Supernova light-curve fitters and dark energy

We show that when a procedure is made to remove the tension between a supernova Ia (SN Ia) data set and observations from BAO and CMB, there might be the case where the same SN Ia set built with two different light-curve fitters behaves as two separate and distinct supernova sets, and the tension fo...

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Autor principal: Bengochea, G.R.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03702693_v696_n1-2_p5_Bengochea
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spelling todo:paper_03702693_v696_n1-2_p5_Bengochea2023-10-03T15:29:05Z Supernova light-curve fitters and dark energy Bengochea, G.R. Cosmology Dark energy experiments Dark energy theory Supernovae Ia We show that when a procedure is made to remove the tension between a supernova Ia (SN Ia) data set and observations from BAO and CMB, there might be the case where the same SN Ia set built with two different light-curve fitters behaves as two separate and distinct supernova sets, and the tension found by some authors between supernova sets actually could be due to tension or inconsistency between fitters. We also show that the information of the fitter used in an SN Ia data set could be relevant to determine whether phantom type models are favored or not when such a set is combined with the BAO/CMB joint parameter. © 2010 Elsevier B.V. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03702693_v696_n1-2_p5_Bengochea
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Cosmology
Dark energy experiments
Dark energy theory
Supernovae Ia
spellingShingle Cosmology
Dark energy experiments
Dark energy theory
Supernovae Ia
Bengochea, G.R.
Supernova light-curve fitters and dark energy
topic_facet Cosmology
Dark energy experiments
Dark energy theory
Supernovae Ia
description We show that when a procedure is made to remove the tension between a supernova Ia (SN Ia) data set and observations from BAO and CMB, there might be the case where the same SN Ia set built with two different light-curve fitters behaves as two separate and distinct supernova sets, and the tension found by some authors between supernova sets actually could be due to tension or inconsistency between fitters. We also show that the information of the fitter used in an SN Ia data set could be relevant to determine whether phantom type models are favored or not when such a set is combined with the BAO/CMB joint parameter. © 2010 Elsevier B.V.
format JOUR
author Bengochea, G.R.
author_facet Bengochea, G.R.
author_sort Bengochea, G.R.
title Supernova light-curve fitters and dark energy
title_short Supernova light-curve fitters and dark energy
title_full Supernova light-curve fitters and dark energy
title_fullStr Supernova light-curve fitters and dark energy
title_full_unstemmed Supernova light-curve fitters and dark energy
title_sort supernova light-curve fitters and dark energy
url http://hdl.handle.net/20.500.12110/paper_03702693_v696_n1-2_p5_Bengochea
work_keys_str_mv AT bengocheagr supernovalightcurvefittersanddarkenergy
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