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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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