{"id":65437,"date":"2022-11-01T14:20:05","date_gmt":"2022-11-01T13:20:05","guid":{"rendered":"https:\/\/aktuelles.uni-frankfurt.de\/?p=65437"},"modified":"2023-02-17T11:16:09","modified_gmt":"2023-02-17T10:16:09","slug":"as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions","status":"publish","type":"post","link":"https:\/\/aktuelles.uni-frankfurt.de\/en\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/","title":{"rendered":"As dense as it gets: New Model for Matter in Neutron Star Collisions"},"content":{"rendered":"<p><strong>With the exception of black holes, neutron stars are the densest objects in our universe. As their name suggests, neutron stars are mainly made of neutrons. However, our knowledge about the matter produced during the collision of two neutron stars is still limited. Scientists from Goethe University Frankfurt and the Asia Pacific Center for Theoretical Physics in Pohang have now developed a new model that gives insights about matter under such extreme conditions.<\/strong><\/p>\n\n\n\n<figure class=\"wp-block-image aligncenter size-full\"><a href=\"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/pm_10_DichteMaterie_en.jpg\"><img fetchpriority=\"high\" decoding=\"async\" width=\"850\" height=\"690\" src=\"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/pm_10_DichteMaterie_en.jpg\" alt=\"\" class=\"wp-image-65522\" srcset=\"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/pm_10_DichteMaterie_en.jpg 850w, https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/pm_10_DichteMaterie_en-300x244.jpg 300w, https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/pm_10_DichteMaterie_en-768x623.jpg 768w, https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/pm_10_DichteMaterie_en-15x12.jpg 15w\" sizes=\"(max-width: 850px) 100vw, 850px\" \/><\/a><figcaption>Illustration of the new method: the researchers use five-dimensional black holes (right) to calculate the phase diagram of strongly coupled matter (middle), enabling simulations of neutron star mergers and the produced gravitational waves (left).<\/figcaption><\/figure>\n\n\n\n<p>After a massive star has burned its fuel and explodes as a supernova, an extremely compact object, called a neutron star, can be formed. Neutron stars are extraordinarily dense: To reach the density inside them, one would need to squeeze a massive body like our sun down to the size of a city like Frankfurt. In 2017, gravitational waves, the small ripples in spacetime that are produced during a collision of two neutron stars, could be directly measured here on earth for the first time. However, the composition of the resulting hot and dense merger product is not known precisely. It is still an open question, for instance, whether quarks, which are otherwise trapped in neutrons, can appear in free form after the collision. Dr. Christian Ecker from the Institute for Theoretical Physics of Goethe University Frankfurt, Germany, and Dr. Matti J\u00e4rvinen and Dr. Tuna Demircik from the Asia Pacific Center for Theoretical Physics in Pohang, South Korea, have now developed a new model that allows them to get one step closer to answering this question.<\/p>\n\n\n\n<p>In their work, they extend models from nuclear physics, which are not applicable at high densities, with a method used in string theory to describe the transition to dense and hot quark matter. \u201cOur method uses a mathematical relationship found in string theory, namely the correspondence between five-dimensional black holes and strongly interacting matter, to describe the phase transition between dense nuclear and quark matter\u201d, explain Dr. Demircik and Dr. J\u00e4rvinen. \u201dWe have already used the new model in computer simulations to calculate the gravitational-wave signal from these collisions and show that both hot and cold quark matter can be produced\u201d, adds Dr. Ecker, who implemented these simulations in collaboration with Samuel Tootle and Konrad Topolski from the working group of Prof. Luciano Rezzolla at Goethe University in Frankfurt. Next, the researchers hope to be able to compare their simulations with future gravitational waves measured from space in order to gain further insights into quark matter in neutron star collisions.