June 5, 2013
Credit: Karin Lind, Davide De Martin.
Communications Officer, Advancement
W.M. Keck Observatory
Kamuela, Hawaii – An international team of scientists using the most powerful telescope on Earth has discovered the moments just after the Big Bang happened more like the theory predicts, eliminating a significant discrepancy that troubled physicists for two decades. The discovery will be published in the international journal Astronomy & Astrophysics on June 6.
One of the most important problems in physics and astronomy was the inconsistency between the lithium isotopes previously observed in the oldest stars in our galaxy, which suggested levels about two hundred times more Li-6 and about three to five time less Li-7 than Big Bang nucleosynthesis predicts. This serious problem in our understanding of the early Universe has invoked exotic physics and fruitless searches for pre-galactic production sources to reconcile the differences.
The team, led by Karin Lind of the University of Cambridge, has proven the decades-old inventory relied on lower quality observational data with analysis using several simplifications that resulted in spurious detections of lithium isotopes.
Using observations of ancient stars with W. M. Keck Observatory's 10-meter telescope and state-of-the-art models of their atmospheres has shown that there is no conflict between their lithium-6 and lithium-7 content and predictions of the standard theory of Big Bang nucleosynthesis, restoring thus the order in our theory of the early universe.
The discovery that the universe was expanding by Edwin Hubble in the 1920s and subsequent observations suggest the universe began about 13.8 billion years ago in an event called the Big Bang. The fundamental observations that corroborate the Big Bang are the cosmic microwave radiation and the chemical abundances of the light elements described in the Big Bang nucleosynthesis theory.
“The predictions of Big Bang nucleosynthesis have been one of the main successes of the standard Big Bang model,” said lead author Lind. “Our findings remove much of the stark tension between 6Li and 7Li abundances in stars and standard BBN, even opening up the door for a full reconciliation. This further consolidates a model resting heavily on the pillars of the cosmic microwave background and the expanding Universe.”
Taking accurate measurements of lithium-6 and lithium-7 in old stars is extremely challenging, both from a theoretical and observational perspective, in particular for lithium-6, because being the less abundant isotope of lithium, its signature is very weak. The required data can only be obtained with the largest telescopes on Earth such as the Keck Observatory on the summit of Mauna Kea, Hawaii equipped with the powerful High Resolution Echelle Spectrometer (HIRES) spectrograph to disperse the stellar light into its constituent colors and absorption features.
“Back in 2004 HIRES was upgraded with CCDs having smaller pixels, allowing to see finer details in the spectrum,” University of Sao Paulo’s Jorge Meléndez said. “A high spectral resolution provided by HIRES is needed to study with exquisite detail the line profile and to estimate the presence of Lithium-6. The large light-collecting power of Keck Observatory allowed us to observe stars with a more 'pristine' composition than any previous study.”
Even with the mighty Keck I telescope, a single star must be observed for several hours to gather enough photons for a detailed observation. The modeling of such data is also very demanding, as different processes in the atmospheres of such metal-deficient old stars may mimic the presence of lithium-6. The data must be analyzed using sophisticated model atmospheres created by the team in 3D and included complex calculations that run for weeks on powerful super computers.
"We simultaneously relaxed two key physical assumptions in the modeling of stellar atmospheres; one-dimensional hydrostatic and local thermodynamic equilibrium,” Lind said. “Using more sophisticated physics and powerful super-computers, we managed to remove the systematic biases that plague traditional modeling and have previously led to false identifications of the 6Li/7Li isotopic signature.”
The synergy of high quality Keck observations and detailed theoretical modeling has solved cosmological problems that haunted particle physicists and astrophysicists during the last two decades.
“Understanding the birth of our Universe is pivotal for the understanding of the later formation of all its constituents, ourselves included,” Lind said. “The Big Bang model sets the initial conditions for structure formation and explains our presence in an expanding universe dominated by dark matter and energy.”
The Big Bang theory now rests on more firm footing.
The international team of astronomers includes Karin Lind (formerly at the Max Planck Institute for Astrophysics [MPA], Germany, and now in Cambridge), Jorge Meléndez (Department of Astronomy, University of Sao Paulo, Brazil), Martin Asplund, Remo Collet (both at the Australian National University, Australia) and Zazralt Magic (MPA). Reference Lind K., Melendez J., Asplund M., Collet R. & Magic Z., The lithium isotopic ratio in very metal-poor stars, Astronomy & Astrophysics.
The W. M. Keck Observatory operates the largest, most scientifically productive telescopes on Earth. The two, 10-meter optical/infrared telescopes on the summit of Mauna Kea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectroscopy and a world-leading laser guide star adaptive optics system. The Observatory is a private 501(c) 3 non-profit organization and a scientific partnership of the California Institute of Technology, the University of California and NASA.