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Quasi-black holes: General features and purely field configurations

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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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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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