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Question: gravitational field due to finite wire...

gravitational field due to finite wire

Answer

Detailed calculation involving integration of gravitational field contributions from infinitesimal mass elements of the wire. The field depends on the position of the point relative to the wire. For a point at perpendicular distance r from a wire of length L, the field components can be calculated by integrating along the length of the wire. Specific formulas are obtained for points opposite the center or opposite an end of the wire.

Explanation

Solution

The gravitational field due to a finite wire of length L and mass M can be calculated at a point P using integration. Let the wire lie along the x-axis. Consider a point P at a perpendicular distance r from the wire. Let the wire extend from x1x_1 to x2x_2 along the x-axis, such that L=x2x1L = x_2 - x_1. The linear mass density is λ=M/L\lambda = M/L.

Consider a small element of the wire of length dx at position (x, 0). The mass of this element is dm=λdxdm = \lambda dx. The distance from this element to the point P at (0, r) is R=x2+r2R = \sqrt{x^2 + r^2}. The gravitational field dE due to this element at P is dE=GdmR2=Gλdxx2+r2dE = \frac{G dm}{R^2} = \frac{G \lambda dx}{x^2 + r^2}, directed from P towards the element (x, 0).

Let θ\theta be the angle the line connecting P and the element makes with the perpendicular line from P to the wire (the y-axis in this setup). The vector from P(0, r) to (x, 0) is (x,r)(x, -r). The angle θ\theta can be defined such that tanθ=x/r\tan \theta = x/r. The components of dE along the x and y directions are: dEx=dEsinθdE_x = dE \sin \theta (towards the wire if x is positive, away if x is negative) dEy=dEcosθdE_y = dE \cos \theta (towards the wire, i.e., downwards in this setup)

From the geometry, sinθ=xx2+r2\sin \theta = \frac{x}{\sqrt{x^2 + r^2}} and cosθ=rx2+r2\cos \theta = \frac{r}{\sqrt{x^2 + r^2}}. So, dEx=Gλdxx2+r2xx2+r2=Gλxdx(x2+r2)3/2dE_x = \frac{G \lambda dx}{x^2 + r^2} \frac{x}{\sqrt{x^2 + r^2}} = \frac{G \lambda x dx}{(x^2 + r^2)^{3/2}}. And dEy=Gλdxx2+r2rx2+r2=Gλrdx(x2+r2)3/2dE_y = \frac{G \lambda dx}{x^2 + r^2} \frac{r}{\sqrt{x^2 + r^2}} = \frac{G \lambda r dx}{(x^2 + r^2)^{3/2}}.

