费米子在二维消失磁场中的对数增强面积定律

Pub Date : 2024-09-14 DOI:10.1007/s00020-024-02778-3
Paul Pfeiffer, Wolfgang Spitzer
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引用次数: 0

摘要

我们考虑在某个固定费米能\(\mu >0\)下,在({\mathbb {R}}^2\)中强度为\(B>0\)的恒定磁场中的朗道哈密顿的费米基态,由费米投影\(P_B:=1(H_B\le \mu )\)描述。对于一些固定的有界域(Lambda子集{\mathbb{R}}^2),其边界集为(Partial \Lambda \)和一个(L>0\),我们将这些基态在空间上限制在缩放域(L \Lambda \)中,并用(P_B(L \Lambda )\)表示相应的局部费米投影。然后我们研究这些局部化基态的多项式f在联合极限(L)和(B)中的希尔伯特空间痕量(textrm{tr} f(P_B(L\Lambda ))\) 的缩放。根据LB的大小,我们可以得到前导阶对数增强的区域律。粗略地说,如果1/B比L更快地趋向于无穷大,那么我们就会得到已知的增强面积律(通过维多姆-索博列夫公式),其形式为\(L \ln (L) a(f,\mu ) |\partial \Lambda |\),即\(L\rightarrow \infty \)为具有费米投影的(二维)拉普拉斯函数\(1(H_0\le \mu )\)。另一方面,如果L以快于1/B的速度趋向于无穷大,那么我们就会得到一个面积定律,其\(L \ln (\mu /B) a(f,\mu ) |\partial \Lambda |\)渐近展开为\(B\rightarrow 0\).这两种情况下的数值系数\(a(f,\mu )\)是相同的,并且只取决于函数f和\(\mu \)。后一种情况下的渐近结果是基于莱施克、索博列夫和第二位作者[7]最近针对固定 B 的联合工作,即对正弦核渐近的全局证明,以及兰道和维多姆在维度一上的增强面积律。一般来说,我们有一个更小的参数(B,L)区域,在这里我们可以证明双尺度渐近展开 \(\textrm{tr} f(P_B(L\Lambda ))\) 为 \(L\rightarrow \infty \) 和 \(B\rightarrow 0\).
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Logarithmically Enhanced Area-Laws for Fermions in Vanishing Magnetic Fields in Dimension Two

We consider fermionic ground states of the Landau Hamiltonian, \(H_B\), in a constant magnetic field of strength \(B>0\) in \({\mathbb {R}}^2\) at some fixed Fermi energy \(\mu >0\), described by the Fermi projection \(P_B:=1(H_B\le \mu )\). For some fixed bounded domain \(\Lambda \subset {\mathbb {R}}^2\) with boundary set \(\partial \Lambda \) and an \(L>0\) we restrict these ground states spatially to the scaled domain \(L \Lambda \) and denote the corresponding localised Fermi projection by \(P_B(L\Lambda )\). Then we study the scaling of the Hilbert-space trace, \(\textrm{tr} f(P_B(L\Lambda ))\), for polynomials f with \(f(0)=f(1)=0\) of these localised ground states in the joint limit \(L\rightarrow \infty \) and \(B\rightarrow 0\). We obtain to leading order logarithmically enhanced area-laws depending on the size of LB. Roughly speaking, if 1/B tends to infinity faster than L, then we obtain the known enhanced area-law (by the Widom–Sobolev formula) of the form \(L \ln (L) a(f,\mu ) |\partial \Lambda |\) as \(L\rightarrow \infty \) for the (two-dimensional) Laplacian with Fermi projection \(1(H_0\le \mu )\). On the other hand, if L tends to infinity faster than 1/B, then we get an area law with an \(L \ln (\mu /B) a(f,\mu ) |\partial \Lambda |\) asymptotic expansion as \(B\rightarrow 0\). The numerical coefficient \(a(f,\mu )\) in both cases is the same and depends solely on the function f and on \(\mu \). The asymptotic result in the latter case is based upon the recent joint work of Leschke, Sobolev and the second named author [7] for fixed B, a proof of the sine-kernel asymptotics on a global scale, and on the enhanced area-law in dimension one by Landau and Widom. In the special but important case of a quadratic function f we are able to cover the full range of parameters B and L. In general, we have a smaller region of parameters (BL) where we can prove the two-scale asymptotic expansion \(\textrm{tr} f(P_B(L\Lambda ))\) as \(L\rightarrow \infty \) and \(B\rightarrow 0\).

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