mcastillo356
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- There is a step I don't understand.
Relativistic Momentum, Mass, and Energy
Momentum and mass
(...), the classic equations for conserving momentum and energy are not adequate for the analysis of high-speed collisions. (...)
The momentum of a particle moving with velocity ##v## is given by
$$p=\cfrac{mv}{\sqrt{1-(v^2/c^2)}}\qquad{R-10}$$
ENERGY
In relativistic mechanics, as in classic mechanics, the net force on a particle is equal to the time rate of change of the momentum of the particle. Considering one-dimensional motion only, we have
$$F_{net}=\cfrac{dp}{dt}\qquad{R-11}$$
We wish to find an expression for the kinetic energy. To do this, we multiply both sides of equation ##R-11## by the displacement ##dl##. This gives
$$F_{net}\,dl=\cfrac{dp}{dt}\,dl\qquad{R-12}$$
where we identify the term on the left as the work and the term on the right as the change in kinetic energy. Substituting ##v\,dt## for ##dl## in the term on the right we obtain
$$dK=\cfrac{dp}{dt}\,v\,dt=v\,dp$$
Integrating both sides gives
$$K=\displaystyle\int_0^{P_f}v\,dp\qquad{R.13}$$
To evaluate this integral, we first change the integration variable from ##p## to ##v##. Using Equation ##R-10## and the quotient rule, we have
$$dp=d\Bigg (\cfrac{v}{\sqrt{1-(v^2/c^2)}}\Bigg )$$
Why in the step above ##m## disappears?
Attempt
##dp=m\cdot{dv}=d\Bigg (\cfrac{m\cdot{v}}{\sqrt{1-(v^2/c^2)}}\Bigg )##, so they cancel.
(...)
##\cfrac{[1-(v^2/c^2)]^{1/2}\,dv-v\frac{1}{2}[1-(v^2/c^2)]^{-\frac{1}{2}}\bigg (-\cfrac{2vdv}{c^2}\bigg )}{1-(v^2/c^2)^{3/2}}=\cfrac{dv}{[1-(v^2/c^2)]^{3/2}}##
Substituting for ##dp## in Equation ##R-13## gives
$$K=\displaystyle\int_0^{P_f}vdp=m\displaystyle\int_0^{v_f}\cfrac{vdv}{[1-(v^2/c^2)]^{3/2}}=mc^2\Bigg (\cfrac{1}{\sqrt{1-(v_f^2/c^2)}}-1\Bigg )$$
So
$$K=\cfrac{mc^2}{\sqrt{1-(v^2/c^2)}}-mc^2\qquad{R-14}$$
(In this expression, because the only speed is ##v_f##, the subscript ##f## is not needed)
Defining ##mc^2/\sqrt{1-(v^2/c^2)}## as the total relativistic energy ##E##, Equation ##R-14## can be written
$$E=K+mc^2=\cfrac{mc^2}{\sqrt{1-(v^2/c^2)}}\qquad{R-15}$$
where ##mc^2##, called the rest energy ##E_0##, is energy the particle has when it is at rest.
By multiplying both sides of Equation ##R-10## by ##c## and then dividing the resulting equation by Equation ##R-15##, we obtain
$$\cfrac{v}{c}=\cfrac{pc}{E}\qquad{R-16}$$
which can be useful when trying to solve for the speed ##v##. Eliminating ##v## from Equations ##R-10## and ##R-16##, and solving for ##E^2##, gives
$$E^2=p^2c^2+m^2c^4$$
Momentum and mass
(...), the classic equations for conserving momentum and energy are not adequate for the analysis of high-speed collisions. (...)
The momentum of a particle moving with velocity ##v## is given by
$$p=\cfrac{mv}{\sqrt{1-(v^2/c^2)}}\qquad{R-10}$$
ENERGY
In relativistic mechanics, as in classic mechanics, the net force on a particle is equal to the time rate of change of the momentum of the particle. Considering one-dimensional motion only, we have
$$F_{net}=\cfrac{dp}{dt}\qquad{R-11}$$
We wish to find an expression for the kinetic energy. To do this, we multiply both sides of equation ##R-11## by the displacement ##dl##. This gives
$$F_{net}\,dl=\cfrac{dp}{dt}\,dl\qquad{R-12}$$
where we identify the term on the left as the work and the term on the right as the change in kinetic energy. Substituting ##v\,dt## for ##dl## in the term on the right we obtain
$$dK=\cfrac{dp}{dt}\,v\,dt=v\,dp$$
Integrating both sides gives
$$K=\displaystyle\int_0^{P_f}v\,dp\qquad{R.13}$$
To evaluate this integral, we first change the integration variable from ##p## to ##v##. Using Equation ##R-10## and the quotient rule, we have
$$dp=d\Bigg (\cfrac{v}{\sqrt{1-(v^2/c^2)}}\Bigg )$$
Why in the step above ##m## disappears?
Attempt
##dp=m\cdot{dv}=d\Bigg (\cfrac{m\cdot{v}}{\sqrt{1-(v^2/c^2)}}\Bigg )##, so they cancel.

(...)
##\cfrac{[1-(v^2/c^2)]^{1/2}\,dv-v\frac{1}{2}[1-(v^2/c^2)]^{-\frac{1}{2}}\bigg (-\cfrac{2vdv}{c^2}\bigg )}{1-(v^2/c^2)^{3/2}}=\cfrac{dv}{[1-(v^2/c^2)]^{3/2}}##
Substituting for ##dp## in Equation ##R-13## gives
$$K=\displaystyle\int_0^{P_f}vdp=m\displaystyle\int_0^{v_f}\cfrac{vdv}{[1-(v^2/c^2)]^{3/2}}=mc^2\Bigg (\cfrac{1}{\sqrt{1-(v_f^2/c^2)}}-1\Bigg )$$
So
$$K=\cfrac{mc^2}{\sqrt{1-(v^2/c^2)}}-mc^2\qquad{R-14}$$
(In this expression, because the only speed is ##v_f##, the subscript ##f## is not needed)
Defining ##mc^2/\sqrt{1-(v^2/c^2)}## as the total relativistic energy ##E##, Equation ##R-14## can be written
$$E=K+mc^2=\cfrac{mc^2}{\sqrt{1-(v^2/c^2)}}\qquad{R-15}$$
where ##mc^2##, called the rest energy ##E_0##, is energy the particle has when it is at rest.
By multiplying both sides of Equation ##R-10## by ##c## and then dividing the resulting equation by Equation ##R-15##, we obtain
$$\cfrac{v}{c}=\cfrac{pc}{E}\qquad{R-16}$$
which can be useful when trying to solve for the speed ##v##. Eliminating ##v## from Equations ##R-10## and ##R-16##, and solving for ##E^2##, gives
$$E^2=p^2c^2+m^2c^4$$