Junction conditions in general relativity

1981 ◽  
Vol 13 (1) ◽  
pp. 29-36 ◽  
Author(s):  
W. B. Bonnor ◽  
P. A. Vickers
2011 ◽  
Vol 20 (11) ◽  
pp. 2239-2252 ◽  
Author(s):  
M. SHARIF ◽  
H. RIZWANA KAUSAR

We consider the modified f(R) theory of gravity whose higher-order curvature terms are interpreted as a gravitational fluid or dark source. The gravitational collapse of a spherically symmetric star, made up of locally anisotropic viscous fluid, is studied under the general influence of the curvature fluid. Dynamical equations and junction conditions are modified in the context of f(R) dark energy and by taking into account the expansionfree evolution of the self-gravitating fluid. As a particular example, the Skripkin model is investigated which corresponds to isotropic pressure with constant energy density. The results are compared with corresponding results in General Relativity.


1967 ◽  
Vol 8 (11) ◽  
pp. 2302-2308 ◽  
Author(s):  
Frank B. Estabrook ◽  
Hugo D. Wahlquist

2020 ◽  
Vol 80 (12) ◽  
Author(s):  
Albert Huber

AbstractIn the present work, a theoretical framework focussing on local geometric deformations is introduced in order to cope with the problem of how to join spacetimes with different geometries and physical properties. This framework is used to show that two Lorentzian manifolds can be matched by considering local deformations of the associated spacetime metrics. Based on the fact that metrics can be suitably matched in this way, it is shown that the underlying geometric approach allows the characterization of local spacetimes in general relativity. Furthermore, it is shown that said approach not only extends the conventional thin shell formalism, but also allows the treatment of geometric problems that cannot be treated with standard gluing techniques.


1983 ◽  
Vol 28 (12) ◽  
pp. 2987-2994 ◽  
Author(s):  
L. Herrera ◽  
J. Jiménez

2006 ◽  
Vol 73 (10) ◽  
Author(s):  
Alex Giacomini ◽  
Ricardo Troncoso ◽  
Steven Willison

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