Goodver said:
Could anyone please recommend/write derivations for relativistic momentum and relativistic mass
Relativistic mass is the mass as used in Newton's definition of momentum under relativistic conditions. In order to make sure that it has the same velocity dependence in all frames of reference I start from
m\left( v \right) = m_0 \cdot f\left( v \right)
where f\left( v \right) is a function that is identical for all bodies in all frames of reference. m_0 is the mass of the body at rest for
f\left( 0 \right) = 1
Isotropy leads to
f\left( { - v} \right) = f\left( v \right)
With Newton's definition of momentum and the second law of motion I get
F = \left( {f + v \cdot f'} \right) \cdot m_0 \cdot a
In order to simplify the following equations I define
K\left( v \right): = f\left( v \right) + v \cdot f'\left( v \right)
The third law now says
F_1 + F_2 = K\left( {v_1 } \right) \cdot m_1 \cdot a_1 + K\left( {v_2 } \right) \cdot m_2 \cdot a_2 = 0
and that should be valid for all frames of reference:
F'_1 + F'_2 = K\left( {v'_1 } \right) \cdot m_1 \cdot a'_1 + K\left( {v'_2 } \right) \cdot m_2 \cdot a'_2 = 0
Wit Galilei transformation this results in f\left( v \right) = 1. But now I leave classical mechanics and turn to Lorentz transformation. With c = 1 that means
v' = \frac{{v - u}}{{1 - u \cdot v}}
and
a' = a \cdot \left( {\frac{{\sqrt {1 - u^2 } }}{{1 - u \cdot v}}} \right)^3
and therefore
\frac{{K\left( {\frac{{v_1 - u}}{{1 - u \cdot v_1 }}} \right)}}{{K\left( {v_1 } \right) \cdot \left( {1 - u \cdot v_1 } \right)^3 }} = \frac{{K\left( {\frac{{v_2 - u}}{{1 - u \cdot v_2 }}} \right)}}{{K\left( {v_2 } \right) \cdot \left( {1 - u \cdot v_2 } \right)^3 }}
This applies for all combination of velocities including u = v_1 = v and v_2 = 0:
K\left( v \right) \cdot K\left( { - v} \right) = \left( {1 - v^2 } \right)^{ - 3}
This is given for
K\left( v \right) = \sqrt {1 - v^2 } ^{ - 3}
After checking that this is not only a solution for the special case but also for the general equation I just need to solve the resulting differential equation
f' = \frac{1}{v}\left( {\sqrt {1 - v^2 } ^{ - 3} - f} \right)
to get
f = \sqrt {1 - v^2 } ^{ - 1}
and therefore
m\left( v \right) = \frac{{m_0 }}{{\sqrt {1 - v^2 } }}
and
p = m\left( v \right) \cdot v = \frac{{m_0 \cdot v}}{{\sqrt {1 - v^2 } }}
With this result you can avoid relativistic mass at least for momentum. To replace it by E/c² you first need to derive E=m·c² but that's another topic.