Tuesday, June 16, 2026

Random means "We have no idea."

What quantum mechanics leaves out of its "randomness is fundamental" picture is the state of the entire rest of the universe.  Equations for quantum states generally cover only one or a very low number of particles, interacting (or not) with a very limited environment.  The equations leave out the near-infinitude of states required by the generator to create the particles in question.  They completely ignore the near-infinitude of states required for the detector to function.  They ignore as irrelevant the near-infinitude of states of the surrounding apparatus.

Why?  Because the math is much, much too hard, and the measurements are essentially impossible to make to the precision required.  Therefore, "randomness is fundamental to the quantum mechanical process!"


Copenhagen Interpretation delenda est!

Sunday, June 14, 2026

Flag Day

You're a grand old flag
You're a high flying flag
And forever in peace may you wave

You're the emblem of
The land I love
The home of the free and the brave

Every heart beats true
'Neath the red, white and blue
Where there's never a boast or brag

Should auld acquaintance be forgot
Keep your eye on the grand old flag!

Saturday, June 13, 2026

Home security cameras

I'm going to say this up front - most home security camera systems are a waste of money.  Cameras don't truly deter crime any more - they provide a record of events after the fact.  And most cops don't care enough to actually use the video.  And lots of criminals wear masks these days, after the covidiocy made them acceptable in public.

That being said, if you really want a home video surveillance system, never, ever have indoor cameras.  Remember, in case of an actual event, the entire system will become evidence.  Do you really want video footage of everything you've been doing inside your own home made public record and examined in court?

Never get cameras that automatically record audio, either.  In many states, recording audio without the permission of all parties is a crime.

Never buy a camera system that sends ANYTHING out to the internet.  "The cloud" is just somebody else's computer.

All that being said, there are a few features you want to look for in a home security camera system.

One of the things you want to look for in a camera is an in-unit SD card.  They're not perfect, but local storage always works, even when the network goes down.  You'll want one that accepts UHS rated cards, if you can find one.

Another thing to look for, especially in places like Florida, is a wide dynamic range (WDR).  That means the camera can get decent pictures of a man standing in the shadows on a sunny day.  It also helps at night, when there are other light sources potentially blinding your camera to what's right in front of it.

Pan-Tilt-Zoom cameras are great as backups to the standard fixed view cameras.  Don't make them your primary cameras, because the PTZ features only work when you're actively using them.  Most people will use them once, then forget about them, and leave the camera zoomed in on where the squirrel (or woman in a bikini) was six months ago.

You want a wired system.  Trust me.  Yes, I understand you don't really want to cut more holes in the outside of your house.  No, you really don't want to run all those cables through your walls and across your attic.  But you do want your cameras to keep working for years, and that requires power.  The battery powered ones don't last any time at all, and you're not going to remember (or want) to get up on a ladder and change them out every month.  Did I say month?  I meant week.

Thursday, June 11, 2026

Larger than life

Some men's lives seem remarkably improbable.  These "larger than life" figures appear over and over throughout history.  These are the "great men" who change the world, for better or worse.  Leftist historians (the children of Marx) say that there are no great men, only the inevitable, scientific progression of history.

Pfaugh!

Please follow this link and read about Prentiss Ingraham, the man who fought in seven wars before the age of 30, then went on to befriend Wild Bill Cody and invent the Western novel genre.

Saturday, May 9, 2026

Post-Modern Education

The modern high school curriculum is misunderstood, even by the teachers. Geometry does not teach math. It teaches logical reasoning. By the same token, science classes don’t really teach science. They teach that the world is understandable, that effects follow from causes.

That being said…  I recommend a completely revamped form of primary education, focused on the 4 R's.  Reading, 'Riting, 'Rithmetic & Reloading.

I really do believe that primary school education should be limited to between the ages of 8 and 13. (Let the younger kids run around and play.  Family time is incredibly important.) You can teach the entire basic curriculum to children during those five years. It should include math (through basic algebra and statistics), English (reading, writing, literature), history & geography (taught together as stories of time and place), science (the basics plus logic), civics (including taxes, banking, and the political & legal processes), media literacy (how to tell when you’re being scammed), the arts (vocal & instrumental music, dance, drawing & painting), and life skills (home economics & child care, wood & metal shop, pottery, crocheting & sewing, laundry, cooking & baking). Daily gym classes for all (they need to move, and they’ll also learn the importance of teamwork and being a good sport.) Then you separate the kids into different groups by talent, interest, and sex for further education to age 16.

The top 20% of boys and 10% of girls (yes, I mean this seriously) go to college prep, formerly known as high school. A third to half should fail out of this process and move on to technical training.

The average middle get apprenticeships.

The bottom 20% get shovels, rakes, hoes, and brooms.

Group activities like sports, band, choir, dance, and theater continue to the age of 16 as well. You can’t do all of them, but you do have to participate in at least one of them. Each community shall create monthly activities to get the young men and women together in a chaperoned but fun environment. Bring back formal dancing (square, line, ballroom, folk, etc.) and roller skating! Add in junior versions of SCA/HEMA and ROTC, along with riflery & archery. Camping, fishing, hunting, gardening, farming, and animal husbandry should be offered as available and appropriate to the region, climate, and time of year. A reformed and restored version of Scouting would be appropriate and encouraged.

