{"id":1737,"date":"2026-08-13T18:16:00","date_gmt":"2026-08-13T15:16:00","guid":{"rendered":"https:\/\/bentanofficial.com.tr\/index.php\/2026\/08\/13\/cerndeki-gizemli-sinyaller-karanlik-maddenin-izi-olabilir\/"},"modified":"2026-08-13T18:16:00","modified_gmt":"2026-08-13T15:16:00","slug":"cerndeki-gizemli-sinyaller-karanlik-maddenin-izi-olabilir","status":"publish","type":"post","link":"https:\/\/bentanofficial.com.tr\/index.php\/2026\/08\/13\/cerndeki-gizemli-sinyaller-karanlik-maddenin-izi-olabilir\/","title":{"rendered":"CERN\u2019deki gizemli sinyaller karanl\u0131k maddenin izi olabilir"},"content":{"rendered":"<p>CERN\u2019deki gizemli sinyaller karanl\u0131k maddenin izi olabilir hakk\u0131ndaki son bilgiler \u015f\u00f6yle:<\/p>\n<h2>\u00d6ne \u00c7\u0131kan Noktalar<\/h2>\n<p>G\u00fcncelleme Tarihi: Temmuz 31, 2026 16:44 Ciddi Hadron \u00c7arp\u0131\u015ft\u0131r\u0131c\u0131s\u0131\u2019nda y\u0131llard\u0131r kaydedilen ve \u201cUFO\u201d olarak adland\u0131r\u0131lan s\u0131ra d\u0131\u015f\u0131 \u0131\u015f\u0131n kay\u0131plar\u0131, karanl\u0131k maddeyle ba\u011flant\u0131l\u0131 olabilir. Kanadal\u0131 fizik\u00e7ilere g\u00f6re D\u00fcnya\u2019n\u0131n i\u00e7inden ge\u00e7en yo\u011fun karanl\u0131k madde par\u00e7alar\u0131, yer alt\u0131nda son derece zay\u0131f titre\u015fimler olu\u015fturarak par\u00e7ac\u0131k h\u0131zland\u0131r\u0131c\u0131s\u0131ndaki mikroskobik tozlar\u0131 harekete ge\u00e7iriyor olabilir. Ancak ara\u015ft\u0131rmac\u0131lar, hipotezin hen\u00fcz mevcut istatistikler \u00fczerinde test edilmedi\u011fini vurguluyor.<\/p>\n<p>Avrupa N\u00fckleer Ara\u015ft\u0131rma Merkezi CERN\u2019de bulunan B\u00fcy\u00fck Hadron \u00c7arp\u0131\u015ft\u0131r\u0131c\u0131s\u0131\u2019ndan (LHC) y\u0131llard\u0131r a\u00e7\u0131klanamayan baz\u0131 sinyaller geliyor. Fizik\u00e7ilerin \u201cUFO\u201d ad\u0131n\u0131 verdi\u011fi bu olaylar\u0131n uzayl\u0131larla veya tan\u0131mlanamayan u\u00e7an cisimlerle ilgisi bulunmuyor. Buradaki k\u0131saltma, \u0130ngilizce \u201cunidentified falling objects\u201d, yani \u201ctan\u0131mlanamayan d\u00fc\u015fen nesneler\u201d ifadesinden geliyor.<\/p>\n<p>S\u00f6z konusu olaylar, proton demetinde beklenmedik \u015fekilde meydana gelen ani \u0131\u015f\u0131n kay\u0131plar\u0131 olarak kay\u0131tlara ge\u00e7iyor. Bilim insanlar\u0131 bu kesintilerin, h\u0131zland\u0131r\u0131c\u0131n\u0131n i\u00e7ine d\u00fc\u015fen mikroskobik toz par\u00e7ac\u0131klar\u0131ndan kaynakland\u0131\u011f\u0131n\u0131 d\u00fc\u015f\u00fcn\u00fcyor. \u00d6te yandan, ancak d\u00fcnyan\u0131n en hassas ve en temiz bilimsel tesislerinden biri olan LHC\u2019de bu tozlar\u0131n nas\u0131l yerinden koparak proton demetine ula\u015ft\u0131\u011f\u0131 hen\u00fcz tam olarak a\u00e7\u0131klanabilmi\u015f de\u011fil.