The Schrödinger equation on time dependent quantum graphs

2025-05-06 0 0 741.78KB 17 页 10玖币
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TIME EVOLUTION AND THE SCHRÖDINGER EQUATION ON
TIME DEPENDENT QUANTUM GRAPHS
UZY SMILANSKY AND GILAD SOFER
Dedicated to Michael Berry on his forthcoming anniversary.
Abstract. The purpose of the present paper is to discuss the time dependent Schrödinger
equation on a metric graph with time-dependent edge lengths, and the proper way to
pose the problem so that the corresponding time evolution is unitary. We show that
the well posedness of the Schrödinger equation can be guaranteed by replacing the
standard Kirchhoff Laplacian with a magnetic Schrödinger operator with a harmonic
potential. We then generalize the result to time dependent families of vertex condi-
tions. We also apply the theory to show the existence of a geometric phase associated
with a slowly changing quantum graph.
1. Introduction
In the present work, we study the time evolution on quantum graphs whose edge
lengths vary in time. A stationary quantum graph consists of a set of vertices con-
nected by edges of prescribed lengths. On each edge, the Schrödinger operator is the
one-dimensional Laplacian. The graph is supplemented with appropriate boundary
conditions at the vertices, which ensure that the operator is self-adjoint and so the
resulting time evolution is unitary. Our goal is to generalize this model by allowing the
edge lengths to be time dependent.
To illustrate the possible difficulties this time dependence causes, we start by consid-
ering the simplest example. Namely, a graph that consists of two vertices connected by
an edge of length L(t/T ). Here, T1measures the rate of change of the edge lengths.
The evolution for this system is dictated by the time-dependent Schrödinger equation:
iψ (x, t)
t =2
2m
2ψ(x, t)
x2, x L(t/T )
2,L(t/T )
2.(1.1)
At the two vertices we impose the standard Neumann boundary condition:
ψ (x, t)
x = 0 at |x|=L(t/T )
2,t0.(1.2)
The operator on the right hand side of (1.1) involves only derivatives with respect to
x. The time dependence is due to the boundary conditions, which are imposed at the
Uzy Smilansky, Department of Physics of Complex Systems, Weizmann Institute of Science, Rehovot
7610001, Israel. Email: uzy.smilansky@weizmann.ac.il
Gilad Sofer, Faculty of Mathematics, Technion - Israel Institute of Technology, Haifa 32000, Israel.
Email: gilad.sofer@campus.technion.ac.il
1
arXiv:2210.14652v2 [math-ph] 19 Jan 2024
2 UZY SMILANSKY AND GILAD SOFER
time dependent boundary. If one considers the time tas a parameter, the operator on
the right is referred to as the instantaneous Hamiltonian.
Given some initial condition ψ(x, 0), we let the system evolve according to (1.1). A
straightforward computation then gives the following expression for the time derivative
of the squared L2norm of ψ(x, t):
d
dtψ2=d
dtZL(t/T )
2
L(t/T )
2|ψ(x, t)|2dx(1.3)
=1
2T·dL(t/T )
dt"
ψL(t/T )
2, t
2
+
ψL(t/T )
2, t
2#,
This rather unexpected change of the L2norm in time is due to the choice of Neumann
boundary condition, which causes the additional term RL(t/T )
2
L(t/T )
2
d
dt|ψ(x, t)|2dxto vanish
after integrating by parts.
Recalling the standard interpretation of |ψ(x, t)|2dx as the probability for finding the
particle in the interval (x, x +dx)at time t, the above result implies that there exists
a probability flux which equals to the product of the density at the boundary and its
speed. Hence, the probability to find the particle within the boundaries changes in
time. This implies that the evolution dictated by (1.1) is not unitary. In this context,
it is worth noting:
1. The instantaneous L2norm is constant in the adiabatic limit T→ ∞.
2. For the Dirichlet boundary condition (ψ(x, t)=0), the instantaneous L2norm
is constant. Equation (1.3) shows that the change in norm arises also for the Robin
boundary condition:
(1.4) ψ
x (x, t) = Cψ (x, t) at |x|=L(t/T )
2, C R.
In Section 2 we return to this problem, and derive the boundary conditions which
render the time evolution unitary, ensuring probability conservation. We follow previous
studies which treat time dependent domains in different contexts. The time dependent
Schrödinger equation on domains in Rnwith time dependent boundary was studied in
[12, 19, 13]. The propagation of electromagnetic waves in vibrating cavities is a closely
related problem studied in [18]. The present work can be considered as an extension of
these studies to quantum graphs. We shall note that the time dependent Schrödinger
equation on a star graph was studied in [17]. However, the vertex boundary conditions
considered there correspond to the Dirichlet condition, and thus do not address the
problem discussed above.
Once the problem is properly reformulated in Section 2, the effect of the moving
boundary is expressed in terms of a gauge field which, when included, renders the
Schrödinger operator self-adjoint (Theorem 2.1). This is analogous to the derivation
