scholarly journals Does black hole continuum spectrum signal f(R) gravity in higher dimensions?

2020 ◽  
Vol 101 (2) ◽  
Author(s):  
Indrani Banerjee ◽  
Bhaswati Mandal ◽  
Soumitra SenGupta
2006 ◽  
Vol 2006 (02) ◽  
pp. 025-025 ◽  
Author(s):  
Craig Helfgott ◽  
Yaron Oz ◽  
Yariv Yanay

2019 ◽  
Vol 100 (8) ◽  
Author(s):  
Hans Bantilan ◽  
Pau Figueras ◽  
Markus Kunesch ◽  
Rodrigo Panosso Macedo

2010 ◽  
Vol 53 (2) ◽  
pp. 285-290 ◽  
Author(s):  
Cao Chao ◽  
Chen Yi-Xin ◽  
Li Jian-Long
Keyword(s):  

Universe ◽  
2021 ◽  
Vol 7 (8) ◽  
pp. 307
Author(s):  
Bobomurat Ahmedov ◽  
Ozodbek Rahimov ◽  
Bobir Toshmatov

We study the capture cross-section of massless (photon) and massive test particles by the Schwarzschild–Tangherlini black hole, which is a solution of pure general relativity in higher dimensional spacetime with R×SD−2 topology. It is shown that an extra dimension weakens the gravitational attraction of a black hole, and consequently, radii of all the characteristic circular orbits, such as the radius of a photonsphere decrease in the higher dimensions. Furthermore, it is shown that in higher dimensions, there are no stable and bounded circular orbits. The critical impact parameters and capture cross-sections of photons and massive particles are calculated for several higher dimensions and it is shown that they also decrease with increasing dimension. Moreover, we calculate the capture cross-section of relativistic and non-relativistic test particles in the higher dimensions..


2016 ◽  
Vol 94 (10) ◽  
Author(s):  
Antonino Flachi ◽  
Gonçalo M. Quinta ◽  
José P. S. Lemos

2006 ◽  
Vol 2 (S238) ◽  
pp. 139-144
Author(s):  
Jiří Bičák ◽  
Vladimír Karas ◽  
Tomáš Ledvinka

AbstractStationary axisymmetric magnetic fields are expelled from outer horizons of black holes as they become extremal. Extreme black holes exhibit Meissner effect also within exact Einstein–Maxwell theory and in string theories in higher dimensions. Since maximally rotating black holes are expected to be astrophysically most important, the expulsion of the magnetic flux from their horizons represents a potential threat to an electromagnetic mechanism launching the jets at the account of black-hole rotation.


2014 ◽  
Vol 29 (18) ◽  
pp. 1450088 ◽  
Author(s):  
Xin-He Meng ◽  
Wei Xu ◽  
Jia Wang

Black holes with multi-horizons may provide new ways to understand the intrinsic thermodynamics. In this work, we focus on the entropy relations of black holes in three, four and higher dimensions. These entropy relations include entropy product, "part" entropy product and entropy sum. We also discuss their differences and similarities, in order to make a further study on understanding the origin of black hole entropy at the microscopic level.


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