# Experimental and theoretical investigations of a plasma fireball dynamics

## Related Articles

- A null-tetrad approach to Kerr-Schild gravitational fields in matter. Udeschini, Elisa Brinis; Magli, Giulio // Journal of Mathematical Physics;Nov96, Vol. 37 Issue 11, p5695
Studies Kerr-Schild gravitational fields in a matter. Use of null tetrad formalism to investigate the structure of Einstein field equations; Reduction to a linear system.

- Multipole structure of stationary gravitational fields at null infinity. Kundu, Prasun K. // Journal of Mathematical Physics;Aug88, Vol. 29 Issue 8, p1866
The multipole structure of the gravitational field produced by a stationary, isolated source at null infinity is investigated using a Bondi-type null polar coordinate system. The results are connected with the previous works of the author on the multipole expansion of stationary, asymptotically...

- A Kerr object embedded in a gravitational field. II. Krori, K. D.; Bhattacharjee, R. // Journal of Mathematical Physics;Jan1990, Vol. 31 Issue 1, p147
Starting with a Weyl solution representing an axially symmetric gravitational field as the seed metric, a generalized Kerr solution is generated by the Belinskiiâ€“Zakharov technique [Sov. Phys. JETP 48, 985 (1978); 50, 1 (1980)]. This solution may be interpreted as a Kerr metric embedded...

- Effects of the shear viscosity on the character of cosmological evolution. Huang, Wung-Hong // Journal of Mathematical Physics;Mar1990, Vol. 31 Issue 3, p659
Bianchi type I cosmological models are studied that contain a stiff fluid with a shear viscosity that is a power function of the energy density, such as Î·=Î±Îµn. These models are analyzed by describing the cosmological evolutions as the trajectories in the phase plane of Hubble functions....

- The gravitational field of a charged, magnetized, accelerating, and rotating mass. García Díaz, Alberto; Bretón Baez, Nora // Journal of Mathematical Physics;Mar1985, Vol. 26 Issue 3, p465
The explicit expression of a Petrov type G solution to the Einsteinâ€“Maxwell equations is given. This new solution is endowed with eight arbitrary parameters; mass, Newmanâ€“Untiâ€“Tamburino (NUT) parameter, angular momentum, acceleration, electric and magnetic charges, and...

- Confined gravitational fields produced by anisotropic fluids. Herrera, L.; Ponce de León, J. // Journal of Mathematical Physics;Nov85, Vol. 26 Issue 11, p2847
A family of solutions of the Einstein equations for a spherically symmetric distribution of anisotropic matter is presented, which can be matched with the flat (Minkowskian) space-time on the boundary of the matter, although the energy density and stresses are nonvanishing within the sphere.

- General exact solutions of Einstein equations for static perfect fluids with spherical symmetry. Berger, Sonia; Hojman, Roberto; Santamarina, Jorge // Journal of Mathematical Physics;Dec87, Vol. 28 Issue 12, p2949
The gravitational field equations for a spherical symmetric perfect fluid are completely solved. The general analytical solution obtained depends on an arbitrary function of the radial coordinate. As illustrations of the proposed procedure the exterior and interior Schwarzschild solutions are...

- On ``Time-Periodic'' Black-Hole Solutions to Certain Spherically Symmetric Einstein-Matter Systems. Dafermos, Mihalis // Communications in Mathematical Physics;Jul2003, Vol. 238 Issue 3, p411
This paper explores black hole solutions of various Einstein-wave matter systems admitting a time-orientation preserving isometry of their domain of outer communications taking some point to its future. In the first two parts, it is shown that such solutions, assuming in addition that they are...

- Magnetic Field Effects on Spacetime Around a Magnetized Spherical Star. Mirza, Babur M.; Saeed, Adnan; Sadiq, Safeer // International Journal of Theoretical Physics;Oct2009, Vol. 48 Issue 10, p2938
We investigate the effects of magnetic field on the background spacetime of a spherically symmetric relativistic star. Using the general relativistic Maxwell equations coupled to the Einstein field equations for the gravitational field, it is shown that not only the backreaction of the spacetime...