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When transferring multiple 100+ MB files between computers or devices, I typically use:

  • USB memory stick, SD card, or similar
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  • The "cloud" (Dropbox, Cloud, Google Drive, etc.)
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[ Results | Polls ]
Comments:164 | Votes:266

posted by janrinok on Wednesday October 08, @09:58PM   Printer-friendly
from the sky-not-falling-department dept.

There have been a lot of recent stories about Google restricting sideloading to apps from developers who have registered with Google. Google has issued the very important clarification that adb will still be able to used to sideload unverified apps: https://support.google.com/android-developer-console/answer/16561738

So, if you own your phone, you can still install whatever you want on it. You just might have to install adb and enable the Developer Options menu first.


Original Submission

posted by janrinok on Wednesday October 08, @05:14PM   Printer-friendly

https://phys.org/news/2025-10-ultra-thin-sodium-alternative-gold.html

From solar panels to next-generation medical devices, many emerging technologies rely on materials that can manipulate light with extreme precision. These materials—called plasmonic materials—are typically made from expensive metals like gold or silver. But what if a cheaper, more abundant metal could do the job just as well or better?

That's the question a team of researchers set out to explore. The challenge? While sodium is abundant and lightweight, it's also notoriously unstable and difficult to work with in the presence of air or moisture—two unavoidable parts of real-world conditions. Until now, this has kept it off the table for practical optical applications.

Researchers from Yale University, Oakland University, and Cornell University have teamed up to change that. By developing a new technique for structuring sodium into ultra-thin, precisely patterned films, they found a way to stabilize the metal and make it perform exceptionally well in light-based applications.

Their approach, published in the journal ACS Nano, involved combining thermally-assisted spin coating with phase-shift photolithography—essentially using heat and light to craft nanoscopic surface patterns that trap and guide light in powerful ways.

Even more impressively, the team used ultrafast laser spectroscopy to observe what happens when these sodium surfaces interact with light on time scales measured in trillionths of a second. The results were surprising: sodium's electrons responded in ways that differ from traditional metals, suggesting it could offer new advantages for light-based technologies like photocatalysis, sensing, and energy conversion.

More information: Conrad A. Kocoj et al, Ultrafast Plasmon Dynamics of Low-Loss Sodium Metasurfaces, ACS Nano (2025). DOI: 10.1021/acsnano.5c04946


Original Submission

posted by hubie on Wednesday October 08, @12:31PM   Printer-friendly

https://www.reuters.com/sustainability/society-equity/apple-removes-ice-tracking-apps-after-pressure-by-trump-administration-2025-10-03/:

Apple said on Thursday that it had removed ICEBlock and other similar ICE-tracking apps from its App Store after it was contacted by President Donald Trump's administration, in a rare instance of apps being taken down due to a U.S. federal government demand.

Alphabet's Google also removed similar apps on Thursday for policy violations, but the company said it was not approached by the Justice Department before taking the action.

The app alerts users to Immigration and Customs Enforcement agents in their area, which the Justice Department says could increase the risk of assault on U.S. agents.

[...] Apple removed more than 1,700 apps from its App Store in 2024 in response to government demands, but the vast majority — more than 1,300 — came from China, followed by Russia with 171 and South Korea with 79.


Original Submission

posted by jelizondo on Wednesday October 08, @07:44AM   Printer-friendly

First Dark Matter Sub-Halo Found In The Milky Way:

There are plenty of theories about what dark matter is and how it might be gravitationally affecting the universe. However, proving those theories out is hard since it hardly ever interacts with anything, especially on "small" scales like galaxies. So when a research team claims to have found evidence for dark matter in our own galaxy, it's worth taking a look at how. A new paper from Dr. Surkanya Chakrabati and her lab at the University of Alabama at Huntsville (UAH) does just that. They found evidence for a dark matter "sub-halo" in the galactic neighborhood, by looking at signals from binary pulsars.

A sub-halo is a clumping of dark matter that is brought together inside of a larger "halo" that is thought to form the core of galaxies. Since dark matter primarily interacts through gravity, going theory suggests that it should attract "baryonic" (i.e. normal) matter when it clumps together. This clumping is thought to the scaffolding that galaxies are built on.

