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Stellar Energy Generation and Nucleosynthesis
Author: Philip Mathew
Added: 03/21/2003
Type: Tutorial
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Introduction: The evolution of stellar objects is inherently caused by the chemical composition of the star.  Internally, thermonuclear reactions leading to the formation of complex atoms lead to a change in chemical composition which in turn will affect the evolutionary position of a star.

Energy Generation: Energy generation is made possible by proton-proton reactions.  In a proton-proton chain, two protons colliding with a minimum energy of 8 X 106 K will lead to the formation of a heavy hydrogen nucleus that will consist of a proton and neutron.  Furthermore, a positron (the electron's anti-particle) and a neutrino will break away.  The positron will collide with an electron and the two particles will annihilate one another (as particle physics dictates) to form two gamma rays.  A hydrogen atom will then crash into another proton to form helium and a gamma ray.

Another form of energy generation in stars is from the carbon-nitrogen-oxygen cycle (mercifully shortened to CNO cycle).  The CNO cycle is vital and predominate in more massive starts of one solar mass or greater.  The minimum energy for a greater CNO output compared to proton-proton output is roughly 20 X 106 K.  The CNO cycle is initiated by the conversion of a radioactive nitrogen isotope which is formed by the collision of a proton and carbon nucleus.  The nitrogen becomes a carbon isotope by emitting a positron and a neutron.  Proton bombardment will lead to the gamma ray emission and the conversion into a stable nucleus of nitrogen.  Further proton bombardment will convert the nitrogen nucleus into radioactive oxygen, which will decay into a nitrogen nucleus, a positron and a neutron.  The nitrogen isotope will then split into a C-12 and a He-4 after a collision with a proton.  The carbon in a CNO cycle serves as the catalyst since it remains unchanged in the CNO cycle.



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