Can you point to resources to safely and legally begin dabbling? Are you familiar with the process to obtain proper licensing?
How are simple reactors like the Farnsworth Fuser regulated, or why are they exempt? Are non power generating reactors exempt from regulation? How does that get defined? Is it based on maximum emitted radiation?
While I work in the same lab as a bunch of nuclear physicists, my physics expertise is in experimental gravity.
To get the official scoop on such things, I'd start with the NRC: http://www.nrc.gov .
If you're at/near a university, many of them have a radiation safety office as a part of their Environmental Health and Safety department. University radiation safety officers are a great resource for timely details regarding rules in an experimental setting. Even if there's no "nuclear science" underway at a school, if there's a medical school or nuclear chemistry at work, there's probably a radiation safety office.
Before you jump ship to precision tests of gravity: graduate students' mean time to graduation in our group is >7-8 years. Our experiments take several years to set up, at least a year to execute, and at least a year to analyze.
When a new idea/theory comes up, we can often test it quickly (or rule it out with existing measurements), but our bread-and-butter work is a direct confrontation with hard experimental problems.
For scale, we can choose to be separately sensitive to both the gravitational signal and the tilt of the ground due to a pickup truck parked outside of our lab.
Perhaps the most important function of precision experimental tests (all of them, not just ours), is to provide very tight constraints for new theories. Any successful new theory of physics must ultimately explain more observed phenomena than existing theory. If experiment is more sensitive than existing theories, it can provide a quick checksum for whether a new theory is correct.
Furthermore, if a precision measurement is able to show that existing theory is not quite correct, it can lead the way to better theories.
In the field of precision gravity, Newton's and Einstein's theories have been perhaps frustratingly correct. At present, nobody knows if/how the "Standard Model" and gravity might connect. They're mathematically incompatible.
With respect to any existing literature, most physicists' position might be approximately summarized as, "Trust, but verify."
The most-important experiment we do is to test the Equivalence Principle [1], the idea that if you drop two things in vacuum, they'll fall at the same rate regardless of what they're made from. Results from our lab have shown that, at 1 part in 10,000,000,000,000 (10^-13), that's apparently true. General Relativity takes the Equivalence Principle as a postulate, and works from there. Many theories of new physics would break the EP at scales of ~10^-15 or so.
My almost-complete thesis research is searching for violations of the gravitational inverse square law at short distances. In short, over distances smaller than the diameter of a hair, nobody knows if gravity acts. It probably does, but you don't know until you check. String theory would suggest that, at short-enough distances, gravity should get unexpectedly stronger. Solutions to the Cosmological Constant problem [2] may suggest that gravity should turn off at distances shorter than the diameter of a hair. Dark Energy/Hubble Constant observations would suggest that gravity might do something interesting at around this same scale.
Our workhorse technology is the venerable torsion balance [4], souped-up with modern experimental readout and data analysis techniques. Our best angle sensors [5] sense a nanoradian's angular displacement in less than a second. For scale, if we shine a laser pointer from Seattle to San Francisco, a nanoradian is equivalent to about a millmeter's displacement of the beamspot on the TransAmerica building.
If you want me to build you an angle sensor or a precision force sensor, I'm interested in hybrid industrial and academic work [6].
Pardon my complete lack of knowledge in this field, but would MEMS (or NEMS) mirror arrays be sensitive / accurate enough to measure the gravitational effect on light at the scales you're talking about?
I'm surprised to read the statement "over distances smaller than the diameter of a hair, nobody knows if gravity acts" as I thought we were accurately measuring all sorts of interactions at or below that scale (10s of microns).
My apologies for the terse nature of my summary above. We measure the deflection of light bounced from a mirror attached to a test mass hanging from a very fine wire.
That said, the geometry of some of the Texas Instruments DLP MEMS chips has interested some of us for years. The chips are designed to be robust in consumer products, but if they instead designed their mirrors to have very soft springs, we'd be interested in playing with them. Once a year or so, I do a survey of the available MEMS accelerometer chips to see if it's worth building an array from them. They're still a few orders of magnitude away in sensitivity from anything we could put to use.
For the second half of your question: Physicists do indeed measure interactions at scales far smaller than the diameter of a proton. The "trouble" with gravity is that it's so very weak. On a handwavy charge-for-charge basis, gravity is 10^40 (that's 10,000,000,000,000,000,000,000,000,000,000,000,000,000) times weaker than electromagnetism. For an experiment that's purely sensitive to electromagnetism (atomic spectroscopy) or other comparably strong forces (particle colliders) to see gravity, it's necessary to resolve the other forces incredibly well in order to see a tiny residual effect from gravity.
For our work, achieving sensitivity to gravity at the scale of tens of microns isn't that hard. Proving to you that we're not seeing another force/experimental influence (the flip side of that 10^40) is very hard, and is what I spend almost all of my time trying to do.
Thanks for your interest; it's sharing the stoke about this stuff that keeps us going when it's hard (and, if you're a US citizen, you're paying for it! Thank you!).
Interesting. Dr Steinberg actually did his design thesis at UQ and there's a 1999 article saying it'd be built there, but by the looks of it he then jumped over to QUT and built it there instead. I certainly don't remember it existing at UQ when I was there in ~2005.
I would really enjoy a blog post/series about what you're doing. I'm sure you think it's ordinary and slightly boring but you'd surprised how many -- even technical -- people have no idea how you can measure gravity over the breadth of a hair, and would be fascinated by it.
How are simple reactors like the Farnsworth Fuser regulated, or why are they exempt? Are non power generating reactors exempt from regulation? How does that get defined? Is it based on maximum emitted radiation?