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<article xmlns:xlink="http://www.w3.org/1999/xlink">
  <front>
    <journal-meta />
    <article-meta>
      <title-group>
        <article-title>Cosmological Aspects of the Particle Physics*</article-title>
      </title-group>
      <contrib-group>
        <aff id="aff0">
          <label>0</label>
          <institution>V.I. Vernadsky Crimean Federal University</institution>
          ,
          <addr-line>Simferopol</addr-line>
          ,
          <country country="RU">Russia</country>
        </aff>
      </contrib-group>
      <pub-date>
        <year>1940</year>
      </pub-date>
      <volume>249</volume>
      <issue>1</issue>
      <fpage>0000</fpage>
      <lpage>0001</lpage>
      <abstract>
        <p>In this paper, the multi-component Higgs field is expressed in terms of one component of this field, which plays the role of an order parameter, following the ideas of H. Haken's synergetics. A mathematical model combining the theory of elementary particles and gravity is proposed. The energy-momentum tensor of the Hilbert - Einstein equation is expressed in terms of an order parameter. The Higgs field, in which the phase transition occurs, eventually plays the role of an inflaton, similar to inflation theories.</p>
      </abstract>
      <kwd-group>
        <kwd>inflaton</kwd>
        <kwd>the Higgs field</kwd>
        <kwd>phase transition</kwd>
        <kwd>inflation</kwd>
        <kwd>energy-momentum tensor</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec id="sec-1">
      <title>Introduction</title>
      <p>
        Research in particle physics and cosmology provides the most in-depth knowledge of
our Universe. It is not surprising that one of the global problems facing modern physics
is the problem of combining cosmology with elementary particle physics [
        <xref ref-type="bibr" rid="ref1 ref2">1, 2</xref>
        ].
      </p>
      <p>
        In the '90s of the 20th century, an accelerated expansion of the Universe was
discovered. As it was found [
        <xref ref-type="bibr" rid="ref3">3</xref>
        ], the universe consists of about 70% of dark energy, 26% of
dark matter, and only 4% of ordinary (baryonic) matter. Currently, we do not have full
knowledge of the nature of dark matter and dark energy. So far, it is only known that
baryon matter itself does not have enough gravity to explain the structure of our
Universe. The rapid rotation of our galaxy would cause its stars to be scattered everywhere.
Everything we can see around us has only 10% of the gravity needed to keep stars in
their orbits. The existence of the galaxies and superclusters we observe can be explained
by the additional gravity of dark matter — a matter that does not emit or reflect light.
However, its concentration bends the light passing nearby. Einstein predicted the
expansion of the Universe at a rate called the Hubble constant, but modern measurements
show a higher rate than Einstein predicted. This continuous acceleration of the Universe
is due to dark energy — a repulsive force that acts oppositely to dark matter, causing
the Universe to expand rather than merge into organized structures. Our universe is
*
      </p>
      <p>Copyright 2021 for this paper by its authors. Use permitted under Creative Commons License
Attribution 4.0 International (CC BY 4.0).
almost completely flat, which can only be possible due to the influx of new energy
throughout space.</p>
      <p>
        The discovery of the accelerated expansion of the Universe contributed to the
recognition of the Guth-Linde-Vilenkin theory of Eternal Inflation [
        <xref ref-type="bibr" rid="ref4 ref5 ref6 ref7">4-7</xref>
        ]. In this theory, the
accelerated expansion of the Universe is caused by a scalar field-an inflaton, when this
field is at the «top" of its potential energy – in a pseudo-vacuum state. The transition of
an inflaton from a pseudo-vacuum state to a true vacuum state is interpreted as a Big
Bang. In the vicinity of a true vacuum, the inflaton behaves like a wave, and its
canonical quantization leads to the appearance of quasiparticles.
      </p>
      <p>
        The interpretation of dark energy and dark matter as different States of the inflaton
allows us to build simple and beautiful mathematical models of the dynamics of the
Universe, taking into account only the curvature of space-time and the inflaton. Such
models can be given the standard form of a Unified field theory. The inflaton
