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  <front>
    <journal-meta />
    <article-meta>
      <title-group>
        <article-title>The Computational Modeling: Dynamic Quantum Model Approach</article-title>
      </title-group>
      <contrib-group>
        <aff id="aff0">
          <label>0</label>
          <institution>Kherson State University</institution>
          ,
          <addr-line>27, Universitetska st., Kherson, 73000</addr-line>
          <country country="UA">Ukraine</country>
        </aff>
      </contrib-group>
      <fpage>0000</fpage>
      <lpage>0002</lpage>
      <abstract>
        <p>After S. Smale's works it became clear that in smooth dynamics the system of a general form is not structurally stable and therefore there is no strict mathematical basis for modeling and computational analysis of systems. The contradiction appeared in science: according to physicists dynamics is simple and universal. The solution to this problem was proposed based on the construction of dynamic quantum models (DQM). From the assumption that quantum effects are caused by unrecoverable “white noise”, a certain mathematical model of quantum mechanics already follows and is essentially unambiguous. On the other hand, in this model spectral problems are reduced tothe usual perturbation theory of smooth dynamical systems. Thus, the construction of such models can be considered as an asymptotic method for solving spectral problems. But the definition of DQM is not formally related to Hamiltonian systems. DQM is defined and constructed universally for both Hamiltonian systems and systems with the truth function. As a result, for example, quantization with the Bohr-Sommerfeld condition also extends to systems with a truth function. Hopefully DQM opens for new applications. The most important is to seek assistance and cooperation in future research.</p>
      </abstract>
      <kwd-group>
        <kwd>modeling</kwd>
        <kwd>computer simulation</kwd>
        <kwd>structural stability</kwd>
        <kwd>dynamical system</kwd>
        <kwd>dynamic quantum model</kwd>
        <kwd>Markov cascade</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec id="sec-1">
      <title>Introduction</title>
      <p>Increasingly, processes and systems are researched or developed through computer
simulations and this trend is likely to continue [1]. Computational modeling has been
used in physics, chemistry and related engineering for many decades because this is
the only way the equations can be solved at all [2]. It consists from two steps: (i)
modeling, i.e. finding a model description of a real system, and (ii) solving the
resulting model equations using computational methods [3].</p>
      <p>But if an arbitrarily small perturbation of the model leads to a qualitatively
different picture of the dynamics, then such a model is not applicable to the real process:
strictly speaking, perturbations are included in the definition of a model [4]. Also
computational methods inevitably lead to errors of discretization and rounding in
calculations [5]. Therefore traditionally the stability of a model with respect to
relaCopyright © 2020 for this paper by its authors. Use permitted under Creative Commons License Attribution 4.0 International (CC BY 4.0).
tively small changes is a necessary condition for its correctness [6]. The qualitative
invariance of a mathematical model under small perturbations is usually called
structural stability [7].</p>
      <p>However, in S. Smale's works [8] was shown, that there exist smooth dynamic
systems whose neighborhoods do not contain any structurally stable system. This meant
that there was no rigorous mathematical basis for modeling and computational
analysis. The contradiction has appeared in science, because physicists believe that the
dynamics is simple and universal [9].</p>
      <p>The solution to this problem was proposed in [10] based on the construction of
dynamic quantum models (DQM). It turned out that taking into account random
fluctuations, necessary for the transition to the quantum model of reality, allows us to return
in fact to the simple picture of A. Poincare’s dynamics: a dense set of structurally
stable systems.</p>
      <p>DQM is so named because for Hamiltonian systems it is simply related to the
corresponding Schrödinger equation. From the assumption that quantum effects are
caused by unrecoverable “white noise”, a certain mathematical model of quantum
mechanics already follows and is essentially unambiguous [11]. Dynamics in it is
described by Markov cascades (time is discrete). This model is simply connected with
the traditional one: there is a simple correspondence between Markov cascades and
quasisolutions of the corresponding Schrödinger equation. Thus, in a sense, DQM is a
bridge between the formal calculus of quantum mechanics and the intuitive vision of
physicists. On the other hand, in this model spectral problems are reduced to the usual
perturbation theory of smooth dynamical systems. Thus, the construction of such
models can be considered as an asymptotic method for solving spectral problems.</p>
      <p>This paper gives an example of such approach to the one-dimensional system with the
quasiperiodic potential (Proposition 2).</p>
      <p>But the definition of DQM is not formally related to Hamiltonian systems; it is
defined for any ordinary differential equation or any diffeomorphism on any smooth
Riemannian manifold. Hopefully this opens the way for absolutely new applications.</p>
      <p>For example, for applications to dynamic systems that using logical operations:
algorithms, theorems, software applications. The use of fuzzy logic in DQM is in principle
completely natural and even almost inevitable. Let J = J (z) be a given smooth
function on phase space (0  J (z) 1), equal to 1 on the true trajectory and 0 outside some
neighborhood of it; we can interpret it as the function of truth. In this paper, DQM is
defined and constructed universally for both Hamiltonian systems and systems with
the truth function J. As a result, for example, the point of the DQM spectrum is
interpreted exactly as the average value of truth for approximate logical conclusions.</p>
      <p>Quantization with the Bohr-Sommerfeld condition also extends to systems with a
truth function (Proposition 1).</p>
      <p>But the reverse is also true. If we construct an approximate model of given theorem
or software application using the training of a neural network, then we get the DQM
of these objects. With further training, these DQMs will approach the original object
(in other words, they will converge to it according semiclassical limit). Perhaps this
will allow a new approach to the problems of solvability in logic, there is some
analogy with the theorem of the equivalence of structural stability and hyperbolicity proved
in [10]. DQM of systems with logical operations are always uniformly limited by the
number of operations (see Section 2.2) and then for them solvability is not in doubt.</p>
      <p>Then everything depends on the semiclassical limit, more precisely, on the uniformity
of the structural stability of DQM.</p>
      <p>The paper goal is 1) to build the foundations of the theory of dynamic quantum
models (DQM); 2) to demonstrate the application of this theory for spectral problems
of quantum mechanics.</p>
      <p>The paper is organized as follows: in part 2 we synthesize the dynamic quantum
model (DQM); in part 3 we demonstrate the application of DQM for spectral
problems of quantum mechanics; part 4 concludes.</p>
      <p>We had to omit proofs of some propositions in order to fit the paper format.
