The 37th European Conference on Laser Interaction with Matter (ECLIM 2024), held from September 16–20, organised by IPFN's Group of Lasers and Plasmas (GoLP), gathered more than 150 participants from 15 countries, including scientists working on physics of laser-matter interaction, laser fusion, plasmas and particle acceleration. Find out more: 🔗https://lnkd.in/dQ723pUz 📸 Check out some highlights from the event: #ipfn #eclim #conference
IPFN - Instituto de Plasmas e Fusão Nuclear’s Post
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🗞 Hot off the press: Our Interim report marks an important step in defining the input on the chapter about muon colliders in the upcoming European Strategy for Particle Physics' Accelerator R&D Roadmap and highlights our progress towards the Muon Collider since 2020 and what we expect to achieve by 2026! Read everything here: https://lnkd.in/dqi5yaKE
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"It is true, that whenever ordinary light strikes an object, the collision gives rise to a small force on the object. This force is called radiation pressure." Read the article 'The Pressure of Laser Light', published #OTD in 1972 by physicist Arthur Ashkin. Ashkin was awarded the 2018 physics prize “for the optical tweezers and their application to biological systems." At the time of the award, he was 96 years old. The whole article is available here: https://bit.ly/2Gbhrta
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The NA62 experiment at CERN has observed the decay of a charged kaon into a charged pion and a neutrino-antineutrino pair! This decay is one of the rarest processes ever observed in the so-called flavor physics: according to the Standard Model, fewer than one in 10 billion charged kaons decay into these particles! Check out this article by INFN explaining all the details about the event here: https://lnkd.in/d4VaHeNJ #cern #infn #rarity #standardmodel #experiment
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Yesterday, we finished a bit more than a standard beamtime. Did you know that ReMade@ARI can support your research in Circular Economy at every stage from materials' manufacturing to advanced characterization at neutron and synchrotron sources? In this project, I was honored to collaborate with Helmholtz-Zentrum Dresden-Rossendorf (HZDR) where the ion beam modification of GaAs substrates was made with subsequent deposition of metal and metal-oxide active layers. A dedicated operando cell designed at PSI Paul Scherrer Institut allowed us to perform XAS experiment in grazing incidence geometry at DESY. Complementary AFM and STEM measurements are also provided in frame of ReMade project. By the way, today is the deadline for Call IV of ReMade@ARI. Next call opens in spring 2025. One proposal = complete investigation. #catalysis #circulareconomy #ionbeam #beamtime #xrays #synchrotron
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The precise measurement of the W boson’s mass is a significant milestone in particle physics. By connecting it to the three laws of Noah’s Ark Technology, we can envision a deeper understanding of universal symmetry, the connections between time and space, and the unification of fundamental forces, especially in extreme environments like those observed in LHC collisions. This approach paves the way for new ways to explore the very foundations of the universe, an objective at the heart of Noah’s Ark Technology.
The CMS Collaboration weighs in on the W boson mass Yesterday, the collaboration has reported how it has analysed proton–proton collision data from the second run of the Large Hadron Collider (#LHC), to make its first mass measurement of the #Wboson. In this video, Piotr explains why this matters. The result is the most precise measurement of the W mass made so far at the LHC, and is in line with the prediction from the #StandardModel of particle physics. Find out more: https://lnkd.in/ezR3rtht
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Associate professor in computational astrophysics. 4th Mexican scholar to obtain tenure in astronomy/astrophysics in the United States. Exploring more research-heavy opportunities. jorgemoreno.org
It’s paper day. Our new FIREbox-HR simulation explains the elevated UV luminosity density seen by JWST. With FIRE physics, we predict a non-evolving, weakly-mass dependent star formation efficiency, alleviating the need to invoke weird baryonic physics or non-LCDM cosmology. 🔥 📦 🌌 https://lnkd.in/eTDxB5Wi
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For Multipactor Aficionados, Just wanted to share our recent exciting discoveries in multipactor prediction and mitigation, now published in Physics of Plasmas. Building upon our in-house developed model, we've predicted a slightly different picture of multipactor susceptibility zones. The multipactor zones can extend into much higher frequency-gap distance regions, suggesting the feasibility of fast, millimeter-wave multipactor occurrences within reasonable gap distances (e.g., 3 mm). Looking forward to a champion that can experimentally validate these results. 😃 Additionally, we've discussed other intriguing facts, such as the overlap between different order multipactor zones and the intricate dependency of multipactor thresholds on both secondary electron yield crossover points. https://lnkd.in/g95wt8AK #Multipactor #AFOSR #satellitecommunications #PlasmaPhysics
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Our contributions this week at #ECCOMAS2024 in Lisbon include several interesting methods and applications: Adaptively Tuned High-Order Methods for iLES by Xesus Nogueira, Lin Fu 傅林 Adaptive Viscosity Methods for Turbulent Compressible Flow Computations by Xesus Nogueira, Luis Ramirez, Javier Fernández Fidalgo Automated Flow Physics Identification and Classification in Multiphysics Multifidelity Simulations by Ahmed Al-Faisal Sheikh Al-Shabab, Paulo Strobel Silva, Martin Skote Comparative Study of Orifice Shapes on Shock Absorber: Impact on Energy Dissipation and Cavitation by Paulo Strobel Silva, Ahmed Al-Faisal Sheikh Al-Shabab, Martin Skote #turbulence #hpc #CFD #multiphysics #cavitation
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📃Scientific paper: Gravitational Wave Symphony from Oscillating Spectator Scalar Fields Abstract: We investigate a generic source of stochastic gravitational wave background (SGWB) due to the parametric resonance of oscillating scalar fields in the early Universe. By systematically analyzing simple benchmark models using lattice simulation and considering a wide range of parameter space, we demonstrate that such a scenario can lead to detectable signals in GW detectors over a broad frequency range and potentially address the recent finding by NANOGrav. Furthermore, these models are found to naturally yield ultra-light dark matter candidates or dark radiation detectable by CMB observatories. ;Comment: 11 pages, 2 figures Continued on ES/IODE ➡️ https://etcse.fr/F5K ------- If you find this interesting, feel free to follow, comment and share. We need your help to enhance our visibility, so that our platform continues to serve you.
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𝗦𝗖𝗖𝗜𝗝 𝗡𝗲𝘄𝘀: "𝗥𝗼𝗯𝗼𝗱𝗼𝗴 𝗽𝗮𝘁𝗿𝗼𝗹𝘀 𝘁𝗵𝗲 𝗖𝗘𝗥𝗡 𝗹𝗮𝗯𝗼𝗿𝗮𝘁𝗼𝗿𝘆 𝗶𝗻 𝗚𝗲𝗻𝗲𝘃𝗮 " 𝘍𝘶𝘭𝘭 𝘢𝘳𝘵𝘪𝘤𝘭𝘦: https://rb.gy/l1geu9 The largest particle physics laboratory in the world in Geneva, known as CERN, has introduced a four-legged #robodog to run #radiation protection tests. This step aims to improve safeguarding the expansive experimental spaces.
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