Sub-halos are even denser groupings of dark matter that coalesce because of their gravitational attraction. Since they are relatively small compared to the big dark matter halos they are contained in, they can be difficult to detect. To do so, cosmologists would have to find a gravitational signal that deviates from what would be expected given the normal matter surrounding the sub-halo. So far, no one has been able to isolate that kind of signal, despite looking throughout our galactic neighborhood.

Enter binary pulsars - these star pairs contain at least one pulsar, a type of neutron star which emits a large amount of energy on a regular cycle (hence their name). These bursts can be measured so accurately they rival atomic clocks in terms of regularity. The researchers had a theory that they could use deviations in that expected cycle to detect the gravitational effects of a dark matter sub-halo, so they began looking at binary pairs in the galaxy to see if they could find any hint of it.

Overall they looked at 27 binary pulsars, and in particular were looking for gravitational changes between two pairs, to increase the chance there was indeed a structure causing the deviation. They found two, called PSR J1640+2224 and PSR J1713+0747, that had the kind of significant correlated gravitational change they were looking for.

To isolate that gravitational change, the researchers had to eliminate other forms of gravitational acceleration that could be caused by things other than dark matter. One is "gravitational radiation", the acceleration caused when the system gives off gravitational waves, and predicted by the theory of general relativity. Another is the Shklovskii Effect, which is an artifact caused by a binary system moving across our line of sight. Thankfully, both of these effects are well understood and can easily be removed from the calculation of the gravitational influence on the binary system.

Some of that gravitational influence can still come from baryonic matter, but in the case of these two binaries there appeared to be a substantial component that couldn't be explained that way. In fact, the statistics of that additional component were so compelling its hard to argue that it was caused by anything other than an unseen gravitational mass.

Defining that mass was the next step. The researchers pinpointed it at about 2,340 light years away, and determined its mass to be around 2.45 x 107 solar masses. An equivalent amount of baryonic matter causing that gravitational change would be 100 times what is observable in that part of the galaxy.

This research represents the first time a dark matter sub-halo has been detected in the general galactic neighborhood, after having been predicted by theory for years. It also offers a technique by which other researchers could do the same with other sets of binary pulsars. Though rare, astronomers are continually collecting new data on them constantly, giving cosmologists even more data to analyze. Likely this won't be the last time we'll hear of this technique being used to find dark matter sub-halos - there are plenty more places to search for them, and likely many more to discover.

arXiv paper: https://doi.org/10.48550/arXiv.2507.16932

Learn More:
    UAH - UAH researchers use pulsar accelerations to detect a dark matter sub-halo in the Milky Way for the first time
    S. Chakrabarti et al - Constraints on a dark matter sub-halo near the Sun from pulsar timing
    UT - Tying Theory To Practice When Searching For Dark Energy
    UT - Astronomers Search for Dark Matter Using Far Away Galaxies


Original Submission

posted by hubie on Wednesday October 08, @03:03AM   Printer-friendly
from the do-you-hear-what-I-hear? dept.

Instagram says it is not listening to users' microphones to serve ads:

Adam Mosseri, the head of Instagram, has shared a video on his account to dismiss the myth that Instagram is actively listening to users, to show them relevant ads. Now, why would you say that? Unless, it was true! Right?

Jokes aside, the timing couldn't be worse. Yesterday, Meta announced that it will be updating its privacy policy by December 16. Why? Because Meta says that it will use the data collected from user interactions with its AI, to sell targeted ads across its social networks. So, how is this going to work, privacy-wise? Well, that's another story.

The story continues at https://www.ghacks.net/2025/10/02/instagram-says/


Original Submission

posted by jelizondo on Tuesday October 07, @10:17PM   Printer-friendly

https://phys.org/news/2025-10-track-medicines-hitchhike-cholesterol.html

Researchers at The University of Queensland have developed a test that could change our understanding of cholesterol and its potential to ferry deadly cancer messages and life-saving medicines around our body.

Technology developed by Ph.D. scholar Raluca Ghebosu and Associate Professor Joy Wolfram has been designed to assess how different medicines bind to cholesterol particles in our bloodstream.

