Developed Method. Interactions and Their Quantum Picture

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Developed Method. Interactions and Their Quantum Picture

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Piotr Ogonowski^*

This version is not peer-reviewed.

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Submitted:

16 June 2023

Posted:

16 June 2023

Read the latest preprint version here

A peer-reviewed article of this preprint also exists.

Abstract

By developing the previously proposed method of combining continuum mechanics with Einstein Field Equations, a complete description of the physical system was obtained. The density of the Lagrangian for the system turns out to be equal to the invariant of the electromagnetic field tensor, vanishing four-divergence of canonical four-momentum appears to be consequence of the Poyinting theorem, and explicit form of one of gauges of the electromagnetic four-potential was introduced. A quantum picture of the system was also proposed, leading to the Klein-Gordon equation, which seems to finally reconcile the curvilinear description, classic relativistic description and quantum description of the physical system.

Keywords:

Subject:

Physical Sciences - Theoretical Physics

1. Introduction

Over the past decades, great strides have been made in attempts to combine quantum description of interactions with General Relativity [1]. There are currently many promising approaches to connecting the quantum mechanics and General Relativity, including perhaps the most promising ones: Loop Quantum Gravity [2,3,4], String Theory [5,6,7] and Noncommutative Spacetime Theory [8,9].

A lot of work has also been done to clear up some challenges related to General Relativity and

Λ C M D

model [10]. An explanation for the problem of dark energy [11] and dark matter [12] is still being sought, and efforts are still being made to explain the origin of the cosmological constant [13,14,15].

The author also tries to bring his own contribution to the explanation of the above physics challenges, based on a recently discovered method, described in [16]. As this article will show, this method seems very promising and can help clarify at least some of the issues mentioned above.

According to conclusions from [16], the description of motion in curved spacetime and its description in flat Minkowski spacetime with fields are equivalent, and the transformation between curved spacetime and Minkowski spacetime is known. This allows for a significant simplification of research, because the results obtained in flat Minkowski spacetime can be easily transformed into curved spacetime. The last missing link seems to be the quantum description.

In this article, the author will focus on developing the method proposed in [16] in such a way, as to obtain the convergence of the description with the description of quantum mechanics. In the first chapter, the Lagrangian density for the system will be derived, allowing to obtain the tensor described in [16]. These conclusions will be used later in the article to propose quantum description of the system.

The author uses the Einstein summation convention, metric signature

(+, -, -, -)

and commonly used notations. In order to facilitate the analysis of the article, the key conclusions from [16] are quoted in the subsection below.

1.1. Short summary of the method

According to [16], stress-energy tensor

T^{α β}

for a system in a given spacetime described by a metric tensor

g^{α β}

is equal to

T^{α β} = ϱ U^{α} U^{β} - (c^{2} ϱ + Λ_{ρ}) (g^{α β} - ξ h^{α β})

(1)

where

ϱ_{o}

is for rest mass density and

ϱ \equiv ϱ_{o} γ

(2)

\frac{1}{ξ} \equiv \frac{1}{4} g_{μ ν} h^{μ ν}

(3)

Λ_{ρ} \equiv \frac{1}{4 μ_{o}} F^{α μ} g_{μ γ} F^{β γ} g_{α β}

(4)

h^{α β} \equiv 2 \frac{F^{α δ} g_{δ γ} F^{β γ}}{\sqrt{F^{α δ} g_{δ γ} F^{β γ} g_{μ β} F_{α η} g^{η ξ} F_{ξ}^{μ}}}

(5)

where

F^{α β}

represents electromagnetic field tensor, and where the stress–energy tensor for electromagnetic filed, denoted as

Υ^{α β}

may be presented as follows

Υ^{α β} \equiv Λ_{ρ} (g^{α β} - ξ h^{α β}) = Λ_{ρ} g^{α β} - \frac{1}{μ_{o}} F^{α δ} g_{δ γ} F^{β γ}

(6)

Thanks to the proposed amendment to the continuum mechanics, in flat Minkowski spacetime occurs

\partial_{α} U^{α} = - \frac{d γ}{d t} \to \partial_{α} ϱ U^{α} = 0

(7)

thus denoting four-momentum density as

ϱ U^{μ} = ϱ_{o} γ U^{μ}

, total four-force density

f^{μ}

acting in the system is

f^{μ} \equiv ϱ A^{μ} = \partial_{α} ϱ U^{μ} U^{α}

(8)

