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Derivation of the Maxwell--Schrödinger Equations from the Pauli--Fierz Hamiltonian
SIAM Journal on Mathematical Analysis ( IF 2 ) Pub Date : 2020-10-08 , DOI: 10.1137/19m1307639
Nikolai Leopold , Peter Pickl

SIAM Journal on Mathematical Analysis, Volume 52, Issue 5, Page 4900-4936, January 2020.
We consider the spinless Pauli--Fierz Hamiltonian which describes a quantum system of nonrelativistic identical particles coupled to the quantized electromagnetic field. We study its time evolution in a mean-field limit where the number $N$ of charged particles gets large while the coupling to the radiation field is rescaled by $1/\sqrt{N}$. At time zero we assume almost all charged particles to be in the same one-body state (a Bose--Einstein condensate) and the photons to be close to a coherent state. In the limit $N \rightarrow \infty$ we show that the time evolution preserves the condensate as well as the coherent structure and that it can be approximated by the Maxwell--Schrödinger system, which models the coupling of a nonrelativistic particle to the classical electromagnetic field. Our result is obtained by an extension of the method of counting, introduced in [P. Pickl, Lett. Math. Phys., 97 (2011), pp. 151--164], to condensates of charged particles in interaction with their radiation field.


中文翻译:

Pauli-Fierz哈密顿量的麦克斯韦-薛定er方程的推导

SIAM数学分析杂志,第52卷,第5期,第4900-4936页,2020年1月。
我们考虑不旋转的Pauli-Fierz哈密顿量,该量描述了耦合到量子电磁场的非相对论性相同粒子的量子系统。我们研究了其在平均场范围内的时间演化,其中带电粒子的数量$ N $变大,而与辐射场的耦合按$ 1 / \ sqrt {N} $重新定标。在零时间,我们假设几乎所有带电粒子都处于同一单体状态(玻色-爱因斯坦凝聚态),光子接近相干态。在极限$ N \ rightarrow \ infty $中,我们证明了时间演化既保留了凝结水又保持了相干结构,并且可以通过麦克斯韦-薛定er系统(Maxwell-Schrödingersystem)对其进行近似,该系统模拟了非相对论粒子与经典粒子的耦合。电磁场。我们的结果是通过扩展计数方法获得的。Pickl,Lett。数学。Phys。,97(2011),pp.151--164],以使带电粒子与其辐射场相互作用而冷凝。
更新日期:2020-10-11
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