Difference between revisions of "Motivation and symmetries / Introduction"

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(Problem 10: Upper bound on frequency)
 
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   <div class="NavHead">solution</div>
 
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     <p style="text-align: left;">Let us consider isolated systems of charges or masses that generate electromagnetic or gravitational waves correspondingly. The momentum of an isolated system is conserved, but existence of positive and negative charges (or just bodies with different rations $q/m$) allows one to create alternating dipole moment $\sum q_{i}\mathbf{r}_{i}$ while conserving the momentum $\sum m_{i}\mathbf{r}_{i}=const$. For gravity, however, the charge ''is'' the mass, which is the principle of equivalence lying at the heart of General Relativity, so that is impossible. This is the reason that in electromagnetic radiation the dominating term is usually the first one allowed, i.e. the dipole one, while for gravitational radiation the first possibly non-zero radiation term is the quadrupole one.
+
     <p style="text-align: left;">Let us consider isolated systems of charges or masses that generate electromagnetic or gravitational waves correspondingly. The momentum of an isolated system is conserved, but existence of positive and negative charges (or just bodies with different rations $q/m$) allows one to create alternating dipole moment $\sum q_{i}\mathbf{r}_{i}$ while conserving the momentum $\sum m_{i}\mathbf{r}_{i}=const$. For gravity, however, the charge ''is'' the mass, which is the principle of equivalence lying at the heart of General Relativity, so that is impossible. This is the reason that in electromagnetic radiation the dominating term is usually the first one allowed, i.e. the dipole one, while for gravitational radiation the first possibly non-zero radiation term is the quadrupole one.</p>
<br/>
+
 
 
<gallery widths=400px heights=200px>
 
<gallery widths=400px heights=200px>
 
File:Dipole.png|
 
File:Dipole.png|
 
</gallery>
 
</gallery>
Einstein writes of this in a letter to K.Shwarzshild (Feb 19, 1916):
+
 
 +
<p style="text-align: left;"> Einstein writes of this in a letter to K.Shwarzshild (Feb 19, 1916):
 
"Thus there are no gravitational waves analogous to light waves.  This probably is also related to the one-sidedness of the sign of scalar $T$, incidentally. (Nonexistence of the "dipole".)"
 
"Thus there are no gravitational waves analogous to light waves.  This probably is also related to the one-sidedness of the sign of scalar $T$, incidentally. (Nonexistence of the "dipole".)"
 
<br/>
 
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\[\frac{dE}{dt}\sim
 
\[\frac{dE}{dt}\sim
 
\frac{G}{c^5}\cdot
 
\frac{G}{c^5}\cdot
\dddot{Q}_{\alpha\beta}
+
{\dddot{Q}}_{\alpha\beta}
\dddot{Q}^{\alpha\beta},\]
+
{\dddot{Q}}^{\alpha\beta},\]
 
where
 
where
 
\[Q_{\alpha\beta}=\int d^3 x \;
 
\[Q_{\alpha\beta}=\int d^3 x \;
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     <p style="text-align: left;">As seen above, from symmetry considerations the gravitational wave amplitude far from the source should be expressed in terms of time derivatives of the second mass (quadrupole) moment $h^{\mu\nu}\sim \frac{d^n}{dt^n}I^{\mu\nu}$, and we expect the energy flux to be quadratic in the wave amplitude. The luminosity $L_{GW}$  (total radiated power) in gravitational radiation should, therefore, also be quadratic in $I^{\mu\nu}$  and its time derivatives.
 
     <p style="text-align: left;">As seen above, from symmetry considerations the gravitational wave amplitude far from the source should be expressed in terms of time derivatives of the second mass (quadrupole) moment $h^{\mu\nu}\sim \frac{d^n}{dt^n}I^{\mu\nu}$, and we expect the energy flux to be quadratic in the wave amplitude. The luminosity $L_{GW}$  (total radiated power) in gravitational radiation should, therefore, also be quadratic in $I^{\mu\nu}$  and its time derivatives.
 