2
2.1</p>
    </sec>
    <sec id="sec-2">
      <title>The Dynamic Quantum Model: Basic Definitions</title>
      <sec id="sec-2-1">
        <title>DQM Definition</title>
        <p>
          Let p(x) be an n -dimensional smooth vector field on an n -dimensional smooth
Riemannian manifold M , where x(x1, x2 ,..., xn ) are local Euclidean coordinates on
M , pi (x) C  (Rn ) ( i = 1,..., n ). On each phase curve x(t)  M of the
dynamical system generated by this vector field
dxi = pi (х) , ( i = 1,..., n )
dt
(
          <xref ref-type="bibr" rid="ref1">1</xref>
          )
х(t)
0
t
consider the integral of the “shortened action” s(t) =  p(x)dx =  p( ) 2 d ,
where p( ) 2 = n pi2 ( ) . The value of s(t) on each curve x(t) , which is
differi=1
ent from a fixed point, is diffeomorphically expressed in t and is called “optical
time”. Let  be a metric such that s(t) =  d : d = p(t) 2 dt . The following is
х(t)
the heuristic derivation or explanation of the definition of dynamic quantum model
(Definition 1).
        </p>
        <p>
          So, the distance d traveled by a point along the path of (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) during the time t is
 t
equal to d =  p( ) d = p(tc )  t , where pc = p(t0 ) is the average value
0
(0  t0  t) . (Of course this is with a single bypass of trajectory during t : turning
points are the special case). Further, we assume that the fluctuations generate “white
noise”  (t) , acting on the configuration space with the dispersion D (t) =  2t ,
where the diffusion coefficient  2 is constant over the considered time interval. It
will take some time t , until the point moves to a distance d from the initial
position, which exceeds the mean square error caused by  (t) during the time t , i.e.
pc t will exceed
 2t . With such a minimal t
pc t =
t , whence
2 t and therefore
.
t =
to  2 . (In other words, the distance between them in the metric  is equal to  2 ).
2) During this time “white noise”  (t) generates an irremovable random error, the
standard deviation of which is equal to the distance d between the nearest
significant measurements along the trajectory.
        </p>
        <p>Now suppose that the configuration space is one-dimensional, there is a turn point
on the segment of the trajectory, the initial position is located near the turn point and
move towards it. To pass a segment of the path, the ends of which are significantly
different, the point must reach the turning point, and then (after turning) pass another
segment of ρ – length  2 . How much will the distance to the nearest significantly
different measurement increase? The points on the segment ρ – lengths  2 , including
the turning point, are indistinguishable among themselves, only their average value is
important. Therefore, the points in the interval between 3 2 and 1 2 to the turning
2 2
point in time  2 will move to the segment centered just on the turning point; and
after a while until the next significantly different position. So, only for points on a
segment with length 1 2 to a turning point, the distance to the nearest significantly
2
different measurement will increase: on average by 1 2 .
4</p>
        <p>In the general case, one should take into account those points that move towards
the caustic K – the set of singular points at which the direction of motion changes
and are located at ρ – distance 1 2 from K. To pass a segment of the path, the ends
2
of which are significantly different, such points must reach K, and then (turning) to
pass another segment of ρ – length  2 in a new direction. Therefore, the travel time
for these points will increase on average by 1 2 . The jump in the time interval at
4
turning points on the optical time scale is a quantum-mechanical phenomenon
traditionally taken into account by means of the Morse index (when establishing a
connection with the Schrödinger equation, it turns out that 1 2 = h , i.e.  2 = 2πh).
4 2
Generally speaking, there may be features on the caustic other than turn points,
however, such a singular point splits into several turn points with an arbitrarily small stir
[6]. At such points, the number 1 2   =  h is added to the ρ - length, where μ
4 2
is the Morse index of the singular point. Here μ is an integer equal to the number of
turning points that arose during small stir and passed in the positive direction to the
caustic minus the number of turning points traveled in the negative direction.</p>
        <p>
          So, a dynamic quantum model first shifts each point along the phase curve of a
given dynamic system over the optical time  2 (or ρ – length  2 ) and in a
neighborhood of the caustic this shift increases abruptly by 1  2 = μ h . And then
4 2
randomly shifts on a distance not exceeding the length of the trajectory from the
original to the new point. The following rigorous definition summarizes this description.
