DESI and other Dark Energy experiments in the era of neutrino mass measurements
Abstract
Here we present Fisher matrix projections for future cosmological parameter measurements, including neutrino masses, Dark Energy, curvature, modified gravity, the inflationary perturbation spectrum, non-Gaussianity, and dark radiation. We focus on DESI and generally redshift surveys (BOSS, HETDEX, eBOSS, Euclid, and WFIRST), but also include CMB (Planck) and weak gravitational lensing (DES and LSST) constraints. The goal is to present a consistent set of projections, for concrete experiments, which are otherwise scattered throughout many papers and proposals. We include neutrino mass as a free parameter in most projections, as it will inevitably be relevant $$-$$ DESI and other experiments can measure the sum of neutrino masses to ~ 0.02 eV or better, while the minimum possible sum is 0.06 eV. We note that constraints on Dark Energy are significantly degraded by the presence of neutrino mass uncertainty, especially when using galaxy clustering only as a probe of the BAO distance scale (because this introduces additional uncertainty in the background evolution after the CMB epoch). Using broadband galaxy power becomes relatively more powerful, and bigger gains are achieved by combining lensing survey constraints with redshift survey constraints. Finally, we do not try to be especially innovative, e.g., with complex treatments of potential systematic errors $$-$$ these projections are intended as a straightforward baseline for comparison to more detailed analyses.
- Authors:
-
- Univ. of Zurich, Irchel (Switzerland). Inst. of Theoretical Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Publication Date:
- Research Org.:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1335437
- Report Number(s):
- BNL-112100-2016-JA
Journal ID: ISSN 1475-7516; KA2301020
- Grant/Contract Number:
- SC00112704
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Additional Journal Information:
- Journal Volume: 2014; Journal Issue: 05; Journal ID: ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; dark energy experiments; cosmological parameters from LSS; neutrino masses from cosmology; inflation
Citation Formats
Font-Ribera, Andreu, McDonald, Patrick, Mostek, Nick, Reid, Beth A., Seo, Hee-Jong, and Slosar, Anže. DESI and other Dark Energy experiments in the era of neutrino mass measurements. United States: N. p., 2014.
Web. doi:10.1088/1475-7516/2014/05/023.
Font-Ribera, Andreu, McDonald, Patrick, Mostek, Nick, Reid, Beth A., Seo, Hee-Jong, & Slosar, Anže. DESI and other Dark Energy experiments in the era of neutrino mass measurements. United States. https://doi.org/10.1088/1475-7516/2014/05/023
Font-Ribera, Andreu, McDonald, Patrick, Mostek, Nick, Reid, Beth A., Seo, Hee-Jong, and Slosar, Anže. Mon .
"DESI and other Dark Energy experiments in the era of neutrino mass measurements". United States. https://doi.org/10.1088/1475-7516/2014/05/023. https://www.osti.gov/servlets/purl/1335437.
@article{osti_1335437,
title = {DESI and other Dark Energy experiments in the era of neutrino mass measurements},
author = {Font-Ribera, Andreu and McDonald, Patrick and Mostek, Nick and Reid, Beth A. and Seo, Hee-Jong and Slosar, Anže},
abstractNote = {Here we present Fisher matrix projections for future cosmological parameter measurements, including neutrino masses, Dark Energy, curvature, modified gravity, the inflationary perturbation spectrum, non-Gaussianity, and dark radiation. We focus on DESI and generally redshift surveys (BOSS, HETDEX, eBOSS, Euclid, and WFIRST), but also include CMB (Planck) and weak gravitational lensing (DES and LSST) constraints. The goal is to present a consistent set of projections, for concrete experiments, which are otherwise scattered throughout many papers and proposals. We include neutrino mass as a free parameter in most projections, as it will inevitably be relevant $-$ DESI and other experiments can measure the sum of neutrino masses to ~ 0.02 eV or better, while the minimum possible sum is 0.06 eV. We note that constraints on Dark Energy are significantly degraded by the presence of neutrino mass uncertainty, especially when using galaxy clustering only as a probe of the BAO distance scale (because this introduces additional uncertainty in the background evolution after the CMB epoch). Using broadband galaxy power becomes relatively more powerful, and bigger gains are achieved by combining lensing survey constraints with redshift survey constraints. Finally, we do not try to be especially innovative, e.g., with complex treatments of potential systematic errors $-$ these projections are intended as a straightforward baseline for comparison to more detailed analyses.},
doi = {10.1088/1475-7516/2014/05/023},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 05,
volume = 2014,
place = {United States},
year = {Mon May 19 00:00:00 EDT 2014},
month = {Mon May 19 00:00:00 EDT 2014}
}
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