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wLw said:here, in section 4
This is a paper on Newtonian gravity, not relativity.
wLw said:here, in section 4
wLw said:if gravitational filed has no energy how can you explain the gravitational radiation
in Newton case we have$$\nabla^2\phi=4\pi\rho$$. does the ##\rho## include binding energy or just only matter massPeterDonis said:Gravitational radiation is not the same as the "gravitational field" you are talking about, nor is the kind of energy that gravitational radiation carries the same as the kind of "energy" that appears in the Komar mass integral.
wLw said:does the ρ\rho include binding energy or just only matter mass
so the gravitational radiation refers to the energy of outside gravitational filed (generated by body), and the gravitational (no filed ,because it is binding energy)energy in komar mass is binding energy,but both of them are nonlocalizable?,is i right.?PeterDonis said:In Newtonian physics ##\rho## only includes "matter mass". But that is also true in General Relativity. Look at the Komar mass integral again: the "binding energy" factor is not ##\rho## (or more generally ##\rho + 3p##, which is the "source" factor that comes from the matter). If you have to pick a particular factor in the integral that represents "binding energy", it would be ##\sqrt{g_{tt}}##, the redshift factor. But really "binding energy" is not localized at all; it's a global property of the system--it's the fact that the mass ##M## of the bound system is less than the total mass of all the constituents would be if they were all widely separated from each other.
wLw said:so the gravitational radiation refers to the energy of outside gravitational filed (generated by body), and the gravitational (no filed ,because it is binding energy)energy in komar mass is binding energy,but both of them are nonlocalizable?,is i right.?
wLw said:thank you a lot