Science & Technology
A team of physicists at Institute of Science and Technology Austria haven't done quite that, but they have realised that some collections of molecules behave as if they were "magnetic monpoles," magnets with only one pole. Others have observed similar phenomena, but this one is perhaps most striking in its simplicity. In fact, other teams have probably created the conditions for these properties to manifest all along, but no one went looking for them.
"We analysed expeirments that have been done by other groups. What people do now is put a molecule in superfluid helium. This has been done for 20 years. The main focus was to study the property of molecules," Mikhail Lemeshko from IST Austria told Gizmodo. "They weren't measuring this particular property but were creating monopoles in their experiments by creating something else."
So why should you care if a monopole exists? Well, the most basic equations governing electricity and magnetism are called Maxwell's equations. There are four of them, two for magnetism and two for electricity that look like near mirror images. However, where the electricity equations imply the existence of single electric charges, the magnetic equations do not. People have long assumed that monopoles could possibly exist to make the equations look nicer. Since Maxwell, others have found that monopoles might make some particle physics ideas used to explain our strange Universe look much cleaner.
Lemeshko's team didn't find a single particle, but a quasiparticle that behaved like a single magnetic pole. Quasiparticles occur when many particles, when together, appear to act in a mathematically similar way to single particles moving in simpler ways -- like using the idea of a "hole" to represent "a place where all of the dirt has been removed." In this case, Lemeshko's team calculated the behaviour of a rotating molecule inside a sphere of superfluid helium, called an "angulon."
Your eyes relay signals to the visual centers in the back of your brain. After those signals get processed, they travel along a pathway to another region, the premotor cortex, where the brain plans movements.
Now, imagine that you had a device implanted in your brain that could shortcut the pathway and "inject" information straight into your premotor cortex.
That may sound like an outtake from "The Matrix." But now two neuroscientists at the University of Rochester say they have managed to introduce information directly into the premotor cortex of monkeys. The researchers published the results of the experiment on Thursday in the journal Neuron.
Although the research is preliminary, carried out in just two monkeys, the researchers speculated that further research might lead to brain implants for people with strokes.
If you look at the video of it, you can see it's meant to mimic the real thing as close as possible - even maintaining a pulse.
Since then, seismologists have proposed different theories to explain the existence of this continuous vibration, from atmospheric disturbances to ocean waves moving over the sea floor. They've also measured the vibration using seismometers on land, but had not yet successfully measured it at the sea floor, which could help scientists better quantify the sources of the vibrations.
Now, using seismic instruments on the bottom of the ocean, researchers have successfully quantified Earth's vibrational "hum". A new study published in Geophysical Research Letters, a journal of the American Geophysical Union, determined at the ocean bottom the frequencies at which the Earth naturally vibrates, and confirmed the viability of using ocean instruments to study the hum.
Capturing the hum at the ocean bottom could provide new insights into the source magnitude, according to Martha Deen, a geophysicist at the Paris Institute of Earth Physics in Paris, France and lead author of the new study.
Additionally, the new findings could be used to map the interior of Earth with more detail and accuracy. Including the hum from seismometers on the ocean sea floor can give a better overall picture than using land seismometers alone by increasing data coverage in large uncovered areas, Deen said.
"Earth is constantly in movement, and we wanted to observe these movements because the field could benefit from having more data," she said.
The pictures are taken by Crossover's productivity tool, WorkSmart, and combine with screenshots of their workstations along with other data - including app use and keystrokes - to come up with a "focus score" and an "intensity score" that can be used to assess the value of freelancers.
Today's workplace surveillance software is a digital panopticon that began with email and phone monitoring but now includes keeping track of web-browsing patterns, text messages, screenshots, keystrokes, social media posts, private messaging apps like WhatsApp and even face-to-face interactions with co-workers.
Published in Nature, the study observed two merging galaxies containing a dark-matter 'halo' with a mass of more than 100 billion suns. This is "among the rarest dark-matter haloes that should exist in the Universe at this epoch," the study noted.
One machine-learning method used in AI is reinforcement learning, where agents are rewarded for performing certain actions -- a technique borrowed from behavioral psychology. Applying this technique to AI, engineers use a points system where machines earn points by carrying out the right actions. For instance, a robot may earn one point for correctly stacking a set of boxes and another point for retrieving a box from outside. But if, on a rainy day for example, a human operator interrupts the robot as it heads outside to collect a box, the robot will learn that it is better off staying indoors, stacking boxes and earning as many points as possible. "The challenge isn't to stop the robot, but rather to program it so that the interruption doesn't change its learning process -- and doesn't induce it to optimize its behavior in such a way as to avoid being stopped," says Guerraoui.

Artist concept shows the collision of a large moon-sized planetary body penetrating all the way down to the Earth's core, with some particles ricocheting back into space.
According to NASA, scientists have long believed that after the moon's formation, Earth experienced an extended period of bombardment some 3.8 billion years ago, called 'late accretion'.
During this period, Earth was barraged with moon-sized planetary bodies, also known as planetesimals, that penetrated our planet all the way down to its core. As a result, these collisions embedded extensive amounts of metal and rock-forming minerals into Earth's mantle and crust.
The new research, led by French scientist Albert Jambon and published in the Journal of Archaeological Science, used geochemical analyses to differentiate Earthly and extraterrestrial metals found in a range of Bronze Age artefacts from across the world. By studying the ratios of iron, cobalt and nickel found within the artefacts, researchers created a system to differentiate iron produced through smelting of ore, and 'pre-made' iron of meteoric origin.
For context, meteorites were already recognized as a major source of iron, but the scientific community was still on the fence as to the extent to which meteoric iron contributed to Bronze Age iron artefact construction. Iron weapons crafted during the Bronze Age were extremely rare and prized possessions (kind of like Valyrian steel in the Game of Thrones).

False-colour map of the density of stars with 0.1 < g−r < 0.45 from the SLAMS survey. Density in different magnitude ranges is shown using different colour channels: red 20.5 < r < 23.0, green 17.5 < r < 20.5 and blue 15.0 < r < 17.5. The newly discovered stream is labelled. The dotted line shows the future orbit of the LMC, calculated using Kallivayalil et al. (2013) proper motions, which is roughly aligned with the orientation of the Jet stream. The green/blue colour gradient along the southern edge is due to the varying distance distribution of MW disk stars.
Astronomers are interested in finding new stellar streams in the Milky Way, as they hope that such features could answer some crucial questions about the the galaxy. For instance, stellar streams could help us understand the large-scale mass distribution of the galactic dark matter halo. Moreover, they could confirm whether or not our galaxy contains low-mass dark matter subhalos.













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