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Boltzmann equation the quantum Boltzmann equation, also known as the Uehling–Uhlenbeck equation, is the quantum mechanical modification of the Boltzmann equation, which gives the nonequilibrium time evolution of a gas of quantum-mechanically interacting particles. Typically, the quantum Boltzmann equation is given as only the “collision term” of the full Boltzmann equation, giving the change of the momentum distribution of a locally homogeneous gas, but not the drift and diffusion in space. In full generality (including the p-space and x-space drift terms, which are often neglected) the equation is represented analogously to the Boltzmann equation. The quantum Boltzmann equation gives irreversible behavior, and therefore an arrow of time; that is, after a long enough time it gives an equilibrium distribution which no longer changes. Although quantum mechanics is microscopically time-reversible, the quantum Boltzmann equation gives irreversible behavior because phase information is discarded only the average occupation number of the quantum states is kept. The solution of the quantum Boltzmann equation is therefore a good approximation to the exact behavior of the system on time scales short compared to the Poincaré recurrence time, which is usually not a severe limitation, because the Poincaré recurrence time can be many times the age of the universe even in small systems. The quantum Boltzmann equation has been verified by direct comparison to time-resolved experimental measurements, and in general has found much use in semiconductor optics. For example, the energy distribution of a gas of excitons as a function of time (in picoseconds), measured using a streak camera, has been shown to approach an equilibrium Maxwell-Boltzmann distribution. A typical model of a semiconductor may be built on the assumptions that:

Application to semiconductor physics

A typical model of a semiconductor may be built on the assumptions that:

The electron distribution is spatially homogeneous to a reasonable approximation (so all x-dependence may be suppressed)
The external potential is a function only of position and isotropic in p-space, and so $𝐅$ may be set to zero without losing any further generality
The gas is sufficiently dilute that three-body interactions between electrons may be ignored.

Considering the exchange of momentum $𝐪$ between electrons with initial momenta $𝐤$ and $𝐤_{𝟏}$ , it is possible to derive the expression $\begin{matrix} 𝒬 [f] (𝐤) & = \frac{- 2}{ℏ (2 π)^{5}} \int d 𝐪 \int d 𝐤_{𝟏} | \hat{v} (𝐪) |^{2} \\ \times δ (\frac{ℏ^{2}}{2 m} (| 𝐤 - 𝐪 |^{2} + | 𝐤_{𝟏} + 𝐪 |^{2} - 𝐤_{1}^{2} - 𝐤^{2})) \\ \times [f_{𝐤} f_{𝐤_{𝟏}} (1 - f_{𝐤 - 𝐪}) (1 - f_{𝐤_{𝟏} + 𝐪}) - f_{𝐤 - 𝐪} f_{𝐤_{𝟏} + 𝐪} (1 - f_{𝐤}) (1 - f_{𝐤_{𝟏}})] \end{matrix}$

