On the uniqueness of solutions to the periodic 3D Gross-Pitaevskii hierarchy

被引:35
|
作者
Gressman, Philip [1 ]
Sohinger, Vedran [1 ]
Staffilani, Gigliola [2 ]
机构
[1] Univ Penn, Dept Math, David Rittenhouse Lab, Philadelphia, PA 19104 USA
[2] MIT, Dept Math, Cambridge, MA 02139 USA
基金
美国国家科学基金会;
关键词
Gross-Pitacvskii hierarchy; Nonlinear Schrodinger equation; BBGKY hierarchy; Bose-Einstein condensation; Determinant of a lattice; U and V spaces; Factorized solutions; Multi linear estimates; NONLINEAR SCHRODINGER-EQUATION; MEAN-FIELD-LIMIT; BOSE-EINSTEIN CONDENSATION; GLOBAL WELL-POSEDNESS; RIGOROUS DERIVATION; SCATTERING THEORY; CLASSICAL-LIMIT; DYNAMICS; DETERMINANTS; EVOLUTION;
D O I
10.1016/j.jfa.2014.02.006
中图分类号
O1 [数学];
学科分类号
0701 ; 070101 ;
摘要
In this paper, we present a uniqueness result for solutions to the Gross-Pitaevskii hierarchy on the three-dimensional torus, under the assumption of an a priori spacetime. bound. We show that this a priori bound is satisfied for factorized solutions to the hierarchy which come from solutions of the nonlinear Schrodinger equation. In this way, we obtain a periodic analogue of the uniqueness result on 1113 previously proved by Klainerman and Machedon [75], except that, in the periodic setting, we need to assume additional regularity. In particular, we need to work in the Sobolev class H degrees for alpha > 1. By constructing a specific counterexample, we show that, on T-3, the existing techniques from the work of Klainerman and Machedon approach do not apply in the endpoint case alpha = 1. This is in contrast to the known results in the nonperiodic setting, where these techniques are known to hold for all alpha >= 1. In our analysis, we give a detailed study of the crucial spacetime estimate associated to the free evolution operator. In this step of the proof, our methods rely on lattice point counting techniques based on the concept of the determinant of a lattice. This method allows us to obtain improved bounds on the number of lattice points which lie in the intersection of a plane and a set of radius R, depending on the number-theoretic properties of the normal vector to the plane. We are hence able to obtain a sharp range of admissible Sobolev exponents for which the spacetime estimate holds. (C) 2014 Elsevier Inc. All rights reserved.
引用
收藏
页码:4705 / 4764
页数:60
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