Newswise — Saul Perlmutter and Brian Schmidt and their teams: the Supernova Cosmology Project and the High-z Supernova Search Team, will receive the 2007 Gruber Cosmology Prize for their discovery that the expansion of the Universe is accelerating. They will receive the prize at a ceremony at the University of Cambridge on September 7.
An accelerating universe was a crazy result that was hard to accept. Yet, two teams, racing neck and neck, simultaneously came to the same conclusion. Their discovery led to the idea of an expansion force, dubbed dark energy. And it suggests that the fate of the universe is to just keep expanding, faster and faster.
The two teams expected to find that the universe would either expand then contract, or it would expand for ever but slowing over the millennia. But there were a growing number of hints that all was not right with the theories of the time.
To find out, they not only needed to be able to measure the speed with which distant objects are travelling away from us, but also how far away they are. And to do this they needed standardized light sources — very bright ones that would be visible to Earth-based telescopes despite being billions of light years away and billions of years old.
The standard light sources they used were exploding stars — in particular Type Ia supernovae. But finding them wasn't easy. Then the analyses over the results turned up very surprising results. "The data wasn't behaving as we thought it would," says Schmidt. "There was a lot of nervous laughter," says Perlmutter. For both teams it was not what they were expecting. For months they both tried to figure out where they had gone wrong, searching for any tiny source of error. But the data was right. The accepted model of the universe was wrong.
Today Perlmutter, Schmidt and their colleagues continue to explore the implications of their work. Schmidt is planning the SkyMapper project, a telescope to map the southern sky. Perlmutter is working on a satellite mission that would study supernovae and the nature of dark energy.
The $US500,000 prize will be shared in four parts: by Schmidt — at the Australian National University; Saul Perlmutter — at the University of California, Berkeley; and the fifty-one co-authors of the key papers.
The Cosmology Prize honors a leading cosmologist, astronomer, astrophysicist or scientific philosopher for theoretical, analytical or conceptual discoveries leading to fundamental advances in the field.
Since 2001, the Cosmology Prize has been awarded in collaboration with the International Astronomical Union. The Foundation's other international prizes are in Genetics, Neuroscience, Justice and Women's Rights. Nominations for the 2008 prizes are now open and close on December 31, 2007.
Profiles of Perlmutter and Schmidt, photos, background information and nomination details for 2008 are available online at http://www.gruberprizes.org.
The official citation reads: The Peter and Patricia Gruber Foundation proudly presents the 2007 Cosmology Prize to Saul Perlmutter and Brian Schmidt, and to the Supernova Cosmology Project and the High-z Supernova Search teams, for their discovery that the expansion of the Universe is currently accelerating.
These observations required the development of new techniques that use supernovae exploding within distant galaxies to measure precise distances across a large fraction of the observable Universe.
The discovery of the accelerated expansion has radically changed our perception of cosmic evolution.
The team members jointly recognized by the prize are:
Saul Perlmutter and the Supernova Cosmology Project team from Australia, Chile, France, Spain, Sweden, UK and USA.1. Gregory Aldering, Lawrence Berkeley National Laboratory2. Brian J. Boyle, Australia Telescope National Facility3. Patricia G. Castro, Instituto Superior Técnico, Lisbon4. Warrick Couch, Swinburne University of Technology5. Susana Deustua, American Astronomical Society6. Richard Ellis, California Institute of Technology7. Sebastien Fabbro, Instituto Superior Técnico, Lisbon8. Alexei Filippenko, University of California, Berkeley (also a member of the High-z team)9. Andrew Fruchter, Space Telescope Science Institute10. Gerson Goldhaber, Lawrence Berkeley National Laboratory11. Ariel Goobar, University of Stockholm12. Donald Groom, Lawrence Berkeley National Laboratory13. Isobel Hook, University of Oxford14. Mike Irwin, University of Cambridge15. Alex Kim, Lawrence Berkeley National Laboratory16. Matthew Kim17. Robert Knop, Vanderbilt University18. Julia C. Lee, Harvard University19. Chris Lidman, European Southern Observatory20. Richard McMahon, University of Cambridge21. Thomas Matheson, NOAO Gemini Science Center22. Heidi Newberg, Rensselaer Polytechnic Institute23. Peter Nugent, Lawrence Berkeley National Laboratory24. Nelson Nunes, University of Cambridge25. Reynald Pain, CNRS-IN2P3, Paris26. Nino Panagia, Space Telescope Science Institute27. Carl Pennypacker, University of California, Berkeley28. Robert Quimby, The University of Texas29. Pilar Ruiz-Lapuente, University of Barcelona30. Brad Schaefer, Louisiana State University31. Nicholas Walton, University of Cambridge
And for the High-z Supernova Search Team: Brian Schmidt and his team from the USA, UK, Germany, Chile and Australia. 1. Peter Challis, Harvard University2. Alejandro Clocchiatti, Pontificia Universidad Católica de Chile3. Alan Diercks, Institute for Systems Biology, Seattle4. Alexei V. Filippenko, University of California, Berkeley5. Peter M. Garnavich, University of Notre Dame6. Ronald L. Gilliland, Space Telescope Science Institute7. Craig J. Hogan, University of Washington8. Saurabh Jha, Stanford Linear Accelerator Center9. Robert P. Kirshner, Harvard University10. Bruno Leibundgut, European Southern Observatory11. Mark M. Phillips, Carnegie Observatories12. David Reiss, Institute for Systems Biology. Seattle13. Adam G. Riess, John Hopkins University14. Robert A. Schommer (Deceased)15. R. Chris Smith, Cerro Tololo Inter-American Observatory, Chile16. Jason Spyromilio, European Southern Observatory17. Christopher Stubbs, Harvard University18. Nicholas B. Suntzeff, Texas A&M University19. John L. Tonry, Institute for Astronomy, Honolulu
There were several papers relating to the discovery. The most significant are: - Riess et al., 1998, AJ, 116, 1009, "Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant"http://www.journals.uchicago.edu/AJ/journal/issues/v116n3/980111/980111.web.pdf - Perlmutter et al. 1999, ApJ, 517, 565, "Measurements of Omega and Lambda from 42 High-Redshift Supernovae"http://www.journals.uchicago.edu/ApJ/journal/issues/ApJ/v517n2/39148/39148.web.pdf
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