The law of conservation of energy is wrong?

Click For Summary
SUMMARY

The discussion centers on the law of conservation of energy in the context of general relativity (GR) and cosmic expansion. Participants clarify that while energy conservation holds in local inertial frames, it fails globally due to the lack of a universal simultaneity definition in GR. The energy of a photon is defined by the equations E=hλ and E=hf, with the latter being correct for energy calculations. Additionally, the conversation highlights the complexities of defining energy at cosmic scales, particularly as the universe expands and radiation density decreases.

PREREQUISITES
  • Understanding of general relativity (GR) principles
  • Familiarity with the concept of simultaneity in physics
  • Knowledge of photon energy equations (E=hλ and E=hf)
  • Basic grasp of cosmic expansion and its effects on energy density
NEXT STEPS
  • Research the implications of general relativity on energy conservation
  • Explore the concept of simultaneity in different reference frames
  • Study the relationship between wavelength and energy in electromagnetic radiation
  • Investigate the effects of cosmic expansion on radiation and matter density
USEFUL FOR

Physicists, students of theoretical physics, and anyone interested in the complexities of energy conservation in the universe, particularly in relation to general relativity and cosmic phenomena.

nibbel11
Messages
36
Reaction score
2
e few days ago i talked with my teacher about the energy in the universe being constant. but we were completely confused when we came to the concept of:
"because of the universe expansion everything moves away from each other. and the same goes for the wavelenghts in light. because of the way electro-magnetic energy is being calculated. the energy increases with the wavelength but isn't converted in anything."
is this right or not
if not where was our mistake.
 
  • Like
Likes   Reactions: Lalpesh
Physics news on Phys.org
what is even the formula of the energy of a phonton
E=hλ
or
E=hf
 
Longer wavelength is lower energy.
 
nibbel11 said:
e few days ago i talked with my teacher about the energy in the universe being constant.
One problem with saying that the amount of energy in the universe is the same from one instant in time to the next is with defining the notion of one instant in time.

In classical Newtonian mechanics the notion of "at the same time" is taken for granted and conservation of energy works. In special relativity, the notion of "at the same time" depends on the coordinate system you choose but as long as you choose an inertial frame of reference, conservation of energy still works. But with general relativity and curved space time, there is no such thing as a globally inertial reference frame. The notion of "at the same" time becomes a matter of pure convention. Locally one can choose to use an inertial frame so that locally, conservation of energy still works. But globally, it does not.

This in addition to the problem with even properly defining "energy" at cosmic scales.
 
jbriggs444 said:
,, instant in time to the next is with defining the notion of one instant in time...
Well conventionally 'seconds' which can be measured by atomic clocks,
Ideally though we need to know if there is a quantized Planck time, either theoretically or in fact.
I won't be placing a bet on it.
 
rootone said:
Well conventionally 'seconds' which can be measured by atomic clocks,
Ideally though we need to know if there is a quantized Plank time, either theoretically or in fact.
I won't be placing a bet on it.
Simultaneity has nothing to do with units of time.
 
jbriggs444 said:
Simultaneity has nothing to do with units of time.
Fair enough, does that imply that in GR, simultaneity is not defined?
 
rootone said:
Fair enough, does that imply that in GR, simultaneity is not defined?
Yes
 
  • Like
Likes   Reactions: rootone
nibbel11 said:
the energy increases with the wavelength
The energy decreases with wavelength. But this still has the same problem. In fact, it is accepted that the radiation density of the universe has decreased more rapidly than the matter density of the universe because of this effect. Thermal energy is also reduced.
General relativity complicates things, but I think if you treat the universe as relatively smooth (using a fluid approximation), it is just a matter of defining an appropriate gravitational potential energy which accounts for the loss in radiation and thermal energy. Maybe this sounds like cheating, but the point is that if you contract the universe, you should be able to get back all the radiation energy that you "lost" by expanding the universe.
 
  • Like
Likes   Reactions: Lalpesh
  • #10
jbriggs444 said:
Yes
Yes too, but buses mostly do turn on time though (within acceptable limits of uncertainty)
 
  • #11
nibbel11 said:
what is even the formula of the energy of a phonton
E=hλ
or
E=hf
Check your units, E=hλ doesn't give the correct units for energy.
 
  • #12
rootone said:
Yes too, but buses mostly do turn on time though (within acceptable limits of uncertainty)
Indeed. The fact that GR does not prescribe a particular simultaneity convention does not preclude us from picking one that works locally.
 
  • #13
thanks everyone that helped a lot
:dademyday:
 

Similar threads

  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 9 ·
Replies
9
Views
4K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 53 ·
2
Replies
53
Views
5K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 19 ·
Replies
19
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 3 ·
Replies
3
Views
4K
  • · Replies 48 ·
2
Replies
48
Views
5K