- #1
Nasher
- 19
- 0
A typical star like the Sun is emitting radiation energy.
Over a duration, say the star emitted radiation energy, E.
This would have required the mass, m=E/(c^2), to be converted to radiation.
For the Universe, is the ratio of radiaton energy to mass energy increasing with time?
Over a duration, say the star emitted radiation energy, E.
This would have required the mass, m=E/(c^2), to be converted to radiation.
For the Universe, is the ratio of radiaton energy to mass energy increasing with time?