Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope
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| Format: | Preprint |
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2026
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| author | Spezzati, Francesco Wang, Yun Hearin, Andrew |
| author_facet | Spezzati, Francesco Wang, Yun Hearin, Andrew |
| contents | We present realistic forecasts for the constraining power of the Nancy Grace Roman Space Telescope on fundamental cosmological parameters, with particular emphasis on the absolute neutrino mass scale, using full-shape analyzes of the galaxy power spectrum. We analyze simulated lightcone mock catalogs of H$α$ emission-line galaxies spanning the redshift range $0.5 < z < 2$ over $2400\ \mathrm{deg}^2$, designed to reproduce the expected properties of the Roman High Latitude Wide Area Spectroscopic Survey. We perform parameter inference on the galaxy power spectrum multipoles using two complementary theoretical frameworks: a model-dependent approach based on the Effective Field Theory of Large-Scale Structure (EFT of LSS) within $Λ$CDM, and a model-independent phenomenological approach that makes no assumptions about the background cosmological model. In the $Λ$CDM analysis, we find $m_ν< 0.380(0.162)\ \mathrm{eV}$ at $95(68)\%$ C.L. using Big Bang Nucleosynthesis (BBN) prior and a broad prior on $n_s$, which tightens to $m_ν< 0.276(0.121)\ \mathrm{eV}$ when Planck priors on $ω_b$, $ω_\mathrm{cdm}$, and $n_s$ are added. Our forecasts show that Roman can additionally constrain $H_0$, $Ω_m$, and $σ_8$ with precisions of $1.3\%$, $4.3\%$, and $2.9\%$ in line with Stage IV galaxy survey measurements and forecasts. In the model-independent analysis, we demonstrate that the phenomenological model can robustly recover unbiased measurements of the angular diameter distance, the Hubble parameter, and the growth of structure across all redshift bins, in the same range of scales as the EFT model, and obtain $m_ν< 0.63(0.36)\ \mathrm{eV}$ at $95(68)\%$ C.L. when Planck priors are included. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2604_14504 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope Spezzati, Francesco Wang, Yun Hearin, Andrew Cosmology and Nongalactic Astrophysics We present realistic forecasts for the constraining power of the Nancy Grace Roman Space Telescope on fundamental cosmological parameters, with particular emphasis on the absolute neutrino mass scale, using full-shape analyzes of the galaxy power spectrum. We analyze simulated lightcone mock catalogs of H$α$ emission-line galaxies spanning the redshift range $0.5 < z < 2$ over $2400\ \mathrm{deg}^2$, designed to reproduce the expected properties of the Roman High Latitude Wide Area Spectroscopic Survey. We perform parameter inference on the galaxy power spectrum multipoles using two complementary theoretical frameworks: a model-dependent approach based on the Effective Field Theory of Large-Scale Structure (EFT of LSS) within $Λ$CDM, and a model-independent phenomenological approach that makes no assumptions about the background cosmological model. In the $Λ$CDM analysis, we find $m_ν< 0.380(0.162)\ \mathrm{eV}$ at $95(68)\%$ C.L. using Big Bang Nucleosynthesis (BBN) prior and a broad prior on $n_s$, which tightens to $m_ν< 0.276(0.121)\ \mathrm{eV}$ when Planck priors on $ω_b$, $ω_\mathrm{cdm}$, and $n_s$ are added. Our forecasts show that Roman can additionally constrain $H_0$, $Ω_m$, and $σ_8$ with precisions of $1.3\%$, $4.3\%$, and $2.9\%$ in line with Stage IV galaxy survey measurements and forecasts. In the model-independent analysis, we demonstrate that the phenomenological model can robustly recover unbiased measurements of the angular diameter distance, the Hubble parameter, and the growth of structure across all redshift bins, in the same range of scales as the EFT model, and obtain $m_ν< 0.63(0.36)\ \mathrm{eV}$ at $95(68)\%$ C.L. when Planck priors are included. |
| title | Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2604.14504 |