Physics
Scientific paper
May 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..aprv13012g&link_type=abstract
American Physical Society, April Meeting, 2004, May 1-4, 2004, Denver, Colorado April 2004, MEETING ID: APR04, abstract #V13.012
Physics
Scientific paper
Observations of Redshifts from Type 1A Supernovae have led to speculations about "Dark Energy". But this Supernova Redshift data is obtained only for a limited range of the variables: (1) Distance, (2) Wavelength Range, (3)Neutrino vs Photon Arrival Times. (1) Data is presented only for very distant Supernovae. Data is also needed at closer distances to compare with Galaxies on an extended Hubble diagram. (2) Data are presented only for a small wavelength range in the UV/visible. Data is critically needed at lower photon energies, especially the H:21cm line if possible. This data is critical since there are several non-Doppler redshift mechanisms (Wolf, Raman, CREIL, etc) that yield smaller redshifts (or even blueshifts) at these low energies. (3) Data is needed on the neutrino vs photon arrival-times over very large distance and wavelength ranges, again related to non-Doppler redshift mechanisms. Conclusion: For Supernova 1A Redshifts, extensive examination must be made of all possible NON-Doppler (or Non-Space-Expansion) redshift mechanisms which may be active. Without these data and critical examinations, Supernova 1A Redshifts and their interpretation are highly speculative.
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