8 October 2002
The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics for 2002 with one half jointly to
Raymond Davis Jr
Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, USA, and
International Center for Elementary Particle Physics, University of Tokyo, Japan
“for pioneering contributions to astrophysics, in particular for the detection of cosmic neutrinos”
and the other half to
Associated Universities Inc., Washington DC, USA
“for pioneering contributions to astrophysics, which have led to the discovery of cosmic X-ray sources”.
The Earth lies in the path of a continuous
flux of cosmic particles and other types of radiation. This
year’s Nobel Laureates in Physics have used these very
smallest components of the universe to increase our understanding
of the very largest: the Sun, stars, galaxies and supernovae. The
new knowledge has changed the way we look upon the
The mysterious particle called a neutrino was predicted as early as 1930 by Wolfgang Pauli (Nobel Prize in 1945), but it would take 25 years to prove its existence (by Frederick Reines, Nobel Prize in 1995). This is because neutrinos, which are formed in the fusion processes in the Sun and other stars when hydrogen is converted into helium, hardly interact at all with matter and are therefore very difficult to detect. For example, thousands of billions of neutrinos pass through us every second without our noticing them. Raymond Davis Jr constructed a completely new detector, a gigantic tank filled with 600 tonnes of fluid, which was placed in a mine. Over a period of 30 years he succeeded in capturing a total of 2,000 neutrinos from the Sun and was thus able to prove that fusion provided the energy from the Sun. With another gigantic detector, called Kamiokande, a group of researchers led by Masatoshi Koshiba was able to confirm Davis’s results. They were also able, on 23 February 1987, to detect neutrinos from a distant supernova explosion. They captured twelve of the total of 1016 neutrinos (10,000,000,000,000,000) that passed through the detector. The work of Davis and Koshiba has led to unexpected discoveries and a new, intensive field of research, neutrino-astronomy.
The Sun and all other stars emit electromagnetic radiation at different wavelengths, both visible and invisible light, e.g. X-rays. In order to investigate cosmic X-ray radiation, which is absorbed in Earth’s atmosphere, it is necessary to place instruments in space. Riccardo Giacconi has constructed such instruments. He detected for the first time a source of X-rays outside our solar system and he was the first to prove that the universe contains background radiation of X-ray light. He also detected sources of X-rays that most astronomers now consider to contain black holes. Giacconi constructed the first X-ray telescopes, which have provided us with completely new – and sharp – images of the universe. His contributions laid the foundations of X-ray astronomy.
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Raymond Davis Jr, born 1914 (87
years), in Washington, DC, USA (US citizen). PhD in Chemistry
1942 at Yale University, Connecticut, USA. Professor Emeritus at
the Department of Physics and Astronomy, University of
Pennsylvania, Philadelphia, USA.
Masatoshi Koshiba, born 1926 (76 years), in Toyohashi , Aichi, Japan (Japanese citizen). PhD 1955 at the University of Rochester, New York, USA. Professor Emeritus at the International Center for Elementary Particle Physics, University of Tokyo, Japan.
Riccardo Giacconi, born 1931 (71 years), in Genoa, Italy (US citizen). PhD 1954 at the University of Milan. President of Associated Universities, Inc., Washington, DC, USA.
Prize amount: SEK 10 million. Davis and Koshiba share one half and Giacconi receives the other half.