<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>0011-1503</journal-id>
<journal-title><![CDATA[Crítica (México, D.F.)]]></journal-title>
<abbrev-journal-title><![CDATA[Crítica (Méx., D.F.)]]></abbrev-journal-title>
<issn>0011-1503</issn>
<publisher>
<publisher-name><![CDATA[Universidad Nacional Autónoma de México, Instituto de Investigaciones Filosóficas]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0011-15032021000300073</article-id>
<article-id pub-id-type="doi">10.22201/iifs.18704905e.2021.1294</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Black hole philosophy]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Romero]]></surname>
<given-names><![CDATA[Gustavo E.]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Universidad Nacional de La Plata  ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
<country>Argentina</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>00</month>
<year>2021</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>00</month>
<year>2021</year>
</pub-date>
<volume>53</volume>
<numero>159</numero>
<fpage>73</fpage>
<lpage>132</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0011-15032021000300073&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0011-15032021000300073&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0011-15032021000300073&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[Summary Black holes are arguably the most extraordinary physical objects we know in the universe. Despite our thorough knowledge of black hole dynamics and our ability to solve Einstein's equations in situations of ever increasing complexity, the deeper implications of the very existence of black holes for our understanding of space, time, causality, information, and many other things remain poorly understood. In this paper I survey some of these problems. If something is going to be clear from my presentation, I hope it will be that around black holes science and metaphysics become more interwoven than anywhere else in the universe.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Resumen Los agujeros negros son posiblemente los objetos físicos más extraordinarios que conocemos en el universo. A pesar de nuestro gran conocimiento de su dinámica y de nuestra capacidad para resolver las ecuaciones de Einstein en situaciones de creciente complejidad, seguimos teniendo un entendimiento limitado de las implicaciones más profundas de la existencia de los agujeros negros para nuestra comprensión del espacio, el tiempo, la causalidad, la información y muchas otras cosas. Aquí examino algunos de estos problemas. Espero que quede claro a partir de mi presentación que alrededor de los agujeros negros la ciencia y la metafísica se entrelazan más que en cualquier otro lugar del universo.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[spacetime]]></kwd>
<kwd lng="en"><![CDATA[causality]]></kwd>
<kwd lng="en"><![CDATA[time arrows]]></kwd>
<kwd lng="en"><![CDATA[thermodynamics]]></kwd>
<kwd lng="en"><![CDATA[ontology]]></kwd>
<kwd lng="es"><![CDATA[espaciotiempo]]></kwd>
<kwd lng="es"><![CDATA[causalidad]]></kwd>
<kwd lng="es"><![CDATA[flechas del tiempo]]></kwd>
<kwd lng="es"><![CDATA[termodinámica]]></kwd>
<kwd lng="es"><![CDATA[ontología]]></kwd>
</kwd-group>
</article-meta>
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