publication . Article . 1987

galaxy formation by cosmic strings and cooling of baryonic matter

Mizuo, IZAWA; Humitaka, SATO; Department of Physics, University of Tokyo; Department of Physics, Kyoto University;
Open Access
  • Published: 01 Dec 1987 Journal: Progress of Theoretical Physics, volume 78, pages 1,219-1,224 (issn: 0033-068X, eissn: 1347-4081, Copyright policy)
  • Publisher: Oxford University Press (OUP)
Abstract
Today we have various kinds of scenarios for the formation of the large-scale structure in the universe (galaxy formation). Nevertheless, it is without doubt that none of them are satisfactory. Recently, much work has been done ·on galaxy formation by cosmic strings, which may be formed at a phase transition in the early universe/),2) especially by closed strings (IoopS).2)-5) A characteristic feature of galaxy formation scenarios by string loops is that virialized objects are formed at an early stage, whose feature may explain large redshifts of quasars. However, the evolution of baryonic matter (e.g., the formation of luminous pattern) has not been investigate...
Subjects
free text keywords: Physics and Astronomy (miscellaneous), Universe, media_common.quotation_subject, media_common, Astrophysics, Physics, Dark matter, Redshift, Galaxy formation and evolution, Quasar, Galaxy, Baryon, Cold dark matter, Particle physics
Related Organizations
Powered by OpenAIRE Open Research Graph
Any information missing or wrong?Report an Issue
publication . Article . 1987

galaxy formation by cosmic strings and cooling of baryonic matter

Mizuo, IZAWA; Humitaka, SATO; Department of Physics, University of Tokyo; Department of Physics, Kyoto University;