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Bill Sloman wrote:In fact is was primitive way of handling elliptical orbits before they were recognised to be elliptical. It was a well-thought-through complication that worked pretty well.Don wrote:Propositions promulgated by PR people such as Bernays are often widelyJeroen Belleman wrote:>john larkin wrote:>Don wrote:>john larkin wrote:>>>
https://www.inc.com/jessica-stillman/einstein-and-adam-grant-agree-the-puzzle-principle-will-make-you-instantly-smarter/91102339
>
Cohen's book looks interesting, so I ordered it.
>
I'm now reading Gleick's short biography of Isaac Newton, who was a
very weird guy.
Einstein loved the sound of his own metaphysical bark and wasn't above
fudging the score:
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<https://pubs.aip.org/physicstoday/article/58/9/43/399405/Einstein-Versus-the-Physical-Review-A-great>
>
Regardless, my followup isn't about this thread's titular Einstein.
It's about Newton.
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"Did you know? It was AYABHATA & not Newton or (sic) Leibniz who
first developed Calculus"
>
<https://x.com/Aelthemplaer/status/1874573331330167032>
Seems to me that if gravity has finite velocity, there have to be
gravitational waves.
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Yes, and if there are gravitational waves, there must be quantization
effects. Where waves and matter interact, quantization occurs. The
scale of the phenomena, both in time and in size, may make it hard
to recognize it as such though.
>
That said, there are plenty of examples of quantization effects in
the behaviour of objects in our solar system. Orbital resonances,
tidal locking, Trojans, what else?.
>
Come to think of it, when a star gets ejected at high speed from a
star cluster, as sometimes happens, isn't that in some way similar
to the decay of a radioactive atom?
For what it's worth, both the photoelectric effect in Einstein's
equation and Millikan's measurement make perfect sense to me. Although
light with weight works with me, things begin to become unworkable
with Schrödinger and Einstein's field equations.
Schroedinger's and Einstein's field equation are both perfectly workable
representations of reality. They wouldn't have become widely accepted if
they weren't. If you can't get them to work for you, you probably need
to sign up for a university course to improve your skills.
accepted.
THE HIGGS FAKE: HOW PARTICLE PHYSICISTS FOOLED THE NOBEL COMMITTEE
the epicycle theory has become a synonym of thoughtless
complication. ...
Einstein's general relativity refined Newton's law ofIt took a long time before we had enough precise observations to nail down the deviations from Newton's Law of Gravitation.
gravitation, but it did not simplify it in the sense that
it needed less parameters. Newton's theory never underwent
the piling up of absurd complications that we know from
the standard model.
Nevertheless they dare to compareThe standard model fits current observations pretty well. As with Einstein's elaboration of Newton's over-simple theory, any new theory has to fit the observations we've made so far.
their illogical turmoil to Newton's clear thoughts, hoping
that the standard model will be "embedded" by a future
theory of the sought-after new Einstein. Wishful thinking.
It is rather a Copernicus or a Kepler that is needed.Copernicus articulated an idea. Kepler took Brahe's precise observations, and gave Newton organised data that was good enough to be worth thinking about
All that will remain after the crash of the standard model,Probably wrong. The standard model fit's some aspects of reality remarkably well
when the thin fouling is brushed off the rocks, is quantum
mechanics as developed in the 1920s.
But this is a much tooDon't be silly.
scary perspective for particle physicists to let it even
faintly cross their minds.
Besides the epicycle model that dominated astronomy forEpicycles fitted the crude eyeball data which was all we had for fifteen centuries. Brahe's data was still eyeball data, but he used huge and expensive observational tools to make his observations somewhat more precise than anybody had managed before.
fifteen centuries, history has instructive examples on a
much shorter time scale.
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