Type Ia supernova discoveries at z > 1 from the hubble space telescope

Evidence for past deceleration and constraints on dark energy evolution

Adam G. Riess, Louis Gregory Sirolger, John Tonry, Stefano Casertano, Henry C. Ferguson, Bahram Mobasher, Peter Challis, Alexei V. Filippenko, Saurabh Jha, Weidong Li, Ryan Chornock, Robert P. Kirshner, Bruno Leibundgut, Mark Dickinson, Mario Livio, Mauro Giavalisco, Charles C. Steidel, Txitxo Benítez, Zlatan Tsvetanov

Research output: Contribution to journalArticle

2808 Citations (Scopus)

Abstract

We have discovered 16 Type la supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration. These objects, discovered during the course of the GOODS ACS Treasury program, include 6 of the 7 highest redshift SNe Ia known, all at z > 1.25, and populate the Hubble diagram in unexplored territory. The luminosity distances to these objects and to 170 previously reported SNe Ia have been determined using empirical relations between light-curve shape and luminosity. A purely kinematic interpretation of the SN Ia sample provides evidence at the greater than 99% confidence level for a transition from deceleration to acceleration or, similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at z = 0.46 ± 0.13. The data are consistent with the cosmic concordance model of Ω M ≈ 0.3, Ω Λ ≈ 0.7 (χ dof 2 = 1.06) and are inconsistent with a simple model of evolution or dust as an alternative to dark energy. For a flat universe with a cosmological constant, we measure Ω M = 0.29± 0.03 0.05 (equivalently, Ω Λ = 0.71). When combined with external flat-universe constraints, including the cosmic microwave background and large-scale structure, we find w = -1.02± 0.19 0.13 (and w < -0.76 at the 95% confidence level) for an assumed static equation of state of dark energy, P = wpc 2. Joint constraints on both the recent equation of state of dark energy, w 0, and its time evolution, dw/dz, are a factor of ∼8 more precise than the first estimates and twice as precise as those without the SNe Ia discovered with HST. Our constraints are consistent with the static nature of and value of w expected for a cosmological constant (i.e., W 0 = -1.0, dw/dz = 0) and are inconsistent with very rapid evolution of dark energy. We address consequences of evolving dark energy for the fate of the universe.

Original languageEnglish
Pages (from-to)665-687
Number of pages23
JournalAstrophysical Journal Letters
Volume607
Issue number2 I
DOIs
Publication statusPublished - 1 Jun 2004
Externally publishedYes

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deceleration
dark energy
Hubble Space Telescope
supernovae
universe
energy
equation of state
confidence
equations of state
luminosity
time measurement
Hubble diagram
light curve
kinematics
dust
diagram
histories
microwaves
expansion
estimates

Keywords

  • Cosmology: Observations
  • Distance scale
  • Galaxies: Distances and redshifts
  • Supernovae: General

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Type Ia supernova discoveries at z > 1 from the hubble space telescope : Evidence for past deceleration and constraints on dark energy evolution. / Riess, Adam G.; Sirolger, Louis Gregory; Tonry, John; Casertano, Stefano; Ferguson, Henry C.; Mobasher, Bahram; Challis, Peter; Filippenko, Alexei V.; Jha, Saurabh; Li, Weidong; Chornock, Ryan; Kirshner, Robert P.; Leibundgut, Bruno; Dickinson, Mark; Livio, Mario; Giavalisco, Mauro; Steidel, Charles C.; Benítez, Txitxo; Tsvetanov, Zlatan.

In: Astrophysical Journal Letters, Vol. 607, No. 2 I, 01.06.2004, p. 665-687.

Research output: Contribution to journalArticle

Riess, AG, Sirolger, LG, Tonry, J, Casertano, S, Ferguson, HC, Mobasher, B, Challis, P, Filippenko, AV, Jha, S, Li, W, Chornock, R, Kirshner, RP, Leibundgut, B, Dickinson, M, Livio, M, Giavalisco, M, Steidel, CC, Benítez, T & Tsvetanov, Z 2004, 'Type Ia supernova discoveries at z > 1 from the hubble space telescope: Evidence for past deceleration and constraints on dark energy evolution', Astrophysical Journal Letters, vol. 607, no. 2 I, pp. 665-687. https://doi.org/10.1086/383612
Riess, Adam G. ; Sirolger, Louis Gregory ; Tonry, John ; Casertano, Stefano ; Ferguson, Henry C. ; Mobasher, Bahram ; Challis, Peter ; Filippenko, Alexei V. ; Jha, Saurabh ; Li, Weidong ; Chornock, Ryan ; Kirshner, Robert P. ; Leibundgut, Bruno ; Dickinson, Mark ; Livio, Mario ; Giavalisco, Mauro ; Steidel, Charles C. ; Benítez, Txitxo ; Tsvetanov, Zlatan. / Type Ia supernova discoveries at z > 1 from the hubble space telescope : Evidence for past deceleration and constraints on dark energy evolution. In: Astrophysical Journal Letters. 2004 ; Vol. 607, No. 2 I. pp. 665-687.
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AU - Casertano, Stefano

AU - Ferguson, Henry C.

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AU - Kirshner, Robert P.

AU - Leibundgut, Bruno

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AU - Livio, Mario

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N2 - We have discovered 16 Type la supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration. These objects, discovered during the course of the GOODS ACS Treasury program, include 6 of the 7 highest redshift SNe Ia known, all at z > 1.25, and populate the Hubble diagram in unexplored territory. The luminosity distances to these objects and to 170 previously reported SNe Ia have been determined using empirical relations between light-curve shape and luminosity. A purely kinematic interpretation of the SN Ia sample provides evidence at the greater than 99% confidence level for a transition from deceleration to acceleration or, similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at z = 0.46 ± 0.13. The data are consistent with the cosmic concordance model of Ω M ≈ 0.3, Ω Λ ≈ 0.7 (χ dof 2 = 1.06) and are inconsistent with a simple model of evolution or dust as an alternative to dark energy. For a flat universe with a cosmological constant, we measure Ω M = 0.29± 0.03 0.05 (equivalently, Ω Λ = 0.71). When combined with external flat-universe constraints, including the cosmic microwave background and large-scale structure, we find w = -1.02± 0.19 0.13 (and w < -0.76 at the 95% confidence level) for an assumed static equation of state of dark energy, P = wpc 2. Joint constraints on both the recent equation of state of dark energy, w 0, and its time evolution, dw/dz, are a factor of ∼8 more precise than the first estimates and twice as precise as those without the SNe Ia discovered with HST. Our constraints are consistent with the static nature of and value of w expected for a cosmological constant (i.e., W 0 = -1.0, dw/dz = 0) and are inconsistent with very rapid evolution of dark energy. We address consequences of evolving dark energy for the fate of the universe.

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