Classical energy calculations with electron correlation of condensed excited states — Rydberg Matter

Fuelling

2011

J Supercond Nov Magn

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Ultra-dense deuterium D(−1) is expected to be both a superfluid and a superconductor as shown by recent theoretical research. Condensed D(−1) can be deposited on surfaces by a source which produces a stream of clusters. A magnetic field strongly influences the type of material formed. Very little of D(−1) and of the form D(1), which is strongly coupled to D(−1), exists on the magnet surface or within several mm from the magnet surface. Even the formation of D(−1) on the source emitter is strongly influenced by a magnetic field, with a critical field strength in the range 0.03-0.07 T. Higher excitation levels D(2) and D(3) dominate in a magnetic field. The excitation level D(2) is now observed for the first time. The removal of D(−1) and D(1) in strong magnetic fields is proposed to be due to a Meissner effect in long D(−1) clusters by large-orbit electron motion. The lifting of long D(−1) clusters above the magnet surface is slightly larger than expected, possibly due to the coupling to D(1). The previously reported oscillation between D(−1) and D(1) in an electric field is proposed to be due to destruction of D(−1).

Section: Theorymentioning

confidence: 99%

Section: Theorymentioning

confidence: 99%

Search for Superconductivity in Ultra-dense Deuterium D(−1) at Room Temperature: Depletion of D(−1) at Field Strength >0.05 T

Andersson

Fuelling

2011

J Supercond Nov Magn

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“…A correct time-dependent quantum mechanical description, of course, provides the best model, but it is probably necessary to use a pilot-wave description 28 to correctly understand the system at the classical limit. 6 The electrons in the conduction band in the finite RM clusters have excited states giving transitions in the same energy range as the possible nuclear vibrations. This is a further clear indication that the motions of the electrons and nuclei cannot be easily separated.…”

Section: Motionsmentioning

confidence: 99%

Vibrational transitions in Rydberg matter clusters from stimulated Raman and Rabi‐flopping phase delay in the infrared

2008

J Raman Spectroscopy

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Recently, rotational spectra of giant Rydberg matter (RM) clusters were studied in the radio frequency range (Mol. Phys. 105 (2007) 933-939), giving high-precision bond distances in the nanometer range. However, the theoretical and experimental problem of vibrational motion or, rather, coupled electronicvibrational motion in the RM clusters is still unsolved; but it is expected that broad phonon bands will exist. Spectroscopic signatures from space make it likely that RM is a common form of matter in the Universe, and phonon bands in this spectroscopic range have not been taken into account so far. Spectroscopic results are now reported on transitions in the range 0.01-20 cm −1 , using primarily infrared (IR) lasers to probe the RM in a tunable open cavity with a Fabry-Perot interferometer to aid in the identification of the shifts. Stimulated Raman scattering from electronic transitions and Rabi-flopping from electronic states in the clusters are observed. The broad stimulated Raman peaks are assigned to one and two consecutive vibrational (electronic-vibrational) transitions. Theoretical values predicted for vibrations (phonon maxima) and electronic processes are in reasonable agreement with the experimental results. Improved calculations are needed to verify the assignments of the vibrational phonon distributions.

“…3 The Bohr radius is indicated as a 0 . Here, 2.9 is a scaling constant determined numerically for ordinary Rydberg matter 26 and confirmed experimentally for ordinary Rydberg matter by radio frequency spectroscopy.…”

Section: Theorymentioning

confidence: 52%

Leptons from decay of mesons in the laser-induced particle pulse from ultra-dense protium p(0)

2016

Int. J. Mod. Phys. E

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Kaons and pions are observed by their characteristic decay times of 12, 52 and 26 ns after impact of relatively weak ns-long laser pulses on ultra-dense hydrogen H(0), as reported previously. The signal using an ultra-dense protium p(0) generator with natural hydrogen is now studied. Deflection in a weak magnetic field or penetration through metal foils cannot distinguish between the types of decaying mesons. The signals observed are thus not caused by the decaying mesons themselves, but by the fast particles often at > 50 MeV u −1 formed in their decay. The fast particles are concluded to be mainly muons from their relatively small magnetic deflection and strong penetration. This is further supported by published studies on the direct observation of the beta decay of muons in scintillators and solid converters using the same type of p(0) generator.