96 research outputs found
On the stability of classical orbits of the hydrogen ground state in Stochastic Electrodynamics
de la Pe\~na 1980 and Puthoff 1987 show that circular orbits in the hydrogen
problem of Stochastic Electrodynamics are stable. Though the Cole-Zou 2003
simulations support the stability, our recent numerics always lead to
self-ionisation. Here the de la Pe\~na-Puthoff argument is extended to elliptic
orbits. For very eccentric orbits with energy close to zero and angular
momentum below some not-small value, there is on the average a net gain in
energy for each revolution, which explains the self-ionisation. Next, an
potential is added, which could stem from a dipolar deformation of the
nuclear charge by the electron at its moving position. This shape retains the
analytical solvability. When it is enough repulsive, the ground state of this
modified hydrogen problem is predicted to be stable. The same conclusions hold
for positronium.Comment: 18 pages latex, 1 figur
Exact solution for the interior of a black hole
Within the Relativistic Theory of Gravitation it is shown that the equation
of state holds near the center of a black hole. For the stiff equation
of state the interior metric is solved exactly. It is matched
with the Schwarzschild metric, which is deformed in a narrow range beyond the
horizon. The solution is regular everywhere, with a specific shape at the
origin. The gravitational redshift at the horizon remains finite but is large,
. Time keeps its standard role also in the interior.
The energy of the Schwarzschild metric, shown to be minus infinity in the
General Theory of Relativity, is regularized in this setup, resulting in
.Comment: 12 pages newFNLstyle. 4 figure
Explanation of the Helium-3 problem
One of the tests of nucleosynthesis theory is the He abundance in the
Galaxy. He is observed through its 3.46 cm hyperfine level in Hii
regions and the He/H ratio compares well with theory. Since He can be
created or destroyed in nuclear reactions, one would expect that its abundance
shows a trend with the amount of such reactions, so with distance to the Center
of the Galaxy and with metallicity. Such trends are lacking in observations.
This is explained by assuming that the Hii clouds are recently formed out of
the primordial micro brown dwarfs of earth mass predicted by gravitational
hydrodynamics. If indeed existing, they would preserve their primordial
He/H ratio and spread this when evaporating into Hii clouds, independent of
the location in the Galaxy.
In the development of the argument, it is also explained that wide binaries
do not rule out the MACHO dark matter predicted by gravitational hydrodynamics,
but are rather immersed as visible partners in Jeans clusters of dark micro
brown dwarfs.Comment: 4 page
Prediction for the neutrino mass in the KATRIN experiment from lensing by the galaxy cluster A1689
The KATRIN experiment in Karlsruhe Germany will monitor the decay of tritium,
which produces an electron-antineutrino. While the present upper bound for its
mass is 2 eV/, KATRIN will search down to 0.2 eV. If the dark matter
of the galaxy cluster Abell 1689 is modeled as degenerate isothermal fermions,
the strong and weak lensing data may be explained by degenerate neutrinos with
mass of 1.5 eV. Strong lensing data beyond 275 kpc put tension on the
standard cold dark matter interpretation. In the most natural scenario, the
electron antineutrino will have a mass of 1.5 eV/, a value that will be
tested in KATRIN.Comment: 13 pages, 5 figure
Observational Derivation of Einstein's``Law of the Constancy of the Velocity of Light in Vacuo"
On the basis of Galilean invariance and the Doppler formula, combined with an
observational condition, it is shown that the constancy of the velocity of
light {\it in vacuo} can be derived, together with time-dilatation and Lorentz
contraction. It is not necessary to take the constancy as a postulate.Comment: 5 pages AIP-tex. Conference "Quantum Theory: Reconsideration of
Foundations 3", Vaxjo Sweden, June 2005. To appear in AIP conference serie
Are observations of the galaxy cluster Abell 1689 consistent with a neutrino dark matter scenario?
Recent weak and strong lensing data of the galaxy cluster A1689 are modelled
by dark fermions that are quantum degenerate within some core. The gas density,
deduced from X-ray observations up to 1 Mpc and obeying a cored power law, is
taken as input, while the galaxy mass density is modelled. An additional dark
matter tail may arise from cold or warm dark matter, axions or non-degenerate
neutrinos. The fit yields that the fermions are degenerate within a 430 kpc
radius. The fermion mass is a few eV and the best case involves 3 active plus 3
sterile neutrinos of equal mass, for which we deduce eV. The eV
mass range will be tested in the KATRIN experiment.Comment: 5 pages latex, 5 figures. Accepted for MNRAS Letter
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