<\/p>\n<h2>Uzman De\u011ferlendirmesi<\/h2>\n<p>KARANLIK MADDE TOZLARI HAREKETE GE\u00c7\u0130R\u0130YOR OLAB\u0130L\u0130RKanada\u2019daki British Columbia \u00dcniversitesinden fizik\u00e7iler Xunyu Liang ve Ariel Zhitnitsky, gizemli olaylar\u0131n arkas\u0131nda karanl\u0131k maddenin bulunabilece\u011fini \u00f6ne s\u00fcrd\u00fc. Ara\u015ft\u0131rmac\u0131lar\u0131n teorisine g\u00f6re D\u00fcnya\u2019n\u0131n i\u00e7inden ge\u00e7en \u00f6zel bir karanl\u0131k madde t\u00fcr\u00fc, yer alt\u0131nda son derece zay\u0131f bir akustik \u015fok dalgas\u0131 olu\u015fturabilir. Bu titre\u015fim, onlarca kilometre uzaktaki Ciddi Hadron \u00c7arp\u0131\u015ft\u0131r\u0131c\u0131s\u0131\u2019na ula\u015farak h\u0131zland\u0131r\u0131c\u0131n\u0131n i\u00e7 y\u00fczeyindeki mikroskobik tozlar\u0131 yerinden oynatabilir.<\/p>\n<p>\u00d6te yandan, serbest kalan toz par\u00e7ac\u0131klar\u0131n\u0131n proton demetine girmesi ise \u0131\u015f\u0131n\u0131n aniden kesilmesine ve UFO olarak s\u0131n\u0131fland\u0131r\u0131lan olaylar\u0131n olu\u015fmas\u0131na yol a\u00e7abilir. Liang ve Zhitnitsky, LHC\u2019yi son derece hassas bir \u0130svi\u00e7re saatine benzeterek, uzakta meydana gelen k\u00fc\u00e7\u00fck bir titre\u015fimin masaya hafif\u00e7e vurulmas\u0131 gibi tesisi etkileyebilece\u011fini ifade etti. AKS\u0130YON KUARK K\u00dcMELER\u0130 MERCEK ALTINDA\u0130ki fizik\u00e7inin \u00fczerinde \u00e7al\u0131\u015ft\u0131\u011f\u0131 varsay\u0131msal karanl\u0131k madde t\u00fcr\u00fc, \u201caksiyon kuark k\u00fcmeleri\u201d veya k\u0131saca AQN olarak adland\u0131r\u0131l\u0131yor.<\/p>\n<p>AQN\u2019lerin, bireysel temel par\u00e7ac\u0131klardan olu\u015fan geleneksel karanl\u0131k madde adaylar\u0131ndan farkl\u0131 olarak yo\u011fun ve bile\u015fik yap\u0131lar oldu\u011fu d\u00fc\u015f\u00fcn\u00fcl\u00fcyor. Buna g\u00f6re, mikroskobik boyutlarda olabilecek bu yap\u0131lar\u0131n k\u00fctlesinin yakla\u015f\u0131k bir kilograma kadar \u00e7\u0131kabilece\u011fi tahmin ediliyor. Ara\u015ft\u0131rmac\u0131lar ba\u015flang\u0131\u00e7ta LHC\u2019deki \u201ctan\u0131mlanamayan d\u00fc\u015fen nesnelerin\u201d do\u011frudan AQN olabilece\u011fini d\u00fc\u015f\u00fcnd\u00fc.<\/p>\n<h2>Konuya \u0130li\u015fkin Di\u011fer Bilgiler<\/h2>\n<p>H\u0131zland\u0131r\u0131c\u0131daki tozlar\u0131n mikron \u00f6l\u00e7e\u011finde olmas\u0131 ile \u00fczerinde \u00e7al\u0131\u015ft\u0131klar\u0131 karanl\u0131k madde yap\u0131lar\u0131n\u0131n benzer b\u00fcy\u00fckl\u00fcklerde bulunmas\u0131 dikkatlerini \u00e7ekti. Ancak yap\u0131lan incelemeler sonucunda bu boyut benzerli\u011finin yaln\u0131zca bir tesad\u00fcf oldu\u011fu sonucuna ula\u015f\u0131ld\u0131. Bu ba\u015far\u0131s\u0131z fikir, ara\u015ft\u0131rmac\u0131lar\u0131 farkl\u0131 bir soruya y\u00f6neltti: AQN\u2019ler tozun kendisi de\u011filse, tozu yerinden koparan g\u00fc\u00e7 olabilir miydi?