<\/p>\n\n\n\n<p class=\"has-background\" style=\"background-color:#eeeeee\"><strong>Publication: <\/strong><a href=\"https:\/\/journals.aps.org\/prx\/abstract\/10.1103\/PhysRevX.12.041012\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/journals.aps.org\/prx\/abstract\/10.1103\/PhysRevX.12.041012<\/a><\/p>","protected":false},"excerpt":{"rendered":"<p>With the exception of black holes, neutron stars are the densest objects in our universe. As their name suggests, neutron stars are mainly made of neutrons. However, our knowledge about [&hellip;]<\/p>\n","protected":false},"author":8,"featured_media":65474,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_eb_attr":"","_price":"","_stock":"","_tribe_ticket_header":"","_tribe_default_ticket_provider":"","_ticket_start_date":"","_ticket_end_date":"","_tribe_ticket_show_description":"","_tribe_ticket_show_not_going":false,"_tribe_ticket_use_global_stock":"","_tribe_ticket_global_stock_level":"","_global_stock_mode":"","_global_stock_cap":"","_tribe_rsvp_for_event":"","_tribe_ticket_going_count":"","_tribe_ticket_not_going_count":"","_tribe_tickets_list":"[]","_tribe_ticket_has_attendee_info_fields":false,"footnotes":""},"categories":[126,254],"tags":[242],"post_folder":[],"class_list":["post-65437","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-english","category-research","tag-physics"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.3 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>As dense as it gets: New Model for Matter in Neutron Star Collisions | Aktuelles aus der Goethe-Universit\u00e4t Frankfurt<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/aktuelles.uni-frankfurt.de\/en\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/\" \/>\n<meta property=\"og:locale\" content=\"en_GB\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"As dense as it gets: New Model for Matter in Neutron Star Collisions | Aktuelles aus der Goethe-Universit\u00e4t Frankfurt\" \/>\n<meta property=\"og:description\" content=\"With the exception of black holes, neutron stars are the densest objects in our universe. As their name suggests, neutron stars are mainly made of neutrons. However, our knowledge about [&hellip;]\" \/>\n<meta property=\"og:url\" content=\"https:\/\/aktuelles.uni-frankfurt.de\/en\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/\" \/>\n<meta property=\"og:site_name\" content=\"Aktuelles aus der Goethe-Universit\u00e4t Frankfurt\" \/>\n<meta property=\"article:published_time\" content=\"2022-11-01T13:20:05+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2023-02-17T10:16:09+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/beitragsbild_Neutronensternenkollisionen.jpg\" \/>\n\t<meta property=\"og:image:width\" content=\"650\" \/>\n\t<meta property=\"og:image:height\" content=\"450\" \/>\n\t<meta property=\"og:image:type\" content=\"image\/jpeg\" \/>\n<meta name=\"author\" content=\"-\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"-\" \/>\n\t<meta name=\"twitter:label2\" content=\"Estimated reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"2 minutes\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\\\/\\\/schema.org\",\"@graph\":[{\"@type\":\"Article\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/#article\",\"isPartOf\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/\"},\"author\":{\"name\":\"-\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#\\\/schema\\\/person\\\/8e55ea338fb65d1ce87a91565d1f1739\"},\"headline\":\"As dense as it gets: New Model for Matter in Neutron Star Collisions\",\"datePublished\":\"2022-11-01T13:20:05+00:00\",\"dateModified\":\"2023-02-17T10:16:09+00:00\",\"mainEntityOfPage\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/\"},\"wordCount\":465,\"publisher\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#organization\"},\"image\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/#primaryimage\"},\"thumbnailUrl\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/wp-content\\\/uploads\\\/2022\\\/11\\\/beitragsbild_Neutronensternenkollisionen.jpg\",\"keywords\":[\"Physics\"],\"articleSection\":[\"English\",\"Research\"],\"inLanguage\":\"en-GB\"},{\"@type\":\"WebPage\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/\",\"url\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/\",\"name\":\"As dense as it gets: New Model for Matter in Neutron Star Collisions | Aktuelles aus der Goethe-Universit\u00e4t Frankfurt\",\"isPartOf\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#website\"},\"primaryImageOfPage\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/#primaryimage\"},\"image\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/#primaryimage\"},\"thumbnailUrl\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/wp-content\\\/uploads\\\/2022\\\/11\\\/beitragsbild_Neutronensternenkollisionen.jpg\",\"datePublished\":\"2022-11-01T13:20:05+00:00\",\"dateModified\":\"2023-02-17T10:16:09+00:00\",\"breadcrumb\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/#breadcrumb\"},\"inLanguage\":\"en-GB\",\"potentialAction\":[{\"@type\":\"ReadAction\",\"target\":[\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/\"]}]},{\"@type\":\"ImageObject\",\"inLanguage\":\"en-GB\