Ghebosu said mapping this cholesterol "hitchhiking" was crucial to establishing how long medicines remain active, which organs they travel to and, ultimately, how effective they are.

"The problem is that this process requires costly, complex, and time-consuming techniques," Ghebosu said.

"All are significant barriers to what could be a crucial breakthrough in medicine. Our test seeks to simplify the mapping process while also making it much cheaper to get answers."

The new test, named lipoprotein association fluorometry (LAF), was developed at UQ's Australian Institute for Bioengineering and Nanotechnology (AIBN) under the mentorship of Associate Professor Wolfram from the AIBN and the UQ School of Chemical Engineering.

Ghebosu said LAF works by using a fluorescent signal to detect when a "molecular handshake" occurs between cholesterol particles and test agents such as medicines.

Crucially, each test is low cost and delivers results in an hour instead of a week.

"By predicting cholesterol binding to various synthetic nanoparticles—as well as polymers, proteins, peptides, and small molecules—we are better placed to uncover information beneficial to drug development," Ghebosu said.

As well as measuring how medicines bind to cholesterol, Ghebosu said the LAF also showed how cancer cells could be exploiting the same hitchhiking system.

The technology revealed that tiny messenger particles released by cancer cells—called extracellular vesicles (EVs)—display a particular affinity for latching onto "bad" cholesterol particles.

Previous studies have shown that these messenger particles help cancers grow and spread, meaning the binding patterns of these particles with cholesterol could open up new inquiries on how to slow or stop the disease.

"Cholesterol is essential for normal body function, but EVs released by cancer cells may be hijacking this system," Ghebosu said.

Ghebosu said their team had already used the LAF technology to show EVs released by metastatic or "super-spreading," cancer cells were much better at binding to bad cholesterol compared to those from healthy cells and less aggressive cancer cells.

Associate Professor Wolfram said the binding patterns revealed by LAF could advance our understanding of biological processes and inform future medical applications.

"Ultimately, this raises the possibility that cholesterol may contribute to the spread of cancer through EV binding," Associate Professor Wolfram said.

"Thankfully, our technique can also be used to explore therapies that help block this binding and assess whether this could slow cancer progression."

The findings are the subject of a patent application, which is available for licensing from UniQuest, the commercialization company of UQ, and are detailed in the Journal of Extracellular Vesicles.

More information: Raluca Ghebosu et al, Lipoprotein Association Fluorometry (LAF) as a Semi-Quantitative Characterization Tool to Assess Extracellular Vesicle-Lipoprotein Binding, Journal of Extracellular Vesicles (2025). DOI: 10.1002/jev2.70172


Original Submission

posted by hubie on Tuesday October 07, @05:32PM   Printer-friendly

Forget Sparta - Leonidas wiped out all 61 drones in the demo:

Drones have become one of the most important elements of modern warfare, which is why finding effective ways of disabling them is so important. US defense technology firm Epirus has developed a countermeasure that could interest a lot of nations: a high-powered microwave (HPM) weapon that recently demonstrated how it can down 49 drones with a single blast.

[...] During the demo, Leonidas successfully disabled all 61 drones taking part. The headline feat was taking down a 49-drone swarm with a single shot.

[...] Because of how cheaply they can be procured, huge numbers of drones are being used in warfare and for reconnaissance. Leonidas' bursts of electromagnetic energy are designed to disable or destroy the electronics inside hostile drones, including swarms.

The latest second-generation of Leonidas introduces gallium nitride semiconductors. This enables a more compact, reliable, and scalable system compared to legacy microwave weapons that relied on bulkier magnetron tubes.

[...] Leonidas' software-defined architecture allows operators to adjust waveforms on the fly, tailoring effects to different targets and minimizing risks to nearby friendly systems. The modular build also means the weapon can be deployed in multiple configurations, from vehicle-mounted platforms to fixed-site defenses.

Epirus has also developed specialized versions of the weapon, such as Leonidas Expeditionary, optimized for rapid deployment by ground forces, and Leonidas H2O, designed for maritime operations capable of disabling small boat motors.

[...] The latest Leonidas weapon comes at a time when AI-powered drone swarms move closer to frontline deployment. Able to fly and fight as one coordinated force, these drones could overwhelm traditional air defenses, which is why HPM weapons are becoming increasingly important.


