模型的形式具有零模型的边界表现。我们表明,粒子的产生还可以填充这些零模式,这与情况与幼稚的特离散化形成鲜明对比,在这种情况下,共形零质量场不显示颗粒的产生。我们提出了一种通过拉曼光学晶格中的超冷原子对这种引力类似物进行量子模拟的方案,该方案需要根据模拟时空的规模对拉曼束对拉曼束的实时控制以及频带映射测量。
We study the phenomenon of cosmological particle production of Dirac fermions in a Friedman-Robertson-Walker spacetime, focusing on a (1+1)-dimensional case in which the evolution of the scale factor is set by the equations of Jackiw-Teitelboim gravity. As a first step towards a quantum simulation of this phenomenon, we consider two possible lattice regularizations, which allow us to explore the interplay of particle production and topological phenomena in spacetimes with a boundary. In particular, for a Wilson-type discretization of the Dirac field, the asymptotic Minkowski vacua connected by the intermediate expansion corresponds to symmetry-protected topological groundstates, and have a boundary manifestation in the form of zero-modes exponentially localized to the spatial boundaries. We show that particle production can also populate these zero modes, which contrasts with the situation with a naïve-fermion discretization, in which conformal zero-mass fields exhibit no particle production. We present a scheme for the quantum simulation of this gravitational analogue by means of ultra-cold atoms in Raman optical lattices, which requires real-time control of the Raman-beam detuning according to the scale factor of the simulated spacetime, as well as band-mapping measurements.