63 research outputs found
Spectrometric method to detect exoplanets as another test to verify the invariance of the velocity of light
Hypothetical influences of variability of light velocity due to the
parameters of the source of radiation, for the results of spectral measurements
of stars to search for exoplanets are considered. Accounting accelerations of
stars relative to the barycenter of the star - a planet (the planets) was
carried out. The dependence of the velocity of light from the barycentric
radial velocity and barycentric radial acceleration component of the star
should lead to a substantial increase (up to degree of magnitude) semi-major
axes of orbits detected candidate to extrasolar planets. Consequently, the
correct comparison of the results of spectral method with results of other
well-known modern methods of detecting extrasolar planets can regard the
results obtained in this paper as a reliable test for testing the invariance of
the velocity of light.Comment: 11 pages, 5 figure
Influence of a forming process and electric fields on the insulator-conductor transition in thin films of polyheteroarylenes
Determination of the parameters of atmospheric gas clouds by radar methods at frequencies in the rotational spectrum
Correlation between IR spectra and electric conductivity of polyethylene-polypyrrole composites
Luminescence spectra of a supramolecular complex of uranyl and a star-shaped polymer based on calix[8]arene
Optical Properties of Potassium Aluminum Phosphate Glass Activated by Trivalent Titanium Ions
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