{"id":8167,"date":"2018-04-24T00:00:00","date_gmt":"2018-04-23T22:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/iccub-colloquia-black-holes-thermodynamics-and-information-loss-not-translated-2\/"},"modified":"2023-01-17T15:13:17","modified_gmt":"2023-01-17T14:13:17","slug":"iccub-colloquia-black-holes-thermodynamics-and-information-loss-not-translated","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/es\/iccub-colloquia-black-holes-thermodynamics-and-information-loss-not-translated\/","title":{"rendered":"ICCUB COLLOQUIA \u2013 Black Holes, Thermodynamics, and Information Loss [NOT TRANSLATED]"},"content":{"rendered":"<p>[et_pb_section fb_built=\u00bb1&#8243; fullwidth=\u00bbon\u00bb _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb background_image=\u00bb\/wp-content\/uploads\/2022\/04\/slider-corpo2.jpg\u00bb height=\u00bb114px\u00bb global_colors_info=\u00bb{}\u00bb][\/et_pb_section][et_pb_section fb_built=\u00bb1&#8243; _builder_version=\u00bb4.14.8&#8243; 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_module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_column type=\u00bb4_4&#8243; _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_image src=\u00bbhttps:\/\/www.ieec.cat\/wp-content\/uploads\/2022\/12\/1543170316_4dc92ae80a2cbdf846eb4d65f8e5bece_image_1136.jpg\u00bb alt=\u00bbICCUB COLLOQUIA \u2013 Black Holes, Thermodynamics, and Information Loss\u00bb title_text=\u00bbICCUB COLLOQUIA \u2013 Black Holes, Thermodynamics, and Information Loss\u00bb _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb width=\u00bb600px\u00bb module_alignment=\u00bbcenter\u00bb global_colors_info=\u00bb{}\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb]A black hole is a &quot;region of no escape&quot; produced by the complete gravitational collapse of a body. During the past 45 years&#8212;and due primarily to the groundbreaking work of Stephen Hawking&#8212;a remarkable relationship has emerged between the theory of black holes in general relativity and the laws of thermodynamics.<\/p>\n<p>Most remarkably, as a result of quantum particle creation, black holes emit thermal radiation at a finite temperature.<\/p>\n<p>This thermal radiation causes a black hole to lose mass in such a way that a perfectly isolated black hole will completely &quot;evaporate&quot; in a finite time. As a result of the entanglement of quantum fields inside and outside of a black hole, when the black hole evaporates, the final quantum state should be mixed even if the initial quantum state was pure, i.e., information should be lost. This colloquium will review black hole thermodynamics and the status of the information loss issue.<\/p>\n<p><strong>Contact email<\/strong>: bfiol(a)ub.edu<\/p>\n<p><strong>Speaker CV<\/strong>: <a href=\"https:\/\/physics.uchicago.edu\/page\/robert-wald\">[Link al CV]<\/a> [NOT TRANSLATED][\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>A black hole is a &quot;region of no escape&quot; produced by the complete gravitational collapse of a body. During the past 45 years&#8212;and due primarily to the groundbreaking work of Stephen Hawking&#8212;a remarkable relationship has emerged between the theory of black holes in general relativity and the laws of thermodynamics. Most remarkably, as a result [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":8162,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"2880","footnotes":""},"categories":[85,73],"tags":[],"class_list":["post-8167","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-conferencia-es","category-eventos"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.5 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>ICCUB COLLOQUIA \u2013 Black Holes, Thermodynamics, and Information Loss [NOT TRANSLATED] - IEEC<\/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:\/\/www.ieec.cat\/es\/iccub-colloquia-black-holes-thermodynamics-and-information-loss-not-translated\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"ICCUB COLLOQUIA \u2013 Black Holes, Thermodynamics, and Information Loss [NOT TRANSLATED] - IEEC\" \/>\n<meta property=\"og:description\" content=\"A black hole is a &quot;region of no escape&quot; produced by the complete gravitational collapse of a body. 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