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GRTLCollaboration · Aug 16, 2023 · e371672 · e371672
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@@ -107,6 +107,9 @@ So far the code has been used to study a range of fundamental physics problems:
 ![Formation of overdense tail of scalar dark matter behind a moving BH, due to dynamical friction \label{fig:friction}](Figures/friction.png){ width=15% }
 ![The evolution of scalar clouds around black hole binaries in, the initial conditions were generated with a modified version of GRDzhadzha \label{fig:accretion}](Figures/accretion.png){ width=15% }
 
+![Formation of overdense tail of scalar dark matter behind a moving BH, due to dynamical friction \label{fig:friction}]<img src="Figures/friction.png" alt= “” width="45%" height="45%">
+![The evolution of scalar clouds around black hole binaries in, the initial conditions were generated with a modified version of GRDzhadzha \label{fig:accretion}]<img src="Figures/accretion.png" alt= “” width="45%" height="45%">
+
 
 - Studying the dynamical friction effects on a Kerr black hole (Magnus effect) [@Wang:inprep]
 - Superradiance with self-interacting vector field [@Clough:2022ygm] and with spatially varying mass [@Wang:2022hra]