At all began with the Big Bang, scientists have been telling us for years. And so that expansive beginning of the universe must have been very special, one would assume.

Not so, according to two physicists at the University of Chicago.

"We like to say that the big bang is nothing special in the history of our universe," said Sean Carroll, an Assistant Professor in Physics at the University of Chicago.

The big bang could be a normal event in the natural evolution of the universe that will happen repeatedly over incredibly vast time scales as the universe expands, empties out and cools off, say Carroll and graduate student Jennifer Chen.

The duo wondered why time flows in only one direction, and whether the Big Bang -- a theory that has not been proven -- arose from an energy fluctuation in empty space that conforms to the known laws of physics.

Other researchers have long suggested that the universe is cyclic, and that the Big Bang was the beginning of our universe as we know it, but not the beginning of the larger Universe that encompasses everything, including that which we can never see because it's beyond our cosmic bubble.

The question about the arrow of time has vexed physicists for a century because "for the most part the fundamental laws of physics don't distinguish between past and future. They're time-symmetric," Carroll says.

Time is closely related to the concept of entropy, a measure of disorder in the universe. Entropy naturally increases with time, physicist Ludwig Boltzmann suggested a century ago.

As Carroll puts it: "You can turn an egg into an omelet, but not an omelet into an egg."

But the mystery remains as to why entropy was low in the universe to begin with. The difficulty of that question has long bothered scientists, who most often simply leave it as a puzzle to answer in the future. Previous researchers have approached whole shebang the assumption that entropy in the universe is finite. Carroll and Chen take the opposite approach.

"We're postulating that the entropy of the universe is infinite," Chen said in a statement issued yesterday. "It could always increase."

To successfully explain why the universe looks as it does today, both approaches must accommodate a process called inflation, which is an extension of the Big Bang theory. According to inflation, the universe underwent a period of very rapid and massive expansion in a fraction of a second after the Big Bang.

But there's a problem with that scenario. To begin inflation, the universe would have encompassed a microscopically tiny patch in an extremely unlikely configuration, not what scientists would expect from a randomly chosen initial condition.

Carroll and Chen argue that a generic initial condition is actually likely to resemble cold, empty space -- not an obviously favorable starting point for the onset of inflation.

In a universe of finite entropy, some scientists have proposed that a random fluctuation could trigger inflation. This, however, would require the molecules of the universe to fluctuate from a high-entropy state into one of low entropy-a statistical longshot.

"The conditions necessary for inflation are not that easy to start," Carroll said. "There's an argument that it's easier just to have our universe appear from a random fluctuation than to have inflation begin from a random fluctuation."

Carroll and Chen's scenario of infinite entropy is inspired by a finding in 1998 that the universe will expand forever because of a mysterious force scientists have come to call "dark energy." Under these conditions, the natural configuration of the universe is one that is almost empty.

"In our current universe, the entropy is growing and the universe is expanding and becoming emptier," Carroll said.

But even empty space has faint traces of energy that fluctuate on the subatomic scale. As suggested previously by Jaume Garriga of Universitat Autonoma de Barcelona and Alexander Vilenkin of Tufts University, these flucuations can generate their own big bangs in tiny areas of the universe, widely separated in time and space. Carroll and Chen extend this idea in dramatic fashion, suggesting that inflation could start "in reverse" in the distant past of our universe, so that time could appear to run backwards (from our perspective) to observers far in our past.

Regardless of the direction they run in, the new universes created in these big bangs will continue the process of increasing entropy. In this never-ending cycle, the universe never achieves equilibrium. If it did achieve equilibrium, nothing would ever happen. There would be no arrow of time.

"There's no state you can go to that is maximal entropy. You can always increase the entropy more by creating a new universe and allowing it to expand and cool off," Carroll explained.