Collide?

Two masses m 1 m_1 and m 2 m_2 are at distance r 1 r_1 and r 2 r_2 in line from the origin respectively, making the distance between them r 2 r 1 r_2-r_1 . Assuming the only forces acting on them are the gravitational forces between them, the time it takes for the two to collide is given by t = π a 2 2 R 0 b c G ( m 1 + m 2 ) , t = \frac{\pi^a}{2\sqrt{2}}\frac{R_0^{\frac{b}{c}}}{\sqrt{G(m_1+m_2)}}, where R 0 = r 2 r 1 R_0 = r_2-r_1 and G G is the gravitational constant. What is a + b + c a+b+c ?


The answer is 6.

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3 solutions

Vincent Moroney
Jun 16, 2018

Let F 12 F_{12} denote the force of mass one on mass two, and F 21 F_{21} be the force of mass two on mass one. Specifically they are F 12 = G m 1 m 2 ( r 2 r 1 ) 2 , F 21 = G m 1 m 2 ( r 2 r 1 ) 2 F_{12} = \frac{Gm_1m_2}{(r_2-r_1)^2}, \, \, \, \, \, \, \, \, F_{21} = -\frac{Gm_1m_2}{(r_2-r_1)^2} and we know they must also satisfy F 12 = m 1 r 1 ¨ F_{12} = m_1 \ddot{r_1} and F 21 = m 2 r 2 ¨ F_{21} = m_2\ddot{r_2} . Using this we can construct the following differential equation r 2 ¨ r 1 ¨ = G ( r 2 r 1 ) 2 ( m 1 + m 2 ) \ddot{r_2}-\ddot{r_1} = -\frac{G}{(r_2-r_1)^2} (m_1 + m_2 ) and we know via the linearity of the derivative that r 2 ¨ r 1 ¨ = d 2 d t 2 ( r 2 r 1 ) \ddot{r_2} - \ddot{r_1} = \frac{d^2}{dt^2}(r_2 - r_1) . So let r 2 r 1 = R r_2 - r_1 = R , giving us R ¨ = G R 2 ( m 1 + m 2 ) . \ddot{R} = -\frac{G}{R^2}(m_1+m_2). Next, we utilize the fact that R ¨ = d v d t = d v d t d R d R = d R d t d v d R \ddot{R} = \frac{dv}{dt} = \frac{dv}{dt}\frac{dR}{dR} = \frac{dR}{dt}\frac{dv}{dR} to give us v d v = G R 2 ( m 1 + m 2 ) d R 0 V v d v = R 0 R ( t ) G R 2 ( m 1 + m 2 ) d R = G ( m 1 + m 2 ) ( 1 R ( t ) 1 R 0 ) V = 2 G ( m 1 + m 2 ) ( 1 R ( t ) 1 R 0 ) , V = d R d t d R 2 G ( m 1 + m 2 ) ( 1 R ( t ) 1 R 0 ) = d t \begin{aligned} vdv =& -\frac{G}{R^2}(m_1+m_2) dR\\ \int_0^{V}v\,dv = &- \int_{R_0}^{R(t)}\frac{G}{R^2}(m_1+m_2)\,dR = G(m_1+m_2)\Big( \frac{1}{R(t)} - \frac{1}{R_0} \Big) \\ V =& \sqrt{2G(m_1+m_2)\Big(\frac{1}{R(t)}-\frac{1}{R_0}\Big)}, \, \, \, \, V = \frac{dR}{dt} \\ &\frac{dR}{\sqrt{2G(m_1+m_2)\Big(\frac{1}{R(t)}-\frac{1}{R_0}\Big)}} = dt \end{aligned} We know that the two objects will start at the distance R 0 R_0 at t = 0 t=0 and they will end at R = 0 R=0 when t = t c t=t_c where t c t_c denotes the time of collision. Therefore we get the following integral R 0 2 G ( m 1 + m 2 ) R 0 0 R ( t ) R 0 R ( t ) d R = 0 t c d t = t c \sqrt{\frac{R_0}{2G(m_1+m_2)}}\int_{R_0}^{0} \sqrt{\frac{R(t)}{R_0-R(t)}}\,dR = \int_0^{t_c} \,dt = t_c via the following integral formula x a x d x = x ( a x ) a arctan ( x ( a x ) x a ) + C \int\sqrt{\frac{x}{a-x}}\,dx = -\sqrt{x(a-x)}-a\arctan\Big( \frac{\sqrt{x(a-x)}}{x-a}\Big) + C we get the following - a limit has to be performed on the arctan term. t c = π 2 2 R 0 3 2 G ( m 1 + m 2 ) t_c = \frac{\pi}{2\sqrt{2}} \frac{R_0^{\frac{3}{2}}}{\sqrt{G(m_1+m_2)}} so we have a + b + c = 6 . \boxed{a+b+c = 6}.

Krishna Karthik
Apr 2, 2020

Watch my boi flammable maths solve this differential equation here, getting the solution above: https://www.youtube.com/watch?v=OtUdGdcfUcE We end up with the equation for time of collision being R o 3 2 8 G M π \Large \frac{R_o ^{\frac{3}{2}}}{\sqrt {8GM}} \pi , where M is the total mass of the system. The steps of solving the second order differential equation is a bit tedious, so just watch the video, it's excellent.

Suhas Sheikh
Jun 16, 2018

The tautochrone problem B=3,C=2 and A=1

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