Until his dying days, the giant of 20th-century physics obsessed over the underpinnings of space and time, and how we can all share the same version of them.
Category: physics
Before arriving at Janelia three years ago, Postdoctoral Scientist Antonio Fiore was designing and building optical instruments like microscopes and spectrometers. Fiore, a physicist by training, came to the Pedram Lab to try something new.
“I focused on the physics rather than investing in the biological applications of the optics I was developing,” Fiore says. “I came to the Pedram Lab in search of a different kind of impact, joining a team that explores areas of biology that need new tools, while keeping a connection to light microscopy.”
So far, Fiore’s new direction is paying off.
Researchers have developed a novel experimental platform to measure the electric fields of light trapped between two mirrors with a sub-cycle precision.
These electro-optic Fabry-Pérot resonators will allow for precise control and observation of light-matter interactions, particularly in the terahertz (THz) spectral range. The study is published in the journal Light: Science & Applications.
The researchers are from the Department of Physical Chemistry at the Fritz Haber Institute of the Max Planck Society and the Institute of Radiation Physics at Helmholtz Center Dresden-Rossendorf.
Combining concepts from statistical physics with machine learning, researchers at the University of Bayreuth have shown that highly accurate and efficient predictions can now be made as to whether a substance will be liquid or gaseous under given conditions. They have published their findings in Physical Review X.
Observation of a glass of water reveals that the water exists in two distinct phases: liquid and gas. Even at room temperature, water molecules are constantly evaporating from the surface of the liquid water and passing into the gas phase. At the same time, some of the water molecules from the gas condense back into the liquid.
The transition from one phase to the other depends on temperature and pressure. Above a critical temperature, the simultaneous coexistence of gas and liquid disappears. The resulting supercritical fluid no longer forms an interface. This is important for industrial processes such as separation, cleaning and production.
Scientists have found a way to achieve negative refraction, using carefully arranged atomic arrays instead of engineered metamaterials. VERY GOOD!
Ask the researchers: Do you understand the spacetime background of atomic arrays interactions?
Scientific research guided by correct theories can enable researchers to think more.
https://chatgpt.com/share/67aa58eb-452c-8011-a942-a4a084a17f23
The recent development of AI presents challenges, but also great opportunities.
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Hello and welcome! My name is Anton and in this video, we will talk about the discovery of the most massive superstructure in the nearby universe — Quipu.
https://arxiv.org/abs/2501.19236
Bohringer et al., Astronomy and Astrophysics, 2025
https://en.wikipedia.org/wiki/Sachs%E2%80%93Wolfe_effect.
Similar videos:
https://youtu.be/wp8zHG1g7bc.
#quipu #superstructure #cosmos.
0:00 Largest superstructure in the universe — Quipu.
0:45 Laniakea discovery of 2014
1:25 Shapley concentration.
2:35 Cosmological issues: Hubble Tension and S8 tension.
3:45 New study mapping galaxies and the discovery.
5:15 Additional findings and implications.
6:25 What is this though?
7:20 Confirming predictions and how this was found.
8:40 What’s next?
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How fast is the speed of light? This video explores the true scale of the universe by simulating travel at light speed and beyond. Starting from outside the Milky Way, we move through cosmic objects like Andromeda, the Pleiades, and even our Solar System. Watch as the limits of light speed reveal just how unimaginably vast the universe is. From 1x the speed of light to trillions of times faster, this journey will change how you see the cosmos and our place within it. Perfect for space enthusiasts and anyone curious about the true scale of the universe.
#astronomy #astrophysics #spaceengine #space
How does a star’s activity influence exoplanet data obtained by scientists? This is what a recent study published in The Astrophysical Journal Supplement Series hopes to address as a team of researchers at University College London (UCL) investigated how stellar activity, specifically star spots, could be “contaminating” exoplanet data, specifically exoplanet atmospheric data. This study has the potential to help astronomers develop more efficient methods for studying exoplanets and their atmospheres, specifically with the number of confirmed exoplanets increasing regularly.
For the study, the researchers used NASA’s Hubble Space Telescope to analyze data from 20 gas giant exoplanets ranging in size between Neptune-like and hot-Jupiter that transited their respective parent stars. To obtain a more complete dataset, the team observed the exoplanets from optical to near-infrared wavelengths. In the end, they discovered a broad range of “stellar contamination”, meaning stellar activity was influencing the exoplanet data, specifically regarding the atmospheric compositions and temperatures. For example, the results indicated that the number of specific molecules had errors as high as 6 orders of magnitude while temperatures had errors as high as 145 percent.
“Hotter, brighter regions (faculae) emit more light and so, for instance, if a planet passes in front of the hottest part of the star, this might lead researchers to over-estimate how large the planet is, as it will seem to block out more of the star’s light, or they might infer the planet is hotter than it is or has a denser atmosphere. The reverse is true if the planet passes in front of a cold starspot, making the planet appear ‘smaller’,” said Alexandra (Alex) Thompson, who is a PhD student in UCL’s Department of Physics & Astronomy and a co-author on the study.
Scientists have just discovered the largest structure ever found in the universe, and it’s changing everything we thought we knew about space! Quipu, a superstructure spanning 1.3 billion light-years, is bending light, distorting cosmic expansion, and even affecting the Cosmic Microwave Background. What does this mean for our understanding of dark matter, energy, and galaxy evolution? Watch this video to explore Quipu’s secrets and their impact on the universe! 🚀✨ paper link: https://arxiv.org/abs/2501.19236 MUSIC TITLE : Starlight Harmonies MUSIC LINK : https://pixabay.com/music/pulses-starlight-harmonies-185900/ Visit our website for up-to-the-minute updates: www.nasaspacenews.com Follow us Facebook: https://www.facebook.com/nasaspacenews Twitter: https://twitter.com/SpacenewsNasa Join this channel to get access to these perks: https://www.youtube.com/channel/UCEuhsgmcQRbtfiz8KMfYwIQ/join #NSN #NASA #Astronomy#SpaceDiscovery #Quipu #LargestStructure #Astronomy #Cosmos #BiggestThingInSpace #DarkMatter #GalaxyClusters #SpaceScience #NASA #Astrophysics #CosmicWeb #ScienceNews #MindBlowing #Intergalactic #BlackHoles #Physics #TimeAndSpace #Superstructure #Galaxies #Universe #Science #Exoplanets #MilkyWay #Astronomers #XrayMapping #SpaceTech #BeyondTheStars #FutureOfSpace #CosmicEvolution …