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= Collective Modes = | = Collective Modes = | ||
Sound waves propagating through air or water are examples for collective modes. Such modes arise without broken symmetry of the system as ordinary gases and fluids do not brake any symmetry. Such waves have wavelengths that are very large compared to the distance between neighboring particles, which is the reason why we will look at very small wave vectors. An example for a collective mode in due to broken symmetry is a shear mode in a solid. | Sound waves propagating through air or water are examples for collective modes. Such modes arise without broken symmetry of the system as ordinary gases and fluids do not brake any symmetry. Such waves have wavelengths that are very large compared to the distance between neighboring particles, which is the reason why we will look at very small wave vectors. An example for a collective mode in due to broken symmetry is a shear mode in a solid.<br/> | ||
Remember that the partition function can be written as the Feynman path integral | Remember that the partition function can be written as the Feynman path integral | ||
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</math> | </math> | ||
== Hubbard-Stratonovich Transformation == | === Hubbard-Stratonovich Transformation === | ||
The partition function can be calculated via the Hubbard-Stratonovich Transformation, which can be motivated by the one-dimensional integral | The partition function can be calculated via the Hubbard-Stratonovich Transformation, which can be motivated by the one-dimensional integral | ||
<math> | <math> | ||
1 = \frac1{\sqrt{\pi a}}\int\limits_{-\infin}^{\infin}dx e^{-\frac1a x^2} | 1 = \frac1{\sqrt{\pi a}}\int\limits_{-\infin}^{\infin}dx e^{-\frac1a x^2}. | ||
</math> | </math> | ||
The pre-factor <math> \sqrt{\pi a} </math> is simply the constant number that equals to the value of the integral. <br/> | |||
In the language of path integrals this implies | In the language of path integrals this implies | ||
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&\equiv \left\langle e^A\right\rangle | &\equiv \left\langle e^A\right\rangle | ||
\end{align}</math> | \end{align}</math> | ||
=== Cumulant Expansion === | |||
This can be calculated by a cumulant expansion, such that | This can be calculated by a cumulant expansion, such that | ||
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Since we have two creation operators and two annihilation operators, two possible contractions are possible. However, one of these contractions is a non-connected Feynman diagram and so, according to the linked cluster theorem, we only have to compute the connected one. Due to Kronecker-delta symbols (arising from the contractions) we will be left with only one sum over <math>k</math> and one sum over <math>\omega</math>. The resulting sum over <math>k</math> can be written as an integral over a continuum (by taking the appropriate limit of <math>L\rightarrow\infin</math>), while the sum over <math>\omega</math> is written as a contour integral. The result of this exercise is | Since we have two creation operators and two annihilation operators, two possible contractions are possible. However, one of these contractions is a non-connected Feynman diagram and so, according to the linked cluster theorem, we only have to compute the connected one. Due to Kronecker-delta symbols (arising from the contractions) we will be left with only one sum over <math>k</math> and one sum over <math>\omega</math>. The resulting sum over <math>k</math> can be written as an integral over a continuum (by taking the appropriate limit of <math>L\rightarrow\infin</math>), while the sum over <math>\omega</math> is written as a contour integral. The result of this exercise is | ||
<math> | |||
\frac Z{Z_0} \simeq \int D\phi e^{S_{eff}(\phi)}, | |||
</math> | |||
where the effective action is | |||
<math>S_{eff}(\phi) = \frac1{\beta}\sum_{\Omega_n}\frac1{L^3} \sum_q\left(\frac1{V_q}-2 \mathcal N\Pi_q(i\Omega_n) \right) \phi_{-q}(i\Omega_n) \phi_q(i\Omega_n) + \mathcal O(\phi^4).</math> | |||
Here we use the degeneracy <math>\mathcal{N}</math> of each level. This action is expressed in terms of an integral that we are about to solve, namely | |||
<math> | |||
\Pi_q(i\Omega_n) = \int \frac{d^3k}{(2\pi)^3} \frac{n_F(\epsilon_k)-n_F(\epsilon_{k-q})} {\epsilon_k - \epsilon_{k-q}-i\Omega_n}. | |||
</math> | |||
In this expression <math>n_F(E)=\frac1{e^{\frac{E-\mu}{kT}+1}}</math> is the Fermi-Dirac distribution function, together with the chemical potential <math>\mu</math>, the Boltzmann factor <math>k_B</math> and the temperature <math>T</math>. | |||
=== Plasmons and Zero Sound === | |||
As said before, our special interest is pointed towards density waves in an electron gas. So finally, the degeneracy <math>\mathcal{N}</math> will be set equal to 2. Notice that <math>\phi_q(i\Omega_n)</math> couples to density.<br/> | |||
We also said in the beginning of the chapter that wavelengths of such excitations are typically very long compared to the distance between molecules; or, in case of a plasma, the distance between electrons. Therefore, when we calculate <math>\Pi_q(i\Omega_n)</math> we look at the limit of very small wave vectors <math>q</math>, and we will also consider small temperatures. For an electron gas the energy dispersion is, of course, quadratic in <math>k</math>, being <math>\epsilon_k=\frac{\hbar^2k^2}{2m}</math>. | |||
Therefore, let us assume <math>|q|\ll k_F</math> and <math>T\ll \mu</math>. <br/> | |||
In that case the difference | |||
<math>\begin{align} | |||
n_F(\epsilon_k)-n_F(\epsilon_{k-q}) | |||
\end{align}</math> | |||
in the integrand of <math>\Pi_q(i\Omega_n)</math> has no contribution for <math>\epsilon_k</math> being far away from <math>\epsilon_F</math>. Hence we can expand the numerator of the integrand by writing | |||
<math> | |||
\begin{align} | |||
n_F(\epsilon_{k-q}) &= n_F(\epsilon_{k}+\epsilon_{k-q}-\epsilon_{k})\\ | |||
&\simeq n_F(\epsilon_k) + n_F'(\epsilon_k) (\epsilon_{k-q} - \epsilon_k). | |||
\end{align} | |||
</math> |
Revision as of 02:58, 6 December 2011
Collective Modes
Sound waves propagating through air or water are examples for collective modes. Such modes arise without broken symmetry of the system as ordinary gases and fluids do not brake any symmetry. Such waves have wavelengths that are very large compared to the distance between neighboring particles, which is the reason why we will look at very small wave vectors. An example for a collective mode in due to broken symmetry is a shear mode in a solid.
