Tag Archives: ultrafast

Unlocking the Secret: Why Your New ‘Ultra-Fast’ Wi-Fi Still Leaves You Feeling Disconnected

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In today’s fast-paced digital world, a reliable Wi-Fi connection is essential. Dealing with slow or erratic Wi-Fi can lead to interruptions in streaming, gaming, and even smart home functionality. It’s no surprise that emerging wireless technologies promise to alleviate these connectivity issues.

Enter Wi-Fi 7, the latest wireless standard poised to revolutionize connectivity. With a staggering top speed of “up to 46 gigabits per second (Gbps),” Wi-Fi 7 can theoretically download a 4K movie in as little as 8 seconds—almost five times quicker than Wi-Fi 6/6E’s maximum of 9.6 Gbps.

However, the reality is that most households won’t achieve these headline speeds. Real-world testing typically reveals speeds in the range of hundreds of megabits per second (Mbps), considering that most UK broadband services max out at 1-2 Gbps.

So, what’s behind the discrepancy?

Understanding Real-World Performance

The gap between theoretical and actual speeds highlights that user experience is largely influenced by real-world conditions. Factors such as construction materials and radio wave interference play significant roles.

Despite the lofty claims, Wi-Fi 7—officially known as 802.11be—incorporates substantial technological advancements. Designed to manage data more efficiently, especially in dense environments with multiple connected devices, Wi-Fi 7 introduces wider channels, allowing for up to 320 megahertz (MHz) of bandwidth, doubling the capacity of Wi-Fi 6E. Think of it as expanding lanes on a busy freeway.

Struggling with poor Wi-Fi? Your home layout could be the culprit. – Photo credit: Getty

Wi-Fi 7 utilizes a feature called Multilink Operation (MLO), which optimizes the use of various frequency bands (2.4 GHz, 5 GHz, and 6 GHz) to find the most reliable path through a congested network. Additionally, it employs a high-density encoding method called 4096-QAM, increasing data throughput under favorable conditions.

Navigating the Challenges

That said, taking full advantage of Wi-Fi 7 requires hardware upgrades across your devices. Since the benefits are hardware-dependent, you’ll need to invest in a new router as well as the latest smartphones, laptops, and smart devices.

Many users will find themselves in a mixed-environment for some time, using a combination of older and newer devices, which may limit the overall experience. The enhancements may not be as pronounced as some users expect.

Moreover, the gains in speed are heavily reliant on maintaining high signal quality. “Wi-Fi 7’s theoretical speeds were measured in ideal lab conditions,” advises Dr. Richard Rudd, a certified engineer and communications consultant.

As Dr. Rudd notes, the actual signal within a home can be severely affected by factors like building materials, interference from other devices, and layout. Frequencies above 6 GHz tend to experience faster signal degradation over distance.

In essence, Wi-Fi 7’s peak performance is contingent on optimal environmental conditions—strong signals and minimal obstructions. As with all wireless standards, there’s a disparity between maximum and actual speeds.

According to Professor Izzat Darwazeh from UCL, “The capacity of a channel is directly proportional to its bandwidth per the Shannon-Hartley theorem.” Thus, while the potential for double the capacity over Wi-Fi 6E exists, noise and interference directly reduce actual speed.

MLO optimizes network pathways—but many variables still influence performance. – Image credit: Getty

While Wi-Fi 7 cannot overcome physical barriers, it does promise real enhancements to connectivity. Research by Ookla revealed that median download speeds for Wi-Fi 7 reached 665.01 Mbps on EE’s service—four times the performance of Wi-Fi 6 in comparable scenarios, with almost double the upload speed.

Beyond Just Speed

While speed is often the focal point, other advantages may hold greater significance. Tests conducted by the Wireless Broadband Alliance (WBA) showed Wi-Fi 7 offering lower latency, reduced jitter, and improved stability across multiple rooms compared to Wi-Fi 6.

“Wi-Fi 7 transcends mere speed—it’s about delivering a consistent, predictable user experience,” says Bruno Tomas, WBA Chief Technology Officer.

“Our testing revealed speeds of 3.5 Gbps in real-world scenarios, with peaks of 4.2 Gbps in Turkey, showcasing stability across multiple rooms—this consistency is what distinguishes Wi-Fi 7 from its predecessors.”

WBA chairman Tiago Rodriguez emphasizes the need for service providers to enhance clarity around Wi-Fi 7’s capabilities. “Understanding the distinction between theoretical and real-world speeds is vital.”

