4 comments

  • srean2 hours ago
    <i>In a 3d world one can escape from the Earth&#x27;s gravitational field. On the flat-world equivalent there is no escape.</i> You can checkout but never leave. There ought to be a science fiction story based on this premise.<p>Things get interesting in 2d flatland.<p>There the field or force has to decay as 1&#x2F;r because the circumference of the boundary scales as O(r). But that&#x27;s the <i>field</i>, to get to the potential you need to integrate and then you get a function that is logarithmic with distance.<p>A consequence of that is the potential does not drop to zero as you go further away. Unlike what is the case for the 3d case.<p>If you have heard that about a random-walking bird that returns infinitely often but a random-flying bird one that doesn&#x27;t, that&#x27;s sorta related.<p>Totally unrelated, was quite thrilled to see this map of the sphere<p><a href="https:&#x2F;&#x2F;substackcdn.com&#x2F;image&#x2F;fetch&#x2F;$s_!8JEP!,f_auto,q_auto:good,fl_progressive:steep&#x2F;https%3A%2F%2Fsubstack-post-media.s3.amazonaws.com%2Fpublic%2Fimages%2F49ffbc16-5e0e-4bce-9a37-e5c7b09019c7_1600x900.png" rel="nofollow">https:&#x2F;&#x2F;substackcdn.com&#x2F;image&#x2F;fetch&#x2F;$s_!8JEP!,f_auto,q_auto:...</a><p>because I had been entertaining myself by making toy globes out of paper and it seems this polyconic map was the one I had used (an interrupted version of this).<p>The more conventional way is to use gores using interrupted sinusoidal that look like a string of lobes connected at their common equatorial hip.<p><a href="https:&#x2F;&#x2F;www.wolframcloud.com&#x2F;obj&#x2F;resourcesystem&#x2F;published&#x2F;DemonstrationRepository&#x2F;deployments&#x2F;InterruptedSinusoidalMapProjection&#x2F;img&#x2F;InterruptedSinusoidalMapProjection_Snapshot-2.png" rel="nofollow">https:&#x2F;&#x2F;www.wolframcloud.com&#x2F;obj&#x2F;resourcesystem&#x2F;published&#x2F;De...</a><p>What I was working with were more like flowers, one for each hemisphere, with the pole at the center.
    • feoren32 minutes ago
      &gt; A consequence of that is the potential does not drop to zero as you go further away. Unlike what is the case for the 3d case.<p>The integral of const&#x2F;r^2 doesn&#x27;t drop to zero as r gets larger, but approaches some constant. Unlike const&#x2F;r, which is unbounded as r gets larger. So potential is bounded in R3, but not in R2.
  • peri-cl2 hours ago
    It&#x27;s fun to puzzle through why optical reflections, active radar, and things like that are inverse R^4. (It&#x27;s just two inverse-square laws composed together).<p>Dipoles, like magnetic fields and planetary tidal forces, decay as an inverse R^3. That&#x27;s less intuitive.
  • redwood2 hours ago
    While we&#x27;re on this... it is arguably even more befuddling to recognize that the information content potential of space apparently correlates with the surface area rather than volume <a href="https:&#x2F;&#x2F;en.wikipedia.org&#x2F;wiki&#x2F;Holographic_principle" rel="nofollow">https:&#x2F;&#x2F;en.wikipedia.org&#x2F;wiki&#x2F;Holographic_principle</a>
  • a3w1 hour ago
    [flagged]
    • fny1 hour ago
      Maybe to signal the opposite. I&#x27;ve started using double dashes ever since LLMs stole my favorite symbol.