{"id":7133,"date":"2018-03-02T00:00:00","date_gmt":"2018-03-01T23:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/iccub-seminar-connecting-type-ia-supernovae-with-the-metallicity-of-their-progenitors-not-translated-2\/"},"modified":"2023-01-17T15:09:08","modified_gmt":"2023-01-17T14:09:08","slug":"iccub-seminar-connecting-type-ia-supernovae-with-the-metallicity-of-their-progenitors-not-translated","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/es\/iccub-seminar-connecting-type-ia-supernovae-with-the-metallicity-of-their-progenitors-not-translated\/","title":{"rendered":"ICCUB SEMINAR \u2013 Connecting Type Ia supernovae with the metallicity of their progenitors [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; 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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\/1544521736_b295d1bf12002ab81514da85224155e0_logoiccub.jpg\u00bb alt=\u00bbICCUB SEMINAR \u2013 Connecting Type Ia supernovae with the metallicity of their progenitors\u00bb title_text=\u00bbICCUB SEMINAR \u2013 Connecting Type Ia supernovae with the metallicity of their progenitors\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]Thermonuclear explosions of carbon-oxygen white dwarfs (CO WDs), or Type Ia supernovae (SNIa) are important tools for cosmology. SNIa observations show the recent acceleration and previous deceleration of the expansion rate of the Universe, in agreement with a 70% of the energy-matter content of the Universe in form of dark energy.<\/p>\n<p>To constrain the nature of the dark energy, based on SNe Ia Hubble diagrams, it is necessary to decrease the current dispersion in the SNIa calibration relation. Observational data show that galaxies with on-going star formation host brighert SNIa. Models and observations agree that brighter SNIa require more 56Ni synthesized during the explosions.<\/p>\n<p>However, Why exploding CO WDs associated with young enviroments should produce more 56Ni ? This question challenges our understanding. In this talk, I will present numerical simulations that may allow to connect the SNIa calibration relation with progenitor metallicity.<\/p>\n<p><strong>Contact email:<\/strong> jmparedes(a)ub.edu [NOT TRANSLATED][\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Thermonuclear explosions of carbon-oxygen white dwarfs (CO WDs), or Type Ia supernovae (SNIa) are important tools for cosmology. SNIa observations show the recent acceleration and previous deceleration of the expansion rate of the Universe, in agreement with a 70% of the energy-matter content of the Universe in form of dark energy. To constrain the nature [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":7128,"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-7133","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 Connecting Type Ia supernovae with the metallicity of their progenitors [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-connecting-type-ia-supernovae-with-the-metallicity-of-their-progenitors-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 Connecting Type Ia supernovae with the metallicity of their progenitors [NOT TRANSLATED] - IEEC\" \/>\n<meta property=\"og:description\" content=\"Thermonuclear explosions of carbon-oxygen white dwarfs (CO WDs), or Type Ia supernovae (SNIa) are important tools for cosmology. 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