<\/p>\n<p>100 K\u0130LOMETRE UZAKTAN ETK\u0130LEYEB\u0130L\u0130RAra\u015ft\u0131rmac\u0131lar\u0131n hesaplamalar\u0131na g\u00f6re bir AQN\u2019nin, Ciddi Hadron \u00c7arp\u0131\u015ft\u0131r\u0131c\u0131s\u0131\u2019n\u0131n yakla\u015f\u0131k 100 kilometre yak\u0131n\u0131ndan ge\u00e7mesi bile h\u0131zland\u0131r\u0131c\u0131da \u00f6l\u00e7\u00fclebilir bir etki olu\u015fturabilir. Karanl\u0131k madde yap\u0131s\u0131n\u0131n D\u00fcnya\u2019n\u0131n i\u00e7inden ge\u00e7erken meydana getirece\u011fi \u00e7ok zay\u0131f akustik \u015fok dalgas\u0131, yer alt\u0131ndaki LHC t\u00fcneline kadar ula\u015fabilir. Bu titre\u015fimin birka\u00e7 toz par\u00e7ac\u0131\u011f\u0131n\u0131 proton demetine d\u00fc\u015f\u00fcrmesi, \u0131\u015f\u0131n kayb\u0131 olay\u0131n\u0131 tetiklemek i\u00e7in yeterli olabilir.<\/p>\n<p>Edinilen bilgilere g\u00f6re, bilim insanlar\u0131, b\u00f6yle bir olaydan kaynaklanan sinyalin arka plan g\u00fcr\u00fclt\u00fcs\u00fcnden yakla\u015f\u0131k be\u015f kat daha g\u00fc\u00e7l\u00fc olaca\u011f\u0131n\u0131 hesaplad\u0131. \u0130K\u0130 SAN\u0130YE \u0130\u00c7\u0130NDE EN AZ \u00dc\u00c7 S\u0130NYALAQN kaynakl\u0131 olaylar\u0131n LHC kay\u0131tlar\u0131nda kendine \u00f6zg\u00fc bir iz b\u0131rakmas\u0131 bekleniyor. Tahmin edilen modele g\u00f6re 27 kilometre uzunlu\u011fundaki LHC t\u00fcnelinin birbirini takip eden noktalar\u0131nda, iki saniye i\u00e7inde en az \u00fc\u00e7 ba\u011flant\u0131l\u0131 UFO olay\u0131 meydana gelmesi gerekiyor.<\/p>\n<h2>Beklentiler ve \u00d6ng\u00f6r\u00fcler<\/h2>\n<p>Bu s\u0131ral\u0131 sinyal modeli, karanl\u0131k madde yap\u0131s\u0131n\u0131n olu\u015fturdu\u011fu akustik dalgan\u0131n h\u0131zland\u0131r\u0131c\u0131 boyunca ilerledi\u011fine i\u015faret edebilir. Konuya ili\u015fkin olarak, ara\u015ft\u0131rmac\u0131lara g\u00f6re ge\u00e7mi\u015f verilerde bu t\u00fcr ba\u011flant\u0131l\u0131 olaylar\u0131n bulunmas\u0131, makroskobik ve bile\u015fik bir karanl\u0131k madde aday\u0131n\u0131n varl\u0131\u011f\u0131n\u0131 destekleyen dikkat \u00e7eken bir bulgu olabilir. Ancak b\u00f6yle bir sonu\u00e7, tek ba\u015f\u0131na karanl\u0131k maddenin kesin olarak ke\u015ffedildi\u011fi anlam\u0131na gelmeyecek.