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Distribution and Entropy

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When analyzing the probability of finding the system in a particular state, we observe that the equilibrium condition (\beta) is an integral part of the distribution's structure. Furthermore, it becomes evident that the function that best models the system is the logarithm of the number of states, which is associated with what we will term entropy.

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Forming a maximum

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When we multiply the number of cases, we obtain a function with a very pronounced peak.

The system is more likely to be found at the energy where the peak of the probability curve occurs.

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Taylor series for the number of states

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To study the behavior of the number of states function, we can expand it around the equilibrium energy value \bar{E}. If we do this expansion in the logarithm of the number of states, we obtain

\ln\Omega(E)=\ln\Omega(\bar{E})+\displaystyle\frac{\partial\ln\Omega}{\partial E}\eta+\displaystyle\frac{1}{2}\displaystyle\frac{\partial^2\ln\Omega}{\partial E^2}\eta^2\ldots



where \eta=E-\bar{E}. Using for the definition of

k_B T \equiv\displaystyle\frac{1}{ \beta }



and

\lambda\equiv-\displaystyle\frac{\partial^2\ln\Omega}{\partial E^2}=-\displaystyle\frac{\partial\ln\beta}{\partial E}



we obtain the expression with :

\ln\Omega(E)=\ln\Omega(\bar{E})+\beta\eta-\displaystyle\frac{1}{2}\lambda\eta^2\ldots

\beta
Beta del sistema
1/J
8823
\eta
Desviación de la energía
J
8829
\ln(\Omega(E))
Logaritmo del numero de estados del sistema con la energía E
-
8833
\ln(\Omega(\bar{E}))
Logaritmo del numero de estados del sistema con la energía media \bar{E}
-
8834
\lambda
Medida del ancho de la distribución de probabilidad
1/J^2
8830
S = k_B * ln( Omega ) S + S_h =maxdisplaystyle rac{1}{T}=displaystyle rac{partial S}{partial E}lnOmega(E)=lnOmega(ar{E})+etaeta-displaystyle rac{1}{2}lambdaeta^2ldotsP(E)=P(ar{E})e^{-lambda_0(E-ar{E})^2/2}lambda_0equiv-displaystyle rac{partial^2lnOmega}{partial E^2}=-displaystyle rac{partiallneta}{partial E}betak_BetaE_2EmESS_maxln_Omega_Eln_Omega_E_mlambdalambda_0Omega_EP_EP_0T

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Shape of the probability function

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If we consider the expansion of the number of states with beta del sistema 1/J, desviación de la energía J, logaritmo del numero de estados del sistema con la energía E -, logaritmo del numero de estados del sistema con la energía media \bar{E} - and medida del ancho de la distribución de probabilidad 1/J^2:

\ln\Omega(E)=\ln\Omega(\bar{E})+\beta\eta-\displaystyle\frac{1}{2}\lambda\eta^2\ldots



we can estimate the logarithm of the probability:

\ln P = \ln[\Omega(E)\Omega'(E')] = \ln\Omega(E) + \ln\Omega'(E') = \ln\Omega(\bar{E}) + \ln\Omega'(\bar{E'}) + (\beta - \beta')\eta - \frac{1}{2}(\lambda + \lambda')\eta^2\ldots



For the case of equilibrium, both betas are equal, and the probability that one of the systems has an energy E is reduced to a Gaussian distribution, which is expressed with beta del sistema 1/J, desviación de la energía J, logaritmo del numero de estados del sistema con la energía E -, logaritmo del numero de estados del sistema con la energía media \bar{E} - and medida del ancho de la distribución de probabilidad 1/J^2 as:

P(E)=P(\bar{E})e^{-\lambda_0(E-\bar{E})^2/2}



where

\lambda_0 = \lambda + \lambda'

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Distribution width

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The factor that defines the width of the probability curve is the quadratic factor in the Taylor series expansion, which is expressed with as follows:

\lambda_0\equiv-\displaystyle\frac{\partial^2\ln\Omega}{\partial E^2}=-\displaystyle\frac{\partial\ln\beta}{\partial E}



It can be shown that the introduced number \lambda is always positive. An indication of this comes from the function of the number of states we have already calculated for the case of free particles. In that case, as the number of states is proportional to the energy raised to the power of the number of degrees of freedom f, we find that with

\Omega\sim E^f



we have

\lambda_0\equiv-\displaystyle\frac{\partial^2\ln\Omega}{\partial E^2}=-f\displaystyle\frac{\partial^2\ln E}{\partial E^2}=\displaystyle\frac{f}{E^2}

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Definition of entropy based on possible states

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The key parameter in the study of equilibrium is given by the logarithm of the number of states, which with is expressed as:

\beta(E)\equiv\displaystyle\frac{\partial\ln\Omega}{\partial E}



The natural logarithm of the number of states multiplied by the Boltzmann constant k_B is defined as the system's entropy, which is expressed with as follows:

S \equiv k_B \ln \Omega

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Thermodynamics relationship

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The definition of \beta is found in

\beta(E)\equiv\displaystyle\frac{\partial\ln\Omega}{\partial E}



that of temperature is in

k_B T \equiv\displaystyle\frac{1}{ \beta }



and that of entropy is in constante de Boltzmann J/K, entropia del sistema J/K and numero de estados del sistema con la energía E -

S \equiv k_B \ln \Omega



These definitions lead us to a thermodynamic relationship that indicates how temperature T is related to constante de Boltzmann J/K, entropia del sistema J/K and numero de estados del sistema con la energía E -:

\displaystyle\frac{1}{T}=\displaystyle\frac{\partial S}{\partial E}

E
Energía del sistema
J
8719
S
Entropia del sistema
J/K
8831
T
Temperatura del sistema
K
8825
S = k_B * ln( Omega ) S + S_h =maxdisplaystyle rac{1}{T}=displaystyle rac{partial S}{partial E}lnOmega(E)=lnOmega(ar{E})+etaeta-displaystyle rac{1}{2}lambdaeta^2ldotsP(E)=P(ar{E})e^{-lambda_0(E-ar{E})^2/2}lambda_0equiv-displaystyle rac{partial^2lnOmega}{partial E^2}=-displaystyle rac{partiallneta}{partial E}betak_BetaE_2EmESS_maxln_Omega_Eln_Omega_E_mlambdalambda_0Omega_EP_EP_0T

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Entropy and system equilibrium

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With the definition of entropy as constante de Boltzmann J/K, entropia del sistema J/K and numero de estados del sistema con la energía E -:

S \equiv k_B \ln \Omega



and considering that in equilibrium it holds with :

\displaystyle\frac{\partial\ln\Omega}{\partial E}-\displaystyle\frac{\partial\ln\Omega_h}{\partial E_h}=0



we conclude that in equilibrium, the energy E must always be maximum with :

S + S_h =max

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