Observer time as a coordinate in relativistic spherical hydrodynamics.
Retarded observer time as coordinate in relativistic spherical hydrodynamic equations prevents Schwarzschild surface formation
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Retarded observer time as coordinate in relativistic spherical hydrodynamic equations prevents Schwarzschild surface formation
Elliptic Kruskal-Schwarzschild space, discussing identification of points which limit Kruskal space into Minkowski space
Correlation properties of quantities depending on space and time
Kruskal space in general relativity and uniform accelerated rigid rod in special relativity show striking formal similarities
Static axisymmetric interior solution of Einstein field equations which matches smoothly to one of Weyl exterior solutions
Parametrization of reduced problem of stationary axially symmetric gravity fields
Dyadic formalism to prove Herglotz-Noether theorem for flat manifolds
The Conservation Element and Solution Element (CESE) method was used as implemented in the NASA research code ez4d (an unstructured Navier-Stokes solver coded in C++ with serial and parallel versions available.) The CESE method is a time-accurate formulation with flux-conservation in both space and time. The method treats the discretized derivatives of space and time identically and while the 2nd-order accurate version was used, high-order versions exist.
The Conservation Element and Solution Element (CESE) method was used as implemented in the NASA research code ez4d. The CESE method is a time accurate formulation with flux-conservation in both space and time. The method treats the discretized derivatives of space and time identically and while the 2nd-order accurate version was used, high-order versions exist, the 2nd-order accurate version was used. In regards to the ez4d code, it is an unstructured Navier-Stokes solver coded in C++ with serial and parallel versions available. As part of its architecture, ez4d has the capability to utilize multi-thread and Messaging Passage Interface (MPI) for parallel runs.