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| In [[quantum mechanics]], specifically [[time-dependent density functional theory]], the '''Runge–Gross theorem''' ('''RG theorem''') shows that for a [[many-body system]] evolving from a given initial [[wavefunction]], there exists a [[one-to-one mapping]] between the potential (or potentials) in which the system evolves and the density (or densities) of the system. The potentials under which the theorem holds are defined up to an additive purely time-dependent function: such functions only change the phase of the wavefunction and leave the density invariant. Most often the RG theorem is applied to molecular systems where the [[electronic density]], ''ρ''('''r''',''t'') changes in response to an external [[scalar potential]], ''v''('''r''',''t''), such as a time-varying electric field.<ref>{{cite book|last=Marques|first=Miguel A. L.|coauthors=Eberhard K. U. Gross|title=Time-Dependent Density Functional Theory, in A Primer in Density Functional Theory|editor=Carlos Fiolhais, Fernando Nogueira, and Miguel Marques|publisher=Springer|year=2003|pages=144–151|isbn=978-3-540-03083-6|url=http://books.google.com/?id=mX793GABep8C&printsec=frontcover}}</ref>
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| The Runge–Gross theorem provides the formal foundation of time-dependent density functional theory. It shows that the density can be used as the fundamental variable in describing quantum [[many-body system]]s in place of the wavefunction, and that all properties of the system are [[Functional (mathematics)|functionals]] of the density.
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| The theorem was published by [[Erich Runge]] and [[Eberhard K. U. Gross]] in 1984.<ref name="RG"/> As of January 2011, the original paper has been cited over 1,700 times.<ref>[[ISI Web of Knowledge]] cited reference search, 7 January 2011.</ref>
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| ==Overview==
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| The Runge–Gross theorem was originally derived for electrons moving in a [[scalar field|scalar external field]].<ref name="RG">{{cite journal|last=Runge|first=Erich|coauthors=E. K. U. Gross|year=1984|title=Density-Functional Theory for Time-Dependent Systems|journal=Phys. Rev. Lett.|volume=52|issue=12|pages=997–1000|doi=10.1103/PhysRevLett.52.997|bibcode=1984PhRvL..52..997R}}</ref> Given such a field denoted by ''v'' and the number of electron, ''N'', which together determine a [[Molecular Hamiltonian|Hamiltonian]] ''H<sub>v''</sub>, and an initial condition on the wavefunction Ψ(''t'' = ''t''<sub>0</sub>) = Ψ<sub>0</sub>, the evolution of the wavefunction is determined by the [[Schrödinger equation]] | |
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| :<math>\hat{H}_v(t)|\Psi(t)\rangle=i\frac{\partial}{\partial t}|\Psi(t)\rangle.</math>
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| At any given time, the ''N''-electron wavefunction, which depends upon 3''N'' spatial and ''N'' [[Spin (physics)|spin]] coordinates, determines the [[electronic density]] through integration as
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| :<math>\rho(\mathbf r,t)=N\sum_{s_1} \cdots \sum_{s_N} \int \ \mathrm d\mathbf r_2 \ \cdots \int\ \mathrm d\mathbf r_N \ |\Psi(\mathbf r_1,s_1,\mathbf r_2,s_2,...,\mathbf r_N,s_N,t)|^2.</math>
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| Two external potentials differing only by an additive time-dependent, spatially independent, function, ''c''(''t''), give rise to wavefunctions differing only by a [[phase factor]] exp(-''ic''(''t'')), and therefore the same electronic density. These constructions provide a mapping from an external potential to the electronic density:
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| :<math>v(\mathbf r,t)+c(t)\rightarrow e^{-ic(t)}|\Psi(t)\rangle\rightarrow\rho(\mathbf r,t).</math>
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| The Runge–Gross theorem shows that this mapping is invertible, modulo ''c''(''t''). Equivalently, that the density is a functional of the external potential and of the initial wavefunction on the space of potentials differing by more than the addition of ''c''(''t''):
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| :<math>\rho(\mathbf r,t)=\rho[v,\Psi_0](\mathbf{r},t)\leftrightarrow v(\mathbf r,t)=v[\rho,\Psi_0](\mathbf r,t)</math>
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| ==Proof==
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| Given two scalar potentials denoted as ''v''('''r''',''t'') and ''v''<nowiki>'</nowiki>('''r''',''t''), which differ by more than an additive purely time-dependent term, the proof follows by showing that the density corresponding to each of the two scalar potentials, obtained by solving the Schrödinger equation, differ.
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| The proof relies heavily on the assumption that the external potential can be expanded in a [[Taylor series]] about the initial time. The proof also assumes that the density vanishes at infinity, making it valid only for finite systems.
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| The Runge–Gross proof first shows that there is a one-to-one mapping between external potentials and current densities by invoking the [[Heisenberg picture|Heisenberg equation of motion]] for the current density so as to relate time-derivatives of the current density to spatial derivatives of the external potential. Given this result, the continuity equation is used in a second step to relate time-derivatives of the electronic density to time-derivatives of the external potential.