Original Submission

posted by jelizondo on Tuesday October 07, @12:49PM   Printer-friendly

https://phys.org/news/2025-10-graphene-reveals-dome-superconductivity-electric.html

Superconductivity is a phenomenon where certain materials can conduct electricity with zero resistance. Obviously, this has enormous technological advantages, which makes superconductivity one of the most intensely researched fields in the world.

But superconductivity is not straightforward. Take, for example, the double-dome effect. When scientists plot where superconductivity appears in material as they change how many electrons are in it, the material's superconducting regions sometimes look like two separate "domes" on a graph.

In other words, the material becomes superconducting, then stops, then becomes superconducting again as we keep changing its electron density.

Double-dome superconductivity has been seen before in some complex materials, such as graphene. Graphene is essentially a sheet of carbon atoms just one atom thick linked together in a honeycomb pattern. Still, it has transformed the field of quantum materials research because it features some really strange effects.

For example, when we stack two graphene layers and twist them at specific angles, the electrons in the graphene behave in new and unexpected ways, creating quantum phases like magnetism, electrical insulation, and, of course, superconductivity.

But there is an even more complex structure of graphene that takes this further by adding a third layer, making the system even more complex and tunable: Magic-angle twisted trilayer graphene (MATTG). With MATTG, researchers can now observe and control a double-dome pattern of superconductivity that was previously only suspected in graphene systems.

In a new study published in Nature Physics, a team led by Mitali Banerjee at EPFL, together with partners in Switzerland, the U.K., and Japan, has shown that MATTG allows direct control of the double-dome superconductivity pattern. By carefully stacking the layers and adjusting the electric field, the researchers could fine-tune the system and track where superconductivity appeared or disappeared as they varied the number of electrons.

Their experiments, supported by theory, revealed that two distinct superconducting regions—the domes—show up as they gradually changed the electron count in MATTG. The work sheds light on how unconventional superconductivity can be created and controlled in 2D materials.

The researchers built devices consisting of three layers of graphene, stacked so the middle one is twisted by about 1.55 degrees relative to the others. They placed the stack between thin layers of insulating hexagonal boron nitride, then added electrodes and gates to precisely control the electron density and apply an electric "displacement field," which let the researchers adjust how electrons move in the material, making it possible to turn superconductivity on or off.

The scientists then measured how MATTG's resistance changed as they varied the electron density, magnetic field, and applied current at temperatures close to absolute zero (100 millikelvin). This allowed them to map out the regions where superconductivity appeared.

By tuning the displacement field, they could further tune the material's band structure (the set of rules that determines how electrons can move and behave inside the material), letting them control the emergence and disappearance of the double-dome pattern.

The team observed that superconductivity in twisted trilayer graphene does not form a single, smooth region but instead splits into two separate domes as the electron density is tuned. Between the domes, superconductivity is strongly suppressed, indicating a possible competition or change in the underlying pairing mechanism.

Each dome displayed unique features: one side showed a sharper and more sudden switch into the superconducting state, and the measurements showed a kind of "memory" in how the material responded to electrical current: how it reacted to increasing current wasn't the same as how it reacted to decreasing current. The other dome had a gentler, slower transition into superconductivity with no evidence of "memory."

The researchers developed theoretical work (Hartree-Fock calculations) to interpret their experimental findings, showing that subtle changes in how the electrons arrange themselves, which are shaped by both interactions and the applied displacement field, determine where superconductivity is favored. The data point to different types of electron pairing in the two domes, possibly linked to changes in the electronic "order" of the system.

The study highlights MATTG as the first system where double-dome superconductivity can be directly controlled by an electric field. It offers a new way to study how unconventional superconductivity emerges and how it can be tuned, opening up possibilities for designing quantum devices or exploring new states of matter in engineered materials.

