The Fishback ramjet revisited
sciencedirect.com
sciencedirect.com
If you were trying to make the CNO cycle
https://en.wikipedia.org/wiki/CNO_cycle
work with an interstellar ramjet you would have to stop interstellar H (drag!), retain it in a reactor for a timescale of tens of minutes because of the beta decay that is part of the cycle and continue to retain almost all of the heavy (compared to Helium) elements and vent only Helium and maybe some hydrogen (like the space shuttle main engine this is great for Isp.)
Unless you have a triple-alpha line
https://en.wikipedia.org/wiki/Triple-alpha_process
that can synthesize carbon from helium you would be stuck with whatever inventory of C,N,O you started with and you'd slowly lose it.
It seems much more transformative to interstellar travel that you can brake yourself with a magsail at the destination. The drag is very real but any thrust from the Bussard ramjet seems elusive.
The drag would be useful in the second half of the trip but can you make a ramjet that rotates the direction of travel of the reaction mass by 180°? You might be able to collect reaction mass for a return trip though, or final deceleration.
We know comets and other interstellar bodies contain a lot of hydrogen which has a higher deuterium content than hydrogen on Earth.
Designs such as ITER and stellerators should scale up with increasing size and it's plausible that D+D fusion could be developed on the existing path. In fact a very large "inertial confinement" fusion device was fired based on D+D
https://en.wikipedia.org/wiki/Ivy_Mike
and got a massive positive energy return.
D+D fusion produces He3 and T, both which are better-burning fuels than D+D. These can be burnt all the way up to He4 in one big reactor, but one can imagine a system that separates out some He3 and T to be burned in smaller secondary reactors. D + T fusion produces terrible neutron radiation but you can let the T sit and it decays with a 12-year half life to He3 and use the much cleaner D + He3 reaction in secondary reactors with favorable scaling, less shielding, no breeding system, etc.
Those travelers only need to get to the next comet so they don't need to be terribly fast, but the great advantage they have is a sustainable lifestyle even if they never arrive at another star -- those kinds of travelers might not find planetary systems interesting at all.
Well, this is a bummer. So, likely unfeasible for type I and II, certainly unfeasible for us... and type III, if they exist, would consider it a toy?
To me it always seemed like a classification system that doesn't fully understand the scale it is trying to use. Or one that assumes exponential unbounded growth as a starting point. The cube square law is one that catches a lot of Sci-Fi authors.
As for type III civilizations, my guess is they would think of it as a toy as the speculation about type III has them doing stuff like harvesting stars on mass for use in stellar engines and galactic scale engineering projects.
I know it's boilerplate, but I appreciate the authors' explicit declaration here that they're not in the pocket of Big Dyson Swarm.
[1] https://memory-alpha.fandom.com/wiki/Bussard_collector
[2] https://forgottentrek.com/designing-the-first-enterprise/
So what are they? (ideally to the nearest 5% of C)
> With graphene, the most suitable material, the cut-off speed for 1 g acceleration would be approached after an on-board flight time of three years at a distance of about 10 light-years. After that, the acceleration would quickly drop to values that shatter the popular dream of reaching the galactic center in a lifetime.
Note that this is already assuming you can build superconducting rings in space with a diameter of 2000 kilometer and with enough graphene to support them. If we assume for convenience that the acceleration will fall to zero after those three years, the relativistic speed calculator at https://www.omnicalculator.com/physics/space-travel (haven't checked it in depth, but I have no reason to doubt it) tells us we will have reached a speed of about 91% of c.