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In [[plasma physics]], an '''ion acoustic wave''' is one type of [[longitudinal wave|longitudinal]] oscillation of the [[ion]]s and [[electron]]s in a [[plasma (physics)|plasma]], much like [[acoustic wave]]s traveling in neutral gas. However, because the waves propagate through positively charged ions, ion acoustic waves can interact with their [[electromagnetic field]]s, as well as simple collisions. In plasmas, ion acoustic waves are frequently referred to as acoustic waves or even just sound waves.  They commonly govern the evolution of mass density, for instance due to [[pressure gradient]]s, on time scales longer than the frequency corresponding to the relevant length scale.  Ion acoustic waves can occur in an unmagnetized  plasma or in a magnetized plasma parallel to the [[magnetic field]]. For a single species plasma, the waves are [[Dispersion relation|dispersionless]] (<math>\omega=v_sk</math>) with a speed (in the long [[wavelength]] limit) given by {{Citation needed|date=October 2013}}
:<math>v_s = \sqrt{\frac{\gamma_{e}ZK_{B}T_e+\gamma_{i}K_{B}T_i}{M}}</math>
where <math>K_{B}</math> is [[Boltzmann's constant]], <math>M</math> is the mass of the ion, <math>Z</math> is its charge, <math>T_e</math> is the temperature of the electrons and <math>T_i</math> is the temperature of the ions. Normally γ<sub>e</sub> is taken to be unity, on the grounds that the [[thermal conductivity]] of electrons is large enough to keep them [[isothermal]] on the time scale of ion acoustic waves, and γ<sub>i</sub> is taken to be 3, corresponding to one-dimensional motion. In [[collisionless]] plasmas, the electrons are often much hotter than the ions, in which case the second term in the numerator can be ignored.
 
== Derivation ==
We derive the ion acoustic wave dispersion relation for a linearized fluid description of a plasma with multiple ion species.  A subscript 0 denotes constant equilibrium quantities, and 1 denotes first-order perturbations. We assume the pressure perturbations for each species (electrons and ions) are a [[Polytropic_process]], namely <math>p_{s1} = \gamma_s T_{s0} n_{s1}</math> for species s.  Using the ion continuity equation, the ion momentum equation becomes
:<math>(-m_i\partial_{tt}+\gamma_iT_i\nabla^2)n_{i1} = Z_ien_{i0}\nabla\cdot\vec E </math>
We relate the electric field <math>\vec E_1</math> to the electron density by the electron momentum equation:
:<math>n_{e0}m_e\partial_t\vec v_{e1} = -n_{e0}e\vec E_1 - \gamma_eT_e\nabla n_{e1} </math>
We now neglect the left-hand side, which is due to electron inertia.  This is valid for waves with frequencies much less than the electron plasma frequency.  The resulting electric field is
:<math>\vec E_1  = - {\gamma_eT_e \over n_{e0}e}\nabla n_{e1} </math>
Since we have already solved for the electric field, we cannot also find it from Poisson's equation. The ion momentum equation now relates <math>n_{i1}</math> for each species to <math>n_{e1}</math>:
:<math>(-m_i\partial_{tt}+\gamma_iT_i\nabla^2)n_{i1} = -\gamma_e T_e \nabla^2 n_{e1} </math>
We arrive at a dispersion relation via Poisson's equation:
:<math> {\epsilon_0 \over e}\nabla\cdot\vec E = [\sum_i n_{i0}Z_i - n_{ne0}] + [\sum_in_{i1}Z_i - n_{e1}] </math>
The first bracketed term on the right is zero by assumption (charge-neutral equilibrium). We substitute for the electric field and rearrange to find
:<math> (1-\gamma_e \lambda_{De}^2\nabla^2)n_{e1} = \sum_iZ_in_{i1} </math>.
<math>\lambda_{De}^2 \equiv \epsilon_0T_e/(n_{e0}e^2)</math> defines the electron Debye length. The second term on the left arises from the <math>\nabla\cdot\vec E</math> term, and reflects the degree to which the perturbation is not charge-neutral. If <math>k\lambda_{De}</math> is small we may drop this term.  This approximation is sometimes called the plasma approximation.
 
