{"id":139,"date":"2016-10-24T09:34:43","date_gmt":"2016-10-24T09:34:43","guid":{"rendered":"http:\/\/astro.uni-frankfurt.de\/sedrakian\/?page_id=139"},"modified":"2023-11-09T20:01:33","modified_gmt":"2023-11-09T20:01:33","slug":"resources","status":"publish","type":"page","link":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/resources\/","title":{"rendered":"Resources"},"content":{"rendered":"<p>Please get in touch with me via email if you are interested in a specific output of my research, e.g., tables of equations of state or transport coefficients, that are not listed below.<\/p>\n<p><span style=\"color: #000000\"><strong>Publicly available information:<\/strong><\/span><\/p>\n<ul>\n<li>Tables of equations of state of nucleonic matter with varying slope of symmetry energy and skewness: \u00a0<em> J.J. Li, A. Sedrakian, Astrophys. J. 957:41 (2023),<\/em> \u00a0<a href=\"https:\/\/github.com\/asedrakian\/DD CDFs\" data-wplink-url-error=\"true\">https:\/\/github.com\/asedrakian\/DD CDFs<\/a> or <a href=\"https:\/\/zenodo.org\/records\/8350680\">https:\/\/zenodo.org\/records\/8350680<\/a><\/li>\n<li>Tables of equations of state of hybrid stars: <em>J.J. Li, A. Sedrakian, \u00a0Astrophys. J. 957:41 (2023),<\/em> <a href=\"https:\/\/github.com\/asedrakian\/DD CDFs\" data-wplink-url-error=\"true\">https:\/\/github.com\/asedrakian\/DD CDFs<\/a><\/li>\n<li>Tables of conductivities of warm crusts on neutron stars, \u00a0outer crust: <em>A. Harutyunyan, A. Sedrakian, Phys. Rev. C 94, 025805 (2016) <\/em><a href=\"https:\/\/arxiv.org\/pdf\/1605.07612.pdf\">https:\/\/arxiv.org\/pdf\/1605.07612.pdf<\/a><\/li>\n<li>Tables of conductivities of warm crusts on neutron stars, \u00a0inner crust: <em>A. Harutyunyan, A. Sedrakian, et al. \u00a0Phys. Rev. C xx, xx (2023)<\/em> <a href=\"https:\/\/arxiv.org\/pdf\/2309.00893.pdf\">https:\/\/arxiv.org\/pdf\/1605.07612.pdf<\/a><\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>Please get in touch with me via email if you are interested in a specific output of my research, e.g., tables of equations of state or transport coefficients, that are not listed below. Publicly available information: Tables of equations of state of nucleonic matter with varying slope of symmetry energy and skewness: \u00a0 J.J. Li, <a class=\"read-more\" href=\"https:\/\/astro.uni-frankfurt.de\/sedrakian\/resources\/\">READ MORE<\/a><\/p>\n","protected":false},"author":3,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"jetpack_post_was_ever_published":false,"footnotes":""},"class_list":["post-139","page","type-page","status-publish","hentry"],"jetpack_sharing_enabled":true,"jetpack_shortlink":"https:\/\/wp.me\/P82uKz-2f","jetpack-related-posts":[],"_links":{"self":[{"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/pages\/139","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/comments?post=139"}],"version-history":[{"count":17,"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/pages\/139\/revisions"}],"predecessor-version":[{"id":627,"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/pages\/139\/revisions\/627"}],"wp:attachment":[{"href":"https:\/\/astro.uni-frankfurt.de\/sedrakian\/wp-json\/wp\/v2\/media?parent=139"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}