More information: Zekang Zhou et al, Gate-tunable double-dome superconductivity in twisted trilayer graphene, Nature Physics (2025). DOI: 10.1038/s41567-025-03040-2


Original Submission

posted by hubie on Tuesday October 07, @07:58AM   Printer-friendly

Harvard researchers hail quantum computing breakthrough with machine that can run for two hours — atomic loss quashed by experimental design, systems that can run forever just 3 years away

A group of physicists from Harvard and MIT just built a quantum computer that ran continuously for more than two hours. Although it doesn't sound like much versus regular computers (like servers that run 24/7 for months, if not years), this is a huge breakthrough in quantum computing. As reported by The Harvard Crimson, most current quantum computers run for only a few milliseconds, with record-breaking machines only able to operate for a little over 10 seconds.

Although two hours is still a bit limited, researchers say that the concept behind this could allow future quantum computers to run for much longer, maybe even indefinitely. "There is still a way to go and scale from where we are now," says research associate Tout T. Wang, "But the roadmap is now clear based on the breakthrough experiments that we've done here at Harvard."

[Source]: The Harvard Crimson


Original Submission

posted by hubie on Tuesday October 07, @03:16AM   Printer-friendly
from the who-will-be-the-new-pets.com? dept.

AI Startup Valuations Raise Bubble Fears as Funding Surges

https://www.reuters.com/legal/transactional/ai-startup-valuations-raise-bubble-fears-funding-surges-2025-10-03/

Artificial intelligence startups are attracting record sums of venture capital, but some of the world's largest investors warned that early-stage valuations are starting to look frothy, senior investment executives said on Friday.

"There's a little bit of a hype bubble going on in the early-stage venture space," said Bryan Yeo, group chief investment officer at Singapore sovereign wealth fund GIC (GIC.UL), as part of a panel discussion at the Milken Institute Asia Summit 2025 in Singapore.

"Any company startup with an AI label will be valued right up there at huge multiples of whatever the small revenue (is)," he said. "That might be fair for some companies and probably not for others."

In the first quarter of 2025, AI startups raised $73.1 billion globally, accounting for 57.9% of all venture capital funding, according to PitchBook. The surge was driven by funding rounds like OpenAI's $40 billion capital raising, as investors raced to catch the AI wave.

"Market expectations could be way ahead of what the technology could deliver," Yeo said. "We're seeing a major AI capex boom today. It is masking some of the potential weaknesses that might be going on in the economy."

Todd Sisitsky, president of alternative asset manager TPG said the fear of missing out is dangerous for investors, though he added that views were divided on whether the AI sector had formed a bubble.

Some AI firms are hitting $100 million in revenue within months, he said, while others in early-stage ventures command valuations at between $400 million and $1.2 billion per employee. He said that was "breathtaking."

And perhaps a case in point? . . .

Database Startup Supabase Notches $5 Billion Valuation in Funding Round

Database startup Supabase notches $5 billion valuation in funding round - The Economic Times:

Open-source database startup Supabase said on Friday it has secured a valuation of $5 billion in its latest funding round, as investors continue to back companies riding the wave of the artificial intelligence boom.

[...] Supabase is a backend platform that helps developers build applications quickly and has benefited from the rise in AI-powered coding assistants.

The platform is built on the PostgreSQL open-source database, a system for organizing and managing information online.

The latest capital-raise comes just months after Supabase's Series D round, which reportedly valued it at $2 billion.

[...] Coding platforms such as Lovable and Bolt run on Supabase, which caters to more than four million developers. The company's customers also include enterprises such as PwC, McDonald's and Github Next.

"This new financing aims to accelerate Supabase's efforts to become the backend for everyone, from startups to some of the most demanding, data-intensive enterprise workloads," said Caryn Marooney, general partner at investment management firm Coatue.

Also see:
    • Reuters
    • MSN


Original Submission #1Original Submission #2

posted by hubie on Monday October 06, @10:31PM   Printer-friendly

https://phys.org/news/2025-10-earth-crust-pacific-northwest-necessarily.html

With unprecedented clarity, scientists have directly observed a subduction zone—the collision point where one tectonic plate dives beneath another—actively breaking apart. The discovery, reported in Science Advances, sheds new light on how Earth's surface evolves and raises fresh questions about future earthquake risks in the Pacific Northwest.

Subduction zones are the sites of Earth's most powerful tectonic events. They drive continents across the globe, unleash devastating earthquakes and volcanic eruptions, and recycle the planet's crust deep into the mantle.

