The gravitational field due to a mass distribution is E=Kx3 in the x−direction, where K is a constant. Taking the gravitational potential to be zero at infinity, its value at a distance x is
A
Kx
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B
K2x
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C
Kx2
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D
K2x2
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Solution
The correct option is DK2x2 dV=−Edx ∫V0dV=−∫x∞Kx3dx V=−(K2x2)x∞=K2x2