energymomentum tensor is included in the right side of the Hilbert-Einstein equation for the
curvature of space-time and, accordingly, in cosmological equations whose solutions
describe the accelerated expansion of the Universe [
        <xref ref-type="bibr" rid="ref4">4</xref>
        ].
      </p>
      <p>In July 2012, scientists working at the Large Hadron Collider announced the
discovery of a new fundamental particle, the Higgs boson. P. Higgs ' prediction of the
existence of this fundamental particle — a necessary part of the family of fundamental
particles in the Standard model of particle physics — was confirmed.</p>
      <p>
        In the 1960s, Peter Higgs developed a theory explaining how particles carrying
electromagnetic or weak interactions could get different masses during the gradual cooling
of the Universe. He assumed that particles like protons, neutrons, and quarks gain mass
by interacting with an invisible electromagnetic field known as the Higgs field [
        <xref ref-type="bibr" rid="ref10">10</xref>
        ].
The discovery of the Higgs boson marked the beginning of new research and a different
understanding of reality.
2
      </p>
    </sec>
    <sec id="sec-2">
      <title>The cosmological model</title>
      <p>
        One of the most fruitful ideas of modern particle physics is the idea of P. Higgs that the
Higgs boson is a multi-component scalar field, interacting with massless (true)
neutrinos gives them masses and charges, thereby turning them into quarks and leptons, and
interacting with a multi-component gauge field breaks it into components that are
carriers of electro-weak and strong interaction [
        <xref ref-type="bibr" rid="ref10 ref11 ref12 ref9">9-12</xref>
        ]. Therefore, the Higgs boson can be
part of any modern mathematical model that combines cosmology with particle
physics, and its energy-momentum tensor must be included in the right side of the Hilbert –
Einstein equation.
      </p>
      <p>The simplest cosmological model that combines cosmology with particle physics
will be the one where the Higgs boson plays the role of an inflaton, that is, dark energy.</p>
      <p>An easy-to-calculate and elegant mathematical model of an inflaton are obtained
from a single-component scalar field, whereas a multi-component Higgs field is needed
to transform neutrinos into different types of quarks and leptons.</p>
      <p>
        This work considers the possibility of reducing the multi-component Higgs field to
an effective one-component inflaton and is based on the ideas of Haken's synergetics
[
        <xref ref-type="bibr" rid="ref13 ref14">13, 14</xref>
        ]. In this case, one of the components of the Higgs field becomes an order
parameter, and the other components are expressed through it. This leads to the fact that
the energy-momentum tensor of the Hilbert – Einstein equation is expressed in terms
of an order parameter, that is, it becomes a one-component inflaton. The components
of the Higgs field interacting with a true neutrino are also expressed in terms of an order
parameter, i.e. an inflaton.
      </p>
      <p>
        Therefore, when a non - equilibrium phase transition from pseudo-to true vacuum
occurs with an inflaton, neutrinos have masses and charges, and they turn into various
quarks, leptons, and dark matter particles. Then the particles and antiparticles
annihilate, heating the rest of the matter-there is a Big Explosion, which, thus, is part of the
process of self-organization of the inflaton-neutrino system. The presence of this
process of self-organization turns the cosmological (mathematical) time of the Universe
into physical (entropic) time since the process of self-organization leads to a decrease
in entropy, and after the Big Bang, it increases [
        <xref ref-type="bibr" rid="ref15 ref16 ref17 ref18 ref19 ref20 ref21 ref22 ref23 ref24 ref25">15-26</xref>
        ].
      </p>
      <p>Let's start our analysis of the possibility of reducing the dynamics of a
multi-component Higgs field to the dynamics of a single component inflaton. We also study the
dynamics of the Higgs scalar field in a certain multiverse. The dynamics of this system
is described by the Cartan system of differential equations for the symplectic metric Ω
[27]:
U
n
x
3
  (da  bdt)(db </p>
      <p>
        U (0 ,n )adt)  d 0(d0 
dt) 
nd n(dn 
dt)  nd nd n (i    kn )n
U
0
and has the form [
        <xref ref-type="bibr" rid="ref8">8</xref>
        ]:
x
3
dt  (i    k n )n d n ,
(1)
(2)
or:
 x  
a  3 U ( 0 , n ),

