Supernova limits on the cosmic equation of state

Peter M. Garnavich, Saurabh Jha, Peter Challis, Alejandro Clocchiatti, Alan Diercks, Alexei V. Filippenko, Ronald Lynn Gilliland, Craig J. Hogan, Robert P. Kirshner, Bruno Leibundgut, M. M. Phillips, David Reiss, Adam G. Riess, Brian P. Schmidt, Robert A. Schummer, R. Chris Smith, Jason Spyromilio, Chris Stubbs, Nicholas B. Suntzeff, John Tonry & 1 others Sean M. Carroll

Research output: Contribution to journalArticle

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Abstract

We use Type la supernovae studied by the High-z Supernova Search Team to constrain the properties of an energy component that may have contributed to accelerating the cosmic expansion. We find that for a flat geometry the equation-of-state parameter for the unknown component, αx = Pxx, must be less than -0.55 (95% confidence) for any value of Ωm, and it is further limited to αx < -0.60 (95% confidence) if Ωm is assumed to be greater than 0.1. These values are inconsistent with the unknown component being topological defects such as domain walls, strings, or textures. The supernova (SN) data are consistent with a cosmological constant (αx = -1) or a scalar field that has had, on average, an equation-of-state parameter similar to the cosmological constant value of -1 over the redshift range of z ≈1 to the present. SN and cosmic microwave background observations give complementary constraints on the densities of matter and the unknown component. If only matter and vacuum energy are considered, then the current combined data sets provide direct evidence for a spatially flat universe with Ωiot = Ωm + ΩΔ = 0.94 ± 0.26 (1 σ).

Original languageEnglish (US)
Pages (from-to)74-79
Number of pages6
JournalAstrophysical Journal
Volume509
Issue number1 PART I
DOIs
StatePublished - Jan 1 1998

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equation of state
supernovae
equations of state
defect
energy
confidence
texture
geometry
domain wall
strings
textures
universe
scalars
microwaves
vacuum
expansion
parameter
defects
microwave

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Garnavich, P. M., Jha, S., Challis, P., Clocchiatti, A., Diercks, A., Filippenko, A. V., ... Carroll, S. M. (1998). Supernova limits on the cosmic equation of state. Astrophysical Journal, 509(1 PART I), 74-79. https://doi.org/10.1086/306495
Garnavich, Peter M. ; Jha, Saurabh ; Challis, Peter ; Clocchiatti, Alejandro ; Diercks, Alan ; Filippenko, Alexei V. ; Gilliland, Ronald Lynn ; Hogan, Craig J. ; Kirshner, Robert P. ; Leibundgut, Bruno ; Phillips, M. M. ; Reiss, David ; Riess, Adam G. ; Schmidt, Brian P. ; Schummer, Robert A. ; Chris Smith, R. ; Spyromilio, Jason ; Stubbs, Chris ; Suntzeff, Nicholas B. ; Tonry, John ; Carroll, Sean M. / Supernova limits on the cosmic equation of state. In: Astrophysical Journal. 1998 ; Vol. 509, No. 1 PART I. pp. 74-79.
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Garnavich, PM, Jha, S, Challis, P, Clocchiatti, A, Diercks, A, Filippenko, AV, Gilliland, RL, Hogan, CJ, Kirshner, RP, Leibundgut, B, Phillips, MM, Reiss, D, Riess, AG, Schmidt, BP, Schummer, RA, Chris Smith, R, Spyromilio, J, Stubbs, C, Suntzeff, NB, Tonry, J & Carroll, SM 1998, 'Supernova limits on the cosmic equation of state', Astrophysical Journal, vol. 509, no. 1 PART I, pp. 74-79. https://doi.org/10.1086/306495

Supernova limits on the cosmic equation of state. / Garnavich, Peter M.; Jha, Saurabh; Challis, Peter; Clocchiatti, Alejandro; Diercks, Alan; Filippenko, Alexei V.; Gilliland, Ronald Lynn; Hogan, Craig J.; Kirshner, Robert P.; Leibundgut, Bruno; Phillips, M. M.; Reiss, David; Riess, Adam G.; Schmidt, Brian P.; Schummer, Robert A.; Chris Smith, R.; Spyromilio, Jason; Stubbs, Chris; Suntzeff, Nicholas B.; Tonry, John; Carroll, Sean M.

In: Astrophysical Journal, Vol. 509, No. 1 PART I, 01.01.1998, p. 74-79.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Supernova limits on the cosmic equation of state

AU - Garnavich, Peter M.

AU - Jha, Saurabh

AU - Challis, Peter

AU - Clocchiatti, Alejandro

AU - Diercks, Alan

AU - Filippenko, Alexei V.

AU - Gilliland, Ronald Lynn

AU - Hogan, Craig J.

AU - Kirshner, Robert P.

AU - Leibundgut, Bruno

AU - Phillips, M. M.

AU - Reiss, David

AU - Riess, Adam G.

AU - Schmidt, Brian P.

AU - Schummer, Robert A.

AU - Chris Smith, R.

AU - Spyromilio, Jason

AU - Stubbs, Chris

AU - Suntzeff, Nicholas B.

AU - Tonry, John

AU - Carroll, Sean M.

PY - 1998/1/1

Y1 - 1998/1/1

N2 - We use Type la supernovae studied by the High-z Supernova Search Team to constrain the properties of an energy component that may have contributed to accelerating the cosmic expansion. We find that for a flat geometry the equation-of-state parameter for the unknown component, αx = Px/ρx, must be less than -0.55 (95% confidence) for any value of Ωm, and it is further limited to αx < -0.60 (95% confidence) if Ωm is assumed to be greater than 0.1. These values are inconsistent with the unknown component being topological defects such as domain walls, strings, or textures. The supernova (SN) data are consistent with a cosmological constant (αx = -1) or a scalar field that has had, on average, an equation-of-state parameter similar to the cosmological constant value of -1 over the redshift range of z ≈1 to the present. SN and cosmic microwave background observations give complementary constraints on the densities of matter and the unknown component. If only matter and vacuum energy are considered, then the current combined data sets provide direct evidence for a spatially flat universe with Ωiot = Ωm + ΩΔ = 0.94 ± 0.26 (1 σ).

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Garnavich PM, Jha S, Challis P, Clocchiatti A, Diercks A, Filippenko AV et al. Supernova limits on the cosmic equation of state. Astrophysical Journal. 1998 Jan 1;509(1 PART I):74-79. https://doi.org/10.1086/306495