The definition of a dynamic quantum model is given for an arbitrary dynamic system
(
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) on an arbitrary compact Riemannian manifold M .
        </p>
        <p>
          Definition 1. By a dynamic quantum model (DQM) for dynamical system (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) we
mean the Markov cascade with the transition function) P(x, A) , which associates
with each point x of the trajectory of (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) and an open subset A of the configuration
space probability of getting from x to A in one iteration:
1
        </p>
        <p>A
where t is the shift time from x to Gx along the path of the ρ-length 2h or 2h
+  h in the neighborhood of the caustic,  2 = 2h . Given the initial
distribu2
tion, we obtain a Markov process P with this initial distribution and the transition
function P( y, A) : if  t is the distribution at time t , t is the lag between the two
nearest measurements, then the DQM sets new distribution P(t ) = t+t at time
P( x, A) =
2t
 e−( y−Gx)2 / 2 2t dy ,
t + t .
2.2</p>
      </sec>
      <sec id="sec-2-2">
        <title>DQM Eigenvalues and Markov Deviations</title>
        <p>Our goal is to determine pure states and eigenvalues of DQM. And now, along with
the discreteness of the measurement process, its limited time will be essential. Of
course, the measurement process cannot continue indefinitely, but here its duration is
dictated by the very definition of DQM. Namely, the duration of the measurement, in
principle, cannot exceed on order
1 since further the measurement errors with
dish
persion  2 t (where the diffusion coefficient  2 is small of order h) are no longer
small and the notion of trajectory loses its meaning. (And you can only talk about the
average values for the ensemble, as in statistical physics). Therefore, we limit the time
to a certain limiting value T of order 1 ( T ~ 1 ): T  B , where B &gt; 0 is a
conh h h
stant. (In general, we say that the quantity u = u (h) in a DQM is of order hk (u ~ hk
or u = O(hk)), if  u  ≤ Chk . And u = u (h) is exactly of the order hk (u ~ = hk), if
chk ≤  u  ≤ Chk for some constants C, c &gt; 0).</p>
        <p>
          Let us now consider the problem: it is required to experimentally determine the
location of the point at which a given point of the phase space (x; p) passes under the
action of dynamical system (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) with the greatest possible accuracy. Note that the time
time scale or of order
interval between the two nearest significant measurements is  2 = 2πh on the optical
h
        </p>
        <p>
          on the usual scale in the neighborhood of the point (x; p)
(see (
          <xref ref-type="bibr" rid="ref2">2</xref>
          )). In addition, the duration of the measurements is limited by the value of T ~
1 . Therefore, the position of the point in the next significant measurement can be
h
obtained, in principle, only a finite number of times, namely N ~ T
h
p
2 ~
p
h2
2
numbers. But this position is determined each time with the unrecoverable error, the
standard deviation of which is equal to d   2 (see (
          <xref ref-type="bibr" rid="ref2">2</xref>
          )) , i.e. d ~ h . Therefore,
p p
the averaging of all such measurements, i.e. then the best approximation to the
unperturbed value, which in principle can be achieved, differs from it by an order of value
d ~ h p 2 ~ h2 . Such a deviation is given at each point z of the
N p h2 p 2
phase space, i.e. defines a vector field Z(z). So,
1. h2 is the least in order error, with which the coordinates of the point in he phase
space can be known, and thus the values observed at the point. Values whose
difference in order of value is less than h2 are not experimentally distinguishable.
2. As a result of averaging the maximum number of maximally accurate
measurements, we arrive to a dynamical system generated not by the diffeomorphism G,
but by its perturbation G = G + Z .
        </p>
        <p>Definition 2. The Markov deviation Z (z) is a smooth vector field on phase space
such that 1)</p>
        <p>
          Z ( z)  B
( B  0 ) is a constant of dynamical system (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) (i.e., the length Z(z) does not exceed in
order h2
p 2
        </p>
        <p>for all points z of the phase space);
2) for any initial point z0 = z(t0) on the phase curve z(t) of the dynamical system</p>
        <p>
          t0 t0
where e(t) is the unit normal vector of the closed phase curve at the point z(t),
B  0 is the constant of dynamical system (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ).
        </p>
        <p>
          Property (
          <xref ref-type="bibr" rid="ref3">3</xref>
          ) of the Markov deviation is due to the fact that, by construction, the
vector Z(z(t)) has a random orientation, therefore, the pluses and minuses of the
accumulations of its projections on the unit vectors are compensated. Therefore, the
integral of the accumulation of projections along the phase curve is experimentally
indistinguishable from zero.
        </p>
        <p>
          If instead of a given time limit T ~ 1 we take T1 ~ 1 ( T1  T ), then we obtain
h h
another Markov deviation; similarly, when replacing the zero point in time. So the
Markov deviation is a smooth vector field that depends on the parameters; further, it
can be assumed to be a general view field.
