Weak Deflection Angle by Casimir Wormhole Using Gauss-Bonnet Theorem and Its Shadow

Wajiha Javed; Ali Hamza; Ali Övgün

doi:10.20944/preprints202001.0126.v1

Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Version 1 : Received: 11 January 2020 / Approved: 12 January 2020 / Online: 12 January 2020 (16:06:05 CET)
Version 2 : Received: 20 March 2020 / Approved: 23 March 2020 / Online: 23 March 2020 (03:48:02 CET)

Here we calculate the deflection angle of photon by Casimir wormhole in weak limit approximation. First we calculate Gaussian optical curvature with the help of optical spacetime geometry and so we use the Gauss-Bonnet theorem on Gaussian optical metric and find deflection angle of photon by Casimir wormhole. Moreover, we calculate the photon's deflection angle in the presence of plasma medium and we also see the graphical nature of deflection angle in both cases. After calculating the deflection angle of Casimir wormhole. Now, we move towards the shadow of Casimir wormhole. After the observations of Event Horizon Telescope, the study of shadow become very important so that we plot the shapes of shadow of Casimir wormhole, and we calculate the photon geodesic around the Casimir wormhole.

Relativity and gravitation; Casimir Wormhole; Gauss-Bonnet; Effect of Plasma; Shadow of Casimir Wormhole

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Weak Deflection Angle by Casimir Wormhole Using Gauss-Bonnet Theorem and Its Shadow

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