Authors: Jamal S. Shrair
An objective and empirical analysis of the data collected from different detectors over four decades reveals that the so-called solar neutrino problem is far from being solved. Contrary to the assessment of the Nobel Committee, the experimental results from the Sudbury Neutrino Observatory cannot be regarded as a confirmation of the Standard Solar Model. However, the obsolescence of the current model (SSM) has recently been exposed by so much observational data, for instance, the crisis in solar abundance. Furthermore, using images obtained by the Solar Dynamics Observatory, researchers found the convective motions (the motions within the Sun's interior) to be nearly 100 times smaller than current theoretical expectations. This is a clear verdict on the notion of thermonuclear reactions that are supposed to be the processes that generate solar neutrinos.
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