(
          <xref ref-type="bibr" rid="ref3">3</xref>
          )
2.3
        </p>
      </sec>
      <sec id="sec-2-3">
        <title>DQM Pure States and Eigenvalues. Quantization of Spectrum in DQM.</title>
        <p>The physical meaning of the eigenvalues is that these are all values of energy that can
be the result of reliable, i.e. the most accurate measurement (ideally of the order of
h2). But as a result of the most accurate experiments, as we have seen, in reality the
dynamics is studied not of the diffeomorphism G, but of its perturbation G = G + Z
. Let J = J (z) be a given smooth function on phase space. We can interpret it as the
Hamiltonian (energy in the phase space) or as a function of truth (0  J (z) 1), equal
to 1 on the true trajectory and 0 outside some neighborhood of it. Given the
irremovable errors of the Markov deviation, the discreteness of the measurement process and
its limited time, we arrive at the maximum number of the most accurate
measurements 1 Nt J (G i z) , where z is the point of phase space, Z is the general view</p>
        <p>Nt i=0
Markov deviation, G = G + Z is a diffeomorphism, Nt is the maximum number of
significantly different measurements over time t ≤ T.</p>
        <p>
          In terms of meaning the eigenvalue of the spectrum is associated with some pure
stationary state of the dynamical system: any reliable measurement in this state leads
to an acceptable error (ideally with a maximum accuracy of the order of h2) and only
to this value. But in a DQM any point in the phase space is always known with the
irremovable error of order h (see (
          <xref ref-type="bibr" rid="ref2">2</xref>
          )). As a result, we average generally speaking over
trajectories with a starting point not z , but some ~z , that is distant from z by a
distance of the order h. Therefore, the carrier of the state associated with some
eigenvalue of α must contain a ball with a diameter of exactly the order of h: otherwise, any
reliable experiment with a significant probability will lead to values significantly
different from α. Hence
        </p>
        <p>Definition 3. Let G = G + Z , where Z is a general view Markov deviation; Nt is
the number of all iterations of the diffeomorphism in time t; α is a real number. Let D
= Dαh be the set of points z of the phase space such that for all sufficiently large t &lt; T
~ = 1
h
1 Nt J (G i z) −  Bh 2 ,</p>
        <p>
          Nt i=0
where B is a constant. Then, if for any Z of a general view and sufficiently small h,
the set Dαh contains a ball with a diameter of exactly the order of h, then α will be
called the eigenvalue of the DQM for dynamical system (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ), and Dαh will be called the
carrier of the pure state corresponding to this eigenvalue.
        </p>
        <p>Thus, all points of a DQM spectrum are formally determined only with an accuracy
of the order of h2, but this corresponds precisely to their meaning. By definition, the
domain Dαh is an open G - invariant subset of the phase space.</p>
        <p>So, to define DQM means to set: 1) the Markov process in accordance with
Definition 1; 2) the Markov deviation Z of general view or, what is the same,
diffeomorphism G = G + Z in accordance with Definition 2.</p>
        <p>
          Consider the two–dimensional dynamical system (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ), the compact phase space Λ
of which is filled with closed phase curves. After the smooth change of variables, in
canonical coordinates, this is the dynamics of uniform rotation along concentric
circles. If we interpret J as a function of truth, then its values on each circle, concentric
to the true path (true circle), are constants (i.e., they do not depend on a point on this
circle). At the semantic level, with such interpretation, we are talking about transitions
to equivalent propositions.
        </p>
        <p>Proposition 1. The DQM eigenvalues of the given dynamical system, with
accuracy of the order h2, are equal to the values of J (z) on the phase circles in Λ, the ρ
length of which satisfies the Bohr - Sommerfeld condition
1
 p( x) dx = I = h(n + )
2
and only they.
3</p>
      </sec>
    </sec>
    <sec id="sec-3">
      <title>The Spectrum of Schrödinger Equation with Quasiperiodic</title>
    </sec>
    <sec id="sec-4">
      <title>Potential and DQM</title>
      <p>Consider the Schrödinger equation

 t</p>
      <p>
        2
= H ( ) = − h2  
x2 + U (x)
with the quasiperiodic potential U(x) = cos x + ε ∙ cos λx (ε, λ &gt; 0). For this
Schrödinger equation we construct its dynamic quantum model (DQM), i.e. in accordance
with Definition 1, the perturbation of the corresponding classical system by the
Markov process. There is a simple connection between these Markov processes and the
quasisolutions of the Schrödinger equation. The connection between the Schrödinger
equation and the corresponding DQM is based on a following modification of the
traditional asymptotic expansion of solution (
        <xref ref-type="bibr" rid="ref4">4</xref>
        ).
      </p>
      <p>
        i S ( x,t )
Lemma 1. Let  (x, t) =  (x, t) e h
is some quasisolution (
        <xref ref-type="bibr" rid="ref4">4</xref>
        ), i.e.
ih

 t
      </p>
      <p>2
= H ( ) = − h2  </p>
      <p>x2 + U (x,t) + O(h2 ) ,
where  (x,t) =h (x,t) and S(x, t) = Sh (x, t) are real-valued. Then
  S (x, t)

  t</p>
      <p>
        +  S (xx, t) 2 + U (x) − h 2S (xx2, t)  (x, t) −
− h   (xt,t) + 2 S (xx,t) (xx,t) − h 2x(x2,t)  = O(h2 ) . (
        <xref ref-type="bibr" rid="ref5">5</xref>
        )
The converse is also true: if S(x, t) = Sh (x, t) and  (x,t) =h (x,t) is some
i S ( x,t)
quasisolution (
        <xref ref-type="bibr" rid="ref5">5</xref>
        ), then  (x, t) =  (x, t) e h
is some quasisolution (
        <xref ref-type="bibr" rid="ref4">4</xref>
        ).
