Skip to content
DraconiticResearch
Search Sources API
197,768 studies31 sourcesUpdated 12 min ago
PreprintCC BYChemRxiv

Spectral Identification of Hydrino Compound Fe2O3:H2(1/4) by Five Complementary Spectroscopies R. L. Mills and W.R. Hagen

Abstract

Mills solves the hydrogen atom and molecule in exact equations that give the experimental observables of both. Uniquely, Mills predicts that in addition to the reciprocal integer squared excited-state electronic energy states of atomic hydrogen, hydrogen possesses integer squared electronic energy levels corresponding to 1/p replacing n in the Rydberg formula, corresponding so-called hydrino state of hydrogen. Hydrino, H(1/p), is any small form of atomic hydrogen with state energy En = -13.598/n2 eV, in which n = 1/p, and p is limited by the energy in the electric field of the proton to 126 whereafter the proton and electron decay. Electron transitions to a hydrino states involve an initial non-radiative energy transfer to a catalyst that serves as an energy hole or sink of a quantized amount of energy, 2mE1 (m is integer) to be transferred to a catalyst such as HOH, a free or nascent water molecule. Furthermore, hydrino atoms can react to form the corresponding diatomic molecule referred to as molecular hydrino H2(1/p). In contrast to molecular hydrogen (H2), the molecular hydrino (H2(1/p)) is paramagnetic with S = ½, the size is 1/p3 that of H2, the internuclear distance is 1/p that of H2, and the energies such as the rotational, vibrational, and total molecular energies are p2 those of H2. These aspects of H2(1/p) give rise to unique spectral signatures that are characteristic of and identify H2(1/p). The recording of unique gas chromatographic (GC), electron paramagnetic resonance (EPR) spectroscopy, Raman spectroscopy, electron beam excitation spectroscopy, and X-ray photoelectron spectroscopy (XPS) peaks of H2(1/4) formed by a high energy impact reaction of FeOOH that served as the source of H and HOH catalyst are reported wherein the observed peaks matched those predicted.

Related

  1. Detection and Characterization of the Cosmological Neutrino Background by EPR Spectroscopy on Molecular Hydrino with Implications for Telecommunications
    Wilfred R. Hagen, Randell L. Mills
    ChemRxivPreprintCC BYFull textAtomic, molecular & optical physicsChemRxiv
  2. Neural-network-based material identification in photon-counting computed tomography using region-of-interest spectral features
    A. Miadzvetski, V. Rozhkov, R. Sotenskii +2
    arXivPreprintCC BY-NC-ND 4.0Full textApplied physics & instrumentationarXiv
  3. PhaseMatcher: Autoregressive Phase-Set Identification with Spectral Decomposition
    Zhonglong Peng, Qiuliang Liu, Chang Chen +5
    arXivPreprintarXiv licenceFull textCondensed matterarXiv
  4. Online Seakeeping Forecast Coupling System Identification With Nonlinear Pseudo Spectral Potential-Flow
    Zev Hoffman, Sara Vahaji, Micheal Candon +2
    arXivPreprintarXiv licenceFull textFluid dynamicsarXiv
  5. Compound-combination anti-synchronization of chaotic dynamical system with external disturbances
    Vijay K. Shukla, K. Santosh Rupa, Ram Sagar +1
    Scientific ReportsPeer-reviewedCC BY-NC-ND 4.0Full textStatistical & nonlinear physicsCrossref
BibTeX
@misc{hagen2026spectral,
  title = {{Spectral Identification of Hydrino Compound Fe2O3:H2(1/4) by Five Complementary Spectroscopies R. L. Mills and W.R. Hagen}},
  author = {Wilfred R. Hagen},
  howpublished = {ChemRxiv},
  year = {2026},
  month = oct,
  doi = {10.26434/chemrxiv.15010920/v1},
  url = {https://chemrxiv.org/doi/full/10.26434/chemrxiv.15010920/v1},
  note = {CC BY},
}
RIS
TY  - UNPB
TI  - Spectral Identification of Hydrino Compound Fe2O3:H2(1/4) by Five Complementary Spectroscopies R. L. Mills and W.R. Hagen
AU  - Wilfred R. Hagen
PY  - 2026
DA  - 2026/10/22
PB  - ChemRxiv
DO  - 10.26434/chemrxiv.15010920/v1
UR  - https://chemrxiv.org/doi/full/10.26434/chemrxiv.15010920/v1
AB  - Mills solves the hydrogen atom and molecule in exact equations that give the experimental observables of both. Uniquely, Mills predicts that in addition to the reciprocal integer squared excited-state electronic energy states of atomic hydrogen, hydrogen possesses integer squared electronic energy levels corresponding to 1/p replacing n in the Rydberg formula, corresponding so-called hydrino state of hydrogen. Hydrino, H(1/p), is any small form of atomic hydrogen with state energy En = -13.598/n2 eV, in which n = 1/p, and p is limited by the energy in the electric field of the proton to 126 whereafter the proton and electron decay. Electron transitions to a hydrino states involve an initial non-radiative energy transfer to a catalyst that serves as an energy hole or sink of a quantized amount of energy, 2mE1 (m is integer) to be transferred to a catalyst such as HOH, a free or nascent water molecule. Furthermore, hydrino atoms can react to form the corresponding diatomic molecule referred to as molecular hydrino H2(1/p). In contrast to molecular hydrogen (H2), the molecular hydrino (H2(1/p)) is paramagnetic with S = ½, the size is 1/p3 that of H2, the internuclear distance is 1/p that of H2, and the energies such as the rotational, vibrational, and total molecular energies are p2 those of H2. These aspects of H2(1/p) give rise to unique spectral signatures that are characteristic of and identify H2(1/p). The recording of unique gas chromatographic (GC), electron paramagnetic resonance (EPR) spectroscopy, Raman spectroscopy, electron beam excitation spectroscopy, and X-ray photoelectron spectroscopy (XPS) peaks of H2(1/4) formed by a high energy impact reaction of FeOOH that served as the source of H and HOH catalyst are reported wherein the observed peaks matched those predicted.
ER  -