A. Feinstein, José M. M. Senovilla
Abstract
The authors present a new exact solution of the Einstein field equations which describes an inhomogeneous cosmological model with a perfect fluid source. The equation of state of the fluid is p= rho /3. Some of the main geometrical and kinematical properties of the solution are briefly discussed.
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The authors present a new exact solution of the Einstein field equations which describes an inhomogeneous cosmological model with a perfect fluid source. The equation of state of the fluid is p= rho /3. Some of the main geometrical and kinematical properties of the solution are briefly discussed.
Key concepts: Physics, Perfect fluid, Equation of state, Cosmological model, Mathematical physics, Einstein, Field equation, Einstein field equations