Black Holes Might Make Dark Matter Shine


http://earthchangesmedia.com/black-holes-might-make-dark-matter-shine
Dark matter circling the drain of a massive black hole could radiate gamma-rays that might be visible from Earth, according to new research.

Dark matter is five times more plentiful in the universe than regular matter, but it does not emit, reflect or absorb light, making it not just dark but…

Dark matter circling the drain of a massive black hole could radiate gamma-rays that might be visible from Earth, according to new research.

black-hole-eating-material

Dark matter is five times more plentiful in the universe than regular matter, but it does not emit, reflect or absorb light, making it not just dark but entirely transparent. But if dark-matter particles around black holes can produce gamma-rays (high-energy light), such emissions would give scientists a new way to study this mysterious material.

The process responsible for creating the gamma-rays is somewhat counterintuitive, because it seems to defy two common assumptions: that nothing can escape from a black hole and that there’s no such thing as a free lunch.

Improbable escape

Jeremy Schnittman is a theoretical astrophysicist at the NASA Goddard Space Flight Center, and he’s beginning a project to look through data from the Fermi Gamma-ray Space telescope for signs of high-energy light around the edge of a black hole that might have been created by dark matter.

“We’re really just getting started on this part of the problem,” Schnittman said. “As a theoretical astrophysicist, I haven’t done a lot of data analysis in my career, so it’s a little bit of a learning curve for me. But fortunately I’m surrounded by people here at Goddard who are real experts at the Fermi data.”

Schnittman’s search for this dark-matter signal began with a computer program that he has been developing for about 10 years. It models in 3D the paths of particles as they zip through space near a black hole, while some of them get close enough to orbit around the black hole or fall in.

Just over a year ago, he decided to adjust the program to model dark-matter particles. The resulting video shows how the subatomic bits get caught up in the gravitational pull of the black hole and swirl around it in a region called the ergosphere (where all particles must orbit in the direction of the black hole’s spin). Some of the particles collide and destroy each other (also known as annihilation), and this produces a pair of gamma-rays.

These particles of light might normally fall into the black hole, helpless against its gravitational pull, were it not for something called the Penrose process.

In 1971, astrophysicist Roger Penrose showed that if two photons are created very close to a black hole, it’s possible for one of them to escape, while the other falls in. This flies counter to the commonly held idea that nothing can escape from a black hole, or at least nothing that goes past the “event horizon” — the point at which the gravitational pull is so strong that nothing, not even light, can ever exert enough force to get away.

According to the Penrose principle, the particles are not created beyond this point of no return, but under normal circumstances, it’s unlikely that either particle would have any means of getting away from the black hole. So the Penrose process still changes the fate of at least one particle, giving it an escape route.

In 2009, a group of researchers showed that the Penrose process could be applied to dark-matter particles that annihilate and form two gamma-rays. If dark-matter particles are annihilating near the surface of a black hole, telescopes on Earth could detect the escaping gamma-rays.

Schnittman’s work using the 3D computer model has shown many more paths that the particles can take, including some that are more likely to produce gamma-rays that can escape the black hole, and with even higher energies than had been previously predicted. A brief description of those results was published in the journal Physical Review Letters last December, and a longer description of the work has been accepted to the Astrophysical Journal.

With those results, Schnittman and his colleagues are now looking for this signal, although they said they expect it to be very dim compared to many other gamma-ray sources. The researchers are creating a list of target galaxies that have few gamma-ray sources and very massive black holes.

“The bigger the black hole, the bigger the signal,” Schnittman said. “It scales in a way that as your black hole [mass] goes up by a factor of 10, the expected signal goes way up, by something like a factor of 1,000.

“The first pass at observing this effect is almost certainly not going to yield an actual detection. But it will provide probably the strongest upper limit on this type of process that has ever been seen before — the idea of high-energy dark-matter particle reactions. Even that is progress.”

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About Earth Changes Media w/ Mitch Battros

Mitch Battros is a scientific journalist who is highly respected in both the scientific and spiritual communities due to his unique ability to bridge the gap between modern science and ancient text. Founded in 1995 – Earth Changes TV was born with Battros as its creator and chief editor for his syndicated television show. In 2003, he switched to a weekly radio show as Earth Changes Media. ECM quickly found its way in becoming a top source for news and discoveries in the scientific fields of astrophysics, space weather, earth science, and ancient text. Seeing the need to venture beyond the Sun-Earth connection, in 2016 Battros advanced his studies which incorporates our galaxy Milky Way - and its seemingly rhythmic cycles directly connected to our Solar System, Sun, and Earth driven by the source of charged particles such as galactic cosmic rays, gamma rays, and solar rays. Now, "Science Of Cycles" is the vehicle which brings the latest cutting-edge discoveries confirming his published Equation.
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