I'd be obliged if you could provide a link that described this in detail .
I was under the apparently wrong impression that f/stop literally meant focal length/f number = diameter.
Sorry, there is no link.
I'm referring to ancient literature (coming from anno 1900) from where I studied some articles years ago.
These articles describe the precise determination of focal length and luminous intensity/amount of light passing a wide open lens system.
David, this articles very physically describe the science for every lens, not only a single lens system which always makes things more easy than systems with 4, 6 or 8 single lenses or different lensgroups.
For a deeper look please make a research for "Compendium der practischen Photographie" from Professor F. Schmidt, Docent der Photographie an der Technischen Hochschule Karlsruhe Baden / Wiesbaden Verlag from Otto Nemmich 1899
Yes, we are talking about diameters and focal length.
Focal length is clear, but "diameter" can say different things.
The most important thing is the wide opening /without any aperture) of a lens from where engineers start to determine the luminous intensity.
This is the effective wide opening.
You can bring an aperture with the same diameter to the lens but then the effective W.O. changes to a relative wide opening, concerning the behaviour of light rays passing a convex front lens in a convex way.
The entrance pupil is the visable diameter from wide opening and a base for measurements, and the aperture is just a tool with it's diameter depending on the entrance pupil.
To my understanding the entrance pupil gives the description of the wide opening diameter.
The visable entrance pupil either lays directly behind the aperture or somewhere within the lens system, depending on the lens design.
By the way there also exists an outgoing or exit pupil which can live her live widely outside of the lens what often is the case to real Tele constructions described by Ian..
Now, to calculate the correct diameter of the physical aperture you need the pupil magnification of the system.
To calculate the pupil magnification, you need the correct focal length (which often isn't the seen number on a lens) and the position of the main planes of the part of the lens in front of the aperture.
Such data are rather difficult to obtain but you can also try to measure or estimate with calipers and things as described before.
Mr. Belitski ( Deutsche Photogr. Zeitung Nr. 7 und 8, from 1889 ) described an experiment for determining the effective wide opening by making visable the focal point of a lens .
This visable focal point will give a perfect measurement of the entrance pupil.
I am aware about the logical f/stop system, and to all of us should be clear that an f/8 will give the same amount of passing light to every lens .
But as said before I can't imagine "f/8 on a 150mm lens will be half the size as f/8 on a 300mm lens" ,
because an f/stop term tells about the amount of light instead of the size of aperture diameters so I believe.
So next I want to determine some values from my big 300mm Tessar and my smaller 305mm G-Claron and probably from my 360mm Heliar (huge) and a 360mm Tele Xenar (small in direct comparism to the Heliar).
I would be surprised seeing results which could lead to "f/8 on a 150mm lens will be half the size as f/8 on a 300mm lens".
Best,
Reginald