English   español  
Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/17777
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:

Gravitational waves from self-ordering scalar fields

AutorFenu, Elisa; García Figueroa, Daniel ; Durrer, Ruth; García-Bellido, Juan
Palabras claveCosmological phase transitions
Gravitational waves / sources
Fecha de publicación7-oct-2009
EditorInstitute of Physics Publishing
CitaciónJournal of Cosmology and Astroparticle Physics (JCAP) 10(2009)005
ResumenGravitational waves were copiously produced in the early Universe whenever the processes taking place were sufficiently violent. The spectra of several of these gravitational wave backgrounds on subhorizon scales have been extensively studied in the literature. In this paper we analyze the shape and amplitude of the gravitational wave spectrum on scales which are superhorizon at the time of production. Such gravitational waves are expected from the self ordering of randomly oriented scalar fields which can be present during a thermal phase transition or during preheating after hybrid inflation. We find that, if the gravitational wave source acts only during a small fraction of the Hubble time, the gravitational wave spectrum at frequencies lower than the expansion rate at the time of production behaves as Ω(GW)(f) α f^3 with an amplitude much too small to be observable by gravitational wave observatories like LIGO, LISA or BBO. On the other hand, if the source is active for a much longer time, until a given mode which is initially superhorizon (kη* << 1), enters the horizon, for kη >~ 1, we find that the gravitational wave energy density is frequency independent, i.e. scale invariant. Moreover, its amplitude for a GUT scale scenario turns out to be within the range and sensitivity of BBO and marginally detectable by LIGO and LISA. This new gravitational wave background can compete with the one generated during inflation, and distinguishing both may require extra information.
Descripción21 pages, 2 figures.-- Full-text version available Open Access at the journal site.
Versión del editorhttp://dx.doi.org/10.1088/1475-7516/2009/10/005
Aparece en las colecciones: (IFT) Artículos
Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
0908.0425v2.pdf264,83 kBAdobe PDFVista previa
Mostrar el registro completo

Artículos relacionados:

NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.