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/#primaryimage\",\"url\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/wp-content\\\/uploads\\\/2022\\\/11\\\/beitragsbild_Neutronensternenkollisionen.jpg\",\"contentUrl\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/wp-content\\\/uploads\\\/2022\\\/11\\\/beitragsbild_Neutronensternenkollisionen.jpg\",\"width\":650,\"height\":450},{\"@type\":\"BreadcrumbList\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/english\\\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\\\/#breadcrumb\",\"itemListElement\":[{\"@type\":\"ListItem\",\"position\":1,\"name\":\"Startseite\",\"item\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/\"},{\"@type\":\"ListItem\",\"position\":2,\"name\":\"As dense as it gets: New Model for Matter in Neutron Star Collisions\"}]},{\"@type\":\"WebSite\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#website\",\"url\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/\",\"name\":\"Aktuelles aus der Goethe-Universit\u00e4t Frankfurt\",\"description\":\"Aktuelles aus der Goethe-Universit\u00e4t | Neues aus Forschung, Lehre, Studium\",\"publisher\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#organization\"},\"potentialAction\":[{\"@type\":\"SearchAction\",\"target\":{\"@type\":\"EntryPoint\",\"urlTemplate\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/?s={search_term_string}\"},\"query-input\":{\"@type\":\"PropertyValueSpecification\",\"valueRequired\":true,\"valueName\":\"search_term_string\"}}],\"inLanguage\":\"en-GB\"},{\"@type\":\"Organization\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#organization\",\"name\":\"Goethe-Universit\u00e4t\",\"url\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/\",\"logo\":{\"@type\":\"ImageObject\",\"inLanguage\":\"en-GB\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#\\\/schema\\\/logo\\\/image\\\/\",\"url\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/wp-content\\\/uploads\\\/2022\\\/03\\\/800px-Goethe-Logo.png\",\"contentUrl\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/wp-content\\\/uploads\\\/2022\\\/03\\\/800px-Goethe-Logo.png\",\"width\":800,\"height\":436,\"caption\":\"Goethe-Universit\u00e4t\"},\"image\":{\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#\\\/schema\\\/logo\\\/image\\\/\"}},{\"@type\":\"Person\",\"@id\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/#\\\/schema\\\/person\\\/8e55ea338fb65d1ce87a91565d1f1739\",\"name\":\"-\",\"description\":\"Dieser Beitrag wurde von der Online-Redaktion ver\u00f6ffentlicht. Wenn der Beitrag von einem Gastautoren verfasst wurde, findet sich dieser Hinweis am Ende des jeweiligen Artikels.\",\"sameAs\":[\"http:\\\/\\\/aktuelles.uni-frankfurt.de\\\/autoren\"],\"url\":\"https:\\\/\\\/aktuelles.uni-frankfurt.de\\\/en\\\/author\\\/redaktion\\\/\"}]}<\/script>\n<!-- \/ Yoast SEO plugin. -->","yoast_head_json":{"title":"As dense as it gets: New Model for Matter in Neutron Star Collisions | Aktuelles aus der Goethe-Universit\u00e4t Frankfurt","robots":{"index":"index","follow":"follow","max-snippet":"max-snippet:-1","max-image-preview":"max-image-preview:large","max-video-preview":"max-video-preview:-1"},"canonical":"https:\/\/aktuelles.uni-frankfurt.de\/en\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/","og_locale":"en_GB","og_type":"article","og_title":"As dense as it gets: New Model for Matter in Neutron Star Collisions | Aktuelles aus der Goethe-Universit\u00e4t Frankfurt","og_description":"With the exception of black holes, neutron stars are the densest objects in our universe. As their name suggests, neutron stars are mainly made of neutrons. However, our knowledge about [&hellip;]","og_url":"https:\/\/aktuelles.uni-frankfurt.de\/en\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/","og_site_name":"Aktuelles aus der Goethe-Universit\u00e4t Frankfurt","article_published_time":"2022-11-01T13:20:05+00:00","article_modified_time":"2023-02-17T10:16:09+00:00","og_image":[{"width":650,"height":450,"url":"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/beitragsbild_Neutronensternenkollisionen.jpg","type":"image\/jpeg"}],"author":"-","twitter_card":"summary_large_image","twitter_misc":{"Written by":"-","Estimated reading time":"2 minutes"},"schema":{"@context":"https:\/\/schema.org","@graph":[{"@type":"Article","@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/#article","isPartOf":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/"},"author":{"name":"-","@id":"https:\/\/aktuelles.uni-frankfurt.de\/#\/schema\/person\/8e55ea338fb65d1ce87a91565d1f1739"},"headline":"As dense as it gets: New Model for Matter in Neutron Star