Denoting rest charge density in the system as

ρ_{o}

and

ρ \equiv ρ_{o} γ

(9)

electromagnetic four-current

J^{α}

is equal to

J^{α} \equiv ρ U^{α} = ρ_{o} γ U^{α}

(10)

The pressure p in the system is equal to

p \equiv c^{2} ϱ + Λ_{ρ}

(11)

In the flat Minkowski spacetime, total four-force density

f^{α}

acting in the system calculated from

\partial_{β} T^{α β} = 0

is the sum of electromagnetic (

f_{E M}^{α}

), gravitational (

f_{g r}^{α}

) and other (

f_{o t h}^{α}

) four-force densities

f^{α} = \{\begin{matrix} f_{E M}^{α} \equiv - Λ_{ρ} \partial_{β} ξ h^{α β} (e l e c t r o m a g n e t i c) \\ + \\ f_{g r}^{α} \equiv (g^{α β} - ξ h^{α β}) \partial_{β} p (g r a v i t a t i o n a l) \\ + \\ f_{o t h}^{α} \equiv \frac{ϱ c^{2}}{Λ_{ρ}} f_{E M}^{α} (o t h e r) \end{matrix}

(12)

As was shown in [16], in curved spacetime (

g_{α β} = h_{α β}

) presented method reproduces Einstein Field Equations with an accuracy of

\frac{4 π G}{c^{4}}

constant and with cosmological constant

Λ

dependent on invariant of electromagnetic field tensor

F^{α γ}

Λ = - \frac{π G}{c^{4} μ_{o}} F^{α μ} h_{μ γ} F^{β γ} h_{α β} = - \frac{4 π G}{c^{4}} Λ_{ρ}

(13)

where

h_{α β}

appears to be metric tensor of the spacetime in which all motion occurs along geodesics and where

Λ_{ρ}

describes vacuum energy density.

It is also shown, that Einstein tensor describes the spacetime curvature related to vanishing in curved spacetime four-force densities

f_{g r}^{α} + f_{o t h}^{α}

2. Lagrangian density for the system

Since for the considered method the transition to curved spacetime is known (based on electromagnetic field tensor), the rest of the article will focus on the calculations in the Minkowski spacetime with presence of fields, where

η^{α β}

represents Minkowski metric tensor.

Using a simplified notation

\frac{d ln (p)}{d τ} = U_{μ} \partial^{μ} ln (p) = U_{μ} \frac{\partial^{μ} p}{p}

(14)

it can be seen that the four-force densities resulting from the obtained stress-energy tensor (12) in flat Minkowski spacetime can be written as follows

\{\begin{matrix} f_{g r}^{α} = (η^{α β} - ξ h^{α β}) \partial_{β} p = \frac{d ln (p)}{d τ} ϱ U^{α} - T^{α β} \partial_{β} ln (p) \\ f_{E M}^{α} = \frac{Λ_{ρ}}{p} (f^{α} - f_{g r}^{α}) \\ f_{o t h}^{α} = \frac{ϱ c^{2}}{p} (f^{α} - f_{g r}^{α}) \end{matrix}

(15)

where

f_{E M}^{μ}

can also be represented in terms of electromagnetic four-potential and four-current. This means that to fully describe the system and derive the Lagrangian density, it is enough to find an explicit equation for the gravitational force or some gauge of electromagnetic four potential.

Referring to definitions from Section 1.1 one may notice, that by proposing following electromagnetic four-potential

A^{μ}

A^{μ} \equiv - \frac{Λ_{ρ}}{p} \frac{ϱ_{o}}{ρ_{o}} U^{μ}

(16)

one obtains electromagnetic four-force density

f_{E M}^{α}

in form of

f_{E M}^{α} = J_{β} (\partial^{α} A^{β} - \partial^{β} A^{α}) = \frac{Λ_{ρ}}{p} (f^{α} - \frac{d ln (p)}{d τ} ϱ U^{α} + ϱ c^{2} \partial^{α} ln (p))

(17)

where

J_{β}

is electromagnetic four-current and where Minkowski metric property was utilized

U_{β} U^{β} = c^{2} \to U_{β} \partial^{α} U^{β} = \frac{1}{2} \partial^{α} (U_{β} U^{β}) = 0

