Optical solitons in curved spacetime

verfasst von
Felix Spengler, Alessio Belenchia, Dennis Rätzel, Daniel Braun
Abstract

Light propagation in curved spacetime is at the basis of some of the most stringent tests of Einstein’s general relativity. At the same time, light propagation in media is at the basis of several communication systems. Given the ubiquity of the gravitational field, and the exquisite level of sensitivity of optical measurements, the time is ripe for investigations combining these two aspects and studying light propagation in media located in curved spacetime. In this work, we focus on the effect of a weak gravitational field on the propagation of optical solitons in non-linear optical media. We derive a non-linear Schrödinger equation describing the propagation of an optical pulse in an effective, gradient-index medium in flat spacetime, encoding both the material properties and curved spacetime effects. In analyzing the special case of propagation in a 1D optical fiber, we also include the effect of mechanical deformations and show it to be the dominant effect for a fiber oriented in the radial direction in Schwarzschild spacetime.

Externe Organisation(en)
Eberhard Karls Universität Tübingen
Queen's University Belfast
Zentrum für angewandte Raumfahrt­technologie und Mikro­gravitation (ZARM)
Humboldt-Universität zu Berlin (HU Berlin)
Typ
Artikel
Journal
Classical and quantum gravity
Band
40
Seiten
145008
Anzahl der Seiten
1
ISSN
1361-6382
Publikationsdatum
01.06.2023
Publikationsstatus
Veröffentlicht
Peer-reviewed
Ja
ASJC Scopus Sachgebiete
Physik und Astronomie (sonstige)
Elektronische Version(en)
https://doi.org/10.1088/1361-6382/acdd43 (Zugang: Unbekannt)