2018
DOI: 10.1103/physrevd.97.124040
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No static spherically symmetric wormholes in Horndeski theory

Abstract: We consider the Horndeski theory in four-dimensional space-time. We show that this theory does not admit stable, static, spherically symmetric, asymptotically flat, Lorentzian wormholes. *

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Cited by 28 publications
(42 citation statements)
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“…One might expect, by analogy to cosmological setting, that there is a no-go theorem in Horndeski theory. This expectation is confirmed in Horndeski theory: static, spherically symmetric, asymptotically flat wormholes are plagued with ghost and/or radial gradient instability [11,12]. By the same analogy, one might expect that the no-go theorem might be circumvented in beyond Horndeski theories, so that a fully stable wormhole might exist.…”
Section: Introductionmentioning
confidence: 80%
“…One might expect, by analogy to cosmological setting, that there is a no-go theorem in Horndeski theory. This expectation is confirmed in Horndeski theory: static, spherically symmetric, asymptotically flat wormholes are plagued with ghost and/or radial gradient instability [11,12]. By the same analogy, one might expect that the no-go theorem might be circumvented in beyond Horndeski theories, so that a fully stable wormhole might exist.…”
Section: Introductionmentioning
confidence: 80%
“…The structure of the stability conditions for spherically symmetric solutions is analogous to that for cosmological solutions, which allows us to formulate the no-go theorem for stable wormholes in the Horndeski theory in a similar way to proving the no-go for nonsingular cosmologies introduced in Sec. 3.3 [301,302,133,303]. Also in the wormhole case, theories beyond Horndeski admit stable solutions [304,293].…”
Section: Black Holes In Horndeski Theory and Beyondmentioning
confidence: 99%
“…It should be pointed out that many of these wormhole solutions were found to be unstable. For example a no-go theorem for wormholes has been proved for Horndeski gravity [23] which basically states that there are no stable static and spherically symmetric wormhole solutions in this theory (although this may not remain the case for the more general beyond Horndeski theories as shown in Ref. [24]).…”
Section: Introductionmentioning
confidence: 99%