{"id":3392,"date":"2026-05-18T02:11:30","date_gmt":"2026-05-18T09:11:30","guid":{"rendered":"https:\/\/coherencegeometry.com\/?page_id=3392"},"modified":"2026-05-18T02:24:08","modified_gmt":"2026-05-18T09:24:08","slug":"black-holes-and-horizon-structure","status":"publish","type":"page","link":"https:\/\/coherencegeometry.com\/index.php\/black-holes-and-horizon-structure\/","title":{"rendered":"Black Holes and Horizon Structure"},"content":{"rendered":"\n<h2 class=\"wp-block-heading has-text-align-center\">Black Holes and Horizon Structure<\/h2>\n\n\n\n<div style=\"height:13px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<p class=\"wp-block-paragraph\">This research area studies horizon-like behavior in Coherence Geometry, including curvature trapping, boundary emission, information flow, gravitational analogues, and radiative flux from coherence-bound regions. Rather than treating horizons only through the standard spacetime or semiclassical formulations, these papers investigate how horizon-like interfaces can arise from internal amplitude-phase dynamics, curvature strain, coherence confinement, and projection. <\/p>\n\n\n\n<div style=\"height:27px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n<style>.kb-image3392_15ef3d-96.kb-image-is-ratio-size, .kb-image3392_15ef3d-96 .kb-image-is-ratio-size{max-width:368px;width:100%;}.wp-block-kadence-column > .kt-inside-inner-col > .kb-image3392_15ef3d-96.kb-image-is-ratio-size, .wp-block-kadence-column > .kt-inside-inner-col > .kb-image3392_15ef3d-96 .kb-image-is-ratio-size{align-self:unset;}.kb-image3392_15ef3d-96 figure{max-width:368px;}.kb-image3392_15ef3d-96 .image-is-svg, .kb-image3392_15ef3d-96 .image-is-svg img{width:100%;}.kb-image3392_15ef3d-96 .kb-image-has-overlay:after{opacity:0.3;border-top-left-radius:15px;border-top-right-radius:15px;border-bottom-right-radius:15px;border-bottom-left-radius:15px;}.kb-image3392_15ef3d-96 img.kb-img, .kb-image3392_15ef3d-96 .kb-img img{border-top:2px solid var(--global-palette3, #1A202C);border-right:2px solid var(--global-palette3, #1A202C);border-bottom:2px solid var(--global-palette3, #1A202C);border-left:2px solid var(--global-palette3, #1A202C);border-top-left-radius:15px;border-top-right-radius:15px;border-bottom-right-radius:15px;border-bottom-left-radius:15px;box-shadow:20px 20px 30px 0px rgba(0, 0, 0, 0.2);}@media all and (max-width: 1024px){.kb-image3392_15ef3d-96 img.kb-img, .kb-image3392_15ef3d-96 .kb-img img{border-top:2px solid var(--global-palette3, #1A202C);border-right:2px solid var(--global-palette3, #1A202C);border-bottom:2px solid var(--global-palette3, #1A202C);border-left:2px solid var(--global-palette3, #1A202C);}}@media all and (max-width: 767px){.kb-image3392_15ef3d-96 img.kb-img, .kb-image3392_15ef3d-96 .kb-img img{border-top:2px solid var(--global-palette3, #1A202C);border-right:2px solid var(--global-palette3, #1A202C);border-bottom:2px solid var(--global-palette3, #1A202C);border-left:2px solid var(--global-palette3, #1A202C);}}<\/style>\n<div class=\"wp-block-kadence-image kb-image3392_15ef3d-96\"><figure class=\"aligncenter size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"600\" height=\"600\" src=\"https:\/\/coherencegeometry.com\/wp-content\/uploads\/2026\/05\/radiation_2_peak.png\" alt=\"\" class=\"kb-img wp-image-3443\" srcset=\"https:\/\/coherencegeometry.com\/wp-content\/uploads\/2026\/05\/radiation_2_peak.png 600w, https:\/\/coherencegeometry.com\/wp-content\/uploads\/2026\/05\/radiation_2_peak-300x300.png 300w, https:\/\/coherencegeometry.com\/wp-content\/uploads\/2026\/05\/radiation_2_peak-150x150.png 150w\" sizes=\"auto, (max-width: 600px) 100vw, 600px\" \/><\/figure><\/div>\n\n\n\n<p class=\"has-text-align-center wp-block-paragraph\"><em>Representative peak-emission frame from the horizon-like coherence simulation. A curvature-bound coherence region emits outward radial structure from its rim, producing a visible radiative shell. In the associated paper, these time-resolved fields are analyzed through rim-flux measurements that exhibit inverse-square scaling with boundary radius.<\/em><\/p>\n\n\n\n<div style=\"height:21px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<p class=\"wp-block-paragraph\">The goal is to understand which features of black-hole and horizon physics may reflect more general geometric mechanisms within structured coherence fields.<\/p>\n\n\n\n<div style=\"height:38px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<h3 class=\"wp-block-heading has-text-align-center has-theme-palette-2-color has-text-color has-link-color wp-elements-5d5bd216eb8bc662448d7b2e3be2623d\">Publication List<\/h3>\n\n\n\n<div class=\"wp-block-query is-layout-flow wp-block-query-is-layout-flow\"><ul class=\"wp-block-post-template is-layout-flow wp-block-post-template-is-layout-flow\"><li class=\"wp-block-post post-3389 post type-post status-publish format-standard hentry category-black-holes-and-horizon-structure category-cosmology category-physics category-research-papers\">\n<h5 style=\"padding-top:var(--wp--preset--spacing--60)\" class=\"wp-block-post-title\"><a href=\"https:\/\/coherencegeometry.com\/index.php\/2026\/05\/18\/horizon-like-emission-from-curvature-bound-coherence-fields\/\" target=\"_self\" >Horizon-Like Emission from Curvature-Bound Coherence Fields<\/a><\/h5>\n\n<div class=\"wp-block-post-excerpt\"><p class=\"wp-block-post-excerpt__excerpt\">CGI-RSR-000023 | We investigate horizon-like emission from curvature-regulated coherence fields within the Coherence Geometry (CG) framework. Using a multi-phase Lagrangian that incorporates curvature stiffness and phase-locking interactions, we numerically simulate the relaxation of a confined coherence region bounded by a curvature rim. <\/p><\/div>\n<\/li><\/ul>\n\n\n\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Black Holes and Horizon Structure This research area studies horizon-like behavior in Coherence Geometry, including curvature trapping, boundary emission, information flow, gravitational analogues, and radiative flux from coherence-bound regions. Rather than treating horizons only through the standard spacetime or semiclassical formulations, these papers investigate how horizon-like interfaces can arise from internal amplitude-phase dynamics, curvature strain,&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_kad_post_transparent":"","_kad_post_title":"hide","_kad_post_layout":"","_kad_post_sidebar_id":"","_kad_post_content_style":"","_kad_post_vertical_padding":"","_kad_post_feature":"","_kad_post_feature_position":"","_kad_post_header":false,"_kad_post_footer":false,"_kad_post_classname":"","footnotes":""},"class_list":["post-3392","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/pages\/3392","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/comments?post=3392"}],"version-history":[{"count":7,"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/pages\/3392\/revisions"}],"predecessor-version":[{"id":3447,"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/pages\/3392\/revisions\/3447"}],"wp:attachment":[{"href":"https:\/\/coherencegeometry.com\/index.php\/wp-json\/wp\/v2\/media?parent=3392"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}