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Future supernovae observations as a probe of dark energy

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Weller, Jochen, Albrecht, Andreas·2002·Physical Review D

Abstract

We study the potential impact of improved future supernovae data on our understanding of the dark energy problem. We carefully examine the relative utility of different fitting functions that can be used to parametrize the dark energy models, and provide concrete reasons why a particular choice (based on a parametrization of the equation of state) is better in almost all cases. We discuss the details of a representative sample of dark energy models and show how future supernova observations could distinguish among these. As a specific example, we consider the proposed ``SNAP'' satellite which is planned to observe around 2000 supernovae. We show how a SNAP-class data set taken alone would be a powerful discriminator among a family of models that would be approximated by a constant equation of state for the most recent epoch of cosmic expansion. We show how this family includes most of the dark energy models proposed so far. We then show how an independent measurement of ${\ensuremath{\Omega}}_{\mathrm{m}}$ can allow SNAP to probe the evolution of the equation of state as well, allowing further discrimination among a larger class of proposed dark energy models. We study the impact of the satellite design parameters on this method to distinguish the models and compare SNAP to alternative measurements. We establish that if we exploit the full precision of SNAP it provides a very powerful probe.

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Metadata

Authors
Weller, J., & Albrecht, A.
Venue
Physical Review D
Published
2002-05-09
Volume
65
Issue
10
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2032400252
Cited by
341
References
10
FWCI
22.64
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Future supernovae observations as a probe of dark energy. https://app.cochat.ai/papers/10.1103/physrevd.65.103512
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Weller, J., & Albrecht, A. (2002). Future supernovae observations as a probe of dark energy. Physical Review D. https://doi.org/10.1103/physrevd.65.103512

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