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how would you describe Newtonian gravity as a vector field?
This discussion provides a detailed mathematical description of Newtonian gravity as a vector field. It begins with a mass located at \(\vec{x}_{0}=(x_{0},y_{0},z_{0})\) with mass \(m_{0}\), generating a force per unit mass at any point \(\vec{x}\neq\vec{x}_{0}\) given by \(\vec{f}(x,y,z)=-\frac{Gm_{0}}{||\vec{x}-\vec{x}_{0}||^{3}}(\vec{x}-\vec{x}_{0})\). The resultant force \(\vec{F}\) acting on an object of mass \(M\) at \((x,y,z)\) is derived by multiplying \(\vec{f}\) with \(M\). Additionally, the discussion presents an alternative representation using spherical coordinates, expressed as \(\vec F (r, \theta, \phi) = - \frac{G m_0}{r^2} \hat r\), where \(\hat r\) indicates the unit vector in the radial direction.
PREREQUISITESStudents of physics, educators teaching classical mechanics, and researchers interested in gravitational theories will benefit from this discussion.