<\/p>\n<p>Sinyallerin di\u011fer \u00e7evresel ve teknik nedenlerden kaynaklanmad\u0131\u011f\u0131n\u0131n da g\u00f6sterilmesi gerekecek. YEN\u0130 B\u0130R C\u0130HAZA \u0130HT\u0130YA\u00c7 YOK\u00d6nerilen y\u00f6ntemin en kritik avantajlar\u0131ndan biri, CERN\u2019de herhangi bir g\u00fcncel donan\u0131m kurulmas\u0131n\u0131 gerektirmemesi. Ciddi Hadron \u00c7arp\u0131\u015ft\u0131r\u0131c\u0131s\u0131\u2019nda, proton demetindeki kay\u0131plar\u0131 takip eden son derece hassas izleme sistemleri h\u00e2lihaz\u0131rda bulunuyor.<\/p>\n<p>Bu dedekt\u00f6rler ba\u015flang\u0131\u00e7ta h\u0131zland\u0131r\u0131c\u0131y\u0131 olas\u0131 hasarlardan korumak amac\u0131yla kurulmu\u015ftu. Liang ve Zhitnitsky\u2019ye g\u00f6re bu sistemler, tasar\u0131m ama\u00e7lar\u0131n\u0131n d\u0131\u015f\u0131nda karanl\u0131k madde kaynakl\u0131 olabilecek titre\u015fimleri de dolayl\u0131 olarak yakalayabilecek hassasiyete sahip olabilir. Ara\u015ft\u0131rmac\u0131lar, \u201cLHC\u2019nin tamamen farkl\u0131 bir ama\u00e7la kurulmu\u015f m\u00fckemmel izleme sistemlerine sahip olmas\u0131 bu fikri \u00f6zellikle cazip h\u00e2le getiriyor.<\/p>\n<h2>Geli\u015fmenin Detaylar\u0131<\/h2>\n<p>Bu cihazlar, kimsenin onlar\u0131 tasarlarken d\u00fc\u015f\u00fcnmedi\u011fi bir olaya kar\u015f\u0131 da duyarl\u0131 olabilir\u201d de\u011ferlendirmesinde bulundu. GE\u00c7M\u0130\u015e KAYITLAR YEN\u0130DEN \u0130NCELENECEK\u0130ki fizik\u00e7i, LHC\u2019nin ge\u00e7mi\u015f UFO kay\u0131tlar\u0131n\u0131 hen\u00fcz kendileri analiz etmedi. \u00c7al\u0131\u015fman\u0131n amac\u0131, CERN\u2019deki mevcut verilerin yeni hipotez do\u011frultusunda yeniden incelenmesini sa\u011flamak.<\/p>\n<p>Bilim insanlar\u0131, ge\u00e7mi\u015f \u0131\u015f\u0131n kayb\u0131 olaylar\u0131nda iki saniyelik s\u00fcre i\u00e7inde meydana gelen ba\u011flant\u0131l\u0131 sinyal k\u00fcmelerinin aranmas\u0131n\u0131 \u00f6neriyor. B\u00f6ylece olas\u0131 karanl\u0131k madde izlerinin y\u0131llard\u0131r verilerin i\u00e7inde fark edilmeden bekleyip beklemedi\u011fi anla\u015f\u0131labilir. Gelecekte ger\u00e7ekle\u015ftirilecek \u00f6zel g\u00f6zlem \u00e7al\u0131\u015fmalar\u0131n\u0131n da teoriyi s\u0131namak i\u00e7in kullan\u0131labilece\u011fi belirtiliyor.<\/p>\n<p>PAR\u00c7ACIK HIZLANDIRICILARI K\u00dcRESEL DEDEKT\u00d6RE D\u00d6N\u00dc\u015eEB\u0130L\u0130R\u00d6nerilen y\u00f6ntem yaln\u0131zca Ciddi Hadron \u00c7arp\u0131\u015ft\u0131r\u0131c\u0131s\u0131\u2019yla s\u0131n\u0131rl\u0131 olmayabilir. Yeterince \u00f6nemli \u00f6l\u00e7\u00fcde ve hassas di\u011fer par\u00e7ac\u0131k h\u0131zland\u0131r\u0131c\u0131lar\u0131n\u0131n da benzer AQN olaylar\u0131n\u0131 alg\u0131layabilece\u011fi d\u00fc\u015f\u00fcn\u00fcl\u00fcyor. D\u00fcnyan\u0131n farkl\u0131 b\u00f6lgelerindeki h\u0131zland\u0131r\u0131c\u0131lardan al\u0131nan verilerin birlikte de\u011ferlendirilmesi, gezegen \u00f6l\u00e7e\u011finde bir akustik karanl\u0131k madde g\u00f6zlem a\u011f\u0131 olu\u015fturulmas\u0131n\u0131 sa\u011flayabilir.