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Primal Scream: The Infant Universe Speaks

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Primal Scream: The Infant Universe Speaks

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DENVER - An astronomer has turned observations of the early universe into a sound clip that represents a primal scream from the first million years after the Big Bang.

Mark Whittle, an astronomer at the University of Virginia, based the work on a "wonderful gift from Nature," the cosmic microwave background (CMB) that was unleashed when the universe was about 380,000 years old. At that point in time, a dense fog began to clear and radiation was first allowed to escape its natal cocoon.

Other studies have generated sound clips out of data from the universe and even from our own solar system. But none have reached so far back in time and space.

Whittle first figured out the sound at the time of the CMB itself. Then he and colleagues made some assumptions about the dense state of things before the CMB and modeled the sound that likely occurred in the interval between the Big Bang and the release of the CMB.

Sound would have traveled easily through the early cosmos, he explained, because the more compact universe was denser, like a hot, thin atmosphere.

"If we want to access times before and after the microwave background, we have to make use of computer simulations," Whittle said here today at a meeting of the American Astronomical Society.

The simulations generated a growing hiss that resembles a roaring jet plane flying low overhead [Hear the clip]. It represents the first million years of the cosmos and it is compressed into about 5 seconds for easy listening.

"I was relieved," Whittle said. "I didn’t want the universe to be some wimpy, quiet thing. But I didn’t want it to be inhumanly, fatally loud. And it isn’t. It’s just loud…and that’s great, just great."

Whittle said that most people think the theoretical Big Bang starts out with a huge explosion, then it gets quieter with time.

"In fact, the Big Bang starts out completely silent," Whittle said. "The expansion…is purely radial – there’s no sideways motion. There are no pressure waves. What they are, are density variations on all scales, everywhere."

The universe expanded rapidly after the Big Bang, during a period called inflation. Later, it continued to expand at a slower rate as it cooled enough for gas to condense and form stars. All this time, density variations contributed characteristics to the sound that Whittle's team has determined.

"It’s nice to kind of get a clean handle on it," Whittle said. "It’s as if the universe is a bad concert hall. It has drapes and carpets which absorb the high frequencies. It deadens the sound. What you’d like to do is to put your instruments right in the middle of the orchestra instead of the back of the hall. And to do that you need to use computer simulations, which are quite accurate to access the pure sound."



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