But they don't last forever. If they did, continents would endlessly collide and stack up, erasing oceans and wiping out the record of Earth's past. The big question geologists have wrestled with is: how exactly do these mighty systems finally shut down?

"Getting a subduction zone started is like trying to push a train uphill—it takes a huge effort," said Brandon Shuck, an assistant professor at Louisiana State University and lead author of the study. "But once it's moving, it's like the train is racing downhill, impossible to stop. Ending it requires something dramatic—basically, a train wreck."

[...] Off the coast of Vancouver Island, in a region of Cascadia where the Juan de Fuca and Explorer plates slowly move beneath the North American plate, scientists have found the answer. Using a combination of seismic reflection imaging—essentially an ultrasound of Earth's subsurface—and detailed earthquake records, the team has captured a subduction zone in the process of tearing itself apart.

[...] The researchers sent sound waves from the ship into the seafloor and recorded the echoes using a 15-kilometer-long streamer of underwater listening devices. This produced high-resolution images of faults and fractures deep beneath the ocean floor, revealing places where the plate is snapping.

"This is the first time we have a clear picture of a subduction zone caught in the act of dying," said Shuck. "Rather than shutting down all at once, the plate is ripping apart piece by piece, creating smaller microplates and new boundaries. So instead of a big train wreck, it's like watching a train slowly derail, one car at a time."

[...] The team observed tears slicing through the Juan de Fuca plate, including a massive break where the plate has dropped by about 5 kilometers. "There's a very large fault that's actively breaking the [subducting] plate," Shuck explained. "It's not 100% torn off yet, but it's close."

Earthquake records confirm the pattern: along the 75-kilometer-long tear, some sections are still seismically active, while others are eerily quiet. "Once a piece has completely broken off, it no longer produces earthquakes because the rocks aren't stuck together anymore," he said. That missing gap of seismicity is a telltale sign that part of the plate has already detached and the gap is growing slowly over time.

The study found that this breakup happens in stages, through what researchers call "episodic" or "piecewise" termination. Rather than a sudden break across the entire tectonic plate, the plate gradually tears apart one section at a time.

By tearing off in smaller chunks, the larger plate loses momentum—like cutting the cars off a runaway train—and eventually stops being pulled downward. The timing for each piece to break away takes several million years, but together these episodes may gradually shut down an entire subduction system.

This episodic breakup helps explain puzzling features in Earth's history preserved elsewhere, such as abandoned fragments of tectonic plates and unusual bursts of volcanic activity. A striking example lies off Baja California, where scientists have long observed fossil microplates—the shattered remains of the once-massive Farallon plate.

For decades, researchers knew these fragments must be evidence of dying subduction zones, but the mechanism that created them was unclear. Cascadia is now providing that missing piece: subduction zones don't collapse in a single catastrophic event but unravel step by step, leaving behind microplates as geological evidence.

More information: Brandon Shuck et al, Slab tearing and segmented subduction termination driven by transform tectonics, Science Advances (2025). DOI: 10.1126/sciadv.ady8347


Original Submission

posted by hubie on Monday October 06, @05:44PM   Printer-friendly

Flock's Gunshot Detection Microphones Will Start Listening for Human Voices

Flock Safety, the police technology company most notable for their extensive network of automated license plate readers spread throughout the United States, is rolling out a new and troubling product that may create headaches for the cities that adopt it: detection of "human distress" via audio. As part of their suite of technologies, Flock has been pushing Raven, their version of acoustic gunshot detection. These devices capture sounds in public places and use machine learning to try to identify gunshots and then alert police—but EFF has long warned that they are also high powered microphones parked above densely-populated city streets. Cities now have one more reason to follow the lead of many other municipalities and cancel their Flock contracts, before this new feature causes civil liberties harms to residents and headaches for cities.

In marketing materials, Flock has been touting new features to their Raven product—including the ability of the device to alert police based on sounds, including "distress." The online ad for the product, which allows cities to apply for early access to the technology, shows the image of police getting an alert for "screaming."

It's unclear how this technology works. For acoustic gunshot detection, generally the microphones are looking for sounds that would signify gunshots (though in practice they often mistake car backfires or fireworks for gunshots). Flock needs to come forward now with an explanation of exactly how their new technology functions. It is unclear how these devices will interact with state "eavesdropping" laws that limit listening to or recording the private conversations that often take place in public.

