<?xml version="1.0" encoding="utf-8" standalone="yes"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom">
  <channel>
    <title>Gabriele Bozzola&#39;s homepage on Gabriele Bozzola</title>
    <link>https://sbozzolo.github.io/</link>
    <description>Recent content in Gabriele Bozzola&#39;s homepage on Gabriele Bozzola</description>
    <generator>Hugo</generator>
    <language>en</language>
    <atom:link href="https://sbozzolo.github.io/index.xml" rel="self" type="application/rss+xml" />
    <item>
      <title></title>
      <link>https://sbozzolo.github.io/talks/</link>
      <pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate>
      <guid>https://sbozzolo.github.io/talks/</guid>
      <description>&lt;p&gt;I always enjoy talking about software and science. Get in touch with me&#xA;(&lt;a href=&#34;../about&#34;&gt;address in the homepage&lt;/a&gt;) if you would like to invite me for a talk.&lt;/p&gt;&#xA;&lt;h2 id=&#34;research-software-engineering&#34;&gt;Research software engineering&lt;/h2&gt;&#xA;&lt;ul&gt;&#xA;&lt;li&gt;&lt;a href=&#34;https://www.youtube.com/watch?v=IFrHXrtXebc&#34;&gt;The Future of Research is code: Embracing Research Software Engineering&lt;/a&gt;&lt;/li&gt;&#xA;&lt;li&gt;&lt;a href=&#34;https://www.youtube.com/watch?v=CP8r30s2SM8&#34;&gt;SCALE 2023 &amp;ndash; How to lower the entry barrier to your scientific software&lt;/a&gt;&lt;/li&gt;&#xA;&lt;/ul&gt;&#xA;&lt;h2 id=&#34;emacs&#34;&gt;Emacs&lt;/h2&gt;&#xA;&lt;ul&gt;&#xA;&lt;li&gt;&lt;a href=&#34;https://www.youtube.com/watch?v=RTVXaDR697k&#34;&gt;EmacsConf 2024 &amp;ndash; EmacsConf 2024: Exploring Shared Philosophies in Julia and Emacs&lt;/a&gt;&lt;/li&gt;&#xA;&lt;li&gt;&lt;a href=&#34;https://www.youtube.com/watch?v=cAep6Kj_4NM&#34;&gt;EmacsConf 2021 &amp;ndash; EmacsConf 2021: telega.el and the Emacs community on Telegram&lt;/a&gt;&lt;/li&gt;&#xA;&lt;li&gt;&lt;a href=&#34;https://www.youtube.com/watch?v=8oNycFLwKfE&#34;&gt;EmacsConf 2020 &amp;ndash; A tour of vterm&lt;/a&gt;&lt;/li&gt;&#xA;&lt;/ul&gt;&#xA;&lt;h2 id=&#34;kuibit--einstein-toolkit&#34;&gt;kuibit / Einstein Toolkit&lt;/h2&gt;&#xA;&lt;ul&gt;&#xA;&lt;li&gt;&#xA;&lt;p&gt;&lt;a href=&#34;https://youtu.be/14YOQ6SqTUU&#34;&gt;Tutorial: Post-processing Cactus simulations with Python&lt;/a&gt;&lt;/p&gt;</description>
    </item>
    <item>
      <title>More about me</title>
      <link>https://sbozzolo.github.io/about_fun/</link>
      <pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate>
      <guid>https://sbozzolo.github.io/about_fun/</guid>
      <description>&lt;style&gt;&#xA;.right {&#xA;  float: right;&#xA;}&#xA;&#xA;&lt;/style&gt;&#xA;&lt;h1 id=&#34;more-about-me&#34;&gt;More about me&lt;/h1&gt;&#xA;&lt;p&gt;Life is not all about numerical simulations and data analysis. In this page, I&#xA;collect some additional information about me that will help you understand&#xA;better who I am.&lt;/p&gt;&#xA;&lt;h2 id=&#34;i-am-a-fan-of&#34;&gt;I am a fan of&amp;hellip;&lt;/h2&gt;&#xA;&lt;p&gt;(in no particular order)&lt;/p&gt;&#xA;&lt;h3 id=&#34;national-parks&#34;&gt;National Parks&lt;/h3&gt;&#xA;&lt;figure class=&#34;right&#34;&gt;&#xA;    &lt;img style=&#34;margin: 2px; border-radius: 8px; &#34; src=&#34;../media/lake.jpg&#34; width=&#34;200&#34;&gt;&#xA;&lt;/figure&gt;&#xA;&lt;p&gt;I have the luck to live in a place that offers endless opportunities to enjoy&#xA;the outdoors, so my favorite weekend activities are hiking and cycling. When I&#xA;have a little bit more time, I love exploring the stunning National Parks and&#xA;Forests that are in Arizona and in the South West.&lt;/p&gt;</description>
    </item>
    <item>
      <title>Publications</title>
      <link>https://sbozzolo.github.io/publications/</link>
      <pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate>
