Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
Open accessAbstract
We detect the correlated peculiar velocities of nearby type Ia supernovae (SNe), while highlighting an error in some of the literature. We find sigma8 = 0.79 +/- 0.22 from SNe, and examine the potential of this method to constrain cosmological parameters in the future. We demonstrate that a survey of 300 low-z SNe (such as the nearby SNfactory) will underestimate the errors on w by approximately 35% if the coherent peculiar velocities are not included.
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This SN sample can be used as a tracer of large-scale structure through peculiar velocities, weak lensing of SN brightnesses, local bulk flow, and low-redshift isotropy constraints.
“This sample of SNe can be used as a tracer of large-scale structure by directly probing the gravitational potential of structure through inferences of their peculiar velocities ( Gordon et al. 2007; Bhattacharya et al. 2011; Howlett et al. 2017 ) , WL of SN brightnesses ( Dodelson & Vallinotto 2006; Quartin et al. 2014; Macaulay et al. 2017; Scovacricchi et al. 2017 ) , and the local bulk fl”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Gordon et al. 2007
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Quantifying Parameter Errors Due to the Peculiar Velocities of Type Ia Supernovae
Vanderveld, R. A. (2008) · The Astrophysical Journal · doi:10.1086/592396 · Cited by 8 · see citing works
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Are Type Ia supernova powerful tool to detect anisotropic expansion of the Universe?
Salehi, A., Farajollahi, H., Motahari, M., Pashamokhtari, P., Yarahmadi, M., & Fathi, S. (2020) · The European Physical Journal C · doi:10.1140/epjc/s10052-020-8269-z · Cited by 7 · see citing works
Dark-siren cosmology with Decihertz gravitational-wave detectors
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Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
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Type Ia supernovae as speed sensors at intermediate redshifts
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The power spectrum of luminosity distance fluctuations in General Relativity
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Joint curvature and growth rate measurements with supernova peculiar velocities and the CMB
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- Authors
- Gordon, C., Land, K., & Slosar, A.
- Affiliations
- University of Oxford (GB)
- ORCID
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2007-08-20
- Volume
- 99
- Issue
- 8
- Pages
- 081301-081301
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W1969030169
- Cited by
- 95
- References
- 28
- Citations by year
- 2026: 5 · 2025: 3 · 2024: 3 · 2023: 4 · 2022: 9 · 2021: 7 · 2020: 6 · 2019: 5 · 2018: 2 · 2017: 7 · 2016: 6 · 2015: 2 · 2014: 6 · 2013: 5 · 2012: 3
- FWCI
- 3.19
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physical Review Letters (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- Type Ia supernovae, peculiar velocities, cosmological constraints, sigma_8, dark energy equation of state, low-redshift supernovae
- MeSH terms
- Astronomy, Humans, Light
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Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
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