A Weinberg's proof of ##{T^{\mu\nu}}_{,\nu}=0## for a perfect fluid

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Weinberg's proof of the conservation of the energy-momentum tensor, expressed as ##{T^{\mu\nu}}_{,\nu}=0##, includes a negative sign at the start due to the identity involving the delta function. The integration by parts-like step is clarified as a product rule for differentiation, which does not require actual integration. The varying notation used by Weinberg complicates the understanding of his proof. Despite the confusion, the discussion reveals insights into the mathematical framework behind the proof. Overall, the clarification helps in grasping the nuances of Weinberg's work.
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His proof is hard to follow, can someone help?
Weinberg ("Gravitation and Cosmology") defines the energy-momentum tensor ##T^{\mu\nu}## in equations (2.8.1)-(2.8.2). He proves $${T^{\mu\nu}}_{,\nu}=0$$ on page 44. But:

(1) Why does he have a minus sign at the very beginning; see the equation which starts $$\frac{\partial}{\partial x^i}T^{\alpha i}(x,t) =$$ when there is no such minus sign in (2.8.2)?

(2) How does he do what looks like an integration by parts (third equality) when there is no integration?

What makes his work more confusing is that on pp. 43-44 he alternately uses the notation ##({\bf{x}}t)##, ##(x)##, ##(x,t)## and ##({\bf{x}},t)##.
 
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Kostik said:
His proof is hard to follow, can someone help?
(1) Weinberg gets his negative sign by using the identity: $$\frac{\partial}{\partial x^{i}}\delta^3\left(\vec{x}-\vec{x}_{n}\right)\equiv -\frac{\partial}{\partial x_{n}^{i}}\delta^3\left(\vec{x}-\vec{x}_{n}\right)$$
(2) This is just the product rule for differentiation written in the form:$$-u\left(t\right)\frac{\partial v\left(t\right)}{\partial t}=-\frac{\partial}{\partial t}\left(u\left(t\right)v\left(t\right)\right)+\frac{\partial u\left(t\right)}{\partial t}v\left(t\right)$$
 
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Of course; thanks. I think I have found another proof, but I should have seen this.
 
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