It is like both like a Maxwellian distribution and Bremstrahlung, but neither of these give a 1/f^2 distribtion. If you overlay a 1/f^2 line over the red dots the fit is perfect, indeed it is so good that it almost looks as if that is how it was generated.

On 10/03/2018 15:46, JonesBeene wrote:

Looks quasi-Maxwellian to me.

Where is the inverse peak?

*From: *Nigel Dyer <>

I have been looking at the graph titled

"After the MASSIVE broad band 'turn on' pulse, the excess heat mode is

between 0 and 100KeV"


which shows the steady state gamma radiation from the Parkhomov-like

experiment, together with a plot of the gamma radiation that is seen

right at the start.

It appears that the initial gamma radiation obeys a perfect inverse

frequency squared law.  I feel that this must be telling us something

about the underlying physics, but it is not clear what.  I cannot find

any other examples of inverse frequency squared emission of radiation.

Any ideas?


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