Collisions","datePublished":"2022-11-01T13:20:05+00:00","dateModified":"2023-02-17T10:16:09+00:00","mainEntityOfPage":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/"},"wordCount":465,"publisher":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/#organization"},"image":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/#primaryimage"},"thumbnailUrl":"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/beitragsbild_Neutronensternenkollisionen.jpg","keywords":["Physics"],"articleSection":["English","Research"],"inLanguage":"en-GB"},{"@type":"WebPage","@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/","url":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/","name":"As dense as it gets: New Model for Matter in Neutron Star Collisions | Aktuelles aus der Goethe-Universit\u00e4t Frankfurt","isPartOf":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/#website"},"primaryImageOfPage":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/#primaryimage"},"image":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/#primaryimage"},"thumbnailUrl":"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/beitragsbild_Neutronensternenkollisionen.jpg","datePublished":"2022-11-01T13:20:05+00:00","dateModified":"2023-02-17T10:16:09+00:00","breadcrumb":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/#breadcrumb"},"inLanguage":"en-GB","potentialAction":[{"@type":"ReadAction","target":["https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/"]}]},{"@type":"ImageObject","inLanguage":"en-GB","@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/#primaryimage","url":"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/beitragsbild_Neutronensternenkollisionen.jpg","contentUrl":"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/11\/beitragsbild_Neutronensternenkollisionen.jpg","width":650,"height":450},{"@type":"BreadcrumbList","@id":"https:\/\/aktuelles.uni-frankfurt.de\/english\/as-dense-as-it-gets-new-model-for-matter-in-neutron-star-collisions\/#breadcrumb","itemListElement":[{"@type":"ListItem","position":1,"name":"Startseite","item":"https:\/\/aktuelles.uni-frankfurt.de\/"},{"@type":"ListItem","position":2,"name":"As dense as it gets: New Model for Matter in Neutron Star Collisions"}]},{"@type":"WebSite","@id":"https:\/\/aktuelles.uni-frankfurt.de\/#website","url":"https:\/\/aktuelles.uni-frankfurt.de\/","name":"Aktuelles aus der Goethe-Universit\u00e4t Frankfurt","description":"Aktuelles aus der Goethe-Universit\u00e4t | Neues aus Forschung, Lehre, Studium","publisher":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/#organization"},"potentialAction":[{"@type":"SearchAction","target":{"@type":"EntryPoint","urlTemplate":"https:\/\/aktuelles.uni-frankfurt.de\/?s={search_term_string}"},"query-input":{"@type":"PropertyValueSpecification","valueRequired":true,"valueName":"search_term_string"}}],"inLanguage":"en-GB"},{"@type":"Organization","@id":"https:\/\/aktuelles.uni-frankfurt.de\/#organization","name":"Goethe University Frankfurt","url":"https:\/\/aktuelles.uni-frankfurt.de\/","logo":{"@type":"ImageObject","inLanguage":"en-GB","@id":"https:\/\/aktuelles.uni-frankfurt.de\/#\/schema\/logo\/image\/","url":"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/03\/800px-Goethe-Logo.png","contentUrl":"https:\/\/aktuelles.uni-frankfurt.de\/wp-content\/uploads\/2022\/03\/800px-Goethe-Logo.png","width":800,"height":436,"caption":"Goethe-Universit\u00e4t"},"image":{"@id":"https:\/\/aktuelles.uni-frankfurt.de\/#\/schema\/logo\/image\/"}},{"@type":"Person","@id":"https:\/\/aktuelles.uni-frankfurt.de\/#\/schema\/person\/8e55ea338fb65d1ce87a91565d1f1739","name":"-","description":"Dieser Beitrag wurde von der Online-Redaktion ver\u00f6ffentlicht. Wenn der Beitrag von einem Gastautoren verfasst wurde, findet sich dieser Hinweis am Ende des jeweiligen Artikels.","sameAs":["http:\/\/aktuelles.uni-frankfurt.de\/autoren"],"url":"https:\/\/aktuelles.uni-frankfurt.de\/en\/author\/redaktion\/"}]}},"_links":{"self":[{"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/posts\/65437","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/users\/8"}],"replies":[{"embeddable":true,"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/comments?post=65437"}],"version-history":[{"count":0,"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/posts\/65437\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/media\/65474"}],"wp:attachment":[{"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/media?parent=65437"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/categories?post=65437"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/tags?post=65437"},{"taxonomy":"post_folder","embeddable":true,"href":"https:\/\/aktuelles.uni-frankfurt.de\/en\/wp-json\/wp\/v2\/post_folder?post=65437"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}