Opening a New Window to Fundamental Physics and Astrophysics: X-ray Polarimetry

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dc.creatorCosta, E.
dc.creatorBellazzini, R.
dc.creatorSoffitta, P.
dc.creatordi Persio, G.
dc.creatorFeroci, M.
dc.creatorMorelli, E.
dc.creatorMuleri, F.
dc.creatorPacciani, L.
dc.creatorRubini, A.
dc.creatorBaldini, L.
dc.creatorBitti, F.
dc.creatorBrez, A.
dc.creatorCavalca, F.
dc.creatorLatronico, L.
dc.creatorMassai, M. M.
dc.creatorOmodei, N.
dc.creatorSgro', C.
dc.creatorSpandre, G.
dc.creatorMatt, G.
dc.creatorPerola, G. C.
dc.creatorSantangelo, A.
dc.creatorCelotti, A.
dc.creatorBarret, D.
dc.creatorVilhu, O.
dc.creatorPiro, L.
dc.creatorFraser, G.
dc.creatorCourvoisier, T. J. -L.
dc.creatorBarcons, X.
dc.date2006-03-15
dc.date.accessioned2026-07-07T07:01:07Z
dc.date.available2026-07-07T07:01:07Z
dc.descriptionAn extensive theoretical literature predicts that X-ray Polarimetry can directly determine relevant physical and geometrical parameters of astrophysical sources, and discriminate between models further than allowed by spectral and timing data only. X-ray Polarimetry can also provide tests of Fundamental Physics. A high sensitivity polarimeter in the focal plane of a New Generation X-ray telescope could open this new window in the High Energy Sky.
dc.description8 pages 1 table 14 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0603399
dc.identifierhttp://arxiv.org/abs/astro-ph/0603399
dc.identifierProc. 39th ESLAB Symposium, Noordwijk, 19-21 April 2005, SP-588, p. 141-149, F. Favata, A. Gimenez. eds
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108183
dc.subjectAstrophysics
dc.titleOpening a New Window to Fundamental Physics and Astrophysics: X-ray Polarimetry
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