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Casimir Self-Interaction Energy Density of Quantum Electrodynamic Fields
Quantum electrodynamic fields possess fluctuations corresponding to transient particle-antiparticle dipoles, which can be characterized by a nonvanishing polarizability density. Here, we extend a recently proposed quantum scaling law to describe the volumetric and radial polarizability density of a...
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Published in: | Physical review letters 2023-01, Vol.130 (4), p.041601-041601, Article 041601 |
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container_end_page | 041601 |
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container_title | Physical review letters |
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creator | Tkatchenko, Alexandre Fedorov, Dmitry V |
description | Quantum electrodynamic fields possess fluctuations corresponding to transient particle-antiparticle dipoles, which can be characterized by a nonvanishing polarizability density. Here, we extend a recently proposed quantum scaling law to describe the volumetric and radial polarizability density of a quantum field corresponding to electrons and positrons and derive the Casimir self-interaction energy (SIE) density of the field, E[over ¯]_{SIE}, in terms of the fine-structure constant. The proposed model obeys the cosmological equation of state w=-1 and the magnitude of the calculated E[over ¯]_{SIE} lies in between the two recent measurements of the cosmological constant Λ obtained by the Planck Mission and the Hubble Space Telescope. |
doi_str_mv | 10.1103/PhysRevLett.130.041601 |
format | article |
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title | Casimir Self-Interaction Energy Density of Quantum Electrodynamic Fields |
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