Document Type
Article
Publication Date
5-2016
Abstract
We present an analysis of the classic wormhole geometries based on conformal Weyl gravity, rather than standard general relativity. The main characteristics of the resulting traversable wormholes remain the same as in the seminal study by Morris and Thorne, namely, that effective super-luminal motion is a viable consequence of the metric. Improving on previous work on the subject, we show that for particular choices of the shape and redshift functions the wormhole metric in the context of conformal gravity does not violate the main energy conditions at or near the wormhole throat. Some exotic matter might still be needed at the junction between our solutions and flat spacetime, but we demonstrate that the averaged null energy condition (as evaluated along radial null geodesics) is satisfied for a particular set of wormhole geometries. Therefore, if fourth-order conformal Weyl gravity is a correct extension of general relativity, traversable wormholes might become a realistic solution for interstellar travel.
Original Publication Citation
Gabriele U. Varieschi and Kellie L. Ault, Int. J. Mod. Phys. D 25, 1650064 (2016) [15 pages] DOI:http://dx.doi.org/10.1142/S0218271816500644
Publisher Statement
Preprint of an article published in International Journal of Modern Physics D, Volume 25, Issue 06, 2016, 15 pages http://dx.doi.org/10.1142/S0218271816500644
© Copyright World Scientific Publishing Company
Journal URL: http://www.worldscientific.com/worldscinet/ijmpd
Digital Commons @ LMU & LLS Citation
Varieschi, Gabriele U. and Ault, Kellie L., "Wormhole Geometries in Fourth-Order Conformal Weyl Gravity" (2016). Physics Faculty Works. 15.
https://digitalcommons.lmu.edu/phys_fac/15