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| The assumption that the two potentials differ by more than an additive spatially independent term, and are expandable in a Taylor series, means that there exists an integer ''k'' ≥ 0, such that
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| :<math>u_{k}(\mathbf{r})\equiv\left.\frac{\partial^k}{\partial t^k}\big(v(\mathbf{r},t)-v'(\mathbf{r},t)\big)\right|_{t=t_0}</math>
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| is not constant in space. This condition is used throughout the argument. | |
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| ===Step 1===
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| From the [[Heisenberg picture|Heisenberg equation of motion]], the time evolution of the [[Probability current|current density]], '''j'''('''r''',''t''), under the external potential ''v''('''r''',''t'') which determines the Hamiltonian ''H''<sub>''v''</sub>, is
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| :<math>i\frac{\partial\mathbf j(\mathbf r,t)}{\partial t}=\langle\Psi(t)|[\hat{\mathbf{j}}(\mathbf r),\hat{H}_v(t)]|\Psi(t)\rangle.</math>
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| Introducing two potentials ''v'' and ''v''<nowiki>'</nowiki>, differing by more than an additive spatially constant term, and their corresponding current densities '''j''' and '''j'''<nowiki>'</nowiki>, the Heisenberg equation implies
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| :<math>
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| \begin{align}
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| i\left.\frac{\partial}{\partial t}\big(\mathbf j(\mathbf r,t)-\mathbf j'(\mathbf r,t) \big)\right|_{t=t_0} &= \langle\Psi(t_0)|[\hat{\mathbf{j}}(\mathbf r),\hat{H}_{v}(t_0)-\hat{H}_{v'}(t_0)]|\Psi(t_0)\rangle,\\
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| &=\langle\Psi(t_0)|[\hat{\mathbf{j}}(\mathbf r),\hat{V}(t_0)-\hat{V}'(t_0)]|\Psi(t_0)\rangle,\\
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| &= i\rho(\mathbf r,t_0)\nabla\big(v(\mathbf{r},t_0)-v'(\mathbf{r},t_0)\big).
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| \end{align}
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| </math>
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| The final line shows that if the two scalar potentials differ at the initial time by more than a spatially independent function, then the current densities that the potentials generate will differ infinitesimally after ''t''<sub>0</sub>. If the two potentials do not differ at ''t''<sub>0</sub>, but ''u''<sub>''k''</sub>('''r''') ≠ 0 for some value of ''k'', then repeated application of the Heisenberg equation shows that | |
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| :<math>i^{k+1}\left.\frac{\partial^{k+1}}{\partial t^{k+1}}\big(\mathbf j(\mathbf r,t)-\mathbf j'(\mathbf r,t)\big)\right|_{t=t_0}=i\rho(\mathbf r,t)\nabla i^k\left.\frac{\partial^{k}}{\partial t^{k}}\big(v(\mathbf{r},t)-v'(\mathbf{r},t) \big)\right|_{t=t_0},</math>
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| ensuring the current densities will differ from zero infinitesimally after ''t''<sub>0</sub>.
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| ===Step 2===
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| The electronic density and current density are related by a [[continuity equation]] of the form
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| :<math>\frac{\partial\rho(\mathbf r,t)}{\partial t}+\nabla\cdot\mathbf j(\mathbf r,t)=0.</math>
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| Repeated application of the continuity equation to the difference of the densities ''ρ'' and ''ρ''<nowiki>'</nowiki>, and current densities '''j''' and '''j'''<nowiki>'</nowiki>, yields
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| :<math>
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| \begin{align}
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| \left.\frac{\partial^{k+2}}{\partial t^{k+2}}(\rho(\mathbf r,t)-\rho'(\mathbf r,t))\right|_{t=t_0}&=-\nabla\cdot\left.\frac{\partial^{k+1}}{\partial t^{k+1}}\big(\mathbf j(\mathbf r,t)-\mathbf j'(\mathbf r,t)\big)\right|_{t=t_0},\\
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| &=-\nabla\cdot[\rho(\mathbf r,t_0)\nabla\left.\frac{\partial^k}{\partial t^k}\big(v(\mathbf{r},t_0)-v'(\mathbf{r},t_0)\big)\right|_{t=t_0}],\\
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| &=-\nabla\cdot[\rho(\mathbf r,t_0)\nabla u_k(\mathbf r)].
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| \end{align}
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| </math>
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| The two densities will then differ if the right-hand side (RHS) is non-zero for some value of ''k''. The non-vanishing of the RHS follows by a [[reductio ad absurdum]] argument. Assuming, contrary to our desired outcome, that
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| :<math>\nabla\cdot(\rho(\mathbf r,t_0)\nabla u_k(\mathbf r)) = 0,</math>
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| integrate over all space and apply Green's theorem.
