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On Thu, 21 Nov 2024 4:12:04 +0000, ProkaryoticCaspaseHomolog wrote:
That can't happen, because, among other things, ultra-highThe important thing is that despite silly computational errors>
on _both_ our parts, we can agree that your statement of
Wed, 20 Nov 2024 08:46 is false, where you wrote:
>
| "The stored energy increases constantly until the temperature of the
| cavity walls (not cancelled by any means) destroy the material that
| form the cavity (either coatings or places on the cavity surface,
| making holes)."
>
Since once it reaches steady state, the ball radiates as much power as
is being pumped in, there is no danger of the ball being destroyed, as
you claimed in earlier posts.
>
I have absolutely no idea what this scaling crap is to which you
refer. The Stefan-Boltzmann law is applicable to small surfaces
as well as large. It _DOES_ need to be modified for bodies that
are not black, by application of an empirical emmisivity term.
You are right on the surface issue. I used πr² instead of 4πr².
>
>
Regarding the subject of constantly increasing stored energy, I repeat
that the internal energy density increases until the cavity breaks down.
This is not the case of Planck's BB cavity, where the BBC was heatedRather than pursuing this topic, which I consider dead, there are
from outside and left to rest until it reached thermal equilibrium.
Then, through a small orifice, experimental physicists at the Berlin
University lab (Physikalisch-Technische Reichsanstalt) measured
externally the irradiated power using a very sensitive heat sensor.
>
Here are some names that worked at the PTR in the 1890s. Ruben, a friend
of Planck, perfected the measurements reaching infrared radiation down
to 40 micrometers. He provided the charts and data to Planck, who
adjusted the 1986 Wien theory.
>
Otto R. Lummer, E. Gehrcke, R. Wien, Pringsheim, Kurlbaum.
>
Planck used the findings of Lummer-Pringsheim (1900) and Rubens-Kurlbaum
(1899-1900), performed at the Berlin PTR (Physical-Technical
Reichsanstalt) laboratory, provided to him by Rubens in Sept. 1900.
Planck had only 3 months to present his theory to the German Physics
Society in Dec. 1900, where he introduced his famous quantum of action.
>
I repeat the link with the history between 1850 and 1900:
>
Thermal Radiation, Black Body Theory and the Birth of Quantum Physics
>
https://physictheories.blogspot.com/2019/
>
http://users.df.uba.ar/dmitnik/fisica4/articulos/cuantica/Lummer.pdf
>
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>
I expect that you may understand the differences between the PTR Black
Body Cavity (externally heated) and my idea of pumping direct energy
into an almost perfectly reflecting cavity.
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