Abstract
In 2011, Chinese researcher Ni found the solution of the Oppenheimer-Volkoff problem for a stable configuration of stellar object with no internal source of energy. The Ni’s solution is the nonrotating hollow sphere having not only an outer, but an inner physical radius as well. The upper mass of the object is not constrained. In our paper, we contribute to the description of the solution. Specifically, we give the explicit description of metrics inside the object and attempt to link it with that in the corresponding outer Schwarzschild solution of Einstein field equations. This task appears to be non-trivial. We discuss the problem and suggest a way how to achieve the continuous linkup of both object-interior and outer-Schwarzschild metrics. Our suggestion implies an important fundamental consequence: there is no universal relativistic speed limit, but every compact object shapes the adjacent spacetime and this action results in the specific speed limit for the spacetime dominated by the object. Regardless our suggestion will definitively be proved or the successful linkup will also be achieved in else, still unknown way, the success in the linkup represents a constraint for the physical acceptability of the models of compact objects.
Highlights
It is known that the final stage of a star that spent all storage of its nuclear fuel is either a white dwarf or a neutron star
Every model of compact object should provide a description of the metrics of spacetime in its interior as well as in the neighboring empty space
Considering a simple model of non-rotating, stable, compact neutron object, we pointed out the serious problem concerning the linkup of metrics at the outer physical surface
Summary
It is known that the final stage of a star that spent all storage of its nuclear fuel is either a white dwarf or a neutron star. Soon after the Ni’s paper was published, Mei independently considered the hollow-sphere concept (he was the first who used the term “hollow sphere”) as well as the solid spheres and described the metrics for the object of a constant density [8]. He did not deal with the metrics of adjacent empty space. The linkup of the interior and empty-space metrics appears to be a non-trivial task It this paper, we deal with this problem.
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