We now work in Fourier space, and find
:<math> n_{i1} = \gamma_eT_eZ_i {n_{i0} \over n_{e0}} [m_iv_s^2-\gamma_iT_i]^{-1} n_{e1} </math>
<math>v_s=\omega/k</math> is the wave phase velocity.  Substituting this into Poisson's equation gives us an expression where each term is proportional to <math>n_{e1}</math>. To find the dispersion relation for natural modes, we look for solutions for <math>n_{e1}</math> nonzero.
:<math> \gamma_eT_e \sum_i Z_i^2f_i[m_iv_s^2-\gamma_iT_i]^{-1} = \bar Z(1+\gamma_ek^2\lambda_{De}^2)</math>
 
<math>n_{i1}=f_in_{I1}</math> where <math>n_{I1}=\Sigma_i n_{i1}</math>, and <math>\bar Z = \Sigma_i Z_if_i </math>. In general it is not possible to further simplify this expression. If <math>k\lambda_{De}</math> is small (the plasma approximation), we can neglect the second term on the term, and the wave is dispersionless <math>\omega = v_sk</math> with <math>v_s</math> independent of k.
 
== Specific Examples ==
To illustrate some features of ion acoustic waves, we can consider some specific examples of the general dispersion relation given above. First, for a single ion species, we find
:<math>v_s^2 = {\gamma_eZ_iT_e \over m_i}[{1 \over 1+\gamma_e(k\lambda_{De})^2} + {\gamma_iT_{i0} \over \gamma_eZ_iT_{e0}}]
</math>
 
For any number of ion species, all of which are cold (<math>\gamma_iT_{i0} \ll m_iv_s^2</math>), we obtain
:<math>v_s^2 = {\gamma_eT_{e0} \over 1+\gamma_e(k\lambda_{De})^2} \sum_i {Z_i^2f_i \over \bar Z m_i}</math>
 
A case of interest to nuclear fusion is an equimolar mixture of deuterium and tritium ions (<math>f_D=f_T=1/2</math>). Let us specialize to full ionization (<math>Z_D=Z_T=1</math>), equal temperatures (<math>T_{e0}=T_{i0}\equiv T_0</math>), polytrope exponents <math>\gamma_e=1, \gamma_i=3</math>, and neglect the <math>(k\lambda_{De})^2</math> contribution. The dispersion relation becomes a quadratic in <math>v_s^2</math>, namely:
:<math>2A_DA_Tu^4 - 7(A_D+A_T)u^2 + 24=0</math>
where <math>A_i=m_i/m_u</math>, <math>m_u</math> is the atomic mass unit, and <math>u^2=m_uv_s^2/T_0</math>. Using <math>(A_D,A_T)=(2.01,3.02)</math> we find the two roots are <math>u^2=(1.10,1.81)</math>.
 
== Damping ==
Ion acoustic waves are damped both by [[Coulomb collision]]s and collisionless [[Landau damping]]. The Landau damping occurs on both electrons and ions, with the relative importance depending on parameters.
 
==See also==
* [[Waves in plasmas]]
* [[Sound]]
* [[Alfvén wave]]
* [[Magnetosonic wave]]
* [[List of plasma (physics) articles]]
 
==External links==
*[http://mr-fusion.hellblazer.com/pdfs/ion-accoustic-waves-and-langmuir-waves.pdf Various patents and articles related to fusion, IEC, ICC and plasma physics]
 
{{DEFAULTSORT:Ion Acoustic Wave}}
[[Category:Waves in plasmas]]

Revision as of 00:31, 13 December 2013

In plasma physics, an ion acoustic wave is one type of longitudinal oscillation of the ions and electrons in a plasma, much like acoustic waves traveling in neutral gas. However, because the waves propagate through positively charged ions, ion acoustic waves can interact with their electromagnetic fields, as well as simple collisions. In plasmas, ion acoustic waves are frequently referred to as acoustic waves or even just sound waves. They commonly govern the evolution of mass density, for instance due to pressure gradients, on time scales longer than the frequency corresponding to the relevant length scale. Ion acoustic waves can occur in an unmagnetized plasma or in a magnetized plasma parallel to the magnetic field. For a single species plasma, the waves are dispersionless (ω=vsk) with a speed (in the long wavelength limit) given by Potter or Ceramic Artist Truman Bedell from Rexton, has interests which include ceramics, best property developers in singapore developers in singapore and scrabble. Was especially enthused after visiting Alejandro de Humboldt National Park.

