Basit öğe kaydını göster

A new model for the formation of mini black holes

dc.contributor.authorEsmer, GD
dc.contributor.authorZebitay, S
dc.date.accessioned2021-03-05T10:11:42Z
dc.date.available2021-03-05T10:11:42Z
dc.date.issued2000
dc.identifier.citationEsmer G., Zebitay S., "A new model for the formation of mini black holes", GENERAL RELATIVITY AND GRAVITATION, cilt.32, ss.1241-1254, 2000
dc.identifier.issn0001-7701
dc.identifier.otherav_a1db11c9-cd28-4ef2-9494-b54237d26d18
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/108428
dc.identifier.urihttps://doi.org/10.1023/a:1001986503301
dc.description.abstractA new model different from the Hawking model is suggested to describe the formation of mini (primordial) black holes. It is based on an idea that the fluids, which All in the universe at the beginning just after the big bang, are separated into mini clusters, moving with supersonic velocities and colliding with each other under the forces of gravitational attractions. We show that between the time era from 10(-43) to 10(-8) sec. about 36 various generations of mini black holes with masses ranging in the interval 10(-5)-10(30) gm are possible.
dc.language.isoeng
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectFizik
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectAstronomi ve Astrofizik
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.titleA new model for the formation of mini black holes
dc.typeMakale
dc.relation.journalGENERAL RELATIVITY AND GRAVITATION
dc.contributor.department, ,
dc.identifier.volume32
dc.identifier.issue7
dc.identifier.startpage1241
dc.identifier.endpage1254
dc.contributor.firstauthorID125933


Bu öğenin dosyaları:

DosyalarBoyutBiçimGöster

Bu öğe ile ilişkili dosya yok.

Bu öğe aşağıdaki koleksiyon(lar)da görünmektedir.

Basit öğe kaydını göster