In d-dimensional spacetime, strange quark stars gain stability with increasing dimension for ranges of central density, with the mass maximum marking the onset of radial instability, and Newtonian stability holds for adiabatic index at or above 2(d-2)/(d-1).
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Extra dimensions' influence on the equilibrium and radial stability of strange quark stars
In d-dimensional spacetime, strange quark stars gain stability with increasing dimension for ranges of central density, with the mass maximum marking the onset of radial instability, and Newtonian stability holds for adiabatic index at or above 2(d-2)/(d-1).