@prefix dbpedia-owl: .
@prefix dbpedia: .
dbpedia:John_Archibald_Wheeler dbpedia-owl:knownFor dbpedia:General_relativity .
@prefix ns2: .
dbpedia:John_Archibald_Wheeler ns2:knownFor dbpedia:General_relativity .
@prefix dbpprop: .
dbpedia:John_Archibald_Wheeler dbpprop:knownFor dbpedia:General_relativity .
dbpedia:Kip_Thorne dbpedia-owl:knownFor dbpedia:General_relativity ;
ns2:knownFor dbpedia:General_relativity ;
dbpprop:knownFor dbpedia:General_relativity .
dbpedia:Relativity dbpprop:disambiguates dbpedia:General_relativity .
@prefix rdf: .
@prefix opencyc: .
dbpedia:General_relativity rdf:type opencyc:Mx4rvVi3_JwpEbGdrcN5Y29ycA ,
opencyc:Mx4rHIBS0h_TEdaAAABQ2rksLw .
@prefix owl: .
@prefix ns7: .
dbpedia:General_relativity owl:sameAs ns7:Mx4rwJlgTZwpEbGdrcN5Y29ycA ,
opencyc:Mx4rwJlgTZwpEbGdrcN5Y29ycA ,
,
opencyc:Mx4r9H3OiKVLEdqAAAACs6hRXg .
@prefix foaf: .
@prefix ns9: .
dbpedia:General_relativity foaf:page ns9:General_relativity ;
dbpprop:reference ,
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@prefix ns10: .
dbpedia:General_relativity dbpprop:reference ns10:en .
@prefix ns11: .
dbpedia:General_relativity dbpprop:reference ns11:special-and-general-relativity .
@prefix rdfs: .
dbpedia:General_relativity rdfs:label "\u00C1ltal\u00E1nos relativit\u00E1selm\u00E9let"@hu ,
"\u041E\u0431\u0449\u0430\u044F \u0442\u0435\u043E\u0440\u0438\u044F \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438"@ru ,
"Relativit\u00E0 generale"@it ,
"Allgemeine Relativit\u00E4tstheorie"@de ,
"Den generelle relativitetsteorien"@no ,
"Relatividad general"@es ,
"Relativit\u00E9 g\u00E9n\u00E9rale"@fr ,
"Relativitat general"@ca ,
"General relativity"@en ,
"\u5EE3\u7FA9\u76F8\u5C0D\u8AD6"@zh ,
"Og\u00F3lna teoria wzgl\u0119dno\u015Bci"@pl ,
"\u0417\u0430\u0433\u0430\u043B\u044C\u043D\u0430 \u0442\u0435\u043E\u0440\u0456\u044F \u0432\u0456\u0434\u043D\u043E\u0441\u043D\u043E\u0441\u0442\u0456"@uk ,
"Obecn\u00E1 teorie relativity"@cs ,
"\u4E00\u822C\u76F8\u5BFE\u6027\u7406\u8AD6"@ja ,
"Relatividade geral"@pt ,
"Algemene relativiteitstheorie"@nl ,
"Allm\u00E4nna relativitetsteorin"@sv ,
"Genel g\u00F6relilik kuram\u0131"@tr ,
"Yleinen suhteellisuusteoria"@fi ;
dbpedia-owl:thumbnail ;
dbpprop:abstract "\u041E\u0301\u0431\u0449\u0430\u044F \u0442\u0435\u043E\u0301\u0440\u0438\u044F \u043E\u0442\u043D\u043E\u0441\u0438\u0301\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 (\u041E\u0422\u041E; \u043D\u0435\u043C. allgemeine Relativit\u00E4tstheorie) \u2014 \u0433\u0435\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u0442\u0435\u043E\u0440\u0438\u044F, \u0440\u0430\u0437\u0432\u0438\u0432\u0430\u044E\u0449\u0430\u044F \u0441\u043F\u0435\u0446\u0438\u0430\u043B\u044C\u043D\u0443\u044E \u0442\u0435\u043E\u0440\u0438\u044E \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 (\u0421\u0422\u041E), \u043E\u043F\u0443\u0431\u043B\u0438\u043A\u043E\u0432\u0430\u043D\u043D\u0430\u044F \u0410\u043B\u044C\u0431\u0435\u0440\u0442\u043E\u043C \u042D\u0439\u043D\u0448\u0442\u0435\u0439\u043D\u043E\u043C \u0432 1915\u20141916 \u0433\u043E\u0434\u0430\u0445. \u0412 \u0440\u0430\u043C\u043A\u0430\u0445 \u043E\u0431\u0449\u0435\u0439 \u0442\u0435\u043E\u0440\u0438\u0438 \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 \u043F\u043E\u0441\u0442\u0443\u043B\u0438\u0440\u0443\u0435\u0442\u0441\u044F, \u0447\u0442\u043E \u0433\u0440\u0430\u0432\u0438\u0442\u0430\u0446\u0438\u043E\u043D\u043D\u044B\u0435 \u044D\u0444\u0444\u0435\u043A\u0442\u044B \u043E\u0431\u0443\u0441\u043B\u043E\u0432\u043B\u0435\u043D\u044B \u043D\u0435 \u0441\u0438\u043B\u043E\u0432\u044B\u043C \u0432\u0437\u0430\u0438\u043C\u043E\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0435\u043C \u0442\u0435\u043B \u0438 \u043F\u043E\u043B\u0435\u0439, \u043D\u0430\u0445\u043E\u0434\u044F\u0449\u0438\u0445\u0441\u044F \u0432 \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u0435-\u0432\u0440\u0435\u043C\u0435\u043D\u0438, \u0430 \u0434\u0435\u0444\u043E\u0440\u043C\u0430\u0446\u0438\u0435\u0439 \u0441\u0430\u043C\u043E\u0433\u043E \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u0430-\u0432\u0440\u0435\u043C\u0435\u043D\u0438, \u043A\u043E\u0442\u043E\u0440\u0430\u044F \u0441\u0432\u044F\u0437\u0430\u043D\u0430, \u0432 \u0447\u0430\u0441\u0442\u043D\u043E\u0441\u0442\u0438, \u0441 \u043F\u0440\u0438\u0441\u0443\u0442\u0441\u0442\u0432\u0438\u0435\u043C \u043C\u0430\u0441\u0441\u044B-\u044D\u043D\u0435\u0440\u0433\u0438\u0438. \u0422\u0430\u043A\u0438\u043C \u043E\u0431\u0440\u0430\u0437\u043E\u043C, \u0432 \u041E\u0422\u041E, \u043A\u0430\u043A \u0438 \u0432 \u0434\u0440\u0443\u0433\u0438\u0445 \u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u0442\u0435\u043E\u0440\u0438\u044F\u0445, \u0433\u0440\u0430\u0432\u0438\u0442\u0430\u0446\u0438\u044F \u043D\u0435 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0441\u0438\u043B\u043E\u0432\u044B\u043C \u0432\u0437\u0430\u0438\u043C\u043E\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0435\u043C. \u041E\u0431\u0449\u0430\u044F \u0442\u0435\u043E\u0440\u0438\u044F \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 \u043E\u0442\u043B\u0438\u0447\u0430\u0435\u0442\u0441\u044F \u043E\u0442 \u0434\u0440\u0443\u0433\u0438\u0445 \u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u0442\u0435\u043E\u0440\u0438\u0439 \u0442\u044F\u0433\u043E\u0442\u0435\u043D\u0438\u044F \u0438\u0441\u043F\u043E\u043B\u044C\u0437\u043E\u0432\u0430\u043D\u0438\u0435\u043C \u0443\u0440\u0430\u0432\u043D\u0435\u043D\u0438\u0439 \u042D\u0439\u043D\u0448\u0442\u0435\u0439\u043D\u0430 \u0434\u043B\u044F \u0441\u0432\u044F\u0437\u0438 \u043A\u0440\u0438\u0432\u0438\u0437\u043D\u044B \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u0430-\u0432\u0440\u0435\u043C\u0435\u043D\u0438 \u0441 \u043F\u0440\u0438\u0441\u0443\u0442\u0441\u0442\u0432\u0443\u044E\u0449\u0435\u0439 \u0432 \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u0435 \u043C\u0430\u0442\u0435\u0440\u0438\u0435\u0439. \u041E\u0422\u041E \u0432 \u043D\u0430\u0441\u0442\u043E\u044F\u0449\u0435\u0435 \u0432\u0440\u0435\u043C\u044F \u2014 \u0441\u0430\u043C\u0430\u044F \u0443\u0441\u043F\u0435\u0448\u043D\u0430\u044F \u0442\u0435\u043E\u0440\u0438\u044F, \u0445\u043E\u0440\u043E\u0448\u043E \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0451\u043D\u043D\u0430\u044F \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F\u043C\u0438. \u041F\u0435\u0440\u0432\u044B\u0439 \u0443\u0441\u043F\u0435\u0445 \u043E\u0431\u0449\u0435\u0439 \u0442\u0435\u043E\u0440\u0438\u0438 \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 \u0441\u043E\u0441\u0442\u043E\u044F\u043B \u0432 \u043E\u0431\u044A\u044F\u0441\u043D\u0435\u043D\u0438\u0438 \u0430\u043D\u043E\u043C\u0430\u043B\u044C\u043D\u043E\u0439 \u043F\u0440\u0435\u0446\u0435\u0441\u0441\u0438\u0438 \u043F\u0435\u0440\u0438\u0433\u0435\u043B\u0438\u044F \u041C\u0435\u0440\u043A\u0443\u0440\u0438\u044F. \u0417\u0430\u0442\u0435\u043C, \u0432 1919 \u0433\u043E\u0434\u0443, \u0410\u0440\u0442\u0443\u0440 \u042D\u0434\u0434\u0438\u043D\u0433\u0442\u043E\u043D \u0441\u043E\u043E\u0431\u0449\u0438\u043B \u043E \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u0438 \u043E\u0442\u043A\u043B\u043E\u043D\u0435\u043D\u0438\u044F \u0441\u0432\u0435\u0442\u0430 \u0432\u0431\u043B\u0438\u0437\u0438 \u0421\u043E\u043B\u043D\u0446\u0430 \u0432 \u043C\u043E\u043C\u0435\u043D\u0442 \u043F\u043E\u043B\u043D\u043E\u0433\u043E \u0437\u0430\u0442\u043C\u0435\u043D\u0438\u044F, \u0447\u0442\u043E \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0434\u0438\u043B\u043E \u043F\u0440\u0435\u0434\u0441\u043A\u0430\u0437\u0430\u043D\u0438\u044F \u043E\u0431\u0449\u0435\u0439 \u0442\u0435\u043E\u0440\u0438\u0438 \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438. \u0421 \u0442\u0435\u0445 \u043F\u043E\u0440 \u043C\u043D\u043E\u0433\u0438\u0435 \u0434\u0440\u0443\u0433\u0438\u0435 \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u0438 \u044D\u043A\u0441\u043F\u0435\u0440\u0438\u043C\u0435\u043D\u0442\u044B \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0434\u0438\u043B\u0438 \u0437\u043D\u0430\u0447\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0435 \u043A\u043E\u043B\u0438\u0447\u0435\u0441\u0442\u0432\u043E \u043F\u0440\u0435\u0434\u0441\u043A\u0430\u0437\u0430\u043D\u0438\u0439 \u0442\u0435\u043E\u0440\u0438\u0438, \u0432\u043A\u043B\u044E\u0447\u0430\u044F \u0433\u0440\u0430\u0432\u0438\u0442\u0430\u0446\u0438\u043E\u043D\u043D\u043E\u0435 \u0437\u0430\u043C\u0435\u0434\u043B\u0435\u043D\u0438\u0435 \u0432\u0440\u0435\u043C\u0435\u043D\u0438, \u0433\u0440\u0430\u0432\u0438\u0442\u0430\u0446\u0438\u043E\u043D\u043D\u043E\u0435 \u043A\u0440\u0430\u0441\u043D\u043E\u0435 \u0441\u043C\u0435\u0449\u0435\u043D\u0438\u0435, \u0437\u0430\u0434\u0435\u0440\u0436\u043A\u0443 \u0441\u0438\u0433\u043D\u0430\u043B\u0430 \u0432 \u0433\u0440\u0430\u0432\u0438\u0442\u0430\u0446\u0438\u043E\u043D\u043D\u043E\u043C \u043F\u043E\u043B\u0435 \u0438, \u043F\u043E\u043A\u0430 \u043B\u0438\u0448\u044C \u043A\u043E\u0441\u0432\u0435\u043D\u043D\u043E, \u0433\u0440\u0430\u0432\u0438\u0442\u0430\u0446\u0438\u043E\u043D\u043D\u043E\u0435 \u0438\u0437\u043B\u0443\u0447\u0435\u043D\u0438\u0435. \u041A\u0440\u043E\u043C\u0435 \u0442\u043E\u0433\u043E, \u043C\u043D\u043E\u0433\u043E\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u044B\u0435 \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u0438\u043D\u0442\u0435\u0440\u043F\u0440\u0435\u0442\u0438\u0440\u0443\u044E\u0442\u0441\u044F \u043A\u0430\u043A \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0435\u043D\u0438\u044F \u043E\u0434\u043D\u043E\u0433\u043E \u0438\u0437 \u0441\u0430\u043C\u044B\u0445 \u0442\u0430\u0438\u043D\u0441\u0442\u0432\u0435\u043D\u043D\u044B\u0445 \u0438 \u044D\u043A\u0437\u043E\u0442\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u043F\u0440\u0435\u0434\u0441\u043A\u0430\u0437\u0430\u043D\u0438\u0439 \u043E\u0431\u0449\u0435\u0439 \u0442\u0435\u043E\u0440\u0438\u0438 \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 \u2014 \u0441\u0443\u0449\u0435\u0441\u0442\u0432\u043E\u0432\u0430\u043D\u0438\u044F \u0447\u0451\u0440\u043D\u044B\u0445 \u0434\u044B\u0440. \u041D\u0435\u0441\u043C\u043E\u0442\u0440\u044F \u043D\u0430 \u043E\u0448\u0435\u043B\u043E\u043C\u043B\u044F\u044E\u0449\u0438\u0439 \u0443\u0441\u043F\u0435\u0445 \u043E\u0431\u0449\u0435\u0439 \u0442\u0435\u043E\u0440\u0438\u0438 \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438, \u0432 \u043D\u0430\u0443\u0447\u043D\u043E\u043C \u0441\u043E\u043E\u0431\u0449\u0435\u0441\u0442\u0432\u0435 \u0441\u0443\u0449\u0435\u0441\u0442\u0432\u0443\u0435\u0442 \u0434\u0438\u0441\u043A\u043E\u043C\u0444\u043E\u0440\u0442, \u0441\u0432\u044F\u0437\u0430\u043D\u043D\u044B\u0439 \u0441 \u0442\u0435\u043C, \u0447\u0442\u043E \u0435\u0451 \u043D\u0435 \u0443\u0434\u0430\u0451\u0442\u0441\u044F \u043F\u0435\u0440\u0435\u0444\u043E\u0440\u043C\u0443\u043B\u0438\u0440\u043E\u0432\u0430\u0442\u044C \u043A\u0430\u043A \u043A\u043B\u0430\u0441\u0441\u0438\u0447\u0435\u0441\u043A\u0438\u0439 \u043F\u0440\u0435\u0434\u0435\u043B \u043A\u0432\u0430\u043D\u0442\u043E\u0432\u043E\u0439 \u0442\u0435\u043E\u0440\u0438\u0438 \u0438\u0437-\u0437\u0430 \u043F\u043E\u044F\u0432\u043B\u0435\u043D\u0438\u044F \u043D\u0435\u0443\u0441\u0442\u0440\u0430\u043D\u0438\u043C\u044B\u0445 \u043C\u0430\u0442\u0435\u043C\u0430\u0442\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u0440\u0430\u0441\u0445\u043E\u0434\u0438\u043C\u043E\u0441\u0442\u0435\u0439 \u043F\u0440\u0438 \u0440\u0430\u0441\u0441\u043C\u043E\u0442\u0440\u0435\u043D\u0438\u0438 \u0447\u0451\u0440\u043D\u044B\u0445 \u0434\u044B\u0440 \u0438 \u0432\u043E\u043E\u0431\u0449\u0435 \u0441\u0438\u043D\u0433\u0443\u043B\u044F\u0440\u043D\u043E\u0441\u0442\u0435\u0439 \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u0430-\u0432\u0440\u0435\u043C\u0435\u043D\u0438. \u0414\u043B\u044F \u0440\u0435\u0448\u0435\u043D\u0438\u044F \u044D\u0442\u043E\u0439 \u043F\u0440\u043E\u0431\u043B\u0435\u043C\u044B \u0431\u044B\u043B \u043F\u0440\u0435\u0434\u043B\u043E\u0436\u0435\u043D \u0440\u044F\u0434 \u0430\u043B\u044C\u0442\u0435\u0440\u043D\u0430\u0442\u0438\u0432\u043D\u044B\u0445 \u0442\u0435\u043E\u0440\u0438\u0439. \u0421\u043E\u0432\u0440\u0435\u043C\u0435\u043D\u043D\u044B\u0435 \u044D\u043A\u0441\u043F\u0435\u0440\u0438\u043C\u0435\u043D\u0442\u0430\u043B\u044C\u043D\u044B\u0435 \u0434\u0430\u043D\u043D\u044B\u0435 \u0443\u043A\u0430\u0437\u044B\u0432\u0430\u044E\u0442, \u0447\u0442\u043E \u043B\u044E\u0431\u043E\u0433\u043E \u0442\u0438\u043F\u0430 \u043E\u0442\u043A\u043B\u043E\u043D\u0435\u043D\u0438\u044F \u043E\u0442 \u041E\u0422\u041E \u0434\u043E\u043B\u0436\u043D\u044B \u0431\u044B\u0442\u044C \u043E\u0447\u0435\u043D\u044C \u043C\u0430\u043B\u044B\u043C\u0438, \u0435\u0441\u043B\u0438 \u043E\u043D\u0438 \u0432\u043E\u043E\u0431\u0449\u0435 \u0441\u0443\u0449\u0435\u0441\u0442\u0432\u0443\u044E\u0442."@ru ,
