TY - JOUR
T1 - Charged slowly rotating toroidal black holes in the (1 + 3)-dimensional Einstein-power-Maxwell theory
AU - Panotopoulos, Grigoris
AU - RINCON RIVERO, ANGEL
PY - 2019/1/1
Y1 - 2019/1/1
N2 - In this work, we find charged slowly rotating solutions in the four-dimensional Einstein-power-Maxwell nonlinear electrodynamics assuming a negative cosmological constant. By solving the system of coupled field equations explicitly, we obtain an approximate analytical solution in the small rotation limit. The solution obtained is characterized by a flat horizon structure, and it corresponds to a toroidal black hole. The Smarr's formula, the thermodynamics and the invariants Ricci scalar and Kretschmann scalar are briefly discussed.
AB - In this work, we find charged slowly rotating solutions in the four-dimensional Einstein-power-Maxwell nonlinear electrodynamics assuming a negative cosmological constant. By solving the system of coupled field equations explicitly, we obtain an approximate analytical solution in the small rotation limit. The solution obtained is characterized by a flat horizon structure, and it corresponds to a toroidal black hole. The Smarr's formula, the thermodynamics and the invariants Ricci scalar and Kretschmann scalar are briefly discussed.
KW - analytical solutions
KW - Classical general relativity
KW - nonlinear electrodynamics
UR - http://www.scopus.com/inward/record.url?scp=85053105492&partnerID=8YFLogxK
U2 - 10.1142/S0218271819500160
DO - 10.1142/S0218271819500160
M3 - Article
AN - SCOPUS:85053105492
VL - 28
JO - International Journal of Modern Physics D
JF - International Journal of Modern Physics D
SN - 0218-2718
IS - 1
ER -