http://wiki.naturalphilosophy.org/index.php?title=Cosmology_and_Quantum_Mechanical_Unstable_States_for_Helium&feed=atom&action=historyCosmology and Quantum Mechanical Unstable States for Helium - Revision history2024-03-29T02:39:37ZRevision history for this page on the wikiMediaWiki 1.34.0http://wiki.naturalphilosophy.org/index.php?title=Cosmology_and_Quantum_Mechanical_Unstable_States_for_Helium&diff=23219&oldid=prevMaintenance script: Imported from text file2017-01-02T02:25:21Z<p>Imported from text file</p>
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<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Precise values are provided for the magnitude of the redshift associated with the helium atom for temporarily absorbed Hd, Fe XIV, NaD , and Ha photons, more details are given regarding the emission wavelengths of the two spin reversal photons that carry away the energy lost by the redshifted photon, and a crude time sequence of pertinent atomic events is suggested. When an Fe XIV photon is fleetingly absorbed with a wavelength of 5,302.30 Angstroms, one spin-reversal photon is emitted with a wavelength of 617,877 Angstroms and the other with 1,040,189. Angstroms. The redshifted photon is emitted with a wavelength of 5,375.84 Angstroms. The amount of the redshift for each single absorption and emission is 0.01387. The redshift per interaction is found to vary by wavelength. This is to be expected.[[Category:Scientific Paper]]</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Precise values are provided for the magnitude of the redshift associated with the helium atom for temporarily absorbed Hd, Fe XIV, NaD , and Ha photons, more details are given regarding the emission wavelengths of the two spin reversal photons that carry away the energy lost by the redshifted photon, and a crude time sequence of pertinent atomic events is suggested. When an Fe XIV photon is fleetingly absorbed with a wavelength of 5,302.30 Angstroms, one spin-reversal photon is emitted with a wavelength of 617,877 Angstroms and the other with 1,040,189. Angstroms. The redshifted photon is emitted with a wavelength of 5,375.84 Angstroms. The amount of the redshift for each single absorption and emission is 0.01387. The redshift per interaction is found to vary by wavelength. This is to be expected.</div></td></tr>
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<p><b>New page</b></p><div>{{Infobox paper<br />
| title = Cosmology and Quantum Mechanical Unstable States for Helium<br />
| url = [http://www.naturalphilosophy.org/pdf/abstracts/abstracts_583.pdf Link to paper]<br />
| author = [[Donald G Carpenter]]<br />
| keywords = [[redshift]], [[helium atom]], [[wavelength]]<br />
| published = 1994<br />
| journal = [[Apeiron]]<br />
| volume = [[1]]<br />
| number = [[20]]<br />
| num_pages = 3<br />
| pages = 14-16<br />
}}<br />
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'''Read the full paper''' [http://www.naturalphilosophy.org/pdf/abstracts/abstracts_583.pdf here]<br />
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==Abstract==<br />
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Precise values are provided for the magnitude of the redshift associated with the helium atom for temporarily absorbed Hd, Fe XIV, NaD , and Ha photons, more details are given regarding the emission wavelengths of the two spin reversal photons that carry away the energy lost by the redshifted photon, and a crude time sequence of pertinent atomic events is suggested. When an Fe XIV photon is fleetingly absorbed with a wavelength of 5,302.30 Angstroms, one spin-reversal photon is emitted with a wavelength of 617,877 Angstroms and the other with 1,040,189. Angstroms. The redshifted photon is emitted with a wavelength of 5,375.84 Angstroms. The amount of the redshift for each single absorption and emission is 0.01387. The redshift per interaction is found to vary by wavelength. This is to be expected.[[Category:Scientific Paper]]<br />
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[[Category:Cosmology]]</div>Maintenance script