The flatness problem is the fact that the observed density of matter is unexpectedly differentfrom the critical density predicted by the inflationary epoch.
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Q31: Before about 50,000 years after the Big
Q32: The critical temperature above which pair production
Q33: Physicists have detected hot dark matter particles
Q34: Before about 4 billion years ago the
Q35: At this time, the universe is:
A)radiation dominated.
B)quark
Q37: How does the energy of the cosmic
Q38: Both protons and neutrons (and their
Q39: Pair production can occur if:
A)the energy of
Q40: When new particle pairs are being created
Q41: The period from about 100 seconds up
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