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-The '''quantum Boltzmann equation,''' also known as the '''Uehling–Uhlenbeck equation''',<ref>{{cite journal |last1=Filbet |first1=Francis |last2=Hu |first2=Jingwei |last3=Jin |first3=Shi |title=A Numerical Scheme for the Quantum Boltzmann Equation Efficient in the Fluid Regime |journal=Esaim: M2An |year=2012 |volume=46 |issue=2 |pages=443–463|doi=10.1051/m2an/2011051|arxiv=1009.3352}}</ref><ref>{{cite book |last1=Bao |first1=Weizhu |last2=Markowich |first2=Peter |last3=Pareschi |first3=Lorenzo|chapter=Quantum kinetic theory: Modelling and numerics for Bose-Einstein condensation |title=Modeling and Computational Methods for Kinetic Equations |series=Modeling and Simulation in Science, Engineering and Technology |year=2004|pages=287–320|doi=10.1007/978-0-8176-8200-2_10|isbn=978-1-4612-6487-3 }}</ref> is the [[Physics:Quantum mechanics|quantum mechanical]] modification of the [[Boltzmann equation]], which gives the nonequilibrium [[Time evolution|time evolution]] of a gas of quantum-mechanically interacting particles. Typically, the quantum Boltzmann equation is given as only the “collision term” of the full Boltzmann equation, giving the change of the momentum distribution of a locally homogeneous gas, but not the drift and diffusion in space. It was originally formulated by [[Biography:Lothar Wolfgang Nordheim|L.W. Nordheim]] (1928),<ref>{{Cite journal|last1=Nordhiem|first1=L. W.|last2=Fowler|first2=Ralph Howard|date=1928-07-02|title=On the kinetic method in the new statistics and application in the electron theory of conductivity|journal=Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character|volume=119|issue=783|pages=689–698|doi=10.1098/rspa.1928.0126|bibcode=1928RSPSA.119..689N|doi-access=free}}</ref> and by and E. A. Uehling and [[Biography:George Uhlenbeck|George Uhlenbeck]] (1933).<ref>{{Cite journal|last1=Uehling|first1=E. A.|last2=Uhlenbeck|first2=G. E.|date=1933-04-01|title=Transport Phenomena in Einstein-Bose and Fermi-Dirac Gases. I|url=https://link.aps.org/doi/10.1103/PhysRev.43.552|journal=Physical Review|language=en|volume=43|issue=7|pages=552–561|doi=10.1103/PhysRev.43.552|bibcode=1933PhRv...43..552U|issn=0031-899X|url-access=subscription}}</ref>
+{{Short description|Quantum Collection topic on Quantum Boltzmann equation}}
+{{Quantum book backlink|Statistical mechanics and kinetic theory}}
+{{Quantum article nav|previous=Physics:Quantum Kinetic theory|previous label=Kinetic theory|next=Physics:Quantum BBGKY hierarchy|next label=BBGKY hierarchy}}
+<div style="display:flex; gap:24px; align-items:flex-start; max-width:1200px;">
-In full generality (including the p-space and x-space drift terms, which are often neglected) the equation is represented analogously to the Boltzmann equation.
+<div style="width:280px;">
-<math display="block">
+__TOC__
-\left[\frac{\partial}{\partial t} + \mathbf{v} \cdot \nabla_x + \mathbf{F} \cdot \nabla_p \right] f(\mathbf{x},\mathbf{p},t) = \mathcal{Q}[f](\mathbf{x},\mathbf{p})
+</div>
-</math>
-where <math>\mathbf{F}</math> represents an externally applied potential acting on the gas' p-space distribution and <math>\mathcal{Q}</math> is the collision operator, accounting for the interactions between the gas particles. The quantum mechanics must be represented in the exact form of <math>\mathcal{Q}</math>, which depends on the physics of the system to be modeled.<ref>{{cite journal |last1=Filbert |first1=Francis |last2=Hu |first2=Jingwei |last3=Jin |first3=Shi |title=A Numerical Scheme for the Quantum Boltzmann Equation Efficient in the Fluid Regime |journal=Esaim: M2An |year=2012 |volume=46 |issue=2 |pages=443–463|doi=10.1051/m2an/2011051|arxiv=1009.3352}}</ref>
+<div style="flex:1; line-height:1.45; color:#006b45; column-count:2; column-gap:32px; column-rule:1px solid #b8d8c8;">