      </p>
      <p>
        Now we show how the DQM of the Schrödinger equation is constructed from its
two-dimensional classical analogue
dx = p dp = − dU . (
        <xref ref-type="bibr" rid="ref6">6</xref>
        )
dt dt dx
Let us consider separately the terms of equation (
        <xref ref-type="bibr" rid="ref5">5</xref>
        ): Hamilton-Jacobi perturbed
equation
order h2 and for  (x,t) (
        <xref ref-type="bibr" rid="ref8">8</xref>
        ) holds with an accuracy of order h, then the function
 (x, t) =  (x, t) e hi S ( x,t ) satisfies (
        <xref ref-type="bibr" rid="ref4">4</xref>
        ) with an accuracy of the order h2 , i.e. it is a
quasisolution of the Schrödinger equation.
(
        <xref ref-type="bibr" rid="ref4">4</xref>
        )
(
        <xref ref-type="bibr" rid="ref7">7</xref>
        )
(
        <xref ref-type="bibr" rid="ref8">8</xref>
        )
      </p>
      <p>
        According to section 2.3 the DQM of the Schrödinger equation is determined by
1) the smooth dynamics from (
        <xref ref-type="bibr" rid="ref7">7</xref>
        ) and 2) its stochastic perturbation from (
        <xref ref-type="bibr" rid="ref8">8</xref>
        ).
      </p>
      <p>
        1) Consider the first two terms of the asymptotic expansion of the solution S(x, t)
of equation (
        <xref ref-type="bibr" rid="ref7">7</xref>
        ) with respect to the small parameter h:
      </p>
      <p>
        S(x, t) = S0 (x, t) + hS1(x, t) + (h2 ) . (
        <xref ref-type="bibr" rid="ref9">9</xref>
        )
      </p>
      <p>
        Substituting this expansion into (
        <xref ref-type="bibr" rid="ref7">7</xref>
        ), in a first approximation, we obtain the
Hamilton - Jacobie equation
S0 (x, t)
 t
      </p>
      <p> S0 (x, t) 2
+   + U (x) = 0</p>
      <p> x </p>
      <p>
        On the trajectory (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ) γ with the energy level  = −
the form
S0 (x, t) , this equation takes
      </p>
      <p> t
 S0 (x, t) 2
  + U (x) =  .
 x 
S0 ( x, t) = </p>
      <p>
         x
The velocity on γ is
 − U (x) =  р0(х) regardless of t.
Assuming that S1(x) is also independent of t, we find from (
        <xref ref-type="bibr" rid="ref7">7</xref>
        ) outside the turning
points x ( S0 (x, t) = 0 )
 x
S1 = 1  2S0
 x 2  x2
S0 = 1 
x 2 х
ln S0 .
      </p>
      <p> x</p>
      <p>
        Now the smooth DQM dynamics corresponding to the perturbed Hamilton - Jacobi
equation (
        <xref ref-type="bibr" rid="ref7">7</xref>
        ) is defined by the system:
dx = S =  S0 + h  S1 =  р0(х) + h  S1 ; dp = − dU ,
dt x  x  x  x dt dx
where in h - neighborhoods of turning points we smooth S1(x) , preserving it with
an accuracy of the order of h .
      </p>
      <p>
        2) DQM also includes stochastic disturbance, “white noise” in the configuration
space. If each point x0, in accordance with the smooth dynamics of the DQM, moves
t0+t S
along the trajectory (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ) during time Δt to the point x = x0 + t0 x (x( ), )d ;
and at this time scattering occurs, defined by the normal distribution with the
dispersion Δt, then [12] the distribution density φ(x, t) at the time t = t0 + Δt is a solution of
the diffusion equation
t  (x, t) = − S( xx, t) ( xx, t) + 22 2 (xx2, t) . (
        <xref ref-type="bibr" rid="ref12">12</xref>
        )
(
        <xref ref-type="bibr" rid="ref10">10</xref>
        )
(
        <xref ref-type="bibr" rid="ref11">11</xref>
        )
 d :
r (t )

      </p>
      <p>
        This equation is equivalent to (
        <xref ref-type="bibr" rid="ref8">8</xref>
        ): if φ(x, t) is a solution of (
        <xref ref-type="bibr" rid="ref8">8</xref>
        ), then this is a
solution of (
        <xref ref-type="bibr" rid="ref12">12</xref>
        ) for  2 = h .
      </p>
      <p>
        Let H (γ) be the energy value on the trajectory (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ) γ. Consider the integral of
“shortened action” on γ (t) = (x(t), p (t)) : s(t) =  p(x)dx = t p( ) 2 d . On
 (t) 0
each trajectory γ (t) other than a fixed point, the quantity s(t) is diffeomorphically
expressed through t and is called the optical time. Let ρ be a metric such that s(t) =
d = p(t) 2 dt . For a closed trajectory γ (γ(0) = γ( )) 2I(γ) = s( )
=  p(x)dx is ρ - length of this trajectory, i.e. optical time of its bypass.
