Mysterious phenomenon at the heart of the Milky Way could point to new dark matter suspect. ‘We may have been overlooking its subtle chemical effects on the cosmos.’
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A clarification of the dark dark matter in the heart of a spiral galaxy. | Credit: Robert Lea (created with Kanfa)
The strange events seen in the heart of the Milky Way can be evidence of a new suspected pistol. If this is the case, scientists may miss the exact effect of Dark materialThe most mysterious “things” in the universe, on cosmic chemistry.
This proposal recently Dark material candidate It will not only be lighter than the current virtual suspects, but it will also be a self -teacher. This means that when two parts of the dark matter meet, they destroy each other and create a negative charge Electron And its positive rewards positively, a Bozetron.
This process and flooding electrons and mediators will provide the energy needed to strip electrons away from neutral atoms, a process called ionization, in thick gas in the middle of the Milky Way. This can explain the reason for the presence of a lot of ionized gas in the central region called Central Molecular Zone (CMZ).
even if Dark material extermination Rarely, it makes sense to occur frequently in the heart of galaxies where the bloc is believed.
We suggest that the dark matter is lighter than a Proton [the particles found in the nuclei of atoms] It can be responsible for an unusual effect in a center milky way“Team leader and post -doctoral research fellow at the King’s College of London Shiham Balaji told Space.com.” Unlike most candidates for the dark matter, which are often studied through their gravitational effects, this form of dark matter may reveal by ionization of gas, which mainly roots of atoms in CMZ.
“This will happen if the dark matter molecules are whitening Electron pairs-BosterronWhich then interacts with the surrounding gas. “
Dark matter chemistry
The dark matter is believed to represent about 85 % of “things” in the universe, but although they are everywhere, scientists cannot “see” as they do with many normal materials. This is because the dark matter does not interact with light, or if it happens, it does so weakly and rarely noticed.
This tells scientists of dark materials that cannot consist of baroni molecules such as electrons, protons and neutrons that make up the atoms that form Stars, Planets, satellites and all that we see around us on a daily basis.
The only reason why scientists look at the existence of the dark matter at all is that it interacts with it attractiveness, This effect affects light and “normal” material.
The graph shows the percentage of the dark matter of the “daily” material that consists of stars, planets and even cats (perhaps). | Credit: Robert Lea (created with Kanfa)
This scholars have pushed to look beyond the so -called “The standard model of particle physicsTo search for molecules can explain the dark matter.
These particles differ in the mass, which is contained in the electronvots (EV), and in the properties. It is suggested that some, such a new suspect, can be subjective.
The current “major suspects” of the dark matter Axis Thought -like molecules, which come in a wide range of masses. However, she was excluded by Al -Jaji and her colleagues often two axes and ax -like molecules as the dark guilty linked to the gas ionization in CMZ.
“Most AXION models do not predict a great extermination in electron pairs-bosterone the way the proposed dark matter works,” said Balaji. “Our proposed dark topic is Sub-GEV (billion volts) in the block and self-panels to electrons and mediators.”
“This distinguishes it because it directly affects The middle of the starsCreate a signature in additional ionization form, which is not expected to do the axes usually. “
Dark material: It is the worst enemy
In overcrowded CMZ heavily, the largely created biotritons can not travel or escape before interacting with nearby hydrogen molecules and stripping their electronics. This makes this process particularly effective in this central area.
“The biggest problem that this model helps to solve is to increase the ionization of CMZ,” said Palaji. “CosmicIt does not seem to be the usual gas perpetrators, strong enough to explain the high levels of ionization that we notice. “
Cosmic rays are charged with molecules that move near Light speedBut according to this team, it appears that the CMZ ionization signal indicates a slower moving source lighter than many other candidates for dark materials.
Also, if the cosmic rays are ionized gas in CMZ, then there should be an attached emission Gamma raysWhich are high -energy molecules of light. However, this emission is missing from CMZ studies.
“If the dark matter is responsible for CMZ ionization, then this means that we discover the dark matter not through its vision, but by monitoring its accurate chemical effect on the gas in our galaxy,” said Palaji.
However, there is a faded gamma glow that is not interpreted from the center of the galaxy, which may also be associated with clutches and lying.
“If we find a direct relationship between ionization and the emission of gamma rays, it may enhance the issue of the dark matter,” said Palaji. “There is some link between these two signs, but we still need more data at this stage to say anything stronger.”
Galaxy cores, such as the Milky Way Center in this image, is full of gas and debris, which makes it very difficult to get any images directly for the stars or black holes there. | Credit
In addition, the annihilation model for dark matter can also explain the distinctive light emissions of CMZ resulting from positively charged biotrocrons and the negatively charged electrons that are shattered and gathered in a state called BiotrocroniumWho is quickly degraded X -ray, Light with a slightly lower energy than gamma rays.
“The numbers are much better than what we expected. Often, the interpretations of the dark matter face problems because they predict the signals that telescopes should have already seen,” said Balaji. “But in this case, the ionization rate produced by the sub-EGEV is perfectly fits within known restrictions, without contradicting the current gamma rays and Cosmic microwave background (CMB) Notes. “
The researcher added that the initial meeting with X -ray emission is very interesting.
“This is a rare and exciting situation in the research of the dark matter,” he added.
They are the first days of this suspect in this dark article
Of course, this new candidate for the dark matter is at the beginning of his theoretical life; It does not even contain the name Snappe like WIMP (a huge particle of weak interaction) or muscle masculinity (a huge compact aura object) so far!
For comparison, the axes have been present since the first theory by theoretical physicists Frank Weltikk and Stephen Winberg In 1978.
This means that there are many theories to be done before this candidate takes his place between the axes, cheated, technicians, primitive black holes, and the rest in The dark matter is suspected.
“We need more accurate measurements of the ionization in CMZ, if we can plan more accurately, we can see if it follows the expected distribution of the dark matter,” said Palaji. “If we exclude other potential sources of ionization, the darker matter becomes more convincing.”
Related stories:
– The dark matter may live in thick fog around the star bodies
– The dark matter can be discovered in the end through self -trivialities
– Something “suspicious” happens with the aura of the Milky Way issue
An additional evidence of a relationship between the extermination in the dark matter and the strange emissions of CMZ can be delivered by the upcoming NASA Kossi (Compvent Spectrometer and Imager) Telescope Gamma-Ray Space, which was launched in 2027.
Cosi must provide better data regarding the Mev (1 million volts) of astronomical physics, which can help confirm or exclude this dark interpretation.
Whatever the case, this research was presented a A new way to consider the effect of the dark matter.
Balji concluded that “the dark matter is still one of the largest puzzles in physics, and this work indicates that we may exceed its accurate chemical effects on the universe.” “If this theory continues, it may open a completely new way to study the dark matter, not only through its attractiveness, but through the way our galaxy is formed.”
The team’s research was published on Monday (10 March) in the physical magazine’s speeches for the review.
