Difference between revisions of "Transverse traceless gauge"

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(Problem 1: Transverse traceless (TT) gauge)
(Problem 3: Plane wave TT gauge transformation)
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=A_{\mu\nu}e^{i\,k_{\lambda}x^\lambda},
 
=A_{\mu\nu}e^{i\,k_{\lambda}x^\lambda},
 
\quad k^\mu k_\mu =0.\]
 
\quad k^\mu k_\mu =0.\]
\begin{enumerate}
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\item Show that the TT gauge is fixed by the coordinate transformation $x\to x+\xi$ with
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1) Show that the TT gauge is fixed by the coordinate transformation $x\to x+\xi$ with
 
\begin{align}
 
\begin{align}
 
\xi_{\mu}&=B_{\mu}e^{ik_\lambda x^\lambda};\\
 
\xi_{\mu}&=B_{\mu}e^{ik_\lambda x^\lambda};\\
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l^{\mu}=(\omega,-\mathbf{k}).
 
l^{\mu}=(\omega,-\mathbf{k}).
 
\end{align}
 
\end{align}
[Padm. p \textsection 9.3, p.403 (wrong signs!), also see  MTW Ex.35.1 for similar formulation; \emph{the solution can probably be derived if we introduce the null frame $k$ and $l$ (the other two spacial basis vectors are not needed) and look for solution in the form
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<!--[Padm. p \textsection 9.3, p.403 (wrong signs!), also see  MTW Ex.35.1 for similar formulation; ''the solution can probably be derived if we introduce the null frame $k$ and $l$ (the other two spacial basis vectors are not needed) and look for solution in the form $B=C_1 k+ C_2 l +C_{3} w$.'']-->
$B=C_1 k+ C_2 l +C_{3} w$.}]
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2) What is the transformation to the Lorenz gauge for arbitrary gravitational wave in vacuum?
\item What is the transformation to the Lorenz gauge for arbitrary gravitational wave in vacuum?
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\end{enumerate}
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   <div class="NavHead">solution</div>
 
   <div class="NavHead">solution</div>
 
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     <p style="text-align: left;">\begin{enumerate}
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     <p style="text-align: left;">1) The gauge transformation for $\bar{h}_{\mu\nu}$ and therefore $A_{\mu\nu}$ is
\item The gauge transformation for $\bar{h}_{\mu\nu}$ and therefore $A_{\mu\nu}$ is
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\[A_{\mu\nu}\to A_{\mu\nu}'
 
\[A_{\mu\nu}\to A_{\mu\nu}'
 
=A_{\mu\nu}-2\partial_{(\mu}\xi_{\nu)}
 
=A_{\mu\nu}-2\partial_{(\mu}\xi_{\nu)}
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\end{equation}
 
\end{equation}
 
Plugging this into the gauge conditions, one can see that the first one (tracelessness) is obeyed immediately, and the second one (transversality) after a little bit of more algebra.
 
Plugging this into the gauge conditions, one can see that the first one (tracelessness) is obeyed immediately, and the second one (transversality) after a little bit of more algebra.
\item The general first-order vacuum solution of Einstein's equations in the Lorenz gauge can be presented through its spatial Fourier transform (temporal part is integrated over due to fixed dispersion relation)
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2) The general first-order vacuum solution of Einstein's equations in the Lorenz gauge can be presented through its spatial Fourier transform (temporal part is integrated over due to fixed dispersion relation)
 
\[h_{\mu\nu}(x)=\int d^{3}k h_{\mu\nu}(\mathbf{k})
 
\[h_{\mu\nu}(x)=\int d^{3}k h_{\mu\nu}(\mathbf{k})
 
e^{ik_{\lambda}x^{\lambda}},\quad\text{with}\quad
 
e^{ik_{\lambda}x^{\lambda}},\quad\text{with}\quad
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<div id="gw28></div>
 
<div id="gw28></div>
 
<div style="border: 1px solid #AAA; padding:5px;">
 
<div style="border: 1px solid #AAA; padding:5px;">
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=== Problem 3: Curvature of a plane wave===
 
=== Problem 3: Curvature of a plane wave===
 
Consider the plane-wave solution, in which
 
Consider the plane-wave solution, in which

Revision as of 14:30, 26 December 2012



From now on we consider only vacuum solutions. Suppose we use the Lorenz gauge. As shown above, we still have the freedom of coordinate transformations with $\square \xi^\mu =0$, which preserve the gauge. So, let us choose some arbitrary (timelike) field $u^\mu$ and, in addition to the Lorenz gauge conditions, demand that the perturbation is also transverse $u^{\mu}\bar{h}_{\mu\nu}=0$ with regard to it plus that it is traceless $\bar{h}^{\mu}_{\mu}=0$. Then $h_{\mu\nu}=\bar{h}_{\mu\nu}$ and we can omit the bars. In the frame of observers with 4-velocity $u^\mu$ the full set of conditions that fix the \emph{transverse traceless (TT) gauge} is then \begin{equation} \partial_\mu {h^{\mu}}_{\nu}=0,\quad h_{0\mu}=0,\quad {h^{\mu}}_{\mu}=0. \end{equation}

Simplest solutions of the vacuum wave equation are plane waves \[h_{\mu\nu}=h_{\mu\nu}e^{ik_{\lambda}x^\lambda}.\] Indeed, substitution into $\square h_{\mu\nu}=0$ yields \[k^{\lambda}k_{\lambda}\cdot h_{\mu\nu}=0.\] Thus

  • either the wave vector is null $k^{\lambda}k_{\lambda}=0$, which roughly translates as that gravitational waves propagate with the speed of light,
  • or $h_{\mu\nu}=0$, which means that in any other (non-TT) coordinate frame, in which metric perturbation is non-zero, it is due to the oscillating coordinate system, while the true gravitational field vanishes.

\end{itemize}



Problem 1: Transverse traceless (TT) gauge

Rewrite the gauge conditions for the TT and Lorenz gauge

1) in terms of scalar, vector and tensor decomposition; 2) in terms of the metric perturbation for the plane wave solution \[h_{\mu\nu}=h_{\mu\nu}e^{ik_{\lambda}x^\lambda} =h_{\mu\nu}e^{i\omega t-ikz}\] with wave vector $k^{\mu}=(\omega,0,0,k)$ directed along the $z$-axis.



So any plane-wave solution with $k^{\mu}=(\omega,0,0,k)$ in the $z$-direction in the TT gauge has the form \begin{equation} h_{\mu\nu}=\bordermatrix{ ~&t&x&y&z\cr t&0&0&0&0\cr x&0&h_{+}&h_{\times}&0\cr y&0&h_{\times}&-h_{+}&0\cr z&0&0&0&0}e^{ikz-i\omega t}, \end{equation} or more generally any wave solution propagating in the $z$ direction can be presented as \begin{align} h_{\mu\nu}(t,z)&= \bordermatrix{ ~&t&x&y&z\cr t&0&0&0&0\cr x&0&1&0&0\cr y&0&0&-1&0\cr z&0&0&0&0}h_{+}(t-z) +\bordermatrix{ ~&t&x&y&z\cr t&0&0&0&0\cr x&0&0&1&0\cr y&0&1&0&0\cr z&0&0&0&0}h_{\times}(t-z)=\\ &=e^{(+)}_{\mu\nu}h_{+}(t-z) +e^{(\times)}_{\mu\nu}h_{\times}(t-z). \end{align} Here $h_{+}$ and $h_\times$ are the amplitudes of the two independent components with linear polarization, and $e^{(\times)}_{\mu\nu},e^{(+)}_{\mu\nu}$ are the corresponding polarization tensors.



Problem 2: Two polarizations

Show that $e^{(\times)}_{\mu\nu}$ and $e^{(+)}_{\mu\nu}$ transform into each other under rotation by $\pi/8$



Problem 3: Plane wave TT gauge transformation

Consider the plane wave solution of the wave equation in the Lorenz gauge: \[\bar{h}_{\mu\nu} =A_{\mu\nu}e^{i\,k_{\lambda}x^\lambda}, \quad k^\mu k_\mu =0.\]

1) Show that the TT gauge is fixed by the coordinate transformation $x\to x+\xi$ with \begin{align} \xi_{\mu}&=B_{\mu}e^{ik_\lambda x^\lambda};\\ B_{\lambda} &=-\frac{A_{\mu\nu}l^\mu l^\nu} {8i \omega^4}k_\lambda -\frac{A^{\mu}_{\mu}}{4i\omega^2}l_\lambda +\frac{1}{2i\omega^2}A_{\lambda\mu}l^\mu;\\ &\text{where}\quad k^\mu=(\omega,\mathbf{k}),\quad l^{\mu}=(\omega,-\mathbf{k}). \end{align} 2) What is the transformation to the Lorenz gauge for arbitrary gravitational wave in vacuum?



Problem 3: Curvature of a plane wave

Consider the plane-wave solution, in which \[R_{\mu\nu\rho\sigma} =C_{\mu\nu\rho\sigma}e^{ik_{\lambda}x^{\lambda}}.\] \begin{enumerate} \item Using the Bianchi identity, show that all components of the curvature tensor can be expressed through UNIQ-MathJax36-QINU; \item Show that in the coordinate frame such that UNIQ-MathJax37-QINU is directed along the UNIQ-MathJax38-QINU-axis the only possible nonzero components are UNIQ-MathJax39-QINU, UNIQ-MathJax40-QINU and UNIQ-MathJax41-QINU, obeying UNIQ-MathJax42-QINU, leaving only two independent non-zero components; \item in the TT gauge (denoted by the superscript UNIQ-MathJax43-QINU) UNIQ-MathJax64-QINU \end{enumerate} [based on Padm p403].