ugalpha
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without having to rely on quantum channeling
The discussion centers on the conditions necessary for nuclear fusion to occur in stars, particularly focusing on the mass and temperature thresholds required for fusion processes like the proton-proton chain. Participants explore the role of quantum tunneling in facilitating these reactions and the implications of various mass thresholds.
Participants express differing views on the necessity of quantum tunneling for fusion at lower masses, with some asserting it is essential while others suggest that sufficient kinetic energy could allow for fusion without tunneling. The discussion remains unresolved regarding the role of quantum tunneling in nuclear reactions at various mass thresholds.
There are limitations in the discussion regarding assumptions about the conditions under which fusion occurs, the definitions of critical mass, and the specifics of quantum tunneling's role in nuclear reactions.
The core has to get to about 15 million K, although some say about 10 million K.The basic process of star formation is that they emerge due to accretion of enough matter to reach a critical mass* of approximately 80 times Jupiter's, at which point internal pressures raise the core temperatures high enough to ignite nuclear fusion.
ugalpha said:without having to rely on quantum channeling
goldsax said:can fusion at 0.13 solar masses occur without quantum tunneling?
infact can nuclear reactions occur without tunneling or can sufficent kinetic energy convey enough energy to get nuclei into actual contact?
ugalpha said:without having to rely on quantum channeling
qraal said:Why even ask? Seems like a pointless question.