Feasibility of measuring the cosmological constant {Lambda} and mass density {Omega} using Type Ia supernovae
- Physics Department, Stockholm University, Box 6730, S-113 85 Stockholm (Sweden)
- Center for Particle Astrophysics, University of California, Berkeley, and Lawrence Berkeley Laboratory, 50-232, Berkeley, California 94720 (United States)
We explore the feasibility of resurrecting the apparent magnitude-redshift relation for a {open_quote}{open_quote}standard candle{close_quote}{close_quote} to measure the cosmological constant and mass density. We show that Type Ia supernovae, if measured with 0.15 mag uncertainty out to a redshift of {ital z}=1, may provide a good standard candle or calibrated candle for this purpose. The recent discovery of probable Type Ia supernovae in the redshift range {ital z}=0.3{minus}0.5 (Perlmutter {ital et} {ital al}. 1994, 1995) indicates that the flux of optical photons from these events can be measured this accurately. The seven distant supernovae discovered to date do not by themselves distinguish among different cosmological models; however, the further discovery of about 50 Type Ia supernovae at redshifts in the range 0.5{le}{ital z}{le}1.0 could strongly constrain the allowed range of these parameters. We estimate that the follow-up photometry necessary for this measurement would be on the order of 20-70 hr of time on a 10 m class telescope at a site with good seeing. {copyright} {ital 1995 The American Astronomical Society.}
- Research Organization:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- DOE Contract Number:
- AC03-76SF00098
- OSTI ID:
- 281950
- Journal Information:
- Astrophysical Journal, Vol. 450, Issue 1; Other Information: PBD: Sep 1995
- Country of Publication:
- United States
- Language:
- English
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