How To Get Dark Matter For Free

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How To Get Dark Matter For Free

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All terms/names/descriptions/images used on the site may or may not be considered the exclusive property of third parties and are used for informational purposes only and we do not endorse or recommend any link/connection with System Geometry DF2 and DF4 individual intellectual property. The radial velocity difference between DF2 and DF4 is 358 km s

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This large difference in speed is accompanied by large distances of 2.1 ± 0.5 megabytes per second. The geometry shows that the galaxies are moving away from each other. By tracing their positions in time, we confirm that they formed into large mass encounters ≥6 Gyr prior. b, An example of a cluster containing NGC 1052. The velocities are proportional to that galaxy (cz = 1.488 km s).

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). A gas-rich galaxy and satellite NGC 1052 collided about 8 Gyr ago, giving rise to dark remnants (possibly RCP 32 and DF7), DF2 and DF4, and three out of seven other galaxies with no dark matter. Description: Nature (2022). DOI: 10.1038/s41586-022-04665-6

A group of astrophysicists associated with several institutions in the United States, one in Germany and one in Canada has developed a new theory to explain the existence of special galaxies without dark matter. In their paper, published in the journal Nature, the researchers suggested that a collision between two dwarf galaxies could explain why nothing dark has been found in recent years. Eun Jin Shin and Jihoon Kim of Seoul National University published an article in News & Views in the same issue of the journal, describing the work and findings of researchers in this new effort.

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In 2018, scientists discovered a dwarf galaxy that appears to have no dark matter — no gravitational pull. And in 2019, the second team got one in the same general field as the first. Since then, scientists have been trying to explain the strange findings.

In this new effort, the researchers extend the results of other teams to point to evidence of the massive separation of dark matter and normal matter when galaxy clusters collide. Something like this happened, the researchers say, leading to the formation of two or more dwarf galaxies with no visible dark matter. They note that there are several other dwarf galaxies already found near the two galaxies, and they appear to be lined up across the sky — possibly evidence of a collision between dwarf galaxies. They note that the two galaxies studied are far apart, which indicates that they may have the same origin.

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According to the researchers, a collision between the two galaxies can fragment the gas inside, leading to the formation of smaller galaxies, some of which are empty, dark matter. The researchers suggest that those without dark matter were able to do so because dark matter does not interact with itself or with ordinary matter, which means it can easily escape the constant disturbances of space.

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Further information: Pieter van Dokkum et al, Detecting dark matter-free galaxies from colliding lead, Nature (2022). DOI: 10.1038/s41586-022-04665-6

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Citation: New theory of colliding dwarf galaxies could explain galaxies without dark matter (2022, May 19) Retrieved January 4, 2023, from https:///news/2022-05-theory-collision-dwarf-galaxies-dark.html

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Earth’s Atmosphere Could Help Detect Dark Matter Using Radar Systems

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This website uses cookies to help manage, analyze your use of our services, collect information to personalize ads and provide three things. By using our site, you confirm that you have read and understood our Privacy Policy and Terms of Use. Fermilab’s 100-meter-deep chamber — which was built for the neutrino experiment years ago — will be home to a new experiment that will investigate the nature of dark matter and gravitational waves.

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Scientists from the MAGIS-100 collaboration will place groups of atoms under a vacuum, followed by the use of light lasers, to study aspects of quantum physics. The experiment aims to detect the existence of dark matter particles and pave the way for the detection of smaller gravitational waves than the first time they were known.

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According to the laws of quantum physics, atoms can exist in two places at the same time: a superposition of two quantum states. Like a wave circling a rock, an atom can form two wave crests in different locations, and then recombine.

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The 100-meter atomic graduated matter wave sensor – called MAGIS-100 – will be the world’s largest atomic interferometer and will push the limits of how far an atom can travel away from itself. One of the most popular interferometers is LIGO, which is funded by the National Science Foundation. LIGO is used to detect gravitational waves by splitting a light wave in half and sending the light to two objects at the same distance. Any difference in arrival time means that a gravitational wave is passing through space and distorting it.

MAGIS-100 will push the boundaries of quantum physics at macroscopic scales, providing a gateway to dark matter studies and gravitational wave experiments. Image: Stanford University

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“We’re going to use atoms on a person’s scale, and achieve a separation of the person’s height,” explains Fermilab scientist Ronnie Harnik. “This has never happened before.”

The light from the laser travels from one end of the vacuum tube to the other and back again, illuminating clouds of falling atoms to measure the different atomic particles produced by the interaction of a particle of light with a single atom.

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This method, called atomic interferometry, typically uses rubidium atoms. But a new invention by the MAGIS group at Stanford University makes it possible to use strontium atoms instead.

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This change means that when the laser interacts with an electron in a strontium atom, the electron will be energized for a long time – within minutes unlike rubidium nanoseconds. This long life makes strontium an excellent atomic clock and is good for measuring the time it takes laser light to travel the length of an evacuated tube.

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Combined with Fermilab’s experience building accelerators and other large science instruments, these advanced technologies allow this interferometer to be built and expand into new fields.

In an effort to test the principles of quantum mechanics, Erwin Schrödinger created his famous experiment known as Schrödinger’s Cat. Main Idea: If you put a cat in a sealed box with a bottle of toxic poison, then, until the box is opened, the standard definition of quantum mechanics states that the cat can be considered life or death.

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This is a good example of what physicists mean when they say that atoms can exist in two states at the same time, or superpositions.

Atomic clocks rely on this kind of arrangement of individual atoms to achieve the highest possible accuracy.

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MAGIS-100 will push the limit of the distance two different states of an atom can be separated. Currently, the record of 54 cm is held by Stanford University. MAGIS-100 is expected to be able to triple the distance.

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In addition to increasing the distance,

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