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Cosmic inflation: Leak suggests BICEP detection was wrong Cosmic inflation: New study says BICEP detection was wrong
(about 9 hours later)
Scientists who claimed last year to have found a pattern in the sky left by the super-rapid expansion of space just fractions of a second after the Big Bang were mistaken.Scientists who claimed last year to have found a pattern in the sky left by the super-rapid expansion of space just fractions of a second after the Big Bang were mistaken.
The signal had been confounded by light emission from dust in our own galaxy.The signal had been confounded by light emission from dust in our own galaxy.
This appears to be the conclusion of a new study involving the US-led BICEP2 team itself. This is the conclusion of a new study involving the US-led BICEP2 team itself.
A summary of the paper was briefly posted on an official French website, but then pulled. A paper describing the findings has been submitted to the peer-reviewed journal Physical Review Letters.
The information was not supposed to have been released until early next week, when the actual paper itself would have been put up on the Arxiv pre-print server. Its ultimate peer-reviewed destination was likely to be the journal Physical Review Letters where previous BICEP papers have been published. A summary was briefly posted on an official French website on Friday before being pulled. A press release was then issued later in the day, although the paper itself is still not in the public domain at the time of writing.
A determination that BICEP2 was mistaken in its observations is not a major surprise.A determination that BICEP2 was mistaken in its observations is not a major surprise.
The team itself had already made known its reduced confidence in the detection. But the new paper is significant because it is co-authored by scientists from the Planck Consortium - researchers operating a European Space Agency satellite that had also been seeking the same expansion pattern. The team itself had already made known its reduced confidence in the detection. But the new paper is significant because it is co-authored by "rival" scientists. These are the Planck Consortium of researchers, who were operating a European Space Agency (Esa) satellite that had also been seeking the same expansion pattern.
It was on the website of one of that satellite's instrument teams - its High Frequency Instrument (HFI) - that the outcome of the joint assessment was briefly leaked. It was on the website of one of this satellite's instrument teams - its High Frequency Instrument (HFI) - that the outcome of the joint assessment was briefly leaked on Friday.
The BBC understands that some of this information was inaccurate, but that its broad thrust was correct. All the unified effort can do, according to the Esa press release, is put an upper limit on the likely size of the real signal.
All the joint effort could do - according to the removed summary - was put an upper limit on the likely size of the signal. This will be important for those future experiments that endeavour to make what would still be one of the great discoveries in modern science.
This will be important for those future experiments that endeavour to make what would be one of the great discoveries in science.
Issues of confusionIssues of confusion
BICEP2 used an extremely sensitive detector in an Antarctic telescope to study light coming to Earth from the very edge of the observable Universe - the famous Cosmic Microwave Background (CMB) radiation. BICEP2 used extremely sensitive detectors in an Antarctic telescope to study light coming to Earth from the very edge of the observable Universe - the famous Cosmic Microwave Background (CMB) radiation.
It was looking for swirls in the polarisation of the light.It was looking for swirls in the polarisation of the light.
This pattern in the CMB's directional quality is a fundamental prediction of inflation - the idea that there was an ultra-rapid expansion of space just fractions of a second after the Big Bang. This pattern in the CMB's directional quality is a fundamental prediction of "inflation" - the idea that there was an ultra-rapid expansion of space just fractions of a second after the Big Bang.
The twists, known as B-modes, are an imprint of the waves of gravitational energy that would have accompanied the violent growth spurt that occurred almost 14 billion years ago. The twists, known as B-modes, are an imprint of the waves of gravitational energy that would have accompanied this violent growth spurt almost 14 billion years ago.
But this primordial signal - if it exists - is expected to be extremely delicate, and a number of independent scientists expressed doubts about the American team's finding as soon as it was announced in March 2014. But the primordial signal - if it exists - is expected to be extremely delicate, and a number of independent scientists expressed doubts about the American team's findings as soon as they were announced at a press conference in March 2014.
At issue are a couple of complications. One is an effect where a "false" B-mode signal can be produced on the sky by the CMB passing through massive objects, such as huge galaxies. This so-called lensing effect must be subtracted.At issue are a couple of complications. One is an effect where a "false" B-mode signal can be produced on the sky by the CMB passing through massive objects, such as huge galaxies. This so-called lensing effect must be subtracted.
But the second and most significant issue is the confusing role played by foreground dust in our galaxy.But the second and most significant issue is the confusing role played by foreground dust in our galaxy.
Nearby spinning grains can produce an identical polarisation pattern, and this effect must also be removed to get an unambiguous view of the primordial, background signal. Nearby spinning grains can produce an identical polarisation pattern, and this effect must also be removed to get an unambiguous view of the primordial background signal.
Bright dust
The BICEP2 team used every piece of dust information it could source on the part of the sky it was observing above Antarctica.The BICEP2 team used every piece of dust information it could source on the part of the sky it was observing above Antarctica.
What it lacked, however, was access to the dust data being compiled by the Planck space telescope, which had mapped the microwave sky at many more frequencies than BICEP2.What it lacked, however, was access to the dust data being compiled by the Planck space telescope, which had mapped the microwave sky at many more frequencies than BICEP2.
This allowed Planck to more easily characterise the dust and discern its confounding effects. The Planck consortium agreed to start working with BICEP2 back in the summer. This allowed Planck to more easily characterise the dust and discern its confounding effects. The Planck Consortium agreed to start working with BICEP2 back in the summer. The European group incorporated its high frequency information - where dust shines most brightly - and the US team added additional data collected by its next-generation instrument in Antarctica called the Keck Array.
The results of the joint assessment leaked by the French Planck HFI website would suggest that whatever signal BICEP2 detected, it cannot be separated out at any significant level from these other spoiling effects. However, the results of the joint assessment would suggest that whatever signal BICEP2 detected, it cannot be separated at any significant level from the spoiling effects. In other words, the original observations are equally compatible with there being no primordial gravitational waves.
"This joint work has shown that the detection of primordial B-modes is no longer robust once the emission from galactic dust is removed," Jean-Loup Puget, principal investigator of Panck's HFI instrument, said in the Esa statement.
"So, unfortunately, we have not been able to confirm that the signal is an imprint of cosmic inflation."
Ongoing quest
This is not the end of the matter. Other experiments are still chasing the B-mode signal using a variety of detector technologies and telescopes.
These groups will have learnt from the BICEP experience and they will all devour Planck's latest batch of relevant data products when they start to be published next week.
Like any field of scientific endeavour, advances are continually being made.
One of the ironies of this story is that BICEP itself may now actually be best paced to make the ultimate detection of the cosmic inflation pattern.
Although the past year, with its quashed claim, will have been painful, the team will have new insights.
What is more, it can still boast world-leading scientists among its members, and detectors that are universally acknowledged to be top-notch.
Jonathan.Amos-INTERNET@bbc.co.uk and follow me on Twitter: @BBCAmosJonathan.Amos-INTERNET@bbc.co.uk and follow me on Twitter: @BBCAmos