      </p>
      <p>
        Lemma 2. For all sufficiently small h, the eigenvalue α of equation (
        <xref ref-type="bibr" rid="ref4">4</xref>
        ) with
accuracy of the order of h2 is equal to the value of the energy H(γ) on some closed path (
        <xref ref-type="bibr" rid="ref6">6</xref>
        )
γ. These and only these trajectories γ are such, for which the Bohr - Sommerfeld
condition holds with accuracy of order h2:
      </p>
      <p>I(γ) = h(n + 1 ) (n = 0, 1, …). (13)</p>
      <p>2</p>
      <p>
        Proof. Suppose that, on a closed trajectory (
        <xref ref-type="bibr" rid="ref11">11</xref>
        ) γ, (13) holds. Using the DQM
construction, we show that  = H(γ) is the eigenvalue of equation (
        <xref ref-type="bibr" rid="ref4">4</xref>
        ) with an accuracy
of the order of h2. Let S0(x, t) be the action on γ, i.e. the solution of the Hamilton
Jacobi equation (
        <xref ref-type="bibr" rid="ref10">10</xref>
        ) on γ  S0 (x, t) 2
      </p>
      <p> + U (x) =  = H ( ) . As the initial
 x 
condition for S0(x, t) we take</p>
      <p>x
S0 ( x,0) =  p0 ( y)dy , (14)</p>
      <p>x0
where р0(y) =  − U ( y) is velocity on γ, р0(x0) = 0, i.e. x0 is the abscissa of the
turning point on γ. Then</p>
      <p>
        S0 (x, t) = S0 (x, 0) − t + kt I ,
(15)
where kt is the number of turns in time t, πI is the ρ - length by γ between turning
points. And for S(x, t) = S0 (x,t) + hS1(x,t) , where in accordance with the construction
of DQM S1(x, t) = S1(x) from (
        <xref ref-type="bibr" rid="ref11">11</xref>
        ), equality (
        <xref ref-type="bibr" rid="ref12">12</xref>
        ) is approximately satisfied:
S (x, t) +  S (x, t) 2 + U (x) − h 2S (x, t) = O(h2 ) . (16)
t  x  x2
      </p>
      <p>We assume that the velocity function р0(x) on the closed curve γ without loss of
generality is analytic with an accuracy of the order of h2, otherwise approximating
р0(x) on γ analytic with this accuracy. Then outside the neighborhood of the turning
points this is also true for S0 (x, t) , S1(x), and in the neighborhood of the turning
S(x, t) = S0 (x, t) + hS1(x, t) = S (x,0) − t + kt (I +
 hi
2
) ,
where, as in (17), kt is the number of turns in time t.</p>
      <p>
        By definition, DQM also includes a stochastic perturbation defined on γ by
equation (
        <xref ref-type="bibr" rid="ref12">12</xref>
        ) with a diffusion coefficient  2 = h. Let φ0(x) be the density of the stationary
state for such a process. Then, for such dynamics at the initial density φ0(x) = φ(x, 0),
the solution of (
        <xref ref-type="bibr" rid="ref12">12</xref>
        ) φ(x, t) is different from φ0(x) by order h for any finite time t: φ(x,
t) – φ0(x) ~ h (due to scattering by “white noise” outside the limits of γ). Thus
S ( x, t)  0 ( x) h 2 0 ( x)
      </p>
      <p>
         x  x − 2  x2 = O(h) ,
which is equivalent to this option (
        <xref ref-type="bibr" rid="ref8">8</xref>
        ):
 0 ( x)
t
      </p>
      <p>S ( x, t)  0 ( x)
+ 2
 x  x</p>
      <p>
        2 0 ( x)
− h  x2
= O(h) .
point S1(x) we can continue analytically. When turning, the sign of S0 ( x, t) = 
 x
р0(х) changes, which in view of (
        <xref ref-type="bibr" rid="ref11">11</xref>
        ), implies the transition S1(x) to another branch of
the logarithm. This means adding to the value of the logarithm, 1i to S1 and then
2
1 hi to S. Therefore, in view of (15)
2
      </p>
      <p>Now replace h by hi in (18), (17) and (16). Then
 0 ( x) S ( x, t)  0 ( x)</p>
      <p>+ 2 − ih
t  x  x
 (x, t) =  0 ( x) e hi S ( x,t ) =  0 ( x) e hi (S ( x)−t )
( S (x, t)
t
+  S (x, t) 2 + U (x) − hi 2S (x, t) )φ(x, t) –</p>
      <p> x  x2
pair (α,  0 ( x) e hi S ( x) ) is quasisolution (quasimode) of the stationary Schrödinger
equation α ψ = H ψ with a small parameter h2. It follows that α is an eigenvalue of the
operator H with order accuracy h2.</p>
      <p>Indeed, assuming that d is the distance from α to the spectrum of the operator H,
║ ║ is the norm in L2 , and R = ( E − H )−1 is resolvent H, we obtain for ψ =
 0 ( x) e hi S ( x) in virtue of (25)
,
where B &gt; 0, whence d ≤ B h2 and then the lemma follows from the Weyl criterion,
QED.</p>
      <p>
        Proposition 2. For Schrödinger equation (
        <xref ref-type="bibr" rid="ref9">9</xref>
        ) with a quasiperiodic potential U(x)
for all sufficiently small h in the scattering region, the spectrum is continuous for all
ε, λ&gt; 0. In the region of vibrational motions
1. the spectrum is discrete if λ is rational.
