- #36
pmb_phy
- 2,952
- 1
I don't believe that you were paying close attention to what I was saying. I stated quite cleary above to da_willem that he and Sariaht were using "m" to mean different things. Sariaht is using "m" to refer to relativistic mass and da_willem was using it to mean proper mass. Also E refers to energy, not proper energy E0. As da_willem is using "m" then it E does not equal mc2, its E0 = mc2 where E0 is E as measured in the rest frame of the particle.humanino said:pmb_phy : I don't see your point here. I think it has been posted several times that [tex]E^2 = \vec{p}\,^2 + m^2[/tex] and that the expressions you use are valid only in the rest frame where [tex]p=0[/tex].
The relation [itex]E^2 - (pc)^2 = m^2 c^2[/itex] is valid if an only if "m" is the proper mass of the particle. If, as Sariaht was using it (and how I use it) m is the relativistic mass of a particle. Defined as such the relation [itex]E^2 - (pc)^2 = m^2 c^2[/itex] is invalid. Also when m is the relativistic mass then the relation E = mc2 is valid.
I've never thought that defining "rest mass" in that way was a very good idea. Also one cannot legitimately define proper mass in that way since its a circular definition since the momentum of a tachyon is defined is defined in terms of proper mass. That is merely a relationship between energy, momentum and proper mass. It can't be taken as a definition of proper mass since that requires leaving momentum undefined - bad idea.One can always formally define [tex]m=\sqrt{E^2 - \vec{p}\,^2} = \sqrt{p^2}[/tex] but no physical interpretation in a rest frame can be obtained from it for a real photon (for which [tex]m=0[/tex]).
Depends on how one defines "gravitational field" and as I said when I posted that at least according to Einstein and according to Einstein the existence of a gravitational field is frame dependant and one can "produce" a gravitational field by chaning coordinates. To be precise - the presence of a gravitational field is dictated by the non-vanishing of the affine connection (when the spatial coordinates are Cartesian) and not the non-vanishing of the Riemann tensor.In a flat spacetime there is no gravitational field.
That is a different notion than that given by Einstein. You're thinking of "gravitational field" as the non-vanishing of the Riemann tensor. I am not and Einstein did not. You can define "gravitational field" anyway you like but I have yet to see a good reason to define it in any other way than Einstein did, e.g. in his 1916 GR paper or any of his texts. In fact not everyone speaks of it that way in the GR literature.Usually one defines the graviton field as a perturbation from the flat metric (even though it might not be the best convention : see Rovelli which defines the graviton field as the vierbein instead) ...if the metric is globally flat in A then their can't be any gravitational field in it.
No.Is this the meaning of your posts ?
Pete
Last edited: