Phase transition temperatures of 405-725 K in superfluid ultra-dense hydrogen clusters on metal surfaces
Source abstract
Abstract
Ultra-dense hydrogen H(0) with its typical H-H bond distance of 2.3 pm is superfluid at room temperature as expected for quantum fluids. It also shows a Meissner effect at room temperature, which indicates that a transition point to a non-superfluid state should exist above room temperature. This transition point is given by a disappearance of the superfluid long-chain clusters H2N(0). This transition point is now measured for several metal carrier surfaces at 405 - 725 K, using both ultra-dense protium p(0) and deuterium D(0). Clusters of ordinary Rydberg matter H(l) as well as small symmetric clusters H4(0) and H3(0) (which do not give a superfluid or superconductive phase) all still exist on the surface at high temperature. This shows directly that desorption or diffusion processes do not remove the long superfluid H2N(0) clusters. The two ultra-dense forms p(0) and D(0) have different transition temperatures under otherwise identical conditions. The transition point for p(0) is higher in temperature, which is unexpected.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Quantum, superfluid, helium dynamics · Cold Atom Physics and Bose-Einstein Condensates · Advanced Chemical Physics Studies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
University of Gothenburg 1 Atmospheric Science, Department of Chemistry, , SE-412 96 Göteborg, Sweden
Airbus DS 2 , Department Mechanical Engineering, D28199 Bremen, Germany
References (24)
Show source-provided references
1. Nucl. Instr. Meth. B · 2012 · 278 · 3410.1016/j.nimb.2012.01.036 ↗
2. Int. J. Mass Spectrom · 2013 · 351 · 6110.1016/j.ijms.2013.04.006 ↗
3. Int. J. Mass Spectrom. · 2013 · 352 · 110.1016/j.ijms.2013.08.003 ↗
4. Phys. Scripta · 2010 · 81 · 04560110.1088/0031-8949/81/04/045601 ↗
5. Phys. Lett. A · 2011 · 375 · 134410.1016/j.physleta.2011.01.035 ↗
6. J. Supercond. Novel Magn. · 2012 · 25 · 87310.1007/s10948-011-1371-6 ↗
7. J. Cluster Science · 2015 · 26 · 115310.1007/s10876-014-0804-3 ↗
8. Appl. Phys. Lett. · 2010 · 96 · 12410310.1063/1.3371718 ↗
9. Rev. Sci. Instrum. · 2011 · 82 · 01350310.1063/1.3514985 ↗
10. Int. J. Mass Spectrom · 2011 · 304 · 5110.1016/j.ijms.2011.04.001 ↗
11. J. Appl. Phys. · 2012 · 111 · 12350210.1063/1.4729078 ↗
12. 2003
13. Chem. Phys · 1998 · 237 · 1110.1016/S0301-0104(98)00259-6 ↗
14. J. Cluster Sci · 2012 · 23 · 510.1007/s10876-011-0417-z ↗
15. Proc. SPIE · 2006 · 6181 · 61810510.1117/12.675004 ↗
16. Sov. Phys. JETP · 1992 · 75 · 440
17. J. Fusion Energ · 2010 · 29 · 31710.1007/s10894-010-9280-4 ↗
18. Phys. Lett. A · 2010 · 374 · 276610.1016/j.physleta.2010.04.055 ↗
19. J. High Energy Phys · 2011 · 4 · 94
20. Physica C · 2010 · 470 · 63510.1016/j.physc.2010.06.005 ↗
21. Appl. Catal. A · 2001 · 212 · 23910.1016/S0926-860X(00)00849-8 ↗
22. J. Catal · 1992 · 138 · 41310.1016/0021-9517(92)90295-S ↗
23. J. Clust. Sci. · 2012 · 23 · 9510.1007/s10876-011-0387-1 ↗
24. Int. J. Mass Spectrom · 2009 · 282 · 7010.1016/j.ijms.2009.02.014 ↗