To discover what kind of universe we are living in it’s necessary to put some observational constraints on the theory, which the observational cosmologist does by looking at remote sources of radiation. The further photons have travelled through the universe to reach our telescopes, the more they tell us about its shape. Science Watch this period has two complementary papers on cosmic geometry, both of them new entrants to the Physics Top Ten. Paper #3 on observations of exploding stars in distant galaxies, together with #7 on microwave background radiation, shows mounting evidence for a flat universe. In 1988 Saul Perlmutter started the Supernova Cosmology Project (SCP), with the primary goal of establishing the relationship between observed brightness and distance for Type Ia supernovae. Science Watch reported the results of a rival collaboration with similar goals in the last period (12 [1]:6, January/February 2001), where evidence that the universe is accelerating was garnered from just 10 supernovae. In #3 Perlmutter analyzes a larger dataset from 42 high-redshift supernovae and reaches essentially the same conclusions. The observational technique is extremely demanding because these supernovae (which erupt without warning) must be detected before they have reached their peak brightness, and then followed with spectrometry and photometry for two to three months. SCP uses several of the world’s largest telescopes to get data. For each supernova the SCP measured the redshift, which is the easy part, and the effective peak magnitude, which is hard. The magnitude estimate needs correction for cosmological effects and the dimming of light by dust in our galaxy. The corrected data are then plotted on a Hubble Diagram (first used in 1929). At low redshift the magnitude-redshift relation is linear, and any deviation from this at high redshift carries information about the geometry of the universe. The conclusions in #3 include an age for the universe of 14.9 billion years, a compelling argument that the geometry is flat (follows Euclidean geometry), and evidence that the expansion is accelerating. Newcomer #7 reports "Boomerang" observations of structure in the cosmic microwave background, the dying echo of the Big Bang that is almost, but not quite, isotropic. Tiny irregularities in the early universe imprinted the background in the form of small anisotropies of the temperature. These wrinkles in the background contain information about basic cosmological parameters. The Boomerang experiment is a microwave telescope taken to 38 km altitude by a balloon over Antarctica. In a 249-hour flight the telescope mapped a part of the sky that is free of thermal radiation from interstellar dust. The resulting maps show variations at the level of 1 part in 100,000 in the cosmic background temperature of 2.73 K, and they give the angular scale of the minuscule fluctuations. What the astronomers are seeing in these ripples are sound waves caused by gravitational forces acting on plasma in the early universe. The power spectrum of temperature fluctuations peaks on an angular scale of about 1 degree which implies a flat universe, as suggested by the supernova data. Papers #3 and #7 find that ordinary matter and dark matter together account for less than half the content of the universe. There is a ubiquitous dark energy as well, which is not subject to gravitational force, and which repels matter, so driving the acceleration of the universe. This fifth force of physics, known as quintessence, represents an energy intrinsic to the structure of spacetime. Right now cosmologists are keen to get more evidence for quintessence, and a battery of new astronomical satellites are on the drawing board. Perlmutter’s supernova hunters are upping their game with a proposal for SNAP, the SuperNova Acceleration Probe, which will discover 2,000 supernovae a year. June 2001 should see the launch of the Microwave Anisotropy Probe, a mission to map the microwave ripples with even greater accuracy. These are exciting times for cosmologists, and more Hot Papers from them are in
prospect. |
| Science
Watch®, March/April 2001, Vol. 12, No. 2 Citing URL: http://www.sciencewatch.com/march-april2001/sw_march-april2001_page6.htm |
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