{"id":6553,"date":"2019-07-08T12:00:00","date_gmt":"2019-07-08T10:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/pbhs-as-cdm-scenario-and-gravitational-waves\/"},"modified":"2023-01-17T15:06:29","modified_gmt":"2023-01-17T14:06:29","slug":"pbhs-as-cdm-scenario-and-gravitational-waves","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/en\/pbhs-as-cdm-scenario-and-gravitational-waves\/","title":{"rendered":"PBHs-as-CDM scenario and Gravitational Waves"},"content":{"rendered":"<p>[et_pb_section fb_built=&#8221;1&#8243; fullwidth=&#8221;on&#8221; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; background_image=&#8221;\/wp-content\/uploads\/2022\/04\/slider-corpo2.jpg&#8221; height=&#8221;114px&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_section][et_pb_section fb_built=&#8221;1&#8243; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;||0px||false|false&#8221; custom_padding=&#8221;||0px||false|false&#8221; 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_module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;]We argue that primordial black holes (PBHs) with the mass of an asteroid can be CDM of the Universe. In this scenario, the associated curvature perturbations will produce secondary gravitational waves with a unique spectral feature, and the amount produced will be large enough to be detected by the future space gravitational wave antenna, LISA.[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>We argue that primordial black holes (PBHs) with the mass of an asteroid can be CDM of the Universe. In this scenario, the associated curvature perturbations will produce secondary gravitational waves with a unique spectral feature, and the amount produced will be large enough to be detected by the future space gravitational wave antenna, LISA.<\/p>\n","protected":false},"author":0,"featured_media":6549,"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":[84,72],"tags":[],"class_list":["post-6553","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-conference","category-events"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>PBHs-as-CDM scenario and Gravitational Waves - 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\/en\/pbhs-as-cdm-scenario-and-gravitational-waves\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"PBHs-as-CDM scenario and Gravitational Waves - IEEC\" \/>\n<meta property=\"og:description\" content=\"We argue that primordial black holes (PBHs) with the mass of an asteroid can be CDM of the Universe. 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