Applying the Viterbi Algorithm to Planetary-Mass Black Hole Searches

Fuente: arXiv
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Autori principali: Alestas, George, Morras, Gonzalo, Yamamoto, Takahiro S., Garcia-Bellido, Juan, Kuroyanagi, Sachiko, Nesseris, Savvas
Natura: Preprint
Pubblicazione: 2024
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author Alestas, George
Morras, Gonzalo
Yamamoto, Takahiro S.
Garcia-Bellido, Juan
Kuroyanagi, Sachiko
Nesseris, Savvas
author_facet Alestas, George
Morras, Gonzalo
Yamamoto, Takahiro S.
Garcia-Bellido, Juan
Kuroyanagi, Sachiko
Nesseris, Savvas
contents The search for subsolar mass primordial black holes (PBHs) poses a challenging problem due to the low signal-to-noise ratio, extended signal duration, and computational cost demands, compared to solar mass binary black hole events. In this paper, we explore the possibility of investigating the mass range between subsolar and planetary masses, which is not accessible using standard matched filtering and continuous wave searches. We propose a systematic approach employing the Viterbi algorithm, a dynamic programming algorithm that identifies the most likely sequence of hidden Markov states given a sequence of observations, to detect signals from small mass PBH binaries. We formulate the methodology, provide the optimal length for short-time Fourier transforms, and estimate sensitivity. Subsequently, we demonstrate the effectiveness of the Viterbi algorithm in identifying signals within mock data containing Gaussian noise. Our approach offers the primary advantage of being agnostic and computationally efficient.
format Preprint
id arxiv_https___arxiv_org_abs_2401_02314
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Applying the Viterbi Algorithm to Planetary-Mass Black Hole Searches
Alestas, George
Morras, Gonzalo
Yamamoto, Takahiro S.
Garcia-Bellido, Juan
Kuroyanagi, Sachiko
Nesseris, Savvas
Cosmology and Nongalactic Astrophysics
Instrumentation and Methods for Astrophysics
General Relativity and Quantum Cosmology
The search for subsolar mass primordial black holes (PBHs) poses a challenging problem due to the low signal-to-noise ratio, extended signal duration, and computational cost demands, compared to solar mass binary black hole events. In this paper, we explore the possibility of investigating the mass range between subsolar and planetary masses, which is not accessible using standard matched filtering and continuous wave searches. We propose a systematic approach employing the Viterbi algorithm, a dynamic programming algorithm that identifies the most likely sequence of hidden Markov states given a sequence of observations, to detect signals from small mass PBH binaries. We formulate the methodology, provide the optimal length for short-time Fourier transforms, and estimate sensitivity. Subsequently, we demonstrate the effectiveness of the Viterbi algorithm in identifying signals within mock data containing Gaussian noise. Our approach offers the primary advantage of being agnostic and computationally efficient.
title Applying the Viterbi Algorithm to Planetary-Mass Black Hole Searches
topic Cosmology and Nongalactic Astrophysics
Instrumentation and Methods for Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2401.02314