Appendix/Ramblings/DarkMatterMusings: Difference between revisions

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Created page with "<!-- __FORCETOC__ will force the creation of a Table of Contents --> <!-- __NOTOC__ will force TOC off --> =Musings Regarding Dark Matter and Dark Energy= [Joel E. Tohline recollection on 3/8/2015] It was during my first year (July 1978 - June 1979) as a J. Willard Gibbs Instructor in the Astronomy Department at Yale University that I started wondering whether the nearly ubiquitous display of "flat rotation curves" in disk galaxies might be explained, not via the dark..."
 
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[Joel E. Tohline recollection on 3/8/2015]  It was during my first year (July 1978 - June 1979) as a J. Willard Gibbs Instructor in the Astronomy Department at Yale University that I started wondering whether the nearly ubiquitous display of "flat rotation curves" in disk galaxies might be explained, not via the dark matter hypothesis, but by invoking a <math>1/r</math> force-law for gravity at large distances.  My reasoning was simple:
[Joel E. Tohline recollection on 3/8/2015]  It was during my first year (July 1978 - June 1979) as a J. Willard Gibbs Instructor in the Astronomy Department at Yale University that I started wondering whether the nearly ubiquitous display of "flat rotation curves" in disk galaxies might be explained, not via the dark matter hypothesis, but by invoking a <math>1/r</math> force-law for gravity at large distances.  My reasoning was simple:
<ol>
<li>I was uncomfortable with the "dark matter" hypothesis, which smelled to me like the story of aether, all over again.</li>
<li>If Isaac Newton had been handed Vera Rubin's observations &#8212; which showed that orbital velocities were approximately constant with distance &#8212; instead of Kepler's observations &#8212; which showed that orbital velocities behaved as <math>v \propto r^{-1/2}</math> &#8212; he likely would have hypothesized that the gravitational acceleration due to a central point mass is proportional to <math>r^{-1}</math> instead of <math>r^{-2}</math>.</li>
</ol>
While I put quite a lot of thought into this idea in the late '70s and early '80s &#8212; and I still give it some thought from time to time because I consider the astrophysics community's fundamental understanding of "dark matter" and now, too, "dark energy" to be weak &#8212; I produced only two publications on the topic, neither of which was in a refereed archival journal:
<ul>
<li>''Stabilizing a Cold Disk with a <math>1/r</math> Force Law.''</li>
<li>''Does Gravity Exhibit a <math>1/r</math> force on the Scale of Galaxies?''</li>
</ul>


=See Also=
=See Also=


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Revision as of 18:55, 2 January 2022

Musings Regarding Dark Matter and Dark Energy

[Joel E. Tohline recollection on 3/8/2015] It was during my first year (July 1978 - June 1979) as a J. Willard Gibbs Instructor in the Astronomy Department at Yale University that I started wondering whether the nearly ubiquitous display of "flat rotation curves" in disk galaxies might be explained, not via the dark matter hypothesis, but by invoking a 1/r force-law for gravity at large distances. My reasoning was simple:

  1. I was uncomfortable with the "dark matter" hypothesis, which smelled to me like the story of aether, all over again.
  2. If Isaac Newton had been handed Vera Rubin's observations — which showed that orbital velocities were approximately constant with distance — instead of Kepler's observations — which showed that orbital velocities behaved as vr1/2 — he likely would have hypothesized that the gravitational acceleration due to a central point mass is proportional to r1 instead of r2.

While I put quite a lot of thought into this idea in the late '70s and early '80s — and I still give it some thought from time to time because I consider the astrophysics community's fundamental understanding of "dark matter" and now, too, "dark energy" to be weak — I produced only two publications on the topic, neither of which was in a refereed archival journal:

  • Stabilizing a Cold Disk with a 1/r Force Law.
  • Does Gravity Exhibit a 1/r force on the Scale of Galaxies?

See Also

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