Flock is no stranger to causing legal challenges for the cities and states that adopt their products. In Illinois, Flock was accused of violating state law by allowing Immigration and Customs Enforcement (ICE), a federal agency, access to license plate reader data taken within the state. That's not all. In 2023, a North Carolina judge halted the installation of Flock cameras statewide for operating in the state without a license. When the city of Evanston, Illinois recently canceled its contract with Flock, it ordered the company to take down their license plate readers–only for Flock to mysteriously reinstall them a few days later. This city has now sent Flock a cease and desist order and in the meantime, has put black tape over the cameras. For some, the technology isn't worth its mounting downsides. As one Illinois village trustee wrote while explaining his vote to cancel the city's contract with Flock, "According to our own Civilian Police Oversight Commission, over 99% of Flock alerts do not result in any police action."

Gunshot detection technology is dangerous enough as it is—police showing up to alerts they think are gunfire only to find children playing with fireworks is a recipe for innocent people to get hurt. This isn't hypothetical: in Chicago a child really was shot at by police who thought they were responding to a shooting thanks to a ShotSpotter alert. Introducing a new feature that allows these pre-installed Raven microphones all over cities to begin listening for human voices in distress is likely to open up a whole new can of unforeseen legal, civil liberties, and even bodily safety consequences.

https://www.eff.org/deeplinks/2025/10/flocks-gunshot-detection-microphones-will-start-listening-human-voices


Original Submission

posted by mrpg on Monday October 06, @12:59PM   Printer-friendly

JWST Finds An Exoplanet Around A Pulsar Whose Atmosphere Is All Carbon:

Science advances through data that don't fit our current understanding. At least that was Thomas Kuhn's theory in his famous On the Structure of Scientific Revolutions. So scientists should welcome new data that challenges their understanding of how the universe works. A recent paper, available in pre-print on arXiv, using data from the James Webb Space Telescope (JWST) might just had found some data that can do that. It looked at an exoplanet around a millisecond pulsar and found its atmosphere is made up of almost entirely pure carbon.

This type of pulsar, PSR J2322-2650, is known as a "black widow" system, as it powers its high energy outbursts by stealing material from a neighboring star. In this case, that neighboring star has likely been degraded to a "hot Jupiter" companion planet that orbits its parent neutron star every 7.8 hours. A typical "black widow" formation process has two steps - one where the neutron star (which in this case is also a pulsar) steals the material, and a second step where it blasts its companion with high energy gamma radiation, ripping off most of the companion star's outer layers and resulting in a Jupiter-sized exoplanet composed mainly of helium.

The exoplanet around PSR J2322-2650, known as PSR J2322-2650b, does fit the description of a Jupiter-sized planet that seems to have the same density as what would be expected if it was made up primarily of helium. However, its atmosphere is unlike any other black widow companion ever seen. According to the spectrographic reports from JWST, its atmosphere is composed mainly of elemental carbon, taking the form of tricarbon (C3) or dicarbon (C2).

Usually those types of elements are found in the tails of comets, or in actual flames here on Earth. Their presence in a planet's atmosphere, especially in such abundant quantities, is new to science.

Another interesting thing about the planet's atmosphere is the difference between the day and night side. On the dayside, which is always facing the pulsar since the planet is tidally locked, temperatures can reach above 2000 ℃ and there are very clear chemical signatures. However, on the night side, there were almost no features at all, suggesting that side of the planet is covered in soot or something similar that doesn't have any distinct features.

To further prove how strange this planet's atmosphere is, the researchers calculated the ratios between carbon and oxygen as well as carbon and nitrogen. The C/O ratio was over 100, while the C/N ratio was over 10,000. In comparison, the Earth has a C/O ratio of .01 and a C/N ratio of 40. Obviously, there's a lot of carbon on this planet.

And that doesn't fit well with models of how scientists thought the planet should form. As part of the "black widow" process, the outer layers of the planet should have been either siphoned up by the companion star or burned away by that star's radiation. The fact that such a rich carbon atmosphere still exists remains a mystery. There are processes that can create such an atmosphere, such as a white-dwarf merger between [two?] "carbon stars", but even that falls short of explaining how the planet's C/O ratio got so high.

