WebNov 8, 2024 · The stress–energy tensor is defined as the tensor Tαβ of order two that gives the flux of the α th component of the momentum vector across a surface with constant xβ coordinate. In the theory of relativity, this momentum vector is taken as the four-momentum. In general relativity, the stress–energy tensor is symmetric, [1] T α β = T β α. http://philsci-archive.pitt.edu/5137/1/Lehmkuhl_MassEnergyMomentum_and_spacetime_structure.pdf

Final fate of spherically symmetric gravitational collapse of a dust ...

WebWhereas black holes can be treated as perfect fluids under the above assumption, their behavior differs from that of cosmic dust in the universe. The energy momentum tensor for a perfect static fluid in an isotropic and homogeneous universe can be simply written using the density ρ and pressure p of the fluid as T 00 = ~Gρ and T 11 = T 22 = T ... WebOct 27, 2015 · The energy-momentum tensor and D-term of Q-clouds Michael Cantara, Manuel Mai, Peter Schweitzer The D-term is, like mass and spin, a fundamental property … bird\u0027s tongue

Dust solution - Wikipedia

WebWe all know that the energy-momentum tensor for dust is just T α β = ρ 0 v α v β, where ρ 0 is the mass density in the dust's rest frame and v α is the dust's four-velocity. I'm trying to … WebThe Einstein equations are completely integrated in the presence of two (incoming and outgoing) streams of null dust, under the assumptions of spherical symmetry and staticity. The solution is also written in double nu… WebIn its own referential S, this cloud has an energy density ρ0=m0n0 where m 0 refers to the mass of a dust particle and n 0 the number of particles by unit of volum. By definition, as the cloud stands at rest in its proper referential, there is no kinetic term. birdum northern territory