      <guid>https://sbozzolo.github.io/publications/</guid>
      <description>&lt;h1 id=&#34;peer-reviewed-publications&#34;&gt;Peer-reviewed publications&lt;/h1&gt;&#xA;&lt;p&gt;In chronological order (first is most recent).&lt;/p&gt;&#xA;&lt;ol start=&#34;16&#34;&gt;&#xA;&lt;li&gt;M.\ Smith, V.\ Paschalidis, &lt;strong&gt;G. Bozzola&lt;/strong&gt;,&#xA;&lt;em&gt;High-energy interactions of charged black holes in full general relativity. II. Near-extremal merger remnants and universality with the irreducible mass&lt;/em&gt;. 2025, PRD 111, 104302 (&lt;a href=&#34;https://arxiv.org/abs/2412.01881&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;M.\ Smith, V.\ Paschalidis, &lt;strong&gt;G. Bozzola&lt;/strong&gt;,&#xA;&lt;em&gt;High-energy interactions of charged black holes in full general relativity. I. Zoom-whirl orbits and universality with the irreducible mass&lt;/em&gt;. 2025,  PRD 111, 104031 (&lt;a href=&#34;https://arxiv.org/abs/2411.11960&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;V. Manikantan, V.\ Paschalidis, &lt;strong&gt;G. Bozzola&lt;/strong&gt;,&#xA;Coincident Multimessenger Bursts from Eccentric Supermassive Binary Black Holes. 2025, APJL 984, L47&#xA;(&lt;a href=&#34;https://arxiv.org/abs/2411.11955&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;M. Naseri, &lt;strong&gt;G. Bozzola&lt;/strong&gt;, V. Paschalidis. &lt;em&gt;Exploring pathways to forming twin stars&lt;/em&gt;. 2024, PRD 110, 4,&#xA;44037084004 (&lt;a href=&#34;https://arxiv.org/abs/2406.15544&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, C. Chan, V. Paschalidis. &lt;em&gt;Not all spacetime coordinates for&#xA;general-relativistic ray tracing are created equal&lt;/em&gt;. 2023, PRD 108, 8,&#xA;084004 (&lt;a href=&#34;https://arxiv.org/pdf/2310.02321&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, V. Paschalidis. &lt;em&gt;Can quasi-circular mergers of charged&#xA;black holes produce extremal black holes?&lt;/em&gt;. 2023, PRD 107, 104059&#xA;(&lt;a href=&#34;https://arxiv.org/pdf/2309.04368&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;P. Espino, &lt;strong&gt;G. Bozzola&lt;/strong&gt;, V.\ Paschalidis, 2023, PRD 107, 104059&#xA;(&lt;a href=&#34;https://arxiv.org/abs/2210.13481&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;R. Luna, &lt;strong&gt;G. Bozzola&lt;/strong&gt;, V. Cardoso, V. Paschalidis, M. Zilhão. _&lt;em&gt;Kicks in&#xA;charged black hole binaries&lt;/em&gt;. 2022, PRD 106, 8, 084017&#xA;(&lt;a href=&#34;https://arxiv.org/abs/2207.06429&#34;&gt;arxiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, C. Chan, V. Paschalidis. Black Hole Physics and Computer&#xA;Graphics. 2022, CISE 24, 2&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;. &lt;em&gt;Does charge matter in high-energy collisions of black&#xA;holes?&lt;/em&gt;. 2022, PRL 128, 071101 (&lt;a href=&#34;https://arxiv.org/pdf/2202.05310&#34;&gt;arXiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, V. Paschalidis. &lt;em&gt;Numerical-relativity simulations of the&#xA;quasi-circular inspiral and merger of non-spinning, charged black holes:&#xA;methods and comparison with approximate approaches&lt;/em&gt;. 2021, PRD 104, 4, 044004&#xA;(&lt;a href=&#34;https://arxiv.org/pdf/2104.06978&#34;&gt;arXiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;.&#xA;&lt;em&gt;kuibit: Analyzing Einstein Toolkit simulations with Python&lt;/em&gt;.&#xA;2021, JOSS 60(6), 3099&#xA;(&lt;a href=&#34;https://arxiv.org/pdf/2104.06376&#34;&gt;arXiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, V. Paschalidis.&#xA;&lt;em&gt;General relativistic simulations of the quasi-circular inspiral and&#xA;merger of charged black holes: GW150914 and fundamental physics implications&lt;/em&gt;.