Robert J. Grave
- 34
- 0
Isn't the big bang, the universe from nothing, a violation of the consevation of mass/energy since mass/energy can not be created or destroyed?
The discussion revolves around the implications of the Big Bang theory on the conservation of mass and energy. Participants explore whether the concept of the universe emerging from "nothing" challenges established physical laws, particularly conservation principles, and delve into the philosophical and theoretical underpinnings of these ideas.
Participants express a range of views, with no consensus reached on whether the Big Bang theory challenges the conservation of mass and energy. Several competing interpretations and philosophical arguments are presented, indicating ongoing debate and uncertainty.
Participants note limitations in current understanding, particularly regarding the application of general relativity in extreme conditions and the lack of a clear definition of energy in the context of gravitational fields. The discussion also highlights the philosophical complexities surrounding the concept of existence and the implications of "nothing."
The Big Bang theory says that our universe once was in a very hot and dense state. What happened before that is open for speculation, since we do not know what physical laws hold under such extreme conditions. The quote "universe from nothing" mearly sounds like some creationism propaganda (i.e. something made up by people who have no clue what the Big Bang theory is about...)Robert J. Grave said:the big bang, the universe from nothing
The singularity is a consequence of GR, which we know is not a correct description of gravity under such extreme conditions. For that we need a quantum gravity theory, something we're still looking for. The singularity is hence just an artefact of applying a physical theory (GR) in a place (early universe) where it does not hold very good.Robert J. Grave said:The big bang therory, I understand, states that the universe began as a singularity at extreme tempatures and expanded from there.
wiki said:the Big Bang is the scientific theory that the universe emerged from a tremendously dense and hot state about 13.7 billion years ago.
EL said:The Big Bang theory says that our universe once was in a very hot and dense state. What happened before that is open for speculation, since we do not know what physical laws hold under such extreme conditions. The quote "universe from nothing" mearly sounds like some creationism propaganda (i.e. something made up by people who have no clue what the Big Bang theory is about...)
hellfire said:heusdens, Vilenkin does not use the term "nothing" to mean nothing at all (as done in philosophy), but to describe a state of vanishing classical space. Take a look to this post and the link there.
wxrocks said:My 2 cents -- Really -- the first 100 to 1000 seconds of existence are pure theory/speculation anyway. Anyone who is trying to explain the universe before that time is selling something! Because we don't have a good understanding of the physics at those extreme conditions, there is no way to say what the universe was doing before that point. Was it nothing, was it something, was it whatever -- all these questions can be asked, but to say for sure it was one way or another is pretty much a guess.
heusdens said:Inflation is past time eternal in the sense that 'once' it occurs, it can go on forever, which also leads to the conclusion, it didn't have to start at some time.
In general, the conservation equation that applies in cosmology follows from the divergenceless energy-momentum tensor of a perfect fluid that describes some of the components of the universe:heusdens said:But to go back to the topic (conservation of mass/energy) how does inflation treat these? I assume the conservation of mass/energy is still valid under inflation?
[itex] <br /> Yes, but if an inflating region keeps it energy density while growing exponentially, this means that there is going to be more energy.[/itex]hellfire said:In general, the conservation equation that applies in cosmology follows from the divergenceless energy-momentum tensor of a perfect fluid that describes some of the components of the universe:
[tex]\partial_0 \rho + 3H(\rho + p) = 0[/tex]
During inflation the energy density of the scalar field that drives inflation remains constant, but [itex]p = - \rho[/tex] and the equation is satisfied.[/itex]