Authors: Pardis Tabaee Damavandi
The Cauchy problem has been applied to a simple case of linear function in the form y=f(x) expressing wavelength values previously acquired through computer simulations and satisfying the observed empirical initial condition that the extrapolated value of the C-N torsion of 14.10 μm from the Spitzer Telescope spectrum should be sustained.
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[v1] 2020-08-14 20:02:14
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