{"id":7439,"date":"2017-10-23T00:00:00","date_gmt":"2017-10-22T22:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/iccub-seminar-the-alleged-small-scale-problems-of-lambdacdm-not-translated-2\/"},"modified":"2023-01-17T15:10:11","modified_gmt":"2023-01-17T14:10:11","slug":"iccub-seminar-the-alleged-small-scale-problems-of-lambdacdm-not-translated","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/es\/iccub-seminar-the-alleged-small-scale-problems-of-lambdacdm-not-translated\/","title":{"rendered":"ICCUB SEMINAR \u2013 The Alleged Small-Scale Problems of LambdaCDM [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\/1545149486_f951fd9d5d26313cd934d69472594f60_logoiccub.jpg\u00bb alt=\u00bbICCUB SEMINAR \u2013 The Alleged Small-Scale Problems of LambdaCDM\u00bb title_text=\u00bbICCUB SEMINAR \u2013 The Alleged Small-Scale Problems of LambdaCDM\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]The Lambda Cold Dark Matter (LCDM) framework successfully accounts for observational constraints on large (&gt; 1 Mpc) scales, from the clustering of galaxies to the angular dependence of the Cosmic Microwave Background to the structure and matter content of galaxy clusters.<\/p>\n<p>On the scale of individual galaxies and, in particular, of dwarf systems much fainter than the Milky Way, a number of apparent conflicts with LCDM expectations have been reported. These have prompted the consideration of a number of radical modifications to LCDM, such as the possibility that dark matter might be &quot;self-interacting&quot;, or that it might not be &ldquo;cold&rdquo;. I will review the status of these alleged problems and will report on recent work that reevaluates the observational evidence and reexamines the role of systematic uncertainties in the comparison between observation and model predictions.<\/p>\n<p>In particular, I will propose a possible resolution to the &ldquo;cusp vs core&rdquo; problem that requires no cores; an explanation for the mass discrepancy-acceleration relation that requires no changes to the mass profile of LCDM halos; and a plausible origin for the enigmatic population of galaxies inhabiting &ldquo;extremely cold&rdquo; dark matter halos, such as the recently discovered Crater 2 satellite.<\/p>\n<p><strong>Contact email:<\/strong> jmiralda(a)fqa.ub.edu [NOT TRANSLATED][\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The Lambda Cold Dark Matter (LCDM) framework successfully accounts for observational constraints on large (&gt; 1 Mpc) scales, from the clustering of galaxies to the angular dependence of the Cosmic Microwave Background to the structure and matter content of galaxy clusters. On the scale of individual galaxies and, in particular, of dwarf systems much fainter [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":7434,"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":[95,73],"tags":[],"class_list":["post-7439","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-charla","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 SEMINAR \u2013 The Alleged Small-Scale Problems of LambdaCDM [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-seminar-the-alleged-small-scale-problems-of-lambdacdm-not-translated\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"ICCUB SEMINAR \u2013 The Alleged Small-Scale Problems of LambdaCDM [NOT TRANSLATED] - IEEC\" \/>\n<meta property=\"og:description\" content=\"The Lambda Cold Dark Matter (LCDM) framework successfully accounts for observational constraints on large (&gt; 1 Mpc) scales, from the clustering of galaxies to the angular dependence of the Cosmic Microwave Background to the structure and matter content of galaxy clusters. 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