Proposal
The evolution of the solar interior is analyzed from a classical, independent, particle interaction model. In this model, it is presumed that the plasma has attained an organized state of development, thus reaching a condition of static equilibrium. Henceforth, the ionized particles remain at essentially fixed distances of interaction.
Most current standard solar parameters, as well as standard data pertinent to the associated atomic particles, have been utilized. All associated energy quantities are computed within the frame-work of the model, employing conventional techniques. The possibly of "strong force" interactions between charged particles separated at nuclear distances, is also considered.
It is shown that the total repulsive energy exceeds all other stabilizing factors. including the gravitational potential energy. A proposal regarding the deficiency in detecting solar neutrinos is also presented.
Print Reference
Pages 111-122
Disclaimer
DigitalCommons@Cedarville provides a publication platform for fully open access journals, which means that all articles are available on the Internet to all users immediately upon publication. However, the opinions and sentiments expressed by the authors of articles published in our journals do not necessarily indicate the endorsement or reflect the views of DigitalCommons@Cedarville, the Centennial Library, or Cedarville University and its employees. The authors are solely responsible for the content of their work. Please address questions to dc@cedarville.edu.
Recommended Citation
Boudreaux, Edward A.
(1994)
"Particle Interaction Analysis of Solar Formation and Stabilization,"
Proceedings of the International Conference on Creationism: Vol. 3, Article 20.
Available at:
https://digitalcommons.cedarville.edu/icc_proceedings/vol3/iss1/20