scholarly journals Non-static vacuum strings: exterior and interior solutions

1986 ◽  
Author(s):  
J.A. Stein-Schabes

The flux integral for axisymmetric polar perturbations of static vacuum space-times, derived in an earlier paper directly from the relevant linearized Einstein equations, is rederived with the aid of the Einstein pseudo-tensor by a simple algorism. A similar earlier effort with the aid of the Landau–Lifshitz pseudo-tensor failed. The success with the Einstein pseudo-tensor is due to its special distinguishing feature that its second variation retains its divergence-free property provided only the equations governing the static space-time and its linear perturbations are satisfied. When one seeks the corresponding flux integral for Einstein‒Maxwell space-times, the common procedure of including, together with the pseudo-tensor, the energy‒momentum tensor of the prevailing electromagnetic field fails. But, a prescription due to R. Sorkin, of including instead a suitably defined ‘Noether operator’, succeeds.


1989 ◽  
Vol 152 (1) ◽  
pp. 175-177 ◽  
Author(s):  
Tarkeshwar Singh
Keyword(s):  

1992 ◽  
Vol 606 (1) ◽  
pp. 87-94 ◽  
Author(s):  
L. Maignial ◽  
P. Pibarot ◽  
G. Bonetti ◽  
A. Chaintreau ◽  
J.P. Marion

2014 ◽  
Vol 525 ◽  
pp. 146-149
Author(s):  
Xin Ming Wang ◽  
Hai Rong Tang ◽  
Xue Zhi Zhou ◽  
Ning Wang ◽  
Feng Hua Yang

BET (Brunauer Emmett and Teller) surface area and pores distribution for the samples DX 09 Carbon were measured for of DX 09 carbon by N2 adsorption (195 °C) with Autosorb-1C (American Quantachrome Company).The adsorption of benzene over DX 09 Carbon was measured in the static vacuum adsorption equipment, which was self-constructed in laboratory. It was experimentally found that the BET surface area is about 1008 m2/g, and the structure coefficients for DX-09 carbon were W=0.365 and B=1.32*10-6 measured by benzene adsorption and calculated by D-R equation.


1988 ◽  
Vol 66 (2) ◽  
pp. 126-131
Author(s):  
K. D. Krori ◽  
P. Borgohain ◽  
Kanika Das ◽  
Arunima Sarma

A simple method of obtaining singularity-free interior solutions in Einstein–Cartan–Yukawa theory is presented here. The validity of the solution is shown by considering two types of configurations, one Schwarzschild-like and the other Tolman-IV-like. We recover the Schwarzschild and Tolman-IV solutions as soon as the Cartan and Yukawa effects are switched off. In both cases the necessary physical conditions are satisfied. The possible role of torsion in halting the collapse of a massive star is also studied.


2021 ◽  
Vol 104 (4) ◽  
Author(s):  
Marcus Khuri ◽  
Gilbert Weinstein ◽  
Sumio Yamada

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