CMB Quadrupole induced polarisation from clusters and filaments

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dc.creatorLiu, Guo-Chin
dc.creatorda Silva, Antonio
dc.creatorAghanim, Nabila
dc.date2004-09-13
dc.date.accessioned2026-07-07T02:14:35Z
dc.date.available2026-07-07T02:14:35Z
dc.descriptionWe present the estimates of the Cosmic Microwave Background (CMB) polarisation power spectrum from galaxy clusters and filaments using hydrodynamical simulations of large scale structure formation. We focus in the present study on the CMB Quadrupole induced polarisation, which is the dominate secondary polarisation effect, and give the E and B mode power spectra between $l \sim 560$ to 20000.
dc.descriptionTo appear in proceedings of the Moriond 2004 meeting
dc.identifierhttps://arxiv.org/abs/astro-ph/0409297
dc.identifierhttp://arxiv.org/abs/astro-ph/0409297
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8168
dc.subjectAstrophysics
dc.titleCMB Quadrupole induced polarisation from clusters and filaments
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