Astronomers have lengthy been puzzled by two unusual phenomena on the coronary heart of our galaxy. First, the gasoline within the central molecular zone (CMZ), a dense and chaotic area close to the Milky Approach’s core, seems to be ionized (that means it’s electrically charged as a result of it has misplaced electrons) at a surprisingly excessive charge.
Second, telescopes have detected a mysterious glow of gamma rays with an vitality of 511 kilo-electronvolts (keV) (which corresponds to the vitality of an electron at relaxation).
Apparently, such gamma rays are produced when an electron and its antimatter counterpart—all basic charged particles have antimatter variations of themselves which might be close to equivalent, however with reverse cost—the positron, collide and annihilate in a flash of sunshine.
The causes of each results have remained unclear, regardless of a long time of commentary. However in a brand new research, printed in Bodily Evaluation Letters, my colleagues and I present that each could possibly be linked to one of the elusive elements within the universe: darkish matter. Specifically, we suggest {that a} new type of darkish matter, much less huge than the categories astronomers sometimes search for, could possibly be the wrongdoer.
Hidden Course of
The CMZ spans virtually 700 gentle years and comprises a number of the most dense molecular gasoline within the galaxy. Over time, scientists have discovered that this area is unusually ionized, that means the hydrogen molecules there are being break up into charged particles (electrons and nuclei) at a a lot quicker charge than anticipated.
This could possibly be the results of sources akin to cosmic rays and starlight that bombard the gasoline. Nonetheless, these alone don’t appear to have the ability to account for the noticed ranges.
The opposite thriller, the 511-keV emission, was first noticed within the Seventies, however nonetheless has no clearly recognized supply. A number of candidates have been proposed, together with supernovas, huge stars, black holes, and neutron stars. Nonetheless, none absolutely clarify the sample or depth of the emission.
We requested a easy query: May each phenomena be brought on by the identical hidden course of?
Darkish matter makes up round 85 % of the matter within the universe, however it doesn’t emit or take up gentle. Whereas its gravitational results are clear, scientists don’t but know what it’s manufactured from.
One chance, typically ignored, is that darkish matter particles could possibly be very gentle, with plenty just some million electronvolts, far lighter than a proton, and nonetheless play a cosmic function. These gentle darkish matter candidates are usually known as sub-GeV (giga electronvolts) darkish matter particles.
Such darkish matter particles could work together with their antiparticles. In our work, we studied what would occur if these gentle darkish matter particles are available contact with their very own antiparticles within the galactic heart and annihilate one another, producing electrons and positrons.
Within the dense gasoline of the CMZ, these low-energy particles would shortly lose vitality and ionize the encircling hydrogen molecules very effectively by knocking off their electrons. As a result of the area is so dense, the particles wouldn’t journey far. As an alternative, they might deposit most of their vitality regionally, which matches the noticed ionization profile fairly properly.
Utilizing detailed simulations, we discovered that this easy course of, darkish matter particles annihilating into electrons and positrons, can naturally clarify the ionization charges noticed within the CMZ.
Even higher, the required properties of the darkish matter, akin to its mass and interplay power, don’t battle with any identified constraints from the early universe. Darkish matter of this sort seems to be a critical possibility.
The Positron Puzzle
If darkish matter is creating positrons within the CMZ, these particles will finally decelerate and finally annihilate with electrons within the atmosphere, producing gamma-rays at precisely 511-keV vitality. This would supply a direct hyperlink between the ionization and the mysterious glow.
We discovered that whereas darkish matter can clarify the ionization, it could additionally be capable to replicate some quantity of 511-keV radiation as properly. This putting discovering means that the 2 alerts could doubtlessly originate from the identical supply, gentle darkish matter.
The precise brightness of the 511-keV line depends upon a number of components, together with how effectively positrons type certain states with electrons and the place precisely they annihilate although. These particulars are nonetheless unsure.
A New Solution to Check the Invisible
No matter whether or not the 511-keV emission and CMZ ionization share a typical supply, the ionization charge within the CMZ is rising as a useful new commentary to check darkish matter. Specifically, it gives a method to check fashions involving gentle darkish matter particles, that are troublesome to detect utilizing conventional laboratory experiments.
Transfer observations of the Milky Approach might assist check theories of darkish matter. ESO/Y. Beletsky, CC BY-SA
In our research, we confirmed that the anticipated ionization profile from darkish matter is remarkably flat throughout the CMZ. That is vital, as a result of the noticed ionization is certainly unfold comparatively evenly.
Level sources such because the black gap on the heart of the galaxy or cosmic ray sources like supernovas (exploding stars) can’t simply clarify this. However a easily distributed darkish matter halo can.
Our findings counsel that the middle of the Milky Approach could provide new clues concerning the basic nature of darkish matter.
Future telescopes with higher decision will be capable to present extra info on the spatial distribution and relationships between the 511-keV line and the CMZ ionization charge. In the meantime, continued observations of the CMZ could assist rule out, or strengthen, the darkish matter rationalization.
Both method, these unusual alerts from the guts of the galaxy remind us that the universe continues to be filled with surprises. Typically, wanting inward, to the dynamic, glowing heart of our personal galaxy, reveals probably the most surprising hints of what lies past.
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