"Az \u00E1ltal\u00E1nos relativit\u00E1selm\u00E9let a gravit\u00E1ci\u00F3 Albert Einstein \u00E1ltal 1916-ban k\u00F6zz\u00E9tett elm\u00E9lete. Az \u00E1ltal\u00E1nos relativit\u00E1selm\u00E9let magja az az \u00E1ll\u00EDt\u00E1s, melyb\u0151l a t\u00F6bbi k\u00F6vetkezik, az ekvivalenciaelv, mely a gravit\u00E1ci\u00F3t \u00E9s a gyorsul\u00E1st ugyanannak a dolognak k\u00E9t l\u00E1t\u00E1sm\u00F3djak\u00E9nt \u00EDrja le. A fenti elvet m\u00E1r 1907-ben megfogalmazta Einstein a k\u00F6vetkez\u0151k\u00E9ppen: Ez\u00E9rt felt\u00E9telezz\u00FCk a gravit\u00E1ci\u00F3s t\u00E9r \u00E9s a vonatkoztat\u00E1si rendszer megfelel\u0151 gyorsul\u00E1s\u00E1nak egyen\u00E9rt\u00E9k\u0171s\u00E9g\u00E9t. Ez a feltev\u00E9s \u00E1ltal\u00E1nos\u00EDtja a relativit\u00E1s elv\u00E9t arra az esetre, amikor a vonatkoztat\u00E1si rendszer egyenletesen gyorsul. M\u00E1ssz\u00F3val arra alapozta az elm\u00E9let\u00E9t, hogy egyetlen k\u00EDs\u00E9rlet sem tud k\u00FCl\u00F6nbs\u00E9get tenni lok\u00E1lisan a homog\u00E9n gravit\u00E1ci\u00F3s t\u00E9r \u00E9s az egyenletes gyorsul\u00E1s k\u00F6z\u00F6tt. Az ekvivalenciaelv jelent\u00E9se fokozatosan b\u0151v\u00FClt Einstein tov\u00E1bbi \u00EDr\u00E1saiban, k\u00E9s\u0151bb mag\u00E1ban foglalta azt az elk\u00E9pzel\u00E9st, hogy semmilyen fizikai m\u00E9r\u00E9s nem k\u00E9pes arra, hogy egy nem gyorsul\u00F3 vonatkoztat\u00E1si rendszer mozg\u00E1s\u00E1llapot\u00E1t meg\u00E1llap\u00EDtsa. Ennek az a k\u00F6vetkezm\u00E9nye, hogy lehetetlen megm\u00E9rni, teh\u00E1t gyakorlatilag sz\u00FCks\u00E9gtelen t\u00E1rgyalni, az alapvet\u0151 fizikai \u00E1lland\u00F3k, mint az elemi r\u00E9szecsk\u00E9k nyugalmi t\u00F6meg\u00E9nek vagy elektromos t\u00F6lt\u00E9s\u00E9nek v\u00E1ltoz\u00E1sait k\u00FCl\u00F6nb\u00F6z\u0151 relat\u00EDv mozg\u00E1sok eset\u00E9n. Minden m\u00E9rt v\u00E1ltoz\u00E1s ezekben az \u00E1lland\u00F3kban vagy k\u00EDs\u00E9rleti hiba, vagy a relativit\u00E1si elv hib\u00E1s vagy hi\u00E1nyos volt\u00E1nak kimutat\u00E1sa."@hu ,
"Em F\u00EDsica, a relatividade geral \u00E9 a generaliza\u00E7\u00E3o da Teoria da gravita\u00E7\u00E3o de Newton, publicada em 1915 por Albert Einstein e cuja base matem\u00E1tica foi desenvolvida pelo cientista franc\u00EAs Henri Poincar\u00E9. A nova teoria leva em considera\u00E7\u00E3o as ideias descobertas na Relatividade restrita sobre o espa\u00E7o e o tempo e prop\u00F5e a generaliza\u00E7\u00E3o do princ\u00EDpio da relatividade do movimento de referenciais em movimento uniforme para a relatividade do movimento mesmo entre referenciais em movimento acelerado. Esta generaliza\u00E7\u00E3o tem implica\u00E7\u00F5es profundas no nosso conhecimento do espa\u00E7o-tempo, levando, entre outras conclus\u00F5es, \u00E0 de que a mat\u00E9ria (energia) curva o espa\u00E7o e o tempo \u00E0 sua volta. Isto \u00E9, a gravita\u00E7\u00E3o \u00E9 um efeito da geometria do espa\u00E7o-tempo."@pt ,
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"Die allgemeine Relativit\u00E4tstheorie beschreibt die Wechselwirkung zwischen Materie einerseits und Raum und Zeit andererseits. Sie deutet Gravitation als geometrische Eigenschaft der gekr\u00FCmmten vierdimensionalen Raumzeit. Die Grundlagen der Theorie wurden ma\u00DFgeblich von Albert Einstein entwickelt, der den Kern der Theorie am 25. November 1915 der Preu\u00DFischen Akademie der Wissenschaften vortrug. Zur Beschreibung der gekr\u00FCmmten Raumzeit bediente er sich der Differentialgeometrie. Die allgemeine Relativit\u00E4tstheorie erweitert die spezielle Relativit\u00E4tstheorie und geht f\u00FCr hinreichend kleine Gebiete der Raumzeit in diese \u00FCber. Gleichzeitig ist sie eine Erweiterung des newtonschen Gravitationsgesetzes und enth\u00E4lt dieses als Grenzfall f\u00FCr hinreichend kleine Massendichten und Geschwindigkeiten. Inzwischen wurde die allgemeine Relativit\u00E4tstheorie ausreichend oft experimentell best\u00E4tigt, so dass sie als Gravitationstheorie allgemein anerkannt ist. Insbesondere hat sie sich bisher in der von Einstein formulierten Form gegen alle sp\u00E4ter vorgeschlagenen Alternativen durchsetzen k\u00F6nnen. Dieser Artikel baut auf den Ausf\u00FChrungen des Artikels Relativit\u00E4tstheorie auf und soll die dortigen Ausf\u00FChrungen vertiefen."@de ,
"La relativit\u00E9 g\u00E9n\u00E9rale est une th\u00E9orie relativiste de la gravitation, c'est-\u00E0-dire qu'elle d\u00E9crit l'influence sur le mouvement des astres de la pr\u00E9sence de mati\u00E8re et, plus g\u00E9n\u00E9ralement d'\u00E9nergie, en tenant compte des principes de la relativit\u00E9 restreinte. La relativit\u00E9 g\u00E9n\u00E9rale englobe et supplante la th\u00E9orie de la gravitation universelle d'Isaac Newton qui en repr\u00E9sente la limite aux petites vitesses (compar\u00E9es \u00E0 la vitesse de la lumi\u00E8re) et aux champs gravitationnels faibles. La relativit\u00E9 g\u00E9n\u00E9rale est principalement l'\u0153uvre d'Albert Einstein, dont elle est consid\u00E9r\u00E9e comme la r\u00E9alisation majeure, qu'il a \u00E9labor\u00E9e entre 1907 et 1915. Les noms de Marcel Grossmann et de David Hilbert lui sont \u00E9galement associ\u00E9s, le premier ayant aid\u00E9 Einstein \u00E0 se familiariser avec les outils math\u00E9matiques n\u00E9cessaires \u00E0 la compr\u00E9hension de la th\u00E9orie, le second ayant franchi conjointement avec Einstein les derni\u00E8res \u00E9tapes menant \u00E0 la finalisation de la th\u00E9orie apr\u00E8s que ce dernier lui eut pr\u00E9sent\u00E9 dans le courant de l'ann\u00E9e 1915 les id\u00E9es g\u00E9n\u00E9rales de sa th\u00E9orie. La relativit\u00E9 g\u00E9n\u00E9rale est bas\u00E9e sur des concepts radicalement diff\u00E9rents de ceux de la gravitation newtonienne. Elle \u00E9nonce notamment que la gravitation n'est pas une force, mais est la manifestation de la courbure de l'espace (en fait de l'espace-temps), courbure elle-m\u00EAme produite par la distribution de mati\u00E8re. Cette th\u00E9orie relativiste de la gravitation donne lieu \u00E0 des effets absents de la th\u00E9orie newtonienne mais v\u00E9rifi\u00E9s, comme l'expansion de l'univers, ou potentiellement v\u00E9rifiables, comme les ondes gravitationnelles et les trous noirs. Aucun des nombreux tests exp\u00E9rimentaux effectu\u00E9s \u00E0 ce jour (2009) n'a pu la mettre en d\u00E9faut, \u00E0 l'exception possible de l'anomalie Pioneer qui pourrait \u00EAtre la premi\u00E8re indication d'un \u00E9cart entre les ph\u00E9nom\u00E8nes observ\u00E9s et la relativit\u00E9 g\u00E9n\u00E9rale, quoique d'autres interpr\u00E9tations de ce ph\u00E9nom\u00E8ne soient envisageables."@fr ,
