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Fission-Fusion Star with Neutron-core and Super-nuclei



 
 
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Old November 19th 06, 11:47 PM posted to sci.physics,sci.astro
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Default Fission-Fusion Star with Neutron-core and Super-nuclei

Fission-Fusion Model of a Star with a rotating Neutron-sphere in the
core and Super-nuclei

By Louis Nielsen, Denmark

In the following I describe an alternative model of the sun and other
similar stars. As an example, let us consider the structure of the sun
and the processes taking place within it. Generally the sun has a
stratified structure and function. The central core consists of a
relatively small rotating neutron-sphere consisting of neutrons. The
rotating neutron-sphere is the source of the primary magnetic field of
the sun. Around the neutron-sphere is a zone of super-nuclei
(macro-nuclei), with different, very high nucleonic numbers. The
super-nuclei 'evaporate' from the surface of the neutron-sphere,
assisted at the escape by the magnetic field.
The super-nuclei can, under certain physical conditions, disintegrate
by different types of reactions. Super-nuclei can disintegrate by alfa,
beta decays and by successive fissions, spontaneous as well as induced.
Also disintegrations by emissions of nuclei of carbon, oxygen,
silicium, sulphur etc. can take place. The processes produce energy,
and simultaneously the heaviest elements are created, down to iron,
which is the most stable nucleus we know. Neutrons, alfa-particles and
lighter elements, created by fission and decay of the super-nuclei, are
'blown' outwards in the sun by the pressure of radiation and particles.
The neutrons are decaying to protons, electrons and anti-neutrinos, by
which hydrogen atoms can be built. Alfa-particles give the possibility
for production of helium atoms. In the zone of super-nuclei, the
abundance of iron is increasing as the disintegration of super-nuclei
takes place. Hydrogen, helium and some of the lighter and heavier
elements will be 'placed' in zones around the super-nucleus zone. In
the inner hydrogen/helium zone, where temperature and pressures are
high, fusion processes can take place, producing energy and lighter
elements. The outer layer of the sun consists, as spectral analysis
shows, of hydrogen, helium and lighter elements, mixed with a small
amount of heavier elements.
By the disintegration processes, energy is released, in the form of
kinetic and radiation energy. The pressure from particles and radiation
causes an 'inflation' of the system of matter. An active and stable
star is formed when stability is reached between the inwards gravity
and the outwards pressure.

The structure and the processes of a star can be resumed as follows:
The star-co A fast rotating neutron-sphere, which is the source of
super-nuclei and the source of the primary magnetic field around the
star.

The super-nuclei zone: A zone consisting of super-nuclei which are
disintegrating with release of energy and simultaneous production of
elements heavier than iron.

The Iron zone: A zone with relatively high abundance of iron, and with
balance between fission and fusion processes.

The Fusion-zone: A zone consisting primarily of hydrogen and helium,
with fusion processes, releasing energy and creating lighter elements.

Fusion free outer-zone: A zone consisting of hydrogen, helium and
lighter elements, mixed with some heavier elements.

The outer zone we know quite well from studies of spectres. On the
contrary, informations from the other zones are presently difficult to
analyze. Detailed studies of neutrino-flux, magnetic fields and
astro-seismology must confirm or reject the above model.

Best regards,
Louis Nielsen, Denmark

 




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