Dadface said:
Is't it so that the relativistic mass equation is still useful in that it gives a quick method of calculating relativistic KE?
The equation is still important, but we now say that it gives the total energy for an item with a given (rest) mass and speed. You can therefore also calculate the kinetic energy by subtracting the rest energy.
Personally, I'm happy with using "relativistic" or "rest" in combination with "mass", and similarly using "total", "rest" and "kinetic" in combination with "energy". However, the important thing to note is that if we say "mass" on its own, the modern convention is that this means what used to be called the "rest mass", and if we say "energy" on its own in a relativity context, this means the total energy.
I'm not entirely happy with the way this modern terminology ignores factors of ##c##, as although this simplifies SR I think this can add confusion to GR later.
In special relativity, energy and mass only differ by factors of ##c##, which can be set to 1, so they are essentially equivalent. However, there is a complication in general relativity when describing events within a coordinate system, in that the coordinate speed of light can vary with direction. This means that coordinate values with dimensions of mass and energy actually vary in different ways with potential (and mass can be different in different directions).
When factors of ##c## are included explicitly and are treated as referring to the variable coordinate-dependent speed of light (which can of course be set to 1 in a local SR frame), various Newtonian equations of motion (relating for example to conservation of momentum, angular momentum and rate of change of momentum in free fall) have natural very similar and easily understood forms in GR.
For example, the rate of change of momentum of something with energy ##E## falling in a weak Newtonian gravitational field ##g## as represented in isotropic coordinates (where the scale factor between local space and coordinate space is the same in all directions) is given in GR by the following equation where all values are expressed as coordinate values including the coordinate speed of light ##c##:
$$\frac{d \mathbf{p}}{dt} = \frac{E}{c^2} \mathbf{g} \left ( 1 + \frac{v^2}{c^2} \right ) $$
This equation holds regardless of the direction of ##v## (radial, tangential or somewhere in between), just like Newtonian gravity, with the only difference being the additional term due to the curvature of space. Even that term only depends on the speed, not the direction. (For tangential motion, it leads to a curved path, and for radial motion it causes a change in momentum due to the change of the coordinate scale factor of space).
This notation is of course very unconventional, as ##c## normally represents the standard speed of light, so any equations using it for the coordinate speed of light either need very clear explanation of this unusual use or need some alternative notation, such as primed variables.
Of course this doesn't change the physics, but to write the above equation in the GR way without using the coordinate speed of light one would have to insert various scale factors from the metric which would obscure the relationship with the Newtonian view.
As I like to remain aware of these relationships between Newtonian and GR quantities, I personally prefer to continue to use "mass" for quantities with dimensions of mass and "energy" for quantities with dimension of energy, with appropriate qualifiers like "rest" when necessary to avoid ambiguity and explicit factors of ##c## when necessary to convert between them.