"La Relativit\u00E0 generale \u00E8 una teoria fisica pubblicata da Albert Einstein nel 1915. Come disse lo stesso Einstein, fu il lavoro pi\u00F9 difficile della sua carriera di teorico a causa delle difficolt\u00E0 matematiche da superare, poich\u00E9 si trattava di far convergere concetti di geometria euclidea in uno spazio che poteva non esserlo. Le basi matematiche erano state esplorate in precedenza dal lavoro di Lobacevskij, Bolyai e Gauss, che avevano dimostrato la non necessariet\u00E0 del quinto postulato di Euclide (enunciabile nella forma di Playfair con l'affermazione due rette parallele restano sempre equidistanti); inoltre il formalismo per uno spazio non-euclideo era stato sviluppato da Riemann, studente di Gauss. Tale formalismo era stato messo da parte come non applicabile alla realt\u00E0, fino all'introduzione appunto della relativit\u00E0 generale."@it ,
"Og\u00F3lna teoria wzgl\u0119dno\u015Bci (OTW) \u2013 popularna nazwa teorii grawitacji sformu\u0142owanej przez Alberta Einsteina w 1915 roku, a opublikowanej w roku 1916. Zgodnie z og\u00F3ln\u0105 teori\u0105 wzgl\u0119dno\u015Bci, si\u0142a grawitacji wynika z lokalnej geometrii czasoprzestrzeni. Aparat matematyczny tej teorii zosta\u0142 opracowany w pracach takich matematyk\u00F3w jak J\u00E1nos Bolyai, a tak\u017Ce Carl Gauss. Og\u00F3lnie geometria nieeuklidesowa zosta\u0142a rozwini\u0119ta przez ucznia Gaussa, Georga Bernharda Riemanna, ale nieeuklidesowa geometria czasoprzestrzeni sta\u0142a si\u0119 znana szerzej dopiero po tym, jak w opracowan\u0105 przez Einsteina szczeg\u00F3ln\u0105 teori\u0119 wzgl\u0119dno\u015Bci Hermann Minkowski wprowadzi\u0142 Czasoprzestrze\u0144 Minkowskiego. Teoria Einsteina zawiera nietrywialne tre\u015Bci fizyczne dotycz\u0105ce koncepcji czasu, przestrzeni, geometrii czasoprzestrzeni, zwi\u0105zk\u00F3w masy bezw\u0142adnej i wa\u017Ckiej oraz spostrze\u017Cenia dotycz\u0105ce r\u00F3wnowa\u017Cno\u015Bci grawitacji i si\u0142 bezw\u0142adno\u015Bci. Jest ona uog\u00F3lnieniem Szczeg\u00F3lnej Teorii Wzgl\u0119dno\u015Bci obowi\u0105zuj\u0105cej dla inercjalnych uk\u0142ad\u00F3w odniesienia na dowolne, tak\u017Ce nieinercjalne uk\u0142ady odniesienia. W warstwie matematycznej korzysta ona obficie z metod rachunku tensorowego, geometrii nieeuklidesowej, teorii przestrzeni Riemanna itp."@pl ,
"La Teor\u00EDa general de la relatividad o relatividad general es una teor\u00EDa del campo gravitatorio y de los sistemas de referencia generales, publicada por Albert Einstein en 1915 y 1916. El nombre de la teor\u00EDa se debe a que generaliza la llamada teor\u00EDa especial de la relatividad. Los principios fundamentales introducidos en esta generalizaci\u00F3n son el Principio de equivalencia, que describe la aceleraci\u00F3n y la gravedad como aspectos distintos de la misma realidad, la noci\u00F3n de la curvatura del espacio-tiempo y el principio de covariancia generalizado. La intuici\u00F3n b\u00E1sica de Einstein fue postular que en un punto concreto no se puede distinguir experimentalmente entre un cuerpo acelerado uniformemente y un campo gravitatorio uniforme. La teor\u00EDa general de la relatividad permiti\u00F3 tambi\u00E9n reformular el campo de la cosmolog\u00EDa."@es ,
"\u4E00\u822C\u76F8\u5BFE\u6027\u7406\u8AD6\uFF08\u3044\u3063\u3071\u3093\u305D\u3046\u305F\u3044\u305B\u3044\u308A\u308D\u3093\u3001\u72EC\u8A9E\uFF1AAllgemeine Relativit\u00E4tstheorie\u3001\u82F1\u8A9E\uFF1Ageneral theory of relativity\uFF09\u306F\u3001\u4E00\u822C\u76F8\u5BFE\u8AD6\uFF08General relativity\uFF09\u3068\u3082\u3044\u3044\u3001\u30A2\u30EB\u30D9\u30EB\u30C8\u30FB\u30A2\u30A4\u30F3\u30B7\u30E5\u30BF\u30A4\u30F3\u304C\u30011905\u5E74\u306E\u7279\u6B8A\u76F8\u5BFE\u6027\u7406\u8AD6\u306B\u7D9A\u3044\u30661915\u5E74 - 1916\u5E74\u306B\u767A\u8868\u3057\u305F\u7269\u7406\u5B66\u306E\u7406\u8AD6\u3002\u30CB\u30E5\u30FC\u30C8\u30F3\u529B\u5B66\u3068\u6BD4\u8F03\u3059\u308B\u3068\u3001\u904B\u52D5\u306E\u901F\u5EA6\u304C\u901F\u3044\u5834\u5408\u3084\u3001\u91CD\u529B\u304C\u5927\u304D\u3044\u5834\u5408\u306E\u73FE\u8C61\u3092\u6B63\u3057\u304F\u8A18\u8FF0\u3067\u304D\u308B\u3002"@ja ,
"La relativitat general \u00E9s una teoria relativista de la gravitaci\u00F3. En aquest escenari, la pres\u00E8ncia d'una massa deforma localment l'espai-temps. El f\u00EDsic Thibault Damour utilitza al respecte l'expressi\u00F3 d'espai-temps el\u00E0stic. Aquesta teoria \u00E9s considerada com la principal obra d'Albert Einstein, at\u00E8s que la seva construcci\u00F3 el va ocupar des de 1907 fins el 1915 que la va finalitzar. Fins ara, cap dels assaigs experimentals efectuats no ha pogut trobar-ne cap defecte."@ca ,
"\u0417\u0430\u0433\u0430\u043B\u044C\u043D\u0430 \u0442\u0435\u043E\u0440\u0456\u044F \u0432\u0456\u0434\u043D\u043E\u0441\u043D\u043E\u0441\u0442\u0456 (\u0417\u0422\u0412) \u2014 \u0442\u0435\u043E\u0440\u0456\u044F \u0433\u0440\u0430\u0432\u0456\u0442\u0430\u0446\u0456\u0457, \u043E\u043F\u0443\u0431\u043B\u0456\u043A\u043E\u0432\u0430\u043D\u0430 \u0410\u043B\u044C\u0431\u0435\u0440\u0442\u043E\u043C \u0415\u0439\u043D\u0448\u0442\u0435\u0439\u043D\u043E\u043C \u0432 1915 \u0440\u043E\u0446\u0456. \u041D\u0430 \u0432\u0456\u0434\u043C\u0456\u043D\u0443 \u0432\u0456\u0434 \u043D\u0435\u0440\u0435\u043B\u044F\u0442\u0438\u0432\u0456\u0441\u0442\u0441\u044C\u043A\u043E\u0457 \u0442\u0435\u043E\u0440\u0456\u0457 \u0433\u0440\u0430\u0432\u0456\u0442\u0430\u0446\u0456\u0457 \u041D\u044C\u044E\u0442\u043E\u043D\u0430 \u0417\u0422\u0412 \u043F\u0440\u0438\u0434\u0430\u0442\u043D\u0430 \u0434\u043B\u044F \u043E\u043F\u0438\u0441\u0443 \u0433\u0440\u0430\u0432\u0456\u0442\u0430\u0446\u0456\u0439\u043D\u043E\u0457 \u0432\u0437\u0430\u0454\u043C\u043E\u0434\u0456\u0457 \u0442\u0456\u043B, \u0449\u043E \u0440\u0443\u0445\u0430\u044E\u0442\u044C\u0441\u044F \u0437\u0456 \u0448\u0432\u0438\u0434\u043A\u043E\u0441\u0442\u044F\u043C\u0438 \u0431\u043B\u0438\u0437\u044C\u043A\u0438\u043C\u0438 \u0434\u043E \u0448\u0432\u0438\u0434\u043A\u043E\u0441\u0442\u0456 \u0441\u0432\u0456\u0442\u043B\u0430. \u0407\u0457 \u0442\u0430\u043A\u043E\u0436 \u043C\u043E\u0436\u043D\u0430 \u0437\u0430\u0441\u0442\u043E\u0441\u043E\u0432\u0443\u0432\u0430\u0442\u0438 \u0443 \u0432\u0438\u043F\u0430\u0434\u043A\u0443 \u0441\u0438\u043B\u044C\u043D\u0438\u0445 \u0433\u0440\u0430\u0432\u0456\u0442\u0430\u0446\u0456\u0439\u043D\u0438\u0445 \u043F\u043E\u043B\u0456\u0432, \u0449\u043E \u0432\u0438\u043D\u0438\u043A\u0430\u044E\u0442\u044C, \u043D\u0430\u043F\u0440\u0438\u043A\u043B\u0430\u0434, \u043F\u043E\u0431\u043B\u0438\u0437\u0443 \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u0438\u0445 \u0437\u0456\u0440\u043E\u043A \u0442\u0430 \u0447\u043E\u0440\u043D\u0438\u0445 \u0434\u0456\u0440. \u0423 \u0441\u043E\u043D\u044F\u0447\u043D\u0456\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u0456 \u0435\u0444\u0435\u043A\u0442\u0438 \u0417\u0422\u0412 \u043F\u0440\u043E\u044F\u0432\u043B\u044F\u044E\u0442\u044C \u0441\u0435\u0431\u0435 \u043D\u0435\u0437\u043D\u0430\u0447\u043D\u0438\u043C\u0438 \u0432\u0456\u0434\u0445\u0438\u043B\u0435\u043D\u043D\u044F\u043C\u0438 \u0444\u0430\u043A\u0442\u0438\u0447\u043D\u0438\u0445 \u0442\u0440\u0430\u0454\u043A\u0442\u043E\u0440\u0456\u0439 \u0440\u0443\u0445\u0443 \u043F\u043B\u0430\u043D\u0435\u0442 \u0442\u0430 \u0456\u043D\u0448\u0438\u0445 \u043A\u043E\u0441\u043C\u0456\u0447\u043D\u0438\u0445 \u0442\u0456\u043B (\u0443 \u043F\u0435\u0440\u0448\u0443 \u0447\u0435\u0440\u0433\u0443 \u041C\u0435\u0440\u043A\u0443\u0440\u0456\u044F) \u0432\u0456\u0434 \u043E\u0440\u0431\u0456\u0442, \u0440\u043E\u0437\u0440\u0430\u0445\u043E\u0432\u0430\u043D\u0438\u0445 \u0443 \u0440\u0430\u043C\u043A\u0430\u0445 \u0442\u0435\u043E\u0440\u0456\u0457 \u041D\u044C\u044E\u0442\u043E\u043D\u0430."@uk ,
"Yleinen suhteellisuusteoria (engl. General relativity, GR) on painovoimaa kuvaava teoria, jonka kehitti saksalainen teoreettinen fyysikko Albert Einstein vuosina 1907–1915. Teorian mukaan kahden kappaleen v\u00E4lill\u00E4 havaittu painovoima johtuu siit\u00E4, ett\u00E4 kappaleiden massat kaareuttavat aika-avaruutta. Yleisess\u00E4 suhteellisuusteoriassa gravitaatio siis tulkitaan avaruuden kaareutumiseksi, toisin sanoen avaruuden geometrian muuttumiseksi. Einsteinin teoria k\u00E4ytt\u00E4\u00E4 geometrianaan Riemannin ep\u00E4euklidista geometriaa. Teoria korvaa Sir Isaac Newtonin vuonna 1686 julkaiseman teorian painovoimasta voimana massallisten kappaleiden v\u00E4lill\u00E4. Kokeiden mukaan Einsteinin teoria on tarkempi ja on n\u00E4in syrj\u00E4ytt\u00E4nyt Newtonin teorian modernissa fysiikassa. Yleinen suhteellisuusteoria ennustaa my\u00F6s gravitaatioaaltojen olemassaolon. Yleinen suhteellisuusteoria korjaa ja ennustaa joitakin todennettavia ilmi\u00F6it\u00E4, joita Newtonin teoria ei kykene selitt\u00E4m\u00E4\u00E4n tai ennustamaan. T\u00E4llaisia ovat esimerkiksi valons\u00E4teiden taipuminen massiivisen kappaleen ymp\u00E4rill\u00E4 ja Merkuriuksen tai muiden planeettojen perihelin kiertyminen. Lis\u00E4ksi yleisen suhteellisuusteorian mukaan aika hidastuu voimakkaassa gravitaatiokent\u00E4ss\u00E4. Yleinen suhteellisuusteoria ei ole ainoa relativistinen painovoimateoria, mutta se on malliltaan kaikkein yksinkertaisin niist\u00E4, jotka ovat kokeellisesti saadun tiedon kanssa sopusoinnussa. Vaikka teoria kykenee selitt\u00E4m\u00E4\u00E4n ja ennustamaan lukuisia ilmi\u00F6it\u00E4, se j\u00E4tt\u00E4\u00E4 joitakin kysymyksi\u00E4 avoimiksi. Kaikkein perustavinta laatua oleva kysymys on se, kuinka yleinen suhteellisuusteoria saadaan sovitetuksi yhteen kvanttifysiikan lakien kanssa, jolloin lopputuloksena saadaan kvanttigravitaatioteoria. Teoriasta on kehittynyt modernin t\u00E4htitieteen yksi t\u00E4rkeimmist\u00E4 teorioista. Yleinen suhteellisuusteoria tarjoaa nykyisen ymm\u00E4rryksen mustien aukkojen suhteen. Yleinen suhteellisuusteoria on my\u00F6s perusta alkur\u00E4j\u00E4hdysteorialle."@fi ,
"Den generelle relativitetsteorien, ofte kalt bare generell relativitet (GR), er den geometriske teorien om gravitasjon som Albert Einstein publiserte i 1916. Den kombinerer spesiell relativitet og Newtons gravitasjonslov med den innsikt at gravitasjon ikke er en f\u00F8lge av noen kraft (i tradisjonell betydning av ordet), men er en manifestasjon av at tidrommet krummer seg. Denne krumningen kommer av mengden masse-energi i tidrommet. Einsteins feltligning viser hvordan rommet krummer seg i p\u00E5 grunn av masse-energien. <math>R_{\\alpha\\beta} - {1 \\over 2} g_{\\alpha\\beta} R = {8 \\pi G \\over c^4} T_{\\alpha\\beta}</math> som tilsvarer en ikke-line\u00E6r differensialligning for hver komponent av den metriske tensoren <math>\\; g_{\\alpha\\beta}(x)</math>. H\u00F8yreleddet i denne ligningen spesifiserer masse-energifordelingen i romtiden og relaterer dette til venstreleddet som gir et m\u00E5l p\u00E5 krumningen. I ligningen over er <math>\\; R_{\\alpha\\beta}</math> Riccis krumningstensor, <math>\\; R</math> skalarkrumningen, <math>\\; g_{\\alpha\\beta}</math> den metriske tensoren, <math>\\; T_{\\alpha\\beta}</math> stressenergitensoren, <math>\\; c</math> lysfarten og <math>\\; G</math> gravitasjonskonstanten"@no ,
"Genel g\u00F6relilik kuram\u0131, ivmeli devinim ile k\u00FCtle\u00E7ekimi a\u00E7\u0131klamas\u0131n\u0131 \u00F6zel g\u00F6relili\u011Fe birle\u015Ftiren, genelleyen kuramd\u0131r. 1916'da Einstein taraf\u0131ndan ortaya konmu\u015Ftur. Genel g\u00F6relilikten \u00F6nce, Newton'un k\u00FCtle\u00E7ekim kuram\u0131 ge\u00E7erli kabul ediliyordu. Newton'un form\u00FClleri (yatay at\u0131\u015F, dikey at\u0131\u015F vb) bugun de duyarl\u0131l\u0131k gerektirmeyen uygulamalarda ge\u00E7erlidir. Ancak aya roket g\u00F6ndermek gibi duyarl\u0131 i\u015Flerde Einstein form\u00FClleri kullan\u0131lmaktad\u0131r. Genel olarak Newton mekani\u011Finde Kuvvet (F), G\u00F6relilik kuram\u0131nda ise K\u00FCtle (M) \u00F6nemli ve \u00F6nceliklidir. Genel g\u00F6relilik ile Einstein \u015Funlar\u0131 ortaya \u00E7\u0131kartm\u0131\u015Ft\u0131r: Yer\u00E7ekimi (k\u00FCtle\u00E7ekimi) ve ivmeli devinim birbirinden ay\u0131rt edilemez K\u00FCtle, i\u00E7inde bulundu\u011Fumuz uzay-zaman'\u0131 e\u011Fip b\u00FCkmektedir. Yer\u00E7ekimi bir kuvvet de\u011Fildir, uzay-zaman'\u0131n geometrik e\u011Frili\u011Finden ortaya \u00E7\u0131kar. Genel g\u00F6relilik, kendi zaman\u0131 i\u00E7in inan\u0131lmas\u0131 g\u00FC\u00E7 pek \u00E7ok \u00F6ng\u00F6r\u00FClerde bulunmu\u015Ftur; bunlardan en \u00F6nemlileri: E\u011Fer k\u00FCtle uzay-zaman\u0131 geometrik olarak e\u011Fiyorsa, G\u00FCne\u015Fin \u00E7ok yak\u0131n\u0131ndan ge\u00E7ip gelen uzak y\u0131ld\u0131zlar\u0131n \u0131\u015F\u0131klar\u0131 e\u011Frilmi\u015F olmal\u0131d\u0131r. Bu e\u011Frilik g\u00FCne\u015F \u00E7ekti\u011Fi i\u00E7in d\u0131\u015F b\u00FCkey de\u011Fil de uzay-zaman\u0131n e\u011Frili\u011Fine uygun i\u00E7 b\u00FCkey olmal\u0131d\u0131r. \u00C7ok \u00E7ok yo\u011Fun k\u00FCtleler uzay-zaman\u0131 \u00F6ylesine b\u00FCkebilir ki, uzay-zaman kendi \u00FCst\u00FCne katlan\u0131r ve i\u00E7ine \u00E7\u00F6ker, b\u00F6ylesine yo\u011Fun bir k\u00FCtle g\u00F6r\u00FClemez \u00E7\u00FCnk\u00FC \u0131\u015F\u0131k dahi bu uzay-zaman e\u011Frili\u011Finden, \u00E7\u00F6kmesinden kurtulamaz. K\u00FCtle uzay-zaman\u0131 e\u011Fiyorsa bu e\u011Filmeden zaman da etkileniyor(g\u00F6receli) olmal\u0131d\u0131r. E\u011Filmi\u015F zaman yava\u015F akmal\u0131d\u0131r. Hareketli b\u00FCy\u00FCk k\u00FCtleler etraflar\u0131ndaki bir k\u0131s\u0131m uzay-zaman\u0131 da s\u00FCr\u00FCkleyebiliyor olmal\u0131d\u0131r. K\u00FCtle uzay-zaman\u0131 e\u011Fiyorsa, k\u00FCtle yak\u0131n\u0131ndaki e\u011Frilikten ilerleyen \u0131\u015F\u0131k, uza\u011F\u0131ndaki d\u00FCzg\u00FCn uzay-zamanda ilerleyenden daha uzun yol almal\u0131d\u0131r. Y\u00FCksek k\u00FCtleli olu\u015Fumlar\u0131n ani hareketleri uzay-zamanda ani de\u011Fi\u015Fimlere, e\u011Frilik dalgalar\u0131 olu\u015Fmas\u0131na neden olabilir. Bu \u00F6ng\u00F6r\u00FClerin hemen hepsi 1916'dan g\u00FCn\u00FCm\u00FCze dek g\u00F6zlenebilmi\u015F, defalarca kez denenmi\u015F ve do\u011Fru \u00E7\u0131km\u0131\u015Ft\u0131r: 1919'da ilk kez \u0130ngiliz bilimciler g\u00FCne\u015F yak\u0131n\u0131ndan gelen \u0131\u015F\u0131\u011F\u0131n e\u011Fri \u00E7izdi\u011Fini g\u00F6zlemlediler. Daha sonralar\u0131 yap\u0131lan b\u00FCt\u00FCn g\u00F6zlemler e\u011Frili\u011Fin GG'nin hesaplad\u0131\u011F\u0131 ile olduk\u00E7a yak\u0131n oldu\u011Funu g\u00F6sterdi. Evrende hi\u00E7 \u0131\u015F\u0131k vermeyen ve etraf\u0131ndaki her \u015Feyi i\u00E7ine \u00E7ekecek kadar yo\u011Fun k\u00FCtle g\u00F6steren olu\u015Fumlar\u0131n varl\u0131\u011F\u0131 tespit edildi. Karadelik ad\u0131 verildi. K\u00FCtle yak\u0131n\u0131nda ve uza\u011F\u0131nda \u00E7ok hassas atom saatleri ile yap\u0131lan deneylerin hepsi k\u00FCtle yak\u0131n\u0131nda zaman\u0131n GG'nin hesaplar\u0131na uygun olarak yava\u015Flad\u0131\u011F\u0131n\u0131 g\u00F6sterdi. Ge\u00E7en y\u0131l a\u00E7\u0131kland\u0131\u011F\u0131 \u00FCzere \u00E7ok hassas jiroskoplarla donat\u0131lm\u0131\u015F LEGOS1 ve LEGOS2 uydular\u0131n\u0131n 11 y\u0131l s\u00FCren \u00F6l\u00E7\u00FCmleri d\u00FCnyan\u0131n etraf\u0131ndaki uzay-zaman\u0131 s\u00FCr\u00FCkledi\u011Fini ortaya koydu. G\u00FCne\u015Fin ard\u0131na ge\u00E7en Viking uzay ara\u00E7lar\u0131ndan d\u00FCnyaya g\u00F6nderilen sinyallerin olmas\u0131 gerekenden daha uzun s\u00FCrede d\u00FCnyaya ula\u015Ft\u0131\u011F\u0131, yani uzay-zaman\u0131n g\u00FCne\u015F taraf\u0131ndan e\u011Filmesinden etkilendikleri ortaya \u00E7\u0131kt\u0131. 1993'te Hulse ve Taylor, ikiz y\u0131ld\u0131zlar\u0131n spiral hareketinden uzay-zaman e\u011Frilik dalgalar\u0131n\u0131n olu\u015Fumunu g\u00F6zleyerek nobel kazand\u0131lar. K\u00FCtle, uzay\u0131 oldu\u011Fu kadar zaman\u0131 da b\u00FCkmektedir. Zaman\u0131n b\u00FCk\u00FClmesi k\u00FCtlenin merkezinde gelece\u011Fi i\u015Faret eder \u015Fekildedir. Etkiyen hi\u00E7bir kuvvet olmad\u0131\u011F\u0131 i\u00E7in, cisim kendi gelece\u011Fine do\u011Fru ilerlemektedir (d\u00FC\u015Fmektedir)."@tr ,
"De algemene relativiteitstheorie werd gepubliceerd door Albert Einstein in 1916 als een serie lezingen voor de Pruisische Academie van Wetenschappen. De theorie gaat anders dan de speciale relativiteitstheorie over de zwaartekracht en de kromming van de ruimte. Einstein voorspelde correct dat licht van verre sterren dat langs de zon scheert in het zwaartekrachtsveld van de zon wordt afgebogen. Na de vele kwantitatieve experimentele bevestigingen van de theorie, werd de relativiteitstheorie beroemd als een elegante opvolger (verfijning) van de voorheen bekende zwaartekrachtstheorie van Newton"@nl ,
"Obecn\u00E1 relativita nebo obecn\u00E1 teorie relativity je z\u00E1kladn\u00ED fyzik\u00E1ln\u00ED teorie gravitace formulovan\u00E1 Albertem Einsteinem, kter\u00E1 opravila a roz\u0161\u00ED\u0159ila Newton\u016Fv koncept gravitace, p\u0159edev\u0161\u00EDm v makroskopick\u00E9m m\u011B\u0159\u00EDtku planet a hv\u011Bzd. Obecnou relativitu lze ch\u00E1pat tak\u00E9 jako roz\u0161\u00ED\u0159en\u00ED speci\u00E1ln\u00ED relativity. Star\u0161\u00ED teorie poskytuje spr\u00E1vn\u00FD popis elektrodynamiky a \u0161\u00ED\u0159en\u00ED sv\u011Btla v inerci\u00E1ln\u00EDch vzta\u017En\u00FDch soustav\u00E1ch a opravuje nep\u0159esnosti Newtonovy mechaniky p\u0159i vysok\u00FDch rychlostech. Obecn\u00E1 relativita nav\u00EDc hraje mezi fyzik\u00E1ln\u00EDmi teoriemi jedine\u010Dnou roli v tom smyslu, \u017Ee vykl\u00E1d\u00E1 gravita\u010Dn\u00ED pole jako geometrick\u00FD fenom\u00E9n. P\u0159esn\u011Bji \u0159e\u010Deno p\u0159edpokl\u00E1d\u00E1, \u017Ee libovoln\u00FD objekt s vlastn\u00ED hmotnost\u00ED zak\u0159ivuje \u201Eprostor\u201C, ve kter\u00E9m se nach\u00E1z\u00ED, a toto zak\u0159iven\u00ED se projevuje jako gravitace. Abychom pochopili tuto rovnost, nen\u00ED dobr\u00E9 uva\u017Eovat, \u017Ee by gravitace zp\u016Fsobovala nebo byla zp\u016Fsobov\u00E1na zak\u0159iven\u00EDm \u010Dasoprostoru, ale sp\u00ED\u0161e, \u017Ee gravitace je zak\u0159iven\u00ED \u010Dasoprostoru. Teorie od sv\u00E9ho formulov\u00E1n\u00ED v roce 1915 dodnes p\u0159e\u017Eila v\u0161echny experimenty pokou\u0161ej\u00EDc\u00ED se o jej\u00ED vyvr\u00E1cen\u00ED. Obecn\u00E1 teorie relativity b\u00FDv\u00E1 tak\u00E9 ozna\u010Dov\u00E1na jako Einsteinova gravita\u010Dn\u00ED teorie."@cs ,
