1994
DOI: 10.1103/physrevd.49.853
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Scalar waves in a wormhole geometry

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1995
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Cited by 20 publications
(28 citation statements)
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“…The string equations of motion for the coordinates θ and φ remain the same as in (15) and (16) while that for the coordinate l becomes :…”
Section: Closed Stringsmentioning
confidence: 99%
“…The string equations of motion for the coordinates θ and φ remain the same as in (15) and (16) while that for the coordinate l becomes :…”
Section: Closed Stringsmentioning
confidence: 99%
“…And because B −A P R 3 min ∼ B −A P (B/2A P ) = B/2 as B → 0, positivity of B demands that theα 2 term be present in Eq. (22), thus that the scalar field φ be present in the field equations, coupled to the space-time geometry with the unconventional polarity. Let us note, moreover, that here there is no mention of a 'slow roll down a potential', a common element in many proposed inflationary scenarios involving an 'inflaton' scalar field.…”
Section: Inflation and The 'Big Bounce'mentioning
confidence: 99%
“…As an application of this idea, Torres et al [7] considered the microlensing caused by wormholes on light coming from distant active galactic nuclei. Also, studying the propagation of different types of perturbations in wormhole geometries was initiated by Kar and Sahdev [8], and Kar et al, who studied the reflection and transmission of massive scalar waves in the presence of an ultrastatic wormhole. Moreover, propagation of electromagnetic waves through a static wormhole is investigated by Bergliaffa and Hibberd [9].…”
Section: Introductionmentioning
confidence: 99%