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DoobleD
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I read that the GUT epoch is estimated to have ended at around 10-36 s, but I can't find any proof or derivation for this. Anyone knows ?
DoobleD said:I read
PeterDonis said:Where? Please give a specific reference.
DoobleD said:I read that the GUT epoch is estimated to have ended at around 10-36 s, but I can't find any proof or derivation for this. Anyone knows ?
PeterDonis said:Where? Please give a specific reference.
George Jones said:Try using (3.2.68) of Daniel Baumann's (Cambridge) excellent cosmology lecture notes
http://www.damtp.cam.ac.uk/user/db275/Cosmology/Lectures.pdf
to find tGUTtGUTt_\rm{GUT} for TGUT≈1015 GeVTGUT≈1015 GeVT_\rm{GUT} \approx 10^{15} ~\rm{GeV} and g∗≈10g∗≈10g_* \approx 10.
DoobleD said:Seems to be it, thank you ! I get, using ##T_\rm{GUT} \approx 10^{15} ~\rm{GeV} = 10^{18} MeV## :
##t \approx \frac{9}{4\sqrt{10}T^2} \approx 7 \times 10^{-37} s##, which is close enough.
DoobleD said:One thing I'm not sure about though is why the choice of ##g_* \approx 10## degrees of freedom ?
George Jones said:We are only looking at order of magnitude stuff. Even so, this is probably too small by an order of magnitude or so, since TGUT≈1015 GeVTGUT≈1015 GeVT_\rm{GUT} \approx 10^{15} ~\rm{GeV} or TGUT≈1016 GeVTGUT≈1016 GeVT_\rm{GUT} \approx 10^{16} ~\rm{GeV} for the Minimal Supersymmetric Standard Model (MSSM), which has loads of particle species.
George Jones said:I have a few books that give expressions equivalent to Baumann's (3.2.68), but, as far as I can see, I have only one book that explicitly uses this expression to estimate tGUTtGUTt_\rm{GUT}, "Introduction to General Relativity" by Lewis Ryder.
The GUT epoch, or Grand Unification Theory epoch, is a period of time in the early universe, lasting from approximately 10^-36 seconds after the Big Bang to 10^-32 seconds. During this time, the four fundamental forces of nature (gravity, electromagnetism, strong nuclear force, and weak nuclear force) were still unified into a single force.
The end of the GUT epoch is marked by a process called symmetry breaking, where the unified force splits into the four separate forces we see today. This occurred as the universe continued to expand and cool, causing the energy levels to drop and the forces to become distinct.
One major piece of evidence for the GUT epoch is the fact that the four fundamental forces we observe today can be mathematically unified at high energies, suggesting that they were once a single force. Additionally, observations of the cosmic microwave background radiation, the leftover energy from the Big Bang, also support the existence of this early period in the universe's history.
While the GUT epoch is a well-supported theory, there are still some unanswered questions about this period in the universe's history. For example, scientists are still trying to understand the exact process of symmetry breaking and what caused it to occur at a specific time during the universe's expansion.
During the GUT epoch, the universe was still too hot and energetic for matter to form. However, as the universe continued to expand and cool, the energy levels dropped enough for particles to start combining to form protons and neutrons. This ultimately led to the formation of atoms and the beginning of the matter-dominated era of the universe.