Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I : Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum

Gravitational Wave (GW) sources are standard sirens that provide an independent way to map the cosmic expansion history by combining with an independent redshift measurement either from an electromagnetic counterpart for a bright siren or using different statistical techniques for dark sirens. In this analysis, we perform the first Blinded Mock Data Challenge (Blinded-MDC) to test the robustness in inferring the value of Hubble constant H0 for a dark siren technique which depends on astrophysical mass distribution of Binary Black Holes (BBHs). We have considered different analysis setups for the Blinded-MDC to test both statistical and systematic uncertainties and demonstrate the capabilities in inferring H0 with detector sensitivity as per the fourth observation run of LIGO-Virgo-KAGRA. We find that when the astrophysical population of BBHs matches with the underlying assumption of the model, a cosmological pipeline can recover the injected parameters using the observed mass distribution. However, when the mock mass distribution of the astrophysical population depends slightly on redshift and one is ignorant about it in analyzing the data, it can cause a systematic discrepancy in the inferred value of H0 by about 1.5σ, above the statistical fluctuations due to noise and a limited number of events. The discrepancy in H0 is arising due to astrophysical mis-modeling, and in the future, elaborate studies will be required to mitigate systematic uncertainties due to unknown astrophysical populations of BBHs. This MDC framework sets the road map for inspecting the precision and accuracy of standard siren cosmology and provides the first insight into the robustness of the population-dependent cosmology inference in a blinded analysis setup.

• Autores: Moreno González, Santiago; Rivera Arismendy, Juan Esteban
• Tipo de recurso: Trabajo de grado de pregrado
• Fecha de publicación: 2025
• Institución: Universidad de Antioquia
• Repositorio: Repositorio UdeA
• Idioma: eng
• OAI Identifier: oai:bibliotecadigital.udea.edu.co:10495/45732
• Acceso en línea: https://hdl.handle.net/10495/45732
• Palabra clave: Gravitational waves; Ondas gravitacionales; Black holes (Astronomy); Agujeros negros (Astronomía); Mass spectrometry; Espectrometría de masas; Probabilities; Probabilidades; Cosmology; Cosmología; Astrophysics; Astrofísica; Cosmology - Observations; Cosmological parameters; http://id.loc.gov/authorities/subjects/sh85056562; http://id.loc.gov/authorities/subjects/sh85014574; http://id.loc.gov/authorities/subjects/sh85081907; http://id.loc.gov/authorities/subjects/sh85107090; http://id.loc.gov/authorities/subjects/sh85033169; http://id.loc.gov/authorities/subjects/sh85009032
• Rights: openAccess
• License: http://creativecommons.org/licenses/by-nc-sa/4.0/