2023
DOI: 10.1140/epjc/s10052-023-12185-4
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Exploring tidal force effects and shadow constraints for Schwarzschild-like black hole in Starobinsky–Bel-Robinson gravity

Dhruv Arora,
Niyaz Uddin Molla,
Himanshu Chaudhary
et al.

Abstract: The current manuscript deals with the tidal force effects, geodesic deviation, and shadow constraints of the Schwarzschild-like black hole theorised in Starobinsky–Bel-Robinson gravity exhibiting M-theory compactification. In the current analysis, we explore the radial and angular tidal force effects on a radially in-falling particle by the central black hole, which is located in this spacetime. We also numerically solve the geodesic deviation equation and study the variation of the geodesic separation vector … Show more

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Cited by 24 publications
(2 citation statements)
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“…By employing equations ( 16) and (17), we investigated the angular diameter of the black hole shadow as a function of the parameter μ, while maintaining the parameters g = 0.2 and q = 0.3 fixed, within a 1-σ confidence region [97,98], as illustrated in figure 2. Our investigation into the angular diameter of the black hole shadow focuses on supermassive black holes, specifically M87 * with mass and distance from Earth approximately M ≈ 6.5 × 10 9 M e and D ol ≈ 16.8 Mpc respectively, and SgrA * with mass and distance from Earth approximately M ≈ 4.28 × 10 6 M e and D ol ≈ 8.32 kpc respectively.…”
Section: Shadows Of Modified Bardeen Black Holementioning
confidence: 99%
“…By employing equations ( 16) and (17), we investigated the angular diameter of the black hole shadow as a function of the parameter μ, while maintaining the parameters g = 0.2 and q = 0.3 fixed, within a 1-σ confidence region [97,98], as illustrated in figure 2. Our investigation into the angular diameter of the black hole shadow focuses on supermassive black holes, specifically M87 * with mass and distance from Earth approximately M ≈ 6.5 × 10 9 M e and D ol ≈ 16.8 Mpc respectively, and SgrA * with mass and distance from Earth approximately M ≈ 4.28 × 10 6 M e and D ol ≈ 8.32 kpc respectively.…”
Section: Shadows Of Modified Bardeen Black Holementioning
confidence: 99%
“…Recent work on tidal forces in different types of spacetime geometries is discussed in [25][26][27][28]. When an object falls freely towards the spacetime center in Schwarzschild spacetime, it always experiences compression in the angular direction and stretching in the radial direction.…”
Section: Introductionmentioning
confidence: 99%