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Stationary configurations imply shift symmetry: no Bondi accretion for quintessence/k-essence

dc.contributor.authorAkhoury, Ratindranathen_US
dc.date.accessioned2010-03-23T15:26:57Z
dc.date.available2010-03-23T15:26:57Z
dc.date.issued2009en_US
dc.identifier.citationAkhoury, Ratindranath (2009). "Stationary configurations imply shift symmetry: no Bondi accretion for quintessence/k-essence." Journal of High Energy Physics 2009(3): 82. <http://hdl.handle.net/2027.42/65115>en_US
dc.identifier.issn1126-6708en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/65115
dc.description.abstractIn this paper we show that, for general scalar fields, stationary configurations are possible for shift symmetric theories only. This symmetry with respect to constant translations in field space should either be manifest in the original field variables or reveal itself after an appropriate field redefinition. In particular this result implies that neither k- Essence nor Quintessence can have exact steady state / Bondi accretion onto Black Holes. We also discuss the role of field redefinitions in k- Essence theories. Here we study the transformation properties of observables and other variables in k- Essence and emphasize which of them are covariant under field redefinitions. Finally we find that stationary field configurations are necessarily linear in Killing time, provided that shift symmetry is realized in terms of these field variables.en_US
dc.format.extent3111 bytes
dc.format.extent268366 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.publisherIOP Publishingen_US
dc.titleStationary configurations imply shift symmetry: no Bondi accretion for quintessence/k-essenceen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/65115/2/1126-6708_2009_03_082.pdf
dc.identifier.sourceJournal of High Energy Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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