Spectroscopic observation of helium-ion- and hydrogen-catalyzed hydrino transitions

Abstract

Abstract:Four predictions of Mills' Grand Unified Theory of Classical Physics (GUTCP) regarding atomic hydrogen undergoing a catalytic reaction with certain atomized elements and ions which resonantly, nonradiatively accept integer multiples of the potential energy of atomic hydrogen, · 27.2 eV wherein is an integer, have been confirmed experimentally. Specifically, a catalyst comprises a chemical or physical process with an enthalpy change equal to an integer multiple of the potential energy of atomic hydrogen, 27.2 eV. For He + = 2, due to its ionization reaction to He 2+ , and two H atoms formed from H 2 by collision with a third, hot H can also act as a catalyst with = 2 for this third H. The product is H(1/ ), fractional Rydberg states of atomic hydrogen called "hydrino atoms" wherein = 1/2, 1/3, 1/4,…, 1/ ( 137 is an integer) replaces the well-known parameter = integer in the Rydberg equation for hydrogen excited states. The predictions for the hydrino reaction of (1) pumping of the catalyst excited states, (2) characteristic EUV continuum radiation, (3) fast H, and (4) hydrino products were observed in multiple catalyst-hydrogen plasma systems. PACS

Mechanism of soft x-ray continuum radiation from low-energy pinch discharges of hydrogen and ultra-low field ignition of solid fuels

“…The flux of 635 Å radiation required to produce hydrogen ionization is given by z s z = =ĺ - catalyst giving rise to a concerted energy exchange of the total energy of 40.8 eV with the excitation of the He 1s 2 -1s 1 2p 1 transition. The predicted 63.3 nm emission associated with dark matter was observed with the addition of hydrogen to helium microwave plasma as shown previously [3,29]. An alternative assignment suggested by Labov and Bowyer [59] is the 63.0 nm line of O V requiring a large-scale non-thermal source of ionization.…”

“…Our EUV continuum results offer resolution to many otherwise inexplicable celestial observations with (a) the energy and radiation from the hydrino transitions being the source of extraordinary temperatures and power regarding the solar corona problem, the cause of sunspots and other solar activity, and why the Sun emits x-rays [3], (b) the hydrino-transition radiation being the radiation source heating the WHIM and behind the observation that diffuse Hα emission is ubiquitous throughout the Galaxy requiring widespread sources of flux shortward of 912 Å, and (c) the identity of dark matter being hydrinos.…”

“…The possibility of a revolutionary discovery of a new source of energy in the Sun based on a prior undiscovered process is an open question [56]. That mH catalyzed hydrino transitions occur in stars and the Sun [57] as evident by corresponding continua in its spectrum resolves the solar corona problem, the cause of sunspots and other solar activity, and why the Sun emits x-rays [3].…”

“…By the same mechanism, the nascent H 2 O molecule (not hydrogen bonded in solid, liquid, or gaseous state) may serve as a catalyst by accepting 81.6 eV (m = 3) to form an intermediate that decays with the emission of a continuum band with a short wavelength cutoff of 10.1 nm and energy of 122.4 eV [1]. The continuum radiation band at 10.1 nm and going to longer wavelengths for theoretically predicted transitions of H to lower-energy, so called 'hydrino' state H(1/4), was observed only arising from pulsed pinch gas discharges comprising some hydrogen first at BlackLight Power, Inc. (BLP) and reproduced at the Harvard Center for Astrophysics (CfA) by Cheimets and Daigneau [2][3][4][5][6].…”

Soft X-ray continuum radiation from low-energy pinch discharges of hydrogen

“…EUV pinch plasma spectra Spectra of discharges in high purity helium were measured as reference for validation of the continuum-free spectra in absence of hydrogen in a manner similar to that of BLP (Mills andLu 2010, 2011;Mills et al 2010b). EUV pinch plasma spectra Spectra of discharges in high purity helium were measured as reference for validation of the continuum-free spectra in absence of hydrogen in a manner similar to that of BLP (Mills andLu 2010, 2011;Mills et al 2010b).…”