See also:


Original Submission

posted by mrpg on Monday October 06, @08:13AM   Printer-friendly
from the return-to-wolfenstein dept.

https://phys.org/news/2025-09-livestock-safe-wolves.html

Wolves had long been extinct in parts of Central Europe. Thanks to strict regulations to protect species, in recent decades they have become more widespread again. This brings new challenges: in many areas, protecting farm livestock is essential to prevent animals such as sheep, goats and cattle from being killed by hungry wolves.

An international research team at the University of Göttingen, Humboldt-University zu Berlin (HU), Dresden University of Technology in Germany and KORA in Switzerland recently conducted a survey to find out how farmers feel about measures such as wolf‐repelling electric fences or guard dogs, and whether the availability of subsidies influences this.

The survey showed that the willingness to protect livestock depends primarily on social pressure. Financial support is associated with a greater willingness to use electric fences against wolves. The study is published in the journal People and Nature.

In order to investigate perceptions and intentions regarding protecting their herds, the research team conducted an online survey in 2022 among farmers with grazing animals in Bavaria in Germany. The researchers evaluated the responses of 353 people using the "Theory of Planned Behavior."

This psychological theory maintains that whether someone does something or not depends primarily on how strongly the person is committed to it. Their intention is influenced by three factors: their own attitude ("Do I think it makes sense?"), social pressure ("What do the people around me think?"), and perceived control ("Am I able to do it?").

According to the survey results, the drivers behind farmers' willingness to protect livestock vary depending on the measures. However, social pressure plays the most important role.

More information: Friederike Riesch et al, How to reconcile pasture grazing and wolf recolonisation? Perceptions of management options by livestock farmers in Germany, People and Nature (2025). DOI: 10.1002/pan3.70141


Original Submission

posted by mrpg on Monday October 06, @03:30AM   Printer-friendly
from the my-galaxy-your-galaxy dept.

https://phys.org/news/2025-10-bounds-seti.html

The Search for Extraterrestrial Intelligence (SETI) has a data scale problem. There are just too many places to look for an interstellar signal, and even if you're looking in the right place you could be looking at the wrong frequency or at the wrong time. Several strategies have come up to narrow the search given this overabundance of data, and a new paper posted to the arXiv preprint server from Naoki Seto of Kyoto University falls nicely into that category—by using the Brightest Of All Time (BOAT) gamma ray burst, with some help from our own galaxy.

When searching for SETI signals, a civilization has to choose three important factors: where to look, what frequency signal to look for, and when to do so. The same problem is faced by the transmitting side—sending signals strong enough to reach other stars coherently in all directions is extraordinarily energy-intensive. In other words, no sane civilization would do that intentionally for long periods of time. And what if you send the wrong frequency? Or worse yet, hop between frequencies? How would a receiving civilization ever know how to find your signal?

[...] To solve these problems, Dr. Seto, who has also published a paper on anchoring events, suggests a "hybrid" strategy. Instead of using only one event, use two—a "spatial" reference and a "temporal" reference. In the paper, he suggests the spatial reference be the center of the Milky Way, while the temporal reference would be an extremely bright event somewhere outside the galaxy.

The underlying idea is to have a "search ring" centered on the event, in the case that your civilization is looking for signals, and a "transmit ring" exactly opposite the event in the case that your civilization is intending to send them. The diameter of each of these rings grows based on the time since the original burst and the distance from the location to the galactic center. Importantly, the angle between the burst and the galactic center is used to "normalize" the time delay at which a signal would be sent to a specific star system.

[...] Unfortunately, all of this spatial and temporal timing doesn't necessarily coordinate the other variable—frequency. There are some theories that a Schelling point for frequency, such as the Hydrogen Line of 1,420 MHz, where hydrogen shines when undergoing a frequency transition, could be used, but realistically, the receiving civilization would still have to search multiple frequencies over that time.

More information: Naoki Seto, Hybrid Strategy for Coordinated Interstellar Signaling: Linking the Galactic Center and Extragalactic Bursts, arXiv (2025). DOI: 10.48550/arxiv.2509.20718


Original Submission