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CY_Leung
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Homework Statement
1 mm3 of gas at normal pressure and temperature contains about 1015 particles. Considering the particles as point-like and classical, provide a rough, conservative estimate for how many hard drives would be necessary to store the initial conditions of all gas particles. (As in 2013, a normal hard drive can store about 5 TB data.)
Homework Equations
This is the first course of statistical mechanics and actually we are not informed about the information theory in the class, except for the mathematical expression of information entropy. The following is all I know:
1 bit (1 Shannon) is defined as the amount of information of an event that occurs with a probability of 1/2.
Where 1 byte = 8 bits, 1 KB = 1000 bytes, 1 MB = 1000 KB, 1 GB = 1000 MB, 1 TB = 1000 GB
For an event with probability p, the number of bits of the corresponding amount of information is equal to -log2p.
Then the expected value of number of bits of a sample space is given by Σpilog2pi, which is actually the information entropy.
As for continuous probability distribution, one may write the information entropy as:
-∫p(x)log2p(x)dx
The Attempt at a Solution
Each classical and point-like particle can be fully described by (x,v) (or (x,p), doesn't really matter here). My interpretation of the question is: calculate the information entropy of the gas with the logarithmic base 2.
For information entropy is additive, i.e. for independent events, the total information entropy can be just summed.
I(p1p2) = I(p1) + I(p2) (read that from Wikipedia)
Thus velocities and positions of the particles can be considered separately, and each individual particle can also be considered separately.
First consider the velocity of a particle. What comes to my mind directly is the Maxwell-Boltzmann probability distribution. For ease of expression, the probability distribution can be written as:
p(v)=Cv2e-βv2, C being the normalization constant and β = m/2kT.
Do the integration:
[tex]I(\overrightarrow{v})=-C\int_{0}^{\infty}\overrightarrow{v}^{2}e^{-\beta\overrightarrow{v}^{2}}{log}_{2}(\overrightarrow{v}^{2}e^{-\beta\overrightarrow{v}^{2}})d\overrightarrow{v}
=-\frac{C}{{ln}2}\int_{0}^{\infty}\overrightarrow{v}^{2}e^{-\beta\overrightarrow{v}^{2}}(2{ln}|\overrightarrow{v}|-\beta\overrightarrow{v}^{2}) d\overrightarrow{v}[/tex]
For the gas is under normal condition, the velocities of the particles are not too large and we may omit the term [tex]ln|\overrightarrow{v}|[/tex]. By this approximation the result of the integration would be 3/(2 ln2) according to my computation.
But I have no idea how to do this for particle positions. I attempted in the following way:
[tex]I(\overrightarrow{x})=-\int_{V}^{ } p(\overrightarrow{x})log_{2} p(\overrightarrow{x}) d\overrightarrow{x} [/tex]
[tex]V[/tex] being the volume bounded by the gas, [tex]p(\overrightarrow{x})[/tex] is the uniform probability density distribution. But now comes the problem: How should I do the logarithm of the uniform probability density distribution function, which is not dimensionless and depends on the unit we use for volume?
Or is the above approach correct at all? Thanks.