Measuring neutrino masses and dark energy with weak lensing tomography
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Surveys of weak gravitational lensing of distant galaxies will be one of the key cosmological probes in the future. We study the ability of such surveys to constrain neutrino masses and the equation of state parameter of dark energy, focusing on how tomographic information can improve the sensitivity to these parameters. We also provide a detailed discussion of systematic effects pertinent to weak lensing surveys, and the possible degradation of sensitivity to cosmological parameters due to these effects. For future probes such as the Large Synoptic Survey Telescope survey, we find that, when combined with cosmic microwave background data from the Planck satellite, a sensitivity to neutrino masses of can be reached. These results are not affected by variations in the running of the scalar spectral index, the time-dependence of the dark energy equation of state, and/or the number of relativistic degrees of freedom.
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The shape of the dark matter fluctuation power spectrum measured by LSST weak lensing will constrain the sum of neutrino masses with accuracy of 0.04 eV or better.
“The shape of the power spectrum of dark matter fl uctuations measured by LSST WL will constrain the sum of neutrino masses with an accuracy of 0.04 eV or better ( Cooray 1999; Song & Knox 2004; Hannestad et al. 2006 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Hannestad et al. 2006
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Neutrino Physics and Cosmology
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Large Synoptic Survey Telescope Town Hall
Willman, B. (2016) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.44768
Neutrino mass bounds from neutrinoless double beta-decays and cosmological probes
Keum, Y. Y. (2016) · Pramana · doi:10.1007/s12043-015-1164-8
The Lsst Data Processing Software Stack
Jenness, T. (2016) · American Astronomical Society Meeting Abstracts #227 · doi:10.5281/zenodo.44634
Bartelmann, M., Bennett, C. L., Bucher, M., Burigana, C., Capaccioli, M., D’Onofrio, M., Ruth Durrer, A., Gioia, I. M., Hasinger, G., Lawrence, C. R., et al. (2009) · Springer eBooks · doi:10.1007/978-3-642-00792-7_5
- Authors
- Hannestad, S., Tu, H., & Wong, Y. Y. Y.
- Affiliations
- Aarhus University (DK)
- Max Planck Institute for Physics (DE)
- ORCID
- Hannestad, Steen
- Venue
- Journal of Cosmology and Astroparticle Physics
- Publisher
- IOP Publishing
- Published
- 2006-06-28
- Volume
- 2006
- Issue
- 06
- Pages
- 025-025
- ISSN
- 1475-7508 (ISSN-L)
- 1475-7516
- OpenAlex
- W1983465483
- Cited by
- 98
- References
- 86
- Citations by year
- 2025: 1 · 2022: 1 · 2020: 2 · 2019: 6 · 2018: 5 · 2017: 1 · 2016: 6 · 2015: 1 · 2014: 2 · 2013: 9 · 2012: 12
- FWCI
- 6.32
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Journal of Cosmology and Astroparticle Physics (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Neutrino Physics Research
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- neutrino mass, dark energy equation of state, weak gravitational lensing, systematic effects, LSST, Planck CMB constraints, relativistic degrees of freedom, cosmological parameter constraints
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