2019
DOI: 10.1007/s10509-019-3561-9
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The vacuum polarization paradox and its solution

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Cited by 13 publications
(33 citation statements)
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“…As is well known, the solution of such equation is a shielded Coulomb field, i.e., an electric field with an exponential decay. In the gravitational equivalent (with the  sign) the near field is enhanced ("anti-screened") [13], because masses are attracting, while electric charges with the same polarity are repelling. The background field shows up as uniformly distributed Dirac/Majorana particles (with dipoles c 2 /  ).…”
Section: The Cosmological Background Fieldmentioning
confidence: 99%
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“…As is well known, the solution of such equation is a shielded Coulomb field, i.e., an electric field with an exponential decay. In the gravitational equivalent (with the  sign) the near field is enhanced ("anti-screened") [13], because masses are attracting, while electric charges with the same polarity are repelling. The background field shows up as uniformly distributed Dirac/Majorana particles (with dipoles c 2 /  ).…”
Section: The Cosmological Background Fieldmentioning
confidence: 99%
“…In the introduction paragraph I have proposed to indicate the constituents of the energetic cosmological background energy as darks. In [13], it has been argued that such a constituent is a Dirac/Majorana particle, characterized by an elementary angular dipole moment 2 /  and an elementary linear dipole moment c 2 / …”
Section: The Potential Function Of a "Dark"mentioning
confidence: 99%
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