The Contribution of Electron-Positron Pair Production to the Vacuum Energy
Bernard R. Durney

TL;DR
This paper explores how electron-positron pair production contributes to vacuum energy, proposing a calculation method that aligns well with observed vacuum energy densities.
Contribution
It introduces a novel approach to calculating vacuum energy from pair production, addressing divergences in traditional Feynman diagram methods.
Findings
Calculated vacuum density matches observational data
Proposed modification to interaction Lagrangian for meaningful amplitude interpretation
Emphasized importance of low virtual photon-energy processes
Abstract
The vacuum, defined as the state where no particles can be observed, is interpreted here to imply that the lifetime of the e-p pair should be equal to the Planck time. Concerning the title's subject, a perfect theory would require that the true vacuum expectation value of the operator associated with pair production, be compatible with the normalization of the true vacuum. At present, a calculation of the vacuum energy based on Feynman diagrams reveals a serious difficulty: if only second order terms of the S-matrix are retained, and because there are no external lines, it follows that the space-time integrations over the coordinates, involved in the calculation of the vacuum expectation value of the S-matrix, give rise to two identical delta functions: the amplitude is thus proportional to the space-time volume of integration, L4. The square of the amplitude defies then any physically…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Neutrino Physics Research · Quantum Mechanics and Applications
