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Thanks for that, I wondered if it had been confirmed. I am always in awe of folks who come into the lab every day and work on figuring out the one thing. I envy that level of focus. |
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As I understand it, that is not an independent discovery but rather replication/confirmation of the results described in the original 14th of March paper by PTB & TU Wien.
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I'm talking about the blackbody radiation of the sun's surface, which accounts for almost all of the light. The X-ray flux at earth is 11 orders of magnitude lower than the blackbody-related flux.
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> suspect the average football field size across the former British Empire is close to the FIFA standard. The FIFA standard (https://downloads.theifab.com/downloads/laws-of-the-game-202...) leaves a lot of leeway: “3. Dimensions The touchline must be longer than the goal line. • Length (touchline): minimum 90 m (100 yds), maximum 120m (130 yds) • Length (goal line): minimum 45 m (50 yds), maximum 90m (100 yds)” So, a field can be almost square at 90m × 89m or approaching thrice as long as wide, at 120m × 45m. Reason for this is prior art that can be hard to change (if there’s a stadium around your field, and it’s deemed too small, you’d have to demolish it to make the field fit the standard) Various competitions restrict this, though. |
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148 doesn't feel too far removed from the visible spectrum, but it's in the wrong direction for animals to make use of it. I'm no biologist, but I'd be shocked if there were any animals that had adapted sensitivity to a type of radiation that they are never exposed to in nature. The sun doesn't really emit much UV-C light: https://en.wikipedia.org/wiki/Solar_irradiance#Absorption_an... and the light that is emitted is absorbed by the atmosphere: https://en.wikipedia.org/wiki/Ultraviolet#Solar_ultraviolet It's useful to be able to see a little UV-A, perhaps, and very useful for predators to see 'heat' into the IR range, but if your eyes were sensitive to 148nm, the world would be pretty dark. Maybe after a few million years, in the grinding dust in the back of my shop, something will evolve that has a symbiotic relationship to arc welders... |
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A long time ago I saw some UV photos of flowers, compared to visible and IR. There were some distinct features. That suggests some insects could see them, but of course it's just speculation.
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For comparison, over the last several years there has been a lot of research into optical frequency standards. Because they run at a higher frequency than (microwave) caesium frequency standards, optical frequency standards can be more precise. The current candidates https://iopscience.iop.org/article/10.1088/1681-7575/ad17d2 have wavelengths between 750nm and 250nm. Caesium frequency standards use a wavelength of 32.6mm, so about 100,000x bigger than optical frequency standards. Based on just the frequency, I dunno what makes the thorium nuclear transition much better than optical transitions. Unless the excitement (as it were) is about scaling up to even higher frequencies. |
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The key factor is the line width, or the range of frequencies over which the transition can be stimulated. The ratio of the stimulus frequency and line width is one way of expressing the resonator Q factor. In general, the lower the line width for a given transition, the higher the Q, the better the signal-to-noise ratio, and the more stable the resulting clock. (Imagine how much more precisely the frequency of a large bell could be measured compared to a cymbal or something else with a broader acoustical spectrum.) Cs or Rb clocks give you a line width of a few hundred Hz at 9 GHz (Q=roughly 100 million), while quantum transitions in optical clocks can achieve line widths on the order of 1 Hz in the PHz region (equivalent Q in the quintillions.) There is a lot more to building a good clock than high Q, but it's a very important consideration ( http://www.leapsecond.com/pages/Q/ ). What caught my eye is the ringdown time of the stimulated optical resonance, apparently in the hundreds of seconds. They talk about line widths in the GHz range, but that seems to refer to the laser rather than the underlying resonance being probed. It would have been interesting to hear more about what they expected regarding the actual transition line width. Probably the information is there but not in a form that I grokked, given insufficient background in that field. |
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The Q of nuclear transitions is just insane (as reflected by their long half life, something in excess of 1700 seconds here for free atoms.) The uncertainty relationship is normally written as delta-p delta-x > hbar/2, but it can also be written as delta-t delta-E > hbar/2. So, if the half life is very long, delta-E can be very small. This fact is used in Mössbauer spectroscopy (recoilless gamma emission in solids). The peak is so sharp that it was famously used by Pound and Rebka to detect the gravitational red shift in the lab at Harvard in 1960, reaching 1% accuracy by 1964. https://en.wikipedia.org/wiki/Pound%E2%80%93Rebka_experiment |
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For free atoms, yes. For atoms in a crystal lattice (or other solid), it's quite common for electrons to decay through phonon interactions, i.e. by emitting vibrations (i.e. heat) to the lattice.