"General relativity or the general theory of relativity is the geometric theory of gravitation published by Albert Einstein in 1916. It is the current description of gravitation in modern physics. It unifies special relativity and Newton's law of universal gravitation, and describes gravity as a geometric property of space and time, or spacetime. In particular, the curvature of spacetime is directly related to the four-momentum of whatever matter and radiation are present. The relation is specified by the Einstein field equations, a system of partial differential equations. Many predictions of general relativity differ significantly from those of classical physics, especially concerning the passage of time, the geometry of space, the motion of bodies in free fall, and the propagation of light. Examples of such differences include gravitational time dilation, the gravitational redshift of light, and the gravitational time delay. General relativity's predictions have been confirmed in all observations and experiments to date. Although general relativity is not the only relativistic theory of gravity, it is the simplest theory that is consistent with experimental data. However, unanswered questions remain, the most fundamental being how general relativity can be reconciled with the laws of quantum physics to produce a complete and self-consistent theory of quantum gravity. Einstein's theory has important astrophysical implications. It points towards the existence of black holes\u2014regions of space in which space and time are distorted in such a way that nothing, not even light, can escape\u2014as an end-state for massive stars. There is evidence that such stellar black holes as well as more massive varieties of black hole are responsible for the intense radiation emitted by certain types of astronomical objects such as active galactic nuclei or microquasars. The bending of light by gravity can lead to the phenomenon of gravitational lensing, where multiple images of the same distant astronomical object are visible in the sky. General relativity also predicts the existence of gravitational waves, which have since been measured indirectly; a direct measurement is the aim of projects such as LIGO. In addition, general relativity is the basis of current cosmological models of a consistently expanding universe."@en ,
"Den allm\u00E4nna relativitetsteorin \u00E4r en teori om gravitation som publicerades av Albert Einstein 1915. Den f\u00F6renar den speciella relativitetsteorin och Isaac Newtons universella gravitation genom id\u00E9n att gravitationen inte \u00E4r en kraft i klassisk fysikalisk mening, utan \u00E4r en manifestation av rumtidens geometri. Rumtiden \u00E4r inte plan, utan kr\u00F6kt, och kr\u00F6kningen p\u00E5verkar hur kroppar f\u00E4rdas genom rumtiden. Denna kr\u00F6kning best\u00E4ms av energins och materiens f\u00F6rdelning i rummet."@sv ;
rdfs:comment "La Relativit\u00E0 generale \u00E8 una teoria fisica pubblicata da Albert Einstein nel 1915. Come disse lo stesso Einstein, fu il lavoro pi\u00F9 difficile della sua carriera di teorico a causa delle difficolt\u00E0 matematiche da superare, poich\u00E9 si trattava di far convergere concetti di geometria euclidea in uno spazio che poteva non esserlo."@it ,
"La relativitat general \u00E9s una teoria relativista de la gravitaci\u00F3. En aquest escenari, la pres\u00E8ncia d'una massa deforma localment l'espai-temps. El f\u00EDsic Thibault Damour utilitza al respecte l'expressi\u00F3 d'espai-temps el\u00E0stic. Aquesta teoria \u00E9s considerada com la principal obra d'Albert Einstein, at\u00E8s que la seva construcci\u00F3 el va ocupar des de 1907 fins el 1915 que la va finalitzar. Fins ara, cap dels assaigs experimentals efectuats no ha pogut trobar-ne cap defecte."@ca ,
"Die allgemeine Relativit\u00E4tstheorie beschreibt die Wechselwirkung zwischen Materie einerseits und Raum und Zeit andererseits. Sie deutet Gravitation als geometrische Eigenschaft der gekr\u00FCmmten vierdimensionalen Raumzeit. Die Grundlagen der Theorie wurden ma\u00DFgeblich von Albert Einstein entwickelt, der den Kern der Theorie am 25. November 1915 der Preu\u00DFischen Akademie der Wissenschaften vortrug. Zur Beschreibung der gekr\u00FCmmten Raumzeit bediente er sich der Differentialgeometrie."@de ,
"\u041E\u0301\u0431\u0449\u0430\u044F \u0442\u0435\u043E\u0301\u0440\u0438\u044F \u043E\u0442\u043D\u043E\u0441\u0438\u0301\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 (\u041E\u0422\u041E; \u043D\u0435\u043C. allgemeine Relativit\u00E4tstheorie) \u2014 \u0433\u0435\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u0442\u0435\u043E\u0440\u0438\u044F, \u0440\u0430\u0437\u0432\u0438\u0432\u0430\u044E\u0449\u0430\u044F \u0441\u043F\u0435\u0446\u0438\u0430\u043B\u044C\u043D\u0443\u044E \u0442\u0435\u043E\u0440\u0438\u044E \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438 (\u0421\u0422\u041E), \u043E\u043F\u0443\u0431\u043B\u0438\u043A\u043E\u0432\u0430\u043D\u043D\u0430\u044F \u0410\u043B\u044C\u0431\u0435\u0440\u0442\u043E\u043C \u042D\u0439\u043D\u0448\u0442\u0435\u0439\u043D\u043E\u043C \u0432 1915\u20141916 \u0433\u043E\u0434\u0430\u0445."@ru ,
"Genel g\u00F6relilik kuram\u0131, ivmeli devinim ile k\u00FCtle\u00E7ekimi a\u00E7\u0131klamas\u0131n\u0131 \u00F6zel g\u00F6relili\u011Fe birle\u015Ftiren, genelleyen kuramd\u0131r. 1916'da Einstein taraf\u0131ndan ortaya konmu\u015Ftur. Genel g\u00F6relilikten \u00F6nce, Newton'un k\u00FCtle\u00E7ekim kuram\u0131 ge\u00E7erli kabul ediliyordu. Newton'un form\u00FClleri (yatay at\u0131\u015F, dikey at\u0131\u015F vb) bugun de duyarl\u0131l\u0131k gerektirmeyen uygulamalarda ge\u00E7erlidir. Ancak aya roket g\u00F6ndermek gibi duyarl\u0131 i\u015Flerde Einstein form\u00FClleri kullan\u0131lmaktad\u0131r."@tr ,
"Obecn\u00E1 relativita nebo obecn\u00E1 teorie relativity je z\u00E1kladn\u00ED fyzik\u00E1ln\u00ED teorie gravitace formulovan\u00E1 Albertem Einsteinem, kter\u00E1 opravila a roz\u0161\u00ED\u0159ila Newton\u016Fv koncept gravitace, p\u0159edev\u0161\u00EDm v makroskopick\u00E9m m\u011B\u0159\u00EDtku planet a hv\u011Bzd. Obecnou relativitu lze ch\u00E1pat tak\u00E9 jako roz\u0161\u00ED\u0159en\u00ED speci\u00E1ln\u00ED relativity."@cs ,
"Em F\u00EDsica, a relatividade geral \u00E9 a generaliza\u00E7\u00E3o da Teoria da gravita\u00E7\u00E3o de Newton, publicada em 1915 por Albert Einstein e cuja base matem\u00E1tica foi desenvolvida pelo cientista franc\u00EAs Henri Poincar\u00E9."@pt ,
""@zh ,
"La Teor\u00EDa general de la relatividad o relatividad general es una teor\u00EDa del campo gravitatorio y de los sistemas de referencia generales, publicada por Albert Einstein en 1915 y 1916. El nombre de la teor\u00EDa se debe a que generaliza la llamada teor\u00EDa especial de la relatividad."@es ,
"La relativit\u00E9 g\u00E9n\u00E9rale est une th\u00E9orie relativiste de la gravitation, c'est-\u00E0-dire qu'elle d\u00E9crit l'influence sur le mouvement des astres de la pr\u00E9sence de mati\u00E8re et, plus g\u00E9n\u00E9ralement d'\u00E9nergie, en tenant compte des principes de la relativit\u00E9 restreinte."@fr ,
