2016
DOI: 10.1134/s0040577916080080
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More about wormholes in generalized Galileon theories

Abstract: We consider a class of generalized Galileon theories within General Relativity in space-times of more than two spatial dimensions. We show that these theories do not admit stable, static, spherically symmetric, asymptotically flat and traversable Lorentzian wormholes.

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Cited by 35 publications
(45 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: 81%
“…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: 81%
“…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%
“…These two sectors are decoupled at linear order and can be studied separately. 9 Although the sector that is typically affected by ghost-like instabilities in Horndeski theories is the even one [17][18][19], for the sake of completeness we will start by briefly reviewing the stability properties of the odd sector.…”
Section: Stability Of Wormhole Solutionsmentioning
confidence: 99%