A numerical algorithm for modelling of boson-fermion stars in dilatonic gravity

DOI10.1016/S0377-0427(01)00539-8zbMath1001.83055arXivmath/0004108MaRDI QIDQ1612391

Plamen Fiziev, Stoytcho S. Yazadjiev, Michail D. Todorov, Todor L. Boyadjiev

Publication date: 22 August 2002

Published in: Journal of Computational and Applied Mathematics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/math/0004108

zbMATH Keywords

nonlinear eigenvalue problemscalar-tensor theory of gravityNewton methodmassive dilaton fieldmixed fermion-boson stars

Mathematics Subject Classification ID

Probabilistic models, generic numerical methods in probability and statistics (65C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Numerical chaos (65P20) Numerical bifurcation problems (65P30)

Uses Software

• COLSYS

Cites Work

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• Brans - Dicke boson stars: configurations and stability through cosmic history
• Tensor mass and particle number peak at the same location in the scalar-tensor gravity boson star models - an analytical proof
• Mach's Principle and Invariance under Transformation of Units
• Mathematical modeling of Boson-Fermion stars in the generalized scalar-tensor theories of gravity
• Effective field theory from quantized strings

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