To find the total gravitational field components ExE_x and EyE_y at P, we integrate these expressions from x1x_1 to x2x_2: Ex=x1x2Gλxdx(x2+r2)3/2=Gλ[1x2+r2]x1x2=Gλ(1x22+r21x12+r2)=Gλ(1x12+r21x22+r2)E_x = \int_{x_1}^{x_2} \frac{G \lambda x dx}{(x^2 + r^2)^{3/2}} = G \lambda \left[ \frac{-1}{\sqrt{x^2 + r^2}} \right]_{x_1}^{x_2} = -G \lambda \left( \frac{1}{\sqrt{x_2^2 + r^2}} - \frac{1}{\sqrt{x_1^2 + r^2}} \right) = G \lambda \left( \frac{1}{\sqrt{x_1^2 + r^2}} - \frac{1}{\sqrt{x_2^2 + r^2}} \right). Ey=x1x2Gλrdx(x2+r2)3/2E_y = \int_{x_1}^{x_2} \frac{G \lambda r dx}{(x^2 + r^2)^{3/2}}. Let x=rtanϕx = r \tan \phi, so dx=rsec2ϕdϕdx = r \sec^2 \phi d\phi. When x=x1x=x_1, tanϕ1=x1/r\tan \phi_1 = x_1/r. When x=x2x=x_2, tanϕ2=x2/r\tan \phi_2 = x_2/r. x2+r2=r2tan2ϕ+r2=r2sec2ϕx^2 + r^2 = r^2 \tan^2 \phi + r^2 = r^2 \sec^2 \phi. (x2+r2)3/2=r3sec3ϕ(x^2 + r^2)^{3/2} = r^3 \sec^3 \phi. Ey=ϕ1ϕ2Gλr(rsec2ϕdϕ)r3sec3ϕ=Gλrϕ1ϕ2sec2ϕsec3ϕdϕ=Gλrϕ1ϕ2cosϕdϕ=Gλr[sinϕ]ϕ1ϕ2=Gλr(sinϕ2sinϕ1)E_y = \int_{\phi_1}^{\phi_2} \frac{G \lambda r (r \sec^2 \phi d\phi)}{r^3 \sec^3 \phi} = \frac{G \lambda}{r} \int_{\phi_1}^{\phi_2} \frac{\sec^2 \phi}{\sec^3 \phi} d\phi = \frac{G \lambda}{r} \int_{\phi_1}^{\phi_2} \cos \phi d\phi = \frac{G \lambda}{r} [\sin \phi]_{\phi_1}^{\phi_2} = \frac{G \lambda}{r} (\sin \phi_2 - \sin \phi_1). Here, ϕ1\phi_1 and ϕ2\phi_2 are the angles such that tanϕ1=x1/r\tan \phi_1 = x_1/r and tanϕ2=x2/r\tan \phi_2 = x_2/r. Alternatively, we can use the angles the ends of the wire make with the perpendicular line from P. Let α1\alpha_1 be the angle made by the line from P to x1x_1 with the perpendicular, and α2\alpha_2 be the angle made by the line from P to x2x_2 with the perpendicular. If the wire is from x=ax=-a to x=bx=b, then x1=ax_1=-a and x2=bx_2=b. The angles ϕ1\phi_1 and ϕ2\phi_2 are such that tanϕ1=a/r\tan \phi_1 = -a/r and tanϕ2=b/r\tan \phi_2 = b/r. The angle α1\alpha_1 made by the line to x1=ax_1=-a with the perpendicular (y-axis) is such that tanα1=a/r=a/r\tan \alpha_1 = |-a|/r = a/r. Let's measure angles from the perpendicular line. Let the angles subtended by the ends of the wire at P with the perpendicular line from P to the wire be θ1\theta_1 and θ2\theta_2. If the point P is at (0, r) and the wire is from x1x_1 to x2x_2, then tanθ1=x1/r\tan \theta_1 = |x_1|/r and tanθ2=x2/r\tan \theta_2 = |x_2|/r. The integration limits for ϕ\phi correspond to the angles the lines from P to the ends of the wire make with the y-axis. Let the angles made by the lines from P to the ends of the wire with the perpendicular be α\alpha and β\beta. If the point is opposite to the center of the wire (from -L/2 to L/2), then x1=L/2x_1 = -L/2, x2=L/2x_2 = L/2. Ex=Gλ(1(L/2)2+r21(L/2)2+r2)=Gλ(1L2/4+r21L2/4+r2)=0E_x = G \lambda \left( \frac{1}{\sqrt{(-L/2)^2 + r^2}} - \frac{1}{\sqrt{(L/2)^2 + r^2}} \right) = G \lambda \left( \frac{1}{\sqrt{L^2/4 + r^2}} - \frac{1}{\sqrt{L^2/4 + r^2}} \right) = 0. Ey=Gλr(sinϕ2sinϕ1)E_y = \frac{G \lambda}{r} (\sin \phi_2 - \sin \phi_1). Here tanϕ1=(L/2)/r\tan \phi_1 = (-L/2)/r and tanϕ2=(L/2)/r\tan \phi_2 = (L/2)/r. ϕ1=arctan(L/2r)\phi_1 = -\arctan(L/2r) and ϕ2=arctan(L/2r)\phi_2 = \arctan(L/2r). Ey=Gλr(sin(arctan(L/2r))sin(arctan(L/2r)))=Gλr(sin(arctan(L/2r))+sin(arctan(L/2r)))E_y = \frac{G \lambda}{r} (\sin(\arctan(L/2r)) - \sin(-\arctan(L/2r))) = \frac{G \lambda}{r} (\sin(\arctan(L/2r)) + \sin(\arctan(L/2r))). Let α=arctan(L/2r)\alpha = \arctan(L/2r). Then tanα=L/2r\tan \alpha = L/2r. Consider a right triangle with opposite side L/2 and adjacent side r. The hypotenuse is (L/2)2+r2\sqrt{(L/2)^2 + r^2}. sinα=L/2(L/2)2+r2\sin \alpha = \frac{L/2}{\sqrt{(L/2)^2 + r^2}}. Ey=Gλr(2sinα)=2GλrL/2L2/4+r2=GλLrL2/4+r2E_y = \frac{G \lambda}{r} (2 \sin \alpha) = \frac{2 G \lambda}{r} \frac{L/2}{\sqrt{L^2/4 + r^2}} = \frac{G \lambda L}{r \sqrt{L^2/4 + r^2}}. Substitute λ=M/L\lambda = M/L: Ey=G(M/L)LrL2/4+r2=GMrL2/4+r2E_y = \frac{G (M/L) L}{r \sqrt{L^2/4 + r^2}} = \frac{GM}{r \sqrt{L^2/4 + r^2}}. This is the magnitude of the field, directed towards the wire.

If the point is perpendicular to one end of the wire (from 0 to L), then x1=0x_1 = 0, x2=Lx_2 = L. Ex=Gλ(102+r21L2+r2)=Gλ(1r1L2+r2)E_x = G \lambda \left( \frac{1}{\sqrt{0^2 + r^2}} - \frac{1}{\sqrt{L^2 + r^2}} \right) = G \lambda \left( \frac{1}{r} - \frac{1}{\sqrt{L^2 + r^2}} \right). Ey=Gλr(sinϕ2sinϕ1)E_y = \frac{G \lambda}{r} (\sin \phi_2 - \sin \phi_1). Here tanϕ1=0/r=0\tan \phi_1 = 0/r = 0, so ϕ1=0\phi_1 = 0. tanϕ2=L/r\tan \phi_2 = L/r, so ϕ2=arctan(L/r)\phi_2 = \arctan(L/r). Ey=Gλr(sin(arctan(L/r))sin(0))=Gλrsin(arctan(L/r))E_y = \frac{G \lambda}{r} (\sin(\arctan(L/r)) - \sin(0)) = \frac{G \lambda}{r} \sin(\arctan(L/r)). Let β=arctan(L/r)\beta = \arctan(L/r). Then tanβ=L/r\tan \beta = L/r. Consider a right triangle with opposite side L and adjacent side r. The hypotenuse is L2+r2\sqrt{L^2 + r^2}. sinβ=LL2+r2\sin \beta = \frac{L}{\sqrt{L^2 + r^2}}. Ey=GλrLL2+r2=G(M/L)rLL2+r2=GMrL2+r2E_y = \frac{G \lambda}{r} \frac{L}{\sqrt{L^2 + r^2}} = \frac{G (M/L)}{r} \frac{L}{\sqrt{L^2 + r^2}} = \frac{GM}{r \sqrt{L^2 + r^2}}. This component is directed towards the wire.

The question is general ("gravitational field due to finite wire"). The calculation depends on the position of the point relative to the wire. The formulas derived above are for a point perpendicular to the wire.