التفاصيل البيبلوغرافية
| العنوان: |
Meissner Effect in Ultra-Dense Protium p(l=0, s=2) at Room Temperature: Superconductivity in Large Clusters of Spin-Based Matter |
| المؤلفون: |
Holmlid, Leif, 1942, Fuelling, S. |
| المصدر: |
Journal of Cluster Science. 26(4):1153-1170 |
| مصطلحات موضوعية: |
Inorganic Chemistry, Oorganisk kemi, Ultra-dense protium, Superconductor, Coulomb explosion, Magnetic field, RYDBERG MATTER, COULOMB EXPLOSIONS, DEUTERIUM, CATALYST, SPECTRA, SURFACE, STYRENE, PHASE, N=4, Chemistry, Inorganic & Nuclear |
| الوصف: |
Ultra-dense protium p(l = 0) is superfluid at room temperature, as is its more often studied deuterium counterpart D(l = 0). p(l = 0) can be deposited on surfaces by a source which produces a stream of clusters. A magnetic field strongly influences the type of clusters formed. Very little of chain clusters of p(l = 0) and the closely related form p(l = 1) exists on the magnet surface or within 0.5 mm from the magnet surface. The removal of the p(l = 0) and p(l = 1) entity in strong magnetic fields is due to a Meissner effect as in the case of D(l = 0). Contrary to the case of D(l = 0), small symmetric p(l = 0) clusters formed by 3 and 4 hydrogen atoms are not left on the magnet pole face when the large chain-clusters lift in the magnetic field. Symmetric p(4)(l = 0) clusters are unlikely since four fermions cannot interact in this way. Instead, p(2) pairs are included as bosons in the chain cluster structure as observed previously. |
| URL الوصول: |
https://gup.ub.gu.se/publication/220223 |
| قاعدة البيانات: |
SwePub |