From 92c16ab89695d12a027e8346ff94e6ccd678d4c1 Mon Sep 17 00:00:00 2001 From: "Josu C. Aurrekoetxea" <32845353+JCAurre@users.noreply.github.com> Date: Wed, 16 Aug 2023 08:48:10 +0100 Subject: [PATCH] Update paper.md --- paper/paper.md | 7 ++----- 1 file changed, 2 insertions(+), 5 deletions(-) diff --git a/paper/paper.md b/paper/paper.md index 0076c1b..3d303ce 100644 --- a/paper/paper.md +++ b/paper/paper.md @@ -104,11 +104,8 @@ So far the code has been used to study a range of fundamental physics problems: - Growth of scalar hair around a Schwarzschild [@Clough:2019jpm] and a Kerr [@Bamber:2020bpu] black hole - Determining the relativistic drag forces on a Schwarzschild black hole moving through a cloud of scalar field dark matter [@Traykova:2021dua;@Traykova:2023qyv] -![Formation of overdense tail of scalar dark matter behind a moving BH, due to dynamical friction \label{fig:friction}](Figures/friction.png){ width=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}](Figures/accretion.png){ width=45% } - -![Formation of overdense tail of scalar dark matter behind a moving BH, due to dynamical friction \label{fig:friction}]“” -![The evolution of scalar clouds around black hole binaries in, the initial conditions were generated with a modified version of GRDzhadzha \label{fig:accretion}]“” +![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% } - Studying the dynamical friction effects on a Kerr black hole (Magnus effect) [@Wang:inprep]