English

Universal Charge-Radius Relation for Subatomic and Astrophysical Compact Objects

High Energy Physics - Phenomenology 2008-11-26 v1 Astrophysics General Relativity and Quantum Cosmology Nuclear Theory

Abstract

Electron-positron pair creation in supercritical electric fields limits the net charge of any static, spherical object, such as superheavy nuclei, strangelets, and Q-balls, or compact stars like neutron stars, quark stars, and black holes. For radii between 4×1024\times10^2 fm and 10410^4 fm the upper bound on the net charge is given by the universal relation Z=0.71RfmZ=0.71R_{fm}, and for larger radii (measured in fm or km) Z=7×105Rfm2=7×1031Rkm2Z = 7 \times 10^{-5} R_{fm}^2 = 7 \times 10^{31} R_{km}^2. For objects with nuclear density the relation corresponds to Z0.7A1/3Z \approx 0.7 A^{1/3} (108<A<101210^{8} < A < 10^{12}) and Z7×105A2/3Z \approx 7\times10^{-5} A^{2/3} (A>1012A > 10^{12}), where AA is the baryon number. For some systems this universal upper bound improves existing charge limits in the literature.

Keywords

Cite

@article{arxiv.0804.2140,
  title  = {Universal Charge-Radius Relation for Subatomic and Astrophysical Compact Objects},
  author = {Jes Madsen},
  journal= {arXiv preprint arXiv:0804.2140},
  year   = {2008}
}
R2 v1 2026-06-21T10:30:28.525Z