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Report for the Academic Year 1992-1993 - The Institute Libraries ...

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THE SCHOOL OF NATURAL SCIENCES<br />

in "Communications in Ma<strong>the</strong>matical Physics." O<strong>the</strong>rs have resulted in preprints<br />

and papers by Bleher alone. <strong>The</strong> general aim of this work is to understand <strong>the</strong><br />

effects of <strong>the</strong> transition from order to chaos in a classical dynamical system upon<br />

<strong>the</strong> statistical behavior of eigenstates in <strong>the</strong> corresponding quantum system. <strong>The</strong>y<br />

are looking in detail at <strong>the</strong> eigenvalue statistics of classical systems that are com-<br />

pletely integrable and so have maximal order. Numerical evidence suggests that<br />

classical order goes with quantum disorder and vice versa. But no rigorous<br />

statement of <strong>the</strong> inverse relationship between classical and quantum order has<br />

been <strong>for</strong>mulated, let alone proved. Dyson and Bleher hope that <strong>the</strong>ir work will<br />

be a small step in this direction. <strong>The</strong>y have had a lot of help from Peter Sarnak<br />

in <strong>the</strong> Princeton University ma<strong>the</strong>matics department.<br />

Professor Dyson spent part of <strong>the</strong> year preparing lectures <strong>for</strong> delivery at a variety<br />

of <strong>for</strong>mal occasions. One was a Compton Memorial Lecture given at Washington<br />

University in St. Louis in conjunction with a meeting of astronomers to discuss<br />

<strong>the</strong> scientific output of <strong>the</strong> Compton Gamma-Ray Observatory now in orbit.<br />

This lecture, with <strong>the</strong> title "Revolutions in Astronomy," was also given as a<br />

Faculty Lecture to <strong>the</strong> <strong>Institute</strong> community. Ano<strong>the</strong>r lecture, with <strong>the</strong> title "Sci-<br />

ence and Ethics," was given at <strong>the</strong> Mellon Seminar on Science and Society at <strong>the</strong><br />

<strong>Institute</strong>. A third lecture, with <strong>the</strong> title "Homage to George Green," was given<br />

in England in July <strong>1993</strong> at <strong>the</strong> celebration of George Green's 200th birthday. He<br />

also gave convocation addresses at a couple of Hberal arts colleges under <strong>the</strong> title<br />

"<strong>The</strong> Scientist as Rebel."<br />

PIET hut's research has focused on <strong>the</strong> study of dense stellar systems, with<br />

applications to globular star clusters and galactic nuclei. He has taken part in <strong>the</strong><br />

design of large-scale simulations in coUisional stellar dynamics, to be per<strong>for</strong>med<br />

on <strong>the</strong> 1 Tflops special-purpose computer under development in <strong>the</strong> astronomy<br />

department at Tokyo University. As part of this ef<strong>for</strong>t, new tree-based algo-<br />

rithms <strong>for</strong> <strong>the</strong> treatment of close encounters and physical collisions were devel-<br />

oped in collaboration with Jun Makino from Tokyo University and Steve<br />

McMillan from Drexel University.<br />

O<strong>the</strong>r studies of globular clusters included a series of Fokker-Planck simulations<br />

of post-collapse evolution, in which a detailed investigation was made of <strong>the</strong><br />

properties of gravo<strong>the</strong>rmal oscillations, in collaboration with Joseph Breeden<br />

and Haldan Cohn of Indiana University. A <strong>the</strong>oretical study of <strong>the</strong> <strong>for</strong>mation<br />

and dynamical evolution of stellar-mass black hole remnants in globular clusters<br />

was carried out in collaboration with Shri Kulkarni from <strong>the</strong> Cali<strong>for</strong>nia <strong>Institute</strong><br />

of Technology and Steve McMillan. This work resulted in potentially interesting<br />

observational consequences, by predicting a significant <strong>for</strong>mation rate of black<br />

hole containing X-ray binaries.<br />

39

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