
Halon451
Audioholic Samurai
It's very interesting that all of this happened in the span of a mere second, and the universe as we know it commenced to exist. Admittedly, I am not quite as keen on the actual specifics of each era that you mentioned (with corresponding timeline mark and temperature), but have in the past done a little reading on the Grand Unified Theory, which is still, unfortunately only a theory at best. It does it's best explaining to simplify what you mentioned a bit, if I may, that because all of the universe's matter and energy existed in such an infinitely small area, that theoretically all known elementary forces could not act independently (I've nearly lost my mind trying to imagine the density!), therefore could only act as one unifying force that held the entire glob together. But I'm a nuclear engineer used to working with particles at energies between only 1 and 10 MeV (as they are called, "Prompt" neutrons), and rather pitiful in comparison to the actual energies estimated during the Big Bang, and even pitiful compared to the 14 TeV energies expected at each intersect point in the LHC when it is in full operation.You are correct sir!
One of the purposes of building larger and large particle colliders is to try and simulate the physics that occurred during the first few moments of the Big Bang when temperatures were extremely high. It is thought that during the "Quantum Era" (0 < t [time] < 10^-43 sec = Planck Time), that T (temperature of the Universe) > 10^32 K [Kelvin] and all the 4 natural forces (see my earlier post) acted as one. The Quantum Era ended when gravity decoupled from the other 3 forces -- such a decoupling is known as "symmetry breaking" in physics (somewhat analogous to a phase transition in matter). This lead to the "GUT (Grand Unified Theory) Era" (10^-43 s < t < 10^-35 s, T_ave = 10^27 K = 10^23 eV [electron-volt] = 10^11 TeV [tera-eV, 1 tera = 10^12]). During this era, the strong, electromagnetic (E/M), and weak forces acted as one and the temp. was so high that only field particles could exist. At 10^-35 s, the strong force decoupled from the electroweak force and this symmetry breaking lead to an inflationary expansion of the Universe (an exponential instead of the normal linear growth). This "Inflationary Era" ended at 10^-32 s when the Universe had a temp. of 10^25 K = 10^9 TeV. Individual quarks were made out of the field particles during this time. This would be the era when the Higgs Boson becomes important. This lead to the "Quark Era" (10^-32 s < t < 10^-6 s) which corresponded to the Universe resuming a linear expansion and it is during this era when the E/M and weak forces decouple from each other. This symmetry breaking is not nearly as energetic as the previous symmetry breaking and has no impact on the expansion of the Universe. The temp. of the Universe at this decoupling is about 10^15 K = 0.1 TeV. (We are now at the energies that the LHC can reach.) At the end of this era, T = 10^13 K = 1 GeV and we enter the "Hadronic Era" which lasts until the Universe celebrates its 1 second birthday.
I won't go any further at this point and I left out a lot of important events during the eras that I did mention. From what I understand, I don't think the LHC will get anywhere close to seeing any evidence of the Higgs Boson (and it certainly won't make any, one would need a collider that was a billion times more energetic to create Higgs Bosons). However, whenever physicists turn on a new, more energetic collider, they always find out something new. I'm sure that the LHC will produce some very interesting results. It's just too bad that the U.S. Congress cut the funding for the Superconducting Supercollider (SSC) when it did since I believe it was suppose to reach higher energies than the LHC.
All I can say is wow... and we'll see what mysteries the LHC indeed reveals.