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The gravitational field due to a mass distribution is E=(K)/(x^(3)) in the x-direction (K is a constant). Taking the gravitational potential to be zero at infinity, its value at a distance x is |
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Answer» `(K)/(x)` `V=overset(oo)underset(x)INT E.DX=overset(oo)underset(x)int(K)/(x^(3))dx=(K)/(2x^(2))` |
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