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Balancing Apples & Oranges
"We go through life on earth experiencing
a downward proper-acceleration applied to each part of
our being,
whose effects may be cancelled by an upward frame-variant
force
on the soles of our feet, if we wish to stand and not fall."
/Onana Namuh (1998)
Staying in Our Own Seat
"We go around curves with the local impression of
an outward proper-acceleration applied to each part of
our being,
whose effects may be cancelled by an inward frame-variant
force
from someone/thing nearby, if we wish to sit and not slide."
/Orcim Namuh (2001)
What's New: Here's the 14 May 2005
upgrade
of our note on making the most of ``one-frame concepts'' first in teaching
kinematics.
A "live
remote platform" for empirical studies of anyspeed spacetime (and
nanoworlds
too) for our April 2005 SLAPT
workshop at SIU-E.
One
path from the
metric equation to Lorentz transforms. See if you can find
some mistakes in this
equation
appendix describing motion in terms of physical coordinates
referenced to a local map-frame. How about a modern story line
for the
intro-physics transition between kinematics and dynamics? A
javascript calculator and
equation summary for one-frame views of unidirectional motion, plus
beginnings
for a system of classroom-ready "web transparencies" on emerging science.
A draft paper on
subtle ways to modernize introductory dynamics.
An extreme physics
motion simulator using Adobe
Atmosphere, along with
some notes on discovering patterns in high speed motion on your own.
Minkowski as a classic
pioneer of deep simplification, in the web-version
of our presentation for a symposium on
"The Legacy of Edwin T. Jaynes". An interpretive
cartooning festival with inital focus on the problem sets
above. "Teaching Newton with anticipation..." is our latest adaptation for
introductory physicists. Answers to the puzzlers above can be
found here
and here.
Check out the new discover it
yourself page, and see how far you can take it. A Pythagorean
infomercial, a "vaccine" to empower intro-students
now and minimize pain later, a Java (JDK1.1) applet
version of our anyspeed solver,
and an updated note on map-based
rules. Also find AAPT Conference abstracts (one
for summer 1998, three for
winter), and one way to solve for everything
in an anyspeed acceleration problem.
What's Young: A non-trivial set of web puzzlers to
solve with these
equations , a light-meme
on the relation between circular and
hyperbolic angles, and some map-based
rules of motion, patterned after those of Newton but good at any speed.
For more on this cf. physics/9704018.
As to curved space-time on earth, here's how Newton-like gravity arises from one non-flat metric and it's derivatives.
An any-speed primer is excerpted here.
What's Mature: We have MathCAD worksheets (snapshot of one here) on constant acceleration in two-clock and three-clock relativity, readable with MathSoft's free browser. These allow one to ``play with'' the equations discussed here in both uni-directional and 3D applications.
What's Ancient: An upgrade of physics/9611011 for teachers starting relativity with the metric equation, rather than with Lorentz transforms. It uses a ``synchrony-free'' speed with no limit, a way to add velocities fast, and a frame-invariant ``oriented-scalar'' form for Newton's 2nd law. The revision adds clearer language, discussion of classroom applications, and 3 tables.
Check out the browser-readable (and most up-to-date) version here . Share your thoughts here. A
copy optimized for printing with Adobe's
free Acrobat
PDF reader is here. April
APS/AAPT conference abstract.
Hot Lists: Our Accel-1D Solver won a National Academy Press ``coolest science site'' award in November 1996. If you enjoy this sort of math, help us show that the puzzle-solving constituency remains a significant force on the web, and vote this applied-math site into Starting Point's lowest-common denominator, sci/ed category-free, hot-list by clicking HERE!
Soon: The high (over 30%) fixed "annual percentage rate" on fuel mass during 1 "gee" accelerations.
Check out a Synopsis of the Science These pages contain resources to empower students familiar with only classical kinematics, in the solution of relativistic acceleration problems with variables defined in context of a single inertial frame. They include web-interactive solvers, a variety of examples and derivations, the self-contained Andromeda problem, and a list of yet unanswered questions. The key to these is a more careful operational definition of time (to bypass Newtonian misconceptions from square one), and use of the metric equation as a spacetime extension of Pythagoras' theorem with traveler-time the invariant. These naturally lead to use of multiple kinematics (time/velocity pairs) defined in terms of distances measured with respect to a single inertial reference frame. Such "non-coordinate" variables allow us to see things more simply, and in the process to find surprising uses for Newton's and Galileo's equations.
Something you might discover herein, for example, is that you can describe accelerated uni-directional motion at any speed by replacing "coordinate", by "proper", acceleration and velocity, and then using c2γ in place of ½v2 in the work-energy equation. In other words:
To list some current outside web-links that point in to the map-based relativity stuff at this site...
Other references to the strategies described here include: