Difference between revisions of "Transverse traceless gauge"

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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
 
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}
 
\begin{equation}
\pa_\mu {h^{\mu}}_{\nu}=0,\quad
+
\partial_\mu {h^{\mu}}_{\nu}=0,\quad
 
h_{0\mu}=0,\quad {h^{\mu}}_{\mu}=0.
 
h_{0\mu}=0,\quad {h^{\mu}}_{\mu}=0.
 
\end{equation}
 
\end{equation}
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  Then the remaining Lorenz condition is reduced to
 
  Then the remaining Lorenz condition is reduced to
 
\begin{align*}
 
\begin{align*}
&0=\pa_0 h^0_\nu +\pa_\alpha h^\alpha_\nu ;\\
+
&0=\partial_0 h^0_\nu +\partial_\alpha h^\alpha_\nu ;\\
 
\nu=0:\quad& 0=0;\\
 
\nu=0:\quad& 0=0;\\
\nu=\beta:\quad&0= \pa_{\alpha}{s^{\alpha}}_{\beta},
+
\nu=\beta:\quad&0= \partial_{\alpha}{s^{\alpha}}_{\beta},
 
\end{align*}
 
\end{align*}
 
so it takes the form
 
so it takes the form
 
\begin{equation}
 
\begin{equation}
\pa_{\alpha}{s^{\alpha}}_{\beta}=0.
+
\partial_{\alpha}{s^{\alpha}}_{\beta}=0.
 
\end{equation}
 
\end{equation}
 
Thus the only remaining non-trivial component of the perturbation is the tensor one (the traceless part) $s_{\alpha\beta}$, and it is transverse, in the sense that for a plane wave solution $s_{\alpha\beta}\sim e^{i\,k_{\mu}x^{\mu}}$ the metric perturbation is transverse with respect to the wave vector:
 
Thus the only remaining non-trivial component of the perturbation is the tensor one (the traceless part) $s_{\alpha\beta}$, and it is transverse, in the sense that for a plane wave solution $s_{\alpha\beta}\sim e^{i\,k_{\mu}x^{\mu}}$ the metric perturbation is transverse with respect to the wave vector:
Line 163: Line 163:
 
\item 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
 
\[A_{\mu\nu}\to A_{\mu\nu}'
 
\[A_{\mu\nu}\to A_{\mu\nu}'
=A_{\mu\nu}-2\pa_{(\mu}\xi_{\nu)}
+
=A_{\mu\nu}-2\partial_{(\mu}\xi_{\nu)}
+\eta_{\mu\nu}\pa_{\lambda}\xi^\lambda,\]
+
+\eta_{\mu\nu}\partial_{\lambda}\xi^\lambda,\]
 
so
 
so
 
\begin{equation}
 
\begin{equation}
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\item in the TT gauge (denoted by the superscript $TT$)
 
\item in the TT gauge (denoted by the superscript $TT$)
 
\[R_{0\alpha 0\beta}
 
\[R_{0\alpha 0\beta}
=-\tfrac{1}{2}\pa_0^2 g_{\alpha\beta}^{TT};\]
+
=-\tfrac{1}{2}\partial_0^2 g_{\alpha\beta}^{TT};\]
 
\end{enumerate}
 
\end{enumerate}
 
[based on Padm p403].
 
[based on Padm p403].
Line 245: Line 245:
 
\item In the TT gauge $g_{00}$ and $g_{0\alpha}$ are zero, so in the first order
 
\item In the TT gauge $g_{00}$ and $g_{0\alpha}$ are zero, so in the first order
 
\[R_{0\alpha 0\beta}=\frac{1}{2}\big(
 
\[R_{0\alpha 0\beta}=\frac{1}{2}\big(
\pa_0 \pa_\beta g_{0\alpha}
+
\partial_0 \partial_\beta g_{0\alpha}
+\pa_\alpha \pa_0 g_{0\beta}
+
+\partial_\alpha \partial_0 g_{0\beta}
-\pa_0 \pa_0 g_{\alpha\beta}
+
-\partial_0 \partial_0 g_{\alpha\beta}
-\pa_\alpha \pa_\beta g_{00}\big)
+
-\partial_\alpha \partial_\beta g_{00}\big)
=-\tfrac12 \pa_0^2 g_{\alpha\beta}.\]
+
=-\tfrac12 \partial_0^2 g_{\alpha\beta}.\]
 
As the curvature tensor is gauge invariant, the last relation allows one to calculate the metric components in the TT gauge $g_{\alpha\beta}^{TT}$ without the prior gauge fixing.
 
As the curvature tensor is gauge invariant, the last relation allows one to calculate the metric components in the TT gauge $g_{\alpha\beta}^{TT}$ without the prior gauge fixing.
 
\end{enumerate}</p>
 
\end{enumerate}</p>
 
   </div>
 
   </div>
 
</div></div>
 
</div></div>

Revision as of 14:25, 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 \begin{enumerate} \item in terms of scalar, vector and tensor decomposition; \item in terms of the metric perturbation for the plane wave solution UNIQ-MathJax58-QINU with wave vector UNIQ-MathJax10-QINU directed along the UNIQ-MathJax11-QINU-axis. \end{enumerate}



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: \[\bar{h}_{\mu\nu} =A_{\mu\nu}e^{i\,k_{\lambda}x^\lambda}, \quad k^\mu k_\mu =0.\] \begin{enumerate} \item Show that the TT gauge is fixed by the coordinate transformation UNIQ-MathJax31-QINU 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} [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 $B=C_1 k+ C_2 l +C_{3} w$.}] \item What is the transformation to the Lorenz gauge for arbitrary gravitational wave in vacuum? \end{enumerate}



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-MathJax39-QINU; \item Show that in the coordinate frame such that UNIQ-MathJax40-QINU is directed along the UNIQ-MathJax41-QINU-axis the only possible nonzero components are UNIQ-MathJax42-QINU, UNIQ-MathJax43-QINU and UNIQ-MathJax44-QINU, obeying UNIQ-MathJax45-QINU, leaving only two independent non-zero components; \item in the TT gauge (denoted by the superscript UNIQ-MathJax46-QINU) UNIQ-MathJax67-QINU \end{enumerate} [based on Padm p403].