BrainTruffle: Fluid dynamics feels natural once you start with quantum mechanics at https://www.youtube.com/watch?v=MXs_vkc8hpY BrainTruffle, You need to use real measurements, on real systems, to match your different simulation strategies to real things. You are guessing by eyeball. You can get massive amounts of data from a number of places, or your own experiments. A billion
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John Turner: N-Body Simulation with 70,000+ Particles at https://www.youtube.com/watch?v=fSeEg5XwGGo John Turner, I can think of many ways to make this easier for humans to see, to monitor for useful event and situations, to visual new things. First, you are showing position. You can also show velocity and acceleration, you can summarize statistic on changes, you can
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The Action Lab: Magnetic Locking WITHOUT a Superconductor! at https://www.youtube.com/watch?v=V5FyFvgxUhE Fantastic. Now do some measurements, write some equations and write some software so people can plug in what they have and get estimates of what regions will be stable. Or give specifics of separation distance, mass and force, to calculate what speed to use and what
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I managed to save my comment: Wikipedia Survey Coordinators, Analysts, Managers, Board, Stakeholders, I started the survey. When I clicked resume later, it cleared the survey and said I had cookies blocked. It mentioned an email, but would not go back to the email page again. I have been using Wikipedia from the first days.
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https://www.researchgate.net/profile/Antoni-Rogalski I came across this entry for your book on ResearchGate but it does not seem to be connected to your profile. https://www.researchgate.net/publication/343958463_2D_Materials_for_Infrared_and_Terahertz_Detectors I am looking at infrared detector sensitivities to see which might be getting close to where they will pick up gravitational variations. Many new detectors now can pick up what is termed
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Anton Petrov: Whole Universe May Be Evaporating According To New Study at https://www.youtube.com/watch?v=vEAKbL04bxQ Anton Petrov, I think you ought to focus on the life of any star. The matter concentrates into stars, reaches critical density to ignite nuclear reactions, and then, for the rest of the stars life, it will be radiating neutrinos, photons, electrons, protons
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The Action Lab: Quantum Locking Will Blow Your Mind—How Does it Work? at https://www.youtube.com/watch?v=8GY4m022tgo I am fairly certain that the “fluid” you are stirring with no internal friction, is the gravitational potential field itself. A super critical fluid made up of magnetically bound pairs much smaller than the electron. At the surface of the earth the
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The Action Lab: What Does The Strong Nuclear Force Look Like? at https://www.youtube.com/watch?v=Rx4lNihOT4U The simplest easy model for the strong force that I found is to simply calculate the magnetic dipole force between the particles. Electrons protons neutrons each have permanent magnetic dipole moments in units of Joules/Tesla. To get the force in Newtons multiply the
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Susumu Komiyama, I was looking for your paper, “Electron temperature of hot spots in quantum Hall conductors” and found this THz imaging paper on ResearchGate. I think at zero temperature the magnetic energy density and its gradients are important. “hot spots” are just part of it. I was looking at ways to push the fields
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APS Physics: Large-scale Scientific Facilities and Diplomacy at https://www.youtube.com/watch?v=qtKEWt-WuCo Laura Greene, I have been studying (looking for ways to create and maintain) high magnetic fields (over 400 Tesla) for more than 50 years now. Every few years I check to see what MagLab has been doing, but the website always seems a bit chaotic and incomplete.
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