On stellar collapse and the black hole limit from a dynamical view
M. Sachs (1978)
Annales de l'I.H.P. Physique théorique
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M. Sachs (1978)
Annales de l'I.H.P. Physique théorique
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Pavle Savić (1976)
Publications of Department of Astronomy
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Li, Ping, Stagnitti, Frank (2004)
Mathematical Problems in Engineering
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Paolo Maria Mariano, Giuseppe Modica (2009)
ESAIM: Control, Optimisation and Calculus of Variations
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A unified framework for analyzing the existence of ground states in wide classes of elastic complex bodies is presented here. The approach makes use of classical semicontinuity results, Sobolev mappings and cartesian currents. Weak diffeomorphisms are used to represent macroscopic deformations. Sobolev maps and cartesian currents describe the inner substructure of the material elements. Balance equations for irregular minimizers are derived. A contribution to the debate about the role...
Horacio Sosa, José Luis Pérez Aparicio (1996)
Extracta Mathematicae
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A. G. Ramm (2007)
Annales Polonici Mathematici
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Consider the Newtonian potential of a homogeneous bounded body D ⊂ ℝ³ with known constant density and connected complement. If this potential equals c/|x| in a neighborhood of infinity, where c>0 is a constant, then the body is a ball. This known result is now proved by a different simple method. The method can be applied to other problems.
Whiteley, Jonathan P. (2005)
Journal of Theoretical Medicine
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J.M. Gambi, P. Zamorano, P. Romero, M.L. García del Pino (2003)
RACSAM
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The velocity field distribution for rigid motions in the Born?s sense applied to Post-Newtonian Relativistic Celestial Mechanics is examined together with its compatibility with the Newtonian distribution.
Katica Stevanović Hedrih (1998)
Zbornik Radova
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