<br/>
 
<br/>
In units $G=c=1$ luminosity  $L_{GW}$ is dimensionless. The third  time derivative of $I^{\mu\nu}$ is also dimensionless; therefore, $L_{GW}$ must be a quadratic combination of $\dddot{I}^{\mu\nu}$. $L_{GW}$  also behaves as a scalar under rotations in space and so must be a quadratic scalar combination of $\dddot{I}_{\mu\nu}\dddot{I}^{\mu\nu}$ or $(\dddot{I}^\mu_\mu)^2$ . The precise combination is fixed by the demand that there is no radiation from a spherically symmetric system. In this case $I^{\mu\nu}\sim \delta^{\mu\nu}$ and the combination (reduced quadrupole momentum tensor)
+
In units $G=c=1$ luminosity  $L_{GW}$ is dimensionless. The third  time derivative of $I^{\mu\nu}$ is also dimensionless; therefore, $L_{GW}$ must be a quadratic combination of ${\dddot{I}}^{\mu\nu}$. $L_{GW}$  also behaves as a scalar under rotations in space and so must be a quadratic scalar combination of ${\dddot{I}}_{\mu\nu}{\dddot{I}}^{\mu\nu}$ or ${(\dddot{I}}^\mu_\mu)^2$ . The precise combination is fixed by the demand that there is no radiation from a spherically symmetric system. In this case $I^{\mu\nu}\sim \delta^{\mu\nu}$ and the combination (reduced quadrupole momentum tensor)
 
\[Q^{\mu\nu}\equiv I^{\mu\nu}
 
\[Q^{\mu\nu}\equiv I^{\mu\nu}
 
-\frac{1}{3}\delta^{\mu\nu}I_{\lambda}^{\lambda}\]
 
-\frac{1}{3}\delta^{\mu\nu}I_{\lambda}^{\lambda}\]
 
vanishes. Consequently,
 
vanishes. Consequently,
 
\[L_{GW}\sim
 
\[L_{GW}\sim
\dddot{Q}^{\mu\nu}\dddot{Q}_{\mu\nu}.\]
+
{\dddot{Q}}^{\mu\nu}{\dddot{Q}}_{\mu\nu}.\]
  
 
The principle of equivalence states that locally gravitational field can always be turned to zero by an appropriate choice of reference frame. Therefore local energy density of a gravitational field will always depend on the coordinate frame (and gauge) and cannot be well-defined: it is not a tensor quantity. So in order to obtain some meaningful notion of $L_{GW}$, one has to average  the obtained expression over spacetime volumes of the scales of the wavelength (which should be much less than curvature radius).</p>
 
The principle of equivalence states that locally gravitational field can always be turned to zero by an appropriate choice of reference frame. Therefore local energy density of a gravitational field will always depend on the coordinate frame (and gauge) and cannot be well-defined: it is not a tensor quantity. So in order to obtain some meaningful notion of $L_{GW}$, one has to average  the obtained expression over spacetime volumes of the scales of the wavelength (which should be much less than curvature radius).</p>

Latest revision as of 12:52, 15 January 2013



Problem 1: Decoupling time

Show that relic neutrinos can provide us with information on the Universe at temperatures less that 1 MeV (i.e. from the age of the order of seconds). What is the corresponding limit for gravitons?


Problem 2: Gravitational waves on curved background

The basic theory of gravitational waves, discussed below, deals mostly with small perturbations on flat Minkowski background. Can this approximation be useful for studying waves on a non-trivial non-flat background, and if yes then in which cases?


Problem 3: No monopole radiation

Show that generation of either electromagnetic or gravitational monopole radiation is impossible.


Problem 4: No dipole gravitational radiation

Show that dipole gravitational radiation is prohibited by the momentum conservation law.



Problem 5: Quadrupole formula from dimensional analysis

Obtain, using dimensional analysis, the quadrupole formula for the energy loss by a system due to emission of gravitational waves \[\frac{dE}{dt}\sim \frac{G}{c^5}\cdot {\dddot{Q}}_{\alpha\beta} {\dddot{Q}}^{\alpha\beta},\] where \[Q_{\alpha\beta}=\int d^3 x \; ( x_\alpha x_\beta -\tfrac13 r^2 \delta_{\alpha\beta}) \rho(\mathbf{x}).\] is the reduced quadrupole moment of the system.



Problem 6: Natural luminosity

Using the quadrupole formula, find the upper limit for gravitational luminosity of a source.



Problem 7: Natural luminosity from dimensional analysis

Construct the limiting luminosity from dimensional analysis



Problem 8: Quantum luminosity limit

Why the upper limit on luminosity, obtained in General Relativity, should not change in the future quantum theory of gravitation?



Problem 9: Gravitationally bound systems

Estimate the gravitational luminosity for gravitationally bound systems



Problem 10: Upper bound on frequency

Estimate the upper bound of the gravitational wave frequency generated by a compact source with size $R$ and mass $M$.