Traceless stress-energy and traversable wormholes
classification
🌀 gr-qc
keywords
betaobtainstracelesstraversablewhenwormholesblackeinstein
read the original abstract
A one-parameter family of static and spherically symmetric solutions to Einstein equations with a traceless energy-momentum tensor is found. When the nonzero parameter $\beta$ lies in the open interval $(0,1)$ one obtains traversable Lorentzian wormholes. One also obtains naked singularities when either $\beta < 0$ or $\beta > 1$ and the Schwarzschild black hole for $\beta = 1$.
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