Ali Rıza ŞAHİN
Gazi Mahallesi İsmet Paşa
Caddesi
We propose interaction space model for field theory and we
focus on this model in order to give details about it. Later, we will show that
Maxwell Equations can be derived exactly, by using the interaction space
concept.
This study is based on completely new ideas in order to achieve a new point
of view for the field theory, elementary particles and interactions. Although
the ideas are new, we are familiar them because of classical mechanics. In
construction of this assumption, there are important motivations of Einstein’s
General Relativity Theory and Kaluza-Klein Theory, especially the latter. Certainty
and objectivity of classical mechanics and similarities between classical
mechanics and field theory lead us to suggest there may or must be a special
space for field theory. This space is defined once; it is easier to get results
of it. Consequently; we define interaction space and try to find equations of
motion by receiving inspirations from General Relativity and Kaluza-Klein,
although we do not use these theories in appearance.
Before we define the interaction space; we will remind some points about
classical mechanics. In classical mechanics; the motion of any point is
described by a position vector (
).
means distance of the point
from an O origin of a fixed three-dimensional
Euclidean space. We can show any point of this space by unique
vector (Figure
,
where
are coordinates and
are unit vectors of the space (
). Unit vectors satisfy
.
For
a moving point in a fixed space, coordinates will be some functions of the time
(
) as
.
If
a rotating frame of reference with respect to a fixed space, unit vectors
become some functions of the time (Figure
.
In order to determine motion of an object which
refers we must calculate equations of the motion. There are
several methods to do this. However; we want to establish a relation between
geometrical structure and motion of the object, similar to General Relativity
and Kaluza-Klein Theory. There is a well-known way in order to do this; it is
geodesic motion of the system. By
determining geodesics of a system we can find equations of motion. Consequently,
metric of the system must be found firstly. The metric is
. (
By
skipping some details; for a classical mechanics system
can
be written, where
is the kinetic energy and
mass of the object.
Geodesics of the system can be derived from
,
where
and
are endpoints of the action.
Now; we will try to adopt these classical mechanics’ variational
principles of the geodesics to field theory. But; we must determine a coordinate
system or space for field theory first of all. In classical mechanics; systems
can be observable and all things depend on the time, so defining an exact
coordinate system is very easy. In field theory; systems can not be observed so
determination of coordinate system is difficult. At this point, we will try to
determine it by using similarity between classical mechanics and field theory. In
the classical mechanics; equations of motion of coordinates are tried to
determine as functions of the time while equations of motion of fields are
tried to find as functions of the space-time in the field theory. This
situation gives an important idea about coordinate systems of the field theory;
fields of the field theory must be coordinates of the coordinate systems. Plus
for a moving point in this space these coordinates are some functions of the
space-time. Naturally; we assume that this system is Euclidean similar to the
classical systems and in general it can be
-dimensional. Figure
are coordinates and
are unit vectors of this
space
. We call this space as (4-dimensional) interaction space.
We can show any point in the
-dimensional interaction space with a position vector
,
where
. Unit vectors of the interaction space satisfy
(
If this point moves in the interaction space
can
be written (Figure
Similar to eq. (
,
where
is the complex
conjugate of
. For the geodesics of the interaction space we need to
calculate
.
In appendix I section, detailed calculation of geodesics and equations
of motion are given. By using results of these, we can use a Lagrangian to find
geodesics of the interaction space as
, (
where
.
Hereafter, superscripts denote complex conjugate of a quantity,
exception of the space-time.
For applications we choose 4-dimensional interaction space since results
of this is easier to understand and explain.
For the first application we assume that we have a fixed 4-dimensional
interaction space and its unit vectors are real. For this space position vector
of any point is
,
(4)
and
the complex conjugate of eq. (4) is
.
From
eq. (
(5)
eq.
(5) leads to the following equations of motion
(6)
and
the conserved quantity from these is
.
In
eq. (6)
.
We
see that eq. (6) represents some massless particles. We do not make any
interpretation for charge and spin for this particles unless we get to results
of next example of the interaction space.
Our next example is the same 4-dimensional interaction space again. But this
time, it is not a fixed space and it rotates with respect to a fixed space.
Because of this, the position vector of any point will be
.
This time unit vectors are some functions of the space-time
and this leads to an important result: Since
are unit vectors of the
interaction space,
is perpendicular to
and therefore must lie in the plane of the
other unit vectors. Because of this we can write for ![]()
, (7)
where
are some coefficients and they are important for the Langrangian.
