brownian motion

The equation explained

S=EˉT+2ϰlg⁡∫e−E2ϰTdp1…dpl.S = \frac{\bar{E}}{T} + 2 \varkappa \lg \int e^{-\frac{E}{2 \varkappa T}} d p_1 \ldots d p_l.
In wordsThe entropy of the system is the energy of the system divided by the absolute temperature, plus twice the constant kappa times the logarithm of an integral, taken over every combination of values of the state variables the problem allows, of e raised to minus the energy as a function of those variables divided by twice kappa times the temperature.OverviewFor such a system the entropy is its mean energy over the temperature, plus a term that counts the states available to it: the logarithm of an integral in which a state of high energy counts for little and one of low energy for much.Full explanationThe letters are named in the sentence under the display. TT is the absolute temperature, Eˉ\bar{E} the energy of the system, EE the energy as a function of the pνp_\nu, and the integral is to be taken over all combinations of values of the pνp_\nu compatible with the conditions of the problem. The bar matters: Eˉ\bar{E} is one number, the energy the system has, while EE under the integral is a function that takes a different value at each combination of the state variables. The constant ϰ\varkappa is not left free. The text ties it to the NN of section 1 by 2ϰN=R2 \varkappa N = R, so 2ϰ2\varkappa is the gas constant RR divided by the number of molecules in a gram-molecule: the gas constant for a single molecule. Put that in and the exponent becomes −EN/RT-EN/RT, which is the form the free energy of the next display is printed in.Every stepS=EˉT+2ϰlg⁡∫e−E2ϰTdp1…dplS = \frac{\bar{E}}{T} + 2 \varkappa \lg \int e^{-\frac{E}{2 \varkappa T}} d p_1 \ldots d p_lAs printed. The integral runs over the whole space of the state variables, restricted only by the conditions of the problem, and dp1…dpld p_1 \ldots d p_l is its element of volume.2ϰN=R2 \varkappa N = RThe relation the same paragraph states between ϰ\varkappa and the NN of section 1, the number of real molecules in a gram-molecule.2ϰ=RN2 \varkappa = \frac{R}{N}Divide by NN. The gas constant belongs to a gram-molecule, so R/NR/N is what belongs to one molecule.E2ϰT=ENRT\frac{E}{2 \varkappa T} = \frac{E N}{R T}The exponent with 2ϰ2\varkappa replaced. Dividing by R/NR/N is multiplying by N/RN/R.S=EˉT+RNlg⁡∫e−ENRTdp1…dplS = \frac{\bar{E}}{T} + \frac{R}{N} \lg \int e^{-\frac{E N}{R T}} d p_1 \ldots d p_lThe same entropy in the letters of section 1, with RR and NN in place of ϰ\varkappa in both the factor and the exponent.Historian's marginThe paper fixes ϰ\varkappa only through 2ϰN=R2 \varkappa N = R, so 2ϰ2\varkappa is the quantity later written kBk_B and ϰ\varkappa is half of it. The notation concordance records the halving, because reading ϰ\varkappa as Boltzmann's constant would double every energy this section counts.Also

Read it in the paper