&#xA;2021, PRL. 126, 041103&#xA;(&lt;a href=&#34;https://arxiv.org/pdf/2006.15764&#34;&gt;arXiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, P. Espino, C. Lewin, V. Paschalidis.&#xA;&lt;em&gt;Maximum mass, solution space and universal relations of rotating&#xA;relativistic hadron-quark hybrid stars&lt;/em&gt;. 2019, EPJA A 55 9, 149&#xA;(&lt;a href=&#34;https://arxiv.org/pdf/1905.00028&#34;&gt;arXiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, V. Paschalidis. &lt;em&gt;Initial data for general relativistic&#xA;simulations of multiple electrically charged black holes with linear and&#xA;angular momenta&lt;/em&gt;. 2019, PRD 99, 10, 104044&#xA;(&lt;a href=&#34;https://arxiv.org/pdf/1903.01036&#34;&gt;arXiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;li&gt;&lt;strong&gt;G. Bozzola&lt;/strong&gt;, N. Stergioulas, A. Bauswein. &lt;em&gt;Universal relations for&#xA;differentially rotating relativistic stars at the threshold to collapse&lt;/em&gt;.&#xA;2018, MNRAS 474, 3557–3564 (&lt;a href=&#34;https://arxiv.org/pdf/1709.02787&#34;&gt;arXiv&lt;/a&gt;)&lt;/li&gt;&#xA;&lt;/ol&gt;</description>
    </item>
    <item>
      <title>Research</title>
      <link>https://sbozzolo.github.io/research/</link>
      <pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate>
      <guid>https://sbozzolo.github.io/research/</guid>
      <description>&lt;style&gt;&#xA;.left {&#xA;  float: left;&#xA;}&#xA;&#xA;.right {&#xA;  float: right;&#xA;}&#xA;&#xA;figure {&#xA;    display: table;&#xA;}&#xA;&#xA;figcaption {&#xA;  font-size: 14px;&#xA;  font-style: italic;&#xA;  text-align: center;&#xA;  display: table-caption;&#xA;  caption-side: bottom;&#xA;}&#xA;&lt;/style&gt;&#xA;&lt;p&gt;The intended audience of this page are specialists (i.e., physicists,&#xA;astronomers, &amp;hellip;). You can find the version for the general public&#xA;&lt;a href=&#34;../research_general&#34;&gt;here&lt;/a&gt;.&lt;/p&gt;&#xA;&lt;h2 id=&#34;numerical-relativity-and-gravitational-wave-astronomy&#34;&gt;Numerical relativity and gravitational wave astronomy&lt;/h2&gt;&#xA;&lt;p&gt;Broadly speaking, my research focuses on strongly gravitating systems, such as&#xA;black holes and neutron stars. I develop and use computational methods and codes&#xA;to tackle problems in strong gravity and I primarily work in numerical&#xA;relativity, field that is concerned with finding numerical solutions to the&#xA;equations of general relativity. I am deeply interested in using simulations to&#xA;push our physical theories to their limits and learn more about fundamental&#xA;physics. One of the main ways I am doing this is by using gravitational waves to&#xA;interface with observations and experiments. Gravitational waves (detected for&#xA;the first time in 2015) offer a completely new way to study the universe and are&#xA;providing invaluable data to address long standing questions.&lt;/p&gt;</description>
    </item>
    <item>
      <title>Research</title>
      <link>https://sbozzolo.github.io/research_general/</link>
      <pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate>
      <guid>https://sbozzolo.github.io/research_general/</guid>
      <description>&lt;style&gt;&#xA;.left {&#xA;  float: left;&#xA;}&#xA;&#xA;.right {&#xA;  float: right;&#xA;}&#xA;&#xA;figure {&#xA;    display: table;&#xA;}&#xA;&#xA;figcaption {&#xA;  font-size: 14px;&#xA;  font-style: italic;&#xA;  text-align: center;&#xA;  display: table-caption;&#xA;  caption-side: bottom;&#xA;}&#xA;&lt;/style&gt;&#xA;&lt;p&gt;The intended audience of this page is the general public. You can find the&#xA;version for specialists &lt;a href=&#34;../research&#34;&gt;here&lt;/a&gt;.