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Self-gravitating field configurations: The role of the energy-momentum trace

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Publication:2257256
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DOI10.1016/j.physletb.2014.11.019zbMath1306.83007arXiv1412.3808OpenAlexW2019784574MaRDI QIDQ2257256

Shahar Hod

Publication date: 24 February 2015

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1412.3808



Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Equations of motion in general relativity and gravitational theory (83C10)


Related Items

Mass-radius ratio bound for horizonless charged compact object in higher dimensions ⋮ Lower bound on the radii of light rings in traceless black-hole spacetimes ⋮ On the number of light rings in curved spacetimes of ultra-compact objects ⋮ No-go theorem for static boson stars ⋮ Isotropic compact stars in 4D Einstein–Gauss–Bonnet gravity



Cites Work

  • Black Holes Have No Short Hair
  • Bounds on the mass-to-radius ratio for non-compact field configurations
  • The Large Scale Structure of Space-Time
  • Dynamical boson stars
  • Upper bound on the radii of black-hole photonspheres
  • Unnamed Item
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