Background Radiation of Hydrogen Atoms
According to the
Dynamic Model
of elementary particles, the hydrogen atom, as a paired proton-electron system,
represents by itself the stable wave system of the longitudinal-transversal
structure. The wave exchange (interaction) takes place continuously
between the longitudinal (spherical) wave field of the proton and
transversal (cylindrical) wave field of the orbiting electron (as
is described in the paper
On the Spectral Terms
of H-atom). This exchange has the dynamically equilibrium
character and runs at the frequency
.
The stable states of the H-atom form, in such an exafrequency wave field, the
spectrum of dynamically stationary states defined by
characteristic values of arguments of Bessel functions:
,
where
,
and generate the
Background Spectrum
of Zero Level Radiation

(both spectra are described in details in the book
Atomic Structure of Matter-Space,
2001), where
,
, . are Bessel functions;
zr,s, zp,m, . are zeros of Bessel functions;
the subscripts p, q, r indicate the order of Bessel
functions and m, n, s - the number of the root. The last
defines the number of the radial shell. Zeros of Bessel functions define the
radial shells with zero values of radial displacements (oscillations), i.e.,
shells of stationary states. The quantity
is the constant equal to
the oscillation amplitude at the sphere of the wave radius
(mp is
the proton mass; r0 is the Bohr radius; h is the Planck
constant, R is the Rydberg constant).
An estimation of perturbation of the most probable stationary
state (n = 1) leads to the following result. The zero of the second
kinetic shell is
; hence, at
and
, we arrive at
.
This wavelength is within the extremum of the spectral
density of black-body radiation of the absolute temperature
,
where
is
the
fundamental period-quantum.
The temperature obtained practically coincides with the temperature of "relict"
background measured by NASA's
Cosmic Background Explorer (COBE) Far Infrared Absolute Spectrophotometer (FIRAS)
to four significant digits (
).
The existence of the zero level radiation of H-atoms
questions the Big Bang hypothesis of the origin of the Universe (in support
of the conclusion made, e.g., by A.K.T. Assis and M.C.D. Neves in
their work of 1995) and
quantum mechanical
probabilistic atomic model,
which excludes an electron's orbital motion along a trajectory as a
matter of principle.
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