Liouville's theorem and time evolution of ensemble average

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SUMMARY

The discussion focuses on the application of Liouville's theorem to the time evolution of ensemble averages in Hamiltonian mechanics. The key equations presented include the time derivative of the probability density function, $$\frac{{d\rho }}{{dt}}$$, and the ensemble average $$\frac{{d\left\langle O \right\rangle }}{{dt}}$$, which is derived using integration by parts. The participants clarify the distinction between total derivatives and partial derivatives, emphasizing that the integration over phase space does not directly relate to time evolution of coordinates and momenta.

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Jeremy1986
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Question about using Liouville's theorem to calculate time evolution of ensemble average
With the Liouville's theorem
$$\frac{{d\rho }}{{dt}} = \frac{{\partial \rho }}{{\partial t}} + \sum\limits_{a = 1}^{3N} {(\frac{{\partial \rho }}{{\partial {p_a}}}\frac{{d{p_a}}}{{dt}} + \frac{{\partial \rho }}{{\partial {q_a}}}\frac{{d{q_a}}}{{dt}})} = 0$$
when we calculate the time evolution of the ensemble average of a quantity ## O(p,q)## we have
$$\frac{{d\left\langle O \right\rangle }}{{dt}} = \int {d\Gamma \frac{{\partial \rho (p,q,t)}}{{\partial t}}O(p,q)} = \sum\limits_{a = 1}^{3N} {\int {d\Gamma } } O(p,q)(\frac{{\partial \rho }}{{\partial {p_a}}}\frac{{\partial H}}{{\partial {q_a}}} - \frac{{\partial \rho }}{{\partial {q_a}}}\frac{{\partial H}}{{\partial {p_a}}})$$
here ## p,q## represents a bunch of generalized coordinates and momentum ## {p_a},{q_a},a = 1,...,3N## .
Then by using the method of integration by parts, the above integration becomes
$$\frac{{d\left\langle O \right\rangle }}{{dt}} = - \sum\limits_{a = 1}^{3N} {\int {d\Gamma } } \rho [(\frac{{\partial O}}{{\partial {p_a}}}\frac{{\partial H}}{{\partial {q_a}}} - \frac{{\partial O}}{{\partial {q_a}}}\frac{{\partial H}}{{\partial {p_a}}}) + O(\frac{{{\partial ^2}H}}{{\partial {p_a}\partial {q_a}}} - \frac{{{\partial ^2}H}}{{\partial {q_a}\partial {p_a}}})$$Here comes my questions, I think the integration by parts uses ## \int {d{p_a}} \frac{{\partial \rho }}{{\partial {p_a}}} = \int {d\rho }## . However as
## \rho$ ~$\rho (p,q,t)## , should we have ## \frac{{d\rho }}{{d{p_a}}} = \frac{{\partial \rho }}{{\partial {p_a}}} + \frac{{\partial \rho }}{{\partial t}}\frac{{dt}}{{d{p_a}}}## .


I take that last relation for granted because when we calculate ## \frac{{dy}}{{dx}}## , if ## y=y(x)## determines implicitly by some relation ## F(x,y)=0## , we use
$$\frac{{\partial F(x,y)}}{{\partial x}} + \frac{{\partial F(x,y)}}{{\partial y}}\frac{{dy}}{{dx}} = 0$$ and get $$\frac{{dy}}{{dx}} = - \frac{{\frac{{\partial F(x,y)}}{{\partial x}}}}{{\frac{{\partial F(x,y)}}{{\partial y}}}}$$ If we differentiate ## F(x,y)=0## with y, in order to get the same value of ## \frac{{dy}}{{dx}}## , we need to have
$$\frac{{\partial F(x,y)}}{{\partial x}}\frac{{dx}}{{dy}} + \frac{{\partial F(x,y)}}{{\partial y}} = 0$$ where we consider ## x## ~## x(y)## . So back to the ## \rho## case, in calculating ## \frac{{d\rho }}{{d{p_a}}}## , I think ## \frac{{\partial \rho }}{{\partial t}}\frac{{dt}}{{d{p_a}}}## term should be taken into account since ## p_a## ~## p_a(t)## . Then the integration by parts seems to be wrong, so I think I have made a mistake.______________________________________________________________________

My second question concerns Liouville's theorem itself, if we have ## \frac{{d\rho }}{{dt}}=0## , then can we have ## \frac{{d\rho }}{{d{q_a}}} = \frac{{d\rho }}{{dt}}\frac{{d{q_a}}}{{dt}} = 0## ? It sounds ridiculous as it indicates that the probability density is everywhere the same in the phase space, regardless of what the system is. Then where did I make a mistake? Thanks for your patience reading my long questions!
 
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Concerning the "integration by parts" question: In multidimensional integration "integration by parts" means to apply the generalized Gauss's theorem in arbitrary dimensions. E.g., for the first piece in your integral (Einstein summation convention applies!),
$$\int \mathrm{d} \Gamma O \frac{\partial \rho}{\partial p_a} \frac{\partial H}{\partial q_a} = \int \mathrm{d} \Gamma [\partial_{p_a} (O \rho \partial_{q_a} H)-\rho \partial_{p_a} (O \partial_{q_a} H)].$$
Now the first is a total divergence in ##p## space and the integral over ##\mathrm{d}^{3N} p## gives a hyper-surface integral due to Gauss's theorem. Since you assume that ##\rho## drops to 0 sufficiently fast at infinity of phase space, this contribution can be dropped, and you are left with the other phase-space integral. Combining everything leads to the desired result (just go on calculating; the result is very intuitive!).

The 2nd question doesn't make sense to me. What is a total derivative of ##\rho## wrt. ##q_a##? Of course ##\rho## is not uniform across phase space. This wouldn't be a properly normalized distribution: Integrating over entire phase space should give the particle number, which is finite!
 
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vanhees71 said:
Concerning the "integration by parts" question: In multidimensional integration "integration by parts" means to apply the generalized Gauss's theorem in arbitrary dimensions. E.g., for the first piece in your integral (Einstein summation convention applies!),
$$\int \mathrm{d} \Gamma O \frac{\partial \rho}{\partial p_a} \frac{\partial H}{\partial q_a} = \int \mathrm{d} \Gamma [\partial_{p_a} (O \rho \partial_{q_a} H)-\rho \partial_{p_a} (O \partial_{q_a} H)].$$
Now the first is a total divergence in ##p## space and the integral over ##\mathrm{d}^{3N} p## gives a hyper-surface integral due to Gauss's theorem. Since you assume that ##\rho## drops to 0 sufficiently fast at infinity of phase space, this contribution can be dropped, and you are left with the other phase-space integral. Combining everything leads to the desired result (just go on calculating; the result is very intuitive!).

The 2nd question doesn't make sense to me. What is a total derivative of ##\rho## wrt. ##q_a##? Of course ##\rho## is not uniform across phase space. This wouldn't be a properly normalized distribution: Integrating over entire phase space should give the particle number, which is finite!
Thank you very much for your nice reply! I think I start to understand my first question. What I was puzzled is actually the difference between ##\frac{{d\rho }}{{dt}}## and ##\frac{{\partial \rho }}{{\partial t}}##, which I now realized defines change in ##\rho## along the path in phase space determined by Hamiltonian and defines the variation of a field "##\rho##" with time at a fixed point in phase space. For the case of ensemble average, the integration is just over phase space, it does not relates to any evolution of ##{q,p}## in the phase space, so the ##{q,p}## in the integration has nothing to do with time t. The only time dependence in ##\left\langle O \right\rangle## is the variation of ##\rho## at each point in phase space.
 
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