&lt;/p&gt;&#xA;&lt;h2 id=&#34;numerical-relativity&#34;&gt;Numerical relativity&lt;/h2&gt;&#xA;&lt;p&gt;General relativity is one of the most famous and well-established physical&#xA;theories. The first formulation is due to Albert Einstein and it is more than&#xA;100 years old. Despite the age, it was only with the advent of computers that&#xA;scientists managed to unlock some of the most ground-braking predictions of the&#xA;theory, such as detailed models for gravitational waves. Putting general&#xA;relativity on a computer was no easy task and an entire new branch of physics&#xA;was born in the effort. I specialize in this field, known as &lt;em&gt;numerical&#xA;relativity&lt;/em&gt;. Today, we can perform successful numerical-relativity simulations&#xA;of several different systems and build models that guide and explain&#xA;astronomical observations. In my research, I apply numerical-relativity&#xA;techniques to study binary systems, and I extend our computational and&#xA;theoretical methods for numerical relativity in general.&lt;/p&gt;</description>
    </item>
    <item>
      <title>Resume</title>
      <link>https://sbozzolo.github.io/resume/</link>
      <pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate>
      <guid>https://sbozzolo.github.io/resume/</guid>
      <description>&lt;h4 id=&#34;interests&#34;&gt;INTERESTS&lt;/h4&gt;&#xA;&lt;p&gt;High-performance computing, (research) software engineering, open source&#xA;software, open science, community and inclusion.&lt;/p&gt;&#xA;&lt;h4 id=&#34;work-experience&#34;&gt;WORK EXPERIENCE&lt;/h4&gt;&#xA;&lt;ul&gt;&#xA;&lt;li&gt;&#xA;&lt;p&gt;Applied Scientist, Center for Quantum Computing, Amazon, San&#xA;Francisco (CA). Jun 2025 &amp;ndash;&lt;/p&gt;&#xA;&lt;/li&gt;&#xA;&lt;li&gt;&#xA;&lt;p&gt;Senior Software Engineer at &lt;a href=&#34;https://clima.caltech.edu&#34;&gt;CliMA&lt;/a&gt;,&#xA;California Institute of Technology, Pasadena (CA). Nov 2024 &amp;ndash; Jun&#xA;2025&lt;/p&gt;&#xA;&lt;/li&gt;&#xA;&lt;li&gt;&#xA;&lt;p&gt;Software Engineer at &lt;a href=&#34;https://clima.caltech.edu&#34;&gt;CliMA&lt;/a&gt;, California&#xA;Institute of Technology, Pasadena (CA). Aug 2023 &amp;ndash; Nov 2024&lt;/p&gt;&#xA;&lt;/li&gt;&#xA;&lt;li&gt;&#xA;&lt;p&gt;Research and Teaching Assistant at University of Arizona, Tucson&#xA;(AZ). Jan 2018 &amp;ndash; Aug 2023&lt;/p&gt;</description>
    </item>
    <item>
      <title>Software</title>
      <link>https://sbozzolo.github.io/software/</link>
      <pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate>
      <guid>https://sbozzolo.github.io/software/</guid>
      <description>&lt;h2 id=&#34;scientific-codes&#34;&gt;Scientific codes&lt;/h2&gt;&#xA;&lt;h3 id=&#34;clima-packages&#34;&gt;CliMA packages&lt;/h3&gt;&#xA;&lt;p&gt;I develop and contribute to several packages at&#xA;&lt;a href=&#34;https://github.com/CliMA&#34;&gt;CliMA&lt;/a&gt; (in particular, I designed and authored&#xA;&lt;a href=&#34;https://github.com/CliMA/ClimaAnalysis.jl&#34;&gt;ClimaAnalysis&lt;/a&gt;,&#xA;&lt;a href=&#34;https://github.com/CliMA/ClimaUtilities.jl&#34;&gt;ClimaUtilities&lt;/a&gt;,&#xA;&lt;a href=&#34;https://github.com/CliMA/ClimaDiagnostics.jl&#34;&gt;ClimaDiagnostics&lt;/a&gt;). While I do a&#xA;little bit of everything (performance, user interface, physics, reliability,&#xA;&amp;hellip;), one of my main areas of focus is data in its entire life cycle, from&#xA;ingestion to post-processing and visualization.&lt;/p&gt;&#xA;&lt;h3 id=&#34;kuibit&#34;&gt;kuibit&lt;/h3&gt;&#xA;&lt;img style=&#34;float: center;&#34; src=&#34;../media/kuibit.png&#34; width=&#34;300&#34;&gt;&#xA;&lt;p&gt;&lt;a href=&#34;https://sbozzolo.github.io/kuibit&#34;&gt;kuibit&lt;/a&gt; is&#xA;a large Python library to analyze simulations performed with the Einstein Toolkit. The&#xA;package takes care of all the low-level details and removes most of the friction&#xA;in studying simulation outputs.&lt;/p&gt;</description>
    </item>
  </channel>
</rss>