<\/p>\n<h2>S\u00fcrecin Arka Plan\u0131<\/h2>\n<p>Karanl\u0131k madde ara\u015ft\u0131rmalar\u0131 bug\u00fcne kadar ciddi \u00f6l\u00e7\u00fcde mikroskobik temel par\u00e7ac\u0131klara odakland\u0131. Liang ve Zhitnitsky, makroskobik ve bile\u015fik karanl\u0131k madde adaylar\u0131n\u0131n ise g\u00f6rece az incelendi\u011fine dikkat \u00e7ekiyor. LHC kay\u0131tlar\u0131nda tahmin edilen ba\u011flant\u0131l\u0131 UFO olaylar\u0131n\u0131n bulunmas\u0131, karanl\u0131k madde ara\u015ft\u0131rmalar\u0131nda son bir pencere a\u00e7abilir.<\/p>\n<p>\u015eimdilik bu dikkat \u00e7ekici senaryo teorik bir \u00f6neriden ibaret olsa da yan\u0131t\u0131n, CERN\u2019in y\u0131llard\u0131r toplad\u0131\u011f\u0131 verilerin i\u00e7inde saklan\u0131yor olabilece\u011fi belirtiliyor.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>CERN\u2019deki gizemli sinyaller karanl\u0131k maddenin izi olabilir hakk\u0131ndaki son bilgiler \u015f\u00f6yle: \u00d6ne \u00c7\u0131kan Noktalar G\u00fcncelleme Tarihi: Temmuz 31, 2026 16:44 Ciddi Hadron \u00c7arp\u0131\u015ft\u0131r\u0131c\u0131s\u0131\u2019nda y\u0131llard\u0131r kaydedilen ve \u201cUFO\u201d olarak adland\u0131r\u0131lan s\u0131ra d\u0131\u015f\u0131 \u0131\u015f\u0131n kay\u0131plar\u0131, karanl\u0131k maddeyle ba\u011flant\u0131l\u0131 olabilir. Kanadal\u0131 fizik\u00e7ilere g\u00f6re D\u00fcnya\u2019n\u0131n i\u00e7inden ge\u00e7en yo\u011fun karanl\u0131k madde par\u00e7alar\u0131, yer alt\u0131nda son derece zay\u0131f titre\u015fimler olu\u015fturarak par\u00e7ac\u0131k [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":1738,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_is_manset":"","_is_son_dakika":"","_is_one_cikan":"","_is_gunun_secimleri":"","_is_cok_okunan":"","_is_sag_widget":"","_tanhaber_views":15,"footnotes":""},"categories":[9],"tags":[],"class_list":["post-1737","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-teknoloji"],"_links":{"self":[{"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/1737","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/comments?post=1737"}],"version-history":[{"count":0,"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/1737\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/media\/1738"}],"wp:attachment":[{"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/media?parent=1737"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/categories?post=1737"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/bentanofficial.com.tr\/index.php\/wp-json\/wp\/v2\/tags?post=1737"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}