
doi: 10.1063/1.525501
New exact solutions to Einstein’s equations are given which are spherically symmetric and static with perfect fluid distributions satisfying a linear equation of state p = nρ and n∈(0,1]. Heintzmann’s generating method is then used to build up a family of new solutions for each value of n.
Quantum hydrodynamics and relativistic hydrodynamics, static, linear density-pressure relation, interior of star in equilibrium, Einstein's equations (general structure, canonical formalism, Cauchy problems), Exact solutions to problems in general relativity and gravitational theory, exact analytic solutions, perfect fluid, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), spherically symmetric, Heintzmann's method
Quantum hydrodynamics and relativistic hydrodynamics, static, linear density-pressure relation, interior of star in equilibrium, Einstein's equations (general structure, canonical formalism, Cauchy problems), Exact solutions to problems in general relativity and gravitational theory, exact analytic solutions, perfect fluid, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), spherically symmetric, Heintzmann's method
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