Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations

被引：8

作者：

Borghi, Nicola ^{[1
,2
]}

Mancarella, Michele ^{[3
,4
]}

Moresco, Michele ^{[1
,2
]}

Tagliazucchi, Matteo ^{[1
,2
]}

Iacovelli, Francesco ^{[5
,6
]}

Cimatti, Andrea ^{[1
,7
]}

Maggiore, Michele ^{[5
,6
]}

机构：

[1] Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy

[2] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy

[3] Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy

[4] Sez Milano Bicocca, INFN, Piazza Sci 3, I-20126 Milan, Italy

[5] Univ Geneva, Dept Phys Theor, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland

[6] Univ Geneva, Grav Wave Sci Ctr GWSC, CH-1211 Geneva, Switzerland

[7] INAF Osservatorio Astrofisico Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

来源：

ASTROPHYSICAL JOURNAL | 2024年 / 964卷 / 02期

基金：

瑞士国家科学基金会; 欧盟地平线“2020”;

关键词：

CHALLENGE LIGHTCONE SIMULATION; MULTI-MESSENGER OBSERVATIONS; HUBBLE CONSTANT; MULTIMESSENGER SEARCHES; ADVANCED LIGO; INFERENCE; POPULATION; EXPANSION; GLADE; DESI;

D O I：

10.3847/1538-4357/ad20eb

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

With the growing number of gravitational wave (GW) detections and the advent of large galaxy redshift surveys, a new era in cosmology is emerging. This study explores the synergies between GWs and galaxy surveys to jointly constrain cosmological and GW population parameters. We introduce CHIMERA, a novel code for GW cosmology combining information from the population properties of compact binary mergers and galaxy catalogs. We study constraints for scenarios representative of the LIGO-Virgo-KAGRA O4 and O5 observing runs, assuming to have a complete catalog of potential host galaxies with either spectroscopic or photometric redshift measurements. We find that a percent-level measurement of H 0 could be achieved with the best 100 binary black holes (BBHs) in O5 using a spectroscopic galaxy catalog. In this case, the intrinsic correlation that exists between H 0 and the BBH population mass scales is broken. Instead, by using a photometric catalog the accuracy is degraded up to a factor of similar to 9, leaving a significant correlation between H 0 and the mass scales that must be carefully modeled to avoid bias. Interestingly, we find that using spectroscopic redshift measurements in the O4 configuration yields a better constraint on H 0 compared to the O5 configuration with photometric measurements. In view of the wealth of GW data that will be available in the future, we argue the importance of obtaining spectroscopic galaxy catalogs to maximize the scientific return of GW cosmology.

引用

页数：19

共 115 条

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