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Monday, November 30, 2015

Basically, matter is the rarest thing in the universe (or at least it used to be)

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 0x2ex1dx2.4.

(b) Use the following values for the constants: kB=1.38×1016erg K1,c=3.00×1010cm s1,h=6.62×1027erg 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 9.2×1030g cm3 . The baryon density is about 4% of it. The masses of proton and neutron are very similar (1.7×1024G).
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=nhν
nν=Enνhν,
which can be defined with the equations for energy density as: nν=uνhν,
so uνdν=8πhPν3c31ehPνkBT1dν,
becomes: uνhνdν=1hν8πhPν3c31ehPνkBT1dν,
nνdν=8πν2c31ehPνkBT1dν,
and integrating it for all frequencies: 0nνdν=08πν2c31ehPνkBT1dν,
nallν=8πc3(kBThP)30ν2ehPνkBT1dν,
and knowing a particular equality established by the problem: 0x2ex1dx2.4,
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=1.38×1016erg K1,
c=3.00×1010cm s1,
h=6.62×1027erg s,
so:  
nall ν=8π3.00×(1010cm s1)3(1.38×1016erg K12.7K6.62×1027erg 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=9.2×1030g cm3
ρbaryons=0.04×ρuniverse,
and knowing the mass of a baryon, we can solve for the number density of baryons: ρbaryons=3.681031g cm3
nbaryons=ρbaryons/mbaryon
nbaryons=3.681031g cm3/1.71024gbaryon
nbaryon=2.16107baryonscm3


(d) Simply doing what the problem establishes, we have: nallν=4×102 photons/cm3
nbaryon=2.16471107baryonscm3
nall ν/nbaryon=1.85109photonsbaryons,
and indeed, there are billions of photons for every baryon. 

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