Does Small Fraction of Dark Matter Particles Carry Electric Mini-Charge?

A duo of astrophysicists is proposing a new model for the invisible material that makes up most of the Universe: it’s possible that a small fraction (less than 1%) of dark matter particles may have a tiny electrical charge — a million times smaller than the charge on the electron.

This artist’s impression shows the evolution of the Universe beginning with the Big Bang on the left followed by the appearance of the Cosmic Microwave Background. The formation of the first stars ends the cosmic dark ages, followed by the formation of galaxies. Image credit: M. Weiss / Harvard-Smithsonian Center for Astrophysics.

This artist’s impression shows the evolution of the Universe beginning with the Big Bang on the left followed by the appearance of the Cosmic Microwave Background. The formation of the first stars ends the cosmic dark ages, followed by the formation of galaxies. Image credit: M. Weiss / Harvard-Smithsonian Center for Astrophysics.

“You’ve heard of electric cars and e-books, but now we are talking about electric dark matter. However, this electric charge is on the very smallest of scales,” said lead author Dr. Julian Munoz, of Harvard University.

Dr. Munoz and his co-author, Professor Avi Loeb of the Harvard-Smithsonian Center for Astrophysics, explore the possibility that charged dark matter particles interact with normal matter by the electromagnetic force.

Their work, published in the journal Nature, dovetails with recently results from the Experiment to Detect the Global Epoch of Reionization Signature (EDGES) Collaboration.

Earlier this year, EDGES scientists said they had detected the radio signature from the first generation of stars, and possible evidence for interaction between dark matter and normal matter.

Meanwhile, Dr. Munoz and Professor Loeb were already looking at the theoretical basis underlying it.

“We’re able to tell a fundamental physics story with our research no matter how you interpret the EDGES result. The nature of dark matter is one of the biggest mysteries in science and we need to use any related new data to tackle it,” Professor Loeb said.

The story begins with the first stars, which emitted UV light.

According to the commonly accepted scenario, this UV light interacted with cold hydrogen atoms in gas lying between the stars and enabled them to absorb the Cosmic Microwave Background (CMB) radiation, the leftover radiation from the Big Bang.

This absorption should have led to a drop in intensity of the CMB during this period, which occurs less than 200 million years after the Big Bang.

The EDGES team claimed to detect evidence for this absorption of CMB light, though this has yet to be independently verified by other scientists. However, the temperature of the hydrogen gas in the EDGES data is about half of the expected value.

“If EDGES has detected cooler than expected hydrogen gas during this period, what could explain it? One possibility is that hydrogen was cooled by the dark matter,” Dr. Munoz said.

At the time when CMB radiation is being absorbed, the any free electrons or protons associated with ordinary matter would have been moving at their slowest possible speeds (since later on they were heated by X-rays from the first black holes).

Scattering of charged particles is most effective at low speeds. Therefore, any interactions between normal matter and dark matter during this time would have been the strongest if some of the dark matter particles are charged.

This interaction would cause the hydrogen gas to cool because the dark matter is cold, potentially leaving an observational signature like that claimed by the EDGES project.

“We are constraining the possibility that dark matter particles carry a tiny electrical charge — equal to one millionth that of an electron — through measurable signals from the cosmic dawn. Such tiny charges are impossible to observe even with the largest particle accelerators,” Professor Loeb said.

Only small amounts of dark matter with weak electrical charge can both explain the EDGES data and avoid disagreement with other observations.

If most of the dark matter is charged, then these particles would have been deflected away from regions close to the disk of our Mily Way Galaxy, and prevented from reentering. This conflicts with observations showing that large amounts of dark matter are located close to the disk of the Milky Way.

Astrophysicists know from observations of the CMB that protons and electrons combined in the early Universe to form neutral atoms.

Only a small fraction of these charged particles, about one in a few thousand, remained free.

Dr. Munoz and Professor Loeb are considering the possibility that dark matter may have acted in a similar way.

The data from EDGES, and similar experiments, might be the only way to detect the few remaining charged particles, as most of the dark matter would be neutral.

_____

Julian B. Muñoz Abraham Loeb. 2018. A small amount of mini-charged dark matter could cool the baryons in the early Universe. Nature 557: 684-686; doi: 10.1038/s41586-018-0151-x

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