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Self-gravitating relativistic disks around black holes can form as transient structures in a number of astrophysical scenarios such as binary neutron star and black hole-neutron star coalescences, as ...
We present a brief overview of the stability analysis of the Einstein static universe in various modified theories of gravity, like f(R) gravity, Gauss-Bonnet or f(G) gravity, and Horava-Lifshitz grav...
2002Vol.37No.1pp.117-124DOI: Stability of Crystal Growth Face and Dissolution Face in Crystallization from Solution under Microgravity ZHU Zhen-He,1,2,3 LUO Lin,1,4 LI Chao-Rong1,...
The stability criteria of quasi-two-dimensional dimensional bipolarons have been studied within the framework of strong coupling and path-integral theories. It is shown that the critical values of the...

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