for slowly varying time dependent domains presented in [13].
In Section 3, we generalize the result for graphs where the vertex conditions depend on
time as well (Theorem 3.4). Moreover, we apply these results by studying the geometric
phase associated with the time evolution in the adiabatic limit. Finally, in Appendix
THE SCHRÖDINGER EQUATION ON TIME DEPENDENT QUANTUM GRAPHS 3
A we derive the secular equation whose zeros give the instantaneous spectrum at each
time.
2. Quantum graphs with time dependent edge lengths and standard
boundary conditions
This section consists of three parts, in which the time dependent Schrödinger equation
for quantum graphs with time dependent edge lengths is formulated and discussed. The
first subsection addresses the problem in the simple case of a single interval. It serves
as a primer for the treatment of a general graph which is presented in the second
subsection. In the third subsection we demonstrate the theory by studying the time
evolution on a time dependent equilateral quantum graph.
2.1. A time dependent interval. Before proceeding further, it is worthwhile to
rewrite the Schrödinger equation (1.1) in dimensionless form. Observing that
2mhas
the dimension of length2
time , then scaling xby Land tby Tresults in the dimensionless
quantity L2
T·
2m. Using the standard convention in which
2mtakes the numerical value
1, we remain with a dimensionless L2
T·
2m. We then get the following Schrödinger
equation:
iψ (x, t)
t =2ψ(x, t)
x2, x 1
2L(t/T ),1
2L(t/T ).(2.1)
Following [12, 19, 13], we wish to write the Schrödinger equation in terms of the
scaled variables
(2.2) τ=t
T, ξ =x
L(t/T ).
To do this, we introduce the unitary transformation:
ω(ξ, τ ) := L(τ)1/2ψ(L(τ)ξ, T τ),(2.3)
where now τ[0,1] and ξ1
2,1
2. The Schrödinger equation (2.1) can be rewritten
in the new coordinates as
i
T
τ ω(ξ, τ )(2.4)
=1
L(τ)2
ξ ˙
L(τ)L(τ)
2T!2
ξ2 ˙
L(τ)L(τ)
2T!2
ω(ξ, τ ).
In the new Schrödinger equation, the Schrödinger operator includes a repelling har-
monic potential, and the Laplacian appears as a magnetic Laplacian with A(ξ, τ) =
ξ˙
L(τ)L(τ)
2Tplaying the role of a vector potential. This suggests that one can render the
magnetic operator above self-adjoint by replacing the original Neumann condition with
the magnetic Neumann condition:
(2.5)
ξ ˙
LL
2T!ω(ξ, τ ) = 0 at |ξ|=1
2.
4 UZY SMILANSKY AND GILAD SOFER
This indeed gives a self-adjoint operator on L21
2,1
2. Using (2.5) and (2.3), we obtain
the corresponding boundary condition for ψ(x, t):
(2.6) ψ (x, t)
x =±i˙
L
4Tψ(x, t) at x=±1
2L(t/T ).
Repeating the computation in (1.3) with the new boundary condition immediately
shows that the resulting time evolution is unitary.
The following alternative explanation for the magnetic boundary condition was sug-
gested by Michael Berry [10]. The movement of the edges induces a nontrivial proba-
bility current at the boundary. One may account for this probability current by intro-
ducing a modified Robin boundary condition:
(2.7) ψ (x, t)
x =Cψ (x, t) at |x|=1
2L(t/T ), C C.
While the usual Robin condition corresponds to CR, a straightforward computation
shows that the requirement d
dtψ2= 0 gives the condition Im (C) = ˙
L
4T. We may thus
solve the problem by suggesting the boundary condition (2.6). The associated Robin
parameter may be considered as an effective magnetic field.
The Schrödinger equation and boundary conditions in (2.4), (2.5) can be further
simplified by introducing the gauge transformation
(2.8) ω(ξ, τ ) = ei
2θ(τ)(ξ21/4)g(ξ, τ ).
One may then eliminate the magnetic Laplacian in Equation (2.4) if the phase is chosen
to be θ(τ) = ˙
LL
2T. Note that in the units used in this work, θis dimensionless.
The Schrödinger equation is now given by
i
T
g (ξ, τ )
τ =(2.9)
1
L(τ)2·2g(ξ, τ )
ξ2+¨
LL
4T2ξ2g(ξ, τ )¨
LL (τ) + ˙
L2(τ)
16T2g(ξ, τ ),|ξ| ≤ 1
2,
and subject to standard Neumann boundary conditions.
A similar equation was presented in [17, 19]. We derived it here as a prelude to the
treatment of the time dependent Schrödinger operator on a graph. Note that the factor
1
Tmultiplies the τderivative, implying that the adiabatic limit T→ ∞ is the analogue
of the semi-classical limit.
2.2. Compact metric graphs with time dependent edge lengths. Consider now
the metric graph Γ = (V,E,L), where Vis the vertex set and Eis the edge set (both
assumed finite). Moreover, L: [0, T ]R|E| is a family of edge lengths parameterized as
{Le(t/T )}e∈E with Le(t/T )positive and twice continuously differentiable. A coordinate
xewith xe1
2Le(t/T ),1
2Le(t/T )is assigned to every edge in E. We denote the set
of edges connected to the vertex vby Svand the degree of the vertex by dv:= |Sv|.
摘要:

TIMEEVOLUTIONANDTHESCHRÖDINGEREQUATIONONTIMEDEPENDENTQUANTUMGRAPHSUZYSMILANSKYANDGILADSOFERDedicatedtoMichaelBerryonhisforthcominganniversary.Abstract.ThepurposeofthepresentpaperistodiscussthetimedependentSchrödingerequationonametricgraphwithtime-dependentedgelengths,andtheproperwaytoposetheproblems...

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