TY - JOUR
T1 - Scale-dependent (2 + 1)-dimensional electrically charged black holes in Einstein-power-Maxwell theory
AU - Rincón, Ángel
AU - Contreras, Ernesto
AU - Bargueño, Pedro
AU - Koch, Benjamin
AU - Panotopoulos, Grigorios
N1 - Funding Information:
The author A.R. was supported by the CONICYT-PCHA/ Doctorado Nacional/2015-21151658. The author P.B. was supported by the Faculty of Science and Vicerrectoría de Investigaciones of Universidad de los Andes, Bogotá, Colombia. The author B.K. was supported by the Fondecyt 1161150. The author G.P. thanks the Fundação para a Ciência e Tecnologia (FCT), Portugal, for the financial support to the Center for Astrophysics and Gravitation-CENTRA, Instituto Superior Técnico, Universidade de Lisboa, through the Grant No. UID/FIS/00099/2013. Ernesto Contreras: On leave from Universidad Central de Venezuela.
Publisher Copyright:
© 2018, The Author(s).
PY - 2018/8/1
Y1 - 2018/8/1
N2 - In this work we extend and generalize our previous work on the scale dependence at the level of the effective action of black holes in the presence of non-linear electrodynamics. In particular, we consider the Einstein-power-Maxwell theory without a cosmological constant in (2 + 1) dimensions, assuming a scale dependence of both the gravitational and the electromagnetic coupling and we investigate in detail how the scale-dependent scenario affects the horizon and thermodynamic properties of the classical black holes for any value of the power parameter. In addition, we solve the corresponding effective field equations imposing the “null energy condition” in order to obtain analytical solutions. The implications of quantum corrections are also briefly discussed.
AB - In this work we extend and generalize our previous work on the scale dependence at the level of the effective action of black holes in the presence of non-linear electrodynamics. In particular, we consider the Einstein-power-Maxwell theory without a cosmological constant in (2 + 1) dimensions, assuming a scale dependence of both the gravitational and the electromagnetic coupling and we investigate in detail how the scale-dependent scenario affects the horizon and thermodynamic properties of the classical black holes for any value of the power parameter. In addition, we solve the corresponding effective field equations imposing the “null energy condition” in order to obtain analytical solutions. The implications of quantum corrections are also briefly discussed.
UR - http://www.scopus.com/inward/record.url?scp=85051477830&partnerID=8YFLogxK
U2 - 10.1140/epjc/s10052-018-6106-4
DO - 10.1140/epjc/s10052-018-6106-4
M3 - Article
AN - SCOPUS:85051477830
VL - 78
JO - European Physical Journal C
JF - European Physical Journal C
SN - 1434-6044
IS - 8
M1 - 641
ER -