Giancoli, 3rd Ed, pr. 55: Ellastic collision. Solved, but is there easier way?

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In summary, a neutron collides elastically with an at-rest helium-nucleus. The helium nucleus rebounds at a 45-degree angle. To find the angle and speeds of the particles after collision, the equations for kinetic energy conservation and momentum conservation can be used. Simplifying and using trigonometric identities leads to a quadratic equation, which can be solved to find the values of the velocities. While there may be physical intuition shortcuts, using these equations is the most reliable and accurate way to solve the problem. It is important to note that there was a mistake in the y-component momentum equation, where the mass factor for the helium nucleus was dropped. Correcting this error will lead to a factorable quadratic equation with one root being v'
  • #1
bjnartowt
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Homework Statement



A neutron collides elastically with an at-rest helium-nucleus. Masses are approximately "m" and "4m", respectively. Helium nucleus rebounds at 45-degree angle

What angle does the neutron rebound at?

What are speeds of two particles after collision?

Notation:
[tex]\begin{array}{l}
{v_{4m}} = \left[ {{\rm{pre - collision He - nucleus velocity}}} \right] = 0 \\
{v_m} = \left[ {{\rm{pre - collision He - nucleus velocity}}} \right] = 6.5 \times {10^5}{\textstyle{m \over s}} \\
{{v'}_{4m}} = \left[ {{\rm{post - collision He - nucleus velocity}}} \right] = ? \\
{{v'}_m} = \left[ {{\rm{post - collision He - nucleus velocity}}} \right] = ? \\
\end{array}[/tex]



Homework Equations


Kinetic energy conservation, simplified, and with appropreiate zero of initial He-nucleus velocity put in, and with factor of (1/2)*m canceled out:
[tex]{v_m}^2 = 4{v'_{4m}}^2 + {v'_m}^2[/tex]

x-component momentum conservation with factor of "m" struck out:
[tex]6.5 \times {10^5}{\textstyle{m \over s}} = {{v'}_m}\cos \theta + 4{{v'}_{4m}}\cos 45[/tex]

y-component momentum conservation with factor of "m" struck out:
[tex]\sin \theta = - \sin 45{\textstyle{{{{v'}_{4m}}} \over {{{v'}_m}}}}[/tex]


The Attempt at a Solution



Isolate [tex]{{{v'}_m}}[/tex] and put next to trig functions and square both sides in preparation to add them together to get a [tex]{\sin ^2} + {\cos ^2}[/tex] simplification:

[tex]\begin{array}{l}
{\left( {{{v'}_m}\cos \theta } \right)^2} = {\left( {6.5 \times {{10}^5}{\textstyle{m \over s}} - 2\sqrt 2 {{v'}_{4m}}} \right)^2} \\
{\left( {{{v'}_m}\sin \theta } \right)^2} = {\left( { - {{v'}_{4m}}\sin 45} \right)^2} \\
\end{array}[/tex]

Adding these equations and using the abovementioned [tex]{\sin ^2} + {\cos ^2}[/tex] leads to:
[tex]{({{v'}_m})^2} = {6.5^2} \times {10^{10}} + 8{({{v'}_{4m}})^2} - 2 \cdot 6.5 \times {10^5} \cdot 2\sqrt 2 {{v'}_{4m}} + {\textstyle{1 \over 2}}{({{v'}_{4m}})^2}[/tex]

Then: use the kinetic-energy balance mentioned way earlier to eliminate an unknown.


THE QUESTION: This leads to the quadratic formula. I am studying to take the Physics GRE. Is there a way to avoid the quadratic formula? Some sort of physical-intuition-shortcut? I tried visiting the CM frame briefly, but that makes things a bit messy...but perhaps I didn't look hard enough?
 
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  • #2
There's a mistake in your momentum y equation. You dropped the factor of four that comes from the mass of the helium nucleus.

Your approach is fine. The quadratic you get is factorable if you do the algebra correctly, with one root being v'4m=0. It might help not to plug in the value for vm so early.
 
  • #3
I mean yeah, unless you know scattering formulas off the top of your head you will have to derive the result just like you have here. Though fix your error as stated above.
 

1. What is an elastic collision?

An elastic collision is a type of collision between two objects where kinetic energy and momentum are conserved. This means that the total amount of energy and momentum before the collision is equal to the total amount after the collision. In an elastic collision, the objects bounce off each other without any loss of energy.

2. How is an elastic collision solved using Giancoli, 3rd Ed, pr. 55?

In Giancoli, 3rd Ed, pr. 55, an elastic collision is solved using the equations for conservation of momentum and conservation of energy. These equations can be used to find the velocities of the objects before and after the collision.

3. Is there an easier way to solve an elastic collision?

There are other methods for solving an elastic collision, such as using the coefficient of restitution or the center of mass frame. However, the approach used in Giancoli, 3rd Ed, pr. 55 is a straightforward and commonly used method for solving elastic collisions.

4. What are some real-life examples of elastic collisions?

Some real-life examples of elastic collisions include a game of billiards, a bouncing ball, or a collision between two air hockey pucks. In all of these scenarios, the objects involved will bounce off each other without any loss of energy.

5. How does an inelastic collision differ from an elastic collision?

In an inelastic collision, the objects involved stick together after the collision, resulting in a loss of kinetic energy. This means that the total amount of energy and momentum before the collision is not equal to the total amount after the collision. In contrast, an elastic collision involves objects bouncing off each other without any loss of energy.

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