at the university. In the fall the same year he received treatment at a sanatorium for what turned out to be tuberculosis. The faculty at the University in Oslo sent Jebsen's thesis for evaluation to Carl Wilhelm Oseen at the University of Uppsala. He had some critical comments with the result that it was approved for the more ordinary cand.real. degree. But Oseen had found this student so promising that he shortly thereafter was invited to work with him. Jebsen came to Uppsala in the fall of 1919 where he could follow lectures by Oseen on general relativity. Jebsen-Birkhoff theorem At that time it was natural to study the exact solution of Einstein’s equations for the metric outside a static, spherical mass distribution found by Karl Schwarzschild in 1916. Jebsen set out to extend this achievement to the more general case for a spherical mass distribution that varied with time. This would be of relevance for pulsating stars. After a relative short time he came to the surprising result that the static Schwarzschild solution still gives the exact metric tensor outside the mass distribution. It means that such a spherical, pulsating star will not emit gravitational waves. During the spring 1920 he hoped to get the results published through the Royal Swedish Academy of Sciences. This was met by some difficulties, but after the intervention by Oseen it was accepted for publication in a Swedish journal for the natural sciences where it appeared the following year. His work did not seem to generate much interest. One reason can be that the Swedish journal was not so well-known abroad. A couple of years later it was rediscovered by George David Birkhoff who included it in a popular science book he wrote. Thus it became known as "Birkhoff's theorem." The original discovery of Jebsen was pointed out first in 2005, and translated into English. From that time on it is now more often called the Jebsen-Birkhoff theorem. Most modern-day proofs are along the lines of the original Jebsen derivation. Final years Einstein came on a visit to Oslo in June 1920. He would give three public lectures about the theory of relativity after the invitation by the Student Society. Jebsen was also there, but it is not clear if he met him personally. In the fall the same year Jebsen traveled with his family to Bolzano in northern Italy in order to