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  1. The CNO cycle (for carbon–nitrogen–oxygen; sometimes called Bethe–Weizsäcker cycle after Hans Albrecht Bethe and Carl Friedrich von Weizsäcker) is one of the two known sets of fusion reactions by which stars convert hydrogen to helium, the other being the proton–proton chain reaction (p–p cycle), which is more efficient at the Sun's core temperature.

  2. Abstract. Since the independent suggestions in 1938 of Bethe (1939) and von Weiszäcker (1938) that captures of protons by carbon and nitrogen isotopes were the source of energy generation in stars, the CNO cycles have developed into what might be considered by some a many-cycled monster rivalling the many-headed Hydra, However, those of us who ...

  3. Capitalism. Business cycles are intervals of general expansion followed by recession in economic performance. The changes in economic activity that characterize business cycles have important implications for the welfare of the general population, government institutions, and private sector firms. There are numerous specific definitions of what ...

  4. The CNO cycle (for carbon - nitrogen - oxygen ), or sometimes Bethe-Weizsäcker-cycle, is one of two fusion reactions by which stars convert hydrogen to helium, the other being the proton-proton chain . The proton-proton chain is more important in stars the mass of the sun or less. Only 1.7% of 4 He nuclei being produced in the Sun are born in ...

  5. Above this mass, in the upper main sequence, the nuclear fusion process mainly uses atoms of carbon, nitrogen, and oxygen as intermediaries in the CNO cycle that produces helium from hydrogen atoms. Main-sequence stars with more than two solar masses undergo convection in their core regions, which acts to stir up the newly created helium and maintain the proportion of fuel needed for fusion to ...

  6. CNO cycle යනු න්‍යෂ්ටි සංස්ලේෂණ ක්‍රියාවලියකි. ආශ්‍රිත [ සංස්කරණය ] න්‍යෂ්ටි සංස්ලේෂණය

  7. en.wikipedia.org › wiki › Solar_cycleSolar cycle - Wikipedia

    The Suess cycle, or de Vries cycle, is a cycle present in radiocarbon proxies of solar activity with a period of about 210 years. It was named after Hans Eduard Suess and Hessel de Vries . [47] Despite calculated radioisotope production rates being well correlated with the 400-year sunspot record, there is little evidence of the Suess cycle in the 400-year sunspot record by itself.