Well I am not really used to the relation E=mc2 and how its used. I've only used it in high energy particle collissions where there is no potential.
I read in the book of W. Rindler that every kind of energy contributes to the mass.
And by that he means the following. If m is there rest mass, then the particle's energy is:
E=mc2+K+V+Q+... [1]
where K,V,Q,... are the various forms of energy (kinetic,potential,heat,...). In the case of two masses that interact gravitationally we have the kinetic and potential energy present.
E=mc2+K+V
Now we can re-use the relation of energy-mass equivalence for the system:
E=m'c2, where m' is the mass of the whole system: m'=m+(K+V)/c2.
Just to note a few things:
1)One reason it took me so long to understand was that i had not realized that the energy of a bound system is negative.. That is: E=K+V=|K|-|V|<0, cause |V|>|K|.
2)The second is that i hadnt realized that the relation E=mc2 can be used so generally (I'm talking about equation [1] from Rindler's book).
3)And last, the thing i did realize now is that mass is almost never equal to the rest mass due to various interactions.. even if the difference is infinitesimal. Due to equation [1], i now understand why in nuclei reactions the mass defect or the mass excess (in the case of quarks) is so large, and why when two nucleons bind there is mass defect and where 3 quarks bind there is mass excess (That has to do with the potential's form)
All these were known to me before but i hadnt 'realize' them.
(I hope you all understand what I am trying to say)
I thank everybody for your effort to try and explain to me..