(18)

and where the forces in the system can be described by the following equality

J_{β} (\partial^{α} A^{β} - \partial^{β} A^{α}) + ϱ U_{β} (\partial^{β} \frac{ϱ c^{2}}{p} U^{α} - \partial^{α} \frac{ϱ c^{2}}{p} U^{β}) = ϱ U_{β} (\partial^{β} U^{α} - \partial^{α} U^{β}) = f^{α}

(19)

Comparing (15) and (17) it is seen, that introduced electromagnetic four-potential yields

0 = (T^{α β} - ϱ c^{2} η^{α β}) \partial_{β} ln (p)

(20)

which is equivalent to imposing following condition on normalized stress-energy tensor

0 = \partial_{β} (\frac{T^{α β}}{T r (T^{α β})}) + \partial^{α} ln (T r (T^{α β}))

(21)

and yields gravitational four-force density in Minkowski spacetime in form of

f_{g r}^{μ} = ϱ (\frac{d ln (p)}{d τ} U^{μ} - c^{2} \partial^{μ} ln (p))

(22)

Now, one may show, that proposed electromagnetic four-potential leads to correct solutions.

At first, recalling the classical Lagrangian density [17] for electromagnetism one may show why, in the light of the conclusions from [16] and above, it does not seem to be correct, and thus does not allow to create a symmetric stress-energy tensor [18]. The classical value of the Lagrangian density for electromagnetic field, written with the notation used in the article, is

- L_{E M c l a s s i c} = Λ_{ρ} + A^{μ} J_{μ}

(23)

In addition to the obvious doubt that by taking the different gauge of the four-potential

A^{μ}

one changes the value of the Lagrangian density, one may notice, that with considered electromagnetic four-potential, such Lagrangian density is equal to

- L_{E M c l a s s i c} = Λ_{ρ} - \frac{Λ_{ρ}}{p} \frac{ϱ_{o}}{ρ_{o}} U^{μ} U_{μ} ρ_{o} γ = Λ_{ρ} - \frac{Λ_{ρ} ϱ c^{2}}{p} = \frac{Λ_{ρ}^{2}}{p}

(24)

As it is seen, above Lagrangian density is not invariant under gradient over four-position and

A^{μ}

and

J_{μ}

are dependent, what is not taken into account in classical calculation

\frac{A^{α}}{A^{μ} A_{μ}} = \frac{J^{α}}{A^{μ} J_{μ}}

(25)

Above yields

\frac{\partial ln (\frac{1}{\sqrt{A^{μ} A_{μ}}})}{\partial A_{α}} = - \frac{J^{α}}{A^{μ} J_{μ}} = \frac{p}{ϱ c^{2}} \frac{J^{α}}{Λ_{ρ}}

(26)

One may decompose

ln (\frac{1}{\sqrt{A^{μ} A_{μ}}}) = ln (\frac{p ρ_{o}}{Λ_{ρ} ϱ_{o} c}) = ln (p) - ln (Λ_{ρ}) - ln (\frac{ϱ_{o} c}{ρ_{o}})

(27)

and since

\frac{ϱ_{o} c}{ρ_{o}}

are constants, one may simplify (26) to

\frac{\partial ln (p)}{\partial A_{α}} - \frac{\partial ln (Λ_{ρ})}{\partial A_{α}} = \frac{p}{ϱ c^{2}} \frac{J^{α}}{Λ_{ρ}} = \frac{J^{α}}{ϱ c^{2}} + \frac{J^{α}}{Λ_{ρ}}

(28)

Above yields

\frac{\partial ln (Λ_{ρ})}{\partial A_{α}} = - \frac{J^{α}}{Λ_{ρ}}

(29)

which leads to the conclusion that

Λ_{ρ}

acts as the Lagrangian density for the system

\frac{\partial Λ_{ρ}}{\partial A_{α}} = \partial_{ν} (\frac{\partial Λ_{ρ}}{\partial (\partial_{ν} A_{α})}) = - J^{α}

(30)

thus stress-energy tensor for the system is equal to

T^{α β} = \frac{1}{μ_{o}} F^{α γ} \partial^{β} A_{γ} - Λ_{ρ} η^{α β}

(31)

In fact, the proof of correctness of the electromagnetic field tensor (noted as

Υ^{α β}

) allows to see this solution

f_{E M}^{β} = \partial_{α} Υ^{α β} = J^{γ} F_{γ}^{β} - \frac{1}{μ_{o}} F^{α γ} \partial_{α} F_{γ}^{β}

