At first, Sandora and his colleagues regarded their idea as little more than a curiosity, since the hypothetical particle's massive nature meant that there was no way any particle collider on Earth could produce it and prove (or refute) its existence.
But now the researchers have suggested that if these particles exist, signs of their existence might be detectable in the cosmic microwave background radiation, the afterglow of the Big Bang that created the universe about 13.8 billion years ago.
Currently, the prevailing view in cosmology is that moments after the Big Bang, the universe grew gigantically in size. This enormous growth spurt, called inflation, would have smoothed out the cosmos, explaining why it now looks mostly similar in every direction.
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After inflation ended, research suggests that the leftover energy heated the newborn universe during an epoch called "reheating." Sandora and his colleagues suggest that extreme temperatures generated during reheating could have produced large amounts of their superheavy particles, enough to explain dark matter's current gravitational effects on the universe.
However, for this model to work, the heat during reheating would have had to be significantly higher than what is typically assumed in universal models. A hotter reheating would in turn leave a signature in the cosmic microwave background radiation that the next generation of cosmic microwave background experiments could detect. "All this will happen within the next few years hopefully, next decade, max," Sandora said.
If dark matter is made of these superheavy particles, such a discovery would not only shed light on the nature of most of the universe's matter, but also yield insights into the nature of inflation and how it started and stopped - all of which remains highly uncertain, the researchers said.
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For example, if dark matter is made of these superheavy particles, that reveals "that inflation happened at a very high energy, which in turn means that it was able to produce not just fluctuations in the temperature of the early universe, but also in space-time itself, in the form of gravitational waves," Sandora said. "Second, it tells us that the energy of inflation had to decay into matter extremely rapidly, because if it had taken too long, the universe would have cooled to the point where it would not have been able to produce any Planckian interacting dark matter particles at all."
Sandora and his colleagues detailed their findings online March 10 in the journal Physical Review Letters.
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