2020
DOI: 10.1088/1361-6382/ab79d6
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Scalar and fermion field interactions with a gravitational wave

Abstract: Given that gravity waves are the future probes of the universe, it is important to test various physical effects of these on matter. This article studies a perturbation of the field of a massless scalar particle caused by a gravity wave. We also discuss the gravitational waves' effect on a chiral fermion. Our results have physical implications for early universe cosmology and also for ground based observations.

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Cited by 8 publications
(14 citation statements)
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“…For recent observations on the background gravitational waves see the NanoGrav experiment [2]. In this paper we analyze and confirm a perturbation for electromagnetic (EM) waves induced by gravitational waves, previously observed for scalars and neutrinos in [3] and in [4,5]. We discuss resonant interactions, and if this new 'frequency' mode as predicted can be detected in current detectors.…”
Section: Introductionsupporting
confidence: 61%
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“…For recent observations on the background gravitational waves see the NanoGrav experiment [2]. In this paper we analyze and confirm a perturbation for electromagnetic (EM) waves induced by gravitational waves, previously observed for scalars and neutrinos in [3] and in [4,5]. We discuss resonant interactions, and if this new 'frequency' mode as predicted can be detected in current detectors.…”
Section: Introductionsupporting
confidence: 61%
“…The perturbation solution is obtained using the methods of [3] and as outlined in the Appendix1. The…”
Section: Interaction Of Electromagnetic Waves With Gravitational Wave...mentioning
confidence: 99%
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“…4 emerge as the Penrose limit. The other quite natural generalization is if we go beyond the plane waves and consider some ppwaves, gravitational wave beams [61] and linearized theory [62]. It is also worth to notice that the case of massless fields involves also a special analysis due to the possibility of massless particles creation by the gravitational field (in particular, see recent considerations in [36,37]); in fact such possibility can exist even for the massive fields; however, then some additional constrains have to be added [63].…”
Section: Discussionmentioning
confidence: 99%