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Supernovae, dark energy and the accelerating universe

Based on an analysis of 42 high-redshift supernovae discovered by the supernovae cosmology project, we have found evidence for a positive cosmological constant, Lambda, and hence an accelerating universe. In particular, the data are strongly inconsistent with a Lambda=0 flat cosmology, the simplest...

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Detalles Bibliográficos
Autor principal: Perlmutter, Saul
Lenguaje:eng
Publicado: CERN 1999
Materias:
Acceso en línea:http://cds.cern.ch/record/403462
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author Perlmutter, Saul
author_facet Perlmutter, Saul
author_sort Perlmutter, Saul
collection CERN
description Based on an analysis of 42 high-redshift supernovae discovered by the supernovae cosmology project, we have found evidence for a positive cosmological constant, Lambda, and hence an accelerating universe. In particular, the data are strongly inconsistent with a Lambda=0 flat cosmology, the simplest inflationary universe model. The size of our supernova sample allows us to perform a variety of statistical tests to check for possible systematic errors and biases. We will discuss results of these and other studies and the ongoing hunt for further loopholes to evade the apparent consequences of the measurements. We will present further work that begins to constrain the alternative physics theories of "dark energy" that have been proposed to explain these results. Finally, we propose a new concept for a definitive supernova measurement of the cosmological parameters.
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institution Organización Europea para la Investigación Nuclear
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publishDate 1999
publisher CERN
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spelling cern-4034622022-11-03T08:17:26Zhttp://cds.cern.ch/record/403462engPerlmutter, SaulSupernovae, dark energy and the accelerating universeAstrophysics and AstronomyBased on an analysis of 42 high-redshift supernovae discovered by the supernovae cosmology project, we have found evidence for a positive cosmological constant, Lambda, and hence an accelerating universe. In particular, the data are strongly inconsistent with a Lambda=0 flat cosmology, the simplest inflationary universe model. The size of our supernova sample allows us to perform a variety of statistical tests to check for possible systematic errors and biases. We will discuss results of these and other studies and the ongoing hunt for further loopholes to evade the apparent consequences of the measurements. We will present further work that begins to constrain the alternative physics theories of "dark energy" that have been proposed to explain these results. Finally, we propose a new concept for a definitive supernova measurement of the cosmological parameters.CERNoai:cds.cern.ch:4034621999
spellingShingle Astrophysics and Astronomy
Perlmutter, Saul
Supernovae, dark energy and the accelerating universe
title Supernovae, dark energy and the accelerating universe
title_full Supernovae, dark energy and the accelerating universe
title_fullStr Supernovae, dark energy and the accelerating universe
title_full_unstemmed Supernovae, dark energy and the accelerating universe
title_short Supernovae, dark energy and the accelerating universe
title_sort supernovae, dark energy and the accelerating universe
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/403462
work_keys_str_mv AT perlmuttersaul supernovaedarkenergyandtheacceleratinguniverse