We are
bounded in a nutshell of Infinite space: Blog Post #35, Worksheet # 11.1, Problem #3: Basically,
matter is the rarest thing in the universe (or at least it used to be)
3. Baryon-to-photon ratio of our universe.
(a) Despite the fact that the CMB has a very
low temperature (that you have calculated above), the number of photons is
enormous. Let us estimate what that number is. Each photon has energy hν. From the Plank Spectrum Equation, figure out the number density, nν,
of the photon per frequency interval dν. Integrate over dνto
get an expression for total number density of photon given temperature T. Now you need to keep all factors, and
use the fact that ∫∞0x2ex−1dx≈2.4.
(b) Use the following values for the constants:
kB=1.38×10−16erg K−1,c=3.00×1010cm s−1,h=6.62×10−27erg s , and use the
temperature of CMB today that you have computed from 2d), to calculate the
number density of photon today in our universe today (i.e. how many photons per
cubic centimeter?)
(c) Let us calculate the average baryon number
density today. In general, baryons refer to protons or neutrons. The
present-day density (matter + radiation + dark energy) of our Universe is 9.2×10−30g cm−3 . The baryon density is about 4% of it.
The masses of proton and neutron are very similar (≈1.7×10−24G).
What is the number density of baryons?
(d) Divide the above two numbers, you get the
baryon-to-photon ratio. As you can see, our universe contains much more photons
than baryons (proton and neutron).
(a) Knowing the energy of a single photon, a
simple scale value defines all photon’s energy: E=hν
En=n⋅hν
nν=Enνhν,
which can be defined with the
equations for energy density as: nν=uνhν,
so uνdν=8πhPν3c31ehPνkBT−1dν,
becomes: uνhνdν=1hν⋅8πhPν3c31ehPνkBT−1dν,
nνdν=8πν2c31ehPνkBT−1dν,
and integrating it for all frequencies: ∫∞0nνdν=∫∞08πν2c31ehPνkBT−1dν,
nallν=8πc3(kBThP)3∫∞0ν2ehPνkBT−1dν,
and knowing a particular equality established by the problem:
∫∞0x2ex−1dx≈2.4,
we have the final
description of the number of photons as: nall ν=8πc3(kBThP)3(2.4)
(b) And now
plugging in the values given in the problem, we have: nall ν=8πc3(kBThP)3(2.4)
kB=1.38×10−16erg K−1,
c=3.00×1010cm s−1,
h=6.62×10−27erg s,
so:
nall ν=8π3.00×(1010cm s−1)3(1.38×10−16erg K−1⋅2.7K6.62×10−27erg s)3(2.4),
and thus the density of photons is: nall ν=4×102 photons/cm3
(c) Being given the density of mass in the
universe, we can now solve for baryon density in particular: ρuniverse=9.2×10−30g cm−3
ρbaryons=0.04×ρuniverse,
and knowing the mass of a baryon, we can solve for the number density of
baryons: ρbaryons=3.68∗10−31g cm−3
nbaryons=ρbaryons/mbaryon
nbaryons=3.68∗10−31g cm−3/1.7∗10−24gbaryon
nbaryon=2.16∗10−7baryonscm3
(d) Simply
doing what the problem establishes, we have: nallν=4×102 photons/cm3
nbaryon=2.16471∗10−7baryonscm3
nall ν/nbaryon=1.85∗109photonsbaryons,
and indeed, there are
billions of photons for every baryon.
Very nice!
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