In my more perfect world, each school day would begin with recitations of the Pledge of Allegiance and the Lord’s Prayer.

Thursday, April 30, 2026

A simple randomizing mechanism

TTRPGs run the gamut from simulation (usually tactical) to “Once upon a time…” and everything in between. Most use dice, others cards, a few just pure imagination. Here is a simple mechanism for resolving chance in a more story-oriented game, using just one or more 6 sided dice. This will require much more active engagement by both the game master and the players. It also makes a simple but useful oracle for solo gaming.

  1. No, and

  2. No

  3. No, but

  4. Yes, but

  5. Yes

  6. Yes, and

Roll as many dice as appropriate, taking either the best or worst result as appropriate.

That’s it. It doesn’t have to be complicated.


Grammatical reminder: one die, many dice. It’s standard English, and has been for almost a thousand years. Don’t let fashionable ignorance ruin a perfectly good word.

Friday, April 24, 2026

How light bends, and other oddities

Einstein’s first prediction for general relativity was that light from distant stars passing closely by the sun during a total eclipse would bend twice as much as Newton’s laws of gravitation and motion called for. (No, this has nothing to do with the eclipse. That’s just the only time you can see things near the sun.) Many observations over the past century have proven him correct. By why does light do this?

Since the days of Newton, we have measured the attractive force of gravity quite precisely. The motion of the moon around the earth, the orbits of the planets about the sun, the falling of apples from trees, these are all data points rigorously collected, compiled, and compared. They all show the same force of gravity acting on massive objects. Well, they almost all do…

Mercury moves just a bit too quickly as it passes close by the sun. This advances its orbit just a tiny bit each revolution. There was no simple explanation for this. It was as if the carefully studied force of gravity changed when you got too close to the sun. Einstein invented general relativity in part to solve this conundrum.

Light from distant stars passing close by the sun during an eclipse was the earliest proof his theory was correct, or at least worked properly, which is generally the same thing. But why does light do this? The answer, as almost always, lies in the geometry. To the graph!

Here we have two test particles in the potential energy field, held motionless by the magic of wanting a simple example. The blue one on the left has a mass of 0.5 (the Planck mass = 1 in this model). The red one on the right has a mass of 0.25. They are close to each other, with one centered at -3, the other at +3. Each is, of course, of radius one, as are all particles regardless of mass. Once we release the less massive particle on the right, what happens to it?

The particle gains an internal energy gradient equal to the gradient of the ambient field inside its boundaries. This internal gradient grants it a velocity in the direction of the lower level of the field, towards the left. The internal gradient is now a permanent part of the particle’s energy profile, shown as dashed green. Well, permanent until the next moment in time, that is. Then the particle will once again gain an internal gradient equal to the gradient of the background field. This works almost like compound interest. As long as time keeps moving forward and the particle keeps moving, the internal gradient (the particle’s kinetic energy) will continue to change. This grants a steadily increasing velocity leftwards, toward the other particle. This is exactly as we expect and Newton so ably described.

But wait, there’s more! Notice that the particle taking energy from the gradient didn’t remove any energy from the gradient. It never does. That’s the trick Newton missed. The background gradient, upon which our humble test particle resides, remains a temporary and very localized modifier to the particle!

The gradient of the orange version of the particle is now doubled - but only while the particle is in this spot. Its internal energy gradient has not changed. That changes with time, which always advances at the speed of light. The modifier changes with position, which is to say distance. Slowly moving objects accelerate more slowly, since the time factor massively outweighs the distance factor.

  • Time for a particle moving along a gradient adds kinetic energy to the particle.

  • Distance for a particle moving along a gradient grants temporary velocity.

These simple rules explain why the perihelion of Mercury precesses too quickly around the sun, why light bends twice too much when passing close by the sun. The faster something moves, the more the temporary velocity boost of distance matters. This effect works with the particle’s velocity as a fraction of the speed of light. Light, moving exactly equally through both space and time, experiences equal effects from both.

What we have measured over the years with our relatively low speeds and feeble gravity around the earth is the compound interest of time. We ignored the simple fee of distance, because it disappeared as a minute rounding error. Remember, in the graphics above, a mass of one crates a black hole. Most particle masses are well below that, creating truly minute gradients. Especially seeing as most of the time, particles are incredibly far from each other at this scale.


An important note about this model: You’ll notice that both particles have radius one. This is true of all particles, regardless of mass/energy. Particles are not truly point-like. They have fixed sizes, even though this size is incredibly small. Particles are discontinuities in the field. They have an inside and an outside. You cannot get infinitely close to a particle without running into it. There are no infinities. There are no singularities.

The fixed radius of a particle has another effect. A slowly moving particle can gain energy from the same background multiple times because of the overlap. The more slowly it moves, the more quickly it will gain kinetic energy from the same background gradient. This, in effect, “flattens out” the force of gravity at great distances for slow speeds. This may help explain some of the effects attributed to dark matter.

Another effect of the field is that the particle’s total energy at that point in the field determines the rate at which time passes for it - the Lorentz alpha factor of time dilation. The lower you sink into the field, the more slowly time passes for you. It’s not just the gradient - it’s also the depth. A particle using up all the available energy would subjectively experience no time passing, or an alpha factor of zero.