Similar to a car’s fuel efficiency, the advertised speeds of Wi-Fi can’t be fully realized unless you have a compatible infrastructure in place.

In the UK, regulatory and physical limitations hinder access to the full benefits of Wi-Fi 7. The broader 6 GHz spectrum that facilitates its features is still largely unavailable. Yet, these conditions may evolve as regulatory frameworks are reassessed.

As Dr. Rudd points out, although full potential isn’t yet realized in the UK or Europe, Wi-Fi 7 still offers significant capabilities that exceed current user demands.

Top-tier Wi-Fi is crucial for environments with high demand—like concerts and lectures. – Photo credit: Getty

Navigating Reality vs. Hype

This brings us to the current dilemma surrounding Wi-Fi 7. While its advancements are clear, the practical benefits may not resonate with users, especially those already equipped with Wi-Fi 6 or 6E routers, according to Mark Jackson from ISPreview UK.

“If your devices are already Wi-Fi 6 compatible, upgrading may not be essential right now,” he notes. “However, users in environments that demand high performance, like online gamers, should consider an upgrade.”

For those using older Wi-Fi technology, it may be less about performance and more about addressing potential security vulnerabilities. Eventually, upgrading will become necessary for most households due to technology advancements.

Professor Darwazeh agrees, stating that Wi-Fi 7’s primary advantages lie in high-density environments like lecture halls and stadiums—most home users won’t notice a substantial difference unless their connection is under high strain.

“New technologies often create new use cases, and we anticipate that Wi-Fi 7 will also reframe user experience over time,” he concludes.

Ultimately, while Wi-Fi 7 represents a leap forward in technology, its tangible benefits may not be immediately recognized by the average consumer. Connectivity issues should be addressed through optimal router placement and mesh systems rather than merely chasing higher speeds.

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Source: www.sciencefocus.com

Exploring Unprecedented Universes: Using Ultra-Fast Measurements with Nuclear Clocks

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Humans have been striving to measure the world we live in for a long time. Our measurement systems and units help us comprehend ourselves and our environment, whether we are dealing with basic physics theories or not.

When we measure something, we compare it to a standard benchmark to ensure accuracy and stability. The current benchmark for time is the atomic clock, which relies on the precise energy levels of electrons in an atom.

Atomic clocks, however, have limitations due to environmental factors affecting the energy levels within the atom. This has led to the exploration of nuclear clocks, especially using the rare thorium-229 isotope.

Thorium-229 has unique characteristics that make it an ideal candidate for creating nuclear clocks. Its nucleus has closely spaced energy levels that can provide more stable measurements of frequency and time compared to atomic clocks.

The recent advancements in using thorium-229 for nuclear clocks have opened up new possibilities for accurate time measurements and potential breakthroughs in fundamental physics theories.

Why go to the nuclear?

Nuclear clocks offer greater stability and accuracy compared to atomic clocks due to the small size of the nucleus and reduced influence from external factors. By utilizing thorium-229 and its unique energy levels, nuclear clocks can revolutionize time measurements.

These advancements in time measurement are not only essential for navigation and communication systems but also play a crucial role in testing fundamental physics theories such as relativity.

Accurate clocks can also help in exploring dark matter and understanding its interactions with normal matter. Nuclear clocks provide a more precise benchmark for detecting the effects of dark matter on time measurements.

What’s next?

The next step after harnessing thorium-229 for nuclear clocks is to develop a functional and reliable clock system. This involves stabilizing a laser to the frequency corresponding to nuclear energy levels and constructing a robust clock design.

While there are challenges in developing nuclear clocks, the potential for unprecedented accuracy in time measurement is promising. These advancements require in-depth calculations and understanding of fundamental forces like quantum chromodynamics (QCD).

Overall, the progress in nuclear clocks signifies a new era in precise timekeeping and could lead to significant advancements in our understanding of the universe and fundamental physics theories.

Source: www.sciencefocus.com

XMM-Newton discovers ultrafast black hole wind in Markarian 817

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Markarian 817 is the Seyfert 1 galaxy located 430 million light-years away in the constellation Draco. Also known as Mrk 817 or QSO J1436+5847, it hosts an active supermassive black hole of 81 million solar masses.

