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• W3178688783 abstract "Analogue gravity experiments make feasible the realisation of black hole spacetimes in a laboratory setting and the observational verification of Hawking radiation. Since such analogue systems are typically dominated by dispersion, efficient techniques for calculating the predicted Hawking spectrum in the presence of strong dispersion are required. In the preceding paper, an integral method in Fourier space is proposed for stationary $1+1$-dimensional backgrounds which are asymptotically symmetric. Here, this method is generalised to backgrounds which are different in the asymptotic regions to the left and right of the scattering region." @default.
• W3178688783 created "2021-07-19" @default.
• W3178688783 creator A5020272506 @default.
• W3178688783 date "2014-11-03" @default.
• W3178688783 modified "2023-09-25" @default.
• W3178688783 title "Integral method for the calculation of Hawking radiation in dispersive media. II. Asymmetric asymptotics" @default.
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• W3178688783 doi "https://doi.org/10.1103/physreve.90.053303" @default.
• W3178688783 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/25493900" @default.
• W3178688783 hasPublicationYear "2014" @default.
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