Toggle light / dark theme

Scientists are diving into the deep sea to study one of the universe’s biggest mysteries—quantum gravity.

Using KM3NeT, a vast underwater neutrino telescope, researchers are watching ghost-like particles that may hold the key to uniting the physics of the very large and the very small. By analyzing how neutrinos oscillate—or don’t—during their journey through space, they’re searching for subtle signs of decoherence, a possible effect of quantum gravity.

A tiny particle and a big physics puzzle.

Fusion is inching closer to reality with continuous development in this field as the United States Domestic Agency for the International Thermonuclear Experimental Reactor (ITER) recently completed the delivery of critical components for the support structure of central solenoid.

Described as an exoskeleton, or a cage, the support structure surrounds the central solenoid, which is a 60-foot-tall superconducting magnet at the heart of the ITER fusion machine.

Astronomers uncover extremely hot and violent eruption from first ever near-infrared analysis of a recurrent nova outside of the Milky Way Galaxy. Using the Gemini South telescope, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation and operated by NSF NOIRLab, and the Magellan Baade Telescope, astronomers have for the first time observed a recurring nova outside of the Milky Way in near-infrared light. The data revealed highly unusual chemical emissions as well as one of the hottest temperatures ever reported for a nova, both indicative of an extremely violent eruption.

Nova explosions occur in binary star systems in which a white dwarf — the dense remnant of a dead star — continually siphons stellar material from a nearby companion star. As the outer atmosphere of the companion gathers onto the surface of the white dwarf it reaches temperatures hot enough to spark an eruption.

Almost all novae discovered to-date have been observed to erupt only once. But a few have been observed to erupt more than once, and are classified as recurrent novae. The span between eruptions for these novae can vary from as little as one year to many decades [1].

I normally don’t post videos, but I think many may want to watch this it’s pretty cool. A guy talks about or rather reviews 7 Free AI tools that you can try out now. Some you get credits, and then subscribe later. They are pretty cool. The one that makes music from a description is hilarious.


🎖️ Hostinger: https://hostinger.com/wearenocode.
❇️ FREE COURSE: https://bit.ly/4aBjbaU
🚀 1-on-1 COACHING: https://www.wearenocode.com/mvp-accelerator.

🛠 TOOLS:

Outbond: https://www.outbond.io/
Google AI Studio: https://aistudio.google.com/live.
Gamma: https://gamma.app/signup?r=mgp7dnjaverd8n2
Hostinger: https://hostinger.com/wearenocode.
Suno: https://suno.com/
Leonardo AI: https://leonardo.ai/
Eleven Labs: https://try.elevenlabs.io/mixajdyhxnx3
Runway AI: https://runwayml.com/

Full Repository: https://bit.ly/4bw2uyI

Immunotactoid glomerulopathy occurs in adults, on average at 60 years of age, and often presents with nephrotic proteinuria, reduced glomerular filtration rate, and hypocomplementemia in half of affected patients. Patients do not have cryoglobulins, but a circulating monoclonal paraprotein and/or lymphoplasmacytic malignancy is present in about two-thirds. Prognosis depends on the outcome of the associated disease, with half of the affected patients achieving remission with therapy directed at the malignancy.

The University of Cincinnati is leading public urban universities into a new era of innovation and impact. Our faculty, staff and students are saving lives, changing outcomes and bending the future in our city’s direction. Next Lives Here.

Study coauthors include UC’s Sreekar Puchala and Anca Ralescu and Ethan Muchnik of the University of Oregon. The study authors declare no competing interests.

This work was supported by the Office of the Assistant Secretary of Defense for Health Affairs, through the Defense Medical Research and Development Program under Award No. W81XWH-16–2–0020. Opinions, interpretations, conclusions and recommendations are those of the author and are not necessarily endorsed by the Department of Defense.