Remember that the partition function can be written as the Feynman path integral
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Z = \int D(c^{*}, c) e^{-S}, }
where
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle S_0 = \frac{1}{\beta} \sum_{\omega_n} \sum_{k}(-i\omega_n + \epsilon_n-\mu) c_{k,\sigma}^{*} c_{k,\sigma}(\omega_n) }
is the action of the non-interacting system; while the action of the interacting system is Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle S_{int} = \frac1{\beta} \sum_{\Omega_n} \frac1{L^3}\sum_{q} V_q n_{-q}(-i\Omega_n) n_q(i\Omega_n) }
with Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle n_q (i\Omega_n) = \frac1{\beta}\sum_{\omega_n}\sum_k c^*_{k+q, \sigma} (i\omega_n + i\Omega_n) c_{k,\sigma}(i \omega_n) }
Hubbard-Stratonovich Transformation
The partition function can be calculated via the Hubbard-Stratonovich Transformation, which can be motivated by the one-dimensional integral
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle 1 = \frac1{\sqrt{\pi a}}\int\limits_{-\infin}^{\infin}dx e^{-\frac1a x^2}. }
The pre-factor Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \sqrt{\pi a} }
is simply the constant number that equals to the value of the integral.
In the language of path integrals this implies
Here the number resembles the pre-factor in the previous example. Rewriting the potential in momentum space, this identity allows to convert the partition function. This is done by a shift of the field
The partition function, as introduced at the beginning of this chapter, simplifies thereby to
Cumulant Expansion
This can be calculated by a cumulant expansion, such that
Now, since the the average of the density is equal to zero,
we only have to calculate the term with in the exponent. This term contains the average of two density operators , which can be evaluated using the Wick's theorem.
Since we have two creation operators and two annihilation operators, two possible contractions are possible. However, one of these contractions is a non-connected Feynman diagram and so, according to the linked cluster theorem, we only have to compute the connected one. Due to Kronecker-delta symbols (arising from the contractions) we will be left with only one sum over and one sum over Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \omega} . The resulting sum over Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle k} can be written as an integral over a continuum (by taking the appropriate limit of Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle L\rightarrow\infin} ), while the sum over Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \omega} is written as a contour integral. The result of this exercise is
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \frac Z{Z_0} \simeq \int D\phi e^{S_{eff}(\phi)}, }
where the effective action is
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle S_{eff}(\phi) = \frac1{\beta}\sum_{\Omega_n}\frac1{L^3} \sum_q\left(\frac1{V_q}-2 \mathcal N\Pi_q(i\Omega_n) \right) \phi_{-q}(i\Omega_n) \phi_q(i\Omega_n) + \mathcal O(\phi^4).}
Here we use the degeneracy Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \mathcal{N}} of each level. This action is expressed in terms of an integral that we are about to solve, namely
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \Pi_q(i\Omega_n) = \int \frac{d^3k}{(2\pi)^3} \frac{n_F(\epsilon_k)-n_F(\epsilon_{k-q})} {\epsilon_k - \epsilon_{k-q}-i\Omega_n}. }
In this expression Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle n_F(E)=\frac1{e^{\frac{E-\mu}{kT}+1}}} is the Fermi-Dirac distribution function, together with the chemical potential Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \mu} , the Boltzmann factor Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle k_B} and the temperature Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle T} .
Plasmons and Zero Sound
As said before, our special interest is pointed towards density waves in an electron gas. So finally, the degeneracy Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \mathcal{N}}
will be set equal to 2. Notice that Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \phi_q(i\Omega_n)}
couples to density.
We also said in the beginning of the chapter that wavelengths of such excitations are typically very long compared to the distance between molecules; or, in case of a plasma, the distance between electrons. Therefore, when we calculate Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \Pi_q(i\Omega_n)}
we look at the limit of very small wave vectors Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle q}
, and we will also consider small temperatures. For an electron gas the energy dispersion is, of course, quadratic in Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle k}
, being Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \epsilon_k=\frac{\hbar^2k^2}{2m}}
.
Therefore, let us assume Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle |q|\ll k_F}
and Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle T\ll \mu}
.
In that case the difference
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \begin{align} n_F(\epsilon_k)-n_F(\epsilon_{k-q}) \end{align}}
in the integrand of Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \Pi_q(i\Omega_n)} has no contribution for Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \epsilon_k} being far away from Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \epsilon_F} . Hence we can expand the numerator of the integrand by writing
Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \begin{align} n_F(\epsilon_{k-q}) &= n_F(\epsilon_{k}+\epsilon_{k-q}-\epsilon_{k})\\ &\simeq n_F(\epsilon_k) + n_F'(\epsilon_k) (\epsilon_{k-q} - \epsilon_k). \end{align} }