Making universe, constants out of nothing.
Such questions have long perplexed researchers interested in understanding why the fundamental constants of nature have the particular values observed in our universe.
Some believe there exists a unique, logically consistent theory of everything from which all constants can, in principle, be calculated -- though no one has yet found a completely convincing candidate for this theory.
Others appeal to the notion that these values are to a large extent consistent with the existence of conscious observers who can wonder about such questions. In other words, if one assumes that the production of heavy elements in stars and their dispersal in supernova explosions are essential for the evolution of life, this anthropic principle imposes strict constraints on the values of the electron and proton masses and other constants.
Now, Alexander Vilenkin of Tufts University in Medford, Mass., has taken an alternative approach to determining the most likely values of the fundamental constants of nature -- one rooted in quantum cosmology. He outlines his argument in the Feb. 6 Physical Review Letters.
Quantum cosmology posits that incredibly tiny universes spontaneously nucleate out of nothing. All of the universes in this metauniverse are disconnected from one another and generally have different initial conditions and values of the fundamental constants.
Once formed, these universes undergo very brief periods of exceedingly rapid expansion. In effect, during this process of inflation, gravity becomes a repulsive force.
In a variation of this picture, quantum cosmology pioneer Andrei D. Linde of Stanford University has proposed that the universe is a huge, growing fractal. Such a universe consists of many inflating balls, which in turn produce new balls, and so on. Only in pockets where inflation has stopped have the laws of physics become fixed.
Vilenkin assumes that we are one of an infinite number of civilizations living in regions of the metauniverse where inflation has virtually ceased.
"Although it may be tempting to believe that our civilization is very special, the history of cosmology demonstrates that the assumption of being average is often a fruitful hypothesis," he says. "I call this the principle of mediocrity."
"It's a reasonable approach to take," says J. Richard Gott III of Princeton University. In 1993, Gott used a similar viewpoint -- calling it the Copernican principle -- to estimate our likelihood of colonizing our galaxy and encountering intelligent extraterrestrial life.
Vilenkin argues that for our type of intelligent life to exist, the local universe must have certain features. By applying the principle of mediocrity, "we can explain some values of the constants that otherwise seem [specially selected] and predict some constants that have not yet been measured," he says.
Vilenkin's approach favors local universes in which inflation plays a significant role in creating a large volume with room for lots of civilizations. But this process tends to wash out any quantum fluctuations that could lead to galaxy formation. Hence, the principle of mediocrity favors scenarios in which cosmic strings or other spacetime defects (SN: 10/15/94, p.248) serve as the seeds for galaxies and other cosmic structures.
It also suggests that the cosmological constant -- a correction term sometimes added to the equations of general relativity -- has a small but appreciable value. Theorists have generally argued that no such correction term is necessary (SN: 1/5/91, p.12).
"Though everything is very speculative at this point, this work suggests that maybe there's another way of thinking about things which would make a nonzero cosmological constant sound much more plausible," says Alan H. Guth of the Massachusetts Institute of Technology.
Vilenkin admits he is pushing the ideas of cosmology and quantum mechanics far beyond the range over which they have been tested. However, "my approach makes direct observational predictions and is therefore falsifiable," he says.
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|Title Annotation:||new theory contributes to understanding values of universe's fundamental constants|
|Date:||Feb 18, 1995|
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