{"id":59,"date":"2020-01-22T12:14:36","date_gmt":"2020-01-22T10:14:36","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/icegiantform\/?page_id=59"},"modified":"2020-01-22T12:14:36","modified_gmt":"2020-01-22T10:14:36","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/icegiantform\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<p>Effect of non-adiabatic thermal profiles on the inferred compositions of Uranus and Neptune. Morris Podolak, Ravit Helled and Gerald Schubert. <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019MNRAS.487.2653P\/abstract\">https:\/\/ui.adsabs.harvard.edu\/abs\/2019MNRAS.487.2653P\/abstract<\/a><\/p>\n<p>Viscosity and Prandtl Number of Warm Dense Water as in Ice Giant\u00a0Planets. Martin French and Nadine Nettelmann. <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019ApJ...881...81F\/abstract\">https:\/\/ui.adsabs.harvard.edu\/abs\/2019ApJ&#8230;881&#8230;81F\/abstract<\/a><\/p>\n<p>How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes. M. G. Brouwers and C. W. Ormel. <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019arXiv190802742B\/abstract\">https:\/\/ui.adsabs.harvard.edu\/abs\/2019arXiv190802742B\/abstract<\/a><\/p>\n<p>Explaining the low luminosity of Uranus: a self-consistent thermal and structural evolution. Allona Vazan and Ravit Helled. <a href=\"https:\/\/ui.adsabs.harvard.ed\/abs\/2020A%26A...633A..50V\/abstract\">https:\/\/ui.adsabs.harvard.ed\/abs\/2020A%26A&#8230;633A..50V\/abstract<\/a><\/p>\n<p>Thermal evolution of Uranus and Neptune I. Adibatic Models. L. Scheibe, N. Nettelmann, R. Redmer. <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201936378\">10.1051\/0004-6361\/201936378<\/a><\/p>\n<p class=\"c-article-title\" data-test=\"article-title\">Uranus and Neptune: Origin, Evolution and Internal Structure. <span style=\"color: #000000\"><a style=\"color: #000000\" data-test=\"author-name\" data-track=\"click\" data-track-action=\"open author\" data-track-label=\"link\" data-author-popup=\"auth-Ravit-Helled\" data-corresp-id=\"c1\">Ravit Helled<\/a>, <a style=\"color: #000000\" data-test=\"author-name\" data-track=\"click\" data-track-action=\"open author\" data-track-label=\"link\" data-author-popup=\"auth-Nadine-Nettelmann\">Nadine Nettelmann<\/a>, <a style=\"color: #000000\" data-test=\"author-name\" data-track=\"click\" data-track-action=\"open author\" data-track-label=\"link\" data-author-popup=\"auth-Tristan-Guillot\">Tristan Guillot<\/a>.<\/span> <a href=\"https:\/\/doi.org\/10.1007\/s11214-020-00660-3\">10.1007\/s11214-020-00660-3<\/a><\/p>\n<p class=\"title mathjax\">Thermodynamically Governed Interior Models of Uranus and Neptune. <span style=\"color: #000000\">Elizabeth Bailey, David J. Stevenson<\/span>. <a href=\"https:\/\/arxiv.org\/abs\/2012.04166\">https:\/\/arxiv.org\/abs\/2012.04166<\/a><\/p>\n<p class=\"title\" style=\"text-align: left\">Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario. <span id=\"aa38458-20-author-1\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038458&amp;n=1\">O. M. Guilera<\/span>, <span id=\"aa38458-20-author-2\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038458&amp;n=2\" data-hasqtip=\"0\">Z. S\u00e1ndor<\/span>, <span id=\"aa38458-20-author-3\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038458&amp;n=3\">M. P. Ronco<\/span>, <span id=\"aa38458-20-author-4\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038458&amp;n=4\">J. Venturini<\/span> and <span id=\"aa38458-20-author-5\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038458&amp;n=5\">M. M. Miller Bertolami. <\/span><a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/202038458\">10.1051\/0004-6361\/202038458<\/a><\/p>\n<p class=\"title\">Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses. <span id=\"aa39140-20-author-1\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039140&amp;n=1\">Julia Venturini<\/span>, <span id=\"aa39140-20-author-2\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039140&amp;n=2\">Octavio Miguel Guilera<\/span>, <span id=\"aa39140-20-author-3\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039140&amp;n=3\">Mar\u00eda Paula Ronco<\/span>\u00a0and <span id=\"aa39140-20-author-4\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039140&amp;n=4\" data-hasqtip=\"0\" aria-describedby=\"qtip-0\">Christoph Mordasini.<a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/202039140\"> https:\/\/doi.org\/10.1051\/0004-6361\/202039140<\/a><br \/>\n<\/span><\/p>\n<p class=\"title\">The nature of the radius valley. Hints from formation and evolution models. <span id=\"aa39141-20-author-1\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039141&amp;n=1\">Julia Venturini<\/span>, <span id=\"aa39141-20-author-2\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039141&amp;n=2\" data-hasqtip=\"0\">Octavio M. Guilera<\/span>, <span id=\"aa39141-20-author-3\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039141&amp;n=3\">Jonas Haldemann<\/span>, <span id=\"aa39141-20-author-4\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039141&amp;n=4\">Mar\u00eda P. Ronco<\/span>\u00a0and <span id=\"aa39141-20-author-5\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202039141&amp;n=5\" data-hasqtip=\"1\" aria-describedby=\"qtip-1\">Christoph Mordasini. <\/span><a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/202039141\">10.1051\/0004-6361\/202039141<\/a><\/p>\n<div><\/div>\n<p data-test=\"article-title\">\n","protected":false},"excerpt":{"rendered":"<p>Effect of non-adiabatic thermal profiles on the inferred compositions of Uranus and Neptune. Morris Podolak, Ravit Helled and Gerald Schubert. https:\/\/ui.adsabs.harvard.edu\/abs\/2019MNRAS.487.2653P\/abstract Viscosity and Prandtl Number of Warm Dense Water as in Ice Giant\u00a0Planets. Martin French and Nadine Nettelmann. https:\/\/ui.adsabs.harvard.edu\/abs\/2019ApJ&#8230;881&#8230;81F\/abstract How &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/icegiantform\/publications\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-59","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/icegiantform\/wp-json\/wp\/v2\/pages\/59","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/icegiantform\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/icegiantform\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/icegiantform\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/icegiantform\/wp-json\/wp\/v2\/comments?post=59"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/icegiantform\/wp-json\/wp\/v2\/pages\/59\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/icegiantform\/wp-json\/wp\/v2\/media?parent=59"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}