Talk about Pivots

dc.creatorMartin, Damien
dc.creatorAlbrecht, Andreas
dc.date2006-04-19
dc.date.accessioned2026-07-07T07:04:42Z
dc.date.available2026-07-07T07:04:42Z
dc.descriptionWe consider two different methods of parameterizing the dark energy equation of state in order to assess possible ``figures of merit'' for evaluating dark energy experiments. The two models are $w(a) = w_0 + (1-a)w_a$ and $w(a) = w_p + (a_p - a)w_a$. This brief note shows that the size of the error contours cannot change under such a reparameterization. This makes the figures of merit associated with these parameterizations mathematically identical. This also means that any ``bias'' exhibited by one model is equally present in the other.
dc.description3 pages; brief comment
dc.identifierhttps://arxiv.org/abs/astro-ph/0604401
dc.identifierhttp://arxiv.org/abs/astro-ph/0604401
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/109410
dc.subjectAstrophysics
dc.titleTalk about Pivots
dc.typetext

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