This artist's impression shows super-fast winds blowing from the center of the galaxy Markarian 817. These winds travel at millions of kilometers per hour and remove interstellar gas from vast regions of space. Without this gas, galaxies cannot form new stars, and the black holes at the galaxies' centers have little left to eat. The inset shows what is happening at the center of the galaxy. A supermassive black hole draws in gas from its surroundings to form a hot, brightly lit accretion disk (orange). The wind (white) is caused by a magnetic field within the disk, which causes particles to fly in all directions at incredibly high speeds. These winds effectively block the X-rays (blue) emitted by the extremely hot plasma surrounding the black hole, called the corona.Zack other. Using his X-ray telescope XMM-Newton at ESA, he captured Markarian 817 blowing out super-fast winds. This wind, which lasts for about a year, will have a major impact on star formation in the galaxy. The fact that black holes at the centers of galaxies exhibited fairly average activity levels before generating winds suggests that supervelocity black hole winds are much more common than previously thought. doing. In other words, black holes and their host galaxies strongly influence each other's evolution. Image credit: ESA / CC BY-SA 3.0 IGO.

At the center of every large galaxy is a supermassive black hole whose enormous gravitational pull pulls in gas from its surroundings.

As the gas spirals inward, it collects in a flat accretion disk around the black hole, where it heats up and glows.

Over time, the gas closest to the black hole passes the point of no return and gets swallowed up.

But black holes consume only a portion of the gas that swirls toward them.

While surrounding the black hole, some matter is bounced back into space, much like a messy toddler spilling everything on his plate.

In a more dramatic episode, a black hole turns the entire table upside down. The gas in the accretion disk is thrown off in all directions at such high velocities that it wipes out the surrounding interstellar gas.

This not only deprives the black hole of food, but also means that new stars cannot form over large areas and the structure of the galaxy changes.

Until now, this ultrafast black hole wind had only been detected as coming from a very bright accretion disk at the limit of its ability to pull in matter.

At this time, ESA's XMM-Newton spacecraft detected superfast winds in Markarian 817, a decidedly average galaxy that could be described as “just having a snack.”

“With the fans on the highest setting, we would expect very fast winds,” said Dr. Miranda Zak, an astronomer at the University of Michigan.

“In the galaxy we studied called Markarian 817, the fans were turned on at a lower power setting, but still produced incredibly energetic winds.”

“It is very rare to observe ultrafast winds, and even rarer to detect winds with enough energy to change the properties of the host galaxy.”

“The fact that Markarian 817 produced these winds for about a year, even though it was not particularly active, suggests that the black hole may have changed the shape of its host galaxy much more than previously thought. “This suggests that there is a sex,” said Roman astronomer Elias Cammun. Tre University.

Active galactic nuclei emit high-energy light, including X-rays. Markarian 817 stood out to astronomers because it was extremely quiet.

“The X-ray signal was so weak that I knew I was doing something wrong,” Zak said.

Follow-up observations using ESA's XMM Newton revealed what was actually happening. The superfast winds from the accretion disk acted like a shroud, blocking the X-rays emitted from the black hole's immediate surroundings.

These measurements were supported by observations made with NASA's NuSTAR telescope.

Detailed analysis of X-ray measurements revealed that Markarian 817's center did not send out a single puff of gas, but instead created a gust of wind storm over a wide area of ​​the accretion disk.

The winds lasted for hundreds of days and consisted of at least three distinct components, each traveling at a few percent of the speed of light.

This solves an unsolved puzzle in understanding how black holes and their surrounding galaxies interact with each other.

Many galaxies, including the Milky Way, appear to have large regions around their centers where few new stars form.

This could be explained by black hole winds sweeping away star-forming gas, but this works only if the winds are fast enough, persist long enough, and are produced by black holes at typical activity levels. limited to cases where

“One of the many unresolved problems in black hole research is the problem of achieving detection through long-term observations over many hours to capture important events,” said Dr. Norbert Schartel, a scientist on the XMM-Newton project. says.

“This highlights the paramount importance of the XMM-Newton mission into the future.”

“No other mission can achieve that combination of high sensitivity and the ability to make long, uninterrupted observations.”

a paper Regarding the survey results, Astrophysics Journal Letter.

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Miranda K. Zackother. 2024. Seyfert 1.2 Markarian 817 Hidden Sub-Eddington Feedback Intense Feedback.APJL 962, L1; doi: 10.3847/2041-8213/ad1407

Source: www.sci.news