{"id":6646,"date":"2019-06-17T12:00:00","date_gmt":"2019-06-17T10:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/shift-symmetric-orbital-inflation-single-field-or-multi-field\/"},"modified":"2023-01-17T15:06:53","modified_gmt":"2023-01-17T14:06:53","slug":"shift-symmetric-orbital-inflation-single-field-or-multi-field","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/en\/shift-symmetric-orbital-inflation-single-field-or-multi-field\/","title":{"rendered":"Shift-symmetric orbital inflation: single field or multi-field?"},"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; 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_module_preset=&#8221;default&#8221; custom_margin=&#8221;0px||||false|false&#8221; custom_padding=&#8221;0px||||false|false&#8221; top_divider_color=&#8221;RGBA(255,255,255,0)&#8221; top_divider_height=&#8221;0px&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_row _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_image src=&#8221;https:\/\/www.ieec.cat\/wp-content\/uploads\/2022\/12\/1560845103_47ba094df879142d5f13c854904cf069_2019_06_shift_symmetric_orbital_inflation.jpg&#8221; alt=&#8221;Shift-symmetric orbital inflation: single field or multi-field?&#8221; title_text=&#8221;Shift-symmetric orbital inflation: single field or multi-field?&#8221; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; width=&#8221;600px&#8221; module_alignment=&#8221;center&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_image][et_pb_text _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;]Multi-field inflation with curved field manifold attracts a lot of attention recently. From a theoretical aspect, this class of models may be more naturally realized in the UV completion of inflation. From the observational point of view, however, the current constraints on primordial non-Gaussianity and isocurvature perturbation already\/marginally ruled out many of these models.<\/p>\n<p>In this talk, I will introduce a new class of two-field inflationary attractors, known as &lsquo;shift-symmetric orbital inflation&rsquo;. It is strongly multi-field, but the phenomenology still mimics single-field inflation with negligible amount of isocurvature modes and slow-roll suppressed non-Gaussianity, since in the end only one degree of freedom (the one with isocurvature origin) is responsible for the prediction of primordial perturbations. This new regime of multi-field attractors provides a different perspective to explore UV completion of inflation, which is free from the problems faced by single field models.[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Multi-field inflation with curved field manifold attracts a lot of attention recently. From a theoretical aspect, this class of models may be more naturally realized in the UV completion of inflation. From the observational point of view, however, the current constraints on primordial non-Gaussianity and isocurvature perturbation already\/marginally ruled out many of these models. In [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":6642,"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":[72,94],"tags":[],"class_list":["post-6646","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-events","category-talk"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.5 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Shift-symmetric orbital inflation: single field or multi-field? - 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\/shift-symmetric-orbital-inflation-single-field-or-multi-field\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Shift-symmetric orbital inflation: single field or multi-field? - IEEC\" \/>\n<meta property=\"og:description\" content=\"Multi-field inflation with curved field manifold attracts a lot of attention recently. From a theoretical aspect, this class of models may be more naturally realized in the UV completion of inflation. From the observational point of view, however, the current constraints on primordial non-Gaussianity and isocurvature perturbation already\/marginally ruled out many of these models. 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