CaltechAUTHORS
  A Caltech Library Service

Bayesian forecasts for dark matter substructure searches with mock pulsar timing data

Lee, Vincent S. H. and Taylor, Stephen R. and Trickle, Tanner and Zurek, Kathryn M. (2021) Bayesian forecasts for dark matter substructure searches with mock pulsar timing data. Journal of Cosmology and Astroparticle Physics, 2021 (8). Art. No. 25. ISSN 1475-7516. doi:10.1088/1475-7516/2021/08/025. https://resolver.caltech.edu/CaltechAUTHORS:20210809-220324539

[img] PDF - Submitted Version
See Usage Policy.

707kB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20210809-220324539

Abstract

Dark matter substructure, such as primordial black holes (PBHs) and axion miniclusters, can induce phase shifts in pulsar timing arrays (PTAs) measurements due to gravitational effects. In order to gain a more realistic forecast for the detectability of such models of dark matter with PTAs, we propose a Bayesian inference framework to search for phase shifts generated by PBHs and perform the analysis on mock PTA data. For most PBH masses the constraints on the dark matter abundance agree with previous (frequentist) analyses (without mock data) to O(1) factors. This further motivates a dedicated search for PBHs (and dense small scale structures) in the mass range from 10⁻⁸ M☉ to well above 10² M☉ with the Square Kilometer Array. Moreover, with a more optimistic set of timing parameters, future PTAs are predicted to constrain PBHs down to 10⁻¹¹ M☉. Lastly, we discuss the impact of backgrounds, such as Supermassive Black Hole Mergers, on detection prospects, suggesting a future program to separate a dark matter signal from other astrophysical sources.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1088/1475-7516/2021/08/025DOIArticle
https://arxiv.org/abs/2104.05717arXivDiscussion Paper
ORCID:
AuthorORCID
Taylor, Stephen R.0000-0003-0264-1453
Trickle, Tanner0000-0003-1371-4988
Zurek, Kathryn M.0000-0002-2629-337X
Additional Information:© 2021 IOP Publishing Ltd and Sissa Medialab. Received 30 April 2021; Accepted 9 July 2021; Published 12 August 2021. VL, TT and KZ are supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics, under Award Number DE-SC0021431 and a Simons Investigator award. SRT acknowledges support from NSF grant AST-#2007993, and a Dean's Faculty Fellowship from Vanderbilt University's College of Arts & Science. The computations presented here were conducted on the Caltech High Performance Cluster, partially supported by a grant from the Gordon and Betty Moore Foundation.
Group:Walter Burke Institute for Theoretical Physics
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-SC0021431
Simons FoundationUNSPECIFIED
NSFAST-2007993
Vanderbilt UniversityUNSPECIFIED
Gordon and Betty Moore FoundationUNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
CALT-TH2021-016
Issue or Number:8
DOI:10.1088/1475-7516/2021/08/025
Record Number:CaltechAUTHORS:20210809-220324539
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210809-220324539
Official Citation:Vincent S.H. Lee et al JCAP08(2021)025
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:110186
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:10 Aug 2021 15:48
Last Modified:20 Sep 2021 18:34

Repository Staff Only: item control page