"Yleinen suhteellisuusteoria (engl. General relativity, GR) on painovoimaa kuvaava teoria, jonka kehitti saksalainen teoreettinen fyysikko Albert Einstein vuosina 1907–1915. Teorian mukaan kahden kappaleen v\u00E4lill\u00E4 havaittu painovoima johtuu siit\u00E4, ett\u00E4 kappaleiden massat kaareuttavat aika-avaruutta. Yleisess\u00E4 suhteellisuusteoriassa gravitaatio siis tulkitaan avaruuden kaareutumiseksi, toisin sanoen avaruuden geometrian muuttumiseksi."@fi ,
"General relativity or the general theory of relativity is the geometric theory of gravitation published by Albert Einstein in 1916. It is the current description of gravitation in modern physics. It unifies special relativity and Newton's law of universal gravitation, and describes gravity as a geometric property of space and time, or spacetime. In particular, the curvature of spacetime is directly related to the four-momentum of whatever matter and radiation are present."@en ,
"De algemene relativiteitstheorie werd gepubliceerd door Albert Einstein in 1916 als een serie lezingen voor de Pruisische Academie van Wetenschappen. De theorie gaat anders dan de speciale relativiteitstheorie over de zwaartekracht en de kromming van de ruimte. Einstein voorspelde correct dat licht van verre sterren dat langs de zon scheert in het zwaartekrachtsveld van de zon wordt afgebogen."@nl ,
"Den allm\u00E4nna relativitetsteorin \u00E4r en teori om gravitation som publicerades av Albert Einstein 1915. Den f\u00F6renar den speciella relativitetsteorin och Isaac Newtons universella gravitation genom id\u00E9n att gravitationen inte \u00E4r en kraft i klassisk fysikalisk mening, utan \u00E4r en manifestation av rumtidens geometri. Rumtiden \u00E4r inte plan, utan kr\u00F6kt, och kr\u00F6kningen p\u00E5verkar hur kroppar f\u00E4rdas genom rumtiden. Denna kr\u00F6kning best\u00E4ms av energins och materiens f\u00F6rdelning i rummet."@sv ,
"\u0417\u0430\u0433\u0430\u043B\u044C\u043D\u0430 \u0442\u0435\u043E\u0440\u0456\u044F \u0432\u0456\u0434\u043D\u043E\u0441\u043D\u043E\u0441\u0442\u0456 (\u0417\u0422\u0412) \u2014 \u0442\u0435\u043E\u0440\u0456\u044F \u0433\u0440\u0430\u0432\u0456\u0442\u0430\u0446\u0456\u0457, \u043E\u043F\u0443\u0431\u043B\u0456\u043A\u043E\u0432\u0430\u043D\u0430 \u0410\u043B\u044C\u0431\u0435\u0440\u0442\u043E\u043C \u0415\u0439\u043D\u0448\u0442\u0435\u0439\u043D\u043E\u043C \u0432 1915 \u0440\u043E\u0446\u0456. \u041D\u0430 \u0432\u0456\u0434\u043C\u0456\u043D\u0443 \u0432\u0456\u0434 \u043D\u0435\u0440\u0435\u043B\u044F\u0442\u0438\u0432\u0456\u0441\u0442\u0441\u044C\u043A\u043E\u0457 \u0442\u0435\u043E\u0440\u0456\u0457 \u0433\u0440\u0430\u0432\u0456\u0442\u0430\u0446\u0456\u0457 \u041D\u044C\u044E\u0442\u043E\u043D\u0430 \u0417\u0422\u0412 \u043F\u0440\u0438\u0434\u0430\u0442\u043D\u0430 \u0434\u043B\u044F \u043E\u043F\u0438\u0441\u0443 \u0433\u0440\u0430\u0432\u0456\u0442\u0430\u0446\u0456\u0439\u043D\u043E\u0457 \u0432\u0437\u0430\u0454\u043C\u043E\u0434\u0456\u0457 \u0442\u0456\u043B, \u0449\u043E \u0440\u0443\u0445\u0430\u044E\u0442\u044C\u0441\u044F \u0437\u0456 \u0448\u0432\u0438\u0434\u043A\u043E\u0441\u0442\u044F\u043C\u0438 \u0431\u043B\u0438\u0437\u044C\u043A\u0438\u043C\u0438 \u0434\u043E \u0448\u0432\u0438\u0434\u043A\u043E\u0441\u0442\u0456 \u0441\u0432\u0456\u0442\u043B\u0430."@uk ,
"Az \u00E1ltal\u00E1nos relativit\u00E1selm\u00E9let a gravit\u00E1ci\u00F3 Albert Einstein \u00E1ltal 1916-ban k\u00F6zz\u00E9tett elm\u00E9lete. Az \u00E1ltal\u00E1nos relativit\u00E1selm\u00E9let magja az az \u00E1ll\u00EDt\u00E1s, melyb\u0151l a t\u00F6bbi k\u00F6vetkezik, az ekvivalenciaelv, mely a gravit\u00E1ci\u00F3t \u00E9s a gyorsul\u00E1st ugyanannak a dolognak k\u00E9t l\u00E1t\u00E1sm\u00F3djak\u00E9nt \u00EDrja le."@hu ,
"Den generelle relativitetsteorien, ofte kalt bare generell relativitet (GR), er den geometriske teorien om gravitasjon som Albert Einstein publiserte i 1916. Den kombinerer spesiell relativitet og Newtons gravitasjonslov med den innsikt at gravitasjon ikke er en f\u00F8lge av noen kraft (i tradisjonell betydning av ordet), men er en manifestasjon av at tidrommet krummer seg. Denne krumningen kommer av mengden masse-energi i tidrommet."@no ,
"\u4E00\u822C\u76F8\u5BFE\u6027\u7406\u8AD6\uFF08\u3044\u3063\u3071\u3093\u305D\u3046\u305F\u3044\u305B\u3044\u308A\u308D\u3093\u3001\u72EC\u8A9E\uFF1AAllgemeine Relativit\u00E4tstheorie\u3001\u82F1\u8A9E\uFF1Ageneral theory of relativity\uFF09\u306F\u3001\u4E00\u822C\u76F8\u5BFE\u8AD6\uFF08General relativity\uFF09\u3068\u3082\u3044\u3044\u3001\u30A2\u30EB\u30D9\u30EB\u30C8\u30FB\u30A2\u30A4\u30F3\u30B7\u30E5\u30BF\u30A4\u30F3\u304C\u30011905\u5E74\u306E\u7279\u6B8A\u76F8\u5BFE\u6027\u7406\u8AD6\u306B\u7D9A\u3044\u30661915\u5E74 - 1916\u5E74\u306B\u767A\u8868\u3057\u305F\u7269\u7406\u5B66\u306E\u7406\u8AD6\u3002\u30CB\u30E5\u30FC\u30C8\u30F3\u529B\u5B66\u3068\u6BD4\u8F03\u3059\u308B\u3068\u3001\u904B\u52D5\u306E\u901F\u5EA6\u304C\u901F\u3044\u5834\u5408\u3084\u3001\u91CD\u529B\u304C\u5927\u304D\u3044\u5834\u5408\u306E\u73FE\u8C61\u3092\u6B63\u3057\u304F\u8A18\u8FF0\u3067\u304D\u308B\u3002"@ja ,
"Og\u00F3lna teoria wzgl\u0119dno\u015Bci (OTW) \u2013 popularna nazwa teorii grawitacji sformu\u0142owanej przez Alberta Einsteina w 1915 roku, a opublikowanej w roku 1916. Zgodnie z og\u00F3ln\u0105 teori\u0105 wzgl\u0119dno\u015Bci, si\u0142a grawitacji wynika z lokalnej geometrii czasoprzestrzeni. Aparat matematyczny tej teorii zosta\u0142 opracowany w pracach takich matematyk\u00F3w jak J\u00E1nos Bolyai, a tak\u017Ce Carl Gauss."@pl ;
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dbpprop:seeAlsoProperty "Mathematics of general relativity"@en ,
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dbpprop:loc "pp. 24\u201326"@en ,
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"ch. 11"@en ,
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"\u00A720.4"@en ,
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"p. 253\u2013254"@en ,
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"section 3.5"@en ,
"section 4.4"@en ,
"sec. 17.2"@en ,
"pp. 469\u2013471."@en ,
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"chapter 3"@en ,
"sec. 1.4."@en ,
"sec. 1.2"@en ,
"sec. \u00A711.4"@en ,
"\u00A714.5"@en ,
"section 22"@en ,
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"p. 202\u2013204."@en ,
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"pp. 312\u2013320"@en ,
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"part VIII"@en ,
"sec. 9.7"@en ,
"sec. 5"@en ,
"ch. 6."@en ,
"sec. 7.3"@en ,
"sec. 2.1"@en ,
"\u00A7 38.5"@en ,
"ch. 2\u20134"@en ,
"chapter 2"@en ,
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