Böyük partlayış: Redaktələr arasındakı fərq

Silinən məzmun Əlavə edilmiş məzmun
Redaktənin izahı yoxdur
Redaktənin izahı yoxdur
Sətir 391:
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Kainat soyuduqca, maddənin qalan kütləvi enerjisinin sıxlığı foton şüalanmasına nisbətdə üstünlük təşkil etdi. Təxminən 379.000 il sonra, elektron və nüvələr atomlara birləşdi (əsasən hidrogendə); bu səbəbdən radiasiya maddədən ayrıldı və kosmosda maneəsiz şəkildə hərəkətinə davam etdi. Bu relikt radiasiya [[Kosmik mikrodalğa arxa plan şüalanması]] kimi tanınır. Biokimya 13.8 milyard il əvvəl, Kainatın cəmi 10-17 milyon yaşının olduğu dövrlərdə Böyük Partlayışdan biraz əvvəl yaranmış ola bilər. <ref name="Loeb_2014">{{cite journal |last= Loeb |first=Abraham |author-link= |date=Oktaybr 2014 |title=The habitable epoch of the early Universe |url=https://www.cfa.harvard.edu/~loeb/habitable.pdf |url-status=live |journal=International Journal of Astrobiology |location=Cambridge, UK |publisher=[[Kembric Universiteti Nəşriyyatı|Kembric Universiteti nəşriyyatı]] |volume=13 |issue=4 |pages=337–339 |doi=10.1017/S1473550414000196 |issn=1473-5504 |archive-url=https://web.archive.org/web/20190429095059/https://www.cfa.harvard.edu/~loeb/habitable.pdf |archive-date=29 aprel 2019 |access-date=30 Novembernoyabr 2019}}</ref><ref name="NYT-20141202">{{cite news |last=Claudia |first=Dreifus |author-link= |date=1 dekabr 2014 |title=Much-Discussed Views That Go Way Back - Avi Loeb Ponders the Early Universe, Nature and Life |url=https://www.nytimes.com/2014/12/02/science/avi-loeb-ponders-the-early-universe-nature-and-life.html |url-status=live |url-access=registration |department=Science |newspaper=[[The New York Times]] |location=[[Nyu-York]] |publisher=[[Nyu-York Tayms]]|issn=0362-4331 |archive-url=https://web.archive.org/web/20150327142444/https://www.nytimes.com/2014/12/02/science/avi-loeb-ponders-the-early-universe-nature-and-life.html |archive-date=27 mart 2015 |access-date=3 Decemberdekabr 2014}} "A version of this article appears in print on Dec. 2, 2014, Section D, Page 2 of the New York edition with the headline: Much-Discussed Views That Go Way Back."</ref>
 
=== Quruluşun formalaşması ===
Sətir 1.344:
=== Baryon asimmetriyası ===
 
Kainatın niyə[[Antimaddə|antimaddədən]] daha önəmli olduğu hələ də başa düşülmür.<ref name=":6" /> Ümumiyyətlə, kainatın cavan və çox isti olduğu dövrdə, statistik tarazlıqda olduğu və bərabər miqdarda baryon və antibaryon saxladığı güman edilir. Ancaq müşahidələr, kainatın ən uzaq hissələri də daxil olmaqla tamamilə maddələrdən təşkil olunduğunu göstərir. Baryogenez adlı bir prosesin asimmetriyanı izah etdiyi güman edilir. Baryogenezin baş verməsi üçün Saxarov şərtlərinə əməl edilməlidir. Bunlar baryon sayının qorunmamasını, C-simmetriyasının və CP-simmetriyasının pozulması və kainatın [[Termodinamika|termodinamik]] tarazlıqdan ayrılmasını tələb edir. <ref name="sakharov">{{cite journal |last=Sakharov |first=Andrei D. |author-link=Andrey Saxarov |date=10 yanvar 1967 |title=Нарушение ''СР''-инвариантности, ''С''-асимметрия и барионная асимметрия Вселенной |trans-title=Violation of ''CP''-invariance, ''C''-asymmetry and baryon asymmetry of the Universe |url=http://www.jetpletters.ac.ru/ps/808/article_12459.pdf |url-status=live |journal=Journal of Experimental and Theoretical Physics |language=ru |location=Moskva |publisher=Nauka (publisher)|Nauka |volume=5 |issue=1 |page=32–35 |doi=10.1070/PU1991v034n05ABEH002497 |archive-url=https://web.archive.org/web/20180728190714/http://www.jetpletters.ac.ru/ps/808/article_12459.pdf |archive-date=28 Julyiyul 2018 |ref=harv}}
* Translated in: {{cite journal |last=Sakharov |first=Andrei D. |author-link=Andrei Sakharov |date=10 yanvar 1967 |title=Violation of CP Invariance, С Asymmetry, and Baryon Asymmetry of the Universe |url=http://www.jetpletters.ac.ru/ps/1643/article_25089.pdf |url-status=live |journal=[[Journal of Experimental and Theoretical Physics|JETP Letters]] |location=Moscow |publisher=Nauka (publisher)|Nauka |volume=5 |issue=1 |pages=24–27 |archive-url=https://web.archive.org/web/20191109163819/http://www.jetpletters.ac.ru/ps/1643/article_25089.pdf |archive-date=9 noyabr 2019 |access-date=13 dekabr 2019}}
** Reprinted in: {{harvnb|Kolb|Turner|1988|pp=371-373}}</ref> Bütün bu şərtlər Standart Modeldə baş verir, lakin cari baryon asimmetriyasını izah etmək üçün əldə edilən nəticələr kifayət qədər güclü deyil.
Sətir 1.486:
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* {{cite book |last=Penrose |first=Roger |author-link=Roger Penrose |year=2007 |orig-year=Originally published: London: Jonathan Cape, 2004 |title=The Road to Reality |title-link=The Road to Reality |edition=1st Vintage Books |location=New York |publisher=Vintage Books |isbn=978-0-679-77631-4 |lccn=2008274126 |oclc=920157277 |ref=harv}} The 2004 edition of the book is available from the [https://archive.org/details/RoadToRealityRobertPenrose Internet Archive]. Retrieved 20 Decemberdekabr 2019.
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