2018
DOI: 10.1140/epjc/s10052-018-5872-3
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Shadows of rotating five-dimensional charged EMCS black holes

Abstract: Higher dimensional theories admit astrophysical objects like supermassive black holes, which are rather different from standard ones, and their gravitational lensing features deviate from general relativity. It is well known that a black hole shadow is a dark region due to the falling geodesics of photons into the black hole and, if detected, a black hole shadow could be used to determine which theory of gravity is consistent with observations. Measurements of the shadow sizes around the black holes can help t… Show more

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Cited by 114 publications
(51 citation statements)
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References 60 publications
(111 reference statements)
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“…3 For the special BPS case Q = M (BMPV solution) they have been thoroughly explored in [34]. It is not in the interest of this work to study the geodesic structure of the more general CCLP geometries, which has been tackled in [35,36]. Finally, yellow lines host solutions that can be lifted to…”
Section: The Metric and Gauge Fieldmentioning
confidence: 99%
“…3 For the special BPS case Q = M (BMPV solution) they have been thoroughly explored in [34]. It is not in the interest of this work to study the geodesic structure of the more general CCLP geometries, which has been tackled in [35,36]. Finally, yellow lines host solutions that can be lifted to…”
Section: The Metric and Gauge Fieldmentioning
confidence: 99%
“…These methods were later developed and generalized widely (see [80][81][82][83][84][85]). Having these methods in hand, a large number of black hole spacetimes, including those with cosmological components, were given rigorous analytical calculations, simulations, numerical, and observational studies [86][87][88][89][90][91][92][93][94][95][96][97][98][99][100]. The black hole shadow is of great importance as it provides information about the light propagation in near-horizon regions.…”
Section: Shadow Of the Black Holementioning
confidence: 99%
“…The study of phenomenon for BH shadow can provide the useful information about the various physical aspects of any given BH spacetime and the recent image from Event Horizon Telescope (EHT) [15][16][17][18][19][20] marks a significant mile stone in the study of BH physics. The mathematical aspect of the very phenomenon which has been developed over the year [21][22][23][24][25][26][27][28][29][30][31][32][33][34][35] can be studied with observed data which can further help to hone the mathematical models of the extraordinary astronomical objects like a BH. Based on such standpoints, we are motivated to study the motion of photons in ADS geometry to observe the effect of different charges on the path of the light along with the shadows and the relation for distance of closest approach with the magnetic charges (v), the gauge coupling constant (g) and NUT charge (N g ).…”
Section: Introductionmentioning
confidence: 99%