Research Article Einstein and Møller Energy-Momentum Complexes for a New Regular Black Hole Solution with a Nonlinear Electrodynamics Source Irina Radinschi, 1 Farook Rahaman, 2 Theophanes Grammenos, 3 and Sayeedul Islam 2 1 Department of Physics, Gh. Asachi Technical University, 700050 Iasi, Romania 2 Department of Mathematics, Jadavpur University, Kolkata, West Bengal 700 032, India 3 Department of Civil Engineering, University of Tessaly, 383 34 Volos, Greece Correspondence should be addressed to Irina Radinschi; radinschi@yahoo.com Received 9 June 2016; Accepted 15 September 2016 Academic Editor: Sally Seidel Copyright © 2016 Irina Radinschi et al. Tis is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Te publication of this article was funded by SCOAP 3 . A study about the energy and momentum distributions of a new charged regular black hole solution with a nonlinear electrodynamics source is presented. Te energy and momentum are calculated using the Einstein and Møller energy-momentum complexes. Te results show that in both pseudotensorial prescriptions the expressions for the energy of the gravitational background depend on the mass  and the charge  of the black hole, an additional factor  coming from the spacetime metric considered, and the radial coordinate , while in both prescriptions all the momenta vanish. Further, it is pointed out that in some limiting and particular cases the two complexes yield the same expression for the energy distribution as that obtained in the relevant literature for the Schwarzschild black hole solution. 1. Introduction Energy-momentum localization plays a leading role in the theories advanced over the years in relation to General Relativity. Tere is a major difculty, however, in formulating a proper defnition for the energy density of gravitational backgrounds. Indeed, the key problem is the lack of a satisfactory description for the gravitational energy. Many researchers have conducted extensive research using diferent methods for energy-momentum localization. Standard research methods include the use of diferent tools, such as super-energy tensors [1–4], quasilocal expressions [5– 9], and the famous energy-momentum complexes of Einstein [10, 11], Landau and Lifshitz [12], Papapetrou [13], Bergmann and Tomson [14], Møller [15], Weinberg [16], and Qadir and Sharif [17]. Te main problem encountered is the dependence on the reference frame of these pseudotensorial prescriptions. An alternative method used in many studies on computing the energy and momentum distributions in order to avoid the dependence on coordinates is the teleparallel theory of gravitation [18–26]. As regards pseudotensorial prescriptions, only the Møller energy-momentum complex is a coordinate independent tool. Schwarzschild Cartesian coordinates and Kerr-Schild Cartesian coordinates are useful to compute the energy- momentum in the case of the other pseudotensorial def- initions. Over the past few decades, despite the criticism directed against energy-momentum complexes concerning mainly the physicalness of the results obtained by them, their application has provided physically reasonable results for many spacetime geometries, more particularly for geometries in (3+1), (2+1), and (1+1) dimensions [27–58]. Tere is an agreement between the Einstein, Landau- Lifshitz, Papapetrou, Bergmann-Tomson, Weinberg, and Møller prescriptions, on the one hand, and the defnition of the quasilocal mass advanced by Penrose [59] and devel- oped by Tod [60] for some gravitating systems, on the other hand (see [61] for a comprehensive review). Several Hindawi Publishing Corporation Advances in High Energy Physics Volume 2016, Article ID 9049308, 9 pages http://dx.doi.org/10.1155/2016/9049308