Quasi-black holes: General features and purely field configurations

dc.contributor.author	Bronnikov K.
dc.contributor.author	Zaslavskii O.
dc.date.accessioned	2018-09-18T20:07:14Z
dc.date.available	2018-09-18T20:07:14Z
dc.date.issued	2015
dc.identifier.issn	0217-7323
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/136694
dc.description.abstract	© 2015 World Scientific Publishing Company Objects that are on the threshold of forming the horizon but never collapse are called quasi-black holes (QBHs). We discuss the properties of the general spherically symmetric QBH metric without addressing its material source, including its limiting cases as the corresponding small parameter tends to zero. We then show that QBHs can exist among self-gravitating configurations of electromagnetic and dilatonic scalar fields without matter. These general results are illustrated by explicit examples of exact solutions.
dc.relation.ispartofseries	Modern Physics Letters A
dc.title	Quasi-black holes: General features and purely field configurations
dc.type	Article in Press
dc.collection	Публикации сотрудников КФУ
dc.source.id	SCOPUS02177323-2015-SID84940399038

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.