User:Tohline/DarkMatter/VeraRubin

Early Interactions with Vera Rubin

Note from Joel E. Tohline:  Whether she knew it or not, Dr. Vera C. Rubin was a significant influence on my early astronomy career. What follows are some highlights of my early professional interactions with her.

Neighborhood Meeting at Yale University (1979)

Yale Neighborhood Meeting (1979)

For two years, beginning in the summer of 1978, I held a J. Willard Gibbs instructorship in the astronomy department at Yale University. In my first year, I was encouraged — along with another young astronomer, Dr. Carol A. Christian — to organize a so-called Neighborhood Meeting at Yale. The idea was to focus on a topic that would bring together faculty and graduate students from universities and research centers that were "within driving distance" of the Yale campus; this, and limiting the gathering to 1.5 days (just one overnight stay) would keep travel expenses to a minimum. We accepted the challenge. Given that the astrophysics community, worldwide, was presently making significant progress on a number of issues — both observationally and theoretically — related to galaxies, the topic we picked was …

Rotation: The Dynamical Structure of Galaxies
(A Neighborhood Meeting at Yale University)
Dates: 23 - 24 March 1979

Dr. Vera Rubin was the opening speaker. It was an opportunity for the (> 90) attendees to hear and see — first hand from the expert — how significant the evidence was for flat rotation curves. Five speakers followed: Dr. Jeremiah Ostriker (Princeton), Dr. Alar Toomre (MIT), Dr. Kevin Prendergast (Columbia University), Dr. Paul Schechter (Harvard-Smithsonian CfA), and Dr. Richard Miller (Chicago).

Tohline Visits CIW:DTM (1980)

In early February, 1980, I visited the Carnegie Institution of Washington's Department of Terrestrial Magnetism (CIW:DTM) in Washington, DC to meet and interact with Vera Rubin and her research group. During that visit, I had the opportunity to present an informal talk in which I pitched the idea that flat rotation curves in galaxies might be explained by modifying Newton's law of gravity at large distances. This is the idea that I first presented in a formal manner at the IAU Symposium No. 100 in a paper titled, Stabilizing a Cold Disk with a 1/r Force Law.

Rubin's Scientific American Article (1983)

Vera Rubin published a detailed description of the observational evidence for Dark Matter in Spiral Galaxies in the June, 1983 issue of Scientific American (pp. 96 - 108). An excerpt from near the bottom of p. 102 of that article reads,

"Perhaps the most radical idea for explaining the observed high rotational velocities is one advanced independently by Joel E. Tohline of Louisiana State University and M. Milgrom and J. Bekenstein of the Weizmann Institute of Science. They have proposed that at great distances the Newtonian theory of gravitation must be modified, thereby allowing rotational velocities in galaxies to remain high at such distances from the galactic center even in the absence of unseen mass."

-- Vera C. Rubin

This nod of recognition from Dr. Rubin broadened my visibility — both professionally and among the public — more than any other single citation.

See Also

• Finzi (1963) — On the Validity of Newton's Law at a Long Distance
• Notes from Beatrice Tinsley dated July 3, 1978
• Stabilizing a Cold Disk with a 1/r Force Law
• Does Gravity Exhibit a 1/r Force on the Scale of Galaxies?
• Kuhn & Kruglyak (1987) — Non-Newtonian forces and the invisible mass problem
• Sanders (2014) — A Historical Perspective on Modified Newtonian Dynamics

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