2000 HSS/PSA Program 1 - History of Science Society
2000 HSS/PSA Program 1 - History of Science Society
2000 HSS/PSA Program 1 - History of Science Society
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<strong>HSS</strong> Abstracts<br />
intellectuals. China’s reception <strong>of</strong> relativity in these early years was fast and<br />
almost unanimously positive. Fifty years later however, during the Cultural<br />
Revolution, Einstein and his relativity became the targets <strong>of</strong> organized criticism.<br />
This criticism was in general not scientific, but philosophical, ideological,<br />
and political. Critics <strong>of</strong>ten deliberately confused relativity in physics with<br />
relativism in philosophy. They labeled Einstein “the greatest bourgeois<br />
reactionary academic authority in natural science,” and relativity a “reactionary<br />
bourgeois theory” . The critics claimed they made Einstein and relativity<br />
“targets <strong>of</strong> revolution” because “Natural science can not be advanced without<br />
revolutionizing the theory <strong>of</strong> relativity.” This organized criticism was only a<br />
beginning <strong>of</strong> the so-called unprecedented “proletarian scientific revolution”<br />
in China. Ironically, the criticism movement in a sense helped promote the<br />
studies on Einstein and relativity in China. One <strong>of</strong> most significant “byproducts”<br />
was the publication <strong>of</strong> the comprehensive three-volume Chinese<br />
translation <strong>of</strong> Einstein’s collected works, which were published in 1976, the<br />
year when the “Cultural Revolution” ended. In this paper, I will trace the<br />
origin and development <strong>of</strong> the criticism during the “Cultural Revolution” . I<br />
will pay special attention to the motivations behind Einstein’s detractors.<br />
Finally, I will discuss the consequences <strong>of</strong> the criticism and the lessons that<br />
may be drawn from this upheaval in Chinese science.<br />
H<br />
S<br />
S<br />
Karl Hufbauer University <strong>of</strong> California, Irvine<br />
J. Robert Oppenheimer’s Path to Black Holes<br />
During the winter and spring <strong>of</strong> 1939, as many leading American physicists<br />
were rapidly following up on the announcement <strong>of</strong> nuclear fission, the<br />
prominent theoretical physicist J. Robert Oppenheimer and his Ph.D. candidate<br />
Hartland S. Snyder were theorizing about the collapse <strong>of</strong> massive stars that<br />
had exhausted their energy reserves into what have come to be called “black<br />
holes.” In this paper I first argue that Oppenheimer’s academic contacts at<br />
Caltech and Mt. Wilson over the preceding decade together with string <strong>of</strong> near<br />
misses in his chosen field set the stage for his astrophysical research. Then I<br />
delineate his immediate intellectual path from an interest in the sources <strong>of</strong><br />
stellar energy to an engagement with the pr<strong>of</strong>ound yet esoteric problem <strong>of</strong><br />
stellar collapse, suggesting that Hans Bethe’s breakthrough on the first issue<br />
was a powerful incentive for work on the second. Next I consider how<br />
Oppenheimer and Snyder developed their scenario for a black hole’s formation.<br />
And finally I discuss the reasons why the contemporary physics and astronomy<br />
communities paid so little heed to their findings. Besides illuminating<br />
Oppenheimer’s career and the history <strong>of</strong> theoretical astrophysics during the<br />
1930s, this story is <strong>of</strong> interest for the light that it sheds on the general issues <strong>of</strong><br />
problem choice and research evaluation in interdisciplinary domains.<br />
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