2. If λ is irrational, then the point spectrum with increasing ε monotonically expands
to its closure – small segments around the original (at ε = 0) eigenvalues and for ε
of order h occupies this entire region. With a further increase in ε to an order of
1 h , such a picture of the spectrum is preserved, only the region of vibrational
motions expands ultimately to the entire space. For ε of order 1 h , with increasing
ε, the point spectrum monotonously narrows to segments converging to discrete
points.
      </p>
      <p>
        Proof. At ε = 0, the potential U(x) = cos x is periodic. In this case, in the region
H(γ) ≤ 1 of the phase space of the dynamical system (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ) (in the region of vibrational
motions), the trajectories γ are closed. By virtue of Lemma 2, the spectrum in this
region is discrete, and its points with an accuracy of the order of h2 are equal to the
energy values H (γ) on such trajectories γ for which condition (13) is satisfied. In the
region H(γ) &gt; 1 (the scattering region), the trajectories γ are unbounded and
unclosed, so the spectrum here is continuous and, with accuracy of the order of h2, is
equal to the energy H(γ) on the trajectories from this region. For the scattering region,
this will always be true with increasing ε.
      </p>
      <p>As  increases from zero, the periodicity of the potential U(x) disappears, on the
interval [2k; 2 (k + 1)] it has the form</p>
      <p>U (x) = cos(x) + cos(2k + x) (x [0;2 ]).
(26)
If λ is rational and λ = p , then there are no more than q different such potentials
q
and for each of them the spectrum is discrete. For irrational λ, the points 2kλ modulo
2 everywhere densely fill the segment [0; 2] and their closure coincides with the
segment.</p>
      <p>
        Consider on the segment [0; 2] dynamic system (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ) with potential U (x) =
cos(x) + cos( + x) , smooth in the parameters ε  0 and   [0; 2], For  =
2kλ (mod 2) for the potential U ρ – length I = I (H, ε, ) of closed trajectory
with given energy H and ε &gt; 0 is equal to ρ – length trajectories for the initial
potential U (26) with the same H and ε on the interval [2k; 2 (k + 1)].
      </p>
      <p>
        As for potential U dI(H , , )  0 at ε = 0, then this is also true for
suffidH
ciently small ε &gt; 0. Let the inverse function f(I) = f(I, , ε) associates the ρ - length
I of a closed trajectory with its energy level H. According to Lemma 2, for I =
h(n + 1 ) (n = 0, 1, …) all this H = f(I, , ε) and there only are the eigenvalues (
        <xref ref-type="bibr" rid="ref4">4</xref>
        )
2
with order of accuracy h2. Since the dependence of f on  is continuous, then for fixed
I and ε &gt; 0 image of the segment [0; 2] along the  axis is some segment KI along
the H axis.
      </p>
      <p>The length of the segment KI smoothly depends on ε, and for sufficiently small h
and ε of order h it increases approximately linearly with increasing ε. Therefore, with
increasing ε, the union of the segments KI over all I = h(n + 1 ) (n = 0, 1, …) will
2
cover all values of energy in the field of oscillatory movements.</p>
      <p>All the above considerations remain valid with a further increase in ε, and therefore
the spectral picture does not change, only the range of vibrational motions expands.
As ε → ∞, this region occupies the entire phase space. Moreover, in the spectral
pattern in this region, a process occurs that is opposite to what was when ε changed from
zero to h. Namely, the point spectrum narrows to segments converging in the limit to
discrete points corresponding to phase curves with ρ – length I = h(n + 1 ) (n = 0,
2</p>
      <p>At ε → ∞, i.e. ~
QED.
4</p>
      <p>Conclusion
ih
</p>
      <p>~ = − h
 t
2 2
~x2</p>
      <p>+ (~ cos x + cos  x) .</p>
      <p>
        → 0 we back to the periodic case with potential U(x) = cos x,
1, …) for potential cos λx. This follows from the symmetry of the plots 0 &lt; ε &lt; h and
1 h &lt; ε &lt; ∞: divide equation (
        <xref ref-type="bibr" rid="ref4">4</xref>
        ) by ε
ih 
  t
As a result of the replacement of variables ~t =  t, ~x =
.
 x, ~ = 1 , we obtain

The structural stability of a mathematical model is a necessary condition for its
correctness. But after S. Smale's works it became clear that in smooth dynamics the
system of a general form is not structurally stable and therefore there is no strict
mathematical basis for modeling and computational analysis of systems. The contradiction
appeared in science: according to physicists dynamics is simple and universal.
The solution to this problem was proposed based on the construction of dynamic
quantum models (DQM). From the assumption that quantum effects are caused by
unrecoverable “white noise”, a certain mathematical model of quantum mechanics
already follows and is essentially unambiguous. This model is simply connected with
the traditional one. Construction of such models can be considered as an asymptotic
method for solving spectral problems, for example, for the one-dimensional system
with the quasiperiodic potential.
