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Article #4645Re: The solar neutrino problem - more confusing than *ever* before!
From: Joe Wang
Date: Tue, 10 Nov 1992 22:00
Date: Tue, 10 Nov 1992 22:00
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3509 bytes
In article <1992Nov5.050258.4240@isus.UUCP> hoyt@isus.UUCP (Hoyt A. Stearns jr.) writes: >The energy generation inside the sun comes not from fusion, >but the thermal destruction of heavy elements. Each element has a >temperature above which it converts to pure energy. If this is true, then 1) Why are there any neutrinos at all? If the source of energy is due to thermal destruction of heavy elements into pure energy, then where are the neutrinos that we do see coming from? 2) What about white dwarf stars? These are presumably the burned out cores of stars, and they seem to be pure helium with no heavy metal content. 3) Why hasn't this energy conversion been detected in earth-bound experiments? 4) Where do the heavy elements come from in the first place? In the standard model, the universe starts out as essentially all hydrogen and helium? 5) If the energy from stars comes from heavy elements, then presumably stars with lower abundances of metals ought to be much dimmer than similar stars (same mass) with heavy elements. They don't seem to be. 6) Have you calculated the impact of your model on stellar evolution? Standard stellar theory says that stars become red giants when the core runs out of hydrogen? Does your model explain why red giants exist? 7) Can you give me the Temperature vs. Luminosity relationship that your model predicts for stars? The standard model gives a relationship which fits the observations closely. Do you have predictions about the lifetime of stars and energy generation rates? These ought to be easy to calculate. 8) If a atomic nuclei turns into energy, you don't conserve charge. Very soon, a star will be extremely charge imbalanced and this ought to have observable consequences in spectra. Why doesn't this happen? It took me about 15 minutes to come up with these questions. It seems that you need to answer the above questions before you can use it to answer the solar neutrino mystery. Otherwise, you seem to be "solving" one mystery at the cost of opening up dozens of other ones. >These discontinuities cause oscillation of output (variables), and >eventually, supernovae. Explain. Standard variable theory states that variables are due to an instablity of the envelope in the star. From standard variable theory, you can get predictions about the temperature vs. luminosity function of stars as well as predictions about their periods. Does your model do this? Also, it seems that your model makes predictions about the elemental abundances observed in supernova. Can you share them with us? Also, can your model explain the abundance of Ni-57 in supernova explosions? Conventional supernova theory says that there is a lot of it because that part of the periodic table is where the most stable elements are found. Since your model of nuclear interactions is different, can you explain this abundance?
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arc1-ca.pugleaf.net!sparky!uunet!charon.amdahl.com!pacbell.com!decwrl!sun-barr!cs.utexas.edu!ut-emx!astro.as.utexas.edu!joeReferences:
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Path: arc1-ca.pugleaf.net!sparky!uunet!charon.amdahl.com!pacbell.com!decwrl!sun-barr!cs.utexas.edu!ut-emx!astro.as.utexas.edu!joe From: joe@astro.as.utexas.edu (Joe Wang) Newsgroups: sci.physics Subject: Re: The solar neutrino problem - more confusing than *ever* before! Keywords: Neutrinos, New Physics, Fusion Message-ID: <83353@ut-emx.uucp> Date: 10 Nov 92 22:00:04 GMT References: <1992Jun3.095319.13581@mpifr-bonn.mpg.de> <1992Nov5.050258.4240@isus.UUCP> Sender: news@ut-emx.uucp Organization: McDonald Observatory, University of Texas @ Austin Lines: 58