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Elon Musk’s Neuralink received approval last week from the US Food and Drug Administration to conduct human clinical trials, which one former FDA official called “really a big deal.” I do not disagree, but I am skeptical that this technology will “change everything.” Not every profound technological advance has broad social and economic implications.

With Neuralink’s device, a robot surgically inserts a device into the brain that can then decode some brain activity and connect the brain signals to computers and other machines. A person paralyzed from the neck down, for example, could use the interface to manipulate her physical environment, as well as to write and communicate.

This would indeed be a breakthrough — for people with paralysis or traumatic brain injuries. For others, I am not so sure. For purposes of argument, as there are many companies working in this space, assume this technology works as advertised. Who exactly will want to use it?

One fear is that the brain-machine connections will be expensive and that only the wealthy will be able to afford them. These people will become a new class of “super-thinkers,” lording over us with their superior intellects.

I do not think that this scenario is likely. If I were offered $100 million for a permanent brain-computer connection, I would not accept it, if only because of fear of side effects and possible neurological damage. And I would want to know for sure that the nexus of control goes from me to the computer, not vice versa.

Besides, there are other ways of augmenting my intelligence with computers, most notably the recent AI innovations. It is true that I can think faster than I can speak or type, but — I’m just not in that much of a hurry. I would rather learn how to type on my phone as fast as a teenager does.

A related vision of direct brain-computer interface is that computers will be able to rapidly inject useful knowledge into our brains. Imagine going to bed, turning on your brain device, and waking up knowing Chinese. Sounds amazing — yet if that were possible, so would all sorts of other scenarios, not all of them benign, where a computer can alter or control our brains.

I also view this scenario as remote — unlike using your brain to manipulate objects, it seems true science fiction. Current technologies read brain signals but do not control them.

Another vision for this technology is that the owners of computers will want to “rent out” the powers of human brains, much the way companies rent out space today in the cloud. Software programs are not good at some skills, such as identifying unacceptable speech or images. In this scenario, the connected brains come largely from low-wage laborers, just as both social media companies and OpenAI have used low-wage labor in Kenya to grade the quality of output or to help make content decisions.

Those investments may be good for raising the wages of those people. Many observers may object, however, that a new and more insidious class distinction will have been created — between those who have to hook up to machines to make a living, and those who do not.

Might there be scenarios where higher-wage workers wish to be hooked up to the machine? Wouldn’t it be helpful for a spy or a corporate negotiator to receive computer intelligence in real-time while making decisions? Would professional sports allow such brain-computer interfaces? They might be useful in telling a baseball player when to swing and when not to.

The more I ponder these options, the more skeptical I become about large-scale uses of brain-computer interfaces for the non-disabled. Artificial intelligence has been progressing at an amazing pace, and it doesn’t require any intrusion into our bodies, much less our brains. There are always earplugs and some future version of Google Glass.

The main advantage of the direct brain-computer interface seems to be speed. But extreme speed is important in only a limited class of circumstances, many of them competitions and zero-sum endeavors, such as sports and games.

Of course, companies such as Neuralink may prove me wrong. But for the moment I am keeping my bets on artificial intelligence and large language models, which sit a comfortable few inches away from me as I write this. 

© 2023 Bloomberg LP


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New Inelastic Dark Matter Model Could Bypass Current Limits of Particle Detection

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New Inelastic Dark Matter Model Could Bypass Current Limits of Particle Detection

A group of physicists at the University of São Paulo’s Institute of Physics has proposed a model of the behaviour of dark matter (DM) in the presence of dark energy (DE) that is compatible with current astronomical observations. A model of inelastic DM can be realised from light-weight particles, which are collectively interacting through the massive vector mediator, and the model is an alternative explanation for DM relics in the universe. Importantly, this framework may have the potential to circumvent the experimental hurdles for the detection of DM that have thus far kept it in the dark. The findings are published in the Journal of High Energy Physics, and its authors believe it has the potential to “revolutionise” how particle physics analyses are conducted in the future.

Light Mediator ZQ Offers New Clues to Elusive Dark Matter and Its Cosmic Origins

As per the users’ report, they have developed the following new model: a heavy, stable DM from a light, unstable one. This can be expressed as a heavy stable DM due to a heavy unstable one, which may give rise to the “thermal freeze-out” in the universe. It doesn’t just interact with visible matter but with dark matter as well, and that’s how you get the new observational windows.

To explain why the dark matter has not been observed until now, the model further involves a decay of the unstable dark matter χ2 to some species not disturbing the CBR, and thus also not presenting a visible/observable decay signal. The picture is consistent with current astrophysical and experimental constraints, avoiding simpler `vanilla’ DM scenarios.