      </p>
      <p>But the definition of DQM is not formally related to Hamiltonian systems; it is
defined for any ordinary differential equation or any diffeomorphism on any smooth
Riemannian manifold. DQM is defined and constructed universally for both
Hamiltonian systems and systems with the truth function. As a result, for example, the point
of the DQM spectrum is interpreted exactly as the average value of truth from
approximate logical conclusions. Quantization with the Bohr-Sommerfeld condition also
extends to systems with a truth function.</p>
      <p>Hopefully this will allow a new approach to the problems of dynamical systems that
using logical operations: algorithms, theorems, software applications.</p>
    </sec>
  </body>
  <back>
    <ref-list>
      <ref id="ref1">
        <mixed-citation>
          1.
          <string-name>
            <surname>Morrison</surname>
            ,
            <given-names>M.</given-names>
          </string-name>
          :
          <article-title>Models, measurement and computer simulation: the changing face of experimentation</article-title>
          .
          <source>Philosophical Studies</source>
          ,
          <volume>143</volume>
          ,
          <fpage>33</fpage>
          -
          <lpage>57</lpage>
          (
          <year>2012</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref2">
        <mixed-citation>
          2.
          <string-name>
            <surname>Dubois</surname>
          </string-name>
          , G.:
          <article-title>Modeling and Simulation: Challenges and Best Practices for Industry</article-title>
          , CRC Press, Boca Raton (
          <year>2018</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref3">
        <mixed-citation>
          3.
          <string-name>
            <surname>Peschard</surname>
            ,
            <given-names>I.</given-names>
          </string-name>
          :
          <article-title>Modeling and Experimenting</article-title>
          . In: P. Humphreys and C. Imbert (eds), Models, Simulations, and Representations. pp.
          <fpage>42</fpage>
          -
          <lpage>61</lpage>
          , Routledge, London: (
          <year>2010</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref4">
        <mixed-citation>
          4.
          <string-name>
            <surname>Winsberg</surname>
          </string-name>
          , E.:
          <article-title>Science in the Age of Computer Simulation</article-title>
          , The University of Chicago Press, Chicago (
          <year>2010</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref5">
        <mixed-citation>
          5.
          <string-name>
            <surname>Yang</surname>
            ,
            <given-names>X. S.</given-names>
          </string-name>
          : Introduction to Computational Mathematics, World Scientific Publishing Company, London (
          <year>2008</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref6">
        <mixed-citation>
          6.
          <string-name>
            <surname>Teschl</surname>
          </string-name>
          , G.:
          <article-title>Ordinary Differential Equations and Dynamical Systems</article-title>
          , Volume
          <volume>140</volume>
          ,
          <source>Amer. Math. Soc.</source>
          ,
          <string-name>
            <surname>Providence</surname>
          </string-name>
          (
          <year>2012</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref7">
        <mixed-citation>
          7.
          <string-name>
            <surname>Arnold</surname>
          </string-name>
          , V.
          <article-title>Mathematical methods of classical mechanics</article-title>
          , Vol.
          <volume>60</volume>
          ,
          <string-name>
            <surname>Springer</surname>
            <given-names>Science</given-names>
          </string-name>
          &amp; Business
          <string-name>
            <surname>Media</surname>
          </string-name>
          , New York (
          <year>1982</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref8">
        <mixed-citation>
          8.
          <string-name>
            <surname>Smale</surname>
            ,
            <given-names>S.</given-names>
          </string-name>
          :
          <article-title>Structurally stable systems are not dense</article-title>
          .
          <source>Matematika</source>
          <volume>11</volume>
          (
          <issue>4</issue>
          ),
          <fpage>107</fpage>
          -
          <lpage>112</lpage>
          (
          <year>1967</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref9">
        <mixed-citation>
          9.
          <string-name>
            <surname>Tesse</surname>
          </string-name>
          , E.:
          <article-title>Principals of Dynamic Systems and the Foundations of Quantum Physics, SIAM (</article-title>
          <year>2011</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref10">
        <mixed-citation>
          10.
          <string-name>
            <surname>Weissblut</surname>
            ,
            <given-names>A.</given-names>
          </string-name>
          :
          <source>Computational Modeling and Structural Stability In: Proceedings of the 15th International Conference on ICT in Education, Research and Industrial Applications</source>
          . Integration, Harmonization and
          <string-name>
            <given-names>Knowledge</given-names>
            <surname>Transfer</surname>
          </string-name>
          . Volume II: Workshops, pp.
          <fpage>552</fpage>
          -
          <lpage>567</lpage>
          , CEUR-WS, Kherson, Ukraine (
          <year>2019</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref11">
        <mixed-citation>
          11.
          <string-name>
            <surname>Weissblut</surname>
            <given-names>A.</given-names>
          </string-name>
          (
          <year>2011</year>
          )
          <article-title>Non-Hamiltonian Quantum Mechanics and the Numerical Researches of the Attractor of a Dynamical System Informational Technologies in Education 11</article-title>
          , pp.
          <fpage>73</fpage>
          -
          <lpage>77</lpage>
          (
          <year>2012</year>
          ).
        </mixed-citation>
      </ref>
      <ref id="ref12">
        <mixed-citation>
          12.
          <string-name>
            <surname>Stirzaker</surname>
            ,
            <given-names>D.</given-names>
          </string-name>
          :
          <source>Stochastic Processes and Models</source>
          , Oxford University Press, Oxford (
          <year>2005</year>
          ).
        </mixed-citation>
      </ref>
    </ref-list>
  </back>
</article>