Rotating black strings in $f(R)$-Maxwell theory
S. Salarpour, A. Sheykhi, Y. Bahrampour

TL;DR
This paper constructs and analyzes charged rotating black string solutions in $f(R)$-Maxwell theory with constant scalar curvature, revealing differences from Einstein theory in thermodynamics and stability, and extends solutions to non-constant Ricci scalar cases.
Contribution
It provides exact analytical solutions for charged rotating black strings in $f(R)$-Maxwell theory with constant curvature, and introduces a new class of solutions with non-constant Ricci scalar including a logarithmic term.
Findings
Solutions depend on $f'(R_0)$ and differ from Einstein theory in AdS spaces.
Entropy does not follow the area law in $f(R)$ gravity.
Black strings are thermodynamically stable in the studied regime.
Abstract
In general, the field equations of theory coupled to a matter field are very complicated and hence it is not easy to find exact analytical solutions. However, if one considers traceless energy-momentum tensor for the matter source as well as constant scalar curvature, one can derive some exact analytical solutions from theory coupled to a matter field. In this paper, by assuming constant curvature scalar, we construct a class of charged rotating black string solutions in -Maxwell theory. We study the physical properties and obtain the conserved quantities of the solutions. The conserved and thermodynamic quantities computed here depend on function and differ completely from those of Einstein theory in AdS spaces. Besides, unlike Einstein gravity, the entropy does not obey the area law. We also investigate the validity of the first law of thermodynamics as…
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