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This video explores fascinating engineering solutions hiding in plain sight — ingenious designs that solve complex problems through elegant simplicity. From shoes that expand when stretched to windshields with hidden patterns, discover how everyday objects incorporate remarkable engineering innovations.

AUXETICS
These metamaterials that defy conventional physics by getting thicker when stretched. Follow their evolution from theoretical designs in 1978 to modern applications in athletic footwear and medical devices, and discover how precise geometric patterns create extraordinary properties that could revolutionize everything from prosthetics to architecture, despite challenging manufacturing requirements.

WINDSHIELD DOTS
The black dots on car windshields serve a dual purpose that revolutionized the automotive industry in the 1950s. This pattern manages extreme thermal stress during glass tempering while protecting crucial adhesive bonds. The precise ceramic frit application process has evolved to support modern safety systems and sensor integration, making these simple dots essential to modern vehicle design.

CURIE POINT HEATERS
Curie point heaters achieve temperature control through magnetic properties alone, eliminating complex control systems. These heaters maintain precise temperatures by becoming “magnetically invisible” at specific points. Modern implementations use sophisticated alloy combinations and multi-layer designs for unprecedented temperature control in medical sterilization and semiconductor processing.

TRIBOELECTRIC GENERATORS

An international team of astronomers has employed the James Webb Space Telescope (JWST) to observe a supermassive Galactic open cluster known as Westerlund 1. Results of the observational campaign, presented in a paper published Nov. 20 on the arXiv preprint server, yield important insights about the structure and properties of this cluster.

Open clusters (OCs), formed from the same giant molecular cloud, are groups of stars loosely gravitationally bound to each other. So far, more than 1,000 of them have been discovered in the Milky Way, and scientists are still looking for more, hoping to find a variety of these stellar groupings. Expanding the list of known galactic and studying them in detail could be crucial for improving our understanding of the formation and evolution of our galaxy.

It is assumed that most takes place in massive clusters of stars, known as superstar clusters (SSCs). They are very massive young OCs usually containing a very large number of young, . The total mass of a typical SSC exceeds 10,000 solar masses.

How long until humans are made redundant by the evolution of technology? Is there an inherent difference between men and women’s intelligence? Daniel Dennett answers questions from the audience following his talk. Watch the main event here: • Information, Evolution, and intellige…
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The concept of information is fundamental to all areas of science, and ubiquitous in daily life in the Internet Age. However, it is still not well understood despite being recognised for more than 40 years. In this talk, Daniel Dennett explored steps towards a unified theory of information, through common threads in evolution, learning, and engineering.

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Most of the diverse elements in the universe come from supernovae. We are, quite literally, made of the dust of those long-dead stars and other astrophysical processes. But the details of how it all comes about are something astronomers strive to understand.

How do the various isotopes produced by supernovae drive the evolution of planetary systems? Of the various types of supernovae, which play the largest role in creating the elemental abundances we see today? One way astronomers can study these questions is to look at presolar grains.

These are dust grains formed long before the formation of the sun. Some of them were cast out of older systems as a star fired up its nuclear furnace and cleared its system of dust. Others formed from the remnants of supernovae and stellar collisions. Regardless of its origin, each presolar grain has a unique isotopic fingerprint that tells us its story.

We’ve all been there. Moments after leaving a party, your brain is suddenly filled with intrusive thoughts about what others were thinking. “Did they think I talked too much?” “Did my joke offend them?” “Were they having a good time?”

In a new Northwestern Medicine study, scientists sought to better understand how humans evolved to become so skilled at thinking about what’s happening in other peoples’ minds. The findings could have implications for one day treating such as anxiety and depression.

“We spend a lot of time wondering, ‘What is that person feeling, thinking? Did I say something to upset them?’” said senior author Rodrigo Braga. “The parts of the brain that allow us to do this are in regions of the human brain that have expanded recently in our evolution, and that implies that it’s a recently developed process. In essence, you’re putting yourself in someone else’s mind and making inferences about what that person is thinking when you cannot really know.”

Unitary collapse of Schrödinger’s cat state https://journals.aps.org/pra/abstract/10.1103/PhysRevA.110.L030202

Schrödinger’s cat, that iconic thought experiment where a cat in a box is both alive and dead until someone peeks.


The authors study a system composed of a single qubit coupled to a soft-mode quantum oscillator. They show that spontaneous unitary evolution of this system create a Schr\ odinger-cat-like state of the oscillator, which is subsequently lost in a sudden process strongly resembling the measurement-induced collapse of wave function.

Some sequences in the genome cause genes to be switched on or off. Until now, each of these gene switches, or so-called enhancers, was thought to have its own place on the DNA. Different enhancers are therefore separated from each other, even if they control the same gene, and switch it on in different parts of the body.

A recent study from the University of Bonn and the LMU Munich challenges this idea. The findings are also important because gene switches are thought to play a central role in evolution. The study has been published in the journal Science Advances.

The blueprint of plant and animal forms is encoded in their DNA. But only a small part of the genome—about two percent in mammals—contains genes, the instructions for making proteins. The rest largely controls when and where these genes are active: how many of their transcripts are produced, and thus how many proteins are made from these transcripts.

Scientists have now performed one such large-scale test by using DESI. They observed almost 6 million galaxies and quasars, which are bright hearts of galaxies powered by feeding supermassive black holes. Perhaps unsurprisingly, this test, which has traced the evolution of the universe since it was around 3 billion years old, has once again shown general relativity to be the right “recipe” for gravity.

“General relativity has been very well tested at the scale of solar systems, but we also needed to test that our assumption works at much larger scales,” study co-leader and the French National Center for Scientific Research (CNRS) cosmologist Pauline Zarrouk said in a statement. “Studying the rate at which galaxies formed lets us directly test our theories and, so far, we’re lining up with what general relativity predicts at cosmological scales.”