In this article we study weak gravitational lensing of regular Bardeen black hole which has scalar charge g and mass m. We investigate the angular position and magnification of non-relativistic images in two cases depending on the presence or absence of photon sphere. Defining dimensionless charge parameter q = g 2m we seek to disappear photon sphere in the case of |q| > 24 √ 5/125 for which the space time metric encounters strongly with naked singularities. We specify the basic parameters of lensing in terms of scalar charge by using the perturbative method and found that the parity of images is different in two cases: (a) The strongly naked singularities is present in the space time. (b) singularity of space time is weak or is eliminated (the black hole lens).

Non-singular Ayon-Beato-Garcia (ABG) spherically symmetric sta tic black hole (BH) with charge to mass ratio q = g 2m is metric solution of Born-Infeld nonlinear Maxwell-Einstein theory. Central region of the BH behaves as (anti-) de Sitter for (|q| > 1) |q| < 1. In case of |q| = 1 the BH central region behaves as Minkowski flat metric. Nonlinear Electromagnetic (NEM) fields counterpart causes to deviate light geodesics and so light rays will forced to move on effective metric. In this paper we study weak and strong gravitational lensing of light rays by seeking affects of NEM fields counterpart on image locations and corresponding magnification. We set our calculations to experimentally observed Sgr A * BH. In short we obtained: For large distances the NEM counterpart is negligible reaching to linear Maxwell fields. The NEM makes enlarge the BH photon sphere radius as linearly by raising |q| > 1 but deceases by raising |q| ≤ 1. Sign of deflection angle of bending light rays is changed in presence of NEM effects with respect to ones obtained in absence of NEM fields. Absolute value of deflection angle raises by increasing |q| → 1. Weak image locations decreases (increases) by raising 0 < |q| < 1 in presence (absence) of NEM fields. By raising the closest distance of the bending light rays weak image locations changes from left (right) to right (left) in absence (presence) of NEM fields. Einstein rings radius and corresponding magnification centroid become larger (smaller) in presence (absence) of NEM fields in case of weak lensing. Angular separation s between the innermost and outermost relativistic images increases (decreases) by increasing 0 < |q| < 1 in absence (presence) of NEM fields. Corresponding magnification r decreases (increases) by raising 0 < |q| < 1 in absence (presence) of NEM fields. s(r) raises (decreases) by increasing |q| >> 1.

We formulate the nonlinear isovector model in a curved background and calculate the spherically symmetric solutions for weak and strong coupling regimes. The question whether gravity has appreciable effects on the structure of solitons will be examined, in the framework of the calculated solutions, by comparing the flat-space and curved-space solutions. It turns out that in the strong coupling regime, gravity has essential effects on the solutions. It is also shown that the asymptotic form of the metric conforms with that of the charged Reissner-Nordstrom metric. The dimensionless coupling constant of the model has a limit, beyond which a horizon appears in the solutions, indicating the presence of black hole solutions.

In this paper the kinetics of Muon Catalyzed Fusion (μCF) in H/D/T mixture, considering the muon transfer from hydrogen isotopes (p,d,t) to helium isotopes (3 He , 4 He ) in the range of temperatures of 300 K < T < 1300 K at the density of Φ = 1 LHD, is presented. Calculation of cycling rate in different branches of fusion such as dtμ, ptμ, pdμ, ddμ, ttμ and energy gain showed that in certain physical conditions, the H/D/T mixture is comparable to D/T one. Finally the results of this research are compared with the experimental results reported by other researchers; and good agreements were found.