(32)

what yields following property of electromagnetic field tensor

F^{α γ} \partial_{α} \partial_{γ} A^{β} = F^{α γ} \partial^{β} \partial_{α} A_{γ}

(33)

Using the above substitution, one may note

\partial_{α} Υ^{α β} = \partial_{α} \frac{1}{μ_{o}} F^{α γ} \partial_{γ} A^{β} - \partial_{α} \frac{1}{μ_{o}} F^{α γ} \partial^{β} A_{γ} = \frac{1}{μ_{o}} F^{α γ} \partial^{β} \partial_{α} A_{γ} - J^{γ} \partial_{γ} A^{β} - \partial_{α} \frac{1}{μ_{o}} F^{α γ} \partial^{β} A_{γ}

(34)

Therefore the invariance of

Λ_{ρ}

with respect to

A_{α}

and

\partial_{ν} A_{α}

is both a condition on the correctness of the electromagnetic stress-energy tensor and on

Λ_{ρ}

in the role of Lagrangian density

0 = \frac{\partial Λ_{ρ}}{\partial (\partial_{α} A_{γ})} \partial^{β} (\partial_{α} A_{γ}) + \frac{\partial Λ_{ρ}}{\partial A_{γ}} \partial^{β} A_{γ} = \frac{1}{μ_{o}} F^{α γ} \partial^{β} \partial_{α} A_{γ} - J^{γ} \partial^{β} A_{γ} = \partial_{α} \frac{1}{μ_{o}} F^{α γ} \partial^{β} A_{γ}

(35)

what yields for (34) that

\partial_{α} Υ^{α β} = J^{γ} \partial^{β} A_{γ} - J^{γ} \partial_{γ} A^{β} = f_{E M}^{β}

(36)

Equations (1), (6) and (31) yield

\frac{1}{μ_{o}} F^{α γ} \partial_{γ} A^{β} = ϱ U^{α} U^{β} - \frac{c^{2} ϱ}{Λ_{ρ}} Υ^{α β}

(37)

what yields second representation of the stress-energy tensor

T^{α β} = \frac{p}{ϱ c^{2}} \cdot \frac{1}{μ_{o}} F^{α γ} \partial_{γ} A^{β} - \frac{Λ_{ρ}}{c^{2}} U^{α} U^{β} = \frac{p}{ϱ c^{2}} \partial_{γ} \frac{1}{μ_{o}} F^{α γ} A^{β}

(38)

After four-divergence, it gives additional expression for relation between forces and gives useful clues about the behavior of the system when transitioning to the description in curved spacetime.

3. Hamiltonian density and quantum picture

Since

\frac{\partial Λ_{ρ}}{\partial (\partial A_{γ} / \partial x_{α})} = \frac{1}{μ_{o}} F^{α γ} \to \frac{\partial Λ_{ρ}}{\partial (\partial A_{γ} / \partial x_{0})} = \frac{1}{μ_{o}} F^{0 γ}

(39)

thus noting Hamiltonian density in terms of the Lagrangian density [19] (and also from (31)) one gets

H = (\frac{\partial Λ_{ρ}}{\partial (\partial A_{γ} / \partial x_{0})}) \frac{\partial A_{γ}}{\partial x_{0}} - Λ_{ρ} = \frac{1}{μ_{o} c} F^{0 γ} \frac{\partial A_{γ}}{\partial t} - Λ_{ρ}

(40)

where conjugate momentum field

Π^{γ}

Π^{γ} \equiv \frac{1}{μ_{o}} F^{0 γ}

(41)

As it is seen, above Hamiltonian density agrees with the classical Hamiltonian density for electromagnetic field [19] except that this Hamiltonian density was currently only considered for sourceless regions and only to consider the system with electromagnetic field. According to the result above, this Hamiltonian density describes the entire physical system, taking into account all known interactions. Above, therefore, significantly simplifies quantum field theory equations [20,21,22].

At first one may notice, that in transformed (31)

- T^{α 0} = - \frac{1}{μ_{o}} F^{α γ} \partial_{γ} A^{0} + Υ^{α 0}

(42)

first row of electromagnetic stress-energy tensor

Υ^{α 0}

is a four-vector, representing energy density of electromagnetic field and Poynting vector [23] - the Poynting four-vector. Therefore vanishing four-divergence of the

T^{α 0}

must represent Poynting theorem. Indeed, properties (33) and (35) provide such equality

0 = - \partial_{α} T^{α 0} = J_{γ} F^{0 γ} + \partial_{α} Υ^{α 0}

(43)

which also shows, that for the constant total energy of the system,

T^{α 0}

is independent of the four-position.

