An anonymous reader quotes a report from BBC: Demand for Stephen Hawking's PhD thesis intermittently crashed part of Cambridge University's website as physics fans flocked to read his work. Prof Hawking's 1966 thesis "Properties of expanding universes" was made freely available for the first time on the publications section of university's website at 00:01 BST. More than 60,000 have so far accessed his work as a 24-year-old postgraduate. Prof Hawking said by making it available he hoped to "inspire people." He added: "Anyone, anywhere in the world should have free, unhindered access to not just my research, but to the research of every great and enquiring mind across the spectrum of human understanding. It's wonderful to hear how many people have already shown an interest in downloading my thesis -- hopefully they won't be disappointed now that they finally have access to it!" The 75-year-old's doctoral thesis is the most requested item in Cambridge University's library. Since May 2016, 199 requests were made for the PhD -- most of which are believed to be from the general public rather than academics. The next most requested publication was asked for just 13 times. The Cambridge Library made several PDF files of the thesis available for download -- a high-resolution "72 Mb" file, digitized version that's less than half the size, and a "reduced" version that was even smaller -- but intense interest overwhelmed the servers. Here's the first paragraph of Hawking's introduction: "The idea that the universe is expanding is of recent origin. All the early cosmologies were essentially stationary and even Einstein whose theory of relativity is the basis for almost all modern developments in cosmology, found it natural to suggest a static model of the universe. However there is a very grave difficulty associated with a static model such as Einstein's which is supposed to have existed for an infinite time. For, if the stars had been radiating energy at their present rates for an infinite time, they would have needed an infinite supply of energy. Further, the flux of radiation now would be infinite. Alternatively, if they had only a limited supply of energy, the whole universe would by now have reached thermal equilibrium which is certainly not the case. This difficulty was noticed by Olders who however was not able to suggest any solution. The discovery of the recession of the nebulae by Hubble led to the abandonment of static models in favour of ones which were expanding."
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