ZQ-induced vector mediators are light portals connecting the two sectors and may mediate the direct interactions between the dark sector and the SM particles. The black line indicates the region in the parameter space where dark matter can be hiding unobserved — this is to be addressed in future experiments.

The study suggests the search for dark matter should pivot from the “discovery frontier”, in which exquisitely sensitive instruments scan for signals, to the “intensity frontier”, which seeks ever-finer measurements to tease out anomalies. Future experiments will seek to dig more deeply into these unexplained corners of particle physics with a new online tool.

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Massive 200-Light-Year Cloud May Be Channeling Matter to the Milky Way’s Core

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Massive 200-Light-Year Cloud May Be Channeling Matter to the Milky Way's Core

Astronomers have found a vast, never-before-noticed reservoir of stellar material, hundreds of light-years across, lurking in a cold, dark, starless swath of our galaxy. It’s dubbed the Midpoint Cloud and was identified using the Green Bank Telescope; it appears to channel dense clouds of material into the heart of our galaxy. It harbours active regions filled with dense dust lanes and star formation possibilities. These lanes could be bringing twisted matter into the galaxy’s central bar, shaping how stars form in this extreme environment and offering a rare snapshot of the first stages of a galaxy’s evolution.

Newly Found Midpoint Cloud May Be Key to Star Formation in the Milky Way’s Core

As per the study, researchers at the National Radio Astronomy Observatory and Green Bank Observatory confirmed the size and shape of the GMC based on mass, density, and movement. The gassy chaos in the cloud mirrors the caustic turmoil at the galactic centre, yielding measurements from a faint object that says something about an energetic event 200 light-years distant. That could be a link from the field-like tranquillity of our own Milky Way’s disk to the mayhem of its core.

Perhaps analogously to gas channels, a thick dust lane in the Midpoint cloud could supply the central stellar bar fragment with fresh gas, again supporting an interpretation that star formation is inhibited in this region by the strong gravitational potential. But regions like the Midpoint could collect such thick gas, spurring the birth of new stars.

The team classified Knot E as a compact gas clump whose material has been eroded by both star radiation and a maser, or microwave emission, within a cloud. A shell-like feature suggests earlier supernova explosions, like those the deaths of massive stars in the region might have initiated.

The Midpoint cloud Larry Morgan, of the Green Bank Observatory, discovered is a valuable clue in our knowledge of how galaxies evolve and form stars near their centers. The finding could give scientists a way to learn how matter flows inward across the cosmos, one hidden cloud at a time.

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Supergiant Star Wd1-9 Investigated: Know Everything about New Findings and Insights from Supergiant

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Supergiant Star Wd1-9 Investigated: Know Everything about New Findings and Insights from Supergiant

In the latest edition of the scientific investigations, it has come to light that the Chandra X-Ray Observatory of NASA has been employed by an international team of astronomers to investigate a supergiant star called Wd1-9. It has certainly performed a detailed investigation, which was accompanied by in-depth analysis and offered essential insights. Considering the supergiant B Stars, these are quite rare in the Milky Way. As these stars grow, they undergo continuous changes. These stars also exhibit strong Balmore emission lines, forbidden lines, and infrared excess.

Wd1-9: What is this Supergiant B Star?

Wd1-9 is a supergiant B (e) star in Westerlund 1. It is located at a distance of 13,800 light years from Earth. This star is the brightest radio source present within the cluster. Likewise, the recent findings presented in the paper published on July 23rd, 2025, suggest that this star displays a rich emission-line spectrum. Significantly, no photospheric features were detected.

Although Wd1-9 has been studied multiple times at different wavelengths, its true nature is still unknown due to it being covered by a cloud of dust. As the previous research suggests, this star may be a cool hypergiant or an interacting binary system. Now, to overcome these suspicions, Konstantina Anastasopolou led a team of the Harvard-Smithsonian Center for Astrophysics (CfA), Cambridge, employed Chandra to dig deeper.

What did the Astronomers Find?

As per the observations offered by Chandra, it was witnessed that Wd1-9 exhibits long-term X-ray variability. The team further identified an orbital period that comprised a 14-day periodic signal. According to the astronomers, this is the first period determination for the Wd1-9.

Significantly, the astronomers found that strong emission lines were detected that surfaced from elements like silicon, sulfur, and argon. Similarly, the iron emission line at 6.7 keV was identified for the first time ever. These identifications have become a part of the new findings.

To Conclude

According to the astronomers, the above-specified findings directly relate to binarity. The spectrum of Wd1-9 resembles the Wolf-Rayet (WR) binaries in Westerlund 1. Also, when the astronomers examined the X-Ray color-color diagrams, they identified that Wd1-9 showcased variations in thermal temperatures. After analysing the findings and putting all the examinations together, the scientists concluded that Wd1-9 is a part of the binary system.

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