Gruber Cosmology Prize 2012 awarded to Charles Bennett and the WMAP Team

June 20th, 2012
This is Charles L. Bennett, Alumni Centennial Professor of Physics and Astronomy at Johns Hopkins University in Baltimore. Bennett and the Wilkinson Microwave Anisotropy Probe team are the recipients of the 2012 Gruber Cosmology Prize. Their observations and analyses of ancient light have provided the unprecedentedly rigorous measurements of the age, content, geometry, and origin of the Universe that now comprise the Standard Cosmological Model. Credit: International Astronomical Union
The 2012 Gruber Cosmology Prize recognises the astronomers for their vital contribution to the study of the properties of the Universe as a whole. The prize citation further recognises that the measurements of the Cosmic Microwave Background (CMB) by Bennett and the WMAP team have helped to transform the current paradigm of the structure formation of the Universe from "appealing scenario into precise science".

Bennett and the WMAP team will receive the US$ 500 000 award. In addition, Bennett will receive a gold medal at the International Astronomical Union meeting in Beijing, which will take place on 21 August 2012.

The Big Bang theory is the prevailing cosmological model that explains the early development and overall properties of the Universe. According to the Big Bang theory, the Universe rapidly expanded from an early, extremely hot and dense plasma of photons, electrons, and protons. This primordial plasma was an opaque fog. As the Universe expanded, it also cooled. Only 378 000 years after the initial expansion, the Universe cooled sufficiently to permit the combination of protons and electrons to form neutral hydrogen atoms. This led to the decoupling of photons, which then could travel freely through the Universe without interacting with matter. The Universe was finally transparent to radiation.

In 1948, Ralph Alpher, Robert Herman, and George Gamow -- among other important results -- predicted that the Universe should be filled with this relic radiation from the Big Bang - the CMB radiation. In 1964, two American radio astronomers -- Penzias and Wilson -- observed the CMB, receiving the 1978 Nobel Prize in Physics for their discovery.

Precise measurements of CMB radiation are critical to cosmology, since any proposed model of the Universe must explain the detailed properties of this radiation. Because everything that is in the Universe now would have to have been there when the Universe was 378 000 years old, some extraordinarily subtle fluctuations in the microwave background would have to have been present -- variations that would represent the seeds that would evolve into the galaxies, clusters of galaxies, and superclusters of galaxies that populate the Universe as we know it.

Seminal work on this topic was performed by the earlier Cosmic Background Explorer (COBE), a satellite telescope. In 1992, the COBE team announced the discovery of those relic wrinkles in space, achieving a major milestone in modern cosmology. However, only follow-up observations at greater sensitivity and resolution, would allow scientists to pin down the fundamental cosmology of the Universe.

Bennett -- the deputy principal investigator of the COBE experiment -- soon became the principal investigator of the Wilkinson Microwave Anisotropy Probe (WMAP). WMAP is a spacecraft launched in 2001 aimed to measure differences in the temperature of the CMB radiation across the full sky. The WMAP's findings have been so precise that they are now commonly known as the Standard Cosmological Model.

"Dr. Bennett's discoveries have literally changed the scientific universe", says John Mather, one of the principal investigators on COBE, who received the 2006 Nobel Prize in Physics as well as the Gruber Cosmology Prize.

Having far exceeded expectations for the quality and quantity of science it produced, the WMAP science team chose to stop taking data in August 2010. Although nobody expects that the release of the final data analysis in late 2012 will contain surprises, it will nonetheless mark the end of an era -- an era that itself marked the dawn of the age of precision cosmology.

Bennett stresses the team nature of the WMAP collaboration. "There are so many heroes who stand up at just the right time and make something happen," Bennett says, "and they all deserve credit for that."

The members of the WMAP team are: Chris Barnes, Rachel Bean, Olivier Dore, Joanna Dunkley, Benjamin M. Gold, Michael Greason, Mark Halpern, Robert Hill, Gary F. Hinshaw, Norman Jarosik, Alan Kogut, Eiichiro Komatsu, David Larson, Michele Limon, Stephan S. Meyer, Michael R. Nolta, Nils Odegard, Lyman Page, Hiranya V. Peiris, Kendrick Smith, David N. Spergel, Greg S. Tucker, Licia Verde, Janet L. Weiland, Edward Wollack, and Edward L. (Ned) Wright.

Provided by International Astronomical Union

This Phys.org Science News Wire page contains a press release issued by an organization mentioned above and is provided to you “as is” with little or no review from Phys.Org staff.

More news stories

Triplefin fish found to have controlled iris radiance

A team of researchers with the University of Tübingen in Germany has found an example of a fish that is able to control light reflected from organs next to its pupils—a form of photolocation. In their paper published in ...

Some black holes erase your past

In the real world, your past uniquely determines your future. If a physicist knows how the universe starts out, she can calculate its future for all time and all space.

'Chameleon' ocean bacteria can shift their colors

Cyanobacteria - which propel the ocean engine and help sustain marine life - can shift their colour like chameleons to match different coloured light across the world's seas, according to research by an international collaboration ...