Our Evolving Universe
Self Test 11
Helium is formed in the early universe, but carbon is not, because
the early universe is too hot to form carbon
the early universe is too cool to form carbon
the process is blocked by the lack of stable nuclei with atomic mass 5 or 8
the neutron lifetime is not long enough for carbon to form
The cosmic microwave background was emitted
when matter and antimatter annihilated, a fraction of a second after the Big Bang
when helium was formed, about 3 minutes after the Big Bang
when electrons combined with nuclei to make neutral atoms, about 300,000 years after the Big Bang
when the first stars started to fuse hydrogen to helium, several million years after the Big Bang
There are now about a billion times more photons than protons because
almost all of the original matter annihilated with antimatter
the photons carry much less energy than the protons
the universe is radiation dominated
the universe is expanding
The extreme smoothness (isotropy) of the cosmic microwave background
is expected, because the universe started with a Big Bang
is surprising, because the universe started with a Big Bang
is expected, because the universe was smaller when the microwave background radiation was first emitted
is surprising, because light did not have time to travel across the now-visible universe before the background radiation was emitted
The inflation theory
explains why the cosmic microwave background is very isotropic
predicts that the universe should be flat (zero curvature)
involves a very short period of very rapid expansion a tiny fraction of a second after the Big Bang
all of the above
out of 5.
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Summary of Lecture 11
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Summary of Lecture 12
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