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| Autore principale: | |
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| Natura: | Recurso digital |
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Zenodo
2025
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| Accesso online: | https://doi.org/10.5281/zenodo.16935625 |
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Sommario:
- <p>OBSOLETE-Dark Matter is something else, it doesn't exists in this form (check Neutrofield)</p> <p>HSF: Dark-Matter Frequency Field (short description)</p> <p>For everyone: we look for a tiny, fixed "twin echo" beside any stable tone in<br>existing recordings; if it’s there, we read off the dark-matter mass and how<br>strongly it couples; if it’s not, we set strong limits.</p> <p>A global, instrument-agnostic prediction: if DM is a frequency field, any stable<br>spectral line shows symmetric sidebands at fixed +/- fDM. Three easy checks on<br>existing data: (1) offset stays under carrier tuning, (2) + and - are equal,<br>(3) channel ratios (ec:plasma ~ 2:1). One OK/NO test yields mphi = h*fDM and a<br>coupling g (or limits). Send 10-60 s baseband around one line; we return a quick<br>yes/no and a g(m) curve.</p>