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Newtonian wormholes with spherical symmetry and tidal forces on test particles

A spherically symmetric wormhole in Newtonian gravitation in curved space, enhanced with a connection between the mass density and the Ricci scalar, is presented. The wormhole, consisting of two connected asymptotically flat regions, inhabits a spherically symmetric curved space. The gravitational potential, gravitational field and the pressure that supports the fluid that permeates the Newtonian wormhole are computed. Particle dynamics and tidal effects in this geometry are studied. The possibility of having Newtonian black holes in this theory is sketched.

preprint2015arXivOpen access
Paulo LuzJosé P. S. Lemos
gr-qcphysics.class-phastro-ph.SRhep-th
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Paulo LuzJosé P. S. Lemos

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