Secondly, it can be assumed that after integration of the

T^{α 0}

with respect to the volume, the total energy transported in the isolated system should be the sum of the four-momentums related to matter and fields. Therefore, by analogy with the Poyting four-vector

\frac{1}{c} Υ^{α 0}

, one may introduce a four-vector

S_{f}^{α}

understood as its equivalent for the remaining fields and rewrite equation (42) taking into account the entire energy transport

- T^{α 0} = c ϱ_{o} U^{α} + c S_{f}^{α} + Υ^{α 0}

(44)

where

c ϱ_{o} U^{β} + c S_{f}^{β} = - \frac{1}{μ_{o}} F^{0 γ} \partial_{γ} A^{β} = U^{β} \cdot \frac{ϱ_{o} Λ_{ρ}}{μ_{o} ρ_{o}} F^{0 γ} \partial_{γ} \frac{1}{p} + \frac{ϱ_{o} Λ_{ρ}}{p μ_{o} ρ_{o}} F^{0 γ} \partial_{γ} U^{β}

(45)

One may now introduce auxiliary variable

ε

with the energy density dimension, defined as follows

ε \equiv - \frac{1}{c μ_{o}} F^{0 γ} \frac{d A_{γ}}{d t}

(46)

and comparing the result

- \frac{1}{c γ} U_{β} T^{0 β} = ε + Λ_{ρ}

(47)

between the two tensor definitions (31), (38) one can see that it must hold

- \frac{p}{ϱ c^{2}} \cdot \frac{1}{μ_{o}} F^{0 γ} \partial_{γ} A^{β} = \frac{γ ε}{c} U^{β} + \frac{Λ_{ρ}}{γ c^{2} μ_{o} ρ_{o}} F^{0 γ} \partial_{γ} U^{β}

(48)

because the second component of above vanishes contracted with four-velocity, due to the property of the Minkowski metric (18). Terefore

c S_{f}^{β} = (γ ε \frac{ϱ c}{p} - ϱ_{o} c) U^{β} + \frac{ϱ_{o} Λ_{ρ}}{p μ_{o} ρ_{o}} F^{0 γ} \partial_{γ} U^{β}

(49)

Based on the knowledge of the existing Lagrangians, a probable assumption can be made at this point that

γ ε = ϱ_{o} c^{2}

(50)

what yields

c S_{f}^{β} = c ρ_{o} A^{β} + \frac{ϱ_{o} Λ_{ρ}}{p μ_{o} ρ_{o}} F^{0 γ} \partial_{γ} U^{β}

(51)

The above result should not be surprising, because considering all interactions in the cannonical four-momentum density, actually one of its components should be the electromagnetic four-potential density.

Finally, one may define another gauge

{\bar{A}}_{γ}

of electromagnetic four-potential

A_{γ}

in following way

{\bar{A}}^{γ} \equiv A^{γ} - \partial^{γ} A^{β} X_{β} = - X_{β} \partial^{γ} A^{β}

(52)

and note, that

- X_{β} T^{0 β} = \frac{1}{μ_{o}} F^{0 γ} {\bar{A}}_{γ} + X_{β} Υ^{0 β}

(53)

Since for constant total energy of the system

\partial^{α} X_{β} T^{0 β} = T^{0 α}

(54)

this brings three more important insights:

$X_{β} T^{0 β}$ plays a role of the density of Hamilton’s principal function,
Hamilton’s principal function may be expressed based on the electromagnetic field only (so in the absence of the electromagnetic field it disappears),
$\frac{1}{c γ} U_{β} T^{0 β} = - ϱ_{o} c^{2} \frac{1}{γ} - Λ_{ρ}$ may also act as a Lagrangian density, used in the classic relativistic description of the system based on four-vectors.

One may now summarize the above and propose a method for quantizing the system and for the description of the system with the use of classical field theory.

At first, it should be noted, that the above reasoning changes the interpretation of what the relativistic principle of least action means. As one may conclude from above, there is no inertial system in which no fields act, and in the absence of fields, the Lagrangian, the Hamiltonian and Hamilton’s principal function vanish. Since the metric tensor (5) for description in curved spacetime depends on the electromagnetic field tensor only, it seems clear, that the absence of the electromagnetic field means actually the disappearance of spacetime and the absence of any action.

