The Holmlid paper is a smoking gun for the mechanism of spin coupling in a coherent system that has been sought for some time.
The paper suggests ultra-dense clusters—small vortex rod like clusters of molecular of P, D and T are possible. Holmlid calls this H(-1) which can exist in 3 spin separate spin states with the spin 2 state being most stable. Holmlid suggests that the dense state H(-1) can oscillate with the H(1) state (a Rydberg hydrogen state) not the same as normal molecular hydrogen, which is identified as H2. Holmlid identifies normal molecular hydrogen with a nuclear separation of 74 pm, compared to the Rydberg state H(1) with a nuclear separation of 150 pm and the ultra dense state H(-1) with a nuclear separation of 2.3 pm. Holmlid does not refer to normal molecular hydrogen as H(0) as best I can tell from reading his paper. I would think that normal molecular hydrogen could have more than one orbital spin state for its two electrons. Thus, a notation of H(0) would not be correct for some normal hydrogen. It would seem to be a small step to reach a more stable state than the H(-1), say He, with a transfer of energy to the rest of the coherent system via the phase transitions and their respective spin energy states. Holmlid even goes so far to suggest that spin may not be conserved in rapid transitions. (I doubt that conjecture.) In the case of ultra dense p molecules, D may form before the He finds itself possible. Bob Cook From: Jones Beene Sent: Thursday, November 05, 2015 8:43 PM To: vortex-l@eskimo.com Subject: RE: [Vo]:Re: Evidence for ultra-dense deuterium It’s very difficult to keep the terminology consistent. I think Holmlid would be wise to ditch the present designations and start over. From: Mark Juric FYI: All, please take a close look at Fig. 2 of this Holmlid Paper: http://fuelrfuture.com/science/holm2.pdf I think it will help explain how Holmlid had viewed/grasped the energy levels back in early 2014. Also keep in mind that H(-1) is now called H(0). It was thought that the apparent Ultra-dense state was Inverted Rydberg Hydrogen (IRH, hence the “-1”), but now this state is seen as somewhat different. The “0” reflects that the orbital angular momentum of the electrons is zero. The picture in Fig 1 may need some modification to take into account the various apparent spin states of H(0). Winterberg’s earlier description has slightly fallen out of favor in regards to more recent data, but I am not sure what the latest findings suggest. Reading more of literature should help clear up the current understanding of H(0). Mark Jurich