 U
0   ,n  
  0
(i    k n )n  0

Here:
a is the radius of curvature of the universe,
b is its conjugate momentum,
 0 , n are the components of the Higgs field,
n are the fields of the (true) massless neutrino interacting with the n-th component
of the Higgs field  n .
      </p>
      <p>System (3) is an approximate model system.</p>
      <p>
        In the equation of the radius of curvature a, from work [
        <xref ref-type="bibr" rid="ref16">16</xref>
        ], the potential energy of
the Higgs fields is taken at the point of its minimum and a small term proportional to
the square of the field change rate is dropped.
      </p>
      <p>The scalar field equation in a homogeneous and isotropic universe has the form:
Since the solution of a, from the first equation (3), has the form
which means:

a
a
  3</p>
      <p>
  U ( )  0
 
a  exp  x U~(~0 ,~n )t a0 ,</p>
      <p> 3 

a
a
 H 
x U~(~0 ,~n )  1
3
</p>
      <p>U ( )  1 and  ~ 1 if  j  ~j ,   H ,
therefore, we can roughly replace equation (4) with the equation:
i  
a ~</p>
      <p>U ( k )  
3a i</p>
      <p>1 ~
3H Ui ( k )  Ui ( k )
(3)
(4)
(5)
where
Equations of this type are included in the system (3). In the lower of the equations (3),
we neglected the interaction of the neutrino with the gravitational field (the curvature
of the space-time of the universe).</p>
      <p>In our mathematical model, we select the potential energy of the Higgs field U as:
U  0
 2
0   ( n
2 n
0  U  0  0 0  n n 0

n  U  n  n n   02
2
We will look for the solution of the second equation of the system (7) in the form [29]:
Then we get the equation for Cn (t) :
 т  Cn (t)ent .</p>
      <p>C n (t)  ent  0 2 .</p>
      <p>2
Cn (t)    e n  0 2 ( ) d
t</p>
      <p>2
(6)
(7)
This gives an expression for </p>
      <p>n in the form:
 n (t )   t e n ( t )  0 2 ( )</p>
      <p>
en ( t )  n 2 ( )
2</p>
      <p>2
 t
 
 
 </p>
      <p> n
 0 2 (t )
2 n

 0 t en ( t ) 0 2 ( )d .
 n </p>
      <p>t  en ( t )  
d    n 
 0 2 ( )
2</p>
      <p>d 
t en ( t )
 </p>
      <p> n

 0 ( ) 0 ( ) 
Assuming  0  1 , we get
 n
 n  
exists only when  0  0</p>
      <p>
        Substituting the expression (10) in (8), we get:
(8)
(9)
(10)
(the principle of subordination of G. Haken, [
        <xref ref-type="bibr" rid="ref12">12, 27</xref>
        ]).
      </p>
      <p>Substituting this relation into equation (7), we get:
its stationary solution:
2 n

In this case, the momentum energy tensor of the Higgs boson, which is included in the
Hilbert – Einstein equation, takes the form:</p>
      <p>T  g U ( 0 , n )  g (0
 g ( 0
Thus, the principle of subordination of Haken leads to the transformation of the n + 1
component Higgs field in the energy-momentum tensor into effective one-component
field  0  inflaton.</p>
      <p>During the period of inflationary expansion of the universe (before the Big Bang) when
 0  0, T  g V0 , and after the phase transition of the field  0 to the true vacuum:
~0  
 20 ,</p>
      <p>1

n n
the energy-momentum tensor takes the form:


  2
T  g   0
  1
 n  n</p>
      <p>1 1
 
8 n  n  1 
  
 k  k </p>
      <p> 
2  V0   g V0 
This shows that after such a phase transition (the Big Bang), the accelerated expansion
of the Universe slows down.</p>
      <p>
        According to the Higgs representations [
        <xref ref-type="bibr" rid="ref13 ref14">13-14</xref>
        ], the interaction of massless neutrinos
with Higgs bosons leads to the appearance of a mass in them. The equation of such a
neutrino has the form:
      </p>
      <p>~
In the period of inflationary expansion, 0  0 , and therefore</p>
      <p>
i    k n n  0.</p>
      <p>~n  
after the phase transition  0 to the true vacuum</p>
      <p>Thus, after the" Big Bang", equation (14) takes the form:
(14)
(15)
The mass appears in neutrinos, and they become quarks and leptons (taking into account
the nature of the interaction with the electromagnetic field). In different local universes,
 0 and  n are different [28-33], so the masses of elementary particles in them are also
different.
3</p>
    </sec>
    <sec id="sec-3">
      <title>Conclusion</title>
      <p>
        This paper implements a model for reducing the multi-component Higgs field to
effective one-component inflation. The model is based on the ideas of Haken's synergetics
[
        <xref ref-type="bibr" rid="ref15">15</xref>
        ].
      </p>
      <p>Thus, it is shown how cosmology and elementary particle physics can be combined
within the framework of the Guth – Linde – Vilenkin theory of eternal inflation
[3739]. This result allows us to impose certain conditions on the mass spectrum of
elementary particles in our Universe based on cosmological observations of the slowing down
of the Universe. It is also seen that non-equilibrium phase transitions occur in universes,
making the cosmological time of the universe physical [35].</p>
      <p>The problem of the cosmological constant, the accelerated cosmic expansion in
recent times, and the coinciding current energy densities of the cosmological constant and
matter, remains a complex puzzle for cosmology [40].</p>
    </sec>
  </body>
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