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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\/1545152110_f25ef0e6997f6a9932878a2f8e0cc7cf_logoiccub.jpg\u00bb alt=\u00bbICCUB Seminar \u2013 The First Axionic Dark Matter Simulations for the \u201cno-WIMP Era\u201d\u00bb title_text=\u00bbICCUB Seminar \u2013 The First Axionic Dark Matter Simulations for the \u201cno-WIMP Era\u201d\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]I will describe cosmological simulations of Axion-like Dark Matter, motivated by string theory, providing a well motivated cold dark matter alternative to the standard heavy particle interpretation. Standing waves and other interference effects are predicted within Galaxies that we test with QSO lensing, pulsar timing and via dynamical effects.<\/p>\n<p>Galaxy formation is delayed in this context relative to LCDM and examined with deep space imaging of the earliest known galaxies.<\/p>\n<p><strong>Contact email:<\/strong> secretariacientifica(a)icc.ub.edu [NOT TRANSLATED][\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>I will describe cosmological simulations of Axion-like Dark Matter, motivated by string theory, providing a well motivated cold dark matter alternative to the standard heavy particle interpretation. Standing waves and other interference effects are predicted within Galaxies that we test with QSO lensing, pulsar timing and via dynamical effects. Galaxy formation is delayed in this [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":7275,"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-7280","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 First Axionic Dark Matter Simulations for the \u201cno-WIMP Era\u201d [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-first-axionic-dark-matter-simulations-for-the-no-wimp-era-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 First Axionic Dark Matter Simulations for the \u201cno-WIMP Era\u201d [NOT TRANSLATED] - IEEC\" \/>\n<meta property=\"og:description\" content=\"I will describe cosmological simulations of Axion-like Dark Matter, motivated by string theory, providing a well motivated cold dark matter alternative to the standard heavy particle interpretation. 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