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Ultrarelativistic generalized Lorentzians and the cosmic ray energy flux

Treumann, R. A., and W. Baumjohann (2017), Ultrarelativistic generalized Lorentzians and the cosmic ray energy flux, arXiv, 1703.02327 [astro-ph.HE], 5, Contribution to Cosmic Ray discussion and generalized Lorentzians.

Abstract
We show that the tentative application of the ultrarelativistic generalized
Lorentzian energy distribution to the spectrum of cosmic ray flux provides
evidence for either high TeV chemical potentials generated in the acceleration
source region of the observed cosmic rays or the presence of hypothetical
particles of rest high TeV rests mass. Such particles are not known in our
accessible Universe at the accessible energies. If true they must have been
produced in the cosmic ray sources. Conclusions of this kind clearly depend on
the validity of the generalized Lorentzian distribution function, a possible
though still hypothetical statistical mechanical equilibrium distribution that
is occasionally encountered in observations, in application to cosmic rays.
Further information
BibTeX
@article{id2232,
  author = {R. A. Treumann and W. Baumjohann},
  journal = {arXiv},
  month = {mar},
  note = {Contribution to Cosmic Ray discussion and generalized Lorentzians},
  pages = {5},
  title = {{Ultrarelativistic generalized Lorentzians and the cosmic ray energy flux}},
  volume = {1703.02327 [astro-ph.HE]},
  year = {2017},
  url = {https://arxiv.org/abs/1703.02327},
}
EndNote
%0 Journal Article
%A Treumann, R. A.
%A Baumjohann, W.
%D 2017
%V 1703.02327 [astro-ph.HE]
%J arXiv
%P 5
%Z Contribution to Cosmic Ray discussion and generalized Lorentzians
%T Ultrarelativistic generalized Lorentzians and the cosmic ray energy flux
%U https://arxiv.org/abs/1703.02327
%8 mar
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Printed 20. Aug 2019 17:58