To help the reader to adapt to the imaginary time, we write the definition of the electromagnetic field strength as reported in Heisenberg-Pauli’s work, which Rosenfeld was referring to ([52], p. 24). The electromagnetic potentials \( \Phi _r \), defined using the vector potential \( ...
Based on a KS-test and a t-test comparing the BGG and model distributions, we conclude that the BGGs generally do not occupy the center of the potential, and that their phase space distribution is consistent with that of the other group members. . . 58 2.7 Contours of κeff =γeff ...
[178], a 20-year data set with characteristics similar to those of the NANOGrav PTA, would have a realistic chance of detecting anistropy at the 3-σ level. This work is based on the assumption that the GW signal strength scales with NpsrNpsr−1/2 (where Npsr is the number of ...
My guess is ks is just kilograms and m is maybe m2. What are the variables in gravitational constant. G= 6.674 x 10^-11 m^3 / kg s^2 m=? kg=? s=? Also First post :D m = meters (unit of distance), kg = kilograms (unit of mass), s = seconds (unit of time), N =...
Here we study the effect of the “Hořava” parameter on the image of the shadow of the KS compact objects and in the weak-field limit its influence on the gravitational lensing, both in the presence of plasma. The paper is organized as follows. In Sect. 2 we introduce the notion of...
KS 1731-260 524 0.2-2 1.3 Aql X-1 549 1.0 1.0 MXB 1658-298 567 0.1 0.3 4U 1636-53 581 4.4 2.0 MXB 1743-29 589 ? ? SAXJ1750.8-2980 601 ? ? 4U 1608-52 619 < 1 < 1 As discussed by Chakrabarty, the ν s ’s inferred from nearly coherent oscilla- tions (given by ν B ...