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Actually the method of detecting mineral deposits by mapping gravitational field is already in use since a long time! The Eotvos pendulum (an instrument aka. Eotvos torsion balance) designed in 1888 started this kind of measurement. It was used commonly by the 1920s by geophysicist for mapping underground deposits by measuring the gradient of the gravitational field very precisely. This instrument was deprecated later by even better tools for surveying. The instrument was initially constructed for the experiment showing that inertial and gravitational mass are the same (well, linearly correlated) to a great precision: https://en.wikipedia.org/wiki/E%C3%B6tv%C3%B6s_experiment https://www.nature.com/articles/118406a0 (pretty useless link, but a famed periodical) Detecting submarines is way harder, practically impossible. as others have already pointed out. |
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Does the average density of most submarines approaching the density of water make that more difficult? Are you looking for density variation between the parts and airspaces of a submarine? |
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No time to elaborate at the moment. Just want to say that this is extremely exciting news. Finding the thorium line is one of the most important open problems in precision/fundamental measurement. |
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My high school physics class flashes back to me, I don't think I understand a fraction of it but it seems very exciting (pun intended). I was reading up on this (now outdated) wiki page: https://en.wikipedia.org/wiki/Isotopes_of_thorium#Thorium-22... And it mentions the application as qubit for quantum computers. If the state change is relatively simple, cheap and stable, what could this do for quantum computing? I picture a crystalline processor holding Thorium nuclei as the brains of a new supercomputer? Would that be viable? |
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Special vs general. Quantum field theory is special relativistic and quantum mechanical. The grand unified theory stuff is about uniting general relativity and quantum mechanics.
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There is a big difference between "classical" quantum mechanics (about 100 years old now!) and quantum field theory (~50 years old). Maybe that's what they mean?
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Man, Vienna is killing it in physics. Nobel in 2022 for Zeilinger Nobel in 2023 for Kraus, who did his work at TU Wien Now this. Giving a lot of other unis a run for their money. |
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Probably just emits another photon of the exact same wavelength a short time later. The time would be probabilistic, like 50% chance of emission in X amount of time.
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Thorium-229 has two energy states. A ground state, and an excited isometric state. The laser is used to transition the nucleus from the ground state to the excited isometric state. |
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25 years ago, there were experiments to move element 72 hafnium (Hf) between its low and excited isomer states, which would allow for the creation of a nuclear battery that could store 100,000 times more energy than a chemical battery, with a 31 year half life, but without neutron release: https://en.wikipedia.org/wiki/Hafnium_controversy This would be Iron Man and Star Wars tech if it worked. Unfortunately experiments went dark after 2009, probably because it worked haha, but maybe because Hf is too rare to make a practical battery. So it looks like they tried spalling element 73 Tantalum (Ta), 74 Tungsten (W) and 75 Rhenium (Re) with protons at 90-650 MeV to create 72 Hf with atomic masses 178, 179 and high spin 178m2, 179m2 isomers if I read this right: https://publications.jinr.ru/record/151982/files/071%28E6-20... https://apps.dtic.mil/sti/tr/pdf/ADA525435.pdf There's a lot here though, so I can't really get a clear picture of what the yields are, or simply how many joules it takes to store one joule in an excited isomer. Which is of course all that matters, but papers often leave off the one part we're curious about, forcing us to learn nearly the entirety of the subject matter to derive it ourselves. Although on the bright side, maybe that protects us from nuclear armageddon and stuff. Maybe someone can fill us in? Edit: dangit _Microft beat me by 17 minutes, please answer there :-) |
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We know how to do this and have observed this tons of times at this point. This would not be novel in any way. This is about exciting the nucleus which is completely different.
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For example, the Earth's gravitational field could be analyzed so precisely that it could provide indications of mineral resources Resources companies are salivating |
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It wouldn't be precise enough to measure things like what type of rock you have underneath when you're thinking about digging a tunnel or to find land mines in dirt right?
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I >think< that this will enable more accurate magnetometers (see OPM-MEG and atomic clock magnetometers). Which can be used, among other things, for measuring neuronal activity.
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Not a physicist, so I am asking out of curiosity and to learn: have the limitations to the precision of current atomic clocks posed any problems?
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If I remember correctly GPS is effected but the ultra precise version the gov uses can error correct pretty well. I would think greater GPS precision at a lower cost?
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> PS: Are you sure it's gamma emission? That takes more energy than the exciting UV photon. Apparently it is neither: Decay of the 229Th isomeric state of the neutral thorium atom occurs predominantly by internal conversion (IC) with emission of an electron https://www.nature.com/articles/nature17669 https://en.wikipedia.org/wiki/Internal_conversion This is pretty weird. You shine UV light (with exactly the right wavelength) on 229Th, and it spits out electrons. But not like the photoelectric effect, where the electrons stop as soon as you turn off the light. No no. The Thorium keeps spitting out an exponentially-decaying stream of electrons for hours after you stop illuminating it. Almost like an exponentially-discharging solar-powered current source (for a very specific wavelength of "solar"). |
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What i was wondering…exactly… how do you make this kind of a laser? And imagine an xray laser… you could fry the guidance system of drone very precisely
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This is important since impurities in the crystals used lead to all kinds of fluorescence that could be mistaken for a signal from the Thorium ions. Now two groups have seen exactly the same signal in different Thorium-doped crystals which is very covincing that they have found the actual nuclear transition.