Does the expansion of the universe violate conservation of energy?

Click For Summary

Discussion Overview

The discussion revolves around whether the expansion of the universe violates the conservation of energy, exploring concepts related to gravitational potential energy, dark energy, and the implications of cosmic expansion on energy conservation. The scope includes theoretical considerations and interpretations of cosmological models.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Exploratory

Main Points Raised

  • Some participants propose that as the distance between galaxies increases, it may imply that matter in those galaxies gains potential gravitational energy, raising questions about the source of this energy.
  • Others argue that in a homogeneous and isotropic universe, the net gravitational pull on isolated galaxies cancels out, suggesting that the increase in distance does not do work in a straightforward manner.
  • A participant mentions that the expansion of the universe consists of two components: the initial expansion from inflation and the later acceleration attributed to dark energy, with implications for energy conservation.
  • One viewpoint suggests that during the original expansion, energy merely changes form without being created or destroyed, aligning with the first law of thermodynamics.
  • Another perspective posits that dark energy may represent newly created energy due to the expansion of the universe, potentially arising from quantum fluctuations, and that standard theory does not assume energy conservation applies to this energy increase.
  • A participant questions the notion of energy conservation on cosmological scales, noting that the total energy of the universe is poorly defined.
  • There is a discussion about the relationship between gravitational energy and expansionary energy, with one participant suggesting that they balance out to a net zero, while another counters that the expansionary energy is greater than the gravitational energy.

Areas of Agreement / Disagreement

Participants express multiple competing views on the relationship between cosmic expansion and energy conservation, with no consensus reached on whether the expansion violates conservation principles or how energy behaves on cosmological scales.

Contextual Notes

Limitations include the ill-defined nature of total energy in the universe and the complexities surrounding the roles of dark energy and gravitational interactions in the context of cosmic expansion.

Anzas
Messages
87
Reaction score
0
Since the distance between galaxies increases with time does that mean that the matter in those galaxies gets potential gravitational energy? and if so where does this energy come from?
 
Space news on Phys.org
Anzas said:
Since the distance between galaxies increases with time does that mean that the matter in those galaxies gets potential gravitational energy?

I don't think that happens in any simple way, Anzas, because in a uniform (homogeneous isotropic) universe there is negligible net pull on an isolated galaxy or cluster of galaxies.
the pulls in different directions cancel out

Were there a net pull on a galaxy that would probably be in a gravitationally bound structure, like a cluster. But the average increase in distance doesn't apply within clusters. Hubble law refers to average longrange distances and doesn't apply equally across the board. Within gravitationally bound systems average distances may not be increasing at all!

So to a first approximation you can say that if the distance between two widely separated things A and B is increasing according to Hubble Law, then the increase in distance is not doing work at least in any obvious straightforward way, because there is no net force on A towards B.

think of the balloon analog with pennies stuck on the balloon surface representing clusters of galaxies. each penny attracts every other along geodesics in the surface (but not acrosss the empty space inside the balloon which does not exist :smile:). each penny is attracted about equally in all directions (2D directions within the space). no net force on it in anyone particular direction

there's more to say, but I have to go. maybe someone else will elaborate.
 
Hi Anzas,
Anzas said:
Since the distance between galaxies increases with time does that mean that the matter in those galaxies gets potential gravitational energy? and if so where does this energy come from?
There are two components to the expansion: the original expansion thought to result from inflation, and the late times acceleration of the expansion thought to be caused by dark energy.

Regarding the original expansion: In a Newtonian sense, as the universal expansion decelerates over time due to the cosmic gravitation, the galaxies' kinetic energy of expansion converts to potential energy of distance. No energy is gained or lost, it just changes form. This expansion conserves energy; it is modeled on the first law of thermodynamics for a closed system.

Regarding the late times acceleration caused by dark energy: This is thought to be energy which is newly created as a result of the volume expansion of the universe. This energy is thought to most likely come from quantum fluctuations in empty space. As far as I know, standard theory does not assume that energy conservation applies to increase in this energy. We just don't know enough about what it is and how it works.

Jon
 
  • Like
Likes   Reactions: RogerWaters
I see, thanks for your answers.
 
in my limited understanding and correct me if I am wrong but the energy of inflation / expansion has gravity, and gravity being a negative energy, they ballance out to a net zero?
 
Hi TalonD,

Dark Energy in its simplest theoretical form, the cosmological constant, is believed to possesses both gravitational mass-energy and expansionary energy. The expansionary energy is in the form of negative pressure, or tension.

The gravity and expansion energy of the cosmological constant do not entirely cancel out. Its expansion energy is 3x its 1x gravity; so after netting out the deceleration component of gravity, the net acceleration energy is 2x.

The fact that there is net acceleration energy explains why the universe has stopped decelerating and begun reaccelerating since around the 7Gy mark in its history.

Jon
 
I think one has to be careful talking about the conservation of energy over cosmological scales when the total energy of the universe is ill-defined.
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 3 ·
Replies
3
Views
4K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
Replies
18
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 12 ·
Replies
12
Views
4K
  • · Replies 17 ·
Replies
17
Views
6K
  • · Replies 23 ·
Replies
23
Views
4K
  • · Replies 14 ·
Replies
14
Views
4K