vs=γeZKBTe+γiKBTiM

where KB is Boltzmann's constant, M is the mass of the ion, Z is its charge, Te is the temperature of the electrons and Ti is the temperature of the ions. Normally γe is taken to be unity, on the grounds that the thermal conductivity of electrons is large enough to keep them isothermal on the time scale of ion acoustic waves, and γi is taken to be 3, corresponding to one-dimensional motion. In collisionless plasmas, the electrons are often much hotter than the ions, in which case the second term in the numerator can be ignored.

Derivation

We derive the ion acoustic wave dispersion relation for a linearized fluid description of a plasma with multiple ion species. A subscript 0 denotes constant equilibrium quantities, and 1 denotes first-order perturbations. We assume the pressure perturbations for each species (electrons and ions) are a Polytropic_process, namely ps1=γsTs0ns1 for species s. Using the ion continuity equation, the ion momentum equation becomes

(mitt+γiTi2)ni1=Zieni0E

We relate the electric field E1 to the electron density by the electron momentum equation:

ne0metve1=ne0eE1γeTene1

We now neglect the left-hand side, which is due to electron inertia. This is valid for waves with frequencies much less than the electron plasma frequency. The resulting electric field is

E1=γeTene0ene1

Since we have already solved for the electric field, we cannot also find it from Poisson's equation. The ion momentum equation now relates ni1 for each species to ne1:

(mitt+γiTi2)ni1=γeTe2ne1

We arrive at a dispersion relation via Poisson's equation:

ϵ0eE=[ini0Zinne0]+[ini1Zine1]

The first bracketed term on the right is zero by assumption (charge-neutral equilibrium). We substitute for the electric field and rearrange to find

(1γeλDe22)ne1=iZini1.

λDe2ϵ0Te/(ne0e2) defines the electron Debye length. The second term on the left arises from the E term, and reflects the degree to which the perturbation is not charge-neutral. If kλDe is small we may drop this term. This approximation is sometimes called the plasma approximation.

We now work in Fourier space, and find

ni1=γeTeZini0ne0[mivs2γiTi]1ne1

vs=ω/k is the wave phase velocity. Substituting this into Poisson's equation gives us an expression where each term is proportional to ne1. To find the dispersion relation for natural modes, we look for solutions for ne1 nonzero.

γeTeiZi2fi[mivs2γiTi]1=Z¯(1+γek2λDe2)

ni1=finI1 where nI1=Σini1, and Z¯=ΣiZifi. In general it is not possible to further simplify this expression. If kλDe is small (the plasma approximation), we can neglect the second term on the term, and the wave is dispersionless ω=vsk with vs independent of k.

Specific Examples

To illustrate some features of ion acoustic waves, we can consider some specific examples of the general dispersion relation given above. First, for a single ion species, we find

vs2=γeZiTemi[11+γe(kλDe)2+γiTi0γeZiTe0]

For any number of ion species, all of which are cold (γiTi0mivs2), we obtain

vs2=γeTe01+γe(kλDe)2iZi2fiZ¯mi

A case of interest to nuclear fusion is an equimolar mixture of deuterium and tritium ions (fD=fT=1/2). Let us specialize to full ionization (ZD=ZT=1), equal temperatures (Te0=Ti0T0), polytrope exponents γe=1,γi=3, and neglect the (kλDe)2 contribution. The dispersion relation becomes a quadratic in vs2, namely:

2ADATu47(AD+AT)u2+24=0

where Ai=mi/mu, mu is the atomic mass unit, and u2=muvs2/T0. Using (AD,AT)=(2.01,3.02) we find the two roots are u2=(1.10,1.81).

Damping

Ion acoustic waves are damped both by Coulomb collisions and collisionless Landau damping. The Landau damping occurs on both electrons and ions, with the relative importance depending on parameters.

See also

External links