Consider a system with 1000 particles that can only have two energies, &, and &, with ɛ, > E,. The difference between these two values is Aɛ = E, -&. Assume that gi = g2 1. Using the equation for the Boltzmann distribution graph the number of particles, n and m2, in states &, and &, as a function of temperature for a Aɛ = 1x10-2 J and for a temperature range from 2 to 300 K. (Note: kB = 1.380x10-23 J K-!. (6-6) 12 =e or n, n, 8,
Consider a system with 1000 particles that can only have two energies, &, and &, with ɛ, > E,. The difference between these two values is Aɛ = E, -&. Assume that gi = g2 1. Using the equation for the Boltzmann distribution graph the number of particles, n and m2, in states &, and &, as a function of temperature for a Aɛ = 1x10-2 J and for a temperature range from 2 to 300 K. (Note: kB = 1.380x10-23 J K-!. (6-6) 12 =e or n, n, 8,
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Transcribed Image Text:Consider a system with 1000 particles that can only have two energies, ɛ, and
with
ɛ, > E,. The difference between these two values is Aɛ = ɛ, -& . Assume that gi = g2 = 1. Using the
%3D
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equation for the Boltzmann distribution graph the number of particles, ni and m, in states &
n2,
E
and
E, as a
function of temperature for a Aɛ = 1×10-2' J and for a temperature range from 2 to 300 K. (Note: kg =
1.380x10-23 J K-!.
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(s,-s,)
gLe
Aɛ/
n2
or
= e
n,
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The number of particles in state 2 can be written as the following:
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