Pattern of radio waves on the sky caused by the combination of radiation from the first stars and the effect of dark matter. Blue regions are those where the dark matter cooled down the ordinary matter most strongly. .
(photo credit: PROF. RENNAN BARKANA)
While attempting to detect the earliest stars in the universe through radio wave signals, a team of astronomers stumbled upon “dark matter” – the most mysterious building block of outer space.
The discovery by the team, led by Prof. Judd Bowman of Arizona State University, that the signals implicate dark matter – just published in the journal Nature – was based on an earlier Nature paper published by a Tel Aviv University scientist.
TAU Prof. Rennan Barkana suggested that the signal is proof of interactions between normal matter and dark matter in the early universe. He said the discovery offers the “first direct proof that dark matter exists and that it is composed of low-mass particles.”
The signal, recorded by a novel radio telescope in Western Australia called EDGES (the Experiment to Detect the Global EoR (Epoch of Reionization) Signature), dates to 180 million years after the Big Bang.
“Dark matter is the key to unlocking the mystery of what the universe is made of,” said Barkana, head of the astrophysics department at TAU’s School of Physics and Astronomy.
“We know quite a bit about the chemical elements that make up the Earth, the sun and other stars, but most of the matter in the universe is invisible and known as ‘dark matter.’ The existence of dark matter is inferred from its strong gravity, but we have no idea what kind of substance it is. Hence, dark matter remains one of the greatest mysteries in physics,” he said.
“To solve it, we must travel back in time. Astronomers can see back in time, since it takes light time to reach us. We see the sun as it was eight minutes ago, while the immensely distant first stars in the universe appear to us on earth as they were billions of years in the past.”
Bowman and colleagues reported the detection of a radio wave signal at a frequency of 78 megahertz. The width of the observed profile is largely consistent with expectations, but they also found it had a larger amplitude (corresponding to deeper absorption) than predicted, indicating that the primordial gas was colder than expected. They suggested that the gas cooled through the interaction of hydrogen with cold, dark matter.
“I realized that this surprising signal indicates the presence of two actors: the first stars, and dark matter,” he said. “The first stars in the universe turned on the radio signal, while the dark matter collided with the ordinary matter and cooled it down. Extra-cold material naturally explains the strong radio signal.”
Physicists expected that any such dark matter particles would be heavy, but the discovery indicates low-mass particles. Based on the radio signal, Barkana maintained that the dark-matter particle is no heavier than several proton masses. “This insight alone has the potential to reorient the search for dark matter.”
Once stars formed in the early universe, their light was predicted to have penetrated the primordial hydrogen gas, altering its internal structure.
This would cause the hydrogen gas to absorb photons from the cosmic microwave background, at the specific wavelength of 21 cm., imprinting a signature in the radio spectrum that should be observable today at radio frequencies below 200 megahertz. The observation matches this prediction except for the unexpected depth of the absorption.
The astrophysicist predicts that the dark matter produced a very specific pattern of radio waves that can be detected with a large array of radio antennas. One such array is the SKA (Square Kilometer Array), the largest radio telescope in the world, now under construction with receiving stations planned in Australia, New Zealand and South Africa.
“Such an observation with the SKA would confirm that the first stars indeed revealed dark matter,” Barkana concluded.
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