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The Value of the Superstring Tension and Dark Matter

Brosche, P.; Tassie, Lindsay

Description

We start from our extended scenario for the formation of astronomical objects from fragmenting macroscopic superstrings, and we combine it with our view of an "orderly" fragmentation applied to the formation of black holes (Brosche, Lentes & Tassie 2003), now to the whole objects: the radial order of the matter should be preserved. Then we have to adapt the value of the superstring tension derived from the observed ratios of κ = (angular momentum)/(mass squared). If we calculate potential...[Show more]

dc.contributor.authorBrosche, P.
dc.contributor.authorTassie, Lindsay
dc.date.accessioned2015-12-13T23:03:34Z
dc.identifier.issn0004-6337
dc.identifier.urihttp://hdl.handle.net/1885/85003
dc.description.abstractWe start from our extended scenario for the formation of astronomical objects from fragmenting macroscopic superstrings, and we combine it with our view of an "orderly" fragmentation applied to the formation of black holes (Brosche, Lentes & Tassie 2003), now to the whole objects: the radial order of the matter should be preserved. Then we have to adapt the value of the superstring tension derived from the observed ratios of κ = (angular momentum)/(mass squared). If we calculate potential energies on the basis of a fragmentation until baryonic elementary particles, it turns out that the changed string tension explains as well the mechanical state of observed astronomical objects (without large energy loss on the way from the parent string parts) as also the fraction of bound to unbound matter (about 1:10). The implied superstring tension is about μ = (1/3000) c2/G. This corresponds to a string tension of 4 × 1040 Newton.
dc.publisherWiley-VCH Verlag GMBH
dc.sourceAstronomische Nachrichten
dc.subjectKeywords: Dark matter; Galaxian parameters; Macroscopic superstrings
dc.titleThe Value of the Superstring Tension and Dark Matter
dc.typeJournal article
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.citationvolume327
dc.date.issued2006
local.identifier.absfor010504 - Mathematical Aspects of General Relativity
local.identifier.ariespublicationMigratedxPub13206
local.type.statusPublished Version
local.contributor.affiliationBrosche, P., Universitatssternwarte Bonn
local.contributor.affiliationTassie, Lindsay, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.issue4
local.bibliographicCitation.startpage379
local.bibliographicCitation.lastpage382
local.identifier.doi10.1002/asna.200510530
dc.date.updated2015-12-12T07:50:11Z
local.identifier.scopusID2-s2.0-33646775671
CollectionsANU Research Publications

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