Optical analogues of the Newton-Schrödinger equation and boson star evolution

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Roger, Thomas and Maitland, Calum and Wilson, Kali and Westerberg, Niclas and Vocke, David and Wright, Ewan M. and Faccio, Daniele (2016) Optical analogues of the Newton-Schrödinger equation and boson star evolution. Nature Communications, 7. 13492. ISSN 2041-1723 (https://doi.org/10.1038/ncomms13492)

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Abstract

Many gravitational phenomena that lie at the core of our understanding of the Universe have not yet been directly observed. An example in this sense is the boson star that has been proposed as an alternative to some compact objects currently interpreted as being black holes. In the weak field limit, these stars are governed by the Newton-Schrodinger equation. Here we present an optical system that, under appropriate conditions, identically reproduces such equation in two dimensions. A rotating boson star is experimentally and numerically modelled by an optical beam propagating through a medium with a positive thermal nonlinearity and is shown to oscillate in time while also stable up to relatively high densities. For higher densities, instabilities lead to an apparent breakup of the star, yet coherence across the whole structure is maintained. These results show that optical analogues can be used to shed new light on inaccessible gravitational objects.

ORCID iDs

Roger, Thomas, Maitland, Calum, Wilson, Kali ORCID logoORCID: https://orcid.org/0000-0001-5683-8441, Westerberg, Niclas, Vocke, David, Wright, Ewan M. and Faccio, Daniele;
  • Item type:Article
    ID code:82396
    Dates:
    Date
    Event
    14 November 2016
    Published
    7 October 2016
    Accepted
    Subjects:Science > Physics
    Department:Faculty of Science > Physics
    Depositing user: Pure Administrator
    Date deposited:21 Sep 2022 12:54
    Last modified:11 Nov 2024 13:37
    URI:https://strathprints.strath.ac.uk/id/eprint/82396
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