We give detailed information about derivation of the Lagrangian for this 4-dimensional
interaction space in the Appendix II section. This Lagrangian is
, (8)
where
.
Lagrangian (8) gives following equations of motion
, (9)
, (
. (
We
show in Appendix III section that eq. (9) can be written as
, (
and
is a conserved
quantity
which can be written in a form (Appendix III section)
, (
where
.
Another
conserved quantity can be derived from equations (
(
Now; turn back
eq. (
in terms
and by writing
components of the electric and magnetic fields vectors E and B as follows
,
,
,
,
,
.
Here
and
are components of the
electric and magnetic fields vectors E
and B respectively.
There are many results of interaction space assumption. But; since they
are extremely speculative now, we try to give the most obvious results.
If eq. (
If eq. (
If eq. (
in (
We can give more consequences of our assumption. But, as we said, they
will be extremely speculative. The important thing is the fact that; the
interaction space assumption gives us a new way to handle field theory, fields,
particles and interactions. However; it needs to be understood first off all.
In this appendix, we will try to find geodesics equations of N-dimensional
interaction space and we will show these equations can be derived from a
Langrangian.
For N-dimensional interaction space, position
vector of any point is
,
where
. The metric this interaction space is
or
briefly
(AI.
can
be written by letting
.
From
definitions of
, we see that
Then
total derivative of
can be written as
(AI.
and
the metric is
. (AI.
By
comparing eqs. (AI.
. (AI.4)
Using
eq. (AI.4) we can write
.
By
letting
eq. (AI.
,
where space-time is
parameterized by
and if variational principles are applied to this metric
(AI.5)
can be written. There is
an important point: for this interaction space; only its coordinates vanishes
at the endpoints (i.e.
). Eq. (AI.5) leads to
the usual Euler-Langrange equations;
(AI.6)
or
,
where
and
. We know; the action (AI.5) must be invariant under any
arbitrary reparameterization. As a result of this fact we can choose a
reparameterization so that
, (AI.7)
where
is a constant. Eq. (AI.7)
leads to the Langrangian
.
Now we will show
another thing. Since ![]()
(AI.8)
can be written. But normally Lagrangian
is
. So
. (AI.9)
However; since
we can write from eq. (AI.8)
. (AI.
By comparing eqs. (AI.9) and (AI.
. (AI.
Now
by writing
eq.
(AI.6) becomes
. (AI.
Since
,
eq. (AI.
,
or from eq. (AI.
.
Thus; we can
use the last equation to find geodesic motion of the interaction space
In this appendix, we derive Lagrangian for the 4-dimensional interaction
space which rotates with respect to a fixed space.
For this 4-dimensional interaction space
,
.
From
eq. (7)
and
.
Let
(AII.
.
Using
eq. (
,
,
let
.
Derivative of the
position vector leads us to define a new vector
. Here
has similar role to
the angular velocity vector ω
in Classical Mechanics. Similar to Classical Mechanics,
derivatives of the position vector can be written as
In the last expression,
and
denote derivatives of R with respect to fixed and relative
interaction spaces, respectively.
In light of above knowledge we can rewrite
.
(AII.
The
second term in the right hand of eq. (AII.
By
performing summation over Levi Civita’s
And
since from eq. (AII.
,
we
can write
(AII.
We
can simplify eq. (AII.
’s in terms of unit vectors. For this we write
(AII.4)
or
. (AII.5)
From
the last equation, using eq. (
.
By
taking differential of the first equation of eq. (
(AII.6)
can be found. By replacing eq. (AII.4)
into eq. (AII.6) we have
. (AII.7)
By eq. (AII.7), we have found that
is anti-symmetric with
respect to the last two indices. We can show it is anti-symmetric with respect
to the first two indices also. For this, we will multiply eq. (AII.4) by
, but we
will denote this product process by
, since we will find that there must be an anti-commutative product between
and
. If we multiply eq. (AII.4) by
, we find
. (AII.8)
We
can rewrite eq. (AII.8), by interchanging m
and n
indices on the right-hand side of it. Now, we have
. (AII.9)
Eqs.
(AII.8) and (AII.9) are the same, so we write
.
There
are two possibilities for
product.
It is either commutative or anti-commutative. If it is commutative,
is symmetric with respect to first two indices. But this
option is impossible; because we have found that
was anti-symmetric with respect to last two indices.
can not be symmetric
with respect to first two indices and anti-symmetric with respect to last two
indices at the same time. Then
product is
anti-commutative, consequently
is anti-symmetric with respect to first two indices. That is;
is totally
anti-symmetric. So
,
,
. (AII.
Using eq. (AII.
![]()
can be written. Let
.
Thus
. (AII.
We can derive some
important relations for
. If we multiply eq. (AII.
, from eq. (AII.5) we find
. (AII.
By multiplying eq. (AII.
we have
.
And
using eq. (AII.
.
So
using these equations we can find
and
the Lagrangian
In this appendix, we will show that
is a conserved
quantity. We have found that
,
. (AIII.
.
From eq. (AIII.
![]()
.
As
a result of summations over anti-symmetrical terms we have
.
We
rewrite it as
.
By
interchanging λ and θ of the first term in the square parentheses we
find
or
or
.
And
Using eq. (AIII.
. (AIII.
From
eq. (AIII.
is conserved as a
result of mathematical requirement. However; there is another probability for eq.
(AIII.
is conserved again.
Therefore; if R is constant
becomes
.

Figure
r= x e

Figure

Figure
R is the
position vector of any arbitrary point in this space
![]()

Figure
Red
axes belong to the fixed 4-dimensional Euclidean Space