Neutrino Properties with Ground-based Millimeter-wavelength Line Intensity Mapping

Moradinezhad Dizgah, Azadeh; Keating, Garrett K.; Karkare, Kirit S.; Crites, Abigail; Choudhury, Shouvik Roy

doi:10.3847/1538-4357/ac3edd

Neutrino Properties with Ground-based Millimeter-wavelength Line Intensity Mapping

Journal Article · Fri Feb 18 00:00:00 EST 2022 · The Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/ac3edd· OSTI ID:1833288

^[1]; ^[2]; ^[3]; Crites, Abigail ^[4]; ^[5]

Univ. of Geneva (Switzerland)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Univ. of Chicago, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Cornell Univ., Ithaca, NY (United States); California Institute of Technology (CalTech), Pasadena, CA (United States)
Indian Inst. of Technology (IIT), Bombay (India)

Line intensity mapping (LIM) is emerging as a powerful technique to map the cosmic large-scale structure and to probe cosmology over a wide range of redshifts and spatial scales. We perform Fisher forecasts to determine the optimal design of wide-field ground-based millimeter-wavelength LIM surveys for constraining properties of neutrinos and light relics. We consider measuring the auto-power spectra of several CO rotational lines (from J = 2–1 to J = 6–5) and the [C _II] fine-structure line in the redshift range of 0.25 < z < 12. We study the constraints with and without interloper lines as a source of noise in our analysis, and for several one-parameter and multiparameter extensions of ΛCDM. We show that LIM surveys deployable this decade, in combination with existing cosmic microwave background (CMB; primary) data, could achieve order-of-magnitude improvements over Planck constraints on N_eff and M_ν. Compared to next-generation CMB and galaxy surveys, a LIM experiment of this scale could achieve bounds that are a factor of ~3 better than those forecasted for surveys such as EUCLID (galaxy clustering), and potentially exceed the constraining power of CMB-S4 by a factor of ~1.5 and ~3 for N_eff and M_ν, respectively. Finally, we show that the forecasted constraints are not substantially affected when enlarging the parameter space, and additionally demonstrate that such a survey could also be used to measure ΛCDM parameters and the dark energy equation of state exquisitely well.

View Accepted Manuscript (DOE)

Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1833288

Report Number(s):: FERMILAB-PUB-21-527-V; arXiv:2110.00014; oai:inspirehep.net:1937327

Journal Information:: The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 926; ISSN 0004-637X

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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Connecting co Intensity Mapping to Molecular gas and star Formation in the Epoch of Galaxy Assembly Li, Tony Y.; Wechsler, Risa H.; Devaraj, Kiruthika The Astrophysical Journal, Vol. 817, Issue 2 https://doi.org/10.3847/0004-637X/817/2/169	journal	January 2016
On Removing Interloper Contamination from Intensity Mapping Power Spectrum Measurements Lidz, Adam; Taylor, Jessie The Astrophysical Journal, Vol. 825, Issue 2 https://doi.org/10.3847/0004-637X/825/2/143	journal	July 2016
${L}_{\mathrm{CO}}^{\prime }/{L}_{\mathrm{FIR}}$ RELATIONS WITH CO ROTATIONAL LADDERS OF GALAXIES ACROSS THE HERSCHEL SPIRE ARCHIVE Kamenetzky, J.; Rangwala, N.; Glenn, J. The Astrophysical Journal, Vol. 829, Issue 2 https://doi.org/10.3847/0004-637X/829/2/93	journal	September 2016
COPSS II: THE MOLECULAR GAS CONTENT OF TEN MILLION CUBIC MEGAPARSECS AT REDSHIFT z ∼ 3 Keating, Garrett K.; Marrone, Daniel P.; Bower, Geoffrey C. The Astrophysical Journal, Vol. 830, Issue 1 https://doi.org/10.3847/0004-637X/830/1/34	journal	October 2016
Spectral line De-Confusion in an Intensity Mapping Survey Cheng, Yun-Ting; Chang, Tzu-Ching; Bock, James The Astrophysical Journal, Vol. 832, Issue 2 https://doi.org/10.3847/0004-637X/832/2/165	journal	November 2016
A Foreground Masking Strategy for [C ii] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift Sun, G.; Moncelsi, L.; Viero, M. P. The Astrophysical Journal, Vol. 856, Issue 2 https://doi.org/10.3847/1538-4357/aab3e3	journal	March 2018
Line Intensity Mapping with [C ii] and CO(1-0) as Probes of Primordial Non-Gaussianity Moradinezhad Dizgah, Azadeh; Keating, Garrett K. The Astrophysical Journal, Vol. 872, Issue 2 https://doi.org/10.3847/1538-4357/aafd36	journal	February 2019
The Impact of Realistic Foreground and Instrument Models on 21 cm Epoch of Reionization Experiments Nasirudin, A.; Murray, S. G.; Trott, C. M. The Astrophysical Journal, Vol. 893, Issue 2 https://doi.org/10.3847/1538-4357/ab8003	journal	April 2020
Cosmological Constraints from Line Intensity Mapping with Interlopers Gong, Yan; Chen, Xuelei; Cooray, Asantha The Astrophysical Journal, Vol. 894, Issue 2 https://doi.org/10.3847/1538-4357/ab87a0	journal	May 2020
Phase-space Spectral Line Deconfusion in Intensity Mapping Cheng, Yun-Ting; Chang, Tzu-Ching; Bock, James J. The Astrophysical Journal, Vol. 901, Issue 2 https://doi.org/10.3847/1538-4357/abb023	journal	October 2020
An Intensity Mapping Detection of Aggregate CO Line Emission at 3 mm Keating, Garrett K.; Marrone, Daniel P.; Bower, Geoffrey C. The Astrophysical Journal, Vol. 901, Issue 2 https://doi.org/10.3847/1538-4357/abb08e	journal	October 2020
Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids Bayer, Adrian E.; Villaescusa-Navarro, Francisco; Massara, Elena The Astrophysical Journal, Vol. 919, Issue 1 https://doi.org/10.3847/1538-4357/ac0e91	journal	September 2021
Probing Cosmic Origins with CO and [C ii] Emission Lines Moradinezhad Dizgah, Azadeh; Keating, Garrett K.; Fialkov, Anastasia The Astrophysical Journal, Vol. 870, Issue 1 https://doi.org/10.3847/2041-8213/aaf813	journal	January 2019

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