Validating the kinetic energy for the two particle collision problem

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SUMMARY

The discussion focuses on validating the kinetic energy equation for a two-particle collision problem, specifically examining the relationship between kinetic energy (T) and potential energy (V) under conservative forces. The equations of motion are defined as m1a1 = F and m2a2 = -F, with F being a function of the relative distance x = x1 - x2. The conservation of energy is expressed as T + V = E = constant, where T is defined as T = (1/2)m1(v1)2 + (1/2)m2(v2)2. The participants clarify the differentiation process required to verify this relationship and emphasize the need to consider the time derivatives of both kinetic and potential energy.

PREREQUISITES
  • Understanding of Newton's laws of motion
  • Familiarity with the concepts of kinetic and potential energy
  • Knowledge of differentiation and partial derivatives in calculus
  • Basic grasp of conservative forces and energy conservation principles
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  • Study the derivation of the conservation of energy in classical mechanics
  • Learn about the application of Lagrangian mechanics in particle systems
  • Explore the relationship between force and potential energy in conservative fields
  • Investigate the role of relative motion in multi-particle systems
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Students of physics, particularly those studying classical mechanics, as well as educators and anyone interested in the mathematical validation of energy conservation in particle dynamics.

Andreasdreas
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Homework Statement


The following is a summaration of a piece of text in my textbook:

The setting is two particles moving in one dimension, under mutual forces, so that the equations of motion are

(1): m_1 a_1=F and m_2 a_2=-F (a stands for acceleration)

F is only a function of the relative distance between the particles x=x_1-x_2 : F=F(x) so F is conservative and a potential energy function V(x) can be introduced.

The law of conservation of energy then takes the form

(2): T + V=E=constant

with

(3):T=\frac{1}{2}m_1(v_1)^2+\frac{1}{2}m_2(v_2)^2 (T is the kinetic energy and v stands for velocity, this is also the relative velocity of the two particles: v=v_1-v_2).

The books then says that:

eq. 3 can easily be verified by differentiating eq. 2 and using eq. 1 and the realtion between V and F.

Homework Equations


The relation between V and F: F(x)=-\frac{dV}{dx}


The Attempt at a Solution


I am quit unsure with what i should differentiate with respect to when differentiating eq. (2)
V is a function of x and T is a function of v. What i have tried is this:

T+V=constant \implies \frac{dT}{dv} \frac{dv}{dt}=-\frac{dV}{dx}=F(x)

Then i am unsure what term i should use for F(x).
What i have done is to put it equal to ma where a is the acceleration of the relative position x=x_1-x_2 and i guess m should be m_1+m_2 .
But integrating ma dosent seem to yield eq. 3, I have integatred like this:
\int \int (ma) dt dv = \int (mv) dv =\frac{1}{2}mv^2=\frac{1}{2}(m_1+m_2)(v_1-v_2)^2
\frac{1}{2}(m_1+m_2)(v_1-v_2)^2 must give a lot of terms which i don't see will cancel out to give eq. 3
 
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When we say tha energy is conserved, we mean that is constant as time passes. So the derivative of energy w.r.t. time will be zero. Althought V depends explicitly on x = x1-x2, since x1 and x2 are functions of time, then V is actually a function of time. So try to differntiate T+V=E w.r.t. time and then use the equations of motions to get rid of the forces. Also, the force applied to "i" particle will be equall to minus the partial derivative of V w.r.t. xi.
 
To elaborate a little on cosmic dust's good suggestion:

Note that ##T## is a function of ##v_1## and ##v_2##: ##T(v_1, v_2)## and ##V## is a function of ##x_1## and ##x_2##: ##V(x_1, x_2)##. So, overall, the total energy is a function of four variables: ##E(v_1, v_2, x_1, x_2)##.

The time derivative is ##\dot E = \frac{\partial E}{\partial v_1} \dot v_1 + \frac{\partial E}{\partial v_2} \dot v_2 + \frac{\partial E}{\partial x_1} \dot x_1 + \frac{\partial E}{\partial x_2} \dot x_2##

In carrying this out, you’ll need to use ##\frac{\partial V}{\partial x_1} = \frac{\partial V}{\partial x} \frac{\partial x}{\partial x_1}## and similarly for ##x_2##.
 
I guess it can be done that way, althought I had something else in mind:

\frac{dE}{dt}=0\Rightarrow \frac{dT}{dt}+\frac{dV}{dt}=0\Rightarrow \frac{dT}{dt}+\frac{\partial V}{\partial {{x}_{1}}}{{v}_{1}}+\frac{\partial V}{\partial {{x}_{2}}}{{v}_{2}}=0\Rightarrow

\Rightarrow \frac{dT}{dt}-{{m}_{1}}{{\dot{v}}_{1}}{{v}_{1}}-{{m}_{2}}{{\dot{v}}_{2}}{{v}_{2}}=0\Rightarrow \frac{dT}{dt}=\frac{d}{dt}\left( \frac{1}{2}{{m}_{1}}v_{1}^{2}+\frac{1}{2}{{m}_{2}}v_{2}^{2} \right)
 
cosmic dust said:
I guess it can be done that way, althought I had something else in mind:

\frac{dE}{dt}=0\Rightarrow \frac{dT}{dt}+\frac{dV}{dt}=0\Rightarrow \frac{dT}{dt}+\frac{\partial V}{\partial {{x}_{1}}}{{v}_{1}}+\frac{\partial V}{\partial {{x}_{2}}}{{v}_{2}}=0\Rightarrow

\Rightarrow \frac{dT}{dt}-{{m}_{1}}{{\dot{v}}_{1}}{{v}_{1}}-{{m}_{2}}{{\dot{v}}_{2}}{{v}_{2}}=0\Rightarrow \frac{dT}{dt}=\frac{d}{dt}\left( \frac{1}{2}{{m}_{1}}v_{1}^{2}+\frac{1}{2}{{m}_{2}}v_{2}^{2} \right)

Yes, that's much better. I lost sight of the question! You want to verify that T has the form given in OP's equation (3). Very good.
(I was assuming (3) and verifying E is constant. Not what was asked.:redface:)
 
Thanks for the responds, i see it clearly now.
I got confused in the different variables and also i was not proberly aware that a kinetic and potential energy is attached to each of the particles.
 

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