+'''Boltzmann equation''' the quantum Boltzmann equation, also known as the Uehling–Uhlenbeck equation, is the quantum mechanical modification of the Boltzmann equation, which gives the nonequilibrium time evolution of a gas of quantum-mechanically interacting particles. Typically, the quantum Boltzmann equation is given as only the “collision term” of the full Boltzmann equation, giving the change of the momentum distribution of a locally homogeneous gas, but not the drift and diffusion in space. In full generality (including the p-space and x-space drift terms, which are often neglected) the equation is represented analogously to the Boltzmann equation. The quantum Boltzmann equation gives irreversible behavior, and therefore an arrow of time; that is, after a long enough time it gives an equilibrium distribution which no longer changes. Although quantum mechanics is microscopically time-reversible, the quantum Boltzmann equation gives irreversible behavior because phase information is discarded only the average occupation number of the quantum states is kept. The solution of the quantum Boltzmann equation is therefore a good approximation to the exact behavior of the system on time scales short compared to the Poincaré recurrence time, which is usually not a severe limitation, because the Poincaré recurrence time can be many times the age of the universe even in small systems. The quantum Boltzmann equation has been verified by direct comparison to time-resolved experimental measurements, and in general has found much use in semiconductor optics. For example, the energy distribution of a gas of excitons as a function of time (in picoseconds), measured using a streak camera, has been shown to approach an equilibrium Maxwell-Boltzmann distribution. A typical model of a semiconductor may be built on the assumptions that:
+</div>
-The quantum Boltzmann equation gives irreversible behavior, and therefore an [[Physics:Entropy (arrow of time)|arrow of time]]; that is, after a long enough time it gives an equilibrium distribution which no longer changes. Although quantum mechanics is microscopically time-reversible, the quantum Boltzmann equation gives irreversible behavior because phase information is discarded<ref>{{cite journal |last1=Snoke |first1=D.W. |last2=Liu |first2=G. |last3=Girvin |first3=S.M. |title=The basis of the Second Law of thermodynamics in quantum field theory |journal=[[Physics:Annals of Physics|Annals of Physics]] |year=2012 |volume=327 |issue=7 |pages=1825–1851 |bibcode=2012AnPhy.327.1825S |doi=10.1016/j.aop.2011.12.016|arxiv=1112.3009 |s2cid=118666925 }}</ref> only the average occupation number of the quantum states is kept. The solution of the quantum Boltzmann equation is therefore a good approximation to the exact behavior of the system on time scales short compared to the [[Poincaré recurrence theorem|Poincaré recurrence time]], which is usually not a severe limitation, because the Poincaré recurrence time can be many times the [[Astronomy:Age of the universe|age of the universe]] even in small systems.
+<div style="width:300px;">
+[[File:Quantum_Boltzmann_equation_yellow.png|thumb|240px]]
+</div>
-The quantum Boltzmann equation has been verified by direct comparison to time-resolved experimental measurements, and in general has found much use in [[Physics:Semiconductor|semiconductor]] optics.<ref>{{cite journal |last1=Snoke |first1=D.W. |title=The quantum Boltzmann equation in semiconductor physics |journal=[[Physics:Annalen der Physik|Annalen der Physik]] |year=2011 |volume=523 |issue=1–2 |pages=87–100 |bibcode=2011AnP...523...87S |doi=10.1002/andp.201000102|arxiv=1011.3849 |s2cid=119250989 }}</ref> For example, the energy distribution of a gas of [[Physics:Exciton|exciton]]s as a function of time (in picoseconds), measured using a [[Engineering:Streak camera|streak camera]], has been shown<ref>{{cite journal |last1=Snoke |first1=D. W. |last2=Braun |first2=D. |last3=Cardona |first3=M. |title=Carrier thermalization in Cu<sub>2</sub>O: Phonon emission by excitons |journal=[[Physics:Physical Review B|Physical Review B]] |year=1991 |volume=44 |issue=7 |pages=2991–3000 |bibcode=1991PhRvB..44.2991S |doi=10.1103/PhysRevB.44.2991|pmid=9999890 }}</ref> to approach an equilibrium [[Maxwell–Boltzmann distribution|Maxwell-Boltzmann distribution]].
+</div>
 == Application to semiconductor physics ==
@@ Line 31: / Line 37: @@
 \end{aligned}
 </math>
+== See also ==
+{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also}}
 == References ==
@@ Line 37: / Line 46: @@
 [[Category:Statistical mechanics]]
-{{Sourceattribution|Quantum Boltzmann equation}}
+{{Author|Harold Foppele}}
+{{Sourceattribution|Physics:Quantum Boltzmann equation|1}}

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Latest revision as of 11:33, 22 May 2026

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