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| :<math>
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| \begin{align}
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| 0&=\int\mathrm d\mathbf r\ u_k(\mathbf r)\nabla\cdot(\rho(\mathbf r,t_0)\nabla u_k(\mathbf r)),\\
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| &=-\int\mathrm d\mathbf r\ \rho(\mathbf r,t_0)(\nabla u_k(\mathbf r))^2+\frac{1}{2}\int \mathrm d\mathbf S\cdot\rho(\mathbf r,t_0)(\nabla u_k^2(\mathbf r)).
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| \end{align}
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| </math>
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| The second term is a surface integral over an infinite sphere. Assuming that the density is zero at infinity (in finite systems, the density decays to zero exponentially) and that ∇''u<sub>k''</sub><sup>2</sup>('''r''') increases slower than the density decays,<ref>{{cite journal|last=Dhara|first=Asish K.|coauthors=Swapan K. Ghosh|year=1987|title=Density-functional theory for time-dependent systems|journal=Phys. Rev. A|volume=35|issue=1|pages=442–444|doi=10.1103/PhysRevA.35.442|bibcode = 1987PhRvA..35..442D }}</ref> the surface integral vanishes and, because of the non-negativity of the density,
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| :<math>\rho(\mathbf r,t_0)(\nabla u_k(\mathbf r))^2=0,</math>
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| implying that ''u<sub>k''</sub> is a constant, contradicting the original assumption and completing the proof.
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| ==Extensions==
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| The Runge–Gross proof is valid for pure electronic states in the presence of a scalar field. The first extension of the RG theorem was to time-dependent [[Statistical ensemble (mathematical physics)|ensembles]], which employed the [[Liouville equation#Quantum mechanics|Liouville equation]] to relate the Hamiltonian and [[density matrix]].<ref>{{cite journal|last=Li|first=Tie-cheng|coauthors=Pei-qing Tong|year=1985|title=Hohenberg-Kohn theorem for time-dependent ensembles|journal=Phys. Rev. A|volume=31|issue=3|pages=1950–1951|doi=10.1103/PhysRevA.31.1950|bibcode = 1985PhRvA..31.1950L }}</ref> A proof of the RG theorem for multicomponent systems—where more than one type of particle is treated within the full quantum theory—was introduced in 1986.<ref>{{cite journal|last=Li|first=Tie-Cheng|coauthors=Pei-qing Tong|year=1986|title=Time-dependent density-functional theory for multicomponent systems|journal=Phys. Rev. A|volume=34|issue=1|pages=529–532|doi=10.1103/PhysRevA.34.529|bibcode = 1986PhRvA..34..529L }}</ref> Incorporation of magnetic effects requires the introduction of a [[vector potential]] ('''A'''('''r''')) which together with the scalar potential uniquely determine the current density.<ref>{{cite journal|last=Ghosh|first=Swapan K.|coauthors=Asish K. Dhara|year=1988|title=Density-functional theory of many-electron systems subjected to time-dependent electric and magnetic fields|journal=Phys. Rev. A|volume=38|issue=3|pages=1149–1158|doi=10.1103/PhysRevA.38.1149|bibcode = 1988PhRvA..38.1149G }}</ref><ref>{{cite journal|last=Vignale|first=Giovanni|year=2004|title=Mapping from current densities to vector potentials in time-dependent current density functional theory|journal=Phys. Rev. B|volume=70|issue=20|pages=201102|doi=10.1103/PhysRevB.70.201102|arxiv = cond-mat/0407682 |bibcode = 2004PhRvB..70t1102V }}</ref> Time-dependent density functional theories of [[superconductivity]] were introduced in 1994 and 1995.<ref>{{cite journal|last=Wacker|first=O. -J.|coauthors=R. Kümmel and E. K. U. Gross|year=1994|title=Time-Dependent Density-Functional Theory for Superconductors|journal=Phys. Rev. Lett.|volume=73|issue=21|pages=2915–2918|doi=10.1103/PhysRevLett.73.2915|bibcode=1994PhRvL..73.2915W}}</ref><ref>{{cite journal|last=Rajagopal|first=A. K.|coauthors=F. A. Buot|year=1995|title=Time-dependent functional theory for superconductors|journal=Phys. Rev. B|volume=52|issue=9|pages= 6769–6774|doi=10.1103/PhysRevB.52.6769|bibcode = 1995PhRvB..52.6769R }}</ref> Here, scalar, vector, and [[pairing potential|pairing]] (''D''(''t'')) potentials map between current and [[anomalous density|anomalous]] (Δ<sub>IP</sub>('''r''',''t'')) densities.
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| ==References==
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| {{reflist}}
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| {{DEFAULTSORT:Runge-Gross theorem}}
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| [[Category:Density functional theory]]
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| [[Category:Theorems in quantum physics]]
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