File:MOND vs Newtonian rotation.gif

Summary

Description
English: MOND is a possible explanation for the observed v(r) curve for stars in a galaxy (which is incompatible with Newtonian gravity). The observed behaviour is explained by assuming that Newton's second law (F=m a) is modified for very small values of a.
Date
Source https://twitter.com/j_bertolotti/status/1283363962780815361
Author Jacopo Bertolotti
Permission
(Reusing this file)
https://twitter.com/j_bertolotti/status/1030470604418428929

Mathematica 12.1 code

\[Rho]0 = 5 ; Rs = 10; a0 =.; G = 1; M[r_] := \[Rho]0 (1 - Cosh[r] + Sinh[r]);(*Exponential mass distribution*)
\[Omega]newton[pos_] := Sqrt[(G M[r])/Norm[pos]^3];
\[Omega]MOND[r_, a0_] := Evaluate[FullSimplify[Sqrt[Evaluate[ a /. Solve[(G M[r])/Norm[r]^2 == a/Sqrt[1 + a0^2/a^2], a][[4]] ]/ Norm[r]]] ]
rmax = 10;
\[Delta]r = 0.1;
a0 = 20;
p0 = Table[
   Grid[{
     {
      Plot[\[Omega]newton[r]*r, {r, 0, rmax}, ImageSize -> Small, PlotRange -> {0, 4}, Axes -> False, Frame -> True, FrameTicks -> None, FrameLabel -> {{"v", ""}, {"r", "Newtonian gravity"}}, LabelStyle -> {Bold, LightGray}, PlotStyle -> {White}, Background -> Black]
      ,
      Plot[\[Omega]MOND[r, a0]*r, {r, 0, rmax}, ImageSize -> Small, PlotRange -> {0, 4}, Axes -> False, Frame -> True, FrameTicks -> None, FrameLabel -> {{"v", ""}, {"r", "MOND"}}, LabelStyle -> {Bold, LightGray}, PlotStyle -> {White}, Background -> Black]
      }, {
      Graphics[{
        Flatten@Table[{
           Orange, 
           Disk[{0, 0}, r + \[Delta]r, {0 + \[Omega]newton[r] t, \[Pi] + \[Omega]newton[r] t}],
           Black, 
           Disk[{0, 0}, r, {0 + \[Omega]newton[r] t, \[Pi] + \[Omega]newton[r] t}],
           Purple, 
           Disk[{0, 0}, r + \[Delta]r, {\[Pi] + \[Omega]newton[r] t, 2 \[Pi] + \[Omega]newton[r] t}],
           Black, 
           Disk[{0, 0}, r, {\[Pi] + \[Omega]newton[r] t, 2 \[Pi] + \[Omega]newton[r] t}]
           }, {r, rmax - \[Delta]r, \[Delta]r/10, -\[Delta]r}]
        }, PlotRange -> 1.1 {{-rmax, rmax}, {-rmax, rmax}}, 
       Background -> Black]
      ,
      Graphics[{
        Flatten@Table[{
           Orange, 
           Disk[{0, 0}, 
            r + \[Delta]r, {0 + \[Omega]MOND[r, a0] t, \[Pi] + \[Omega]MOND[r, a0] t}],
           Black, 
           Disk[{0, 0}, r, {0 + \[Omega]MOND[r, a0] t, \[Pi] + \[Omega]MOND[r, a0] t}],
           Purple, 
           Disk[{0, 0}, r + \[Delta]r, {\[Pi] + \[Omega]MOND[r, a0] t, 2 \[Pi] + \[Omega]MOND[r, a0] t}],
           Black, 
           Disk[{0, 0}, r, {\[Pi] + \[Omega]MOND[r, a0] t, 2 \[Pi] + \[Omega]MOND[r, a0] t}]
           }, {r, rmax - \[Delta]r, \[Delta]r/10, -\[Delta]r}]
        }, PlotRange -> 1.1 {{-rmax, rmax}, {-rmax, rmax}}, 
       Background -> Black]
      }}, Background -> Black]
   , {t, 0, 10, 0.1}];
ListAnimate[p0]

Licensing

I, the copyright holder of this work, hereby publish it under the following license:
Creative Commons CC-Zero This file is made available under the Creative Commons CC0 1.0 Universal Public Domain Dedication.
The person who associated a work with this deed has dedicated the work to the public domain by waiving all of their rights to the work worldwide under copyright law, including all related and neighboring rights, to the extent allowed by law. You can copy, modify, distribute and perform the work, even for commercial purposes, all without asking permission.

Category:CC-Zero#MOND%20vs%20Newtonian%20rotation.gif
Category:Self-published work Category:Animated GIF files Category:Galactic rotation profiles Category:Images with Mathematica source code Category:Modified Newtonian Dynamic Category:Animations of astrophysics Category:Spirals
Category:Animated GIF files Category:Animations of astrophysics Category:CC-Zero Category:Galactic rotation profiles Category:Images with Mathematica source code Category:Modified Newtonian Dynamic Category:Pages using deprecated source tags Category:Self-published work Category:Spirals