Cosmological constant, conical defect and classical test of general relativity

DOI10.1023/A:1012013809911zbMath1014.83039arXivgr-qc/0201036MaRDI QIDQ5955374

José A. S. Lima, Valdir B. Bezerra, Wilson H. C. Freire

Publication date: 2 July 2003

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0201036

zbMATH Keywords

conical defect parameterSchwarzschild field

Mathematics Subject Classification ID

Black holes (83C57) String and superstring theories in gravitational theory (83E30) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (5)

DOES THE COSMOLOGICAL TERM INFLUENCE GRAVITATIONAL LENSING? ⋮ Quasiperiodic oscillations, weak field lensing and shadow cast around black holes in symmergent gravity ⋮ Solar system tests in Rastall gravity ⋮ Gravitational lensing for power-Maxwell charged quintessence black hole in Rastall gravity ⋮ Bounds on the deficit solid angle parameter from solar system tests

Cites Work

• The cosmological constant is back
• Unnamed Item

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