Microwave Anisotropy Probe

Is the Universe Infinite?

``Some Say the World Will End in Fire, Others Say in Ice''

Just as Robert Frost imagined two possible fates for the Earth in his poem, cosmologists envision two possible fates for the universe:

The evolution of the universe is determined by a struggle between the momentum of expansion and the pull of gravity. The rate of expansion is determined by the Hubble Constant, H0, while the strength of gravity depends on the density of the universe. If the density of the universe is less than the ``critical density'' which is proportional to the square of the Hubble constant, then the universe will expand forever. If the density of the universe is greater than the ``critical density'', then gravity will eventually win and the universe will collapse back on itself.

Geometry of the Universe

The density of the universe also determines its geometry. If the density of the universe exceeds the critical density, then the geometry of space is closed and positively curved like the surface of a sphere. This implies that photon paths diverge slowly and eventually return back to a point. If the density of the universe is less than the critical density, then the geometry of space is open, negatively curved like the surface of a saddle. If the density of the universe exactly equals the critical density, then the geometry of the universe is flat like a sheet of paper. Thus, there is a direct link between the geometry of the universe and its fate.

The simplest version of the inflationary theory, an extension of the Big Bang theory, predicts that the density of the universe is very close to the critical density, and that the geometry of the universe is flat, like a sheet of paper.

Measurements from MAP

The MAP satellite aims to measure the basic parameters of the Big Bang theory including the geometry of the universe. If the universe is open, then the cosmic microwave background fluctuations are largest on the half degree scale. If the universe is flat, the the fluctuations are largest on the degree scale. While if the universe is closed, the fluctuations are largest on even larger scale. Thus, MAP's measurement of the fluctuation scale directly probes the density of the universe and will give cosmologists insight into the ultimate fate of the universe.



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David N. Spergel / dns@astro.princeton.edu
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Last updated: March 22, 1996