scholarly journals Contribution of Pressure to the Energy–Momentum Density in a Moving Perfect Fluid: A Physical Perspective

2021 ◽  
Vol 51 (1) ◽  
Author(s):  
Ashok K. Singal
Author(s):  
Ashok Singal

In the energy-momentum density expressions for a relativistic perfect fluid with a bulk motion, one comes across a couple of pressure-dependent terms, which though well known, are to an extent, lacking in their conceptual basis and the ensuing physical interpretation. In the expression for the energy density, the rest mass density along with the kinetic energy density of the fluid constituents due to their random motion, which contributes to the pressure as well, are already included. However, in a fluid with a bulk motion, there are, in addition, a couple of explicit, pressure-dependent terms in the energy-momentum densities, whose presence to an extent, is shrouded in mystery, especially from a physical perspective. We show here that one such pressure-dependent term appearing in the energy density, represents the work done by the fluid pressure against the Lorentz contraction during transition from the rest frame of the fluid to another frame in which the fluid has a bulk motion. This applies equally to the electromagnetic energy density of electrically charged systems in motion and explains in a natural manner an apparently paradoxical result that the field energy of a charged capacitor system decreases with an increase in the system velocity. The momentum density includes another pressure-dependent term, that represents an energy flow across the system, due to the opposite signs of work being done by pressure on two opposite sides of the moving fluid. From Maxwell's stress tensor we demonstrate that in the expression for electromagnetic momentum of an electric charged particle, it is the presence of a similar pressure term, arising from electrical self-repulsion forces in the charged sphere, that yields a natural explanation for the famous, more than a century old, 4/3 factor in the electromagnetic mass.


We consider axially symmetric stationary relativistic flows of a perfect fluid which is characterized by a general density-pressure relation µ ( p ). It is shown that the meridional components of velocity can be derived from a stream-function, the trajectories of the fluid particles being spirals wound around torus-shaped surfaces. The moment of the velocity, and another dynamical variable, are conserved for fluid particles along their motion. However, the relativistic angular-momentum-density is convectively conserved only in a fluid in which the velocity of sound equals the velocity of light. We evaluate the total angular momentum L and the total energy E of a spherical vortex in such a fluid, based on a solution given previously. Putting L = 1/2ℏ and E = mc 2 , where m denotes the mass of the neutron, and letting the maximum value of the flow in the vortex equal c , we get a value of 1.2 x 10 -13 cm for the radius of the vortex.


2016 ◽  
Vol 12 (3) ◽  
pp. 4350-4355
Author(s):  
VIBHA SRIVASTAVA ◽  
P. N. PANDEY

The object of the present paper is to study a perfect fluid K¨ahlerspacetime. A perfect fluid K¨ahler spacetime satisfying the Einstein field equation with a cosmological term has been studied and the existence of killingand conformal killing vectors have been discussed. Certain results related to sectional curvature for pseudo projectively flat perfect fluid K¨ahler spacetime have been obtained. Dust model for perfect fluid K¨ahler spacetime has also been studied.


2021 ◽  
Vol 62 (3) ◽  
pp. 032501
Author(s):  
U. C. De ◽  
S. K. Chaubey ◽  
S. Shenawy

2008 ◽  
Vol 246 (1) ◽  
pp. 124-128 ◽  
Author(s):  
R. K. Kothari ◽  
M. Sharma ◽  
K. B. Joshi ◽  
B. K. Sharma

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