For decades, neutrinos have been introduced with essentially the same sentence: they pass through matter almost without interacting. True. But "almost" is a remarkably important word in physics. XENONnT has now pushed real-time solar-neutrino spectroscopy down to energies of about 17 keV — opening an experimental window that, until recently, remained beyond reach.
| # | Наименование новости | Тональность | Информативность | Дата публикации |
|---|---|---|---|---|
| 1 | 17 keV. Das Wort „unmöglich“ ist gerade kleiner geworden. | 0 | 11.87 | 25-09-2026 |
| 2 | When the Invisible Becomes Measurable | 0 | 7.35 | 15-09-2026 |
| 3 | Neutrinos and the Case for an Infinite, Overlooked Energy Source | 0 | 7.77 | 09-08-2026 |
| 4 | What Happens When a Solar Neutrino Hits Matter? | 0 | 8.26 | 24-09-2026 |
| 5 | From Elusive Signal to Precision Measurement | 0 | 6.4 | 23-09-2026 |
| 6 | Solar Neutrino Constraints on Inelastic Dark Matter Scattering in Light of Recent LUX-ZEPLIN Observations | 0 | 11.19 | 12-09-2026 |
| 7 | How Neutrino Oscillation Teaches Us Energy Is Never Lost | 0 | 10.02 | 30-07-2026 |
| 8 | What the World's Most Sensitive Neutrino Experiment Tells Us About the Next Fifty Years of Energy | 0 | 8.77 | 19-08-2026 |
| 9 | Neutrino transition magnetic moments within the non-standard neutrino-nucleus interactions | 0 | 11.72 | 25-08-2026 |
| 10 | From Detecting Neutrinos to Designing Matter That Responds | 0 | 10.75 | 06-08-2026 |