Scientists have advanced in discovering how to use ripples in space-time
known as gravitational waves to peer back to the beginning of everything we
know. The researchers say they can better understand the state of the cosmos
shortly after the Big Bang by learning how these ripples in the fabric of
the universe flow through planets and the gas between the galaxies.
"We can't see the early universe directly, but maybe we can see it
indirectly if we look at how gravitational waves from that time have
affected matter and radiation that we can observe today," said Deepen Garg,
lead author of a paper reporting the results in the Journal of Cosmology and
Astroparticle Physics. Garg is a graduate student in the Princeton Program
in Plasma Physics, which is based at the U.S. Department of Energy's (DOE)
Princeton Plasma Physics Laboratory (PPPL).
Garg and his advisor Ilya Dodin, who is affiliated with both Princeton
University and PPPL, adapted this technique from their research into fusion
energy, the process powering the sun and stars that scientists are
developing to create electricity on Earth without emitting greenhouse gases
or producing long-lived radioactive waste. Fusion scientists calculate how
electromagnetic waves move through plasma, the soup of electrons and atomic
nuclei that fuels fusion facilities known as tokamaks and stellarators.
It turns out that this process resembles the movement of gravitational waves
through matter. "We basically put plasma wave machinery to work on a
gravitational wave problem," Garg said.
Gravitational waves, first predicted by Albert Einstein in 1916 as a
consequence of his theory of relativity, are disturbances in space-time
caused by the movement of very dense objects. They travel at the speed of
light and were first detected in 2015 by the Laser Interferometer
Gravitational Wave Observatory (LIGO) through detectors in Washington State
and Louisiana.
Garg and Dodin created formulas that could theoretically lead gravitational
waves to reveal hidden properties about celestial bodies, like stars that
are many light years away. As the waves flow through matter, they create
light whose characteristics depend on the matter's density.
A physicist could analyze that light and discover properties about a star
millions of light years away. This technique could also lead to discoveries
about the smashing together of neutron stars and black holes, ultra-dense
remnants of star deaths. They could even potentially reveal information
about what was happening during the Big Bang and the early moments of our
universe.
The research began without any sense of how important it might become. "I
thought this would be a small, six-month project for a graduate student that
would involve solving something simple," Dodin said. "But once we started
digging deeper into the topic, we realized that very little was understood
about the problem and we could do some very basic theory work here."
The scientists now plan to use the technique to analyze data in the near
future. "We have some formulas now, but getting meaningful results will take
more work," Garg said.
Reference:
Deepen Garg et al, Gravitational wave modes in matter, Journal of Cosmology
and Astroparticle Physics (2022).
DOI: 10.1088/1475-7516/2022/08/017
Tags:
Physics