One may then introduce generalized, canonical four-momentum

H^{μ}

as four-gradient on Hamilton’s principal function S, where relation with wave four-vector

K^{μ}

occurs

H^{μ} \equiv - \frac{1}{c} \int T^{0 μ} d^{3} x \equiv - \partial^{μ} S \equiv ℏ K^{μ}

(55)

where

- S \equiv H^{μ} X_{μ}

(56)

and where

H^{μ}

and

K^{μ}

do not depend on four-position. One may also conclude from previous findings, that canonical four-momentum should be in form of

H^{μ} = P^{μ} - V^{μ}

(57)

where

- V^{α} \equiv \int S_{f}^{α} + \frac{1}{c} Υ^{0 α} d^{3} x

(58)

and where four-momentum

P^{μ}

may be now considered as just other gauge of this four-potential

\partial^{α} P^{μ} = \partial^{α} V^{μ}

(59)

Since in the limit of the inertial system one gets

P^{μ} X_{μ} = m c^{2} τ

, therefore, to ensure the decay of Hamilton’s principal function in the inertial system, one can expect that

V^{μ} X_{μ} \equiv m c^{2} τ

(60)

what also yields vanishing in the inertial system Lagrangian in form of

- L = \frac{1}{γ} F^{μ} X_{μ}

(61)

where

F^{μ}

is four-force, and

H^{μ} H_{μ} + m^{2} c^{2} = 2 m F^{μ} X_{μ} - V^{μ} V_{μ}

(62)

Using the above definitions, the action, the Hamiltonian and Lagrangian vanish for an inertial system (when

P^{μ} = V^{μ}

) as expected. To ensure compatibility with the equations of quantum mechanics it is enough to assume the following

- γ L = X_{μ} F^{μ} = \frac{V^{μ} V_{μ}}{2 m}

(63)

Thanks to above, by introducing quantum wave function

Ψ

in form of

Ψ \equiv e^{\pm i K^{μ} X_{μ}}

(64)

from (62) one obtains Klein-Gordon equation

(□ + \frac{m^{2} c^{2}}{ℏ^{2}}) Ψ = 0

(65)

which allows for further analysis of the system in the quantum approach, eliminating the problem of negative energy appearing in solutions [24].

The above representation allows the analysis of the system in the quantum approach, classical approach based on (42) and the introduction of a field-dependent metric in (5) for curved spacetime, which connects previously divergent descriptions of physical systems.

4. Conclusions and Discussion

As shown above, the proposed method of physical systems analysis summarized in Section 1.1 seems to be very promising area of farther research. By imposing condition (20) on normalized stress-energy tensor, one obtains consistent results, developing the knowledge of the physical system:

Lagrangian density for the systems appears to be equal to $L = Λ_{ρ} = \frac{1}{4 μ_{o}} F^{α β} F_{α β}$
Generalized cannonical four-momentum is known, it is equal to volume integration of (44), it includes electromagnetic four-potential and other terms responsible for other fields
Some gauge of electromagnetic four-potential may be expressed as $A^{μ} = - \frac{Λ_{ρ}}{p} \frac{ϱ_{o}}{ρ_{o}} U^{μ}$
The vanishing four-divergence of the canonical four-momentum turns out to be the consequence of Poynting theorem
Four-force densities acting in the system may be expressed as shown in (15) where gravitational four-force is dependent on the pressure p in the system as shown in (22)

It also seems, that this approach allows to combine previously divergent methods of curvilinear and classic description with the quantum description and simplifies further research on the quantum picture of individual fields, significantly simplifying equations of the quantum field theory. Such approach also drives in natural way to Klein-Gordon equation (62).

Further analysis using the variational method may also lead to next discoveries regarding both the theoretical description of quantum fields and elementary particles associated with them, and the possibility of experimental verification of the obtained results.

5. Statements

Data sharing is not applicable to this article, as no datasets were generated or analyzed during the current study.

The author did not receive support from any organization for the submitted work.

The author has no relevant financial or non-financial interests to disclose.

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Developed Method. Interactions and Their Quantum Picture

Abstract

Keywords:

Subject:

1. Introduction

1.1. Short summary of the method

2. Lagrangian density for the system

3. Hamiltonian density and quantum picture

4. Conclusions and Discussion

5. Statements

References

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