Scientists will have to wait a while longer to find out what kicked off the Big Bang.
Last spring, a team of astronomers who go by the name of BICEP announced they had detected ripples in space-time, or gravitational waves, reverberating from the first trillionth of a trillionth of a trillionth of a second of time long-sought evidence that the expansion of the universe had started out with a giant whoosh called inflation.
The discovery was heralded as potentially the greatest of the new century, but after months of spirited debate, the group conceded the result could have been caused by interstellar dust, a notion buttressed by subsequent measurements by the European Space Agency’s Planck satellite that showed the part of the sky BICEP examined was in fact dusty.
Now a new analysis, undertaken jointly by the BICEP group and the Planck group, has confirmed that the BICEP signal was mostly, if not all, stardust, and that there is no convincing evidence of the gravitational waves. No evidence of inflation.
This analysis shows that the amount of gravitational waves can probably be no more than about half the observed signal, Clem Pryke of the University of Minnesota said on Friday in an interview.
“We can’t say with any certainty whether any gravity wave signals remain,” Mr. Pryke added. “Obviously, we are not exactly thrilled, but we are scientists and our job is to try and uncover the truth. In the scientific process, the truth will emerge.”
When the galactic dust is correctly subtracted, the scientists said, there was indeed a small excess signal — a glimmer of hope for inflation fans — but it was too small to tell whether it was due to gravitational waves or just experimental noise.
The BICEP/Planck analysis was led by Mr. Pryke, one of the four BICEP principal investigators. Brendan Crill, of the California Institute of Technology and a member of Planck, acted as a liaison between the groups. They had planned to post their paper on Monday, but the data was posted early, apparently by accident. It was soon taken down, but not before it triggered an outburst of Twitter messages and hasty news releases.
A paper is to be posted to the BICEP website and has been submitted to the Physical Review Letters .
But it will be far from the final word. A flotilla of experiments devoted to the cause are under way, studying a thin haze of microwaves, known as cosmic background radiation, left from the Big Bang, when the cosmos was about 380,000 years old. Among them is a sister experiment to BICEP called Spider, led by Bill Jones of Princeton and involving a balloon-borne telescope that just completed a trip around Antarctica, as well as BICEP’s own Keck Array and the recently installed BICEP3.
At stake is an idea that has galvanised cosmologists since Alan Guth of the Massachusetts Institute of Technology invented it in 1979. Inflation theory holds that the universe underwent a violent and brief surge of expansion in the earliest moments, driven by a mysterious force field that exerted negative gravity. It would explain such things as why the universe looks so uniform and where galaxies come from quantum dents in the inflating cosmos.
Such an explosion would have left faint corkscrew swirls, known technically as B-modes, in the pattern of polarisation of the microwaves. So, however, does interstellar dust.
The BICEP group — its name is an acronym for Background Imaging of Cosmic Extragalactic Polarization — is led by John M. Kovac of the Harvard-Smithsonian Center for Astrophysics; Jamie Bock of Caltech; Pryke; and Chao-Lin Kuo of Stanford. They have deployed a series of radio telescopes at the South Pole in search of the swirl pattern.
Their second scope, BICEP2, detected a signal whose strength was in the sweet spot for some of the most popular models of inflation, leading to a sensational news conference attended by Guth and Andrei Linde, two of the founding fathers of inflation.
But that was before critics raised the dust question. — New York Times News Service
