Please use this identifier to cite or link to this item: https://doi.org/10.21256/zhaw-3854
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dc.contributor.authorCardona, Wilmar-
dc.contributor.authorHollenstein, Lukas-
dc.contributor.authorKunz, Martin-
dc.date.accessioned2018-07-12T11:39:01Z-
dc.date.available2018-07-12T11:39:01Z-
dc.date.issued2014-07-16-
dc.identifier.issn1475-7516de_CH
dc.identifier.urihttps://digitalcollection.zhaw.ch/handle/11475/7940-
dc.description.abstractWe study a dark energy model with non-zero anisotropic stress, either linked to the dark energy density or to the dark matter density. We compute approximate solutions that allow to characterise the behaviour of the dark energy model and to assess the stability of the perturbations. We also determine the current limits on such an anisotropic stress from the cosmic microwave background data by the Planck satellite, and derive the corresponding constraints on the modified growth parameters like the growth index, the effective Newton's constant and the gravitational slip.de_CH
dc.language.isoende_CH
dc.publisherIOP Publishingde_CH
dc.relation.ispartofJournal of Cosmology and Astroparticle Physicsde_CH
dc.rightsLicence according to publishing contractde_CH
dc.subjectCosmological parameters from CMBRde_CH
dc.subjectDark energy theoryde_CH
dc.subjectModified gravityde_CH
dc.subject.ddc530: Physikde_CH
dc.titleThe traces of anisotropic dark energy in light of Planckde_CH
dc.typeBeitrag in wissenschaftlicher Zeitschriftde_CH
dcterms.typeTextde_CH
zhaw.departementLife Sciences und Facility Managementde_CH
zhaw.organisationalunitInstitut für Computational Life Sciences (ICLS)de_CH
dc.identifier.doi10.21256/zhaw-3854-
dc.identifier.doi10.1088/1475-7516/2014/07/032de_CH
zhaw.funding.euNode_CH
zhaw.issue7de_CH
zhaw.originated.zhawYesde_CH
zhaw.pages.start032de_CH
zhaw.publication.statussubmittedVersionde_CH
zhaw.volume2014de_CH
zhaw.publication.reviewPeer review (Publikation)de_CH
zhaw.webfeedSimulation and Optimizationde_CH
Appears in collections:Publikationen Life Sciences und Facility Management

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Cardona, W., Hollenstein, L., & Kunz, M. (2014). The traces of anisotropic dark energy in light of Planck. Journal of Cosmology and Astroparticle Physics, 2014(7), 32. https://doi.org/10.21256/zhaw-3854
Cardona, W., Hollenstein, L. and Kunz, M. (2014) ‘The traces of anisotropic dark energy in light of Planck’, Journal of Cosmology and Astroparticle Physics, 2014(7), p. 032. Available at: https://doi.org/10.21256/zhaw-3854.
W. Cardona, L. Hollenstein, and M. Kunz, “The traces of anisotropic dark energy in light of Planck,” Journal of Cosmology and Astroparticle Physics, vol. 2014, no. 7, p. 032, Jul. 2014, doi: 10.21256/zhaw-3854.
CARDONA, Wilmar, Lukas HOLLENSTEIN und Martin KUNZ, 2014. The traces of anisotropic dark energy in light of Planck. Journal of Cosmology and Astroparticle Physics. 16 Juli 2014. Bd. 2014, Nr. 7, S. 032. DOI 10.21256/zhaw-3854
Cardona, Wilmar, Lukas Hollenstein, and Martin Kunz. 2014. “The Traces of Anisotropic Dark Energy in Light of Planck.” Journal of Cosmology and Astroparticle Physics 2014 (7): 32. https://doi.org/10.21256/zhaw-3854.
Cardona, Wilmar, et al. “The Traces of Anisotropic Dark Energy in Light of Planck.” Journal of Cosmology and Astroparticle Physics, vol. 2014, no. 7, July 2014, p. 32, https://doi.org/10.21256/zhaw-3854.


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