Another example of our resident polymath shortcomings is his inability to count.
He used the example of deuterium in this link to "prove" the three body problem involving electromagnetic forces is stable because deuterium is composed of an electron, proton and neutron, 1+1+1=3.
Ignoring the circular argument and synchrotron radiation kills off orbits what he didn't take into account is that the proton and neutron are bound by the strong force and therefore with respect to the electromagnetic force this a two body problem.
On a different subject the link illustrates the average binding energy per nucleon for atomic nuclei which is shown in greater detail below.
This curve shows the remarkable connection between experimental nuclear physics and the mechanism behind typeII supernova explosions.
In the curve the average binding energy per nucleon drops for atomic numbers greater than iron (Fe).
This means there is no excess energy produced when iron nuclei are fused.
It's no coincidence that stars that are massive enough to have iron in their cores explode as their is no longer any excess energy to oppose the gravitational collapse of the core.
He used the example of deuterium in this link to "prove" the three body problem involving electromagnetic forces is stable because deuterium is composed of an electron, proton and neutron, 1+1+1=3.
Ignoring the circular argument and synchrotron radiation kills off orbits what he didn't take into account is that the proton and neutron are bound by the strong force and therefore with respect to the electromagnetic force this a two body problem.
On a different subject the link illustrates the average binding energy per nucleon for atomic nuclei which is shown in greater detail below.
This curve shows the remarkable connection between experimental nuclear physics and the mechanism behind typeII supernova explosions.
In the curve the average binding energy per nucleon drops for atomic numbers greater than iron (Fe).
This means there is no excess energy produced when iron nuclei are fused.
It's no coincidence that stars that are massive enough to have iron in their cores explode as their is no longer any excess energy to oppose the gravitational collapse of the core.
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