A scalar field matter model for dark halos of galaxies and gravitational redshift

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dc.creatorSchunck, Franz E.
dc.date1998-02-19
dc.date.accessioned2026-07-07T02:26:08Z
dc.date.available2026-07-07T02:26:08Z
dc.descriptionWe analyze the spherically symmetric Einstein field equation with a massless complex scalar field. We can use the Newtonian solutions to fit the rotation curve data of spiral and dwarf galaxies. From the general relativistic solutions, we can derive high gravitational redshift values.
dc.description11 pages, RevTeX, 10 Postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9802258
dc.identifierhttp://arxiv.org/abs/astro-ph/9802258
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12150
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA scalar field matter model for dark halos of galaxies and gravitational redshift
dc.typetext

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